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| SDSS J144518.88+025012.3 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST16:41:53 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
2009MNRAS.395..255M 
|
15 | D | 1 | 397037 | 82 | Compact groups in theory and practice - III. Compact groups of galaxies in the sixth data release of the Sloan Digital Sky Survey. | McCONNACHIE A.W., PATTON D.R., ELLISON S.L., et al. | ||
|
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.446.3526C | 16 | D | 4 | 41 | 49 | HIGHz: a survey of the most HI-massive galaxies at z ∼ 0.2. | CATINELLA B. and CORTESE L. | ||
|
2017A&A...599A..71D
|
16 | D | 1 | 209271 | 41 | Aperture-free star formation rate of SDSS star-forming galaxies. | DUARTE PUERTAS S., VILCHEZ J.M., IGLESIAS-PARAMO J., et al. | ||
| 2017ApJ...848L...7C | 16 | D | 2 | 9 | 12 | ALMA shows that gas reservoirs of star-forming disks over the past 3 billion years are not predominantly molecular. | CORTESE L., CATINELLA B. and JANOWIECKI S. | ||
|
2018MNRAS.474.3875B
|
16 | D | 1 | 133173 | 163 | Galaxy And Mass Assembly: the G02 field, Herschel-ATLAS target selection and data release 3. | BALDRY I.K., LISKE J., BROWN M.J.I., et al. | ||
| 2018MNRAS.479.3319T | 96 | D | F | 4 | 40 | 1 | CO Tully-Fisher relation of star-forming galaxies at = 0.05-0.3. | TOPAL S., BUREAU M., TILEY A.L., et al. | |
|
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. | ||
|
2022A&A...666A.186D
|
17 | D | 1 | 194359 | 6 | Mass-metallicity and star formation rate in galaxies: A complex relation tuned to stellar age. | DUARTE PUERTAS S., VILCHEZ J.M., IGLESIAS-PARAMO J., et al. |
