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arxiv: 2302.03676 · v1 · pith:LLDDH5NQnew · submitted 2023-02-07 · 🌀 gr-qc

Open data from the third observing run of LIGO, Virgo, KAGRA and GEO

The LIGO Scientific Collaboration , the Virgo Collaboration , the KAGRA Collaboration: R. Abbott , H. Abe , F. Acernese , K. Ackley , S. Adhicary , N. Adhikari
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R. X. Adhikari V. K. Adkins V. B. Adya C. Affeldt D. Agarwal M. Agathos O. D. Aguiar L. Aiello A. Ain P. Ajith T. Akutsu S. Albanesi R. A. Alfaidi A. Al-Jodah C. All\'en\'e A. Allocca M. Almualla P. A. Altin A. Amato L. Amez-Droz A. Amorosi S. Anand A. Ananyeva R. Andersen S. B. Anderson W. G. Anderson M. Andia M. Ando T. Andrade N. Andres M. Andr\'es-Carcasona T. Andri\'c S. Ansoldi J. M. Antelis S. Antier M. Aoumi T. Apostolatos E. Z. Appavuravther S. Appert S. K. Apple K. Arai A. Araya M. C. Araya J. S. Areeda M. Ar\`ene N. Aritomi N. Arnaud M. Arogeti S. M. Aronson K. G. Arun H. Asada G. Ashton Y. Aso M. Assiduo S. Assis de Souza Melo S. M. Aston P. Astone F. Aubin K. AultONeal S. Babak A. Badalyan F. Badaracco C. Badger S. Bae S. Bagnasco Y. Bai J. G. Baier L. Baiotti J. Baird R. Bajpai T. Baka M. Ball G. Ballardin S. W. Ballmer G. Baltus S. Banagiri B. Banerjee D. Bankar P. Baral J. C. Barayoga J. Barber B. C. Barish D. Barker P. Barneo F. Barone B. Barr L. Barsotti M. Barsuglia D. Barta S. D. Barthelmy M. A. Barton I. Bartos S. Basak A. Basalaev R. Bassiri A. Basti M. Bawaj J. C. Bayley A. C. Baylor M. Bazzan B. B\'ecsy V. M. Bedakihale F. Beirnaert M. Bejger A. S. Bell V. Benedetto D. Beniwal W. Benoit J. D. Bentley M. Ben Yaala S. Bera M. Berbel F. Bergamin B. K. Berger S. Bernuzzi M. Beroiz C. P. L. Berry D. Bersanetti A. Bertolini J. Betzwieser D. Beveridge N. Bevins R. Bhandare A. V. Bhandari U. Bhardwaj R. Bhatt D. Bhattacharjee S. Bhaumik A. Bianchi I. A. Bilenko M. Bilicki G. Billingsley S. Bini O. Birnholtz S. Biscans M. Bischi S. Biscoveanu A. Bisht B. Biswas M. Bitossi M.-A. Bizouard J. K. Blackburn C. D. Blair D. G. Blair R. M. Blair F. Bobba N. Bode M. Bo\"er G. Bogaert G. Boileau M. Boldrini G. N. Bolingbroke L. D. Bonavena R. Bondarescu F. Bondu E. Bonilla G. S. Bonilla R. Bonnand P. Booker R. Bork V. Boschi N. Bose S. Bose V. Bossilkov V. Boudart Y. Bouffanais A. Bozzi C. Bradaschia P. R. Brady M. Braglia A. Branch M. Branchesi J. E. Brau M. Breschi T. Briant A. Brillet M. Brinkmann P. Brockill A. F. Brooks J. Brooks D. D. Brown S. Brunett G. Bruno R. Bruntz J. Bryant F. Bucci J. Buchanan O. Bulashenko T. Bulik H. J. Bulten A. Buonanno K. Burtnyk R. Buscicchio D. Buskulic C. Buy R. L. Byer G. S. Cabourn Davies G. Cabras R. Cabrita L. Cadonati S. Caesar G. Cagnoli C. Cahillane J. Calder\'on Bustillo J. D. Callaghan T. A. Callister E. Calloni J. B. Camp M. Canepa G. Caneva Santoro M. Cannavacciuolo K. C. Cannon H. Cao Z. Cao L. A. Capistran E. Capocasa E. Capote G. Carapella F. Carbognani M. Carlassara J. B. Carlin M. Carpinelli J. J. Carter G. Carullo J. Casanueva Diaz C. Casentini G. Castaldi S. Y. Castro-Lucas S. Caudill M. Cavagli\`a R. Cavalieri G. Cella P. Cerd\'a-Dur\'an E. Cesarini W. Chaibi W. Chakalis S. Chalathadka Subrahmanya E. Champion C. Chan C. L. Chan K. Chandra I. P. Chang W. Chang P. Chanial S. Chao C. Chapman-Bird E. L. Charlton P. Charlton E. Chassande-Mottin L. Chastain C. Chatterjee Debarati Chatterjee Deep Chatterjee M. Chaturvedi S. Chaty K. Chatziioannou D. Chen H. Chen H. Y. Chen J. Chen K. H. Chen X. Chen Y.