Resolving the hard X-ray background in the Chandra Deep Field South

被引：0

作者：

Gilli, R ^{[1
]}

Giacconi, R ^{[1
]}

Tozzi, P ^{[1
]}

Rosati, P ^{[1
]}

Hasinger, G ^{[1
]}

Kewley, L ^{[1
]}

Wang, JX ^{[1
]}

Zirm, A ^{[1
]}

Mainieri, V ^{[1
]}

Borgani, S ^{[1
]}

Bergeron, J ^{[1
]}

Gilmozzi, R ^{[1
]}

Schreier, E ^{[1
]}

Koekemoer, A ^{[1
]}

Grogin, N ^{[1
]}

Nonino, M ^{[1
]}

Norman, C ^{[1
]}

机构：

[1] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA

来源：

LIGHTHOUSES OF THE UNIVERSE: THE MOST LUMINOUS CELESTIAL OBJECTS AND THEIR USE FOR COSMOLOGY | 2002年

关键词：

D O I：

10.1007/10856495_90

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The 1Msec observation of the Chandra Deep Field South (CDFS) has almost entirely resolved into single sources the hard X-ray background as measured by the HEAO-1 A2 experiment. The main population of sources, as determined by the first optical identifications, seems to be constituted by an admixture of type 1 and type 2 AGNs. We will consider the X-ray properties of the sources in the CDFS and test their consistency with the predictions from the AGN synthesis models of the X-ray background. An apparent excess of sources at z < 0.8 is found with respect to the model predictions. The X-ray background flux produced by these sources is also exceeding the predictions, suggesting that the bulk of the XRB is produced closer than expected.

引用

页码：573 / 579

页数：7

共 50 条

[31] Chandra spectra of the soft X-ray diffuse background
Markevitch, M
Bautz, MW
Biller, B
Butt, Y
Edgar, R
Gaetz, T
Garmire, G
Grant, CE
Green, P
Juda, M
Plucinsky, PP
Schwartz, D
Smith, R
Vikhlinin, A
Virani, S
Wargelin, BJ
Wolk, S
ASTROPHYSICAL JOURNAL, 2003, 583 (01): : 70 - 84
[32] Chandra probes deeper into the mystery of the x-ray background
Day, C
PHYSICS TODAY, 2000, 53 (05) : 18 - 20
[33] Chandra Probes Deeper into the Mystery of the X-Ray Background
2000, American Institute of Physics Inc. (53)
[34] The X-ray background and the deep X-ray surveys
Gilli, R
NEW X-RAY RESULTS, THE NEXT GENERATION OF X-RAY OBSERVATORIES AND GAMMA RAY BURST AFTERGLOW PHYSICS, 2004, 34 (12): : 2470 - 2477
[35] On the origin of the hard X-ray background
Di Matteo, T
Esin, A
Fabian, AC
Narayan, R
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1999, 305 (01) : L1 - L5
[36] The sources of the hard X-ray background
Setti, G
Comastri, A
EXAMINING THE BIG BANG AND DIFFUSE BACKGROUND RADIATIONS, 1996, (168): : 263 - 270
[37] AGN predictions for the Hubble Deep Field and the X-ray background
Almaini, O
Fabian, AC
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1997, 288 (01) : L19 - L22
[38] AGNs in deep X-ray surveys and the X-ray background
Gilli, R
DEEP FIELDS, 2001, : 297 - 297
[39] SPATIALLY RESOLVING A STARBURST GALAXY AT HARD X-RAY ENERGIES: NuSTAR, CHANDRA, AND VLBA OBSERVATIONS OF NGC 253
Wik, D. R.
Lehmer, B. D.
Hornschemeier, A. E.
Yukita, M.
Ptak, A.
Zezas, A.
Antoniou, V.
Argo, M. K.
Bechtol, K.
Boggs, S.
Christensen, F.
Craig, W.
Hailey, C.
Harrison, F.
Krivonos, R.
Maccarone, T. J.
Stern, D.
Venters, T.
Zhang, W. W.
ASTROPHYSICAL JOURNAL, 2014, 797 (02):
[40] Seyfert galaxies and the hard X-ray background:: Artificial Chandra observations of z=0.3 active galaxies
Peterson, KC
Gallagher, SC
Hornschemeier, AE
Muno, MP
Bullard, EC
ASTRONOMICAL JOURNAL, 2006, 131 (01): : 133 - 142

← 1 2 3 4 5 →