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| SDSS J091803.34+285815.9 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST21:58:45 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
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. | |||||
|
2009ApJ...702..441G |
15 | D | 1 | 127 | 41 | The growth of black holes: insights from obscured active galaxies. | GREENE J.E., ZAKAMSKA N.L., LIU X., et al. | ||
|
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. | ||
|
2018MNRAS.474.1873W |
16 | D | 1 | 35327 | 23 | Spectral classification and composites of galaxies in LAMOST DR4. | WANG L.-L., LUO A.-L., SHEN S.-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. | ||
|
2022ApJ...929...61D |
17 | D | 1 | 11555 | 3 | Quiescent Galaxy Size, Velocity Dispersion, and Dynamical Mass Evolution. | DAMJANOV I., SOHN J., UTSUMI Y., 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. | ||
| 2024ApJ...966..128W | 18 | D | 3 | 48 | ~ | Identifying Changing-look AGNs Using Variability Characteristics. | WANG S., WOO J.-H., GALLO E., et al. |