Radio observations of the XMM-Newton/Chandra 13hr deep survey field

被引：5
|
作者：
Gunn, KF [1 ]
McHardy, IM
Seymour, N
Newsam, AM
Page, MJ
Mason, KO
Loaring, N
Jones, LR
Muxlow, T
Takata, T
Sekiguchi, K
Sasseen, T
机构：
[1] Univ Southampton, Dept Phys & Astron, Southampton SO17 1BJ, Hants, England
[2] Liverpool John Moores Univ, Astrophys Res Inst, Birkenhead CH41 1LD, Merseyside, England
[3] UCL, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England
[4] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England
[5] Univ Manchester, Nuffield Radio Astron Labs, Macclesfield SK11 9DL, Cheshire, England
[6] Natl Astron Observ Japan, Hilo, HI 96720 USA
[7] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA
来源：
ASTRONOMISCHE NACHRICHTEN | 2003年 / 324卷 / 1-2期
关键词：
surveys; X-rays; radio continuum; galaxies : active;
D O I：
10.1002/asna.200310027
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Our VLA observations of the XMM-Newton/Chandra 13hr deep survey field (see Page et al., this proceedings) result in one of the two deepest 1.4GHz radio maps ever made. Within the 15' radius field covered by the deep X-ray data (0.19 deg(2)), a total of 556 radio sources are detected, down to a 4sigma flux limit of 28muJy. Of the 214 Chandra sources, 55 have radio counterparts. The sub-arcsecond accuracy of the VLA and Chandra positions enable us to determine with high confidence the sources common to both surveys. Here we present the relationship between the X-ray and radio source populations at the faintest radio flux limits yet probed by such a study, We discuss how the X-ray/radio relationship differs as a function of optical morphology. ie between unresolved 'stellar' objects and well resolved galaxies. We then discuss the origin of the X-ray and radio emission. ie AGN, starburst or a mixture of both, in these two classes of object.
引用
收藏
页码：105 / 108
页数：4
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