SDSS J123031.37+251834.1 , the SIMBAD biblio

SDSS J123031.37+251834.1 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST23:13:42


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Title First 3 Authors
1995AJ....110.2009O viz 32173 32 Galaxy properties at the North Galactic Pole. I. Photometric properties on large spatial scales. ODEWAHN S.C. and ALDERING G.
2011AJ....142..170H viz 15       D               1 15886 568 The Arecibo Legacy Fast ALFA survey: the α.40 H I source catalog, its characteristics and their impact on the derivation of the H I mass function. HAYNES M.P., GIOVANELLI R., MARTIN A.M., et al.
2015ApJ...809..146B viz 16       D               1 1719 72 A study in blue: the baryon content of isolated low-mass galaxies. BRADFORD J.D., GEHA M.C. and BLANTON M.R.
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               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.
2018ApJ...861...49H viz 16       D               1 31270 293 The Arecibo Legacy Fast ALFA survey: the ALFALFA extragalactic H I source catalog. HAYNES M.P., GIOVANELLI R., KENT B.R., 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.
2019ApJ...884..180D 17       D               1 28 42 AGN all the way down? AGN-like line ratios are common in the lowest-mass isolated quiescent galaxies. DICKEY C.M., GEHA M., WETZEL A., et al.
2022ApJS..261...21Y viz 17       D               1 29963 6 Statistical Analysis of H I Profile Asymmetry and Shape for Nearby Galaxies. YU N., HO L.C., WANG J., et al.
2023ApJS..265...25J viz 17       D               1 12814 1 The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Quasar Survey: Quasar Properties from Data Releases 6 to 9. JIN J.-J., WU X.-B., FU Y., et al.

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