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11.6. Spectral monitoring of AGN at the 6 meter telescope
Published online by Cambridge University Press: 25 May 2016
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To study broad line region (BLR) size and kinematics spectral monitoring of NGC 3516, NGC 4151, NGC 5548, NGC 7469 and 3C390.3 has been performed with the 6 m telescope of the Special Astrophysical Observatory (N. Arkhyz- North Caucasus) in 1986–1996. The spectra are obtained in the Nasmyth focus using the TV scanner with a resolution of 3–4Å and S/N= 10–25 within 4000–5200ÅÅ (1986–94, 500 spectra), and in the prime focus with the spectrograph UAGS (a long-slit mode) + CCD (resolution 5–10Å) or multi-pupil field spectrograph (MPFS) + CCD (resolution 4Å) within 4000–7000ÅÅ and S/N=50–100 (1995–96, 270 spectra).
- Type
- Part III. Black Holes and Central Activity
- Information
- Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 467 - 468
- Copyright
- Copyright © Kluwer 1998
References
Bochkarev, N.G., Shapovalova, A.I., Nazarova, L.S., 1996, Astron. Astrophys. Trans.
10,241.Google Scholar
Shapovalova, A.I., Burenkov, A.N., Bochkarev, N.G., 1996, Bul. Spec. Astrophys. Obs.
41,28.Google Scholar
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