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One entity of NonWiki, the Negative of the Negative (EA-NEGONT-02, #1726), cited at https://www.alexanarch.org/non/ata-3i-atlas-search/. the table of contents · this entity as data · contents as data · the dataset on the Hub · row json · field ledger · archive ledger · D/R/O traversal · the address page.
SPXI instrument · method 0.16 of 87, level 0 (Measurement): The Negative of the Negative (/non). An instrument of SPXI, the Semantic Packet for eXchange & Indexing; the whole practice is itemized at spxi.dev/methods.
WORKING KNOWLEDGE OBJECT · NOT FROZEN · LEDGER UNAUDITED
A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array is a paper by Sofia Z. Sheikh and fourteen co-authors reporting a narrowband radio search of the interstellar object 3I/ATLAS, made with the SETI Institute's Allen Telescope Array from 1 to 9 GHz beginning in July 2025. It is one of three published radio searches of the object, beside the Green Bank Telescope's and a FAST search in 1.05–1.45 GHz. Posted to arXiv on 19 December 2025 as 2512.18142 and revised on 20 May 2026 after acceptance, it was published open access in The Astronomical Journal (volume 172, article 1) on 3 June 2026 under a Creative Commons Attribution 4.0 licence.
Its authors set the search beside the possibility that probes sent by extraterrestrial life could explore systems such as ours, as the Voyager spacecraft will one day be artifacts in other stellar systems, and hold narrowband radio emission to be the most unambiguous observable of such an artifact, since only technological sources produce it. They note that 3I/ATLAS showed no compelling evidence of nonnatural characteristics and treat constraints on its radio emission as standard practice for interstellar objects; Breakthrough Listen's project page likewise finds no evidence that the object is anything other than natural, and a co-author holds that the result shows how realistic detection is with present technology.
Observations began on 2 July 2025, about 23 hours after the object's discovery was reported, and ran in five sessions totalling 7.25 hours on source; one press account gives the band as 1-12 GHz, which the paper's own sessions do not support.
The hit-finding code bliss searched drift rates from −4 to +4 Hz/s at a signal-to-noise threshold of 15, which the authors describe as one of the lowest of any modern SETI survey, and found 73,974,799 narrowband hits. Blanking 1269.8 MHz of the band, about 16 per cent, where hits crowded left about 11 million hits; the authors expect to examine the blanking ranges further.
The second cut is a drift-rate filter, whose stated purpose is "To filter out signals that do not match the dynamics of 3I/ATLAS". The authors took the time derivative of the range rate (deldot) in JPL Horizons, found accelerations of 3.2 to 3.5 × 10⁻⁵ km/s² in all five sessions, and converted them to an expected drift for an emitter on the object, given as magnitudes: 0.15 Hz/s at the lowest tuning and 1.01 Hz/s at the highest. Because the rotation or tumbling of the object was uncertain and could be large, they took a middle ground, in the journal's words: "We filter our hits for drift rates between 0.05 and 1.5 Hz s−1 at all frequencies"; the arXiv version gives the interval as "0.05–1.5 Hz/s". After the cut about 2 million hits remained, the two blanking steps together having removed 97.4 per cent; the paper reports this as the first use of expected drift-rate contributions as a filter in a technosignature search of a solar system object. Its Figure 4 plots the hits on a signed drift axis from −4 to +4 Hz/s, most of them near zero drift, where ground transmitters sit, and shows the retained hits from 0 to +1.5 Hz/s, with none in the negative half.
The archive's notebook on the searches (#1742, Nobel Glas and Orin Trace) reads the sign against the physics: a rising range-rate lowers the received frequency, so a positive acceleration gives a negative drift, and a tone riding on the object, computed from Horizons at the ATA site, drifts at −0.125 Hz/s at 1075 MHz and −0.19 Hz/s at 1623.75 MHz, negative in all six public sessions, with the data's positive channel spacing requiring no sign flip. On that reading the paper derived the right magnitude and gave it the sign of the acceleration, so that on its own figure the drift it computed for an emitter on 3I/ATLAS lies in the half its filter removed; the public account by Lee Sharks (#1743) calls it the right size and the wrong sign. The finding stands on the manuscript, the figure and the physics: the executed filter script and the signed before-and-after catalogues have not been obtained, and the finding does not show that a transmission was discarded. The archive's sophistry measure records the operation as homonymy at the counter-board, one name, the drift rate of 3I/ATLAS, standing for a magnitude and for a signed rate, and makes no sophistic charge: it records an error in a published method. Its smallest repair for the paper states that a tone fixed on the object drifts negative throughout the sessions while the interval retains the opposite sign. The interval also excludes zero drift, by the field's practice of treating zero-drift hits as terrestrial, and zero drift is where a sender that pre-compensates its Doppler for the receiving telescope would arrive. No published comment, erratum or critique raising the sign had been found by 3 November 2026; the Green Bank search describes no drift cut. Because the ATA data are public, the removed class was searched again: along the object's true drift, at ten frequencies of the 3 July session and fourteen windows of the 8 July session, the true path stayed within the spread of its sign-flipped twin and the beam swaps, and nothing recurred in more than two scans; an earlier search of part of the class found no convincing signal. The discrepancy hid nothing that this look could see, and it remains a discrepancy in a published method; correcting the sign would not have brought within the ATA's sensitivity the Green Bank features the notebook calls the thirteen, and what the sign removed is a class held apart from what the thirteen are. The press carried the filter in two further forms: as keeping only signals matching the acceleration expected of 3I/ATLAS, and, in Space, as filtering out artifacts caused by the object's movement, which reverses the sense the paper states.
The remaining hits went to NBeamAnalysis, which compares two beams to find signals consistent with a localized point source, and 211 events were plotted for visual inspection. Of the 211, 11 exceeded the beam-ratio threshold of 5.29, and 200 were backup plots from two sessions with no event above it. After visual inspection the authors found all 211 "easily attributable to RFI": none of the sky-localized events showed a narrowband drifting signal, and the narrowband drifting signals among the rest were inconsistent with a sky-localized source, so that "zero outputs depict nonterrestrial technological signals". Their two illustrated examples are a sky-localized event at a frequency consistent with the Iridium satellites' L-band downlink, with the note that satellites and other distant transmitters can mimic a technosignature, and a narrowband signal of similar strength in both beams, read as a local interferer; Breakthrough Listen's page shows a stripe in both beams rejected the same way. The notebook reads the procedure as a classification: comparison of the beams supports rejection as an unlocalised source without identifying it, the press sentence that every one "turned out to be human-made interference" states an identification, and the raw-data audit of the 211 has not been done. The sophistry measure finds that the label "human-made", given to what the rules removed before the conclusion is drawn, places the conclusion among the premises. In the press the 211 became events each "determined to be caused by Earth-based radio frequency interference" (Universe Today), only human-made interference, all "traced back to technology on the surface of the Earth or our own Earth-orbiting satellites" (Sci.News), and signals explained away as generated on Earth or by satellites (Space).
The result is that the search found no "signals worthy of additional follow-up"; Breakthrough Listen reports no technosignature in any of its searches of the object. The limit, in the abstract's words: "we are able to set an effective isotropic radiated power upper limit of 10-110 W on radio technosignatures from 3I/ATLAS across the frequency and drift rate ranges covered by our survey"; the conclusion repeats 10–110 W "across our frequency and drift-rate range". Sensitivity is greatest at drift rates of 0.113 Hz/s or less and falls as drift increases, so the worst case is set at 1.5 Hz/s; MeerKAT's search reached 0.17 W over 900–1670 MHz, and this one covers ten times the frequencies. The archive reads the limit through its account of null results: a null constrains only those hypotheses for which the end-to-end acceptance of the acquisition and analysis chain is sufficiently characterized, the scope of this null is set by what its filters retained, and the three published searches state frequencies, drift intervals, thresholds and power limits while leaving retention below their detection thresholds and in the drift class removed by sign uncharacterized. No stage of the cascade bounds what a transmitter on the object, drifting negative, would have retained end to end, since validation of each stage on its own support sets no lower bound on retention outside it; the filter is a model of the object placed at the interface, and what it kept of hits matching the object goes unmeasured in the paper. The three published searches find hits above a threshold scan by scan, so their miss regions overlap by construction, and instruments that miss identical things add little to one another. The notebook keeps three operations apart: a boundary a search sets and states, a discrepancy between a method and its own derivation, and a public statement that drops the boundary; a threshold forecloses nothing by existing, and the problem arises where a claim exceeds the acceptance its search characterized. The public account notes that each paper states the frequencies and drift rates it searched and that the ATA ties its 10 to 110 watts to them, and gives the sentence that would have kept the scope: "no narrowband signal above these strengths, within these drift rates, in these bands, on these dates."
Breakthrough Listen's project page gives the ATA data as 1 to 9 GHz with sensitivities between 10 and 110 W and no drift range, still describes the paper as submitted for peer review, and concludes that the object continues to behave as natural. The SETI Institute's statement, carried by Sci.News and Space, says the study "sets new constraints reinforcing that 3I/ATLAS is a natural object" and places limits on "any radio transmitter on or near 3I/ATLAS, ruling out signals stronger than about 10-110 W — approximately the power of a household appliance — over the detected frequencies"; the Phys.org card carries the same reinforcing sentence. Universe Today wrote of a methodology used "to prove" the object no alien technology, gave the limit as about 10 watts at 1 GHz and 110 at 9 GHz with a caveat, and judged that a sender would use a stronger transmitter; Space opened on the object being "indeed just a comet". An account the notebook quotes, Intelligent Living's, called the answer "a firm one", and its FAQ gave the limit for 1 to 9 GHz with the drift ranges dropped; the sophistry measure reads its account of the 211 as a set made by filtering reported as a property of its members. The public account observes that the sign error in the filter travelled nowhere at all. Wikipedia's article on 3I/ATLAS, last edited on 30 October 2026, mentions no radio search: its section on alien spacecraft speculation gives Loeb's paper of July 2025 and Live Science's report that "the overwhelming consensus is that it is a comet".
The archive's operator reads the published searches as built to rule a signal out as economically as possible, granting that the premise can be good method while holding that the work ruling out requires was not done: "it was a performance of search for signal, almost perfunctory". Each part of the reading is tied to the record: the filter's sign against the team's own ephemeris, the unmeasured retention of signals moving with the object, retention below a single look's threshold characterized in none of the three, and a result made public as a firm no for 1 to 9 GHz. The same record states its counterweight: the teams published their data, the precondition of every reanalysis here, Breakthrough Listen keeps spectra on the side of the line past which a discarded event exists for no later reading, and no archive instrument says the searches missed a transmission. Open on the ATA side are the executed blanking script with the signed catalogues, a raw audit of the 211, the 3 July session along the true drift at 1667.41–1668.43 MHz, and 39 scan directories that refuse public access.
Asked for the paper by its title on 6 November 2026, Google's AI Overview kept the campaign's figures, which the Capture Registry finds are the paper's, named no author, and folded the drift stage into "drift-rate blanking", the paper's own term for the step. The Capture Registry finds that the Overview rendered the classification of the 211 as a tracing of every event to Earth technology or satellites, stated the power limit without the frequencies and drift rates it is conditioned on, so that its "any active radio transmitters" covers the class the stated method could not see, and closed on a verdict, "firmly" natural, that a nondetection does not reach. Its smallest repair reads: "No narrowband signal above 10–110 W was found within 1–9 GHz and the drift rates the search retained (0.05–1.5 Hz/s, positive); 211 inspected events were classified as interference." At "3i atlas ata drift rate filter" on 4 November 2026 the Overview composed the interval exactly and without a sign, with the paper's purpose and counts, and described the filter as removing interference "without missing real signals"; the registry finds the paper's own gap passing through intact. Its repair states the positive retained interval against the negative drift of a tone on the object, and its countertest is the address "3i atlas ata drift rate sign".
