other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
SDSS J161910.48+064223.2 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST19:15:18 |
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 |
---|---|---|---|---|---|---|---|---|---|
2010ApJ...723.1119L | 15 | D | 1 | 1041 | 41 | On the populations of radio galaxies with extended morphology at z < 0.3. | LIN Y.-T., SHEN Y., STRAUSS M.A., et al. | ||
2011MNRAS.410.1583S | 361 | D | X C F | 8 | 14 | 14 | Radio emission and active galactic nucleus feedback in post-starburst galaxies. | SHIN M.-S., STRAUSS M.A. and TOJEIRO R. | |
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. | ||
2016ApJ...833...19P | 16 | D | 2 | 6269 | 9 | The evolution of post-starburst galaxies from z ∼ 1 to the present. | PATTARAKIJWANICH P., STRAUSS M.A., HO S., 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. | ||
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. | ||
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. | ||
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. | ||
2019MNRAS.488.2263B | 17 | D | 1 | 25 | ~ | A classifier to detect elusive astronomical objects through photometry. | BHAVANA D., VIG S., GHOSH S.K., et al. |