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| 2MASS J13132744+1453386 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST23:30:16 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
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...698.1095U
|
15 | D | 3 | 125 | 129 | The FIRST-2MASS red quasar survey. II. An anomalously high fraction of LoBALs in searches for dust-reddened quasars. | URRUTIA T., BECKER R.H., WHITE R.L., 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. | ||
|
2012ApJ...757...51G
|
15 | D | 1 | 398 | 129 | FIRST-2MASS red quasars: transitional objects emerging from the dust. | GLIKMAN E., URRUTIA T., LACY M., et al. | ||
|
2015ApJ...804L..15S
|
16 | D | 1 | 7921 | 26 | Dissecting the quasar main sequence: insight from host galaxy properties. | SUN J. and SHEN Y. | ||
|
2015ApJ...812...66K
|
133 | D | X | 4 | 17 | 7 | Accretion rates of red quasars from the hydrogen Pβ line. | KIM D., IM M., GLIKMAN E., 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...934..119G
|
145 | D | X | 4 | 1141 | 9 | The WISE-2MASS Survey: Red Quasars Into the Radio Quiet Regime. | GLIKMAN E., LACY M., LAMASSA S., 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. | ||
| 2024A&A...690A.283K | 18 | D | 3 | 30 | ~ | Eddington ratios of dust-obscured quasars at z ≲ 1: Evidence supporting dust-obscured quasars as young quasars. | KIM D., KIM Y., IM M., et al. |
