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| SDSS J101440.21+192448.9 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST21:17:56 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2013ApJ...775..116R |
16 | D | 1 | 174 | 355 | Dwarf galaxies with optical signatures of active massive black holes. | REINES A.E., GREENE J.E. and GEHA M. | ||
| 2016ApJ...829...57B | 16 | D | 1 | 90 | 75 | Multi-epoch spectroscopy of dwarf galaxies with AGN signatures: identifying sources with persistent broad Hα emission. | BALDASSARE V.F., REINES A.E., GALLO E., et al. | ||
|
2017A&A...599A..71D |
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. | ||
| 2019ApJ...884...54M | 182 | D | X F | 4 | 16 | 61 | AGN-Driven outflows in dwarf galaxies. | MANZANO-KING C.M., CANALIZO G. and SALES L.V. | |
| 2020MNRAS.498.4562M | 222 | D | X | 6 | 50 | ~ | Active galactic nucleus and dwarf galaxy gas kinematics. | MANZANO-KING C.M. and CANALIZO G. | |
|
2021Sci...373..789B |
17 | D | 1 | 344 | 46 | A characteristic optical variability time scale in astrophysical accretion disks. | BURKE C.J., SHEN Y., BLAES O., et al. | ||
| 2022AJ....163...73S | 17 | D | 1 | 40 | 4 | Search for intermediate-mass black holes at low redshift with intra-night variability. | SHIN L., WOO J.-H., SON D., et al. | ||
|
2022A&A...666A.186D |
17 | D | 1 | 194359 | 6 | Mass-metallicity and star formation rate in galaxies: A complex relation tuned to stellar age. | DUARTE PUERTAS S., VILCHEZ J.M., IGLESIAS-PARAMO J., et al. | ||
| 2023ApJ...950...33A | 453 | D | S X C | 9 | 11 | ~ | A Comparison of Outflow Properties in AGN Dwarfs versus Star-forming Dwarfs. | ARAVINDAN A., LIU W., CANALIZO G., et al. | |
| 2025MNRAS.544.2713C | 205 | D | X F | 4 | 40 | ~ | Investigating the impacts of AGN activities on dwarf galaxies with FAST H I observations. | CHEN H.-Y., TSAI C.-W., ZUO P., et al. |