Quasi-simultaneous multi-frequency observations of inverted-spectrum GPS candidate sources
arXiv:0806.3694 · doi:10.1051/0004-6361:20078857
Abstract
Gigahertz-Peaked Spectrum (GPS) sources are probably the precursors of local radio galaxies.Existing GPS source samples are small (<200). It is necessary to extend the availabe sample of the Gigahertz-Peaked Spectrum (GPS) and High Frequency Peaker (HFP) sources in order to study their nature with greater details and higher statistical significance. A sample of 214 radio sources, which were extracted from the SPECFIND catalog and show an inverted radio spectrum, were observed quasi-simultaneously at 4.85, 10.45, and 32GHz with the 100-m Effelsberg radio telescope. Using the VLBA calibrator survey (VCS) we have investigated the parsec-scale morphology of the sources. About 45% of the sources in our sample are classified as GPS or HFP candidates. We add 65 new GPS/HFP candidates to existing samples. We confirm the expected tendency that HFP are more compact on milliarcsecond scale than the 'classical' GPS sources, which peak at lower frequencies. The data mining of the SPECFIND database represents a promising tool for the discovery of new GPS/HFP sources.
16 pages, 7 figures, accepted for publication in A&A
References in corpus (22)
- The SIMBAD astronomical database
- The VizieR database of Astronomical Catalogues
- Sub-milliarcsecond Imaging of Quasars and Active Galactic Nuclei. IV. Fine Scale Structure
- The VLBA Calibrator Survey - VCS1
- A complete sample of GHz-Peaked-Spectrum radio sources and its radio properties
- On the evolution of young radio-loud AGN
- The Third VLBA Calibrator Survey
- The Sixth VLBA Calibrator Survey: VCS6
- The Fifth VLBA Calibrator Survey: VCS5
- The Fourth VLBA Calibrator Survey - VCS4
- The COINS Sample - VLBA Identifications of Compact Symmetric Objects
- Extended emission around GPS radio sources
- A new sample of faint Gigahertz Peaked Spectrum radio sources
- GPS radio sources: new optical observations and an updated master list
- VLBA images of High Frequency Peakers
- EVN observations of candidate Compact Symmetric Objects
- Gigahertz Peaked Spectrum sources from the Jodrell Bank-VLA Astrometric Survey
- Multi-frequency VLBI observations of faint gigahertz peaked spectrum sources
- A method for determining radio continuum spectra, and its application to large surveys
- European VLBI Network observations of fourteen GHz-Peaked-Spectrum radio sources at 5 GHz
- EVN observations of eleven GHz-Peaked-Spectrum radio sources at 2.3/8.4GHz
- The precision of large radio continuum source catalogues- An application of the SPECFIND tool
Cited by in corpus (15)
- Fermi/LAT discovery of gamma-ray emission from a relativistic jet in the narrow-line quasar PMN J0948+0022
- Resonant Absorption of Transverse Oscillations and Associated Heating in a Solar Prominence. II- Numerical aspects
- Resonant Absorption of Transverse Oscillations and Associated Heating in a Solar Prominence. I- Observational aspects
- The Origin of Double-Peaked Narrow Lines in Active Galactic Nuclei I: Very Large Array Detections of Dual AGNs and AGN Outflows
- High--frequency predictions for number counts and spectral properties of extragalactic radio sources. New evidences of a break at mm wavelengths in spectra of bright blazar sources
- Planck early results XIV: ERCSC validation and extreme radio sources
- The SPECFIND V2.0 catalogue of radio cross-identifications and spectra. SPECFIND meets the Virtual Observatory
- Gravitational lensing reveals extreme dust-obscured star formation in quasar host galaxies
- Continuum sources from the THOR survey between 1 and 2 GHz
- Multifrequency study of GHz-peaked spectrum sources
- VLBI-selected sample of Compact Symmetric Object candidates and frequency-dependent position of hotspots
- Planck intermediate results. XVIII The millimetre and sub-millimetre emission from planetary nebulae
- Multifrequency VLBI Observations of the Broad Absorption Line Quasar J1020+4320: Recently Restarted Jet Activity?
- WMAP extragalactic point sources as potential Space VLBI calibrators
- Deep survey of millimeter RRLs towards the planetary nebulae IC 418 and NGC 7027