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VIII/41        The UTR-2 Very Low-Frequency Sky Survey Data  (Braude+ 1978-1982)

The UTR-2 Very Low-Frequency Sky Survey Data Decametric survey of discrete sources in the northern sky. II. Source catalogue in the range of declinations +10 to +20 Braude S.Ya., Megn A.V., Rashokovski S.L., Ryabov B.P., Sharykin N.K., Sokolov K.P., Tkatchenko A.P., Zhouk I.N. <Astrophys. Space Sci., 54, 37 (1978)> =1978Ap&SS..54...37B Decametric survey of discrete sources in the northern sky. V. Source catalogue in the range of declinations 0 to +10. Braude S.Ya., Megn A.V., Sokolov K.P., Tkatchenko A.P., Sharykin N.K. <Astrophys. Space Sci., 64, 73 (1979)> =1979Ap&SS..64...73B Decametric survey of discrete sources. VII. Source catalogue in the range of declination -2 to -13. Braude S.Ya., Miroshnitchenko A.P., Sokolov K.P., Sharykin N.K. <Astrophys. Space Sci., 74, 409 (1981)> =1981Ap&SS..74..409B Decametric survey of discrete sources in the northern sky. IX. Source catalogue in the declination range 52 to 60. Braude S.Ya., Sharykin N.K., Sokolov K.P., Zakcharenko S.M. <Astrophys. Space Sci., 111, 1 (1985)> =1985Ap&SS.111....1B Decametric survey of discrete sources in the northern sky. XI. The results of the UTR-2 very low-frequency sky survey in the declination range 41 deg. to 52 Braude S.Ya., Sokolov K.P., Zakcharenko S.M. <Astrophys. Space Sci., 213, 1 (1994)> =1994Ap&SS.213....1B
ADC_Keywords: Radio sources Description: The results of the very-low frequency (16.7MHz) survey of discrete sources made with the UTR-2 radio telescope is presented. The survey concerns the declination zones -13° to -2°, 0° to 20°, and 41° to 60°. The UTR-2 radio source catalogue contains an estimate of the coordinates and flux densities of 1819 sources measured at a number of the lowest frequencies used in contemporary radio astronomy within the range from 10 to 25 MHz. The catalogue is made of two parts: mean.dat: the averaged values of the coordinates and the corresponding errors, the source flux-density at the middle UTR-2 frequency 16.7 MHz as obtained from measured spectrum of the source at all UTR-2 frequencies and its error, the value of measured low-frequency spectral index with respect to which the estimate of has been obtained, the parameter W characterizing the integral reliability of the obtained source estimates and the corresponding object name from higher-frequency radio survey provided the source has been identified. To indicate the integral readability of the source parameters obtained we used the symbols A, B and C. These reliability estimates take into account the total number of measurements, coordinate scatter, number of frequencies and hour-angle settings at which the source parameters have been evaluated. The highly reliable observation results have been marked with symbol A . The sources whose parameters can be used without an additional analysis are marked with B and sources whose parameters are to be used with care have been marked with C. data.dat: this file contains the experimental estimates of the source coordinates and flux densities as well as their errors at each operating frequency of the UTR-2 in the order of their increasing; the total number (N) of successive observations according to which the estimates were obtained and the number of different hour-angle settings (NRA) of the reception pattern at which the source was observed. In cases when the observations did not allow us to obtain a reliable estimates of a source flux density the catalogue contains only their upper limits which are not accompanied by errors. The approximated values of as well as low-frequency spectral indices are presented only for those sources which have flux density estimates obtained at not less than three different UTR-2 frequencies. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file mean.dat 112 1819 Averaged values and cross-identifications data.dat 59 8094 Experimental estimates at each operating frequency of the UTR-2
