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| MGC 24169 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST15:28:41 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2003MNRAS.344..307L |
63299 | 194 | The Millennium Galaxy Catalogue: 16 ≤BMGC< 24 galaxy counts and the calibration of the local galaxy luminosity function. | LISKE J., LEMON D.J., DRIVER S.P., 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. | ||
|
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. | ||
| 2017MNRAS.470.3775V | 95 | D | F | 5 | 68 | 26 | VALES I: the molecular gas content in star-forming dusty H-ATLAS galaxies up to z = 0.35. | VILLANUEVA V., IBAR E., HUGHES T.M., et al. | |
|
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. | ||
| 2019MNRAS.482.1499M | 97 | D | F | 2 | 39 | ~ | VALES V: a kinematic analysis of the molecular gas content in H-ATLAS galaxies at z ∼ 0.03-0.35 using ALMA. | MOLINA J., IBAR E., VILLANUEVA V., 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. | ||
|
2022MNRAS.517..962D |
17 | D | 1 | 387 | 17 | Dust, CO, and [C I]: cross-calibration of molecular gas mass tracers in metal-rich galaxies across cosmic time. | DUNNE L., MADDOX S.J., PAPADOPOULOS P.P., 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. |