2MASS J00523062-0115484 , the SIMBAD biblio

2MASS J00523062-0115484 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST15:16:57


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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.
2009ApJS..182..543A 248 9 4475 The seventh data release of the Sloan Digital Sky Survey. ABAZAJIAN K.N., ADELMAN-McCARTHY J.K., AGUEROS M.A., et al.
2009ApJ...702..441G viz 15       D               1 127 41 The growth of black holes: insights from obscured active galaxies. GREENE J.E., ZAKAMSKA N.L., LIU X., 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.
2012MNRAS.421.1569B viz 15       D               1 18458 511 On the fundamental dichotomy in the local radio-AGN population: accretion, evolution and host galaxy properties. BEST P.N. and HECKMAN T.M.
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.
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 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.
2023MNRAS.522.1736P 104       D         F     4 49 1 Galaxy interactions are the dominant trigger for local type 2 quasars. PIERCE J.C.S., TADHUNTER C., RAMOS ALMEIDA C., et al.
2024A&A...689A.271B 197       D     X         5 48 ~ QSOFEED: Relationship between star formation and active galactic nuclei feedback. BESSIERE P.S., RAMOS ALMEIDA C., HOLDEN L.R., et al.
2026MNRAS.545f2075H 20       D               3 49 ~ Electron densities from [S II] lines significantly overestimate the impact of ionized AGN outflows. HOLDEN L.R., SMITH D.J.B., ARNAUDOVA M.I., et al.

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