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| SDSS J101754.72-002811.9 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST22:07:02 |
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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. | ||
|
2014ApJ...788...45T
|
15 | D | 1 | 224166 | 54 | Luminosity and redshift dependence of the covering factor of active galactic nuclei viewed with WISE and Sloan Digital Sky Survey. | TOBA Y., OYABU S., MATSUHARA H., 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. | ||
|
2020MNRAS.492..468D
|
16 | D | 1 | 467 | 19 | Chemical abundances of Seyfert 2 AGNs - I. Comparing oxygen abundances from distinct methods using SDSS. | DORS O.L., FREITAS-LEMES P., AMORES E.B., et al. | ||
| 2021MNRAS.508.3023M | 17 | D | 1 | 70 | 3 | Chemical abundances in Seyfert galaxies - VIII. Argon abundance estimates. | MONTEIRO A.F. and DORS O.L. | ||
|
2022MNRAS.514.5506D
|
17 | D | 1 | 71 | 4 | Chemical abundances in Seyfert galaxies - IX. Helium abundance estimates. | DORS O.L., VALERDI M., FREITAS-LEMES P., et al. | ||
|
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. |
