SDSS J112712.77+084717.0 , the SIMBAD biblio

SDSS J112712.77+084717.0 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST18:03:50


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Title First 3 Authors
2009AJ....138..338S viz 15       D               1 635 47 The Arecibo Legacy Fast ALFA Survey. IX. The Leo region H I catalog, group membership, and the H I mass function for the Leo I group. STIERWALT S., HAYNES M.P., GIOVANELLI R., et al.
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.
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.
2019MNRAS.483.1754D viz 16       D               1 1130 7 Low Surface Brightness Galaxy catalogue selected from the α.40-SDSS DR7 Survey and Tully-Fisher relation. DU W., CHENG C., WU H., et al.
2020NatAs...4..246G 207           X C       4 26 38 Further evidence for a population of dark-matter-deficient dwarf galaxies. GUO Q., HU H., ZHENG Z., et al.
2020MNRAS.494.2090J viz 16       D               1 5735 ~ The H I mass function of group galaxies in the ALFALFA survey. JONES M.G., HESS K.M., ADAMS E.A.K., et al.
2021MNRAS.501..254K 17       D               1 21 ~ Dwarf galaxies without dark matter: constraints on modified gravity. KHALIFEH A.R. and JIMENEZ R.
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.
2023MNRAS.525.2535O 44           X         1 7 ~ Frequency of the dark matter subhalo collisions and bifurcation sequence arising formation of dwarf galaxies. OTAKI K. and MORI M.
2025PASP..137j4102C 19       D               1 280 ~ Fitting the Shadows: Star Formation Scaling Relations in the Low Surface Brightness Regime. CHRISTIE H.S., BARMBY P. and YOUNG J.E.

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