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R. Coziol

Researcher at Universidad de Guanajuato

Publications -  15
Citations -  244

R. Coziol is an academic researcher from Universidad de Guanajuato. The author has contributed to research in topics: Star formation & Stars. The author has an hindex of 5, co-authored 15 publications receiving 242 citations.

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Journal ArticleDOI

AGN population in Hickson's Compact Groups. I. Data and Nuclear Activity Classification

TL;DR: In this paper, the authors conducted a new spectroscopic survey to characterize the nature of nuclear activity in Hickson Compact Groups (HCGs) galaxies and establish its frequency, and they found a large fraction of galaxies, 63%, with emission lines.
Book ChapterDOI

A Search for Giant Radio Galaxy Candidates and Their Radio-Optical Follow-up

TL;DR: In this article, a computer algorithm was designed to identify contiguous emission regions, large and elongated enough to serve as GRG candidates, and applied it to the entire 1.4GHz NRAO VLA Sky survey (NVSS) image atlas.
Journal ArticleDOI

Agn population in hickson compact groups. i. data and nuclear activity classification

TL;DR: In this paper, the authors conducted a new spectroscopic survey to characterize the nature of nuclear activity in Hickson compact group (HCG) galaxies and establish its frequency, and obtained new intermediate-resolution optical spectroscopy for 200 member galaxies and corrected for underlying stellar population contamination.
Book ChapterDOI

A Semi-automatic Search for Giant Radio Galaxy Candidates and their Radio-Optical Follow-up

TL;DR: In this paper, the authors presented results of a search for giant radio galaxies (GRGs) with a projected largest linear size in excess of 1 Mpc, and designed a computational algorithm to identify contiguous emission regions, large and elongated enough to serve as GRG candidates.
Journal ArticleDOI

Comparative study of asymmetry origin of galaxies in different environments. i. optical observations

TL;DR: In this article, the influence of environment on the formation and evolution of galaxies observed in the nearby universe was analyzed using both characteristic isophotal parameters and evidence of asymmetries in the optical and the near-infrared.