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| LEDA 1600415 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST08:34:58 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
| 1985ApJS...57..665B | 1432 | 62 | The evolution of galaxies in clusters. IV. Photometry of 10 low-redshift clusters. | BUTCHER H.R. and OEMLER A. | |||||
2003A&A...412...45P 
|
15 | D | 1 | 956205 | 750 | HYPERLEDA. I. Identification and designation of galaxies. | PATUREL G., PETIT C., PRUGNIEL P., et al. | ||
|
2010MNRAS.404.1745M
|
15 | D | 1 | 314 | 42 | Star formation, starbursts and quenching across the Coma supercluster. | MAHAJAN S., HAINES C.P. and RAYCHAUDHURY S. | ||
|
2015ApJ...812...89M
|
16 | D | 1 | 12670 | 7 | ECO and RESOLVE: galaxy disk growth in environmental context. | MOFFETT A.J., KANNAPPAN S.J., BERLIND A.A., et al. | ||
|
2017A&A...597A.134M
|
16 | D | 1 | 2666 | 17 | A large sample of Kohonen selected E+A (post-starburst) galaxies from the Sloan Digital Sky Survey. | MEUSINGER H., BRUNECKE J., SCHALLDACH P., et al. | ||
|
2017ApJ...849...20E
|
16 | D | 1 | 9926 | 2 | The baryonic collapse efficiency of galaxy groups in the RESOLVE and ECO surveys. | ECKERT K.D., KANNAPPAN S.J., LAGOS C.D.P., et al. | ||
|
2018ApJ...862....2F
|
16 | D | 1 | 1165 | 51 | Clocking the evolution of post-starburst galaxies: methods and first results. | FRENCH K.D., YANG Y., ZABLUDOFF A.I., et al. | ||
|
2018MNRAS.478.4336M
|
16 | D | 1 | 4285 | 3 | Ultraviolet and optical view of galaxies in the Coma supercluster. | MAHAJAN S., SINGH A. and SHOBHANA D. | ||
|
2020ApJS..246....2A
|
17 | D | 1 | 36251 | ~ | GalWeight application: a publicly available catalog of dynamical parameters of 1800 galaxy clusters from SDSS-DR13, (GalWCat19). | ABDULLAH M.H., WILSON G., KLYPIN A., et al. | ||
|
2020MNRAS.494.1784A
|
17 | D | 1 | 47437 | 9 | Local AGN survey (LASr): I. Galaxy sample, infrared colour selection, and predictions for AGN within 100 Mpc. | ASMUS D., GREENWELL C.L., GANDHI P., et al. |
