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| SDSSCGB 31502.1 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST22:10:47 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2009MNRAS.395..255M |
15 | D | 1 | 397037 | 82 | Compact groups in theory and practice - III. Compact groups of galaxies in the sixth data release of the Sloan Digital Sky Survey. | McCONNACHIE A.W., PATTON D.R., ELLISON S.L., et al. | ||
|
2010ApJS..191..254H |
15 | D | 1 | 20101 | 235 | A GMBCG galaxy cluster catalog of 55,424 rich clusters from SDSS DR7. | HAO J., McKAY T.A., KOESTER B.P., et al. | ||
|
2012MNRAS.423..422L |
15 | D | 1 | 128 | 36 | Star formation activities in early-type brightest cluster galaxies. | LIU F.S., MAO S. and MENG X.M. | ||
|
2012ApJS..201...31G |
15 | D | 1 | 15563 | 75 | Double-peaked narrow emission-line galaxies from the Sloan Digital Sky Survey. I. Sample and basic properties. | GE J.-Q., HU C., WANG J.-M., et al. | ||
|
2014ApJ...788...45T |
15 | D | 1 | 224166 | 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 | 209271 | 41 | Aperture-free star formation rate of SDSS star-forming galaxies. | DUARTE PUERTAS S., VILCHEZ J.M., IGLESIAS-PARAMO J., et al. | ||
|
2018ApJ...853...47R |
16 | D | 1 | 162 | 3 | "red" but not "dead": actively star-forming brightest cluster galaxies at low redshifts. | RUNGE J. and YAN H. | ||
|
2020ApJS..247...53K |
16 | D | 1 | 23378 | 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 |
17 | D | 1 | 194359 | 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. |