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| XLSSC 032 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST03:47:04 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| 2005MNRAS.359.1250A | 1 | 11 | 36 | Batch discovery of nine z∼ 1 clusters using X-ray and K or R, z' images. | ANDREON S., VALTCHANOV I., JONES L.R., et al. | ||||
| 2010ApJ...718...23S | 92 | D | F | 1 | 20 | 94 | The XMM cluster survey: the build-up of stellar mass in brightest cluster galaxies at high redshift. | STOTT J.P., COLLINS C.A., SAHLEN M., et al. | |
| 2012MNRAS.425.2058B | 171 | D | C F | 5 | 7 | 43 | Measurement of the intracluster light at z ∼ 1. | BURKE C., COLLINS C.A., STOTT J.P., et al. | |
| 2012MNRAS.427..550L | 15 | D | 1 | 150 | 160 | Evidence for significant growth in the stellar mass of brightest cluster galaxies over the past 10 billion years. | LIDMAN C., SUHERLI J., MUZZIN A., et al. | ||
| 2013MNRAS.430..134W | 15 | D | 2 | 73 | 32 | Distant galaxy clusters in the XMM Large Scale Structure survey. | WILLIS J.P., CLERC N., BREMER M.N., et al. | ||
| 2018MNRAS.477.5517W | 16 | D | 1 | 19 | 1 | X-ray versus infrared selection of distant galaxy clusters: a case study using the XMM-LSS and SpARCS cluster samples. | WILLIS J.P., RAMOS-CEJA M.E., MUZZIN A., et al. | ||
| 2018A&A...620A...5A | 16 | D | 1 | 381 | 77 | The XXL Survey. XX. The 365 cluster catalogue. | ADAMI C., GILES P., KOULOURIDIS E., et al. | ||
2020ApJ...890..148U 
|
16 | D | 2 | 137 | 50 | Weak-lensing analysis of X-ray-selected XXL galaxy groups and clusters with Subaru HSC data. | UMETSU K., SERENO M., LIEU M., et al. | ||
|
2021ApJ...911...82C
|
17 | D | 1 | 388 | ~ | Cosmological constraints from galaxy cluster sparsity, cluster gas mass fraction, and baryon acoustic oscillation data. | CORASANITI P.-S., SERENO M. and ETTORI S. |
