Finding Rare AGN: X-ray Number Counts of Chandra Sources in Stripe 82

Дата и время публикации : 2012-10-01T20:02:14Z

Авторы публикации и институты :
Stephanie M. LaMassa
C. Megan Urry
Eilat Glikman
Nico Cappelluti
Francesca Civano
Andrea Comastri
Ezequiel Treister
Hans Boehringer
Carie Cardamone
Gayoung Chon
Miranda Kephart
Stephen S. Murray
Gordon Richards
Nic Ross
Joshua S. Rozner
Kevin Schawinski

Ссылка на журнал-издание: Ссылка на журнал-издание не найдена
Коментарии к cтатье: Accepted for publication in MNRAS, 15 pages, 6 Figures, 2 Tables
Первичная категория: astro-ph.CO

Все категории : astro-ph.CO

Краткий обзор статьи: We present the first results of a wide area X-ray survey within the Sloan Digital Sky Survey (SDSS) Stripe 82, a 300 deg$^2$ region of the sky with a substantial investment in multi-wavelength coverage. We analyzed archival {it Chandra} observations that cover 7.5 deg$^2$ within Stripe 82 ("Stripe 82 ACX"), reaching 4.5$sigma$ flux limits of 7.9$times10^{-16}$, 3.4$times10^{-15}$ and 1.8$times10^{-15}$ erg s$^{-1}$ cm$^{-2}$ in the soft (0.5-2 keV), hard (2-7 keV) and full (0.5-7 keV) bands, to find 774, 239 and 1118 X-ray sources, respectively. Three hundred twenty-one sources are detected only in the full band and 9 sources are detected solely in the soft band. Utilizing data products from the {it Chandra} Source Catalog, we construct independent Log$N$-Log$S$ relationships, detailing the number density of X-ray sources as a function of flux, which show general agreement with previous {it Chandra} surveys. We compare the luminosity distribution of Stripe 82 ACX with the smaller, deeper CDF-S + E-CDFS surveys and with {it Chandra}-COSMOS, illustrating the benefit of wide-area surveys in locating high luminosity AGN. We also investigate the differences and similarities of X-ray and optical selection to uncover obscured AGN in the local Universe. Finally, we estimate the population of AGN we expect to find with increased coverage of 100 deg$^2$ or 300 deg$^2$, which will provide unprecedented insight into the high redshift, high luminosity regime of black hole growth currently under-represented in X-ray surveys.

Category: Physics