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arXiv 2015-12-03 DOI 10.3847/0004-637X/817/1/34 0 views

The Chandra COSMOS Legacy survey: optical/IR identifications

Marchesi, S. · Civano, F. · Elvis, M. · Salvato, M. · Brusa, M. · Comastri, A. · Gilli, R. · Hasinger, G. · Lanzuisi, G. · Miyaji, T. · Treister, E. · Urry, C. M. · Vignali, C. · Zamorani, G. · Allevato, V. · Cappelluti, N. · Cardamone, C. · Finoguenov, A. · Griffiths, R. E. · Karim, A. · Laigle, C. · LaMassa, S. M. · Jahnke, K. · Ranalli, P. · Schawinski, K. · Schinnerer, E. · Silverman, J. D. · Smolcic, V. · Suh, H. · Trakhtenbrot, B.

Original · EN

We present the catalog of optical and infrared counterparts of the Chandra COSMOS-Legacy Survey, a 4.6 Ms Chandra program on the 2.2 square degrees of the COSMOS field, combination of 56 new overlapping observations obtained in Cycle 14 with the previous C-COSMOS survey. In this Paper we report the i, K, and 3.6 micron identifications of the 2273 X-ray point sources detected in the new Cycle 14 observations. We use the likelihood ratio technique to derive the association of optical/infrared (IR) counterparts for 97% of the X-ray sources. We also update the information for the 1743 sources detected in C-COSMOS, using new K and 3.6 micron information not available when the C-COSMOS analysis was performed. The final catalog contains 4016 X-ray sources, 97% of which have an optical/IR counterpart and a photometric redshift, while 54% of the sources have a spectroscopic redshift. The full catalog, including spectroscopic and photometric redshifts and optical and X-ray properties described here in detail, is available online. We study several X-ray to optical (X/O) properties: with our large statistics we put better constraints on the X/O flux ratio locus, finding a shift towards faint optical magnitudes in both soft and hard X-ray band. We confirm the existence of a correlation between X/O and the the 2-10 keV luminosity for Type 2 sources. We extend to low luminosities the analysis of the correlation between the fraction of obscured AGN and the hard band luminosity, finding a different behavior between the optically and X-ray classified obscured fraction.

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