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Publikováno v:
2012ARep...56..336P
Published data from long-term observations of a strip of sky at declination +5 degrees carried out at 7.6 cm on the RATAN-600 radio telescope are used to estimate some statistical properties of radio sources. Limits on the sensitivity of the survey d
Externí odkaz:
http://arxiv.org/abs/1205.5178
Publikováno v:
Astrophysical Bulletin, Vol 65, N 1, pp.42-59, 2010
We use two independent methods to reduce the data of the surveys made with RATAN-600 radio telescope at 7.6 cm in 1988-1999 at the declination of the SS433 source. We also reprocess the data of the "Cold" survey (1980-1981). The resulting RCR (RATAN
Externí odkaz:
http://arxiv.org/abs/1003.0829
Autor:
Kopylov, A. I., Goss, W. M., Pariiskii, Yu. N., Soboleva, N. S., Verkhodanov, O. V., Temirova, A. V., Zhelenkova, O. P.
Publikováno v:
Astron.Lett.32:433-438,2006
A strong emission line at 6703A has been detected in the optical spectrum for the host galaxy (R=23.1) of the radio source RC J0311+0507 (4C+04.11). This radio galaxy, with a spectral index of 1.31 in the frequency range 365-4850 MHz, is one of the u
Externí odkaz:
http://arxiv.org/abs/0705.2971
Publikováno v:
Astron.Lett.31:219-224,2005
Using the photometric data on FR II radio galaxies obtained in the Big Trio Program and data from other sources, we confirmed the stable correlation between the spectroscopic and photometric redshifts up to z~4 determined from the evolutionary synthe
Externí odkaz:
http://arxiv.org/abs/0705.3046
Autor:
Abramov-Maximov, V. E., Arshakian, T. G., Bogod, V. M., Borovik, V. N., Burenkov, A. N., Bursov, N. N., Doroshenko, V. T., Efimov, Yu. S., Fabrika, S. N., Golubchina, O. A., Gorshkov, A. G., Gosachinskij, I. V., Harinov, M., Hovatta, T., Kaltman, T. I., Korzhavin, A. N., Kotelnikov, V., Kovalev, Yu. A., Kouprianova, E. G., Lahteenmaki, A., Lehto, H. J., Mingaliev, M. G., Modin, E. V., Nieppola, E., Parijskij, Yu. N., Riehokainen, A., Soboleva, N. S., Stepanov, A. V., Tlatov, A. G., Torniainen, I., Tornikoski, M., Trushkin, S. A., Valtaoja, E., Verkhodanov, O. V., Volvach, A. E., Zinchenko, I. I.
The IX Russian-Finnish Symposium on Radio Astronomy was held in Special astrophysical observatory RAS in Nizhnij Arkhyz, Russia on 15-20 October 2006. It was dedicated to the two-side collaboration in the field of multi-wavelength investigations of s
Externí odkaz:
http://arxiv.org/abs/astro-ph/0612153
Autor:
Verkhodanov, O. V., Parijskij, Yu. N., Soboleva, N. S., Kopylov, A. I., Temirova, A. V., Zhelenkova, O. P., Goss, W. M.
BVRI data for the majority of the objects of the RC catalogue with steep spectra and $m_R<24^m$ are presented. These data have been used to estimate colour redshifts and the age of stellar systems of host galaxies. By way of example of distant radio
Externí odkaz:
http://arxiv.org/abs/astro-ph/0203522
Autor:
Verkhodanov, O. V., Parijskij, Yu. N., Soboleva, N. S., Kopylov, A. I., Temirova, A. V., Zhelenkova, O. P., Goss, W. M.
About 100 steep spectrum radio sources from the RATAN--600 RC catalog were mapped by the VLA and identified with optical objects down to 24$^m$--25$^m$ in the R band using the 6 m telescope. An updated list of calibrators with known redshifts of the
Externí odkaz:
http://arxiv.org/abs/astro-ph/0112144
Autor:
Verkhodanov, O. V., Kopylov, A. I., Verkhodanova, N. V., Zhelenkova, O. P., Chernenkov, V. N., Parijskij, Yu. N., Soboleva, N. S., Temirova, A. V.
The system allowing a user to operate with simulated curves of spectral energy distribution (SED) and to estimate ages and redshifts by photometric data at server {\bf sed.sao.ru} is described.
Comment: 2 pages, uses newpasp.sty. To appear in Pr
Comment: 2 pages, uses newpasp.sty. To appear in Pr
Externí odkaz:
http://arxiv.org/abs/astro-ph/0112142
Autor:
Parijskij, Yu. N., Goss, W. M., Kopylov, A. I., Soboleva, N. S., Temirova, A. V., Verkhodanov, O. V., Zhelenkova, O. P.
Powerful radio galaxies belong to the population of massive stellar systems that can be picked at high redshifts. With measured redshift, morphology and age determination these objects can help greatly in understanding of the way of formation and evo
Externí odkaz:
http://arxiv.org/abs/astro-ph/0005240