activity
20012007
most citedThe First Release COSMOS Optical and Near-IR Data and Catalog

803 citations · 3.3k across the 38 of their papers we have counts for

collaborators

38 papers

astro-ph2007★ 80 cited

The H Luminosity Function and Star Formation Rate at in the Cosmos 2 Square-Degree Field

Y. Shioya, Y. Taniguchi, S. S. Sasaki +25

To derive a new H luminosity function and to understand the clustering properties of star-forming galaxies at , we have made a narrow-band imaging survey for H$α…

astro-ph2007★ 803 cited

The First Release COSMOS Optical and Near-IR Data and Catalog

P. Capak, H. Aussel, M. Ajiki +54

We present imaging data and photometry for the COSMOS survey in 15 photometric bands between 0.3um and 2.4um. These include data taken on the Subaru 8.3m telescope, the KPNO and CT…

astro-ph2007★ 55 cited

The [OII]3727 Luminosity function and Star Formation Rate at z~1.2 in the COSMOS 2 Square-degree Field and the Subaru Deep Field

M. I. Takahashi, Y. Shioya, Y. Taniguchi +31

We have carried out a wide-field imaging survey for [OII]3727 emitting galaxies at z~1.2 in the HST COSMOS 2 square degree field using the Suprime-Cam on the Subaru Telescope. The…

astro-ph2007★ 23 cited

High-redshift Ly alpha emitters with a large equivalent width: Properties of i-dropout galaxies with an NB921-band depression in the Subaru Deep Field

Tohru Nagao, Takashi Murayama, Roberto Maiolino +11

We report new follow-up spectroscopy of i-dropout galaxies with an NB921-band depression found in the Subaru Deep Field. The NB921-depressed i-dropout selection method is expected…

astro-ph2007★ 143 cited

The redshift evolution of early-type galaxies in COSMOS: Do massive early-type galaxies form by dry mergers?

C. Scarlata, C. M. Carollo, S. J. Lilly +26

ABRIDGED: We study the evolution since z~1 of the rest-frame B luminosity function of the early-type galaxies (ETGs) in ~0.7 deg^2 in the COSMOS field. In order to identify ALL pro…

astro-ph2007★ 169 cited

The HI content of star-forming galaxies at z = 0.24

Philip Lah, Jayaram N. Chengalur, Frank H. Briggs +12

We use observations from the Giant Metrewave Radio Telescope (GMRT) to measure the atomic hydrogen gas content of star-forming galaxies at z = 0.24 (i.e. a look-backtime of ~3 Gyr)…