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| CXOU J100047.6+013940 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST18:36:01 |
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| 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 |
|---|---|---|---|---|---|---|---|---|---|
2011ApJ...742..125G 
|
15 | D | 1 | 3590 | 124 | Galaxies in X-ray groups. I. Robust membership assignment and the impact of group environments on quenching. | GEORGE M.R., LEAUTHAUD A., BUNDY K., et al. | ||
| 2012ApJ...758...47A | 15 | D | 1 | 112 | 41 | Occupation of x-ray-selected galaxy groups by X-ray active galactic nuclei. | ALLEVATO V., FINOGUENOV A., HASINGER G., et al. | ||
| 2013ApJ...778...74K | 16 | D | 2 | 11 | 22 | Weak lensing calibrated M-T scaling relation of galaxy groups in the COSMOS field{sstarf}. | KETTULA K., FINOGUENOV A., MASSEY R., et al. | ||
|
2015MNRAS.450.3665S
|
16 | D | 1 | 430 | 35 | CoMaLit - III. Literature catalogues of weak lensing clusters of galaxies (LC2). | SERENO M. | ||
|
2016ApJS..224....1R
|
16 | D | 1 | 670875 | 246 | The redMaPPer galaxy cluster catalog from DES science verification data. | RYKOFF E.S., ROZO E., HOLLOWOOD D., et al. | ||
| 2018ApJ...857..122C | 16 | D | 1 | 45 | 3 | Stellar mass and 3.4 µm M/L ratio evolution of brightest cluster galaxies in COSMOS since z ∼ 1.0. | COOKE K.C., FOGARTY K., KARTALTEPE J.S., et al. | ||
| 2019MNRAS.488....1Z | 16 | D | 1 | 93 | ~ | Galaxies in X-ray selected clusters and groups in Dark Energy Survey data - II. Hierarchical Bayesian modelling of the red-sequence galaxy luminosity function. | ZHANG Y., MILLER C.J., ROONEY P., et al. | ||
|
2020MNRAS.497.2163P
|
16 | D | 1 | 173 | ~ | The relation between the diffuse X-ray luminosity and the radio power of the central AGN in galaxy groups. | PASINI T., BRUGGEN M., DE GASPERIN F., et al. | ||
| 2021MNRAS.502.2419F | 18 | D | 3 | 19 | 27 | The growth of intracluster light in XCS-HSC galaxy clusters from 0.1 < z < 0.5. | FURNELL K.E., COLLINS C.A., KELVIN L.S., et al. |
