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| SDSS J102855.67+095145.4 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST16:53:50 |
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| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
2009AJ....138..338S 
|
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
|
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. | ||
|
2015ApJS..217...27A
|
16 | D | 1 | 5847 | 53 | A catalog of visually classified galaxies in the local (z ∼ 0.01) universe. | ANN H.B., SEO M. and HA D.K. | ||
|
2015AstBu..70....1K
|
16 | D | 1 | 373 | 5 | Large-scale structure and galaxy motions in the Leo/Cancer constellations. | KARACHENTSEV I.D., NASONOVA O.G. and KARACHENTSEVA V.E. | ||
| 2015ApJ...812...98J | 16 | D | 2 | 12 | 11 | The gas phase mass metallicity relation for dwarf galaxies: dependence on star formation rate and H I gas mass. | JIMMY, TRAN K.-V., SAINTONGE A., et al. | ||
| 2016ApJ...825...34J | 134 | D | X | 4 | 15 | 3 | Spatial correlation between dust and Hα emission in dwarf irregular galaxies. | JIMMY, TRAN K.-V., SAINTONGE A., et al. | |
|
2018ApJ...861...49H
|
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. | ||
|
2020MNRAS.494.1784A
|
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. | ||
|
2022ApJS..261...21Y
|
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. |
