Abstract
Abstract: * Aims. Identify optical counterparts, address uncertain identifications and measure previously unknown redshifts of the host galaxies of candidate GPS radio sources, and study their stellar populations. * Methods. Long slit spectroscopy and deep optical imaging in the B, V and R bands, obtained with the Very Large Telescope. * Results. We obtain new redshifts for B0316+161, B0407-658, B0904+039, B1433-040, and identify the optical counterparts of B0008-421 and B0742+103. We confirm the previous identification for B0316+161, B0407-658, B0554-026, and B0904+039, and find that the previous identification for B0914+114 is incorrect. Using updated published radio spectral information we classify as non GPS the following sources: B0407-658, B0437-454, B1648+015. The optical colors of typical GPS sources are consistent with single instantaneous burst stellar population models but do not yield useful information on age or metallicity. A new master list of GPS sources is presented.
Original language | English |
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Pages (from-to) | 97-U10 |
Number of pages | 10 |
Journal | Astronomy & Astrophysics |
Volume | 463 |
Issue number | 1 |
DOIs | |
Publication status | Published - 3-Feb-2007 |
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Optical observations of GPS radio sources
Labiano, A. (Contributor), Barthel, P. (Contributor), O'Dea, C. P. (Contributor), De Vries, W. H. (Contributor), Pérez, I. (Contributor) & Baum, S. A. (Contributor), University of Groningen, 9-Mar-2007
DOI: 10.26093/cds/vizier.34630097
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