Optical and X-ray monitoring of the NLS1 galaxy Ark 564
| dc.creator | Papadakis, I. E. | |
| dc.creator | Brinkmann, W. | |
| dc.creator | Negoro, H. | |
| dc.creator | Detsis, E. | |
| dc.creator | Papamastorakis, I. | |
| dc.creator | Gliozzi, M. | |
| dc.date | 2000-12-14 | |
| dc.date.accessioned | 2026-07-07T01:57:02Z | |
| dc.date.available | 2026-07-07T01:57:02Z | |
| dc.description | The Narrow-line Seyfert galaxy Ark 564 was monitored between June 04, 2000 and June 24, 2000 from Skinakas Observatory. The B,V,R and I band light curves show night to night variations of 0.1 mag. Comparison with X-ray data from a simultaneous ASCA observation shows that the X-ray variations are more pronounced than in the optical band. Cross correlation analysis yields a time lag of ~ 0.8 days in the sense that the X-rays are leading the optical but with low statistical significance. We discuss possible implications of our results to current physical models of AGN. | |
| dc.description | 7 pages, 3 figures, accepted for publication in Astronomy and Astrophysics | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0012317 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0012317 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/2227 | |
| dc.subject | Astrophysics | |
| dc.title | Optical and X-ray monitoring of the NLS1 galaxy Ark 564 | |
| dc.type | text |