dc.creatorLaMassa, Stephanie
dc.creatorUrry, C. Megan
dc.creatorCappellut, Nico
dc.creatorBöhringer, Hans
dc.creatorComastri, Andrea
dc.creatorGlikman, Eilat
dc.creatorRichards, Gordon
dc.creatorAnanna, Tonima
dc.creatorBrusa, Marcella
dc.creatorCardamone, Carie
dc.creatorChon, Gayoung
dc.creatorCivano, Francesca
dc.creatorFarrah, Duncan
dc.creatorGilfanov, Marat
dc.creatorGreen, Paul
dc.creatorKomossa, S.
dc.creatorLira Teillery, Paulina
dc.creatorMakler, Martin
dc.creatorMarchesi, Stefano
dc.creatorPecoraro, Robert
dc.creatorRanalli, Piero
dc.creatorSalvato, Mara
dc.creatorSchawinski, Kevin
dc.creatorStern, Daniel
dc.creatorTreister, Ezequiel
dc.creatorViero, Marco
dc.date.accessioned2017-01-12T13:41:09Z
dc.date.available2017-01-12T13:41:09Z
dc.date.created2017-01-12T13:41:09Z
dc.date.issued2016-02-01
dc.identifierThe Astrophysical Journal, 817:172 (21pp), 2016 February 1
dc.identifier10.3847/0004-637X/817/2/172
dc.identifierhttps://repositorio.uchile.cl/handle/2250/142389
dc.description.abstractWe release the next installment of the Stripe 82 X-ray survey point-source catalog, which currently covers 31.3 deg2 of the Sloan Digital Sky Survey (SDSS) Stripe 82 Legacy field. In total, 6181 unique X-ray sources are significantly detected with XMM-Newton (>5σ) and Chandra (>4.5σ). This catalog release includes data from XMM-Newton cycle AO 13, which approximately doubled the Stripe 82X survey area. The flux limits of the Stripe 82X survey are 8.7 × 10−16 erg s−1 cm−2, 4.7 × 10−15 erg s−1 cm−2, and 2.1 × 10−15 erg s−1 cm−2 in the soft (0.5–2 keV), hard (2–10 keV), and full bands (0.5–10 keV), respectively, with approximate half-area survey flux limits of 5.4 × 10−15 erg s−1 cm−2, 2.9 × 10−14 erg s−1 cm−2, and 1.7 × 10−14 erg s−1 cm−2. We matched the X-ray source lists to available multi-wavelength catalogs, including updated matches to the previous release of the Stripe 82X survey; 88% of the sample is matched to a multi-wavelength counterpart. Due to the wide area of Stripe 82X and rich ancillary multi-wavelength data, including coadded SDSS photometry, mid-infrared WISE coverage, near-infrared coverage from UKIDSS and VISTA Hemisphere Survey, ultraviolet coverage from GALEX, radio coverage from FIRST, and far-infrared coverage from Herschel, as well as existing ~30% optical spectroscopic completeness, we are beginning to uncover rare objects, such as obscured high-luminosity active galactic nuclei at high-redshift. The Stripe 82X point source catalog is a valuable data set for constraining how this population grows and evolves, as well as for studying how they interact with the galaxies in which they live.
dc.languageen
dc.publisherThe American Astronomical Society
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile
dc.sourceThe Astrophysical Journal
dc.subjectCatalogs
dc.subjectGalaxies: active
dc.subjectQuasars: general
dc.subjectSurveys
dc.subjectX-rays: general
dc.titleThe 31 DEG2 release of the stripe 82 X-RAY survey: the point source catalog
dc.typeArtículo de revista


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