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

0517370 - ASÚ 2020 RIV US eng J - Článek v odborném periodiku
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
Grant CEP: GA ČR GA17-16287S
Institucionální podpora: RVO:67985815
Klíčová slova: active galactic nuclei * focus imaging spectrograph * african large telescope
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 5.746, rok: 2019
Způsob publikování: Omezený přístup
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.
Trvalý link: http://hdl.handle.net/11104/0302689