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| [BGM2013] BHC 17 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST03:59:58 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
| 1991ApJ...382...82T | 117 | 116 | The discrete X-ray source population in M 31. | TRINCHIERI G. and FABBIANO G. | |||||
| 1993ApJ...410..615P | 137 | 118 | High-resolution X-ray observations of the central region of M31 with the ROSAT satellite. | PRIMINI F.A., FORMAN W. and JONES C. | |||||
2002ApJ...577..738K 
|
209 | 126 | X-ray point sources in the central region of M31 as seen by Chandra. | KONG A.K.H., GARCIA M.R., PRIMINI F.A., et al. | |||||
|
2002ApJ...578..114K
|
148 | 76 | A Chandra high resolution camera observation of X-ray point sources in M31. | KAARET P. | |||||
|
2005A&A...434..483P
|
915 | 86 | An XMM-Newton survey of M 31. | PIETSCH W., FREYBERG M. and HABERL F. | |||||
|
2008A&A...480..599S
|
15 | D | 317 | 21 | Time variability of X-ray sources in the M 31 centre field. | STIELE H., PIETSCH W., HABERL F., et al. | |||
| 2010A&A...523A..89H | 15 | D | 1 | 58 | 36 | X-ray monitoring of classical novae in the central region of M 31. I. June 2006-March 2007. | HENZE M., PIETSCH W., HABERL F., et al. | ||
|
2011A&A...534A..55S
|
15 | D | 1 | 2367 | 70 | The deep XMM-Newton survey of M 31. | STIELE H., PIETSCH W., HABERL F., et al. | ||
| 2013ApJ...770..148B | 16 | D | 1 | 58 | 12 | Chandra identification of 26 new black hole candidates in the central region of M31. | BARNARD R., GARCIA M.R. and MURRAY S.S. | ||
|
2013A&A...555A..65H
|
16 | D | 1 | 335 | 16 | X-ray source variability study of the M 31 central field using Chandra HRC-I. | HOFMANN F., PIETSCH W., HENZE M., et al. | ||
| 2014ApJ...791...33B | 16 | D | 4 | 72 | 9 | Fifty M31 black hole candidates identified by Chandra and XMM-Newton. | BARNARD R., GARCIA M.R., PRIMINI F., et al. |
