LEDA 3092170 , the SIMBAD biblio

LEDA 3092170 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.05.14CEST03:20:40


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Title First 3 Authors
2003A&A...412...45P viz 15       D               1 956205 750 HYPERLEDA. I. Identification and designation of galaxies. PATUREL G., PETIT C., PRUGNIEL P., et al.
2015ApJ...810..166E viz 16       D               1 2287 10 RESOLVE survey photometry and volume-limited calibration of the photometric gas fractions technique. ECKERT K.D., KANNAPPAN S.J., STARK D.V., et al.
2015ApJ...812...89M viz 16       D               1 12670 7 ECO and RESOLVE: galaxy disk growth in environmental context. MOFFETT A.J., KANNAPPAN S.J., BERLIND A.A., et al.
2016ApJ...832..126S viz 16       D               1 2164 18 The RESOLVE survey atomic gas census and environmental influences on galaxy gas reservoirs. STARK D.V., KANNAPPAN S.J., ECKERT K.D., et al.
2017ApJ...849...20E viz 16       D               2 9926 2 The baryonic collapse efficiency of galaxy groups in the RESOLVE and ECO surveys. ECKERT K.D., KANNAPPAN S.J., LAGOS C.D.P., et al.
2017MNRAS.471.2687B viz 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.
2018ApJ...857..144H viz 16       D               1 2288 40 The origin of faint tidal features around galaxies in the RESOLVE survey. HOOD C.E., KANNAPPAN S.J., STARK D.V., et al.
2019ApJS..244....3D viz 17       D               1 23802 ~ 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.
2019MNRAS.487.5572M viz 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 viz 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.

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