SDSS J100854.44+461300.6 , the SIMBAD biblio

SDSS J100854.44+461300.6 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST02:08:50

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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
2003AJ....126.2125Z viz 289 306 Candidate type II quasars from the Sloan Digital Sky Survey. I. Selection and optical properties of a sample at 0.3<z<0.83. ZAKAMSKA N.L., STRAUSS M.A., KROLIK J.H., et al.
2004AJ....128.1002Z viz 177 92 Candidate type II quasars from the Sloan Digital Sky Survey. II. From radio to x-rays. ZAKAMSKA N.L., STRAUSS M.A., HECKMAN T.M., et al.
2004MNRAS.354..720V 17 18 Evidence for X-ray obscuration in Type II quasar candidates from the Sloan Digital Sky Survey. VIGNALI C., ALEXANDER D.M. and COMASTRI A.
2006A&A...455..773V viz 108223 628 A catalogue of quasars and active nuclei: 12th edition. VERON-CETTY M.-P. and VERON P.
2008AJ....136.2373R viz 890 251 Space density of optically selected type 2 quasars. REYES R., ZAKAMSKA N.L., STRAUSS M.A., et al.
2010AJ....139.1089L 354       D     X C       9 61 34 The radio properties of type 2 quasars. LAL D.V. and HO L.C.
2010A&A...518A..10V viz 15       D               1 168913 597 A catalogue of quasars and active nuclei: 13th edition. VERON-CETTY M.-P. and VERON P.
2018ApJ...859..116K viz 16       D               1 888 24 The black hole masses and Eddington ratios of type 2 quasars. KONG M. and HO L.C.
2019MNRAS.484.1021O viz 16       D               1 2523 ~ The redshift distribution of infrared-faint radio sources. ORENSTEIN B.J., COLLIER J.D. and NORRIS R.P.
2019AJ....157..126G viz 16       D               1 4305 35 Radio Galaxy Zoo: the distortion of radio galaxies by galaxy clusters. GARON A.F., RUDNICK L., WONG O.I., et al.
2019RAA....19..127L viz 16       D               1 401 ~ The environment of C- and S-shaped radio galaxies. LIU Y.-X., XU H.-G., ZHENG D.-C., et al.
2023MNRAS.518..130S viz 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.

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