activity
20062008
most citedCOSMOS Photometric Redshifts with 30-bands for 2-deg2

1.2k citations · 2.6k across the 7 of their papers we have counts for

collaborators

7 papers

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-ph200857 cited

The zCOSMOS redshift survey: the three-dimensional classification cube and bimodality in galaxy physical properties

M. Mignoli, G. Zamorani, M. Scodeggio +56

Aims. We investigate the relationships between three main optical galaxy observables (spectral properties, colours, and morphology), exploiting the data set provided by the COSMOS/…

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-ph200839 cited

The optical spectra of 24 micron galaxies in the COSMOS field: I. Spitzer/MIPS bright sources in the zCOSMOS-bright 10k catalogue

K. I. Caputi, S. J. Lilly, H. Aussel +23

We study zCOSMOS-bright optical spectra for 609 Spitzer/MIPS 24 micron-selected galaxies with S(24um)> 0.30 mJy and I<22.5 (AB mag) over 1.5 sq. deg. of the COSMOS field. From emis…

astro-ph200721 cited

The contribution of very massive high-redshift SWIRE galaxies to the stellar mass function

S. Berta, C. J. Lonsdale, M. Polletta +18

(Abridged) We selected high-z massive galaxies at 5.8 microns, in the SWIRE ELAIS-S1 field (1 sq. deg.). Galaxies with the 1.6 microns stellar peak redshifted into the IRAC bands (…

astro-ph2007145 cited

Precision photometric redshift calibration for galaxy-galaxy weak lensing

R. Mandelbaum, U. Seljak, C. M. Hirata +26

Accurate photometric redshifts are among the key requirements for precision weak lensing measurements. Both the large size of the Sloan Digital Sky Survey (SDSS) and the existence…