UVR CCD photometry of stars in five sky areas with matched IR/radio sources

Five sky areas about the radio sources ICRS 1254+571, ICRS 1345+125, ICRS 1641+399, ICRS 1732+389, and ICRS 1807+698 were observed with the aim to identify reliably the extragalactic radio sources in these areas with bright infrared objects and objects in the optical range. The test CCD observations...

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Veröffentlicht in:Kinematics and physics of celestial bodies 2007-08, Vol.23 (4), p.147-156
Hauptverfasser: Kharin, A S, Andruk, V N, Bartasiute, S, Butenko, G Z, Vedenicheva, I P, Perekhod, A V, Sergeev, A V
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Sprache:eng
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Zusammenfassung:Five sky areas about the radio sources ICRS 1254+571, ICRS 1345+125, ICRS 1641+399, ICRS 1732+389, and ICRS 1807+698 were observed with the aim to identify reliably the extragalactic radio sources in these areas with bright infrared objects and objects in the optical range. The test CCD observations were made in the U, V, and R bands of the Johnson system with the 2-meter telescope of the Terskol Peak Observatory (North Caucasus, Russian Federation). The U, V, and B magnitudes and the equatorial coordinates α and δ in the USNO-A2.0 catalog system were determined for objects down to V [asymptotically =] 23^sup m^ in 8.5' × 8.5' areas, and these objects were identified with stars and infrared objects in the 2MASS catalog. The CCD image processing realized within the MIDAS/ROMAFOT program package on the basis of a new method for flat-field elimination is briefly described.[PUBLICATION ABSTRACT]
ISSN:0884-5913
1934-8401
DOI:10.3103/S0884591307040022