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| 1RXS J231839.4+425745 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST05:45:33 |
Sort references on where and how often the object is cited
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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 |
|---|---|---|---|---|---|---|---|---|---|
2000ApJS..129..547B 
|
14 | D | 1 | 1633 | 94 | RBSC-NVSS sample. I. Radio and optical identifications of a complete sample of 1556 bright X-ray sources. | BAUER F.E., CONDON J.J., THUAN T.X., et al. | ||
|
2002ApJ...580..774E
|
88 | 129 | A systematic X-ray search for clusters of galaxies behind the Milky Way. | EBELING H., MULLIS C.R. and TULLY R.B. | |||||
|
2009ApJS..182...12C
|
15 | D | 1 | 277 | 460 | Intracluster medium entropy profiles for a Chandra archival sample of galaxy clusters. | CAVAGNOLO K.W., DONAHUE M., VOIT G.M., et al. | ||
|
2009ApJS..184..138H
|
15 | D | 1 | 20666 | 68 | XID II: statistical cross-association of ROSAT bright source catalog X-ray sources with 2MASS point source catalog near-infrared sources. | HAAKONSEN C.B. and RUTLEDGE R.E. | ||
|
2009ApJ...704.1586S
|
15 | D | 1 | 259 | 141 | Every BCG with a strong radio AGN has an X-ray cool core: is the cool core-noncool core dichotomy too simple? | SUN M. | ||
|
2011A&A...534A.109P
|
15 | D | 1 | 1770 | 422 | The MCXC: a meta-catalogue of X-ray detected clusters of galaxies. | PIFFARETTI R., ARNAUD M., PRATT G.W., et al. | ||
|
2012MNRAS.425..477N
|
15 | D | 1 | 1763 | 27 | γ-rays from annihilating dark matter in galaxy clusters: stacking versus single source analysis. | NEZRI E., WHITE R., COMBET C., et al. | ||
|
2017MNRAS.468.3322S
|
16 | D | 1 | 28168 | 37 | CoMaLit - V. Mass forecasting with proxies: method and application to weak lensing calibrated samples. | SERENO M. and ETTORI S. | ||
|
2021A&A...656A.144B
|
235 | D | X C | 5 | 111 | ~ | The Cosmic Large-Scale Structure in X-rays (CLASSIX) Cluster Survey. IV. Superclusters in the local Universe at z ≤ 0.03. | BOHRINGER H. and CHON G. |