-R. Chen Y. Chen H. Cheng P. Chessa H. Y. Cheung H. Y. Chia F. Chiadini C-I. Chiang C. Chiang G. Chiarini A. Chiba R. Chiba R. Chierici A. Chincarini M. L. Chiofalo A. Chiummo S. Choudhary N. Christensen S. S. Y. Chua K. W. Chung G. Ciani P. Ciecielag M. Cie\'slar M. Cifaldi A. A. Ciobanu R. Ciolfi F. Clara J. A. Clark T. A. Clarke P. Clearwater S. Clesse F. Cleva E. Coccia E. Codazzo P.-F. Cohadon M. Colleoni C. G. Collette A. Colombo M. Colpi C. M. Compton L. Conti S. J. Cooper P. Corban T. R. Corbitt I. Cordero-Carri\'on S. Corezzi N. J. Cornish A. Corsi S. Cortese A. C. Coschizza R. Cottingham M. W. Coughlin J.-P. Coulon S. T. Countryman J.-F. Coupechoux B. Cousins P. Couvares D. M. Coward M. J. Cowart B. D. Cowburn D. C. Coyne R. Coyne K. Craig J. D. E. Creighton T. D. Creighton A. W. Criswell J. C. G. Crockett-Gray M. Croquette S. G. Crowder J. R. Cudell T. J. Cullen A. Cumming R. Cummings E. Cuoco M. Cury{\l}o P. Dabadie T. Dal Canton S. Dall'Osso G. D\'alya B. D'Angelo S. Danilishin S. D'Antonio K. Danzmann K. E. Darroch C. Darsow-Fromm A. Dasgupta L. E. H. Datrier Sayantani Datta V. Dattilo I. Dave A. Davenport M. Davier D. Davis M. C. Davis E. J. Daw M. Dax D. DeBra M. Deenadayalan J. Degallaix M. De Laurentis S. Del\'eglise V. Del Favero F. De Lillo N. De Lillo D. Dell'Aquila W. Del Pozzo F. De Matteis V. D'Emilio N. Demos T. Dent A. Depasse R. De Pietri R. De Rosa C. De Rossi R. DeSalvo R. De Simone S. Dhurandhar R. Diab P. Z. Diamond M. C. D\'iaz N. A. Didio T. Dietrich L. Di Fiore C. Di Fronzo C. Di Giorgio F. Di Giovanni M. Di Giovanni T. Di Girolamo D. Diksha A. Di Lieto A. Di Michele S. Di Pace I. Di Palma F. Di Renzo Divyajyoti A. Dmitriev Z. Doctor E. Dohmen P. P. Doleva L. Donahue L. D'Onofrio F. Donovan K. L. Dooley T. Dooney S. Doravari O. Dorosh M. Drago J. C. Driggers Y. Drori J.-G. Ducoin L. Dunn U. Dupletsa O. Durante D. D'Urso P.-A. Duverne S. E. Dwyer C. Eassa P. J. Easter M. Ebersold T. Eckhardt G. Eddolls B. Edelman T. B. Edo O. Edy A. Effler J. Eichholz M. Eisenmann R. A. Eisenstein A. Ejlli E. Engelby A. J. Engl L. Errico R. C. Essick H. Estell\'es D. Estevez T. Etzel C. Evans M. Evans T. M. Evans T. Evstafyeva B. E. Ewing F. Fabrizi F. Faedi V. Fafone H. Fair S. Fairhurst P. C. Fan X. Fan A. M. Farah B. Farr W. M. Farr E. J. Fauchon-Jones G. Favaro M. Favata M. Fays J. Feicht M. M. Fejer E. Fenyvesi D. L. Ferguson A. Fernandez-Galiana I. Ferrante T. A. Ferreira F. Fidecaro P. Figura A. Fiori I. Fiori M. Fishbach R. P. Fisher R. Fittipaldi V. Fiumara R. Flaminio S. M. Fleischer L. S. Fleming E. Floden H. K. Fong J. A. Font B. Fornal P. W. F. Forsyth A. Franke S. Frasca F. Frasconi J. P. Freed Z. Frei A. Freise O. Freitas R. Frey P. Fritschel V. V. Frolov G. G. Fronz\'e Y. Fujimoto I. Fukunaga P. Fulda M. Fyffe H. A. Gabbard W. E. Gabella B. U. Gadre K. Gaglani J. R. Gair J. Gais S. Galaudage S. Gallardo R. Gamba D. Ganapathy A. Ganguly D. Gao S. G. Gaonkar B. Garaventa J. Garcia-Bellido C. Garc\'ia-N\'u\~nez C. Garc\'ia-Quir\'os K. A. Gardner J. Gargiulo F. Garufi C. Gasbarra B. Gateley V. Gayathri G. Gemme A. Gennai J. George O. Gerberding L. Gergely S. Ghonge Abhirup Ghosh Archisman Ghosh Shaon Ghosh Shrobana Ghosh Tathagata Ghosh L. Giacoppo J. A. Giaime