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ClG J1419+5326 , the SIMBAD biblio (21 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST12:33:44 |
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 |
---|---|---|---|---|---|---|---|---|---|
2003ApJ...593...48G | 4 | 9 | 113 | The incidence of strong-lensing clusters in the Red-sequence Cluster Survey. | GLADDERS M.D., HOEKSTRA H., YEE H.K.C., et al. | ||||
2007A&A...461..813C | 1 | 46 | 151 | The CFHTLS strong lensing legacy survey. I. Survey overview and T0002 release sample. | CABANAC R.A., ALARD C., DANTEL-FORT M., et al. | ||||
2007ApJ...654..714H | 12 | 7 | 171 | Characterizing the cluster lens population. | HENNAWI J.F., DALAL N., BODE P., et al. | ||||
2007A&A...462..429B | O | 67 | 128 | Tracing the evolution in the iron content of the intra-cluster medium. | BALESTRA I., TOZZI P., ETTORI S., et al. | ||||
2008A&A...483...35S | 55 | D | X | 2 | 38 | 177 | Searching for cool core clusters at high redshift. | SANTOS J.S., ROSATI P., TOZZI P., et al. | |
2008ApJ...680.1022H | 355 | D | X | 10 | 13 | 44 | Chandra X-ray observations of the 0.6 < z < 1.1 red-sequence cluster survey sample. | HICKS A.K., ELLINGSON E., BAUTZ M., et al. | |
2008A&A...489..967B | 542 | D | X C | 14 | 12 | 11 | Intra cluster medium properties and AGN distribution in high-z RCS clusters. | BIGNAMINI A., TOZZI P., BORGANI S., et al. | |
2009A&A...501...61E | 16 | D | 1 | 60 | 165 | The cluster gas mass fraction as a cosmological probe: a revised study. | ETTORI S., MORANDI A., TOZZI P., et al. | ||
2010MNRAS.406.1318H | 15 | D | 1 | 91 | 29 | The lensing efficiencies of MACS X-ray-selected versus RCS optically selected galaxy clusters. | HORESH A., MAOZ D., EBELING H., et al. | ||
2011A&A...535A...4R | 15 | D | 2 | 225 | 108 | Observational constraints on the redshift evolution of X-ray scaling relations of galaxy clusters out to z ∼ 1.5. | REICHERT A., BOEHRINGER H., FASSBENDER R., et al. | ||
2012MNRAS.419.1983N | 596 | D | X C F | 14 | 15 | 9 | Submillimetre source counts in the fields of high-redshift galaxy clusters. | NOBLE A.G., WEBB T.M.A., ELLINGSON E., et al. | |
2012ApJ...749...38M | 116 | X C | 2 | 261 | 120 | The CFHTLS-Strong Lensing Legacy Survey (SL2S): investigating the group-scale lenses with the SARCS sample. | MORE A., CABANAC R., MORE S., et al. | ||
2011RAA....11.1185W | 15 | D | 1 | 39 | 13 | Lensing clusters of galaxies in the SDSS-III. | WEN Z.-L., HAN J.-L. and JIANG Y.-Y. | ||
2013MNRAS.432...62E | 601 | D | X C F | 14 | 183 | 12 | X-ray selected galaxy clusters in the Pan-STARRS Medium Deep Survey. | EBELING H., EDGE A.C., BURGETT W.S., et al. | |
2013AJ....146...84W | 16 | D | 1 | 43 | 33 | The evolution of dusty star formation in galaxy clusters to z = 1: Spitzer infrared observations of the first Red-Sequence Cluster Survey. | WEBB T.M.A., O'DONNELL D., YEE H.K.C., et al. | ||
2014ApJ...788..109J | 159 | X C | 3 | 3 | 17 | Probability Friends-of-Friends (PFOF) group finder: performance study and observational data applications on photometric surveys. | JIAN H.-Y., LIN L., CHIUEH T., et al. | ||
2014ApJ...789..134B | 16 | D | 5 | 82 | 11 | The inside-out growth of the most massive galaxies at 0.3 < z < 0.9. | BAI L., YEE H.K.C., YAN R., et al. | ||
2014ARep...58..587B | 16 | D | 1 | 137 | 42 | Chandra X-ray galaxy clusters at z < 1.4: Constraints on the inner slope of the density profiles. | BABYK Y.V., DEL POPOLO A. and VAVILOVA I.B. | ||
2016MNRAS.455..892G | 16 | D | 1 | 353 | 14 | The galaxy cluster concentration-mass scaling relation. | GROENER A.M., GOLDBERG D.M. and SERENO M. | ||
2018ApJ...859...65Y | 16 | D | 2 | 23 | 15 | X-ray properties of AGN in brightest cluster galaxies. I. A systematic study of the Chandra archive in the 0.2 < z < 0.3 and 0.55 < z < 0.75 redshift range. | YANG L., TOZZI P., YU H., et al. | ||
2021A&A...649A..42C | 17 | D | 1 | 141 | 14 | Physical properties of brightest cluster galaxies up to redshift 1.80 based on HST data. | CHU A., DURRET F. and MARQUEZ I. |