NGP9 F322-1932092 , the SIMBAD biblio

NGP9 F322-1932092 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST12:03:14


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Title First 3 Authors
1995AJ....110.2009O viz 32173 32 Galaxy properties at the North Galactic Pole. I. Photometric properties on large spatial scales. ODEWAHN S.C. and ALDERING G.
2008AJ....136.2373R viz 890 251 Space density of optically selected type 2 quasars. REYES R., ZAKAMSKA N.L., STRAUSS M.A., et al.
2009MNRAS.393.1408C viz 504 3 Infrared photometric study of type II quasars. CHEN P.S. and SHAN H.G.
2010ApJ...708..427L viz 15       D               1 174 147 Type 2 active galactic nuclei with double-peaked [O III] lines: narrow-line region kinematics or merging supermassive black hole pairs? LIU X., SHEN Y., STRAUSS M.A., 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.
2012MNRAS.421.1043S viz 15       D               2 3198 151 Strongly star forming galaxies in the local Universe with nebular He II λ4686 emission. SHIRAZI M. and BRINCHMANN J.
2012ApJS..201...31G viz 15       D               1 15563 75 Double-peaked narrow emission-line galaxies from the Sloan Digital Sky Survey. I. Sample and basic properties. GE J.-Q., HU C., WANG J.-M., et al.
2014ApJ...788...45T viz 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 viz 16       D               1 888 24 The black hole masses and Eddington ratios of type 2 quasars. KONG M. and HO L.C.
2020ApJS..247...53K viz 16       D               1 23378 20 Radio sources associated with Optical Galaxies and having Unresolved or Extended morphologies (ROGUE). I. A catalog of SDSS galaxies with FIRST core identifications. KOZIEL-WIERZBOWSKA D., GOYAL A. and ZYWUCKA N.
2023MNRAS.518..130S viz 17       D               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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