K. D. Giardina D. R. Gibson C. Gier P. Giri F. Gissi S. Gkaitatzis J. Glanzer A. E. Gleckl F. Glotin J. Godfrey P. Godwin E. Goetz R. Goetz J. Golomb B. Goncharov G. Gonz\'alez M. Gosselin R. Gouaty D. W. Gould S. Goyal B. Grace A. Grado V. Graham M. Granata V. Granata S. Gras P. Grassia C. Gray R. Gray G. Greco A. C. Green R. Green S. Green S. R. Green A. M. Gretarsson E. M. Gretarsson D. Griffith W. L. Griffiths H. L. Griggs G. Grignani A. Grimaldi H. Grote A. S. Gruson D. Guerra D. Guetta G. M. Guidi A. R. Guimaraes H. K. Gulati F. Gulminelli A. M. Gunny H. Guo Y. Guo Anchal Gupta Anuradha Gupta Ish Gupta N. C. Gupta P. Gupta S. K. Gupta J. Gurs Y. Gushima E. K. Gustafson N. Gutierrez F. Guzman L. Haegel G. Hain S. Haino O. Halim E. D. Hall E. Z. Hamilton G. Hammond W.-B. Han M. Haney J. Hanks C. Hanna M. D. Hannam O. A. Hannuksela H. Hansen J. Hanson R. Harada T. Harder K. Haris T. Harmark J. Harms G. M. Harry I. W. Harry D. Hartwig B. Haskell C.-J. Haster J. S. Hathaway K. Haughian H. Hayakawa K. Hayama F. J. Hayes J. Healy A. Heffernan A. Heidmann M. C. Heintze J. Heinze J. Heinzel H. Heitmann F. Hellman P. Hello A. F. Helmling-Cornell G. Hemming M. Hendry I. S. Heng E. Hennes J.-S. Hennig M. Hennig C. Henshaw F. Hernandez Vivanco M. Heurs A. L. Hewitt S. Higginbotham S. Hild P. Hill Y. Himemoto A. S. Hines N. Hirata C. Hirose J. Ho S. Hochheim D. Hofman J. N. Hohmann D. G. Holcomb N. A. Holland K. Holley-Bockelmann I. J. Hollows Z. J. Holmes K. Holt D. E. Holz Q. Hong J. Hornung S. Hoshino J. Hough S. Hourihane D. Howell E. J. Howell C. G. 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Magee R. Maggiore M. Magnozzi M. Mahesh S. Mahesh M. Maini E. Majorana C. N. Makarem S. Maliakal A. Malik N. Man V. Mandic V. Mangano B. Mannix G. L. Mansell G. Mansingh M. Manske M. Mantovani M. Mapelli F. Marchesoni D. Mar\'in Pina F. Marion S. M\'arka Z. M\'arka C. Markakis A. S. Markosyan A. Markowitz E. Maros A. Marquina S. Marsat F. Martelli I. W. Martin R. M. Martin B. B. Martinez M. Martinez V. A. Martinez V. Martinez K. Martinovic D. V. Martynov E. J. Marx H. Masalehdan K. Mason A. Masserot M. Masso Reid M. Mastrodicasa S. Mastrogiovanni M. Mateu-Lucena M. Matiushechkina K. Matsunaga N. Mavalvala R. McCarthy D. E. McClelland P. K. McClincy S. McCormick L. McCuller G. I. McGhee J. McGinn C. McIsaac J. McIver A. McLeod T. McRae S. T. McWilliams D. Meacher M. Mehmet A. K. Mehta Q. Meijer A. Melatos G. Mendell A. Menendez-Vazquez C. S. Menoni R. A. Mercer L. Mereni K. Merfeld E. L. Merilh J. D. Merritt M. Merzougui C. Messenger C. Messick P. M. Meyers F. Meylahn A. Mhaske A. Miani H. Miao I. Michaloliakos C. Michel Y. Michimura H. Middleton D. P. Mihaylov A. Miller A. L. Miller B. Miller S. Miller M. Millhouse J. C. Mills E. Milotti Y. Minenkov N. Mio Ll. M. Mir M. Miravet-Ten\'es A. Mishra C. Mishra T. Mishra T. Mistry A. L. Mitchell S. Mitra V. P. Mitrofanov G. Mitselmakher R. Mittleman O. Miyakawa S. Miyoki Geoffrey Mo L. M. Modafferi E. Moguel S. R. P. Mohapatra S. R. Mohite M. Molina-Ruiz C. Mondal M. Mondin M. Montani C. J. Moore J. Moragues D. Moraru F. Morawski A. More S. More C. Moreno G. Moreno S. Morisaki Y. Moriwaki G. Morras A. Moscatello B. Mours C. M. Mow-Lowry S. Mozzon F. Muciaccia D. Mukherjee Soma Mukherjee Subroto Mukherjee Suvodip Mukherjee N. Mukund A. Mullavey J. Munch E. A. Mu\~niz P. G. Murray J. Murray-Dean S. Muusse S. L. Nadji A. Nagar T. Nagar N. Nagarajan K. Nakamura H. Nakano M. Nakano Y. Nakayama V. Napolano I. Nardecchia T. Narikawa H. Narola L. Naticchioni R. K. Nayak B. F. Neil J. Neilson A. Nelson T. J. N. Nelson M. 