Naslov
The Chandra Cosmos Legacy Survey: Overview and Point Source Catalog

Autori
Civano, F. ; Marchesi, S. ; Comastri, A. ; Urry, M. C. ; Elvis, M. ; Cappelluti, N. ; Puccetti, S. ; Brusa, M. ; Zamorani, G. ; Hasinger, G. ; Aldcroft, T. ; Alexander, D. M. ; Allevato, V. ; Brunner, H. ; Capak, P. ; Finoguenov, A. ; Fiore, F. ; Fruscione, A. ; Gilli, R. ; Glotfelty, K. ; Griffiths, R. E. ; Hao, H. ; Harrison, F. A. ; Jahnke, K. ; Kartaltepe, J. ; Karim, A. ; LaMassa, S. M. ; Lanzuisi, G. ; Miyaji, T. ; Ranalli, P. ; Salvato, M. ; Sargent, M. ; Scoville, N. J. ; Schawinski, K. ; Schinnerer, E. ; Silverman, J. ; Smolčić, Vernesa ; Stern, D. ; Toft, S. ; Trakhenbrot, B. ; Treister, E. ; Vignali, C.

Izvornik
The Astrophysical journal (0004-637X) 819 (2016), 1; 62-80

Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni

Ključne riječi
catalogs ; cosmology: observations ; galaxies: evolution ; quasars: general ; surveys ; X-rays: general

Sažetak
The COSMOS-Legacy survey is a 4.6 Ms Chandra program that has imaged 2.2 deg2 of the COSMOS field with an effective exposure of ≃ 160 ks over the central 1.5 deg2 and of ≃ 80 ks in the remaining area. The survey is the combination of 56 new observations obtained as an X-ray Visionary Project with the previous C-COSMOS survey. We describe the reduction and analysis of the new observations and the properties of 2273 point sources detected above a spurious probability of 2 × 10‑5. We also present the updated properties of the C-COSMOS sources detected in the new data. The whole survey includes 4016 point sources (3814, 2920 and 2440 in the full, soft, and hard band). The limiting depths are 2.2 × 10‑16, 1.5 × 10‑15, and 8.9 × 10‑16 {; ; ; \text{; ; ; erg cm}; ; ; }; ; ; -2 {; ; ; {; ; ; {; ; ; s}; ; ; }; ; ; }; ; ; -1 in the 0.5–2, 2–10, and 0.5–10 keV bands, respectively. The observed fraction of obscured active galactic nuclei with a column density >1022 cm‑2 from the hardness ratio (HR) is ∼50{; ; ; }; ; ; -16+17%. Given the large sample we compute source number counts in the hard and soft bands, significantly reducing the uncertainties of 5%–10%. For the first time we compute number counts for obscured (HR > ‑0.2) and unobscured (HR < ‑0.2) sources and find significant differences between the two populations in the soft band. Due to the unprecedent large exposure, COSMOS-Legacy area is three times larger than surveys at similar depths and its depth is three times fainter than surveys covering similar areas. The area-flux region occupied by COSMOS-Legacy is likely to remain unsurpassed for years to come.

Izvorni jezik
Engleski

Znanstvena područja
Fizika

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