The first release COSMOS optical and near-IR data and catalog

P. Capak; H. Aussel; M. Ajiki; H. J. McCracken; B. Mobasher; N. Scoville; P. Shopbell; Y. Taniguchi; D. Thompson; S. Tribiano; S. Sasaki; A. W. Blain; M. Brusa; C. Carilli; A. Comastri; C. M. Carollo; P. Cassata; J. Colbert; R. S. Ellis; M. Elvis; M. Giavalisco; W. Green; L. Guzzo; G. Hasinger; O. Ilbert; C. Impey; K. Jahnke; J. Kartaltepe; J. P. Kneib; J. Koda; A. Koekemoer; Y. Komiyama; A. Leauthaud; O. Lefevre; S. Lilly; C. Liu; R. Massey; S. Miyazaki; T. Murayama; T. Nagao; J. A. Peacock; A. Pickles; C. Porciani; A. Renzini; J. Rhodes; M. Rich; M. Salvato; D. B. Sanders; C. Scarlata; D. Schiminovich; E. Schinnerer; M. Scodeggio; K. Sheth; Y. Shioya; L. A.M. Tasca; J. E. Taylor; L. Yan; G. Zamorani

doi:10.1086/519081

The first release COSMOS optical and near-IR data and catalog

P. Capak, H. Aussel, M. Ajiki, H. J. McCracken, B. Mobasher, N. Scoville, P. Shopbell, Y. Taniguchi, D. Thompson, S. Tribiano, S. Sasaki, A. W. Blain, M. Brusa, C. Carilli, A. Comastri, C. M. Carollo, P. Cassata, J. Colbert, R. S. Ellis, M. ElvisM. Giavalisco, W. Green, L. Guzzo, G. Hasinger, O. Ilbert, C. Impey, K. Jahnke, J. Kartaltepe, J. P. Kneib, J. Koda, A. Koekemoer, Y. Komiyama, A. Leauthaud, O. Lefevre, S. Lilly, C. Liu, R. Massey, S. Miyazaki, T. Murayama, T. Nagao, J. A. Peacock, A. Pickles, C. Porciani, A. Renzini, J. Rhodes, M. Rich, M. Salvato, D. B. Sanders, C. Scarlata, D. Schiminovich, E. Schinnerer, M. Scodeggio, K. Sheth, Y. Shioya, L. A.M. Tasca, J. E. Taylor, L. Yan, G. Zamorani

SCI - Astronomy

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Abstract

We present imaging data and photometry for the COSMOS survey in 15 photometric bands between 0.3 and 2.4 μm. These include data taken on the Subaru 8.3 m telescope, the KPNO and CTIO 4 m telescopes, and the CFHT 3.6 m telescope. Special techniques are used to ensure that the relative photometric calibration is better than 1 % across the field of view. The absolute photometric accuracy from standard-star measurements is found to be 6%. The absolute calibration is corrected using galaxy spectra, providing colors accurate to 2% or better. Stellar and galaxy colors and counts agree well with the expected values. Finally, as the first step in the scientific analysis of these data we construct panchromatic number counts which confirm that both the geometry of the universe and the galaxy population are evolving.

Original language	English
Pages (from-to)	99-116
Number of pages	18
Journal	Astrophysical Journal, Supplement Series
Volume	172
Issue number	1
DOIs	https://doi.org/10.1086/519081
Publication status	Published - 2007

Keywords

Cosmology: observations
Galaxies: evolution
Large-scale structure of universe
Surveys

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10.1086/519081

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Capak, P., Aussel, H., Ajiki, M., McCracken, H. J., Mobasher, B., Scoville, N., Shopbell, P., Taniguchi, Y., Thompson, D., Tribiano, S., Sasaki, S., Blain, A. W., Brusa, M., Carilli, C., Comastri, A., Carollo, C. M., Cassata, P., Colbert, J., Ellis, R. S., ... Zamorani, G. (2007). The first release COSMOS optical and near-IR data and catalog. Astrophysical Journal, Supplement Series, 172(1), 99-116. https://doi.org/10.1086/519081

