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The Cosmic Evolution Survey (COSMOS): Subaru Observations of the HST COSMOS Field

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arxiv astro-ph/0612295 v1 pith:OPVESPFH submitted 2006-12-12 astro-ph

Y. Taniguchi , N. Scoville , T. Murayama , D. B. Sanders , B. Mobasher , H. Aussel , P. Capak , M. Ajiki
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S. Miyazaki Y. Komiyama Y. Shioya T. Nagao S. S. Sasaki J. Koda C. Carilli M. Giavalisco L. Guzzo G. Hasinger C. Impey O. LeFevre S. Lilly A. Renzini M. Rich E. Schinnerer P. Shopbell N. Kaifu H. Karoji N. Arimoto S. Okamura K. Ohta
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We present deep optical imaging observations of 2 square degree area, covered by the Cosmic Evolution Survey (COSMOS), made by the prime-focus Camera (Supreme-Cam) on the 8.2m Subaru Telescope. Observations were done in six broad-band [B (4459.7 AA), g' (4723.1 AA), V (5483.8 AA), r' (6213.0 AA), i' (7640.8 AA), z' (8855.0 AA)], and one narrow-band (NB816) filters. A total of 10^6 galaxies were detected to i'~26.5 mag. These data, combined with observations at u* and K-band are used to construct the photometric catalogs for the COSMOS and to measure their photometric redshifts, multi-band spectral energy distributions, stellar masses and identification of high redshift candidates. This catalog provides multi-waveband data for scientific analysis of the COSMOS survey.

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Cited by 2 Pith papers

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  1. Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters

    astro-ph.GA 2026-06 unverdicted novelty 7.0 of 10

    Anisotropic quenching is detected at the highest redshift yet and linked to preprocessing dominating over intrahalo effects by ~20% along the major axis in a delay-then-rapid quenching model informed by cluster accret...

  2. COSMOS-Web: does halo mass alone shape the clustering of star-forming and quiescent galaxies?

    astro-ph.GA 2026-06 unverdicted novelty 5.0 of 10

    Quiescent galaxies cluster more strongly than star-forming ones by 0.5-1 dex after halo-mass matching, with one-halo conformity up to z~2 that disappears at higher redshifts.

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