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Radio identification of decametric sources. I. Catalogue.
O.V. Verkhodanov, H. Andernach, N.V. Verkhodanova.
Bulletin SAO No.49, pp. 53-100, 2000.
7 tables, 2316 objects.
The new list from UTR13 identifications is
here
Abstract
We describe a method of plotting continuous spectra for radio sources
on the basis of entries of various source catalogues in comparatively
large error boxes around a given sky position. Sources from the
UTR-2 catalogue (Braude et al.,
1978, 1979, 1981, 1985, 1994), observed
at decametric wavelengths (10-25 MHz) with an antenna beam of about 40',
were cross-identified with entries from other radio catalogues at higher
frequencies. Using the CATS database we extracted all sources within 40'
around UTR positions to find candidate identifications. The spectrum for
each source was fitted with a set of curves using the least squares method
to find the best fit. We preferentially selected radio counterparts whose
radio spectrum extrapolated to low frequencies matched the UTR decametric
flux densities, and whose coordinates
were close to the gravity centre of UTR positions. Among all 1822
sources in the UTR catalogue we found about 350 sources to be blends of
two or more sources. As the most probable true coordinates of the radio
counterparts we used positions from the FIRST, NVSS, TXS, GB6, or
PMN catalogues. Using low-frequency sources (26, 38, 85 MHz) from CATS
we checked the reliability of some of our identifications. We show examples
of the above methods, including raw and "cleaned" spectra.
Identifications with objects from optical, X-ray and infrared
catalogues, as well as a subsample of UTR sources with ultra-steep
spectrum are presented.
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