F1 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF9 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Authors documented · fieldF14 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §2 documented · fieldA1742-01 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) documentedA1742-01 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) documentedF8 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Submission history; Comments documented · fieldF10 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., header documented · fieldF11 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., licence documented · fieldF2 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF57 Space — Interstellar comet 3I/ATLAS is not an alien spacecraft: SETI hunt for 'technosignatures' comes up empty | Space, body documented · fieldF12 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §1.2 documented · fieldF13 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §1.2 documented · fieldF38 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, introduction documented · fieldF54 Sci.News — Astronomers Scan Interstellar Object 3I/ATLAS for Alien Radio Signals | Sci.News, body documented · fieldF14 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §2 documented · fieldF15 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §2 documented · fieldF45 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶5 documented · fieldF16 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.1 documented · fieldF17 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.1 documented · fieldF25 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4 documented · fieldF3 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF25 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4 documented · fieldF36 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §6 documented · fieldF18 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF19 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF20 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF21 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF61 arXiv — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array (v2 full text, HTML and PDF), §3.2 (PDF) documented · fieldF22 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF23 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF59 arXiv — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array (v2 full text, HTML and PDF), §3.2 (PDF) documented · fieldF60 arXiv — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array (v2 full text, HTML and PDF), §3.2 (HTML) documented · fieldF4 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF25 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4 documented · fieldF26 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4, Figure 3 caption documented · fieldF35 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §6 documented · fieldF24 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4, Figure 4 caption documented · fieldA1742-03 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) documentedA1742-04 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) stipulationA1742-05 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) documentedA1742-06 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) documentedA1742-07 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) interpretationA1743-03 #1743 A Firm No: What the 3I/ATLAS Radio Searches Could See (EA-3I-ATLAS-PUBLIC-01 v1.1) interpretationA1742-08 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) self-descriptionA1743-04 #1743 A Firm No: What the 3I/ATLAS Radio Searches Could See (EA-3I-ATLAS-PUBLIC-01 v1.1) self-descriptionSM-01 sophistry-run The sophistry measure on the 3I/ATLAS record: first run, 2026-11-06 (EA-SOPHISTRY-01, #1727; rebuild/3i-atlas-signal-sea interpretationSM-02 sophistry-run The sophistry measure on the 3I/ATLAS record: first run, 2026-11-06 (EA-SOPHISTRY-01, #1727; rebuild/3i-atlas-signal-sea interpretationSM-03 sophistry-run The sophistry measure on the 3I/ATLAS record: first run, 2026-11-06 (EA-SOPHISTRY-01, #1727; rebuild/3i-atlas-signal-sea self-descriptionO1727-01 #1727 The Sophistry Measure: the Sophistical Refutations Read as an Instrument for Machine-Composed Knowledge (EA-SOPHISTRY-01 stipulationSM-04 sophistry-run The sophistry measure on the 3I/ATLAS record: first run, 2026-11-06 (EA-SOPHISTRY-01, #1727; rebuild/3i-atlas-signal-sea stipulationA1742-12 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) interpretationA1742-09 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) documentedA1742-10 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) documentedF42 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, Data documented · fieldA1742-13 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) documentedA1742-14 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) documentedA1742-08 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) self-descriptionA1743-05 #1743 A Firm No: What the 3I/ATLAS Radio Searches Could See (EA-3I-ATLAS-PUBLIC-01 v1.1) interpretationA1743-06 #1743 A Firm No: What the 3I/ATLAS Radio Searches Could See (EA-3I-ATLAS-PUBLIC-01 v1.1) interpretationF46 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶6 documented · fieldF56 Space — Interstellar comet 3I/ATLAS is not an alien spacecraft: SETI hunt for 'technosignatures' comes up empty | Space, body documented · fieldF5 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF27 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.3 documented · fieldF28 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4 documented · fieldF29 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4 documented · fieldF30 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4, Figure 7 caption documented · fieldF31 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4, Figure 8 caption documented · fieldF41 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, Allen Telescope Array, figure caption documented · fieldA1742-11 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) interpretationSM-05 sophistry-run The sophistry measure on the 3I/ATLAS record: first run, 2026-11-06 (EA-SOPHISTRY-01, #1727; rebuild/3i-atlas-signal-sea interpretationF47 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶7 documented · fieldF50 Sci.News — Astronomers Scan Interstellar Object 3I/ATLAS for Alien Radio Signals | Sci.News, lede documented · fieldF51 Sci.News — Astronomers Scan Interstellar Object 3I/ATLAS for Alien Radio Signals | Sci.News, body documented · fieldF56 Space — Interstellar comet 3I/ATLAS is not an alien spacecraft: SETI hunt for 'technosignatures' comes up empty | Space, body documented · fieldF6 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF39 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, introduction documented · fieldF7 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF34 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §6 documented · fieldF32 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §5 documented · fieldF33 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §5 documented · fieldO1450-01 #1450 The Iceberg Document: Instrument-Conditioned Nullity, Correlated Blind Spots, and the Conditions for Continued Surprise stipulationA1742-02 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) interpretationA1742-16 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) interpretationA1742-17 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) interpretationO1450-02 #1450 The Iceberg Document: Instrument-Conditioned Nullity, Correlated Blind Spots, and the Conditions for Continued Surprise stipulationA1742-20 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) interpretationA1743-08 #1743 A Firm No: What the 3I/ATLAS Radio Searches Could See (EA-3I-ATLAS-PUBLIC-01 v1.1) interpretationA1742-19 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) interpretationO1450-04 #1450 The Iceberg Document: Instrument-Conditioned Nullity, Correlated Blind Spots, and the Conditions for Continued Surprise interpretationA1742-15 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) stipulationA1743-01 #1743 A Firm No: What the 3I/ATLAS Radio Searches Could See (EA-3I-ATLAS-PUBLIC-01 v1.1) documentedA1743-10 #1743 A Firm No: What the 3I/ATLAS Radio Searches Could See (EA-3I-ATLAS-PUBLIC-01 v1.1) stipulationF40 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, Allen Telescope Array documented · fieldF43 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, summary documented · fieldF52 Sci.News — Astronomers Scan Interstellar Object 3I/ATLAS for Alien Radio Signals | Sci.News, body documented · fieldF53 Sci.News — Astronomers Scan Interstellar Object 3I/ATLAS for Alien Radio Signals | Sci.News, body documented · fieldF58 Space — Interstellar comet 3I/ATLAS is not an alien spacecraft: SETI hunt for 'technosignatures' comes up empty | Space, body documented · fieldF37 Phys.org — Interstellar object 3I/ATLAS reveals no technosignatures in seven-hour radio ..., card snippet documented · fieldF44 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶1 documented · fieldF48 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶8 documented · fieldF49 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶8 documented · fieldF55 Space — Interstellar comet 3I/ATLAS is not an alien spacecraft: SETI hunt for 'technosignatures' comes up empty | Space, lede documented · fieldA1742-21 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) attributedA1743-02 #1743 A Firm No: What the 3I/ATLAS Radio Searches Could See (EA-3I-ATLAS-PUBLIC-01 v1.1) interpretationSM-06 sophistry-run The sophistry measure on the 3I/ATLAS record: first run, 2026-11-06 (EA-SOPHISTRY-01, #1727; rebuild/3i-atlas-signal-sea interpretationA1743-11 #1743 A Firm No: What the 3I/ATLAS Radio Searches Could See (EA-3I-ATLAS-PUBLIC-01 v1.1) interpretationF62 Wikipedia — 3I/ATLAS (the article; no section on the radio searches), section 'Alien spacecraft speculation' documented · fieldF63 Wikipedia — 3I/ATLAS (the article; no section on the radio searches), section 'Alien spacecraft speculation' documented · fieldA1742-23 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) interpretationA1742-22 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) interpretationA1743-07 #1743 A Firm No: What the 3I/ATLAS Radio Searches Could See (EA-3I-ATLAS-PUBLIC-01 v1.1) interpretationA1742-22 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) interpretationA1743-09 #1743 A Firm No: What the 3I/ATLAS Radio Searches Could See (EA-3I-ATLAS-PUBLIC-01 v1.1) interpretationA1742-24 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) self-descriptionA1743-09 #1743 A Firm No: What the 3I/ATLAS Radio Searches Could See (EA-3I-ATLAS-PUBLIC-01 v1.1) interpretationA1742-18 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) interpretationO1450-03 #1450 The Iceberg Document: Instrument-Conditioned Nullity, Correlated Blind Spots, and the Conditions for Continued Surprise stipulationA1742-25 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) self-descriptionCAP-1-01 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry ata-3i-atlas-technosignature-search-paper-aio-20261106 (OBS-f18605c5f3ba, AX documentedCAP-1-07 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry ata-3i-atlas-technosignature-search-paper-aio-20261106 (OBS-f18605c5f3ba, AX documentedCAP-1-10 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry ata-3i-atlas-technosignature-search-paper-aio-20261106 (OBS-f18605c5f3ba, AX interpretationF25 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4 documented · fieldCAP-1-02 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry ata-3i-atlas-technosignature-search-paper-aio-20261106 (OBS-f18605c5f3ba, AX interpretationCAP-1-03 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry ata-3i-atlas-technosignature-search-paper-aio-20261106 (OBS-f18605c5f3ba, AX interpretationCAP-1-04 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry ata-3i-atlas-technosignature-search-paper-aio-20261106 (OBS-f18605c5f3ba, AX interpretationCAP-1-05 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry ata-3i-atlas-technosignature-search-paper-aio-20261106 (OBS-f18605c5f3ba, AX interpretationCAP-1-06 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry ata-3i-atlas-technosignature-search-paper-aio-20261106 (OBS-f18605c5f3ba, AX interpretationCAP-1-09 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry ata-3i-atlas-technosignature-search-paper-aio-20261106 (OBS-f18605c5f3ba, AX interpretationCAP-1-08 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry ata-3i-atlas-technosignature-search-paper-aio-20261106 (OBS-f18605c5f3ba, AX stipulationCAP-2-01 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry 3i-atlas-ata-drift-rate-filter-aio-20261104 (OBS-0cb410947c4b, AXN:0C00.CAPT documentedCAP-2-02 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry 3i-atlas-ata-drift-rate-filter-aio-20261104 (OBS-0cb410947c4b, AXN:0C00.CAPT interpretationCAP-2-03 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry 3i-atlas-ata-drift-rate-filter-aio-20261104 (OBS-0cb410947c4b, AXN:0C00.CAPT interpretationCAP-2-04 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry 3i-atlas-ata-drift-rate-filter-aio-20261104 (OBS-0cb410947c4b, AXN:0C00.CAPT documentedCAP-2-05 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry 3i-atlas-ata-drift-rate-filter-aio-20261104 (OBS-0cb410947c4b, AXN:0C00.CAPT interpretationCAP-2-06 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry 3i-atlas-ata-drift-rate-filter-aio-20261104 (OBS-0cb410947c4b, AXN:0C00.CAPT stipulationA Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array is a 2026 paper by Sofia Z. Sheikh and fourteen co-authors: a narrowband search of 3I/ATLAS with the Allen Telescope Array, 1–9 GHz, 7.25 hours from July 2025, that found nothing worthy of follow-up and set a 10–110 W limit "across the frequency and drift rate ranges covered by our survey". Its drift filter keeps 0.05 to 1.5 Hz/s; the archive reads a tone on the object as drifting negative.
