/ftp/cats/VIII/104



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VIII/104   SPECFIND V3.0 Catalog of radio continuum spectra       (Stein+, 2021)
The following files can be converted to FITS (extension .fit or fit.gz)
	spectra.dat waste.dat beam.dat ghzbreak_cand.dat mhzbreak_cand.dat
	figa2.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=VIII/104
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Beginning of ReadMe : VIII/104 SPECFIND V3.0 Catalog of radio continuum spectra (Stein+, 2021) ================================================================================ The SPECFIND V3.0 catalog of radio continuum cross-identifications and spectra: Reaching lower frequencies. Stein Y., Vollmer B., Boch T., Landais G., Vannier P., Brouty M., Allen M.G., Derriere S., Ocvirk P. <Astron. Astrophys., 655, A17 (2021)> =2021A&A...655A..17S =2020yCat.8104....0S ================================================================================ ADC_Keywords: Radio sources ; Galaxies, radio ; Radio continuum Keywords: catalogs - radio continuum: general - astronomical data bases: miscellaneous Abstract: Many radio continuum catalogs with different sensitivity limits and spatial resolutions are published via the VizieR database. Because of the diversity of spatial resolution, the cross-identification of individual sources is complex. By assuming a power-law spectrum, the SPECFIND tool is able to handle radio surveys at different frequencies from different instruments and different resolutions. Since the former version of the SPECFIND catalog was released ten years ago, hundreds of new radio continuum catalogs have been published. We upgraded the SPECFIND tool to reach a wider frequency range, especially the lower-frequency radio regime, as well as to have better spatial sky coverage. We adapted special selection criteria to all radio tables listed in VizieR to define a final sample of new catalogs. We implemented the new catalogs into the SPECFIND tool by unifying them and then compare the results to the last version. Furthermore we present and investigate sources with spectral breaks around 1.4GHz and around 325MHz. By increasing the number of implemented SPECFIND catalogs from 115 to 204, we improve the number of resulting spectra from 107500 to 340000 and increase the number of cross-identified sources from 600000 to 1.6 million. Furthermore, we present two samples of spectral break sources. The first sample includes 3104 spectral break sources with turnover frequencies around 1.4GHz, the second sample includes 18075 spectral break sources with turnover frequencies around 325MHz. Both samples include concave sources and Gigaherz-Peaked Spectrum (GPS) or Megaherz-Peaked Spectrum (MPS) sources. The SPECFIND V3.0 catalog is a very useful resource and a powerful open access tool, reachable via VizieR. By tripling the resulting spectra and including many radio continuum surveys from the last 50 years, we provide a significantly extended catalog of cross-identified radio continuum sources. Furthermore, the SIMBAD database will be updated using the SPECFIND V3.0 catalog and will contain more radio continuum data, serving the needs of future projects. Description: We present a new version of SPECFIND. The SPECFIND tool was successfully upgraded from 115 catalogs in version 2.0 to version 3.0 with a final number of 204 processed catalogs. 89 new catalogs were ingested and two catalogs were updated. The final number of resulting spectra was increased more than a factor of three from 107500 in version 2.0 to 340000 in version 3.0. The number of objects with cross-identified sources was more than doubled from 600000 in version 2.0 to 1.6 million in version 3.0. The main result is presented in table "spectra" with every radio continuum source having one entry row. The different objects/spectra are named by different sequence numbers (column "Seq"). All radio continuum sources with the same sequence number belong to the same object/spectrum. In the second column, the name of the source is given followed by the number of sources within the spectrum ("N"). The columns "a" and "b" are the spectral index and the abscissa of the spectral fit, respectively. The sixth column contains the frequency of the catalog, followed by the flux density, its error and the position of the source (Right Ascension and Declination). The column "SED" is a link to the spectral fit, i.e. the spectrum containing this source. The next column "Aladin" shows an Aladin Lite6 view of the source. The last column gives the beam size of the observation. The "beam" table contains all 204 tables from the VizieR catalogs which were used in SPECFIND V3.0. The "waste" table has the same general structure as "spectra", but contains measurements which were cross-identified by position but did not match the power-law spectrum. These points are added to the VizieR SED plot. The spectral break sources are provided in two different tables. The first table contains all 5515 spectral break sources including the 210 concave sources with turnover frequencies around 1.4GHz. The second table lists the 19691 spectral break sources including the 900 concave sources with turnover frequencies around 325MHz. The structure of the tables is similar to the spectra table. The first column gives the running number "Seq". The sources belonging to the same spectrum have the same sequence number. The second column provides the source name; the third column the type (spectral break (sb), concave (conc), GPS/MPS (gps/mps), GGPS/GMPS (ggps/gmps)), followed by the spectral slope and the abscissa associated with the source. In the next column, the mean spectral slope of the part of the spectrum (lower or higher frequency part) is given. Then the frequency, the flux density and its error are listed. Lastly, the position (Right Ascension and Declination) and the beam/resolution are specified.