activity
20022009
most citedThe Subaru/XMM-Newton Deep Survey (SXDS) - II. Optical Imaging and Photometric Catalogs

316 citations · 521 across the 4 of their papers we have counts for

collaborators

9 papers

astro-ph.CO2009115 cited

MOIRCS Deep Survey IV: Evolution of Galaxy Stellar Mass Function Back to z ~ 3

M. Kajisawa, T. Ichikawa, I. Tanaka +11

We use very deep near-infrared (NIR) imaging data obtained in MOIRCS Deep Survey (MODS) to investigate the evolution of the galaxy stellar mass function back to z~3. The MODS data…

astro-ph.CO200928 cited

MOIRCS Deep Survey III: Active Galactic Nuclei in Massive Galaxies at z=2-4

T. Yamada, M. Kajisawa, M. Akiyama +9

We investigate the X-ray properties of the K-band-selected galaxies at redshift 2 < z < 4 by using our deep near-infrared images obtained in the MOIRCS Deep Survey project and the…

astro-ph2008316 cited

The Subaru/XMM-Newton Deep Survey (SXDS) - II. Optical Imaging and Photometric Catalogs

H. Furusawa, G. Kosugi, M. Akiyama +33

We present multi-waveband optical imaging data obtained from observations of the Subaru/XMM-Newton Deep Survey (SXDS). The survey field, centered at R.A.=02:18:00, decl.=-05:00:00,…

astro-ph200662 cited

Proto-Clusters with Evolved Populations around Radio Galaxies at z~2.5

Masaru Kajisawa, Tadayuki Kodama, Ichi Tanaka +2

We report a discovery of proto-cluster candidates around high redshift radio galaxies at z~2.5 on the basis of clear statistical excess of colour-selected galaxies around them seen…

astro-ph2005

Spectroscopically Confirmed Large-Scale Structures Associated to a z=0.83 Cluster

Masayuki Tanaka, Tadayuki Kodama, Nobuo Arimoto +1

(Abridged) We present a discovery of definitive large-scale structures around RXJ0152.7--1352 at z=0.83 based on spectroscopic redshifts. In our previous papers, we reported a phot…

astro-ph2005

The Number Density of Old Passively-Evolving Galaxies at z=1 in the Subaru/XMM-Newton Deep Survey Field

Toru Yamada, Tadayuki Kodama, Masayuki Akiyama +10

We obtained the number counts and the rest-frame B-band luminosity function of the color-selected old passively-evolving galaxies (OPEGs) at z=1 with very high statistical accuracy…