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  • 标题:The deep Chandra survey in the SDSS J1030+0524 field ⋆
  • 本地全文:下载
  • 作者:R. Nanni ; R. Gilli ; C. Vignali
  • 期刊名称:Astronomy & Astrophysics
  • 印刷版ISSN:0004-6361
  • 电子版ISSN:1432-0746
  • 出版年度:2020
  • 卷号:637
  • 页码:1-20
  • DOI:10.1051/0004-6361/202037914
  • 语种:English
  • 出版社:EDP Sciences
  • 摘要:We present the X-ray source catalog for the ∼479 ksChandraexposure of the SDSS J1030+0524 field, which is centered on a region that shows the best evidence to date of an overdensity around az > 6 quasar, and also includes a galaxy overdensity around a Compton-thick Fanaroff-Riley type II (FRII) radio galaxy atz = 1.7. Usingwavdetectfor initial source detection and ACIS Extract for source photometry and significance assessment, we create preliminary catalogs of sources that are detected in the full (0.5−7.0 keV), soft (0.5−2.0 keV), and hard (2−7 keV) bands, respectively. We produce X-ray simulations that mirror ourChandraobservation to filter our preliminary catalogs and achieve a completeness level of > 91% and a reliability level of ∼95% in each band. The catalogs in the three bands are then matched into a final main catalog of 256 unique sources. Among them, 244, 193, and 208 are detected in the full, soft, and hard bands, respectively. TheChandraobservation covers a total area of 335 arcmin2and reaches flux limits over the central few square arcmins of ∼3 × 10−16, 6 × 10−17, and 2 × 10−16erg cm−2s−1in the full, soft, and hard bands, respectively This makes J1030 field the fifth deepest extragalactic X-ray survey to date. The field is part of the Multiwavelength Survey by Yale-Chile (MUSYC), and is also covered by optical imaging data from the Large Binocular Camera (LBC) at the Large Binocular Telescope (LBT), near-infrared imaging data from the Canada France Hawaii Telescope WIRCam (CFHT/WIRCam), andSpitzerIRAC. Thanks to its dense multi-wavelength coverage, J1030 represents a legacy field for the study of large-scale structures around distant accreting supermassive black holes. Using a likelihood ratio analysis, we associate multi-band (r,z,J, and 4.5 μm) counterparts for 252 (98.4%) of the 256Chandrasources, with an estimated reliability of 95%. Finally, we compute the cumulative number of sources in each X-ray band, finding that they are in general agreement with the results from theChandraDeep Fields.
  • 关键词:ensurveysX-rays: generalcatalogsgalaxies: high-redshiftquasars: supermassive black holes
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