SDSS J135855.82+493414.1 , the SIMBAD biblio

SDSS J135855.82+493414.1 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.02.22CET19:51:43


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Title First 3 Authors
2014ApJ...788...45T viz 16       D               1 224162 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.
2015ApJ...804L..15S viz 16       D               1 7921 26 Dissecting the quasar main sequence: insight from host galaxy properties. SUN J. and SHEN Y.
2017ApJ...842...44K 16       D               1 72 5 Active galactic nuclei with a low-metallicity narrow-line region. KAWASAKI K., NAGAO T., TOBA Y., et al.
2018ApJ...862..109Y 185       D     X         5 35 142 Discovery of 21 new changing-look AGNs in the northern sky. YANG Q., WU X.-B., FAN X., et al.
2019ApJ...881L..24V viz 17       D               1 1524 ~ Are narrow-line Seyfert 1 galaxies powered by low-mass black holes? VISWANATH G., STALIN C.S., RAKSHIT S., et al.
2019ApJS..243...21L viz 17       D               1 14589 47 A comprehensive and uniform sample of broad-line active galactic nuclei from the SDSS DR7. LIU H.-Y., LIU W.-J., DONG X.-B., et al.
2020MNRAS.491.4925G viz 17       D               1 174 65 Understanding extreme quasar optical variability with CRTS - II. Changing-state quasars. GRAHAM M.J., ROSS N.P., STERN D., et al.
2021A&A...650A..33P 496       D     X C       11 9 3 A systematic search for changing-look quasars in SDSS-II using difference spectra. POTTS B. and VILLFORTH C.
2021ApJ...915...63L 104       D     X         3 60 4 Local active galactic nuclei with large broad-Hα variability reside in red galaxies. LIU W.-J., LIRA P., YAO S., et al.
2022ApJ...926..184J 197       D     X         5 35 6 A Systematic Analysis of Stellar Populations in the Host Galaxies of Changing-look AGNs. JIN J.-J., WU X.-B. and FENG X.-T.
2023ApJ...958..146W 19       D               1 27 ~ Magnetized Accretion Disks with Outflows for Changing-look AGNs. WU W.-B. and GU W.-M.

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