Detailed Information on Publication Record
2024
Powerful Radio Sources in the Southern Sky. III. First Results of the Optical Spectroscopic Campaign
GARCIA-PEREZ, A., H. A. PENA-HERAZO, A. JIMENEZ-GALLARDO, V. CHAVUSHYAN, F. MASSARO et. al.Basic information
Original name
Powerful Radio Sources in the Southern Sky. III. First Results of the Optical Spectroscopic Campaign
Authors
GARCIA-PEREZ, A., H. A. PENA-HERAZO, A. JIMENEZ-GALLARDO, V. CHAVUSHYAN, F. MASSARO, S. V. WHITE, A. CAPETTI, B. BALMAVERDE, W. R. FORMAN, C. C. CHEUNG, J. P. MADRID, C. MAZZUCCHELLI, N. P. H. NESVADBA, I. ANDRUCHOW, S. CELLONE, Romana GROSSOVÁ (703 Slovakia, belonging to the institution), A. PAGGI, E. SANI, V. REYNALDI, R. P. KRAFT and C. LETO
Edition
Astrophysical Journal, Supplement Series, IOP Publishing Ltd, 2024, 0067-0049
Other information
Language
English
Type of outcome
Článek v odborném periodiku
Field of Study
10308 Astronomy
Country of publisher
United Kingdom of Great Britain and Northern Ireland
Confidentiality degree
není předmětem státního či obchodního tajemství
References:
Impact factor
Impact factor: 8.700 in 2022
Organization unit
Faculty of Science
UT WoS
001161932200001
Keywords in English
Extragalactic radio sources (508)
Tags
Tags
International impact, Reviewed
Změněno: 3/4/2024 13:50, Mgr. Marie Šípková, DiS.
Abstract
V originále
We recently built the G4Jy-3CRE catalog of extragalactic radio sources. This catalog lists 264 powerful radio sources selected with similar criteria to those of the revised Third Cambridge Catalog, but visible from the Southern Hemisphere. A literature search revealed that 119 sources in the G4Jy-3CRE catalog (i.e., 45%) lack a firm spectroscopic redshift measurement. Here, we present a campaign aimed at acquiring optical spectra of G4Jy-3CRE sources and measuring their redshifts. We used single-slit observations obtained with the Victor Blanco Telescope, the New Technology Telescope, the Southern Astrophysical Research Telescope, and the 2.1 m telescope of the Observatorio Astronomico Nacional at San Pedro Martir, Mexico. In addition, we analyzed Very Large Telescope/MUSE archival observations. From these observations, we report the spectra and redshifts of 93 sources, 42 of which are the first optical spectra and redshift determinations for the respective sources. With our new data, approximately 71% of the sources in the G4Jy-3CRE catalog now have firm spectroscopic redshift measurements. This data set will be the basis of our future analysis of the optical properties of the G4Jy-3CRE catalog.