Byte-by-byte Description of file: mean.dat
Bytes Format Units Label Explanations
1- 13 A13 --- Name *Source name (individual data in file data.dat) 15- 16 I2 h RAh Right ascension (1950) 18- 19 I2 min RAm Right ascension (1950) 21- 22 I2 s RAs Right ascension (1950) 24- 26 I3 s e_RAs rms uncertainty on RAs 28- 33 F6.2 deg DEdeg Declination (1950) 35- 39 F5.2 deg e_DEdeg rms uncertainty on DEdeg 41- 44 F4.1 MHz Freq ? Frequency 46 A1 --- l_S Limit flag on fLux density 47- 50 I4 Jy S ? Flux-density at frequency Freq 52- 54 I3 % e_S ? rms uncertainty on flux density 62- 65 F4.1 --- SI ? Low-frequency spectral index 67- 69 F3.1 --- e_SI ? rms uncertainty on SI 71 A1 --- W *[ABC] Integrated estimate of reliability 74-112 A39 --- OtherName Other names
Note on Name: the name includes the publication number (2,5,7,9,11), "GRB" (the B indicates that 1950 positions are used in the name). hours and minutes of RA(1950), and degrees of Declination(1950). Up to 6 lines in file data.dat contain the experimental estimates of the source coordinates and flux densities as well as their errors at each operating frequency of the UTR-2. Note on W: the reliability index takes the values: A: Highly reliable data B: Results that can be used without an additional analysis C: Data requiring additional analysis, up to an examination of the original analogue records
Byte-by-byte Description of file: data.dat
Bytes Format Units Label Explanations
1- 13 A13 --- Name *Source name, as in file mean.dat 15- 16 I2 h RAh Right ascension (1950) 18- 19 I2 min RAm Right ascension (1950) 21- 22 I2 s RAs Right ascension (1950) 24- 26 I3 s e_RAs rms uncertainty on RAs 28- 33 F6.2 deg DEdeg Declination (1950) 35- 39 F5.2 deg e_DEdeg rms uncertainty on DEdeg 41- 44 F4.1 MHz Freq Frequency 46 A1 --- l_S Limit flag on fLux density 47- 50 I4 Jy S Flux-density at frequency Freq 52- 54 I3 % e_S ? rms uncertainty on flux density 56- 57 I2 --- N Total number of successful measurements 59 I1 --- NRA Number of angular positions on RA of the reception pattern at which the source was observed
Note on Name: the name includes the publication number (2,5,7,9,11), "GRB" (the B indicates that 1950 positions are used in the name). hours and minutes of RA(1950), and degrees of Declination(1950). Up to 6 lines in file data.dat contain the experimental estimates of the source coordinates and flux densities as well as their errors at each operating frequency of the UTR-2.
Acknowledgements: For any information concerning to the UTR-2 Very Low-Frequency Sky Survey, please, contact to: Dr. K.P. Sokolov Institute of Rsdio Astronomy 4, Krasnoznamennaya Street Kharkov 310002 UKRAINE E-mail:rai@ira.kharkov.ua FAX: 38 (0572) 47-65-06 Phone: 38 (0572) 45-10-14 (office), 38 0572-44-09-37 (home) References: Braude S.Ya. et al., Paper I., The UTR-2 Radio Telescope. Experimental Techniques and Data Processing =1978Ap&SS..54....3B Braude S.Ya. et al., Paper II., 10° < DE < 20° =1978Ap&SS..54...37B Braude S.Ya. et al., Paper IV., Spectra =1978Ap&SS..54..145B Braude S.Ya. et al., Paper V., 0° < DE < 10° =1979Ap&SS..64...73B Braude S.Ya. et al., Paper VI., Spectra =1979Ap&SS..64..127B Braude S.Ya. et al., Paper VII., -2°< DE ←13° =1981Ap&SS..74..409B Braude S.Ya. et al., Paper VIII., Spectra =1981Ap&SS..76..279B Braude S.Ya. et al., Paper IX., 52° < DE < 60° =1985Ap&SS.111....1B Braude S.Ya. et al., Paper X., Spectra =1985Ap&SS.111..237B Braude S.Ya. et al., Paper XI., 41° < DE < 52° =1994Ap&SS.213....1B Braude S.Ya. et al., Paper XII., Spectra =1995Ap&SS.226..245B
(End) K.P. Sokolov [Ukrainia], Francois Ochsenbein [CDS] 15-Sep-1997
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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