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| [VV2003c] J154832.4-010811 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST01:29:38 |
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trying to find the most relevant references on this object.
More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
2006A&A...455..773V 
|
108223 | 628 | A catalogue of quasars and active nuclei: 12th edition. | VERON-CETTY M.-P. and VERON P. | |||||
|
2008AJ....136.2373R
|
890 | 251 | Space density of optically selected type 2 quasars. | REYES R., ZAKAMSKA N.L., STRAUSS M.A., et al. | |||||
|
2009MNRAS.393.1408C
|
504 | 3 | Infrared photometric study of type II quasars. | CHEN P.S. and SHAN H.G. | |||||
|
2010A&A...518A..10V
|
15 | D | 1 | 168913 | 597 | A catalogue of quasars and active nuclei: 13th edition. | VERON-CETTY M.-P. and VERON P. | ||
|
2012MNRAS.421.1043S
|
15 | D | 2 | 3198 | 151 | Strongly star forming galaxies in the local Universe with nebular He II λ4686 emission. | SHIRAZI M. and BRINCHMANN J. | ||
|
2018AJ....155...17C
|
16 | D | 1 | 802 | ~ | Infrared photometric study of Wolf-Rayet galaxies. | CHEN P.S., YANG X.H., LIU J.Y., et al. | ||
|
2018ApJ...859..116K
|
16 | D | 1 | 888 | 24 | The black hole masses and Eddington ratios of type 2 quasars. | KONG M. and HO L.C. | ||
|
2023MNRAS.518..130S
|
17 | D | 1 | 813 | 1 | Efficient analysis routines for single and double peaked Type 2 AGN spectra. | SELWOOD M., CALDERONE G., FOTOPOULOU S., et al. | ||
| 2023MNRAS.522.1736P | 409 | D | X C F | 8 | 49 | 1 | Galaxy interactions are the dominant trigger for local type 2 quasars. | PIERCE J.C.S., TADHUNTER C., RAMOS ALMEIDA C., et al. | |
| 2024A&A...689A.271B | 287 | D | X C | 6 | 48 | ~ | QSOFEED: Relationship between star formation and active galactic nuclei feedback. | BESSIERE P.S., RAMOS ALMEIDA C., HOLDEN L.R., et al. | |
| 2026MNRAS.545f2075H | 20 | D | 3 | 49 | ~ | Electron densities from [S II] lines significantly overestimate the impact of ionized AGN outflows. | HOLDEN L.R., SMITH D.J.B., ARNAUDOVA M.I., et al. |
