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| GAMA 397294 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST09:40:56 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2005MNRAS.360..587B |
222 | 39 | Near-infrared imaging of 222 nearby Hδ-strong galaxies from the Sloan Digital Sky Survey. | BALOGH M.L., MILLER C., NICHOL R., et al. | |||||
|
2013MNRAS.431.2034M |
15 | D | 1 | 816 | 11 | The spectral energy distributions of K+A galaxies from the UV to the mid-IR: stellar populations, star formation and hot dust. | MELNICK J. and DE PROPRIS R. | ||
|
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. | ||
|
2015MNRAS.452.2087L |
16 | D | 1 | 71490 | 449 | Galaxy And Mass Assembly (GAMA): end of survey report and data release 2. | LISKE J., BALDRY I.K., DRIVER S.P., et al. | ||
|
2016A&A...590A..29P |
16 | D | 1 | 13088 | 7 | Multifrequency studies of galaxies and groups. I. Environmental effect on galaxy stellar mass and morphology. | POUDEL A., HEINAMAKI P., NURMI P., et al. | ||
|
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. | ||
|
2018ApJ...868...99F |
16 | D | 2 | 19564 | 4 | Identifying tidal disruption events via prior photometric selection of their preferred hosts. | FRENCH K.D. and ZABLUDOFF A.I. | ||
|
2022MNRAS.513..439D |
17 | D | 1 | 302202 | 70 | Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions. | DRIVER S.P., BELLSTEDT S., ROBOTHAM A.S.G., et al. |