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| FIRST J082407.9+472037 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST16:14:34 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
1995A&AS..110..313F 
|
1177 | 17 | Properties of nearby clusters of galaxies. II. A 151, A 637, A 646, A 649, A 655, A 1132, A 1314, A 1377, A 1570, A 1589. | FLIN P., TREVESE D., CIRIMELE G., et al. | |||||
|
2003A&A...412...45P
|
15 | D | 1 | 956205 | 750 | HYPERLEDA. I. Identification and designation of galaxies. | PATUREL G., PETIT C., PRUGNIEL P., et al. | ||
|
2005MNRAS.362....9B
|
15 | D | 2707 | 245 | A sample of radio-loud active galactic nuclei in the Sloan Digital Sky Survey. | BEST P.N., KAUFFMANN G., HECKMAN T.M., et al. | |||
|
2013ApJ...767...15R
|
16 | D | 1 | 25361 | 168 | Measuring the ultimate halo mass of galaxy clusters: redshifts and mass profiles from the Hectospec Cluster Survey (HeCS). | RINES K., GELLER M.J., DIAFERIO A., et al. | ||
|
2014ApJ...788...45T
|
16 | D | 1 | 224162 | 54 | Luminosity and redshift dependence of the covering factor of active galactic nuclei viewed with WISE and Sloan Digital Sky Survey. | TOBA Y., OYABU S., MATSUHARA H., et al. | ||
|
2017A&A...599A..71D
|
16 | D | 1 | 209270 | 41 | Aperture-free star formation rate of SDSS star-forming galaxies. | DUARTE PUERTAS S., VILCHEZ J.M., IGLESIAS-PARAMO J., et al. | ||
|
2018ApJS..237...14O
|
16 | D | 1 | 1423 | 5 | KYDISC: galaxy morphology, quenching, and mergers in the cluster environment. | OH S., KIM K., LEE J.H., et al. | ||
|
2020ApJS..247...53K
|
17 | D | 1 | 23374 | 20 | Radio sources associated with Optical Galaxies and having Unresolved or Extended morphologies (ROGUE). I. A catalog of SDSS galaxies with FIRST core identifications. | KOZIEL-WIERZBOWSKA D., GOYAL A. and ZYWUCKA N. | ||
|
2022A&A...666A.186D
|
18 | D | 1 | 194358 | 6 | Mass-metallicity and star formation rate in galaxies: A complex relation tuned to stellar age. | DUARTE PUERTAS S., VILCHEZ J.M., IGLESIAS-PARAMO J., et al. |