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Pedurand R. Pegna M. Pegoraro A. Pele F. E. Pe\~na Arellano S. Penn A. Perego A. Pereira C. J. Perez C. P\'erigois C. C. Perkins A. Perreca S. Perri\`es J. W. Perry D. Pesios J. Petermann C. Petrillo H. P. Pfeiffer H. Pham K. A. Pham K. S. Phukon H. Phurailatpam O. J. Piccinni M. Pichot M. Piendibene F. Piergiovanni L. Pierini G. Pierra V. Pierro G. Pillant M. Pillas F. Pilo L. Pinard C. Pineda-Bosque I. M. Pinto B. J. Piotrzkowski K. Piotrzkowski M. Pirello M. D. Pitkin A. Placidi E. Placidi M. L. Planas W. Plastino R. Poggiani E. Polini L. Pompili D. Y. T. Pong S. Ponrathnam E. Porcelli J. Portell E. K. Porter C. Posnansky R. Poulton Jade Powell Jonathan Powell M. Pracchia T. Pradier A. K. Prajapati K. Prasai R. Prasanna G. Pratten M. Principe G. A. Prodi L. Prokhorov P. Prosposito L. Prudenzi A. Puecher J. Pullin M. Punturo F. Puosi P. Puppo M. P\"urrer H. Qi V. Quetschke P. J. Quinonez R. Quitzow-James F. J. Raab G. Raaijmakers N. Radulesco P. Raffai S. X. Rail S. Raja C. Rajan K. 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Soldateschi S. N. Somala K. Somiya K. Soni S. Soni V. Sordini F. Sorrentino N. Sorrentino H. Sotani R. Soulard T. Souradeep E. Sowell V. Spagnuolo A. P. Spencer M. Spera P. Spinicelli A. K. Srivastava V. Srivastava C. Stachie F. Stachurski D. A. Steer J. Steinlechner S. Steinlechner N. Stergioulas M. StPierre L. C. Strang G. Stratta M. D. Strong A. Strunk R. Sturani A. L. Stuver M. Suchenek S. Sudhagar N. Sueltmann T. Sugiyama H. G. Suh A. G. Sullivan T. Z. Summerscales L. Sun S. Sunil A. Sur J. Suresh P. J. Sutton Takamasa Suzuki Takanori Suzuki B. L. Swinkels A. Syx M. J. Szczepa\'nczyk P. Szewczyk M. Tacca H. Tagoshi S. C. Tait H. Takahashi R. Takahashi A. Takamori S. Takano H. Takeda M. Takeda C. J. Talbot C. Talbot M. Tamaki N. Tamanini D. Tanabe K. Tanaka T. Tanaka A. J. Tanasijczuk S. Tanioka D. B. Tanner D. Tao L. Tao R. D. Tapia E. N. Tapia San Mart\'in R. Tarafder C. Taranto A. Taruya J. D. Tasson M. Teloi R. Tenorio J. E. S. Terhune L. Terkowski H. Themann M. P. Thirugnanasambandam L. M. Thomas M. Thomas P. Thomas S. Thomas J. E. Thompson S. R. Thondapu K. A. Thorne E. Thrane Shubhanshu Tiwari Srishti Tiwari V. Tiwari A. M. Toivonen A. E. Tolley T. Tomaru K. Tomita T. Tomura M. Tonelli A. Torres-Forn\'e C. I. Torrie I. Tosta e Melo E. Tournefier A. Trapananti F. Travasso G. Traylor J. Trenado M. Trevor M. C. Tringali A. Tripathee L. Troiano A. Trovato L. Trozzo R. J. Trudeau K. W. Tsang T. Tsang M. Tse R. Tso S. Tsuchida L. Tsukada T. Tsutsui K. Turbang M. Turconi C. Turski D. Tuyenbayev H. Ubach A. S. Ubhi N. Uchikata T. Uchiyama R. P. Udall T. Uehara K. Ueno C. S. Unnikrishnan T. Ushiba A. Utina H. Vahlbruch N. Vaidya G. Vajente A. Vajpeyi G. Valdes M. Valentini S. Vallero V. Valsan N. van Bakel M. van Beuzekom M. van Dael J. F. J. van den Brand C. Van Den Broeck D. C. Vander-Hyde M. van der Sluys A. Van de Walle J. van Dongen H. van Haevermaet J. V. van Heijningen J. Vanosky M. H. P. M. van Putten Z. van Ranst N. van Remortel M. Vardaro A. 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This is my paper

