[VV2000] J141221.8+004717 , the SIMBAD biblio

[VV2000] J141221.8+004717 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST00:01:23


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Title First 3 Authors
2000A&A...358...77W viz 415 273 The Hamburg/ESO survey for bright QSOs. III. A large flux-limited sample of QSOs. WISOTZKI L., CHRISTLIEB N., BADE N., 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.
2009A&A...495...83M 16       D   O           5 35 90 VLT/ISAAC spectra of the Hβ region. in intermediate-redshift quasars. III. Hβ broad-line profile analysis and inferences about BLR structure. MARZIANI P., SULENTIC J.W., STIRPE G.M., 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.
2015ApJS..217....3M 484       D     X C       12 24 ~ O I and Ca II observations in intermediate redshift quasars. MARTINEZ-ALDAMA M.L., DULTZIN D., MARZIANI P., et al.
2017A&A...608A.122S viz         O           27 18 What does CIVλ1549 tell us about the physical driver of the Eigenvector quasar sequence? SULENTIC J.W., DEL OLMO A., MARZIANI P., et al.
2018AJ....155..189D viz 16       D               1 18896 7 The Large Sky Area Multi-Object Fibre Spectroscopic Telescope (LAMOST) Quasar Survey: quasar properties from data release two and three. DONG X.Y., WU X.-B., AI Y.L., et al.
2020ApJ...902...76P 16       D               1 53 ~ The CaFe project: optical Fe II and near-infrared Ca II triplet emission in active galaxies. I. Photoionization modeling. PANDA S., MARTINEZ-ALDAMA M.L., MARINELLO M., et al.
2021ApJ...918...29M 17       D               2 54 7 The CaFe project: optical Fe II and near-infrared Ca II triplet emission in active galaxies. II. The Driver(s) of the Ca II and Fe II and its potential use as a chemical clock. MARTINEZ-ALDAMA M.L., PANDA S., CZERNY B., et al.
2024A&A...691A..15D viz 18       D               2 144 ~ Exploring the links between quasar winds and radio emission along the main sequence at high redshift. DECONTO-MACHADO A., DEL OLMO A. and MARZIANI P.

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