|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Help |
| 2MASX J15252654+4310114 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2022.06.28CEST08:52:59 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
2003A&A...412...45P 
|
15 | D | 1 | 956227 | 675 | HYPERLEDA. I. Identification and designation of galaxies. | PATUREL G., PETIT C., PRUGNIEL P., et al. | ||
|
2010MNRAS.405..783M
|
15 | D | 1 | 5435 | 142 | Galaxy Zoo: passive red spirals. | MASTERS K.L., MOSLEH M., ROMER A.K., et al. | ||
|
2014ApJ...788...45T
|
16 | D | 1 | 224163 | 19 | 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. | ||
| 2017MNRAS.465.2317J | 84 | F | 1 | 25 | 12 | SDSS-IV MaNGA: bulge-disc decomposition of IFU data cubes (BUDDI). | JOHNSTON E.J., HAUSSLER B., ARAGON-SALAMANCA A., et al. | ||
|
2017MNRAS.466.2570B
|
17 | D | 1 | 587 | 25 | SDSS-IV MaNGA - the spatially resolved transition from star formation to quiescence. | BELFIORE F., MAIOLINO R., MARASTON C., et al. | ||
|
2017AJ....154...86W
|
17 | D | 2 | 4613 | 26 | The SDSS-IV MaNGA sample: design, optimization, and usage considerations. | WAKE D.A., BUNDY K., DIAMOND-STANIC A.M., et al. | ||
|
2018MNRAS.476.1765L
|
17 | D | 1 | 2080 | 7 | SDSS-IV MaNGA: global stellar population and gradients for about 2000 early-type and spiral galaxies on the mass-size plane. | LI H., MAO S., CAPPELLARI M., et al. | ||
|
2018MNRAS.477.4711G
|
17 | D | 1 | 2754 | 5 | SDSS-IV MaNGA: stellar angular momentum of about 2300 galaxies: unveiling the bimodality of massive galaxy properties. | GRAHAM M.T., CAPPELLARI M., LI H., et al. | ||
| 2020MNRAS.495.4820L | 18 | D | 1 | 60 | ~ | SDSS-IV MaNGA: stellar population correlates with stellar root-mean-square velocity Vrms gradients or total-density-profile slopes at fixed effective velocity dispersion σe. | LU S., CAPPELLARI M., MAO S., et al. |
© Université de Strasbourg/CNRS
• Contact
