X-ray sources in the 1.75 Ms Ultra Narrow Deep Field observed by XMM-Newton
arXiv:2106.10455 · doi:10.3847/1538-4357/ac0d5d
Abstract
In this work we present the results of the survey carried out on one of the deepest X-ray fields observed by the XMM-Newton satellite. The 1.75 Ms Ultra Narrow Deep Field (XMM175UNDF) survey is made by 13 observations taken over 2 years with a total exposure time of 1.75 Ms (1.372 Ms after flare-filtered) in a field of centered around the blazar 1ES 1553+113. We stacked the 13 observations reaching flux limits of , , and in the soft , hard , and full bands, respectively. Using a conservative threshold of Maximum Likelihood significance of , corresponding to , we detected 301 point-sources for which we derived positions, fluxes in different bands, and hardness ratios. Thanks to an optical follow-up carried out using the 10.4m the Gran Telescopio Canarias (GTC) on the same field in the bands, combined with WISE/2MASS IR data; we identified 244 optical/IR counterpart candidates for our X-ray sources and estimated their X-ray luminosities, redshift distribution, X-ray/optical X-ray/IR flux ratios, and absolute magnitudes. Finally, we divided this subsample in 40 non-active sources and 204 AGNs, of which 139 are classified as Seyfert galaxies and 41 as Quasars.
30 pages, 19 figures, to be published in ApJ
References in corpus (15)
- The Cosmic Evolution Survey (COSMOS) -- Overview
- The Sixteenth Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra
- The synthesis of the cosmic X-ray background in the Chandra and XMM-Newton era
- The Chandra Deep Field-South Survey: 7 Ms Source Catalogs
- The Chandra COSMOS Survey, I: Overview and Point Source Catalog
- The XMM-Newton serendipitous survey IX. The fourth XMM-Newton serendipitous source catalogue
- Cosmic X-ray Surveys of Distant Active Galaxies: The Demographics, Physics, and Ecology of Growing Supermassive Black Holes
- The XMM-Newton wide-field survey in the COSMOS field: III. optical identification and multiwavelength properties of a large sample of X-ray selected sources
- The VLA Survey of the Chandra Deep Field South: I. Overview of the Radio Data
- The deepest X-ray view of high-redshift galaxies: constraints on low-rate black-hole accretion
- The XMM-Newton serendipitous survey. X: The second source catalogue from overlapping XMM-Newton observations and its long-term variable content
- Low-Level Nuclear Activity in Nearby Spiral Galaxies
- The Physical Origins of the Identified and Still Missing Components of the Warm-Hot Intergalactic Medium: Insights from Deep Surveys in the Field of Blazar 1ES1553+113
- Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras
- Observational characteristics of accretion onto black holes