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[YHW2016] 191.04630+14.48250 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST19:22:29 |
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 |
---|---|---|---|---|---|---|---|---|---|
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.421.1569B | 15 | D | 2 | 18499 | 511 | On the fundamental dichotomy in the local radio-AGN population: accretion, evolution and host galaxy properties. | BEST P.N. and HECKMAN T.M. | ||
2014ApJ...785..104R | 16 | D | 1 | 72334 | 578 | redMaPPer. I. Algorithm and SDSS DR8 catalog. | RYKOFF E.S., ROZO E., BUSHA M.T., et al. | ||
2016ApJS..224....1R | 16 | D | 1 | 670876 | 246 | The redMaPPer galaxy cluster catalog from DES science verification data. | RYKOFF E.S., ROZO E., HOLLOWOOD D., et al. | ||
2016MNRAS.460.3669Y | 16 | D | 1 | 7138 | 25 | Radio luminosity function of brightest cluster galaxies. | YUAN Z.S., HAN J.L. and WEN Z.L. | ||
2017MNRAS.466.4346M | 16 | D | 1 | 1437 | 66 | The nuclear properties and extended morphologies of powerful radio galaxies: the roles of host galaxy and environment. | MIRAGHAEI H. and BEST P.N. | ||
2018A&A...611A..42B | 16 | D | 1 | 183 | 7 | The GALEX Ultraviolet Virgo Cluster Survey (GUViCS). VII. Brightest cluster galaxy UV upturn and the FUV-NUV color up to redshift 0.35. | BOISSIER S., CUCCIATI O., BOSELLI A., et al. | ||
2018AJ....155..188L | 16 | D | 1 | 13494 | 1 | An analysis framework for understanding the origin of nuclear activity in low-power radio galaxies. | LIN Y.-T., HUANG H.-J. and CHEN Y.-C. | ||
2019AJ....157..126G | 17 | D | 1 | 4305 | 35 | Radio Galaxy Zoo: the distortion of radio galaxies by galaxy clusters. | GARON A.F., RUDNICK L., WONG O.I., et al. | ||
2019ApJS..243...14O | 17 | D | 1 | 1527 | 25 | A catalog of the most optically luminous galaxies at z < 0.3: super spirals, super lenticulars, super post-mergers, and giant ellipticals. | OGLE P.M., LANZ L., APPLETON P.N., et al. |