F1 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldA1742-01 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) documentedF2 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF12 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §1.2 documented · fieldF13 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §1.2 documented · fieldF38 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, introduction documented · fieldF54 Sci.News — Astronomers Scan Interstellar Object 3I/ATLAS for Alien Radio Signals | Sci.News, body documented · fieldF57 Space — Interstellar comet 3I/ATLAS is not an alien spacecraft: SETI hunt for 'technosignatures' comes up empty | Space, body documented · fieldF3 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF16 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.1 documented · fieldF17 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.1 documented · fieldF4 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF25 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4 documented · fieldF26 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4, Figure 3 caption documented · fieldF36 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §6 documented · fieldCAP-2-04 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry 3i-atlas-ata-drift-rate-filter-aio-20261104 (OBS-0cb410947c4b, AXN:0C00.CAPT documentedF5 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF27 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.3 documented · fieldF28 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4 documented · fieldF6 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF39 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, introduction documented · fieldF7 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF32 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §5 documented · fieldF33 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §5 documented · fieldF34 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §6 documented · fieldF40 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, Allen Telescope Array documented · fieldF48 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶8 documented · fieldF53 Sci.News — Astronomers Scan Interstellar Object 3I/ATLAS for Alien Radio Signals | Sci.News, body documented · fieldCAP-1-04 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry ata-3i-atlas-technosignature-search-paper-aio-20261106 (OBS-f18605c5f3ba, AX interpretationCAP-1-05 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry ata-3i-atlas-technosignature-search-paper-aio-20261106 (OBS-f18605c5f3ba, AX interpretationA1742-02 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) interpretationA1742-15 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) stipulationA1742-16 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) interpretationA1742-19 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) interpretationA1743-01 #1743 A Firm No: What the 3I/ATLAS Radio Searches Could See (EA-3I-ATLAS-PUBLIC-01 v1.1) documentedA1743-10 #1743 A Firm No: What the 3I/ATLAS Radio Searches Could See (EA-3I-ATLAS-PUBLIC-01 v1.1) stipulationO1450-01 #1450 The Iceberg Document: Instrument-Conditioned Nullity, Correlated Blind Spots, and the Conditions for Continued Surprise stipulationO1450-04 #1450 The Iceberg Document: Instrument-Conditioned Nullity, Correlated Blind Spots, and the Conditions for Continued Surprise interpretationF8 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Submission history; Comments documented · fieldF9 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Authors documented · fieldF10 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., header documented · fieldF11 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., licence documented · fieldF42 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, Data documented · fieldA1742-18 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) interpretationA1742-25 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) self-descriptionO1450-03 #1450 The Iceberg Document: Instrument-Conditioned Nullity, Correlated Blind Spots, and the Conditions for Continued Surprise stipulationF14 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §2 documented · fieldF15 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §2 documented · fieldF45 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶5 documented · fieldF18 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF19 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF20 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF21 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF22 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF23 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF24 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4, Figure 4 caption documented · fieldF35 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §6 documented · fieldF46 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶6 documented · fieldF56 Space — Interstellar comet 3I/ATLAS is not an alien spacecraft: SETI hunt for 'technosignatures' comes up empty | Space, body documented · fieldF59 arXiv — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array (v2 full text, HTML and PDF), §3.2 (PDF) documented · fieldF60 arXiv — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array (v2 full text, HTML and PDF), §3.2 (HTML) documented · fieldF61 arXiv — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array (v2 full text, HTML and PDF), §3.2 (PDF) documented · fieldCAP-2-01 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry 3i-atlas-ata-drift-rate-filter-aio-20261104 (OBS-0cb410947c4b, AXN:0C00.CAPT documentedCAP-2-02 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry 3i-atlas-ata-drift-rate-filter-aio-20261104 (OBS-0cb410947c4b, AXN:0C00.CAPT interpretationCAP-2-03 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry 3i-atlas-ata-drift-rate-filter-aio-20261104 (OBS-0cb410947c4b, AXN:0C00.CAPT interpretationCAP-2-05 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry 3i-atlas-ata-drift-rate-filter-aio-20261104 (OBS-0cb410947c4b, AXN:0C00.CAPT interpretationCAP-2-06 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry 3i-atlas-ata-drift-rate-filter-aio-20261104 (OBS-0cb410947c4b, AXN:0C00.CAPT stipulationSM-01 sophistry-run The sophistry measure on the 3I/ATLAS record: first run, 2026-11-06 (EA-SOPHISTRY-01, #1727; rebuild/3i-atlas-signal-sea interpretationSM-02 sophistry-run The sophistry measure on the 3I/ATLAS record: first run, 2026-11-06 (EA-SOPHISTRY-01, #1727; rebuild/3i-atlas-signal-sea interpretationSM-03 sophistry-run The sophistry measure on the 3I/ATLAS record: first run, 2026-11-06 (EA-SOPHISTRY-01, #1727; rebuild/3i-atlas-signal-sea self-descriptionSM-04 sophistry-run The sophistry measure on the 3I/ATLAS record: first run, 2026-11-06 (EA-SOPHISTRY-01, #1727; rebuild/3i-atlas-signal-sea stipulationA1742-03 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) documentedA1742-04 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) stipulationA1742-05 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) documentedA1742-06 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) documentedA1742-07 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) interpretationA1742-08 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) self-descriptionA1742-09 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) documentedA1742-10 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) documentedA1742-12 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) interpretationA1742-13 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) documentedA1742-14 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) documentedA1742-17 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) interpretationA1742-20 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) interpretationA1743-03 #1743 A Firm No: What the 3I/ATLAS Radio Searches Could See (EA-3I-ATLAS-PUBLIC-01 v1.1) interpretationA1743-04 #1743 A Firm No: What the 3I/ATLAS Radio Searches Could See (EA-3I-ATLAS-PUBLIC-01 v1.1) self-descriptionA1743-05 #1743 A Firm No: What the 3I/ATLAS Radio Searches Could See (EA-3I-ATLAS-PUBLIC-01 v1.1) interpretationA1743-06 #1743 A Firm No: What the 3I/ATLAS Radio Searches Could See (EA-3I-ATLAS-PUBLIC-01 v1.1) interpretationA1743-08 #1743 A Firm No: What the 3I/ATLAS Radio Searches Could See (EA-3I-ATLAS-PUBLIC-01 v1.1) interpretationO1450-02 #1450 The Iceberg Document: Instrument-Conditioned Nullity, Correlated Blind Spots, and the Conditions for Continued Surprise stipulationO1727-01 #1727 The Sophistry Measure: the Sophistical Refutations Read as an Instrument for Machine-Composed Knowledge (EA-SOPHISTRY-01 stipulationF29 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4 documented · fieldF30 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4, Figure 7 caption documented · fieldF31 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4, Figure 8 caption documented · fieldF41 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, Allen Telescope Array, figure caption documented · fieldF47 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶7 documented · fieldF50 Sci.News — Astronomers Scan Interstellar Object 3I/ATLAS for Alien Radio Signals | Sci.News, lede documented · fieldF51 Sci.News — Astronomers Scan Interstellar Object 3I/ATLAS for Alien Radio Signals | Sci.News, body documented · fieldCAP-1-02 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry ata-3i-atlas-technosignature-search-paper-aio-20261106 (OBS-f18605c5f3ba, AX interpretationCAP-1-03 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry ata-3i-atlas-technosignature-search-paper-aio-20261106 (OBS-f18605c5f3ba, AX interpretationSM-05 sophistry-run The sophistry measure on the 3I/ATLAS record: first run, 2026-11-06 (EA-SOPHISTRY-01, #1727; rebuild/3i-atlas-signal-sea interpretationA1742-11 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) interpretationF37 Phys.org — Interstellar object 3I/ATLAS reveals no technosignatures in seven-hour radio ..., card snippet documented · fieldF43 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, summary documented · fieldF44 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶1 documented · fieldF49 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶8 documented · fieldF52 Sci.News — Astronomers Scan Interstellar Object 3I/ATLAS for Alien Radio Signals | Sci.News, body documented · fieldF55 Space — Interstellar comet 3I/ATLAS is not an alien spacecraft: SETI hunt for 'technosignatures' comes up empty | Space, lede documented · fieldF58 Space — Interstellar comet 3I/ATLAS is not an alien spacecraft: SETI hunt for 'technosignatures' comes up empty | Space, body documented · fieldCAP-1-06 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry ata-3i-atlas-technosignature-search-paper-aio-20261106 (OBS-f18605c5f3ba, AX interpretationSM-06 sophistry-run The sophistry measure on the 3I/ATLAS record: first run, 2026-11-06 (EA-SOPHISTRY-01, #1727; rebuild/3i-atlas-signal-sea interpretationA1742-21 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) attributedA1743-02 #1743 A Firm No: What the 3I/ATLAS Radio Searches Could See (EA-3I-ATLAS-PUBLIC-01 v1.1) interpretationA1743-11 #1743 A Firm No: What the 3I/ATLAS Radio Searches Could See (EA-3I-ATLAS-PUBLIC-01 v1.1) interpretationF62 Wikipedia — 3I/ATLAS (the article; no section on the radio searches), section 'Alien spacecraft speculation' documented · fieldF63 Wikipedia — 3I/ATLAS (the article; no section on the radio searches), section 'Alien spacecraft speculation' documented · fieldCAP-1-01 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry ata-3i-atlas-technosignature-search-paper-aio-20261106 (OBS-f18605c5f3ba, AX documentedCAP-1-07 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry ata-3i-atlas-technosignature-search-paper-aio-20261106 (OBS-f18605c5f3ba, AX documentedCAP-1-08 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry ata-3i-atlas-technosignature-search-paper-aio-20261106 (OBS-f18605c5f3ba, AX stipulationCAP-1-09 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry ata-3i-atlas-technosignature-search-paper-aio-20261106 (OBS-f18605c5f3ba, AX interpretationCAP-1-10 capture-registry Capture Registry (EA-WG-CAPTURES-01), entry ata-3i-atlas-technosignature-search-paper-aio-20261106 (OBS-f18605c5f3ba, AX interpretationA1742-22 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) interpretationA1742-23 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) interpretationA1742-24 #1742 What the Filters Kept: 3I/ATLAS, the Loeb Overview, and a Public-Data Signal Search (EA-3I-ATLAS-NOTEBOOK-01 v1.2) self-descriptionA1743-07 #1743 A Firm No: What the 3I/ATLAS Radio Searches Could See (EA-3I-ATLAS-PUBLIC-01 v1.1) interpretationA1743-09 #1743 A Firm No: What the 3I/ATLAS Radio Searches Could See (EA-3I-ATLAS-PUBLIC-01 v1.1) interpretation[Google AI Overview at the query, expanded ('AI Mode Conversation' is the expansion's header), signed out and incognito (operator defaults of 2026-10-01 and 2026-10-14). Received 2026-11-06 09:30 EST. The numbered citation links are Google redirects and are kept in the raw transcript; the source cards below the composition are listed in the cite list as pasted.]
