천문학회보 (The Bulletin of The Korean Astronomical Society)
- 제42권2호
- /
- Pages.77.1-77.1
- /
- 2017
- /
- 1226-2692(pISSN)
Variability study of AGN in NGC 4395
- Cho, Hojin (Department of Physics and Astronomy, Seoul National University) ;
- Woo, Jong-Hak (Department of Physics and Astronomy, Seoul National University) ;
- Son, Donghoon (Department of Physics and Astronomy, Seoul National University) ;
- Le, Huynh Anh (Department of Physics and Astronomy, Seoul National University) ;
- Bae, Hyun-Jin (Department of Physics and Astronomy, Seoul National University) ;
- Shin, Jaejin (Department of Physics and Astronomy, Seoul National University) ;
- Park, Songyoun (Department of Physics and Astronomy, Seoul National University) ;
- Cho, Wanjin (Department of Physics and Astronomy, Seoul National University) ;
- Hodges-Kluck, Edmund (Department of Astronomy, University of Michigan) ;
- Gallo, Ellena (Department of Astronomy, University of Michigan) ;
- Kim, Minjin (Korea Astronomy and Space Science Institute) ;
- Park, Daeseong (Korea Astronomy and Space Science Institute) ;
- Sung, Hyun-il (Korea Astronomy and Space Science Institute) ;
- Kim, Taewoo (National Youth Space Center) ;
- Kang, Wonseok (National Youth Space Center)
- 발행 : 2017.10.10
초록
We present the preliminary results from our intensive monitoring campaign for measuring continuum and line variability of a low-mass Seyfert galaxy, NGC 4395, which host a smallest known AGN black hole in the reverberation mapping studies. We performed consecutive photometric observations during 5 nights in April 2017. Various telescopes in the world, including BOAO 1.8-m, NYSC 1-m, MDM 2.4-m, 1.3-m, etc, were dedicated for this campaign. Preliminary results show that the tentative time lag can be determined, which is approximately order of 1-2 hours.
키워드