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Record W2529446898 · doi:10.1002/asna.201713352

The <scp>XXL</scp> survey: First results and future

2017· article· en· W2529446898 on OpenAlexaff
M. Pierre, C. Adami, M. Birkinshaw, L. Chiappetti, S. Ettori, A. E. Evrard, L. Faccioli, F. Gastaldello, Paul Giles, C. Horellou, A. Iovino, E. Koulouridis, C. Lidman, A.M.C Le Brun, B. J. Maughan, S. Maurogordato, Ian G. McCarthy, Satoshi Miyazaki, F. Pacaud, S. Paltani, M. Plionis, T. H. Reiprich, T. Sadibekova, V. Smolčić, S. L. Snowden, Jean Surdej, M. Tsirou, C. Vignali, J. P. Willis, Sinan Aliş, B. Altieri, N. Baran, C. Benoist, A. Bongiorno, L. Pozzetti, A. Butler, A. Cappi, C. A. Caretta, P. Ciliegi, N. Clerc, Pier-Stefano Corasaniti, J. Coupon, J. Delhaize, I. Delvecchio, J. Démoclès, S. Desai, Julien Devriendt, Yohan Dubois, D. Eckert, A. Elyiv, Arya Farahi, C. Ferrari, S. Fotopoulou, W. Forman, I. Georgantopoulos, V. Guglielmo, Minh Huynh, N. Jerlin, C. Jones, S. Lavoie, J. P. Le Fèvre, Maggie Lieu, M. Kilbinger, F. MaruIli, A. Mantz, Sean McGee, J.‐B. Melin, О. Melnyk, L. Moscardini, Mladen Novak, E. Piconcelli, Bianca M. Poggianti, D. M. Pomarede, E. Pompei, T. J. Ponman, M. E. Ramos-Ceja, Parul Rana, David Rapetti, Somak Raychaudhury, M. Ricci, H. Röttgering, M Sahlén, J.‐L. Sauvageot, C. Schimd, M. Sereno, G. P. Smith, Keiichi Umetsu, Patrick Valageas, A. Valotti, I. Valtchanov, A. Veropalumbo, B. Ascaso, David J Barnes, M. De Petris, F. Durret, Megan Donahue, M. Ithana, M. J. Jarvis, M. Johnston‐Hollitt, E. Kalfountzou, Scott T. Kay, F. La Franca, N. Okabe, Adam Muzzin, A. Rettura, F. Ricci, J. Ridl, G. Risaliti, Motokazu Takizawa, P. Thomas, Nhut Truong

Bibliographic record

VenueAstronomische Nachrichten · 2017
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysical Phenomena and Observations
Canadian institutionsYork UniversityUniversity of Victoria
FundersScience and Technology Facilities Council
KeywordsPhysicsAstrophysicsCluster (spacecraft)AngstromAstronomyRedshiftCOSMIC cancer databaseCosmologyCalibrationSurvey researchGalaxyComputer science

Abstract

fetched live from OpenAlex

The XXL survey currently covers two 25 deg2 patches with XMM observations of ∼10 ks. We summarize the scientific results associated with the first release of the XXL dataset, which occurred in mid‐2016. We review several arguments for increasing the survey depth to 40 ks during the next decade of XMM operations. X‐ray (z < 2) cluster, (z < 4) active galactic nuclei (AGN), and cosmic background survey science will then benefit from an extraordinary data reservoir. This, combined with deep multi‐λ observations, will lead to solid standalone cosmological constraints and provide a wealth of information on the formation and evolution of AGN, clusters, and the X‐ray background. In particular, it will offer a unique opportunity to pinpoint the z > 1 cluster density. It will eventually constitute a reference study and an ideal calibration field for the upcoming eROSITA and Euclid missions.

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 machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.006
metaresearch head score (Gemma)0.008
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: none
Teacher disagreement score0.020
Threshold uncertainty score0.067

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0060.008
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0030.005
Science and technology studies0.0010.001
Scholarly communication0.0040.004
Open science0.0010.003
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0200.020

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 head0.015
GPT teacher head0.236
Teacher spread0.221 · 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 source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
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

Citations10
Published2017
Admission routes1
Has abstractyes

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