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ClG J2038-0125 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST16:27:16 |
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 |
---|---|---|---|---|---|---|---|---|---|
2002ApJS..140..265P | 295 | 90 | The WARPS survey. VI. Galaxy cluster and source identifications from phase I. | PERLMAN E.S., HORNER D.J., JONES L.R., et al. | |||||
2003MNRAS.341.1093B | 97 | 27 | The Southern SHARC catalogue: a ROSAT survey for distant galaxy clusters. | BURKE D.J., COLLINS C.A., SHARPLES R.M., et al. | |||||
2004A&A...424.1097S | 15 | D | 1 | 1674 | 24 | Introducing BAX: A database for X-ray clusters and groups of galaxies. | SADAT R., BLANCHARD A., KNEIB J.-P., et al. | ||
2007AJ....133.2209D | 30 | 36 | The rest-frame K-band luminosity function of galaxies in clusters to z = 1.3. | DE PROPRIS R., STANFORD S.A., EISENHARDT P.R., et al. | |||||
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.423.3561C | 15 | D | 1 | 424 | 44 | The cosmological analysis of X-ray cluster surveys – II. Application of the CR–HR method to the XMM archive. | CLERC N., SADIBEKOVA T., PIERRE M., 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. | ||
2018ApJ...867...12R | 16 | D | 1 | 113 | 3 | Mass-richness relations for X-ray and SZE-selected clusters at 0.4 < z < 2.0 as seen by Spitzer at 4.5 µm. | RETTURA A., CHARY R., KRICK J., et al. | ||
2021A&A...652A..12K | 17 | D | 1 | 1564 | 14 | The X-CLASS survey: A catalogue of 1646 X-ray-selected galaxy clusters up to z ∼ 1.5. | KOULOURIDIS E., CLERC N., SADIBEKOVA T., et al. |