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Toward Monitoring of Blazars at Abastumani: Progress Report
Published online by Cambridge University Press: 13 May 2016
Abstract
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We present a brief summary of the ongoing Abastumani Blazar Monitoring Program started in the May of 1997. More than 50 000 frames have been collected during 498 observing nights for about 50 blazars.
- Type
- The Inner Regions of Galaxies
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 2001
References
Kurtanidze, O.M., Nikolashvili, M.G., Takalo, L.O., 1998, in: Tosti, G., Takalo, L., (eds.) Proc. OJ-94 Annual Meeting 1997, Multifrequency Monitoring of Blazars. Publ. Osservatorio Astron. Università di Perugia, Perugia, Vol. 3, p. 193.Google Scholar
Kurtanidze, O.M., Richter, G.M., Nikolashvili, M.G., 1999, in: Raiteri, C.M., Villata, M. & Takalo, L.O. (eds.) Proc. OJ-94 Annual Meeting 1999, Blasar monitoring towards the third millennium. Publ. Osservatorio Astron. di Torino, p.29.Google Scholar
Nikolashvili, M.G., Kurtanidze, O.M., Richter, G.M., 1999a, in: Raiteri, C.M., Villata, M. & Takalo, L.O (eds.) Proc. OJ-94 Annual Meeting 1999, Blasar monitoring towards the third millennium. Publ. Osservatorio Astron. di Torino, p.36.Google Scholar
Nikolashvili, M.G., Kurtanidze, O.M., Richter, G.M., 1999b, in: Raiteri, C.M., Villata, M. & Takalo, L.O (eds.) Proc. OJ-94 Annual Meeting 1999, Blasar monitoring towards the third millennium. Publ. Osservatorio Astron. di Torino, p.33.Google Scholar
Smith, A., 1996, in: Miller, R., Webb, J., Noble, J., (eds.) Blazar Continuum Variability, 3.Google Scholar
Takalo, L.O., Silanpää, A., Kidger, M., 1994, in: Kidger, M., Takalo, L.O. (eds.), Workshop on Intensive Monitoring of OJ 287. Tuorla Observatory reports no. 174, 3.Google Scholar
Véron-Cetty, M.-P., Véron, P., 1993, A Catalogue of Quasars and Active Nuclei
(6th Edition). ESO Scientific Report 13.Google Scholar
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