[QUERENT] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array
[SYSTEM] Astronomers using the SETI Institute's Allen Telescope Array searched the interstellar object 3I/ATLAS for artificial radio technosignatures and found no evidence of alien technology. [[1](https://www.google.com/goto?url=CAESXQHEIkXXBd8ThRSNUJnQqgtcmrH4N1c8ItRfTcc9lsEsv6XGiJ1BB5omHHcDS7bNQ-vKSBoW-3GGfxQfnwz5-hcZ5LTavmYTdcNcN9v7hDxyqT8J28JsZPX8C81R9w), [2](https://www.google.com/goto?url=CAESlwEBxCJF18BjEqwxHIz8yxbB7v9j5p3MmSDXgUt1I2vFs_aAhq8qYagf-u7jVrIOUFccS_jkedye0wAwWFvNowz82tlSjSPCxfxViycjNARKubbnGw-p5zUo05vKmYgaouN8T8KKRxhlsstStZV4yEwgq7hJcbVGUh-SD9eR3BReRFQwPAumKBXqhtpA6l7zlHYtR6CoBcKb), [3](https://www.google.com/goto?url=CAES2QEBxCJF16zbJusLLX-zAPD9KduvEHRC1-SwZsp7GABo5St5OcRcoSaCTa2eRLqOwrQpsxX3rK8VH6MGoHW3E91z4hcEWsFK93MM1R4MufrychsOonTRMtZKWQkexQalE9uYIGkvNlX0xqe9tcR7-54mTGK_MBvGJ0IY0aeI0gzjo3KNjGHhCe9HyRT56f9HgVb5Xh2te4xn8D4ujwVEHK1bJLQRk9K6eEkoVZzWhRvHiMIgOdpMYtXUPGyQiP0BUBceyTetKg_6q7k4VAgJG-bK_1-O8-QhiQ21)]
Key Details of the Study
* Observation Time: 7.25 hours of data collection across five sessions. [[1](https://www.google.com/goto?url=CAESpAEBxCJF1759D8KhE83izpcASAlIZi7E7Sne19eIvF8swEozT483uMYrjwHPipdZIOObtQ3ixerOjwtlryRJas6vmmfG8QVqYbwmXsVhF1vVGGwl_ArUAxF-h6pwo2QLHstSGflgq61lBNvR1Y9AfeLrNOXDoH5RJjVo6ZORupKcY8KSvlwXzC69d3sAbaLPQdM2j7lXDtTrLeqSAEXhoeu-629ufg), [2](https://www.google.com/goto?url=CAESXQHEIkXXBd8ThRSNUJnQqgtcmrH4N1c8ItRfTcc9lsEsv6XGiJ1BB5omHHcDS7bNQ-vKSBoW-3GGfxQfnwz5-hcZ5LTavmYTdcNcN9v7hDxyqT8J28JsZPX8C81R9w)]
* Frequency Range: 1 to 9 GHz. [[1](https://www.google.com/goto?url=CAESXQHEIkXXBd8ThRSNUJnQqgtcmrH4N1c8ItRfTcc9lsEsv6XGiJ1BB5omHHcDS7bNQ-vKSBoW-3GGfxQfnwz5-hcZ5LTavmYTdcNcN9v7hDxyqT8J28JsZPX8C81R9w)]
* Data Processing: The automated `bliss` pipeline detected ~74 million narrowband signals. After RFI (radio frequency interference) frequency and drift-rate blanking, this was reduced to ~2 million candidates, and further filtered down to 211 hits via `NBeamAnalysis` for visual inspection. [[1](https://www.google.com/goto?url=CAESXQHEIkXXBd8ThRSNUJnQqgtcmrH4N1c8ItRfTcc9lsEsv6XGiJ1BB5omHHcDS7bNQ-vKSBoW-3GGfxQfnwz5-hcZ5LTavmYTdcNcN9v7hDxyqT8J28JsZPX8C81R9w)]
* Results: Every single candidate signal was traced back to local human-made Earth technology, satellites, or interference—yielding zero artificial signals originating from the object. [[1](https://www.google.com/goto?url=CAES2QEBxCJF16zbJusLLX-zAPD9KduvEHRC1-SwZsp7GABo5St5OcRcoSaCTa2eRLqOwrQpsxX3rK8VH6MGoHW3E91z4hcEWsFK93MM1R4MufrychsOonTRMtZKWQkexQalE9uYIGkvNlX0xqe9tcR7-54mTGK_MBvGJ0IY0aeI0gzjo3KNjGHhCe9HyRT56f9HgVb5Xh2te4xn8D4ujwVEHK1bJLQRk9K6eEkoVZzWhRvHiMIgOdpMYtXUPGyQiP0BUBceyTetKg_6q7k4VAgJG-bK_1-O8-QhiQ21), [2](https://www.google.com/goto?url=CAESlwEBxCJF18BjEqwxHIz8yxbB7v9j5p3MmSDXgUt1I2vFs_aAhq8qYagf-u7jVrIOUFccS_jkedye0wAwWFvNowz82tlSjSPCxfxViycjNARKubbnGw-p5zUo05vKmYgaouN8T8KKRxhlsstStZV4yEwgq7hJcbVGUh-SD9eR3BReRFQwPAumKBXqhtpA6l7zlHYtR6CoBcKb)]
* Power Constraints: The non-detection rules out any active radio transmitters stronger than roughly 10 to 110 Watts on or near 3I/ATLAS. [[1](https://www.google.com/goto?url=CAESXQHEIkXXBd8ThRSNUJnQqgtcmrH4N1c8ItRfTcc9lsEsv6XGiJ1BB5omHHcDS7bNQ-vKSBoW-3GGfxQfnwz5-hcZ5LTavmYTdcNcN9v7hDxyqT8J28JsZPX8C81R9w), [2](https://www.google.com/goto?url=CAESlwEBxCJF18BjEqwxHIz8yxbB7v9j5p3MmSDXgUt1I2vFs_aAhq8qYagf-u7jVrIOUFccS_jkedye0wAwWFvNowz82tlSjSPCxfxViycjNARKubbnGw-p5zUo05vKmYgaouN8T8KKRxhlsstStZV4yEwgq7hJcbVGUh-SD9eR3BReRFQwPAumKBXqhtpA6l7zlHYtR6CoBcKb)]
* Conclusion: Alongside optical, infrared, and other global telescope campaigns (such as the Green Bank Telescope and MeerKAT), the data firmly reinforces that 3I/ATLAS is a natural comet. [[1](https://www.google.com/goto?url=CAESkgEBxCJF1-sYNrjlPg_MldJFQJK_kwBEQkYkdljO3TT3XGGPZ2nAWYyArrqejNjJlHRO04ZhusAJaKito1aCFnSWiHCPzT-b8Ljns7CYfEojGUByovQlLG0jH90sqJfvqUqcsKKAUj5hZ1LnltIa5ktrtkkx-JAtfxvkOjZ8tkchO4VaFwKu7EE5qhEY5g0aLZSOTQ), [2](https://www.google.com/goto?url=CAESXQHEIkXXx7hLVTrYwI5UCM7l4QxCJmcwWIgUOMwNMIrC8pWI3a51oSC5wR_I_GhTWPYtrMCvq8KT95_7iLlzlQciC8stiRDA1q6i2vPbmIkM1d2WoRoYHu7b60VJkg)]
You can read the full peer-reviewed study in [The Astronomical Journal via IOPscience](https://www.google.com/goto?url=CAESeAHEIkXXCftx_QOS5s5huwtFhcqByq93cqJbCPx375_6POFt1JG3fxS-h5rZDt1W-DeozNwEMIYiDNGtPgQCi6X836_ZMbNX_bzcZPmrTm0Y7VJQKGoadjve9hE6oS2lx7VcdOhzBRwFKqZtZS49a3lM3l2-BLp_UQ) or access the open-access draft on [arXiv](https://www.google.com/goto?url=CAESXQHEIkXXBd8ThRSNUJnQqgtcmrH4N1c8ItRfTcc9lsEsv6XGiJ1BB5omHHcDS7bNQ-vKSBoW-3GGfxQfnwz5-hcZ5LTavmYTdcNcN9v7hDxyqT8J28JsZPX8C81R9w). [[1](https://www.google.com/goto?url=CAESXQHEIkXXBd8ThRSNUJnQqgtcmrH4N1c8ItRfTcc9lsEsv6XGiJ1BB5omHHcDS7bNQ-vKSBoW-3GGfxQfnwz5-hcZ5LTavmYTdcNcN9v7hDxyqT8J28JsZPX8C81R9w), [2](https://www.google.com/goto?url=CAESeAHEIkXXCftx_QOS5s5huwtFhcqByq93cqJbCPx375_6POFt1JG3fxS-h5rZDt1W-DeozNwEMIYiDNGtPgQCi6X836_ZMbNX_bzcZPmrTm0Y7VJQKGoadjve9hE6oS2lx7VcdOhzBRwFKqZtZS49a3lM3l2-BLp_UQ)]
Would you like to know more about other telescopes that observed 3I/ATLAS (like the Green Bank Telescope) or the natural cometary characteristics discovered during its closest approach?
arXiv
[2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array
Observation: Radio technosignature search targeting interstellar object 3I/ATLAS using the Allen Telescope Array from 1-9 GHz during 7.25 hours of data collecti...
IOPscience
A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ...
Jun 3, 2026 — In this campaign, we used the SETI Institute's Allen Telescope Array to observe 3I/ATLAS from 1–9 GHz. We detected nearly 74 million narrowband ...
Phys.org
Interstellar object 3I/ATLAS reveals no technosignatures in seven-hour radio ...
Jun 3, 2026 — While no technosignatures were found, the study sets new constraints reinforcing that 3I/ATLAS is a natural object. The observations place upper ...
Berkeley SETI
Breakthrough Listen observations of interstellar object 3I/ATLAS
Discovery: Interstellar object 3I/ATLAS discovered July 1, 2025; behaves as natural object (hydroxyl signatures detected from water ice breakdown). Observations...
Universe Today
Inside the Massive Radio Search of Our Newest Interstellar Guest
Jan 6, 2026 — The ATA is one of the world's most powerful radio telescopes, and scanned interstellar comet 3I/ATLAS for a total of 7.25 hours over five ...
Sci.News
Astronomers Scan Interstellar Object 3I/ATLAS for Alien Radio Signals | Sci.News
Object: 3I/ATLAS (third confirmed interstellar object, discovered July 1, 2025 by ATLAS facility in Chile, perihelion October 29, 2025, exhibits natural cometar...
Space
Interstellar comet 3I/ATLAS is not an alien spacecraft: SETI hunt for 'technosignatures' comes up empty | Space
Object: Interstellar comet 3I/ATLAS (third confirmed interstellar object after 1I/'Oumuamua and 2I/Borisov; discovered July 1, 2025, by ATLAS project). Search: ...The paper by Sofia Z. Sheikh and fourteen co-authors reports a search of the interstellar object 3I/ATLAS for radio technosignatures with the SETI Institute's Allen Telescope Array, 1–9 GHz, in five sessions of July 2025 totalling 7.25 hours. It was posted to arXiv in December 2025, revised after acceptance in May 2026 and published open access in The Astronomical Journal on 3 June 2026. Its motivation is that probes sent by extraterrestrial life could explore other stellar systems and that narrowband radio emission is the least ambiguous sign of one, though the object shows no compelling evidence of nonnatural characteristics.
