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Time Delay Measurement of MgII Line in CTS C30.10 with SALT

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    0517370 - ASÚ 2020 RIV US eng J - Journal Article
    Czerny, B. - Olejak, A. - Ralowski, M. - Kozlowski, S. - Aldama, M.L. M. - Zajaček, M. - Pych, W. - Hryniewicz, K. - Pietrzynski, G. - Figaredo, C. S. - Haas, M. - Sredzinska, J. - Krupa, M. - Kurcz, A. - Udalski, A. - Gorski, M. - Karas, Vladimír - Panda, S. - Sniegowska, M. - Naddaf, S. R. - Bilicki, M. - Sarna, M.
    Time Delay Measurement of MgII Line in CTS C30.10 with SALT.
    Astrophysical Journal. Roč. 880, č. 1 (2019), č. článku 46. ISSN 0004-637X. E-ISSN 1538-4357
    R&D Projects: GA ČR GA17-16287S
    Institutional support: RVO:67985815
    Keywords : active galactic nuclei * focus imaging spectrograph * african large telescope
    OECD category: Astronomy (including astrophysics,space science)
    Impact factor: 5.746, year: 2019
    Method of publishing: Limited access
    https://doi.org/10.3847/1538-4357/ab2913

    We report 6 yr monitoring of distant bright quasar CTS C30.10 (z = 0.90052) with the Southern African Large Telescope. We measured the rest-frame time lag of 562(+116)(-68) days between the continuum variations and the response of the Mg II emission line, using six different methods. This time delay, combined with other available measurements of Mg II line delay, mostly for lower-redshift sources, shows that the Mg II line reverberation implies a radius-luminosity relation very similar to the one based on a more frequently studied H beta line.
    Permanent Link: http://hdl.handle.net/11104/0302689

     
     
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