most citedA Deficit of Faint Red Galaxies in the Possible Large-Scale Structures around the RDCS J1252.9-2927 Cluster at z=1.24

47 citations · 59 across the 3 of their papers we have counts for

collaborators
Showing astro-phShow all

13 papers · 1 filter

astro-ph2008107 cited

The spatial clustering of X-ray selected AGN in the XMM-COSMOS field

R. Gilli, G. Zamorani, T. Miyaji +70

We study the spatial clustering of 538 X-ray selected AGN in the 2 deg^2 XMM-COSMOS field that are spectroscopically identified to I_{AB}<23 and span the redshift range z=0.2-3.0.…

astro-ph200868 cited

Mapping dusty star formation in and around a cluster at z=0.81 by wide-field imaging with AKARI

Yusei Koyama, Tadayuki Kodama, Kazuhiro Shimasaku +8

We present environmental dependence of dusty star forming activity in and around the cluster RXJ1716.4+6708 at z=0.81 based on wide-field and multi-wavelength observations with Sup…

astro-ph20081.2k cited

COSMOS Photometric Redshifts with 30-bands for 2-deg2

O. Ilbert, P. Capak, M. Salvato +60

We present accurate photometric redshifts in the 2-deg2 COSMOS field. The redshifts are computed with 30 broad, intermediate, and narrow bands covering the UV (GALEX), Visible-NIR…

astro-ph200840 cited

The Environmental Dependence of Properties of Galaxies around the RDCSJ0910+54 Cluster at z=1.1

M. Tanaka, A. Finoguenov, T. Kodama +6

(Abridged) We report on the environmental dependence of properties of galaxies around the RDCSJ0910+54 cluster at z=1.1. We have obtained multi-band wide-field images of the cluste…

astro-ph2008573 cited

The Milky Way Tomography with SDSS: II. Stellar Metallicity

Zeljko Ivezic, Branimir Sesar, Mario Juric +50

Using effective temperature and metallicity derived from SDSS spectra for ~60,000 F and G type main sequence stars (0.2<g-r<0.6), we develop polynomial models for estimating these…

astro-ph200735 cited

Dependence of the Build-up of the Colour-Magnitude Relation on Cluster Richness at z ~ 0.8

Yusei Koyama, Tadayuki Kodama, Masayuki Tanaka +2

We present environmental dependence of the build-up of the colour-magnitude relation (CMR) at z ~ 0.8. It is well established that massive early-type galaxies exhibit a tight CMR i…