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 language | English |
|---|---|
| Article number | e230018 |
| Journal | Astronomische Nachrichten |
| Volume | 344 |
| Issue number | 4 |
| DOIs | |
| Publication status | Published - 16 Feb 2023 |
| Externally published | Yes |
Bibliographical note
Publisher Copyright:© 2023 Wiley-VCH GmbH.
Funding
information STFC, Grant/Award Number: ST/R000638/1; FJC2020-043334-I, MCIN/AEI/10.13039/501100011033, NextGenerationEU/PRTR, Grant/Award Number: PID2020-120323GB-I00The authors are grateful to the anonymous referee for the comments which significantly improved the manuscript. This project was supported by the STFC funding ST/R000638/1. F. M. Vincentelli acknowledges financial support from grant FJC2020-043334-I financed by MCIN/AEI/10.13039/501100011033 and NextGenerationEU/PRTR as well as from the Spanish Ministery of Science and Innovation research project PID2020-120323GB-I00. The authors are grateful to the anonymous referee for the comments which significantly improved the manuscript. This project was supported by the STFC funding ST/R000638/1. F. M. Vincentelli acknowledges financial support from grant FJC2020‐043334‐I financed by MCIN/AEI/10.13039/501100011033 and NextGenerationEU/PRTR as well as from the Spanish Ministery of Science and Innovation research project PID2020‐120323GB‐I00.
| Funders | Funder number |
|---|---|
| UK Research and Innovation | |
| Science and Technology Facilities Council (STFC) | FJC2020-043334-I, MCIN/AEI/10.13039/501100011033, ST/R000638/1 |
| Ministry of Science, Innovation and Universities | PID2020‐120323GB‐I00 |
Keywords
- accretion
- accretion disks
- galaxies: active
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science