COSMOS2020: A Panchromatic View of the Universe to z ∼ 10 from Two Complementary Catalogs

Weaver, J. R.; Kauffmann, O. B.; Ilbert, O.; McCracken, H. J.; Moneti, A.; Toft, S.; Brammer, G.; Shuntov, M.; Davidzon, I.; Hsieh, B. C.; Laigle, C.; Anastasiou, A.; Jespersen, C. K.; Vinther, J.; Capak, P.; Casey, C. M.; McPartland, C. J. R.; Milvang-Jensen, B.; Mobasher, B.; Sanders, D. B.; Zalesky, L.; Arnouts, S.; Aussel, H.; Dunlop, J. S.; Faisst, A.; Franx, M.; Furtak, L. J.; Fynbo, J. P. U.; Gould, K. M. L.; Greve, T. R.; Gwyn, S.; Kartaltepe, J. S.; Kashino, D.; Koekemoer, A. M.; Kokorev, V.; Le Fèvre, O.; Lilly, S.; Masters, D.; Magdis, G.; Mehta, V.; Peng, Y.; Riechers, D. A.; Salvato, M.; Sawicki, M.; Scarlata, C.; Scoville, N.; Shirley, R.; Silverman, J. D.; Sneppen, A.; Smolc̆ić, Vernesa; Steinhardt, C.; Stern, D.; Tanaka, M.; Taniguchi, Y.; Teplitz, H. I.; Vaccari, M.; Wang, W.-H.; Zamorani, G.

doi:10.3847/1538-4365/ac3078

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Scientific paper - Original scientific paper

COSMOS2020: A Panchromatic View of the Universe to z ∼ 10 from Two Complementary Catalogs

The Astrophysical Journal Supplement Series, 258 (2022), 1; 11. https://doi.org/10.3847/1538-4365/ac3078

Weaver, J. R.; Kauffmann, O. B.; Ilbert, O.; McCracken, H. J.; Moneti, A.; Toft, S.; Brammer, G.; Shuntov, M.; Davidzon, I.; Hsieh, B. C.; Laigle, C.; Anastasiou, A.; Jespersen, C. K.; Vinther, J.; Capak, P.; Casey, C. M.; McPartland, C. J. R.; Milvang-Jensen, B.; Mobasher, B.; Sanders, D. B.; Zalesky, L.; Arnouts, S.; Aussel, H.; Dunlop, J. S.; Faisst, A.; Franx, M.; Furtak, L. J.; Fynbo, J. P. U.; Gould, K. M. L.; Greve, T. R.; Gwyn, S.; Kartaltepe, J. S.; Kashino, D.; Koekemoer, A. M.; Kokorev, V.; Le Fèvre, O.; Lilly, S.; Masters, D.; Magdis, G.; Mehta, V.; Peng, Y.; Riechers, D. A.; Salvato, M.; Sawicki, M.; Scarlata, C.; Scoville, N.; Shirley, R.; Silverman, J. D.; Sneppen, A.; Smolc̆ić, Vernesa; Steinhardt, C.; Stern, D.; Tanaka, M.; Taniguchi, Y.; Teplitz, H. I.; Vaccari, M.; Wang, W.-H.; Zamorani, G. More authors...

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APA 6th Edition

Weaver, J. R., Kauffmann, O. B., Ilbert, O., McCracken, H. J., Moneti, A., Toft, S. ... Zamorani, G. (2022). COSMOS2020: A Panchromatic View of the Universe to z ∼ 10 from Two Complementary Catalogs. The Astrophysical Journal Supplement Series, 258. (1). doi: 10.3847/1538-4365/ac3078

MLA 8th Edition

Weaver, J. R., et al. "COSMOS2020: A Panchromatic View of the Universe to z ∼ 10 from Two Complementary Catalogs." The Astrophysical Journal Supplement Series, vol. 258, no. 1, 2022. https://doi.org/10.3847/1538-4365/ac3078

Chicago 17th Edition

Weaver, J. R., O. B. Kauffmann, O. Ilbert, H. J. McCracken, A. Moneti, S. Toft, G. Brammer, et al. "COSMOS2020: A Panchromatic View of the Universe to z ∼ 10 from Two Complementary Catalogs." The Astrophysical Journal Supplement Series 258, no. 1 (2022). https://doi.org/10.3847/1538-4365/ac3078

Harvard

Weaver, J. R., et al. (2022) 'COSMOS2020: A Panchromatic View of the Universe to z ∼ 10 from Two Complementary Catalogs', The Astrophysical Journal Supplement Series, 258(1). doi: 10.3847/1538-4365/ac3078

