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20042009
most citedCOSMOS Photometric Redshifts with 30-bands for 2-deg2

1.2k citations · 5k across the 31 of their papers we have counts for

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21 papers · 1 filter

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-ph2008380 cited

Photometric redshift and classification for the XMM-COSMOS sources

M. Salvato, G. Hasinger, O. Ilbert +40

We present photometric redshifts and spectral energy distribution (SED) classifications for a sample of 1542 optically identified sources detected with XMM in the COSMOS field. Our…

astro-ph2008131 cited

Spectroscopic Confirmation Of An Extreme Starburst At Redshift 4.547

Peter Capak, C. L. Carilli, N. Lee +22

We report the spectroscopic confirmation of a sub-mm galaxy (SMG) at z=4.547 with an estimated L_IR=0.5-2.0x10^13 L_sun. The spectra, mid-IR, and X-ray properties indicate the bolo…

astro-ph200863 cited

A photometric survey for Lyalpha-HeII dual emitters: Searching for Population III stars in high-redshift galaxies

Tohru Nagao, Shunji Sasaki, Roberto Maiolino +9

We present a new photometric search for high-z galaxies hosting Population III (PopIII) stars based on deep intermediate-band imaging observations obtained in the Subaru Deep Field…

astro-ph200780 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-ph200764 cited

The angular correlations of galaxies in the COSMOS field

H. J. McCracken, J. A. Peacock, L. Guzzo +21

We present measurements of the two-point galaxy angular correlation function w(θ) in the COSMOS field. Independent determinations of w(θ) as a function of magnitude limit are prese…