2MASS J20582990-4236343 , the SIMBAD biblio

2MASS J20582990-4236343 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST00:00:24


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Title First 3 Authors
2004A&A...416..901C         O           30 75 The XMM-Newton HBS28 sample: Studying the obscuration in hard X-ray selected AGNs. CACCIANIGA A., SEVERGNINI P., BRAITO V., et al.
2004A&A...428..383D viz 15       D               402 114 Exploring the X-ray sky with the XMM-Newton Bright Serendipitous Survey. DELLA CECA R., MACCACARO T., CACCIANIGA A., et al.
2006A&A...455..773V viz 108224 628 A catalogue of quasars and active nuclei: 12th edition. VERON-CETTY M.-P. and VERON P.
2008A&A...477..735C 15       D               1 350 36 The XMM-Newton bright serendipitous survey. Identification and optical spectral properties. CACCIANIGA A., SEVERGNINI P., DELLA CECA R., et al.
2010A&A...518A..10V viz 15       D               1 168913 597 A catalogue of quasars and active nuclei: 13th edition. VERON-CETTY M.-P. and VERON P.
2011A&A...530A..42C viz 15       D               1 305 76 The X-ray spectral properties of the AGN population in the XMM-Newton bright serendipitous survey. CORRAL A., DELLA CECA R., CACCIANIGA A., et al.
2012A&A...539A..48M viz 93       D         F     2 202 33 The optical-UV spectral energy distribution of the unabsorbed AGN population in the XMM-Newton Bright Serendipitous Survey. MARCHESE E., DELLA CECA R., CACCIANIGA A., et al.
2013A&A...549A.119C viz 16       D               1 154 4 Black-hole masses of type 1 AGN in the XMM-Newton bright serendipitous survey. CACCIANIGA A., FANALI R., SEVERGNINI P., et al.
2015MNRAS.447..517L 16       D               1 58 17 Relativistic Fe Kα line revealed in the composite X-ray spectrum of narrow-line Seyfert 1 galaxies - do their black holes have averagely low or intermediate spins? LIU Z., YUAN W., LU Y., et al.
2017ApJ...836...99L viz 16       D               1 518 50 The NuSTAR serendipitous survey: the 40-month catalog and the properties of the distant high-energy X-ray source population. LANSBURY G.B., STERN D., AIRD J., et al.

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