The Chandra Cygnus OB2 Legacy Survey: Design and X-Ray Point-source Catalog

IF 8.6 1区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Nicholas J. Wright, Jeremy J. Drake, Mario G. Guarcello, Tom L. Aldcroft, Vinay L. Kashyap, Francesco Damiani, Joe DePasquale, Antonella Fruscione
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引用次数: 8

Abstract

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 deg 2 of the Cyg OB2 association with an effective exposure of ∼120 ks and an outer 0.35 deg 2 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 deg 2 . The full X-ray catalog is described here and is made available online.
钱德拉天鹅座OB2遗产调查:设计和x射线点源目录
天鹅座OB2星群是距离太阳2kpc内年轻大质量恒星最集中的星系,包括约65颗o型恒星和数百颗OB型恒星。钱德拉天鹅座OB2遗产巡天是一项大型成像项目,由钱德拉x射线天文台搭载的先进CCD成像光谱仪承担。该调查对Cyg OB2关联的中心0.5°2区域进行了成像,有效曝光时间为~ 120 ks,对外部0.35°2区域进行了成像,曝光时间为~ 60 ks。在这里,我们描述了调查设计和观测,讨论了数据缩减和源检测,并提出了一个约8000个x射线点源的目录。调查设计采用36个严重(~ 50%)重叠点的网格,这种方法克服了钱德拉的低离轴灵敏度,并在0.5°2内产生高度均匀的曝光。完整的x射线目录在这里描述,并在网上提供。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Astrophysical Journal Supplement Series
Astrophysical Journal Supplement Series 地学天文-天文与天体物理
CiteScore
14.50
自引率
5.70%
发文量
264
审稿时长
2 months
期刊介绍: The Astrophysical Journal Supplement (ApJS) serves as an open-access journal that publishes significant articles featuring extensive data or calculations in the field of astrophysics. It also facilitates Special Issues, presenting thematically related papers simultaneously in a single volume.
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