LEDA 1167422 , the SIMBAD biblio

LEDA 1167422 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST05:09:34


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Title First 3 Authors
2001MNRAS.328.1039C viz 206872 1908 The 2dF Galaxy Redshift Survey: spectra and redshifts. COLLESS M., DALTON G., MADDOX S., et al.
2003A&A...412...45P viz 15       D               1 956189 750 HYPERLEDA. I. Identification and designation of galaxies. PATUREL G., PETIT C., PRUGNIEL P., et al.
2014ApJ...788...45T viz 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 viz 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 viz 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.
2018MNRAS.474.3875B viz 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.
2019ApJS..244....3D viz 16       D               1 23803 ~ Circumventing the effects of projection and dust using inclination-independent infrared galaxy structure measurements: method, error analysis, and a new public catalog of near-infrared galaxy structures. DEVOUR B.M. and BELL E.F.
2021ApJ...909...74M viz 17       D               1 1188 6 The Dragonfly Wide Field Survey. II. Accurate total luminosities and colors of nearby massive galaxies and implications for the Galaxy stellar-mass function. MILLER T.B., VAN DOKKUM P., DANIELI S., et al.
2022MNRAS.513..439D viz 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.

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