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The XMM-Newton serendipitous survey - IV. Optical identification of the XMM-Newton medium sensitivity survey (XMS)
Barcons, X.; Carrera, F. J.; Ceballos, M. T.; Page, M. J.; Bussons-Gordo, J.; Corral, A.; Ebrero, J.; Mateos, S.; Tedds, J. A.; Watson, M. G.; Baskill, D.; Birkinshaw, M.; Boller, T.; Borisov, N.; Bremer, M.; Bromage, G. E.; Brunner, H.; Caccianiga, A.; Crawford, C. S.; Cropper, M. S.; Della Ceca, R.; Derry, P.; Fabian, A. C.; Guillout, P.; Hashimoto, Y.; Hasinger, G.; Hassall, B. J. M.; Lamer, G.; Loaring, N. S.; Maccacaro, T.; Mason, K. O.; McMahon, R. G.; Mirioni, L.; Mittaz, J. P. D.; Motch, C.; Negueruela, I.; Osborne, J. P.; Panessa, F.; Perez-Fournon, I.; Pye, J. P.; Roberts, T. P.; Rosen, S.; Schartel, N.; Schurch, N.; Schwope, A.; Severgnini, P.; Sharp, R.; Stewart, G. C.; Szokoly, G.; Ullan, A.; Ward, M. J.; Warwick, R. S.; Wheatley, P. J.; Webb, N. A.; Worrall, D.; Yuan, W.; Ziaeepour, H.
2007-12-01
Source PublicationASTRONOMY & ASTROPHYSICS
Volume476Issue:3Pages:1191-U35
AbstractAims. X-ray sources at intermediate fluxes (a few x 10(-14) erg cm(-2) s(-1)) with a sky density of similar to 100 deg(-2) are responsible for a significant fraction of the cosmic X-ray background at various energies below 10 keV. The aim of this paper is to provide an unbiased and quantitative description of the X-ray source population at these fluxes and in various X-ray energy bands.
KeywordX-rays : General X-rays : Galaxies X-rays : Stars Galaxies : Active
DOI10.1051/0004-6361:20077606
Indexed BySCI
Language英语
WOS IDWOS:000251507500014
Citation statistics
Cited Times:39[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8969
Collection空间科学研究部
Affiliation1.CSIC UC, Inst Fis Cantabria, Santander 39005, Spain
2.UCL, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England
3.Univ Leicester, Dept Phys & Astron, X Ray & Observ Astron Grp, Leicester LE1 7RH, Leics, England
4.Univ Bristol, HH Wills Phys Lab, Bristol BS8 1TL, Avon, England
5.Max Planck Inst Extraterr Phys, D-85740 Garching, Germany
6.Special Astrophys Observ, Nizhnii Arkhyz 369167, Russia
7.Univ Cent Lancashire, Ctr Astrophys, Preston PR1 2HE, Lancs, England
8.Osserv Astron Brera, INAF, I-20121 Milan, Italy
9.Astron Inst, Cambridge CB3 0HA, England
10.Observ Astron, F-67000 Strasbourg, France
11.Astrophys Inst Potsdam, D-144482 Potsdam, Germany
12.S African Large Telescope, ZA-7935 Cape Town, South Africa
13.Univ Alicante, Dept Fis Ingn Sist & Teor Senal, Alicante 03080, Spain
14.Inst Astrofis Canarias, San Cristobal la Laguna 0308200, Spain
15.Univ Durham, Dept Phys, Durham DH1 3LE, England
16.European Space Astron Ctr, Madrid 50727, Spain
17.Anglo Australian Observ, Epping, NSW 1710, Australia
18.CSIC, INTA, Ctr Astrobiol, Madrid 28080, Spain
19.Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England
20.Ctr Etud Spatiale Rayonnements, CNRS, UPS, F-31028 Toulouse, France
21.Natl Astron Observ China, Yunnan Observ, Kunming, Peoples R China
Recommended Citation
GB/T 7714
Barcons, X.,Carrera, F. J.,Ceballos, M. T.,et al. The XMM-Newton serendipitous survey - IV. Optical identification of the XMM-Newton medium sensitivity survey (XMS)[J]. ASTRONOMY & ASTROPHYSICS,2007,476(3):1191-U35.
APA Barcons, X..,Carrera, F. J..,Ceballos, M. T..,Page, M. J..,Bussons-Gordo, J..,...&Ziaeepour, H..(2007).The XMM-Newton serendipitous survey - IV. Optical identification of the XMM-Newton medium sensitivity survey (XMS).ASTRONOMY & ASTROPHYSICS,476(3),1191-U35.
MLA Barcons, X.,et al."The XMM-Newton serendipitous survey - IV. Optical identification of the XMM-Newton medium sensitivity survey (XMS)".ASTRONOMY & ASTROPHYSICS 476.3(2007):1191-U35.
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