2MASX J09173114+3328323 , the SIMBAD biblio

2MASX J09173114+3328323 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST00:34:57


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Title First 3 Authors
1998AJ....116.1529H viz 788 20 Dynamics of cD clusters of galaxies. III. Redshift data for 11 Abell clusters. HILL J.M. and OEGERLE W.R.
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.
2008ApJ...685..904P viz 15       D               1 45 23 Outliers from the mass-metallicity relation. I. A sample of metal-rich dwarf galaxies from SDSS. PEEPLES M.S., POGGE R.W. and STANEK K.Z.
2012ApJS..199...22H viz 15       D               4 5021 8 UV to Far-IR catalog of a galaxy sample in nearby clusters: spectral energy distributions and environmental trends. HERNANDEZ-FERNANDEZ J.D., IGLESIAS-PARAMO J. and VILCHEZ J.M.
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.
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.
2017A&A...599A..71D viz 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.
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.
2020ApJS..246....2A viz 16       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 16       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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