[VV2010c] J151711.5+033059 , the SIMBAD biblio

[VV2010c] J151711.5+033059 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST11:24:35


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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.
2005AJ....129.1212Z 3 12 124 Candidate type II quasars from the Sloan Digital Sky Survey. III. Spectropolarimetry reveals hidden type I nuclei. ZAKAMSKA N.L., SCHMIDT G.D., SMITH P.S., et al.
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.
2010MNRAS.401.1429D viz 15       D               1 81094 425 The WiggleZ dark energy survey: survey design and first data release. DRINKWATER M.J., JUREK R.J., BLAKE C., et al.
2010MNRAS.404...48V 15       D               1 31 45 Discovery of Compton-thick quasars in the Sloan Digital Sky Survey. VIGNALI C., ALEXANDER D.M., GILLI R., et al.
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.
2013ApJ...777...27J 92       D     X         3 75 34 An archival Chandra and XMM-Newton survey of type 2 quasars. JIA J., PTAK A., HECKMAN T., et al.
2017A&A...604L...3H 43 6 Polarization of the changing-look quasar J1011+5442. HUTSEMEKERS D., AGIS GONZALEZ B., SLUSE D., et al.
2018MNRAS.474.4151D viz 16       D               1 223704 6 The WiggleZ Dark Energy Survey: final data release and the metallicity of UV-luminous galaxies. DRINKWATER M.J., BYRNE Z.J., BLAKE C., et al.
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.
2023MNRAS.518..130S viz 104       D       C       2 813 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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