Papers › The COSMOS2015 Catalog: Exploring the 1<z<6 Universe with half a million galaxies

The COSMOS2015 Catalog: Exploring the 1<z<6 Universe with half a million galaxies

8 Apr 2016arXiv:1604.02350links table onlyarchive 2025-07-28

C. Laigle, H. J. McCracken, O. Ilbert, B. C. Hsieh, I. Davidzon, P. Capak, G. Hasinger, J. D. Silverman, C. Pichon, J. Coupon, H. Aussel, D. Le Borgne, K. Caputi, P. Cassata, Y. -Y. Chang, F. Civano, J. Dunlop, J. Fynbo, J. S. kartaltepe, A. Koekemoer, O. Le Fevre, E. Le Floc'h, A. Leauthaud, S. Lilly, L. Lin, S. Marchesi, B. Milvang-Jensen, M. Salvato, D. B. Sanders, N. Scoville, V. Smolcic, M. Stockmann, Y. Taniguchi, L. Tasca, S. Toft, M. Vaccari, J. Zabl

The archive published only this paper's code-link row. Authors, date and abstract are from arXiv's metadata (CC0), read from the Kaggle arXiv metadata snapshot of 2026-09-12 where its title matched the archive's; the title is the archive's.

We present the COSMOS2015 catalog which contains precise photometric redshifts and stellar masses for more than half a million objects over the 2deg² COSMOS field. Including new YJHKₛ images from the UltraVISTA-DR2 survey, Y-band from Subaru/Hyper-Suprime-Cam and infrared data from the Spitzer Large Area Survey with the Hyper-Suprime-Cam Spitzer legacy program, this near-infrared-selected catalog is highly optimized for the study of galaxy evolution and environments in the early Universe. To maximise catalog completeness for bluer objects and at higher redshifts, objects have been detected on a χ² sum of the YJHKₛ and z⁺⁺ images. The catalog contains ∼6×10⁵ objects in the 1.5 deg² UltraVISTA-DR2 region, and ∼1.5×10⁵ objects are detected in the "ultra-deep stripes" (0.62 deg²) at Kₛ≤24.7 (3σ, 3", AB magnitude). Through a comparison with the zCOSMOS-bright spectroscopic redshifts, we measure a photometric redshift precision of σ_(Δz/(1+zₛ)) = 0.007 and a catastrophic failure fraction of η=0.5%. At 3<z<6, using the unique database of spectroscopic redshifts in COSMOS, we find σ_(Δz/(1+zₛ)) = 0.021 and η=13.2%. The deepest regions reach a 90\% completeness limit of 10¹⁰M_⊙ to z=4. Detailed comparisons of the color distributions, number counts, and clustering show excellent agreement with the literature in the same mass ranges. COSMOS2015 represents a unique, publicly available, valuable resource with which to investigate the evolution of galaxies within their environment back to the earliest stages of the history of the Universe. The COSMOS2015 catalog is distributed via anonymous ftp (ftp://ftp.iap.fr/pub/from_users/hjmcc/COSMOS2015/) and through the usual astronomical archive systems (CDS, ESO Phase 3, IRSA).

PaperPDFCodeCode Syntology ran

In Syntology Open this paper in Syntology's Atlas, the map of the papers in Syntology's graph and their citations.

For agents, Syntology's MCP tool lists every function and class Syntology harvested from this paper and whether it ran (how to connect): get_harvested_code_for_paper(arxiv_id="1604.02350")

Code

Syntology Ran 0 of 6 code samples harvested from 1 repository linked to this paper; 6 have no recorded run.

By repository: community (archive-listed): 6 samples from 1 repository, 0 ran. The run record, sample by sample. “Ran” means executed on a synthesized input, not that the code is correct or reproduces the paper.

sidd0529/COSMOS_Lens mentioned on GitHubMIT report

Repository list and official/mentioned flags are the archive's, frozen 2025-07-28. Reachability, where shown, is from one Syntology probe window (2026-09-16 to 2026-09-18); repositories not probed show nothing. GitHub stars are not tracked.

Code Syntology ran Syntology

6 samples harvested; 0 ran; 0 honoured the contract we drafted; 6 have no recorded run. Read from Syntology's graph 2026-09-24; that is when this build read the record, not when the samples ran.

6unverified

Licence: 0 of the 6 samples are pointer only, meaning Syntology does not serve that copy's text. This page shows no code text for any sample; each one links to its file in the repository.

Harvested from sidd0529/COSMOS_Lens. “Ran” means the sample executed on a synthesized input. It does not mean the output is correct, and nothing here reproduces the paper's results. “Honoured” and “violated” refer to a contract Syntology drafted from the code itself; “our draft was wrong” and “fixture could not drive it” are failures of Syntology's instrument, not of the code.

Each sample ends with its code_sha256, Syntology's identity for that exact code. An agent fetches the stored sample with Syntology's MCP tool get_code(code_sha256="…") (how to connect); click an identity to copy that call.

Repository labels, per sample. official repository: The archive marks this repository official for the paper. named in the paper: The archive records that the paper mentions this repository; it is not marked official. community (archive-listed): In the archive's code links for this paper, not marked official and not recorded as mentioned in the paper. found in paper text by Syntology: Syntology found this repository in the paper's own text; whether it is the authors' implementation is not asserted. community: Not in the archive's code links for this paper; a community repository Syntology harvested. Samples from a repository marked official are listed first. Licence labels name the repository's licence as recorded at harvest. “Pointer only” means Syntology does not serve that copy's text, for one of four reasons: no licence file was found; the licence was not identified; the licence is recorded as permissive but that copy's record is not marked cleared; or the licence is outside the permissive list Syntology serves text under (MIT, Apache-2.0, BSD and similar). Some licences outside that list permit redistribution, such as WTFPL, and GPL-3.0 under its conditions; they are simply not on the list. Hover a licence label for the reason. File links open the file on GitHub at the default branch, which may have changed since the harvest.

bias_Amara sidd0529/COSMOS_Lens/galaxy_bias.py community (archive-listed) unverified MIT (permissive) · af2b612d81710343 · report
bias_Porto sidd0529/COSMOS_Lens/galaxy_bias.py community (archive-listed) unverified MIT (permissive) · 07a957f7feef6205 · report
fwhm2sigma sidd0529/COSMOS_Lens/gauss_smooth.py community (archive-listed) unverified MIT (permissive) · b9a8fcd80b62ec6c · report
gauss_smooth_func sidd0529/COSMOS_Lens/gauss_smooth.py community (archive-listed) unverified MIT (permissive) · 526d33e8b8c11d8e · report
low_density_fill sidd0529/COSMOS_Lens/hole_fill.py community (archive-listed) unverified MIT (permissive) · 9dbad6a2c3539de6 · report
sigma2fwhm sidd0529/COSMOS_Lens/gauss_smooth.py community (archive-listed) unverified MIT (permissive) · 79218629f8d11892 · report

Results from the paper archive 2025-07-28

No leaderboard rows for this paper in the archive.

Report a problem or propose a change · a person checks every report against the paper or source before anything changes; decisions are listed on /corrections