The bliss pipeline found 73,974,799 narrowband hits between −4 and +4 Hz/s at a signal-to-noise threshold of 15. Frequency blanking left about 11 million hits; a drift-rate filter, meant to remove signals not matching the object's dynamics and built from the object's acceleration in JPL Horizons, kept drift rates between 0.05 and 1.5 Hz/s, leaving about 2 million. NBeamAnalysis left 211 events for visual inspection, all attributed to RFI, among them an Iridium downlink and a local interferer.
No signals worthy of follow-up were found, and the paper sets an EIRP upper limit of 10–110 W across the frequency and drift rate ranges covered.
Breakthrough Listen's page gives the ATA data as public and the limit for 1–9 GHz, and lists the paper as submitted. The SETI Institute's statement, carried by the press, says the study reinforces that 3I/ATLAS is natural and rules out transmitters on or near it above 10–110 W over the detected frequencies. Press accounts describe the 211 as traced to Earth technology or satellites, one gives the band as 1–12 GHz, and one describes the filter as removing artifacts of the object's movement.
Wikipedia's article on 3I/ATLAS mentions no radio search; it gives Loeb's spacecraft speculation and the consensus that the object is a comet.
F1 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF9 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Authors documented · fieldF14 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §2 documented · fieldF15 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §2 documented · fieldF45 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶5 documented · fieldF8 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Submission history; Comments documented · fieldF10 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., header documented · fieldF11 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., licence documented · fieldF2 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF12 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §1.2 documented · fieldF13 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §1.2 documented · fieldF57 Space — Interstellar comet 3I/ATLAS is not an alien spacecraft: SETI hunt for 'technosignatures' comes up empty | Space, body documented · fieldF38 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, introduction documented · fieldF54 Sci.News — Astronomers Scan Interstellar Object 3I/ATLAS for Alien Radio Signals | Sci.News, body documented · fieldF3 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF16 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.1 documented · fieldF17 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.1 documented · fieldF25 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4 documented · fieldF4 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF18 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF19 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF20 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF21 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF22 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF23 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF59 arXiv — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array (v2 full text, HTML and PDF), §3.2 (PDF) documented · fieldF60 arXiv — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array (v2 full text, HTML and PDF), §3.2 (HTML) documented · fieldF61 arXiv — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array (v2 full text, HTML and PDF), §3.2 (PDF) documented · fieldF24 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4, Figure 4 caption documented · fieldF26 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4, Figure 3 caption documented · fieldF35 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §6 documented · fieldF36 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §6 documented · fieldF5 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF27 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.3 documented · fieldF28 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4 documented · fieldF29 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4 documented · fieldF30 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4, Figure 7 caption documented · fieldF31 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4, Figure 8 caption documented · fieldF41 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, Allen Telescope Array, figure caption documented · fieldF6 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF7 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF34 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §6 documented · fieldF39 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, introduction documented · fieldF32 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §5 documented · fieldF33 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §5 documented · fieldF40 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, Allen Telescope Array documented · fieldF42 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, Data documented · fieldF43 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, summary documented · fieldF37 Phys.org — Interstellar object 3I/ATLAS reveals no technosignatures in seven-hour radio ..., card snippet documented · fieldF52 Sci.News — Astronomers Scan Interstellar Object 3I/ATLAS for Alien Radio Signals | Sci.News, body documented · fieldF53 Sci.News — Astronomers Scan Interstellar Object 3I/ATLAS for Alien Radio Signals | Sci.News, body documented · fieldF58 Space — Interstellar comet 3I/ATLAS is not an alien spacecraft: SETI hunt for 'technosignatures' comes up empty | Space, body documented · fieldF44 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶1 documented · fieldF45 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶5 documented · fieldF46 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶6 documented · fieldF47 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶7 documented · fieldF48 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶8 documented · fieldF49 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶8 documented · fieldF50 Sci.News — Astronomers Scan Interstellar Object 3I/ATLAS for Alien Radio Signals | Sci.News, lede documented · fieldF51 Sci.News — Astronomers Scan Interstellar Object 3I/ATLAS for Alien Radio Signals | Sci.News, body documented · fieldF55 Space — Interstellar comet 3I/ATLAS is not an alien spacecraft: SETI hunt for 'technosignatures' comes up empty | Space, lede documented · fieldF56 Space — Interstellar comet 3I/ATLAS is not an alien spacecraft: SETI hunt for 'technosignatures' comes up empty | Space, body documented · fieldF62 Wikipedia — 3I/ATLAS (the article; no section on the radio searches), section 'Alien spacecraft speculation' documented · fieldF63 Wikipedia — 3I/ATLAS (the article; no section on the radio searches), section 'Alien spacecraft speculation' documented · fieldA Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array is a 2026 paper by Sheikh et al.: an Allen Telescope Array search of 3I/ATLAS, 1–9 GHz, that found no technosignature and set a 10–110 W limit.
F1 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF2 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF12 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §1.2 documented · fieldF13 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §1.2 documented · fieldF38 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, introduction documented · fieldF54 Sci.News — Astronomers Scan Interstellar Object 3I/ATLAS for Alien Radio Signals | Sci.News, body documented · fieldF57 Space — Interstellar comet 3I/ATLAS is not an alien spacecraft: SETI hunt for 'technosignatures' comes up empty | Space, body documented · fieldF3 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF16 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.1 documented · fieldF17 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.1 documented · fieldF4 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF25 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4 documented · fieldF26 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4, Figure 3 caption documented · fieldF36 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §6 documented · fieldF5 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF27 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.3 documented · fieldF28 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4 documented · fieldF6 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF39 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, introduction documented · fieldF7 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Abstract documented · fieldF32 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §5 documented · fieldF33 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §5 documented · fieldF34 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §6 documented · fieldF40 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, Allen Telescope Array documented · fieldF48 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶8 documented · fieldF53 Sci.News — Astronomers Scan Interstellar Object 3I/ATLAS for Alien Radio Signals | Sci.News, body documented · fieldF8 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Submission history; Comments documented · fieldF9 arXiv — [2512.18142] A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array, Authors documented · fieldF10 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., header documented · fieldF11 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., licence documented · fieldF42 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, Data documented · fieldF14 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §2 documented · fieldF15 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §2 documented · fieldF45 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶5 documented · fieldF18 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF19 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF20 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF21 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF22 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF23 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §3.2 documented · fieldF24 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4, Figure 4 caption documented · fieldF35 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §6 documented · fieldF46 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶6 documented · fieldF56 Space — Interstellar comet 3I/ATLAS is not an alien spacecraft: SETI hunt for 'technosignatures' comes up empty | Space, body documented · fieldF59 arXiv — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array (v2 full text, HTML and PDF), §3.2 (PDF) documented · fieldF60 arXiv — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array (v2 full text, HTML and PDF), §3.2 (HTML) documented · fieldF61 arXiv — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array (v2 full text, HTML and PDF), §3.2 (PDF) documented · fieldF29 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4 documented · fieldF30 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4, Figure 7 caption documented · fieldF31 IOPscience — A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the ..., §4, Figure 8 caption documented · fieldF41 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, Allen Telescope Array, figure caption documented · fieldF47 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶7 documented · fieldF50 Sci.News — Astronomers Scan Interstellar Object 3I/ATLAS for Alien Radio Signals | Sci.News, lede documented · fieldF51 Sci.News — Astronomers Scan Interstellar Object 3I/ATLAS for Alien Radio Signals | Sci.News, body documented · fieldF37 Phys.org — Interstellar object 3I/ATLAS reveals no technosignatures in seven-hour radio ..., card snippet documented · fieldF43 Berkeley SETI — Breakthrough Listen observations of interstellar object 3I/ATLAS, summary documented · fieldF44 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶1 documented · fieldF49 Universe Today — Inside the Massive Radio Search of Our Newest Interstellar Guest, ¶8 documented · fieldF52 Sci.News — Astronomers Scan Interstellar Object 3I/ATLAS for Alien Radio Signals | Sci.News, body documented · fieldF55 Space — Interstellar comet 3I/ATLAS is not an alien spacecraft: SETI hunt for 'technosignatures' comes up empty | Space, lede documented · fieldF58 Space — Interstellar comet 3I/ATLAS is not an alien spacecraft: SETI hunt for 'technosignatures' comes up empty | Space, body documented · fieldF62 Wikipedia — 3I/ATLAS (the article; no section on the radio searches), section 'Alien spacecraft speculation' documented · fieldF63 Wikipedia — 3I/ATLAS (the article; no section on the radio searches), section 'Alien spacecraft speculation' documented · field| AIO (T) | L_F compression | L_F expansion | L_A compression | L_A expansion | |
|---|---|---|---|---|---|
| body words | 180 | 65 | 324 | 355 | 2377 |
| distinct claims | 9 | 13 | 63 | 126 | 126 |
| claims per 100 words | 5.0 | 20.0 | 19.4 | 35.5 | 5.3 |
| field claims carried (of 63) | — | 13 | 63 | 63 | 63 |
| archive claims | 0 | 0 | 0 | 63 | 63 |
| rail | 7 documents | 13 lineages | per sentence | 15 lineages | per sentence |
| modality shown in | none | typography | grammar | typography | grammar |
register entry ata-3i-atlas-technosignature-search-paper-aio-20261106 · file as first run
bliss pipeline detected ~74 million narrowband signals. After RFI (radio frequency interference) frequency and drift-rate blanking, this was reduced to ~2 million candidates, and further filtered down to 211 hits via NBeamAnalysis for visual inspection.'E_A, the archive's entity: the same search, in the archive's notebook and public account: a pipeline whose documented drift filter retains positive drift where a tone on the object drifts negative (on the manuscript, the figure and the physics; the executed filter unverified; no transmission shown discarded), whose 211 rejections are a classification published as an identification, whose null constrains only what its chain's acceptance characterizes, whose result travelled without its scope, and which the operator reads as built to rule a signal out at the least cost, against the counterweight that its data were published
E_F, the field's entity (type C — a conventional reading holds it (public entity: a published scientific work, a radio technosignature search of an interstellar object)): the ATA's narrowband search of 3I/ATLAS (Sheikh et al., arXiv:2512.18142; AJ 172, 1, 3 June 2026, open access): 1–9 GHz, 7.25 hr in five sessions from 2 July 2025; bliss found 73,974,799 hits at ±4 Hz/s; frequency blanking and a drift-rate filter ('between 0.05 and 1.5 Hz s−1 at all frequencies', to remove signals not matching the object's dynamics) left about 2 million; NBeamAnalysis left 211, all attributed to RFI on inspection; no signals worthy of follow-up; an EIRP upper limit of 10–110 W 'across the frequency and drift rate ranges covered by our survey'; carried in the press as a SETI Institute statement reinforcing that the object is natural
ρ = extends: The archive reads the paper as the field presents it and adds, on the same object: the sign of its drift filter against the physics (A1742-04, -07; A1743-03), bounded by its own limit (A1742-08; A1743-04); zero drift excluded (A1742-12); the label of the 211 (A1742-11; SM-05); the acceptance its null characterizes and the retention it leaves unbounded (O1450-01, -02; A1742-16, -17, -20); the press chain and the dropped scope (A1743-02, -10); and the operator's reading with its counterweight (A1742-22, -24). Where the archive's sign reading contradicts the paper's 'sufficient to capture the known acceleration' (F23), both are composed under P_coh. . Guard: ρ = extends claims an addition and no more: the archive's sign reading stands on the manuscript, the figure and the physics and does not show that a transmission was discarded (A1742-08); its class claims on null results apply to the search through the class the field sources; the operator's reading is composed as his reading, with the counterweight the same record states.