Pith reviewed 2026-05-21 22:01 UTC · model grok-4.3

classification 🌀 gr-qc
keywords gravitational wavesLIGOVirgoKAGRAopen datadata releaseobserving run
0
0 comments X

The pith

Gravitational-wave strain data from the third observing run of LIGO, Virgo, KAGRA and GEO have been released publicly with supporting materials.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The paper announces the public availability of data collected during the third observing run of the global gravitational-wave detector network. This run included three phases with five detectors and produced strain time series that contain astrophysical signals. The release bundles these main data files with auxiliary information, documentation, tutorials, and software packages. A sympathetic reader cares because the materials are provided through a single online center so that researchers anywhere can analyze the signals or verify results without needing special access to the original teams.

Core claim

The authors release the gravitational-wave strain time series data collected during the third observing run, together with auxiliary data, documentation, tutorials, and software packages, all accessible via the Gravitational Wave Open Science Center.

What carries the argument

The open data release through the Gravitational Wave Open Science Center, which distributes the strain time series containing astrophysical signals along with analysis tools.

If this is right

  • Independent groups can search the O3 strain data for additional gravitational-wave signals not identified in the original publications.
  • The included software and tutorials allow reproduction of published analyses by outside teams.
  • Supporting data products enable separate studies of detector noise properties and calibration across the five sites.
  • The release expands the pool of researchers who can contribute to gravitational-wave astronomy without joining the large collaborations.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • Future improvements in analysis methods can be applied to the archived data to extract new information years later.
  • The dataset could support educational projects where students learn signal processing using real observations.
  • Cross-checks between independent analyses might reveal subtle features in the data that single-team studies overlook.

Load-bearing premise

The released data products are accurately calibrated and the accompanying documentation is complete enough for independent users to perform reliable analyses without undisclosed proprietary details or corrections.

