ASCA observations of deep ROSAT fields - III. The discovery of an obscured Type 2 AGN at z=0.67

被引:17
作者
Boyle, BJ
Almaini, O
Georgantopoulos, I
Blair, AJ
Stewart, GC
Griffiths, RE
Shanks, T
Gunn, KF
机构
[1] Anglo Australian Observ, Epping, NSW 2121, Australia
[2] Univ Edinburgh, Inst Astron, Edinburgh EH9 3HJ, Midlothian, Scotland
[3] Natl Observ Athens, GR-15236 Athens, Greece
[4] Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England
[5] Carnegie Mellon Univ, Dept Phys, Pittsburgh, PA 15213 USA
[6] Univ Durham, Dept Phys, Durham DH1 3LE, England
关键词
galaxies; active; individual; AXJ0341.4-4453; quasars; general; X-rays;
D O I
10.1046/j.1365-8711.1998.01709.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report on the discovery of a narrow-emission-line object at z = 0.672 detected in a deep ASCA survey. The object, AXJ0341.4-4453, has a flux in the 2-10 keV band of 1.1 +/- 0.27 x 10(-13) erg s(-1) cm(-2), corresponding to a luminosity of 1.8 x 10(44) erg s(-1) (q(0) = 0.5, H-0 = 50 km s(-1) Mpc(-1)). It is also marginally detected in the ROSAT 0.5-2 keV band with a flux 5.8 x 10(-15) erg s(-1) cm(-2). Both the ASCA data alone and the combined ROSAT/ASCA data show a very hard X-ray spectrum, consistent with either a flat power law (alpha < 0.1) or photoelectric absorption with a column of n(H) > 4 x 10(22) cm(-2) (alpha = 1). The optical spectrum shows the high-ionization, narrow emission lines typical of a Seyfert 2 galaxy. We suggest that this object may be typical of the hard sources required to explain the remainder of the X-ray background at hard energies.
引用
收藏
页码:L53 / L56
页数:4
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