LEDA 1377131 , the SIMBAD biblio

LEDA 1377131 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST21:02:34


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Title First 3 Authors
2003A&A...412...45P viz 15       D               1 956189 750 HYPERLEDA. I. Identification and designation of galaxies. PATUREL G., PETIT C., PRUGNIEL P., et al.
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.
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.
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.
2014MNRAS.440.3202V 15       D               3 21 39 The triggering mechanism and properties of ionized outflows in the nearest obscured quasars. VILLAR MARTIN M., EMONTS B., HUMPHREY A., et al.
2016ApJ...832...67N viz 16       D               1 71 19 The origin of double-peaked narrow lines in active galactic nuclei. II. Kinematic classifications for the population at z < 0.1. NEVIN R., COMERFORD J., MULLER-SANCHEZ F., et al.
2018ApJ...856..102F 380       D     X C       9 17 66 Hubble Space Telescope observations of extended [O III]λ 5007 emission in nearby QSO2s: new constraints on AGN host galaxy interaction. FISCHER T.C., KRAEMER S.B., SCHMITT H.R., 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.
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.
2021MNRAS.500.1491T 477       D     X         12 13 16 Hubble Space Telescope observations of [O III] emission in nearby QSO2s: physical properties of the ionized outflows. TRINDADE FALCAO A., KRAEMER S.B., FISCHER T.C., et al.
2022A&A...658A.155R 1295       D S   X C       29 21 24 The diverse cold molecular gas contents, morphologies, and kinematics of type-2 quasars as seen by ALMA. RAMOS ALMEIDA C., BISCHETTI M., GARCIA-BURILLO S., et al.
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.
2023MNRAS.522.1736P 104       D         F     5 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 18       D               4 48 ~ QSOFEED: Relationship between star formation and active galactic nuclei feedback. BESSIERE P.S., RAMOS ALMEIDA C., HOLDEN L.R., et al.
2024MNRAS.535..621T 18       D               1 20 ~ Hubble Space Telescope observations of nearby type 1 quasars. I. Characterization of the extended [O III] 5007 Å emission. TRINDADE FALCAO A., KRAEMER S.B., FISCHER T.C., et al.
2025ApJ...981..194L 19       D               5 182 ~ Measuring the Interstellar Medium Content of Nearby, Luminous, Type 1 and Type 2 QSOs through CO and [C II]. LUO Y., PETRIC A.O., JANSSEN R.M.J., 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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