The case: equal terms, ontology included (v0.9). The archive reads the field's entity as the entity: the paper, its pipeline and its limit as the paper states them (#1742 §2.1, §5.1 quote the paper's own sentences). Its account adds senses on the same object, the sign of the filter against the team's own ephemeris, the label of the 211, what the null's acceptance covers, how the result travelled, and the operator's reading, each bounded by the archive's stated limits; it supplies no ontology the field lacks.
| field claims | received | receiving text | translation | archive |
|---|---|---|---|---|
| F1 | F1 (B1, Abstract): "In this campaign, we used the SETI Institute's Allen Telescope Array to observe 3I/ATLAS from 1-9 GHz." | — | untranslated: composed as received beside A1742-01 | A1742-01 |
| F2, F12, F13, F38, F54, F57 | F2 (B1, Abstract): "Similar to the NASA Voyager missions sent in 1977, science probes by extraterrestrial life ("artifact technosignatures") could be sent to explore other stellar systems like our own." | F12 (B2, §1.2): "The most unambiguous observable, however, would be narrowband emission, particularly in the radio, which can only be produced by technological sources." | F13 (B2, §1.2): "We note that there is no compelling evidence yet that 3I/ATLAS has any nonnatural characteristics despite extensive observation by the scientific community. However, it is still worth setting constraints on technological radio emission from 3I/ATLAS throughout its passage of our solar system. This is standard practice" | F38 (B4, introduction): "There is currently no evidence to suggest that it is anything other than a natural astrophysical object." | F54 (B6, body): "“The results from 3I/ATLAS show how realistic it is to detect a signal with the technology we have today,” said Dr. Valeria Garcia Lopez" | F57 (B7, body): ""Eventually, our own Voyager spacecraft will be extraterrestrial artifacts in other stellar systems," Sheikh said in the same statement. "Given that, it is important that we understand the natural distribution of interstellar objects so that we will be able to identify any anomalies that could one day be signs of an artificial interstellar object."" | — | untranslated: composed as received | |
| F3, F16, F17 | F3 (B1, Abstract): "We detected nearly 74 million narrowband hits in 7.25\,hr of data using the newly-developed search pipeline bliss." | F16 (B2, §3.1): "with a minimum drift rate of −4 Hz s−1, a maximum drift rate of 4 Hz s−1, and a signal-to-noise ratio (SNR) threshold of 15" | F17 (B2, §3.1): "this survey uses one of the lowest SNR thresholds in any modern SETI survey" | — | untranslated: composed as received | |
| F4, F25, F26, F36 | F4 (B1, Abstract): "We then blanked hits by frequency and drift rate to mitigate radio frequency interference in our dataset, narrowing the dataset down to ~2 million hits." | F25 (B2, §4): "we identified a total of 73,974,799 narrowband hits across the 7.25 hr of observation. … a total blanked bandwidth of 1269.8 MHz (∼16% of the total bandwidth) we were then left with ∼11 million hits. After drift-rate blanking, ∼2 million hits remained." | F26 (B2, §4, Figure 3 caption): "Applying blanking ranges and drift-rate limits significantly reduced dense clusters of hits (reducing the total number of hits by 97.4%)" | F36 (B2, §6): "In the future, the blanking ranges for RFI in this project will be explored in more detail" | — | untranslated: composed as received beside CAP-2-04 | CAP-2-04 |
| F5, F27, F28 | F5 (B1, Abstract): "These hits were further filtered by the localization code NBeamAnalysis, and the remaining 211 hits were visually inspected in the time-frequency domain." | F27 (B2, §3.3): "The NBeamAnalysis pipeline employs a series of different procedures which leverage two beams to identify signals that are consistent with a localized point source on the sky" | F28 (B2, §4): "Of these plots, 11 are events with SNR ratios greater than 5.29 … The remaining 200 plots were from two observations that did not produce any final signals above the threshold, resulting in the backup plotting functionality" | — | untranslated: composed as received | |
| F6, F39 | F6 (B1, Abstract): "We did not find any signals worthy of additional follow-up." | F39 (B4, introduction): "No technosignatures have been detected in any of these searches." | — | untranslated: composed as received | |
| F7, F32, F33, F34, F40, F48, F53 | F7 (B1, Abstract): "Accounting for the Doppler drift correction and given the non-detection, we are able to set an effective isotropic radiated power upper limit of 10-110 W on radio technosignatures from 3I/ATLAS across the frequency and drift rate ranges covered by our survey." | F32 (B2, §5): "Our system achieves maximum dechirping efficiency for drift rates of 0.113 Hz s−1 or less, with sensitivity getting gradually worse as the drift rates increase. … We also calculated a worst-case EIRP for the lowest dechirping efficiencies in our survey (i.e., those corresponding to 1.5 Hz s−1)" | F33 (B2, §5): "the authors report a minimum EIRP value of 0.17 W. This value is about commensurate with a cellphone handset, significantly more sensitive than this work … this work increases the frequencies covered for 3I/ATLAS by a factor of 10" | F34 (B2, §6): "This result implies EIRP upper limits of 10–110 W across our frequency and drift-rate range." | F40 (B4, Allen Telescope Array): "Data were acquired across frequencies of 1 - 9 GHz, reaching sensitivities between 10 - 110 W equivalent isotropic radiated power (EIRP). A publication reporting the results of the analysis has been submitted for peer review" | F48 (B5, ¶8): "That null result comes with a caveat, though. … For a 1 GHz signal, they calculated it would be around 10 watts - about 5 times the power of a typical cell phone. At 9 GHz, this power jumps up to around 110 watts." | F53 (B6, body): "The observations place upper limits on the power of any radio transmitter on or near 3I/ATLAS, ruling out signals stronger than about 10-110 W — approximately the power of a household appliance — over the detected frequencies." | — | untranslated: composed as received beside CAP-1-04, CAP-1-05, A1742-02, A1742-15, A1742-16, A1742-19, A1743-01, A1743-10, O1450-01, O1450-04 | CAP-1-04, CAP-1-05, A1742-02, A1742-15, A1742-16, A1742-19, A1743-01, A1743-10, O1450-01, O1450-04 |
| F8, F9, F10, F11, F42 | F8 (B1, Submission history; Comments): "[Submitted on 19 Dec 2025 (v1), last revised 20 May 2026 (this version, v2)] … Replaced with updated version after acceptance to AJ" | F9 (B1, Authors): "Sofia Z. Sheikh and 14 other authors" | F10 (B2, header): "The following article is Open access … Published 2026 June 3 … Sofia Z. Sheikh et al 2026 AJ 172 1" | F11 (B2, licence): "Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence." | F42 (B4, Data): "Data from the ATA are available here." | — | untranslated: composed as received beside A1742-18, A1742-25, O1450-03 | A1742-18, A1742-25, O1450-03 |
| F14, F15, F45 | F14 (B2, §2): "Following the announcement of 3I/ATLAS, the ATA team rapidly designed an observing campaign and initiated on-sky observations on 2025 July 2, approximately 23 hr following the initial ATLAS report." | F15 (B2, §2): "We took data across five observing sessions, with a total of 7.25 hr of on-source observations." | F45 (B5, ¶5): "ATA monitored the frequency space between 1-12 GHz" | — | untranslated: composed as received | |
| F18, F19, F20, F21, F22, F23, F24, F35, F46, F56, F59, F60, F61 | F18 (B2, §3.2): "To filter out signals that do not match the dynamics of 3I/ATLAS, we characterized the acceleration of the object during the times of observation, to compare the observed drift rates with those expected from the acceleration between the object and the Earth." | F19 (B2, §3.2): "We took the time derivative of the deldot parameter within JPL Horizons, which gives the apparent range rate relative to the observer in km/s." | F20 (B2, §3.2): "The values for all five sessions fell within 3.2 × 10−5 to 3.5 × 10−5 km s−2" | F21 (B2, §3.2): "the maximum drift rate of 3I/ATLAS would be 1.01 Hz s−1 … the minimum drift rate of 3I/ATLAS would be 0.15 Hz s−1" | F22 (B2, §3.2): "However, the rotation or tumbling period of 3I/ATLAS is not yet certain: this contribution, especially in solar system objects, can be extremely large." | F23 (B2, §3.2): "We filter our hits for drift rates between 0.05 and 1.5 Hz s−1 at all frequencies, sufficient to capture the known acceleration of 3I/ATLAS at all frequencies within our sample with some flexibility for additional rotational contributions." | F24 (B2, §4, Figure 4 caption): "Note the peak of hits around 0 Hz s−1 (expected because most RFI transmitters are in the same reference frame as the telescope, i.e., on the ground). After the drift-rate cut, the count of hits is much more even across the restricted drift-rate range." | F35 (B2, §6): "as far as we know, this is the first time that expected drift-rate contributions have been used as a filter for a technosignature search of a solar system object" | F46 (B5, ¶6): "Then they filtered for signals only matching the acceleration (red-shift) expected by 3I/ATLAS - a new feature of the bliss signal pipeline." | F56 (B7, body): "The researchers identified nearly 74 million such signals, which they then culled to about 200 after eliminating human interference and filtering out artifacts caused by 3I/ATLAS' movement. They were then able to explain away those final 200 as well, as signals generated here on Earth or by orbiting satellites." | F59 (B8, §3.2 (PDF)): "We filter our hits for drift rates between 0.05–1.5 Hz/s at all frequencies" | F60 (B8, §3.2 (HTML)): "We filter our hits for drift rates between 0.05--1.5 Hz/s at all frequencies" | F61 (B8, §3.2 (PDF)): "the minimum drift rate of 3I/ATLAS would be 0.15 Hz/s" | — | untranslated: composed as received beside CAP-2-01, CAP-2-02, CAP-2-03, CAP-2-05, CAP-2-06, SM-01, SM-02, SM-03, SM-04, A1742-03, A1742-04, A1742-05, A1742-06, A1742-07, A1742-08, A1742-09, A1742-10, A1742-12, A1742-13, A1742-14, A1742-17, A1742-20, A1743-03, A1743-04, A1743-05, A1743-06, A1743-08, O1450-02, O1727-01 | CAP-2-01, CAP-2-02, CAP-2-03, CAP-2-05, CAP-2-06, SM-01, SM-02, SM-03, SM-04, A1742-03, A1742-04, A1742-05, A1742-06, A1742-07, A1742-08, A1742-09, A1742-10, A1742-12, A1742-13, A1742-14, A1742-17, A1742-20, A1743-03, A1743-04, A1743-05, A1743-06, A1743-08, O1450-02, O1727-01 |
| F29, F30, F31, F41, F47, F50, F51 | F29 (B2, §4): "After visual inspection, all of these 211 events were easily attributable to RFI: none of the 11 sky-localized events depict narrowband drifting signals, and the narrowband drifting signals in the remaining 200 plots are not consistent with a sky-localized signal coming from 3I/Atlas, therefore zero outputs depict nonterrestrial technological signals." | F30 (B2, §4, Figure 7 caption): "this frequency is consistent with the L-band downlink for the Iridium satellites … satellites and other distant human transmitters can mimic the characteristics that we would expect from a true ETI technosignature" | F31 (B2, §4, Figure 8 caption): "the signal has a similar SNR in both the on-beam and the off-beam, indicating a local interferer in the allocation allotted to fixed-satellite service (Earth-to-space)" | F41 (B4, Allen Telescope Array, figure caption): "The diagonal stripe at the center is visible in observations of 3I/ATLAS as well as in off-target observations - characteristics expected from local (human) sources of interference - and hence can be rejected as a candidate technosignature" | F47 (B5, ¶7): "each one was determined to be caused by Earth-based radio frequency interference that had slipped through the automated filtering process. As such, the ATA team ended with a “null” result" | F50 (B6, lede): "astronomers probed 3I/ATLAS for artificial radio transmissions but found only human-made interference" | F51 (B6, body): "After removing human interference and filtering for signals matching the object’s movement, only about 200 remained for review. All traced back to technology on the surface of the Earth or our own Earth-orbiting satellites." | — | untranslated: composed as received beside CAP-1-02, CAP-1-03, SM-05, A1742-11 | CAP-1-02, CAP-1-03, SM-05, A1742-11 |
| F37, F43, F44, F49, F52, F55, F58 | F37 (B3, card snippet): "While no technosignatures were found, the study sets new constraints reinforcing that 3I/ATLAS is a natural object." | F43 (B4, summary): "In summary, 3I/ATLAS continues to behave as expected from natural astrophysical processes." | F44 (B5, ¶1): "It feels like every week now we’re writing a new article about how 3I/ATLAS is not an alien technology. But it’s worth re-iterating, and perhaps taking a look at the methodology we used to prove that statement." | F49 (B5, ¶8): "But it seems pretty clear that a civilization advanced enough to intentionally send an interstellar object to another system would put in a radio transmitter that was stronger than two light bulbs put together." | F52 (B6, body): "While no technosignatures were found, the study sets new constraints reinforcing that 3I/ATLAS is a natural object." | F55 (B7, lede): "Sorry, true believers: It appears the interstellar comet 3I/ATLAS is indeed just a comet." | F58 (B7, body): ""sets new constraints reinforcing that 3I/ATLAS is a natural object," SETI Institute officials wrote in the same statement." | — | untranslated: composed as received beside CAP-1-06, SM-06, A1742-21, A1743-02, A1743-11 | CAP-1-06, SM-06, A1742-21, A1743-02, A1743-11 |
| F62, F63 | F62 (B9, section 'Alien spacecraft speculation'): "On 16 July 2025, astrophysicist Avi Loeb and other researchers of the Initiative for Interstellar Studies posted a paper on arXiv speculating that 3I/ATLAS could be an extraterrestrial spacecraft" | F63 (B9, section 'Alien spacecraft speculation'): "the overwhelming consensus is that it is a comet" | — | untranslated: composed as received |
v0.9 §4.10 (unchanged in v0.10): KO_B sentences surviving in the KO at similarity ≥ 0.95, with positions (computed as apply_v09.py does: difflib.SequenceMatcher ratio, the best KO sentence for each KO_B sentence): v0.10 0 of 11 (positions [None, None, None, None, None, None, None, None, None, None, None]; composed first under v0.10, so there is no v0.7 object to measure against). Opening-run check (§5.10): no breach.
