LEDA 1610890 , the SIMBAD biblio

LEDA 1610890 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST05:01:47


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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.
2004A&A...425..429C viz 126 62 Multiple merging in the Abell cluster 1367. CORTESE L., GAVAZZI G., BOSELLI A., et al.
2004AJ....128.1558S viz 15       D               1 5584 130 NOAO fundamental plane survey. I. Survey design, redshifts, and velocity dispersion data. SMITH R.J., HUDSON M.J., NELAN J.E., et al.
2011MNRAS.412.1295M 15       D               1 79 3 The galaxy population of Abell 1367: the stellar mass–metallicity relation. MOUHCINE M., KRIWATTANAWONG W. and JAMES P.A.
2011A&A...527A.101K viz 15       D               1 360 5 The galaxy population of Abell 1367: photometric and spectroscopic data. KRIWATTANAWONG W., MOSS C., JAMES P.A., et al.
2012ApJS..199...36S viz 15       D               1 473 4 A deep, wide-field Hα survey of nearby clusters of galaxies: data. SAKAI S., KENNICUTT R.C.Jr and MOSS C.
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.
2017ApJ...849...20E viz 16       D               1 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.
2018MNRAS.478.4336M viz 16       D               1 4285 3 Ultraviolet and optical view of galaxies in the Coma supercluster. MAHAJAN S., SINGH A. and SHOBHANA D.
2020ApJS..246....2A viz 17       D               1 36251 ~ GalWeight application: a publicly available catalog of dynamical parameters of 1800 galaxy clusters from SDSS-DR13, (GalWCat19). ABDULLAH M.H., WILSON G., KLYPIN A., et al.
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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