Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/24897
DC Field | Value | Language |
---|---|---|
dc.contributor.author | LaMassa, Stephanie M. | en_US |
dc.contributor.author | Urry, C. Megan | en_US |
dc.contributor.author | CAPPELLUTI, Nico | en_US |
dc.contributor.author | Böhringer, Hans | en_US |
dc.contributor.author | COMASTRI, Andrea | en_US |
dc.contributor.author | Glikman, Eilat | en_US |
dc.contributor.author | Richards, Gordon | en_US |
dc.contributor.author | Ananna, Tonima | en_US |
dc.contributor.author | Brusa, Marcella | en_US |
dc.contributor.author | Cardamone, Carie | en_US |
dc.contributor.author | Chon, Gayoung | en_US |
dc.contributor.author | Civano, Francesca | en_US |
dc.contributor.author | Farrah, Duncan | en_US |
dc.contributor.author | Gilfanov, Marat | en_US |
dc.contributor.author | Green, Paul | en_US |
dc.contributor.author | Komossa, S. | en_US |
dc.contributor.author | Lira, Paulina | en_US |
dc.contributor.author | Makler, Martin | en_US |
dc.contributor.author | MARCHESI, STEFANO | en_US |
dc.contributor.author | Pecoraro, Robert | en_US |
dc.contributor.author | Ranalli, Piero | en_US |
dc.contributor.author | Salvato, Mara | en_US |
dc.contributor.author | Schawinski, Kevin | en_US |
dc.contributor.author | Stern, Daniel | en_US |
dc.contributor.author | Treister, Ezequiel | en_US |
dc.contributor.author | Viero, Marco | en_US |
dc.date.accessioned | 2020-05-15T16:17:12Z | - |
dc.date.available | 2020-05-15T16:17:12Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 0004-637X | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/24897 | - |
dc.description.abstract | We release the next installment of the Stripe 82 X-ray survey point-source catalog, which currently covers 31.3 deg<SUP>2</SUP> 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<SUP>-16</SUP> erg s<SUP>-1</SUP> cm<SUP>-2</SUP>, 4.7 × 10<SUP>-15</SUP> erg s<SUP>-1</SUP> cm<SUP>-2</SUP>, and 2.1 × 10<SUP>-15</SUP> erg s<SUP>-1</SUP> cm<SUP>-2</SUP> 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<SUP>-15</SUP> erg s<SUP>-1</SUP> cm<SUP>-2</SUP>, 2.9 × 10<SUP>-14</SUP> erg s<SUP>-1</SUP> cm<SUP>-2</SUP>, and 1.7 × 10<SUP>-14</SUP> erg s<SUP>-1</SUP> cm<SUP>-2</SUP>. 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. | en_US |
dc.language.iso | eng | en_US |
dc.title | The 31 Deg2 Release of the Stripe 82 X-Ray Survey: The Point Source Catalog | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3847/0004-637X/817/2/172 | en_US |
dc.identifier.scopus | 2-s2.0-84958020000 | en_US |
dc.identifier.isi | 000369437900089 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/0004-637X/817/2/172 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/0004-637X/817/2/172/pdf | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 817 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | 172 | en_US |
dc.relation.lastpage | 192 | en_US |
dc.relation.numberofpages | 21 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 26 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | THE ASTROPHYSICAL JOURNAL | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2016ApJ...817..172L | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.orcid | 0000-0003-3451-9970 | - |
crisitem.author.orcid | 0000-0001-5544-0749 | - |
crisitem.journal.journalissn | 0004-637X | - |
crisitem.journal.ance | E016252 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
1510.00852.pdf | preprint | 3.78 MB | Adobe PDF | View/Open |
LaMassa_2016_ApJ_817_172.pdf | pdf editoriale | 1.91 MB | Adobe PDF | View/Open |
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