The evolution of the UV/optical lag spectrum of NGC 7469 seen by the Liverpool Telescope

F. M. Vincentelli*, M. Beard, I. Mc Hardy, E. Cackett, K. Horne, M. Pahari

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

We present the results regarding the analysis of an intensive monitoring of the Active Galactic Nucleus (AGN) NGC 7469. We observed the source for 4 months with almost daily cadence in the ugriz bands, using the IO:O on the Liverpool Telescope. We measured the lags with respect to the u band and found a clear change in the lag spectrum between the first and the second half of the campaign. Given that the source varies on different timescales during these two segments, it is likely that different components are dominating the variability at different times. This result further confirms that reverberation models require a more complex geometry than a static illuminating point source and that particular attention has to be given in the interpretation of these delays.
Original languageEnglish
Article numbere20230018
Number of pages5
JournalAstronomische Nachrichten
Volume344
Issue number4
Early online date16 Feb 2023
DOIs
Publication statusPublished - 1 May 2023

Keywords

  • Accretion
  • Accretion disks
  • Galaxies: active

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