@article{5873a83a79bb4ac7831c0900ccfa5880,

title = "The first release COSMOS optical and near-IR data and catalog",

abstract = "We present imaging data and photometry for the COSMOS survey in 15 photometric bands between 0.3 and 2.4 μm. These include data taken on the Subaru 8.3 m telescope, the KPNO and CTIO 4 m telescopes, and the CFHT 3.6 m telescope. Special techniques are used to ensure that the relative photometric calibration is better than 1 % across the field of view. The absolute photometric accuracy from standard-star measurements is found to be 6%. The absolute calibration is corrected using galaxy spectra, providing colors accurate to 2% or better. Stellar and galaxy colors and counts agree well with the expected values. Finally, as the first step in the scientific analysis of these data we construct panchromatic number counts which confirm that both the geometry of the universe and the galaxy population are evolving.",

keywords = "Cosmology: observations, Galaxies: evolution, Large-scale structure of universe, Surveys",

author = "P. Capak and H. Aussel and M. Ajiki and McCracken, {H. J.} and B. Mobasher and N. Scoville and P. Shopbell and Y. Taniguchi and D. Thompson and S. Tribiano and S. Sasaki and Blain, {A. W.} and M. Brusa and C. Carilli and A. Comastri and Carollo, {C. M.} and P. Cassata and J. Colbert and Ellis, {R. S.} and M. Elvis and M. Giavalisco and W. Green and L. Guzzo and G. Hasinger and O. Ilbert and C. Impey and K. Jahnke and J. Kartaltepe and Kneib, {J. P.} and J. Koda and A. Koekemoer and Y. Komiyama and A. Leauthaud and O. Lefevre and S. Lilly and C. Liu and R. Massey and S. Miyazaki and T. Murayama and T. Nagao and Peacock, {J. A.} and A. Pickles and C. Porciani and A. Renzini and J. Rhodes and M. Rich and M. Salvato and Sanders, {D. B.} and C. Scarlata and D. Schiminovich and E. Schinnerer and M. Scodeggio and K. Sheth and Y. Shioya and Tasca, {L. A.M.} and Taylor, {J. E.} and L. Yan and G. Zamorani",

year = "2007",

doi = "10.1086/519081",

language = "English",

volume = "172",

pages = "99--116",

journal = "Astrophysical Journal, Supplement Series",

issn = "0067-0049",

publisher = "American Astronomical Society",

number = "1",

}

Capak, P, Aussel, H, Ajiki, M, McCracken, HJ, Mobasher, B, Scoville, N, Shopbell, P, Taniguchi, Y, Thompson, D, Tribiano, S, Sasaki, S, Blain, AW, Brusa, M, Carilli, C, Comastri, A, Carollo, CM, Cassata, P, Colbert, J, Ellis, RS, Elvis, M, Giavalisco, M, Green, W, Guzzo, L, Hasinger, G, Ilbert, O, Impey, C, Jahnke, K, Kartaltepe, J, Kneib, JP, Koda, J, Koekemoer, A, Komiyama, Y, Leauthaud, A, Lefevre, O, Lilly, S, Liu, C, Massey, R, Miyazaki, S, Murayama, T, Nagao, T, Peacock, JA, Pickles, A, Porciani, C, Renzini, A, Rhodes, J, Rich, M, Salvato, M, Sanders, DB, Scarlata, C, Schiminovich, D, Schinnerer, E, Scodeggio, M, Sheth, K, Shioya, Y, Tasca, LAM, Taylor, JE, Yan, L & Zamorani, G 2007, 'The first release COSMOS optical and near-IR data and catalog', Astrophysical Journal, Supplement Series, vol. 172, no. 1, pp. 99-116. https://doi.org/10.1086/519081

TY - JOUR

T1 - The first release COSMOS optical and near-IR data and catalog

AU - Capak, P.

