Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/35827
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Wright, Nicholas J. | en_US |
dc.contributor.author | Drake, Jeremy J. | en_US |
dc.contributor.author | GUARCELLO, Mario Giuseppe | en_US |
dc.contributor.author | Aldcroft, Tom L. | en_US |
dc.contributor.author | Kashyap, Vinay L. | en_US |
dc.contributor.author | DAMIANI, Francesco | en_US |
dc.contributor.author | DePasquale, Joe | en_US |
dc.contributor.author | Fruscione, Antonella | en_US |
dc.date.accessioned | 2025-02-06T15:06:06Z | - |
dc.date.available | 2025-02-06T15:06:06Z | - |
dc.date.issued | 2023 | en_US |
dc.identifier.issn | 0067-0049 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/35827 | - |
dc.description.abstract | The Cygnus OB2 association is the largest concentration of young and massive stars within 2 kpc of the Sun, including an estimated ∼65 O-type stars and hundreds of OB stars. The Chandra Cygnus OB2 Legacy Survey is a large imaging program undertaken with the Advanced CCD Imaging Spectrometer on board the Chandra X-ray Observatory. The survey has imaged the central 0.5 deg2 of the Cyg OB2 association with an effective exposure of ∼120 ks and an outer 0.35 deg2 area with an exposure of ∼60 ks. Here we describe the survey design and observations, discuss the data reduction and source detection, and present a catalog of ∼8000 X-ray point sources. The survey design employs a grid of 36 heavily (∼50%) overlapping pointings, a method that overcomes Chandra's low off-axis sensitivity and produces a highly uniform exposure over the inner 0.5 deg2. The full X-ray catalog is described here and is made available online. | en_US |
dc.language.iso | eng | en_US |
dc.title | The Chandra Cygnus OB2 Legacy Survey: Design and X-Ray Point-source Catalog | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3847/1538-4365/acdd62 | en_US |
dc.identifier.scopus | 2-s2.0-85176422107 | en_US |
dc.identifier.isi | 001087307700001 | en_US |
dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/85176422107 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/1538-4365/acdd62 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 269 | en_US |
dc.relation.issue | 1 | en_US |
dc.relation.firstpage | 7 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 8 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.contributor.country | GBR | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | THE ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering | en_US |
dc.description.apc | sì | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.cerifentitytype | Publications | - |
crisitem.author.dept | O.A. Palermo | - |
crisitem.author.dept | O.A. Palermo | - |
crisitem.author.orcid | 0000-0002-3010-2310 | - |
crisitem.author.orcid | 0000-0002-7065-3061 | - |
crisitem.journal.journalissn | 0067-0049 | - |
crisitem.journal.ance | E016254 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
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Wright_2023_ApJS_269_7.pdf | PDF editoriale | 1.19 MB | Adobe PDF | View/Open |
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