A. V. Temirova
Special Astrophysical Observatory
16 Papers
14 Citations
A. V. Temirova is an academic researcher from Special Astrophysical Observatory. The author has contributed to research in topics: Radio galaxy & Redshift. The author has an hindex of 4, co-authored 16 publications. Previous affiliations of A. V. Temirova include Russian Academy of Sciences.
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Papers
Ratan-600-vla-BTA-6m ('big trio') project: Multicolor study of distant frii radio galaxies
Yu. N. Parijskij,W. M. Goss,Alexander I. Kopylov,N. S. Soboleva,A. V. Temirova,O. V. Verkhodanov,Olga P. Zhelenkova +6 more
TL;DR: In this article, the authors used multicolor CCD photometry in B, V, R c, I c bands to estimate the photometric redshift and the age of 50 FRII and CSS radio galaxies.
On the photometric redshift estimates for FR II radio galaxies
TL;DR: Using the photometric data on FR II radio galaxies obtained during the Big Trio program and data from other sources, this article confirmed the stable correlation between the spectroscopic and photometric redshifts up to z ∼ 4, determined from the evolutionary synthetic spectra of elliptical galaxies.
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Spectroscopy of RC Sources
V. L. Afanas'ev,S. N. Dodonov,Alexei Moiseev,O. V. Verkhodanov,A. I. Kopylov,Yu. N. Pariiskii,N. S. Soboleva,A. V. Temirova,Olga P. Zhelenkova,W. M. Goss +9 more
TL;DR: The results of spectroscopic observations of the host galaxies of objects in the RC catalog (the Big Trio program) obtained using the new SCORPIO spectrograph of the Special Astrophysical Observatory are presented in this article.
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Deep RATAN-600 Surveys at the Declination of SS433 Carried Out in 1987-2000 at 7.6 and 2.7 cm
N. S. Soboleva,A. V. Temirova,N. N. Bursov,Yu. K. Zverev +3 more
- 01 Aug 2006
TL;DR: In this paper, the results of deep surveys of a ±10′ strip of the sky, centered on the declination of SS 433, carried out on the Northern sector of the RATAN-600 telescope at 2.7 and 7.6 cm in 1987-2000 were discussed.
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Results of investigation of radio galaxies of the survey "Cold": photometry, colour redshifts and the age of the stellar population
Oleg V. Verkhodanov,Yu. N. Parijskij,N. S. Soboleva,A. I. Kopylov,A. V. Temirova,Olga P. Zhelenkova,W. M. Goss +6 more
TL;DR: In this article, BVRI data for the majority of the objects of the RC catalogue with steep spectra and $m_R<24^m$ are presented. But the age estimates are less confident, however, the lower age limit for not too distant (<1.5$) objects is determined quite reliably.
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