2MASS J11233090+3105195 , the SIMBAD biblio

2MASS J11233090+3105195 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST19:18:15


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Title First 3 Authors
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.
2016MNRAS.463.3056A 645       D     X   F     16 23 2 Sensitive radio survey of obscured quasar candidates. ALEXANDROFF R.M., ZAKAMSKA N.L., VAN VELZEN S., 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.
2018ApJ...867...66C viz 16       D               1 95 8 The origin of double-peaked narrow lines in active galactic nuclei. IV. Association with galaxy mergers. COMERFORD J.M., NEVIN R., STEMO A., et al.
2019ApJ...873...90S 16       D               1 87 4 Testing the evolutionary link between type 1 and type 2 quasars with measurements of the interstellar medium. SHANGGUAN J. and HO L.C.
2022MNRAS.512...86B viz 17       D               1 304 3 Quantifying the cool ISM in radio AGNs: evidence for late-time retriggering by galaxy mergers and interactions. BERNHARD E., TADHUNTER C.N., PIERCE J.C.S., et al.
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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