J/A+AS/87/1 J/A+AS/87/1 RATAN-600 7.6 cm catalog of radio sources Yu N Parijskij N N Bursov N M Lipovka N S Soboleva A V Temirova Astron. Astrophys. Suppl. Ser. 87 1 1991 1991A&AS...87....1P VIII/33 : Spectral characteristics of RATAN Catalog (Bursov et al., =1989SoSAO..63...50B) J/A+AS/106/119 : Larionov et al., 1994, "A 3.9 GHz survey for declination -1 to 0deg" Radio sources catalogs radio sources: general radio sources: spectra A catalog containing 840 radio sources obtained during the Experiment Cold-80 at 7.6 cm wavelength using RATAN-600 are presented. The completeness of the list in the central zone is about 0.7-0.8 for sources with flux density 7.5-15 mJy. For sources brighter than 15 mJy the completeness reaches one. The number of sources-flux density differential curve is constructed.

Name Name of Source: RC, J2000-based position; "t" stands for "twin" objects --- RAh right ascension (2000) h RAm right ascension (2000) min RAs right ascension (2000) s DE- declination sign --- DEd declination (2000) deg DEm declination (2000) arcmin DEs declination (2000) arcsec RAh1950 right ascension (1950) h RAm1950 right ascension (1950) min RAs1950 right ascension (1950) s e_RAs rms error on RA s DEd1950 declination (1950) deg DEm1950 declination (1950) arcmin DEs1950 declination (1950) arcsec e_DEs rms error on DE arcsec l_S7.6 Limit flag (>) on S7.6 --- S7.6 Flux density at wavelength of 7.6cm (3.95GHz) mJy e_S7.6 Flux density error in percent % S31 Flux density at wavelength of 31cm (0.97GHz) mJy e_S31 Flux density error in percent % Delta_h The deviation in elevation (Delta h) of the source position from the electrical axis of radio telescope in arcmin. arcmin Rem Remarks number=1 Sources marked with "D" were identified with objects of the 365 MHz (delta= 5deg +/-2deg) survey made at the University of Texas Radio Astronomy Observatory. Sources marked by "i" were identified by us with catalogued optical objects (galaxies, quasars, clusters of galaxies). Sources marked by "VLA" were observed with the Very Large Array The position and/or flux density of sources marked with asterisks may have larger errors than those shown. --- l_SpInd '<' for lower limit of SpInd, 'C' for curved spectrum. --- SpInd Spectral index. (S prop.to. nu**(-SpInd)) --- Joseph Florsch CDS 1993Jun14 UNKNOWN UNKNOWN * The catalogue was received on diskette in January 1993 at CDS; it was documented by Joseph Florsch [CDS] in June 1993. * The documentation was standardized in December 1995 J_A+AS_87_1.xml