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MCG-02-02-029 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST14:29:40 |
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 |
---|---|---|---|---|---|---|---|---|---|
1998PASP..110..779C | 4311 | 3 | Accurate positions for MCG galaxies. | CORWIN H.G.Jr, PESENSON I., SCHMITZ M., et al. | |||||
2003A&A...412...45P | 15 | D | 1 | 956205 | 750 | HYPERLEDA. I. Identification and designation of galaxies. | PATUREL G., PETIT C., PRUGNIEL P., et al. | ||
2009MNRAS.399..683J | 15 | D | 1 | 124640 | 796 | The 6dF galaxy survey: final redshift release (DR3) and southern large-scale structures. | JONES D.H., READ M.A., SAUNDERS W., et al. | ||
2011MNRAS.416.2840L | 15 | D | 1 | 72554 | 178 | The 2M++ galaxy redshift catalogue. | LAVAUX G. and HUDSON M.J. | ||
2014ApJ...788...45T | 16 | D | 1 | 224162 | 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. | ||
2016A&A...588A..14T | 16 | D | 1 | 84076 | 35 | Friends-of-friends galaxy group finder with membership refinement. | TEMPEL E., KIPPER R., TAMM A., et al. | ||
2017ApJ...837..120G | 16 | D | 1 | 14403 | 66 | LOSS revisited. I. Unraveling correlations between supernova rates and galaxy properties, as measured in a reanalysis of the Lick Observatory Supernova Search. | GRAUR O., BIANCO F.B., HUANG S., et al. | ||
2017MNRAS.471.2687B | 16 | D | 1 | 7831 | 45 | On the interdependence of galaxy morphology, star formation and environment in massive galaxies in the nearby Universe. | BAIT O., BARWAY S. and WADADEKAR Y. | ||
2019MNRAS.487.5572M | 17 | D | 1 | 4573 | ~ | Connecting galaxy structure and star formation: the role of environment in formation of S0 galaxies. | MISHRA P.K., WADADEKAR Y. and BARWAY S. | ||
2020MNRAS.494.1784A | 17 | D | 1 | 47437 | 9 | Local AGN survey (LASr): I. Galaxy sample, infrared colour selection, and predictions for AGN within 100 Mpc. | ASMUS D., GREENWELL C.L., GANDHI P., et al. |