Alexander I. Kopylov
Russian Academy of Sciences
111 Papers
389 Citations
Alexander I. Kopylov is an academic researcher from Russian Academy of Sciences. The author has contributed to research in topics: Galaxy & Galaxy cluster. The author has an hindex of 13, co-authored 102 publications.
Chat about Author
Papers
Photometric Study of Radio Galaxies in the RATAN-600 “Cold” Survey
O. V. Verkhodanov,Yurij N. Parijskij,N. S. Soboleva,Alexander I. Kopylov,A. V. Temirova,Olga P. Zhelenkova,W. M. Goss +6 more
- 01 Jan 2002
Abstract: 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 same class RGs was compiled to evaluate the accuracy of photometric redshifts estimates. BVRI photometry for 60 RC objects was performed with the 6 m telescope, and by standard model fitting we have estimated colour redshifts and ages of stellar population of host gE galaxies. The mean redshift of FRII RGs from the RC list happened to be $\approx$1. Several objects were found in which active star formation began in the first billion years after the Big Bang.
•Posted Content
Redshifts and age of stellar systems of distant radio galaxies from multicolour photometry data
TL;DR: In this article, a possibility has been investigated of using two evolutionary models of stellar systems (PEGASE and Poggianti) to evaluate readshifts and ages of stellar system in these galaxies.
Quenched Galaxies in Clusters of Galaxies and Their Outskirts
TL;DR: The properties of galaxies with quenched star formation (QGs) within the splashback radius of galaxy clusters Rsp and beyond it have been studied in this paper based on the SDSS catalog data.
Evolution of galaxy groups
TL;DR: In this paper, the authors studied the variations of the properties of groups of galaxies with dynamical masses of 1013m, and found that the fraction of early-type galaxies in the considered systems is equal, on average, to 0.65 ± 0.01, and varies significantly for galaxies with σ200 < 300 kms−1.