Vancouver

Weaver JR, Kauffmann OB, Ilbert O, McCracken HJ, Moneti A, Toft S, and sur.. COSMOS2020: A Panchromatic View of the Universe to z ∼ 10 from Two Complementary Catalogs. The Astrophysical Journal Supplement Series [Internet]. 2022 January 10 [cited 2024 October 03];258(1). doi: 10.3847/1538-4365/ac3078

IEEE

J. R. Weaver, et al., "COSMOS2020: A Panchromatic View of the Universe to z ∼ 10 from Two Complementary Catalogs", The Astrophysical Journal Supplement Series, vol. 258, no. 1, January 2022. [Online]. Available at: https://urn.nsk.hr/urn:nbn:hr:217:628862. [Accessed: 03 October 2024]

Cite this item: https://urn.nsk.hr/urn:nbn:hr:217:628862

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Metadata

Title (english)	COSMOS2020: A Panchromatic View of the Universe to z ∼ 10 from Two Complementary Catalogs
Author	J. R. Weaver
Author	O. B. Kauffmann
Author	O. Ilbert
Author	H. J. McCracken
Author	A. Moneti
Author	S. Toft
Author	G. Brammer
Author	M. Shuntov
Author	I. Davidzon
Author	B. C. Hsieh
Author	C. Laigle
Author	A. Anastasiou
Author	C. K. Jespersen
Author	J. Vinther
Author	P. Capak
Author	C. M. Casey
Author	C. J. R. McPartland
Author	B. Milvang-Jensen
Author	B. Mobasher
Author	D. B. Sanders
Author	L. Zalesky
Author	S. Arnouts
Author	H. Aussel
Author	J. S. Dunlop
Author	A. Faisst
Author	M. Franx
Author	L. J. Furtak
Author	J. P. U. Fynbo
Author	K. M. L. Gould
Author	T. R. Greve
Author	S. Gwyn
Author	J. S. Kartaltepe
Author	D. Kashino
Author	A. M. Koekemoer
Author	V. Kokorev
Author	O. Le Fèvre
Author	S. Lilly
Author	D. Masters
Author	G. Magdis
Author	V. Mehta
Author	Y. Peng
Author	D. A. Riechers
Author	M. Salvato
Author	M. Sawicki
Author	C. Scarlata
Author	N. Scoville
Author	R. Shirley
Author	J. D. Silverman
Author	A. Sneppen
Author	Vernesa Smolc̆ić
Author	C. Steinhardt
Author	D. Stern
Author	M. Tanaka
Author	Y. Taniguchi
Author	H. I. Teplitz
Author	M. Vaccari
Author	W.-H. Wang
Author	G. Zamorani
Author's institution	University of Zagreb Faculty of Science (Department of Physics)
Scientific / art field, discipline and subdiscipline	NATURAL SCIENCES Physics
Abstract (english)	The Cosmic Evolution Survey (COSMOS) has become a cornerstone of extragalactic astronomy. Since the last public catalog in 2015, a wealth of new imaging and spectroscopic data have been collected in the COSMOS field. This paper describes the collection, processing, and analysis of these new imaging data to produce a new reference photometric redshift catalog. Source detection and multiwavelength photometry are performed for 1.7 million sources across the 2 deg2 of the COSMOS field, ∼966, 000 of which are measured with all available broadband data using both traditional aperture photometric methods and a new profile- fitting photometric extraction tool, The Farmer, which we have developed. A detailed comparison of the two resulting photometric catalogs is presented. Photometric redshifts are computed for all sources in each catalog utilizing two independent photometric redshift codes. Finally, a comparison is made between the performance of the photometric methodologies and of the redshift codes to demonstrate an exceptional degree of self-consistency in the resulting photometric redshifts. The i < 21 sources have subpercent photometric redshift accuracy and even the faintest sources at 25 < i < 27 reach a precision of 5%. Finally, these results are discussed in the context of previous, current, and future surveys in the COSMOS field. Compared to COSMOS2015, it reaches the same photometric redshift precision at almost one magnitude deeper. Both photometric catalogs and their photometric redshift solutions and physical parameters will be made available through the usual astronomical archive systems (ESO Phase 3, IPAC-IRSA, and CDS).
Keywords (english)
Language	english
Publication type	Scientific paper - Original scientific paper
Publication status	Published
Peer review	Peer review - international
Publication version	Published version
Journal title	The Astrophysical Journal Supplement Series
Numbering	vol. 258, no. 1, 11
p-ISSN	0067-0049
e-ISSN	1538-4365
DOI	https://doi.org/10.3847/1538-4365/ac3078
URN:NBN	urn:nbn:hr:217:628862
Publication	2022-01-10
Document URL	https://iopscience.iop.org/article/10.3847/1538-4365/ac3078
Type of resource	Text
Access conditions	Open access
Terms of use
Public note	© 2022. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. Received 2020 December 23; revised 2021 September 30; accepted 2021 October 15; published 2022 January 10.
Created on	2024-08-09 19:12:39