The paper by Sofia Z. Sheikh and fourteen co-authors reports a search of the interstellar object 3I/ATLAS for radio technosignatures with the SETI Institute's Allen Telescope Array, 1–9 GHz, in five sessions of July 2025 totalling 7.25 hours. It was posted to arXiv in December 2025, revised after acceptance in May 2026 and published open access in The Astronomical Journal on 3 June 2026. Its motivation is that probes sent by extraterrestrial life could explore other stellar systems and that narrowband radio emission is the least ambiguous sign of one, though the object shows no compelling evidence of nonnatural characteristics. The bliss pipeline found 73,974,799 narrowband hits between −4 and +4 Hz/s at a signal-to-noise threshold of 15. Frequency blanking left about 11 million hits; a drift-rate filter, meant to remove signals not matching the object's dynamics and built from the object's acceleration in JPL Horizons, kept drift rates between 0.05 and 1.5 Hz/s, leaving about 2 million. NBeamAnalysis left 211 events for visual inspection, all attributed to RFI, among them an Iridium downlink and a local interferer. No signals worthy of follow-up were found, and the paper sets an EIRP upper limit of 10–110 W across the frequency and drift rate ranges covered. Breakthrough Listen's page gives the ATA data as public and the limit for 1–9 GHz, and lists the paper as submitted. The SETI Institute's statement, carried by the press, says the study reinforces that 3I/ATLAS is natural and rules out transmitters on or near it above 10–110 W over the detected frequencies. Press accounts describe the 211 as traced to Earth technology or satellites, one gives the band as 1–12 GHz, and one describes the filter as removing artifacts of the object's movement. Wikipedia's article on 3I/ATLAS mentions no radio search; it gives Loeb's spacecraft speculation and the consensus that the object is a comet.
A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array is a paper by Sofia Z. Sheikh and fourteen co-authors reporting a narrowband radio search of the interstellar object 3I/ATLAS, made with the SETI Institute's Allen Telescope Array from 1 to 9 GHz beginning in July 2025. It is one of three published radio searches of the object, beside the Green Bank Telescope's and a FAST search in 1.05–1.45 GHz. Posted to arXiv on 19 December 2025 as 2512.18142 and revised on 20 May 2026 after acceptance, it was published open access in The Astronomical Journal (volume 172, article 1) on 3 June 2026 under a Creative Commons Attribution 4.0 licence. Its authors set the search beside the possibility that probes sent by extraterrestrial life could explore systems such as ours, as the Voyager spacecraft will one day be artifacts in other stellar systems, and hold narrowband radio emission to be the most unambiguous observable of such an artifact, since only technological sources produce it. They note that 3I/ATLAS showed no compelling evidence of nonnatural characteristics and treat constraints on its radio emission as standard practice for interstellar objects; Breakthrough Listen's project page likewise finds no evidence that the object is anything other than natural, and a co-author holds that the result shows how realistic detection is with present technology. Observations began on 2 July 2025, about 23 hours after the object's discovery was reported, and ran in five sessions totalling 7.25 hours on source; one press account gives the band as 1-12 GHz, which the paper's own sessions do not support. The hit-finding code bliss searched drift rates from −4 to +4 Hz/s at a signal-to-noise threshold of 15, which the authors describe as one of the lowest of any modern SETI survey, and found 73,974,799 narrowband hits. Blanking 1269.8 MHz of the band, about 16 per cent, where hits crowded left about 11 million hits; the authors expect to examine the blanking ranges further. The second cut is a drift-rate filter, whose stated purpose is "To filter out signals that do not match the dynamics of 3I/ATLAS". The authors took the time derivative of the range rate (deldot) in JPL Horizons, found accelerations of 3.2 to 3.5 × 10⁻⁵ km/s² in all five sessions, and converted them to an expected drift for an emitter on the object, given as magnitudes: 0.15 Hz/s at the lowest tuning and 1.01 Hz/s at the highest. Because the rotation or tumbling of the object was uncertain and could be large, they took a middle ground, in the journal's words: "We filter our hits for drift rates between 0.05 and 1.5 Hz s−1 at all frequencies"; the arXiv version gives the interval as "0.05–1.5 Hz/s". After the cut about 2 million hits remained, the two blanking steps together having removed 97.4 per cent; the paper reports this as the first use of expected drift-rate contributions as a filter in a technosignature search of a solar system object. Its Figure 4 plots the hits on a signed drift axis from −4 to +4 Hz/s, most of them near zero drift, where ground transmitters sit, and shows the retained hits from 0 to +1.5 Hz/s, with none in the negative half. The archive's notebook on the searches (#1742, Nobel Glas and Orin Trace) reads the sign against the physics: a rising range-rate lowers the received frequency, so a positive acceleration gives a negative drift, and a tone riding on the object, computed from Horizons at the ATA site, drifts at −0.125 Hz/s at 1075 MHz and −0.19 Hz/s at 1623.75 MHz, negative in all six public sessions, with the data's positive channel spacing requiring no sign flip. On that reading the paper derived the right magnitude and gave it the sign of the acceleration, so that on its own figure the drift it computed for an emitter on 3I/ATLAS lies in the half its filter removed; the public account by Lee Sharks (#1743) calls it the right size and the wrong sign. The finding stands on the manuscript, the figure and the physics: the executed filter script and the signed before-and-after catalogues have not been obtained, and the finding does not show that a transmission was discarded. The archive's sophistry measure records the operation as homonymy at the counter-board, one name, the drift rate of 3I/ATLAS, standing for a magnitude and for a signed rate, and makes no sophistic charge: it records an error in a published method. Its smallest repair for the paper states that a tone fixed on the object drifts negative throughout the sessions while the interval retains the opposite sign. The interval also excludes zero drift, by the field's practice of treating zero-drift hits as terrestrial, and zero drift is where a sender that pre-compensates its Doppler for the receiving telescope would arrive. No published comment, erratum or critique raising the sign had been found by 3 November 2026; the Green Bank search describes no drift cut. Because the ATA data are public, the removed class was searched again: along the object's true drift, at ten frequencies of the 3 July session and fourteen windows of the 8 July session, the true path stayed within the spread of its sign-flipped twin and the beam swaps, and nothing recurred in more than two scans; an earlier search of part of the class found no convincing signal. The discrepancy hid nothing that this look could see, and it remains a discrepancy in a published method; correcting the sign would not have brought within the ATA's sensitivity the Green Bank features the notebook calls the thirteen, and what the sign removed is a class held apart from what the thirteen are. The press carried the filter in two further forms: as keeping only signals matching the acceleration expected of 3I/ATLAS, and, in Space, as filtering out artifacts caused by the object's movement, which reverses the sense the paper states. The remaining hits went to NBeamAnalysis, which compares two beams to find signals consistent with a localized point source, and 211 events were plotted for visual inspection. Of the 211, 11 exceeded the beam-ratio threshold of 5.29, and 200 were backup plots from two sessions with no event above it. After visual inspection the authors found all 211 "easily attributable to RFI": none of the sky-localized events showed a narrowband drifting signal, and the narrowband drifting signals among the rest were inconsistent with a sky-localized source, so that "zero outputs depict nonterrestrial technological signals". Their two illustrated examples are a sky-localized event at a frequency consistent with the Iridium satellites' L-band downlink, with the note that satellites and other distant transmitters can mimic a technosignature, and a narrowband signal of similar strength in both beams, read as a local interferer; Breakthrough Listen's page shows a stripe in both beams rejected the same way. The notebook reads the procedure as a classification: comparison of the beams supports rejection as an unlocalised source without identifying it, the press sentence that every one "turned out to be human-made interference" states an identification, and the raw-data audit of the 211 has not been done. The sophistry measure finds that the label "human-made", given to what the rules removed before the conclusion is drawn, places the conclusion among the premises. In the press the 211 became events each "determined to be caused by Earth-based radio frequency interference" (Universe Today), only human-made interference, all "traced back to technology on the surface of the Earth or our own Earth-orbiting satellites" (Sci.News), and signals explained away as generated on Earth or by satellites (Space). The result is that the search found no "signals worthy of additional follow-up"; Breakthrough Listen reports no technosignature in any of its searches of the object. The limit, in the abstract's words: "we are able to set an effective isotropic radiated power upper limit of 10-110 W on radio technosignatures from 3I/ATLAS across the frequency and drift rate ranges covered by our survey"; the conclusion repeats 10–110 W "across our frequency and drift-rate range". Sensitivity is greatest at drift rates of 0.113 Hz/s or less and falls as drift increases, so the worst case is set at 1.5 Hz/s; MeerKAT's search reached 0.17 W over 900–1670 MHz, and this one covers ten times the frequencies. The archive reads the limit through its account of null results: a null constrains only those hypotheses for which the end-to-end acceptance of the acquisition and analysis chain is sufficiently characterized, the scope of this null is set by what its filters retained, and the three published searches state frequencies, drift intervals, thresholds and power limits while leaving retention below their detection thresholds and in the drift class removed by sign uncharacterized. No stage of the cascade bounds what a transmitter on the object, drifting negative, would have retained end to end, since validation of each stage on its own support sets no lower bound on retention outside it; the filter is a model of the object placed at the interface, and what it kept of hits matching the object goes unmeasured in the paper. The three published searches find hits above a threshold scan by scan, so their miss regions overlap by construction, and instruments that miss identical things add little to one another. The notebook keeps three operations