AU - Aussel, H.

AU - Ajiki, M.

AU - McCracken, H. J.

AU - Mobasher, B.

AU - Scoville, N.

AU - Shopbell, P.

AU - Taniguchi, Y.

AU - Thompson, D.

AU - Tribiano, S.

AU - Sasaki, S.

AU - Blain, A. W.

AU - Brusa, M.

AU - Carilli, C.

AU - Comastri, A.

AU - Carollo, C. M.

AU - Cassata, P.

AU - Colbert, J.

AU - Ellis, R. S.

AU - Elvis, M.

AU - Giavalisco, M.

AU - Green, W.

AU - Guzzo, L.

AU - Hasinger, G.

AU - Ilbert, O.

AU - Impey, C.

AU - Jahnke, K.

AU - Kartaltepe, J.

AU - Kneib, J. P.

AU - Koda, J.

AU - Koekemoer, A.

AU - Komiyama, Y.

AU - Leauthaud, A.

AU - Lefevre, O.

AU - Lilly, S.

AU - Liu, C.

AU - Massey, R.

AU - Miyazaki, S.

AU - Murayama, T.

AU - Nagao, T.

AU - Peacock, J. A.

AU - Pickles, A.

AU - Porciani, C.

AU - Renzini, A.

AU - Rhodes, J.

AU - Rich, M.

AU - Salvato, M.

AU - Sanders, D. B.

AU - Scarlata, C.

AU - Schiminovich, D.

AU - Schinnerer, E.

AU - Scodeggio, M.

AU - Sheth, K.

AU - Shioya, Y.

AU - Tasca, L. A.M.

AU - Taylor, J. E.

AU - Yan, L.

AU - Zamorani, G.

PY - 2007

Y1 - 2007

N2 - We present imaging data and photometry for the COSMOS survey in 15 photometric bands between 0.3 and 2.4 μm. These include data taken on the Subaru 8.3 m telescope, the KPNO and CTIO 4 m telescopes, and the CFHT 3.6 m telescope. Special techniques are used to ensure that the relative photometric calibration is better than 1 % across the field of view. The absolute photometric accuracy from standard-star measurements is found to be 6%. The absolute calibration is corrected using galaxy spectra, providing colors accurate to 2% or better. Stellar and galaxy colors and counts agree well with the expected values. Finally, as the first step in the scientific analysis of these data we construct panchromatic number counts which confirm that both the geometry of the universe and the galaxy population are evolving.

AB - We present imaging data and photometry for the COSMOS survey in 15 photometric bands between 0.3 and 2.4 μm. These include data taken on the Subaru 8.3 m telescope, the KPNO and CTIO 4 m telescopes, and the CFHT 3.6 m telescope. Special techniques are used to ensure that the relative photometric calibration is better than 1 % across the field of view. The absolute photometric accuracy from standard-star measurements is found to be 6%. The absolute calibration is corrected using galaxy spectra, providing colors accurate to 2% or better. Stellar and galaxy colors and counts agree well with the expected values. Finally, as the first step in the scientific analysis of these data we construct panchromatic number counts which confirm that both the geometry of the universe and the galaxy population are evolving.

KW - Cosmology: observations

KW - Galaxies: evolution

KW - Large-scale structure of universe

KW - Surveys

UR - http://www.scopus.com/inward/record.url?scp=35348871176&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=35348871176&partnerID=8YFLogxK

U2 - 10.1086/519081

DO - 10.1086/519081

M3 - Article

AN - SCOPUS:35348871176

SN - 0067-0049

VL - 172

SP - 99

EP - 116

JO - Astrophysical Journal, Supplement Series

JF - Astrophysical Journal, Supplement Series

IS - 1

ER -

The first release COSMOS optical and near-IR data and catalog

Abstract

Keywords

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