Deep Hard X-ray Survey of the M81 Field Based on INTEGRAL1 Data

IF 1.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Astronomy Letters-A Journal of Astronomy and Space Astrophysics Pub Date : 2024-05-13 DOI:10.1134/S1063773724600115
R. A. Krivonos, I. A. Mereminskiy, S. Yu. Sazonov
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Abstract

We have carried out a deep survey of the M81 field in the 25–60 keV energy band based on long-term (2003–2023) INTEGRAL observations. A record sensitivity of 0.16 mCrab at a detection significance of \(4\sigma\) has been achieved in the central part of the field owing to the long accumulated exposure (19.2 Ms). The total area of the survey is 1004 deg\({}^{2}\) at a sensitivity level better than 0.72 mCrab. We have produced a catalog of sources detected at a significance level higher than \(4\sigma\). It contains 51 objects most of which are active galactic nuclei (AGNs). The median redshift of the Seyfert galaxies in the catalog is \(z=0.0366\). Six sources have not been detected previously in any of the X-ray surveys. According to the available indirect data, all of them and two more sources that have already been entered previously into the INTEGRAL survey catalogs can also be AGNs, including those with strong internal absorption.

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基于 INTEGRAL1 数据的 M81 场深层硬 X 射线巡天观测
摘要 我们在 INTEGRAL 长期(2003-2023 年)观测的基础上,对 M81 场的 25-60 keV 能段进行了一次深入的巡天观测。由于累积曝光时间较长(19.2 Ms),我们在该星域的中央部分实现了创纪录的0.16 mCrab灵敏度,探测意义为\(4\sigma\)。巡天的总面积为 1004 deg\({}^{2}\) ,灵敏度优于 0.72 mCrab。我们已经制作了一份以高于\(4\sigma\)的显著性水平探测到的源星表。它包含了51个天体,其中大部分是活动星系核(AGN)。星表中塞弗特星系的中位红移是\(z=0.0366\)。有六个源以前没有在任何X射线巡天中被探测到过。根据现有的间接数据,所有这些源和另外两个已经进入INTEGRAL巡天目录的源也可能是AGN,包括那些具有强烈内部吸收的源。
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来源期刊
CiteScore
1.70
自引率
22.20%
发文量
0
审稿时长
6-12 weeks
期刊介绍: Astronomy Letters is an international peer reviewed journal that publishes the results of original research on all aspects of modern astronomy and astrophysics including high energy astrophysics, cosmology, space astronomy, theoretical astrophysics, radio astronomy, extragalactic astronomy, stellar astronomy, and investigation of the Solar system.
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