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Record W3176140341 · doi:10.1051/0004-6361/202141631

The eROSITA Final Equatorial-Depth Survey (eFEDS)

2022· article· en· W3176140341 on OpenAlexfundno aff
M. Salvato, J. Wolf, T. Dwelly, A. Georgakakis, M. Brusa, A. Merloni, Teng Liu, Yoshiki Toba, K. Nandra, G. Lamer, Johannes Büchner, P. C. Schneider, S. Freund, A. Rau, A. Schwope, Atsushi J. Nishizawa, Matthias Klein, R. Arcodia, Johan Comparat, B. Musiimenta, Tohru Nagao, H. Brunner, A. Malyali, A. Finoguenov, Scott F. Anderson, Yue Shen, Héctor J. Ibarra-Medel, Jonathan R. Trump, W. N. Brandt, C. M. Urry, Chipana Rivera, M. Krumpe, T. Urrutia, T. Miyaji, Kohei Ichikawa, Donald P. Schneider, Alejandra Fresco, Thomas Böller, Joachim Haase, Joel R. Brownstein, Richard R. Lane, Dmitry Bizyaev, Christian Nıtschelm

Bibliographic record

VenueAstronomy and Astrophysics · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsnot available
FundersLawrence Berkeley National LaboratoryRussian Academy of SciencesJapan Society for the Promotion of ScienceLeibniz-GemeinschaftOffice of ScienceUniversity of Colorado BoulderCarnegie Institution for ScienceInstituto de Astrofísica de CanariasRheinische Friedrich-Wilhelms-Universität BonnMax-Planck-Institut für AstronomieLeibniz-Institut für Astrophysik PotsdamUniversidad Nacional Autónoma de MéxicoJapan Science and Technology AgencyUniversität HamburgMax-Planck-GesellschaftUniversità degli Studi di PadovaMax-Planck-Institut für AstrophysikNuclear Safety and Security CommissionEberhard Karls Universität TübingenYork UniversityMinistério da Ciência, Tecnologia e InovaçãoCabinet Office, Government of JapanAcademia SinicaDeutsche ForschungsgemeinschaftNederlandse Organisatie voor Wetenschappelijk OnderzoekMinistry of Education, Culture, Sports, Science and TechnologyEuropean CommissionPennsylvania State UniversityUniversity of OxfordUniversity of Notre DameCarnegie Mellon UniversityUniversity of WashingtonEuropean Space AgencyPrinceton UniversityAlfred P. Sloan FoundationJohns Hopkins UniversityCarnegie Institution of WashingtonUniversity of PortsmouthNew Mexico State UniversityUniversity of UtahToray Science FoundationHigh Energy Accelerator Research OrganizationUniversity of TokyoOhio State UniversityYale UniversityU.S. Department of EnergySmithsonian InstitutionUniversity of PennsylvaniaNational Aeronautics and Space AdministrationNational Astronomical Observatory of JapanVanderbilt UniversityNational Science Foundation
KeywordsPhysicsAstrophysicsROSATSkyRedshiftGalaxyPhotometry (optics)AstronomyActive galactic nucleusObservatoryStars

Abstract

fetched live from OpenAlex

Context. In November 2019, eROSITA on board of the Spektrum-Roentgen-Gamma (SRG) observatory started to map the entire sky in X-rays. After the four-year survey program, it will reach a flux limit that is about 25 times deeper than ROSAT. During the SRG performance verification phase, eROSITA observed a contiguous 140 deg 2 area of the sky down to the final depth of the eROSITA all-sky survey (eROSITA Final Equatorial-Depth Survey; eFEDS), with the goal of obtaining a census of the X-ray emitting populations (stars, compact objects, galaxies, clusters of galaxies, and active galactic nuclei) that will be discovered over the entire sky. Aims. This paper presents the identification of the counterparts to the point sources detected in eFEDS in the main and hard samples and their multi-wavelength properties, including redshift. Methods. To identifyy the counterparts, we combined the results from two independent methods ( NWAY and ASTROMATCH ), trained on the multi-wavelength properties of a sample of 23k XMM-Newton sources detected in the DESI Legacy Imaging Survey DR8. Then spectroscopic redshifts and photometry from ancillary surveys were collated to compute photometric redshifts. Results. Of the eFEDS sources, 24 774 of 27 369 have reliable counterparts (90.5%) in the main sample and 231 of 246 sourcess (93.9%) have counterparts in the hard sample, including 2514 (3) sources for which a second counterpart is equally likely. By means of reliable spectra, Gaia parallaxes, and/or multi-wavelength properties, we have classified the reliable counterparts in both samples into Galactic (2695) and extragalactic sources (22 079). For about 340 of the extragalactic sources, we cannot rule out the possibility that they are unresolved clusters or belong to clusters. Inspection of the distributions of the X-ray sources in various optical/IR colour-magnitude spaces reveal a rich variety of diverse classes of objects. The photometric redshifts are most reliable within the KiDS/VIKING area, where deep near-infrared data are also available. Conclusions. This paper accompanies the eROSITA early data release of all the observations performed during the performance and verification phase. Together with the catalogues of primary and secondary counterparts to the main and hard samples of the eFEDS survey, this paper releases their multi-wavelength properties and redshifts.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesScience and technology studies
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.677
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0020.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.020
GPT teacher head0.225
Teacher spread0.205 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations112
Published2022
Admission routes1
Has abstractyes

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