What would settle it

An external researcher using the released strain data and tutorials to recover a previously published gravitational-wave event but obtaining inconsistent results due to missing calibration steps would show the release does not support independent work.

read the original abstract

The global network of gravitational-wave observatories now includes five detectors, namely LIGO Hanford, LIGO Livingston, Virgo, KAGRA, and GEO 600. These detectors collected data during their third observing run, O3, composed of three phases: O3a starting in April of 2019 and lasting six months, O3b starting in November of 2019 and lasting five months, and O3GK starting in April of 2020 and lasting 2 weeks. In this paper we describe these data and various other science products that can be freely accessed through the Gravitational Wave Open Science Center at https://gwosc.org. The main dataset, consisting of the gravitational-wave strain time series that contains the astrophysical signals, is released together with supporting data useful for their analysis and documentation, tutorials, as well as analysis software packages.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

0 major / 2 minor

Summary. The manuscript announces the public release of gravitational-wave strain time series data collected during the third observing run (O3) of the LIGO Hanford, LIGO Livingston, Virgo, KAGRA, and GEO 600 detectors. O3 is divided into O3a (six months starting April 2019), O3b (five months starting November 2019), and the short O3GK phase (two weeks starting April 2020). The central claim is that the main strain dataset, together with supporting products for analysis, documentation, tutorials, and software packages, is freely available via the Gravitational Wave Open Science Center at gwosc.org.

Significance. If the released products match the description, the work provides a valuable public resource that enables independent verification, re-analysis, and new scientific investigations by the broader community. Open data releases of this type have demonstrably accelerated progress in gravitational-wave astronomy by supporting reproducibility and external contributions; the inclusion of supporting data products and analysis tools strengthens this utility.

minor comments (2)
  1. The abstract states that the strain data 'contains the astrophysical signals' but does not quantify the total amount of science-quality data or the number of confident detections; adding a brief numerical summary would improve the reader's immediate grasp of dataset scope.
  2. Documentation completeness is asserted but not itemized in the provided abstract; a short table or enumerated list of released products (e.g., calibration files, segment lists, noise curves) in the main text would help users confirm they have all necessary components for analysis.

Simulated Author's Rebuttal

0 responses · 0 unresolved

We thank the referee for their positive assessment of the manuscript and for recommending acceptance. We appreciate the recognition that this open data release provides a valuable resource for the gravitational-wave community.

Circularity Check

0 steps flagged

Factual data release paper with no derivations or predictions

full rationale

This is a data-release announcement describing the public availability of O3 strain time series and supporting products via GWOSC. It contains no equations, no fitted parameters, no predictions, and no derivation chain of any kind. The central claim is a factual statement about repository contents and documentation, which stands or falls on the actual files being present and usable rather than on any internal logical reduction. No self-citation load-bearing steps, uniqueness theorems, or ansatzes appear. The paper is therefore self-contained against external benchmarks with zero circularity.

Axiom & Free-Parameter Ledger

0 free parameters · 0 axioms · 0 invented entities

This is a data-release paper with no theoretical model, derivation, or new physical claim. No free parameters, axioms, or invented entities are introduced or required for the central contribution of making the O3 dataset public.

pith-pipeline@v0.9.0 · 15567 in / 1015 out tokens · 56078 ms · 2026-05-21T22:01:58.831459+00:00 · methodology

discussion (0)

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Lean theorems connected to this paper

Citations machine-checked in the Pith Canon. Every link opens the source theorem in the public Lean library.

  • IndisputableMonolith/Foundation/DimensionForcing.lean dimension_forced unclear
    ?
    unclear

    Relation between the paper passage and the cited Recognition theorem.

    The main dataset, consisting of the gravitational-wave strain time series that contains the astrophysical signals, is released together with supporting data useful for their analysis and documentation, tutorials, as well as analysis software packages.

What do these tags mean?
matches
The paper's claim is directly supported by a theorem in the formal canon.
supports
The theorem supports part of the paper's argument, but the paper may add assumptions or extra steps.
extends
The paper goes beyond the formal theorem; the theorem is a base layer rather than the whole result.
uses
The paper appears to rely on the theorem as machinery.
contradicts
The paper's claim conflicts with a theorem or certificate in the canon.
unclear
Pith found a possible connection, but the passage is too broad, indirect, or ambiguous to say the theorem truly supports the claim.

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