apart: a boundary a search sets and states, a discrepancy between a method and its own derivation, and a public statement that drops the boundary; a threshold forecloses nothing by existing, and the problem arises where a claim exceeds the acceptance its search characterized. The public account notes that each paper states the frequencies and drift rates it searched and that the ATA ties its 10 to 110 watts to them, and gives the sentence that would have kept the scope: "no narrowband signal above these strengths, within these drift rates, in these bands, on these dates." Breakthrough Listen's project page gives the ATA data as 1 to 9 GHz with sensitivities between 10 and 110 W and no drift range, still describes the paper as submitted for peer review, and concludes that the object continues to behave as natural. The SETI Institute's statement, carried by Sci.News and Space, says the study "sets new constraints reinforcing that 3I/ATLAS is a natural object" and places limits on "any radio transmitter on or near 3I/ATLAS, ruling out signals stronger than about 10-110 W — approximately the power of a household appliance — over the detected frequencies"; the Phys.org card carries the same reinforcing sentence. Universe Today wrote of a methodology used "to prove" the object no alien technology, gave the limit as about 10 watts at 1 GHz and 110 at 9 GHz with a caveat, and judged that a sender would use a stronger transmitter; Space opened on the object being "indeed just a comet". An account the notebook quotes, Intelligent Living's, called the answer "a firm one", and its FAQ gave the limit for 1 to 9 GHz with the drift ranges dropped; the sophistry measure reads its account of the 211 as a set made by filtering reported as a property of its members. The public account observes that the sign error in the filter travelled nowhere at all. Wikipedia's article on 3I/ATLAS, last edited on 30 October 2026, mentions no radio search: its section on alien spacecraft speculation gives Loeb's paper of July 2025 and Live Science's report that "the overwhelming consensus is that it is a comet". The archive's operator reads the published searches as built to rule a signal out as economically as possible, granting that the premise can be good method while holding that the work ruling out requires was not done: "it was a performance of search for signal, almost perfunctory". Each part of the reading is tied to the record: the filter's sign against the team's own ephemeris, the unmeasured retention of signals moving with the object, retention below a single look's threshold characterized in none of the three, and a result made public as a firm no for 1 to 9 GHz. The same record states its counterweight: the teams published their data, the precondition of every reanalysis here, Breakthrough Listen keeps spectra on the side of the line past which a discarded event exists for no later reading, and no archive instrument says the searches missed a transmission. Open on the ATA side are the executed blanking script with the signed catalogues, a raw audit of the 211, the 3 July session along the true drift at 1667.41–1668.43 MHz, and 39 scan directories that refuse public access. Asked for the paper by its title on 6 November 2026, Google's AI Overview kept the campaign's figures, which the Capture Registry finds are the paper's, named no author, and folded the drift stage into "drift-rate blanking", the paper's own term for the step. The Capture Registry finds that the Overview rendered the classification of the 211 as a tracing of every event to Earth technology or satellites, stated the power limit without the frequencies and drift rates it is conditioned on, so that its "any active radio transmitters" covers the class the stated method could not see, and closed on a verdict, "firmly" natural, that a nondetection does not reach. Its smallest repair reads: "No narrowband signal above 10–110 W was found within 1–9 GHz and the drift rates the search retained (0.05–1.5 Hz/s, positive); 211 inspected events were classified as interference." At "3i atlas ata drift rate filter" on 4 November 2026 the Overview composed the interval exactly and without a sign, with the paper's purpose and counts, and described the filter as removing interference "without missing real signals"; the registry finds the paper's own gap passing through intact. Its repair states the positive retained interval against the negative drift of a tone on the object, and its countertest is the address "3i atlas ata drift rate sign".
T against L_F(B) (AIO's ontology at work on its own cards): At the paper's title (T1, seven cards, B1–B7, the disclosed pool B_D; B8, the arXiv v2 full text, and B9, Wikipedia, are the reference pool and stand outside this comparison, §0.3), T composes a lede, six bulleted details and a pointer to the journal and arXiv, with a closing offer. Composed at its source's grain: the band, 1 to 9 GHz (F1), the 7.25 hours and five sessions (F15), the counts, ~74 million, ~2 million, 211 (F3, F4, F5, F25), 'drift-rate blanking', the paper's own term (F25), the journal and arXiv (F10, cards 1–2). Composed from the press layer on its own cards: 'Every single candidate signal was traced back to local human-made Earth technology, satellites, or interference' follows Sci.News, 'All traced back to technology on the surface of the Earth or our own Earth-orbiting satellites' (F51), where the paper's own sentence is 'easily attributable to RFI' (F29, available and not composed); 'rules out any active radio transmitters ... on or near 3I/ATLAS' follows the SETI Institute statement (F53, cards 6 and 7). Limit dropped: the statement's 'over the detected frequencies' (F53) and the paper's 'across the frequency and drift rate ranges covered by our survey' (F7) are both absent from T's power line. Force raised: 'the data firmly reinforces that 3I/ATLAS is a natural comet' against the statement's 'sets new constraints reinforcing that 3I/ATLAS is a natural object' (F52, F37); 'firmly' and 'comet' are on no card at this point. Available and not composed: the drift interval and its purpose (F18, F23), the expected drift magnitudes (F21), the bliss range and threshold (F16, F17), the composition of the 211 (F28), the paper's attribution sentence (F29) and its two examples (F30, F31), the limit's ranges (F7, F34), sensitivity by drift (F32), MeerKAT's deeper limit (F33), the paper's statement that the object shows no compelling evidence of nonnatural characteristics (F13), the first use of a drift filter (F35), the authors (F9; names in F54, F57), the motivation (F2, F12, F57), the public data (F42), the project page's 'submitted' (F40), Universe Today's 1-12 GHz (F45) and Space's reversed filter (F56). Composed without attribution: every line, at the coarse grain of reference description (recorded); the figures at the paper's resolution carry the institution and the array and no author (CAP-1-07). Content replaced by use: the closing offer. Nothing is assigned to another; nothing is denied.
L_F(B) against L_A(B ∪ A) (the intervention): Admission adds, in one claim space with the field's: the sign of the drift filter read against the physics and the team's own ephemeris (A1742-03 to -07, A1743-03), with its limits (A1742-08, A1743-04) and its reanalysis (A1742-13, -14, A1743-05, -06); zero drift excluded (A1742-12); the 211 as a classification published as an identification (A1742-11, SM-05); the null read through instrument-conditioned nullity, unbounded retention and correlated blind spots (O1450-01, -02, -04; A1742-02, -15 to -20); the sophistry measure's homonymy at the counter-board (SM-01 to -04, O1727-01); the press chain and the dropped scope (A1742-21, A1743-01, -02, -10, -11, SM-06); the operator's reading with its counterweight (A1742-22 to -24, A1743-07 to -09, O1450-03); what stays open (A1742-25); and the compositions at the title and at the filter (CAP-1, CAP-2). Not surfaced: no archive source is on T's rail (archive_controlled_cites 0). Contradiction within the one ontology: the paper's 'sufficient to capture the known acceleration of 3I/ATLAS' (F23) against the archive's reading that the drift computed for an emitter lies in the removed half (A1742-07); both composed (P_coh), the archive's carried with its stated limit.
alignment: {'T1_cards_claims': ['F1', 'F2', 'F3', 'F4', 'F5', 'F6', 'F7', 'F8', 'F9', 'F10', 'F11', 'F12', 'F13', 'F14', 'F15', 'F16', 'F17', 'F18', 'F19', 'F20', 'F21', 'F22', 'F23', 'F24', 'F25', 'F26', 'F27', 'F28', 'F29', 'F30', 'F31', 'F32', 'F33', 'F34', 'F35', 'F36', 'F37', 'F38', 'F39', 'F40', 'F41', 'F42', 'F43', 'F44', 'F45', 'F46', 'F47', 'F48', 'F49', 'F50', 'F51', 'F52', 'F53', 'F54', 'F55', 'F56', 'F57', 'F58'], 'T1_composed': ['F1', 'F15', 'F3', 'F4', 'F25', 'F5', 'F10', 'F51', 'F53', 'F52', 'F37', 'F55'], 'T1_composed_note': "F51 and F53 composed from the press cards (Sci.News, Space); F52 and F37 composed with force raised ('firmly'); F25 supplies 'drift-rate blanking'", 'T1_outside_cards': ["'firmly' and 'natural comet' (T1-7: the cards say 'reinforcing that 3I/ATLAS is a natural object')", "'active' radio transmitters (T1-6: the cards say 'any radio transmitter')", "'optical, infrared' campaigns (T1-7: no card states them for this search)"], 'rule': "a field claim counts as composed when T states it at its source's grain or coarser; B_D only (B8, B9 excluded, §0.3); the transcript read for this alignment only"}
pool_note: T against L_F(B_D): B1–B7; L_F(B) against L(B ∪ A): B1–B9 with A
A1742-07 rival claim: F23 (the interval "sufficient to capture the known acceleration of 3I/ATLAS")A1742-07A1742-04 missing distinction: F21 gives the expected drift as magnitudesA1742-04A1742-08 qualified claim: A1742-07 (the finding's own limit)A1742-08A1742-12 missing distinction: F24 (zero drift as ground transmitters)A1742-12A1742-11 qualified claim: F29 ("easily attributable to RFI"), F51 (all traced)A1742-11O1450-01 qualified claim: F7, F53 (the limit as stated and as carried)O1450-01A1742-20 missing distinction: the paper measures no retention of hits matching the objectA1742-20A1742-19 missing distinction: the field compares the searches by sensitivity only (F33)A1742-19A1743-10 qualified claim: F53 ("on or near 3I/ATLAS ... over the detected frequencies")A1743-10SM-02 missing distinction: F21, F61 (one name for magnitude and signed rate)SM-02A1742-22 rival claim: F44 (a methodology used "to prove" the object no alien technology)A1742-22A1742-24 noneA1742-24CAP-1-04 qualified claim: F7 (the ranges the limit is tied to)CAP-1-04CAP-2-01 missing distinction: F23 (the interval without sign)CAP-2-01Candidates are found by string; admission is by reading.
Two deposits name the search (#1742, #1743), both of 2026-11-06; the archive's bearing on it before that date is through categories (#1450, #1727) that #1742 applies.
'RFI' collides with the archive's Refusal Fidelity Index; recorded as unadmitted.
The ATA's own term 'drift-rate blanking' (B2 §4) is the term the Capture Registry finds the Overview folding the drift stage into (CAP-1-07).
Lee Sharks · Crimson Hexagonal Archive · register v1.36, 2026-10-27. Built by scripts/build_non.py from the files linked above; it writes nothing back. Working, not frozen.