VII/14           Galactic Supernova Remnants Catalogue             (Clark+ 1976)

Galactic Supernova Remnants Catalogue Clark D.H., Caswell J.L. <Mon. Not. Roy. Astron. Soc., 174, 267 (1976)> =1976MNRAS.174..267C 1976MNRAS.174..267C
ADC_Keywords: Supernova remnants; Radio sources Description: The catalog contains observations for southern galactic supernova remnants (SNRs). The observations were made at 408MHz with the one-mile cross-type radio telescope at the Molonglo radio observatory between 1969 December and 1971 June and were made at 5000MHz with the Parkes 64-m radio telescope between 1968 May and 1973 April. The catalog has two files (two tables in published version). The first file lists the 97 known SNRs south of declination +18° (i.e., within the scope of the Molonglo survey and gives Molonglo and Parkes observational data where available). For completeness the 23 known SNRs north of declination +18° are listed in a second file. The catalog includes identifications, the 408-MHz integrated flux densities, mean angular diameters, and surface brightnesses of the SNRs. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file data1.dat 109 97 Southern (Dec < +18 deg) galactic SNRs data2.dat 123 23 Northern (Dec > +18 deg) galactic SNRs -------------------------------------------------------------------------------- See also: VII/15 : Galactic Supernova Remnants Catalog (Ilovaisky+ 1972) VII/227 : A Catalogue of Galactic Supernova Remnants (Green 2001) Byte-by-byte Description of file: data1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- SNR Galactic source number 12- 29 A18 --- Alt Other catalogue number or name 30 A1 --- n_S(408) [(*> ] Flux density flag 1 (G1) 31- 36 F6.1 Jy S(408) ?=- Integrated flux density estimate at 408MHz 37 A1 --- n_S(408)b [) *] Flux density flag 2 (G1) 39 A1 --- n_S(5000) [( *] Flux density flag 3 (G1) 40- 44 F5.1 Jy S(5000) ?=- Integrated flux density at 5000MHz 45 A1 --- n_S(5000)b [) *] Flux density flag 4 (G1) 47 A1 --- n_SI [( ] Spectral Index flag 1 (G2) 48- 52 F5.2 --- SI ? Spectral index between 408/5000 MHz (G3) 53 A1 --- n_SIb [ )] Spectral Index flag 2 (G2) 55 A1 --- l_AngDiam [< >] " < " or " > " where applicable (1) 56- 60 F5.1 arcmin AngDiam ?=- Angular diameter of remnant 63- 71 E9.3 W/m2/sr/Hz B(408) ?Surface brightness at 408 MHz 72- 86 A15 --- r_S(408) Original reference to 408MHz flux density (2) 90- 97 A8 --- r_S(5000) Original reference to 5000 MHz flux density 99-109 A11 --- MapRef Map reference (where possible Molonglo maps) -------------------------------------------------------------------------------- Note (1): "<" or ">" mean less or larger than the size of the angular diameter of remnant. Note (2): "revised" implies a reassessment of the earlier Molonglo data by the authors. -------------------------------------------------------------------------------- Byte-by-byte Description of file: data2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- SNR Galactic source number 12- 29 A18 --- Alt Other catalogue number or name 30 A1 --- n_S(408) [( *] Flux density flag 1 (G1) 31- 36 F6.1 Jy S(408) ? Integrated flux density estimate at 408MHz 37 A1 --- n_S(408)b [* )] Flux density flag 2 (G1) 39 A1 --- n_S(5000) [( *] Flux density flag 3 (G1) 40- 44 F5.1 Jy S(5000) ?Integrated flux density at 5000 MHz 45 A1 --- n_S(5000)b [) *] Flux density flag 4 (G1) 47 A1 --- n_SI [( ] Spectral Index flag 1 (G2) 48- 52 F5.2 --- SI ? Spectral index between 408/5000MHz, S(alpha)v(alpha) (G3) 53 A1 --- n_SIb [ )] Spectral Index flag 2 (G2) 55 A1 --- l_AngDiam [< >] " < " or " > " where applicable 56- 60 F5.1 arcmin AngDiam Angular diameter of remnant 63- 71 E9.3 W/m2/sr/Hz B(408) Surface brightness at 408 MHz 72- 87 A16 --- RefList List of references to recent data (1) 90- 97 A8 --- r_SI Reference for spectral index information 100-110 A11 --- MapRef Map reference of the source (2) 113-116 I4 MHz Freq1 Lower value of alpha 118-123 I6 MHz Freq2 Upper value of alpha -------------------------------------------------------------------------------- Note (1): List of references to recent observational data for each source Note (2): Map reference of the source with brightest resolution available -------------------------------------------------------------------------------- Global Notes: Note (G1): Flag as follows: ( = Flux densities are estimates as obtained by Shaver and Goss from fitting Gaussians to the individual source brightness distributions (1970 Aust. J. Phys. Astrophys. Suppl. No. 14, 133). ) = Same as above. * = estimated flux density is not obtained from the Molonglo pencil-beam survey. Note (G2): The notes in n_SI mean the following: ( = data other than at 408 and 5000MHz were used to compute the spectral index between 408 and 5000 MHz. ) = Same as above. Note (G3): SI is the spectral index for those sources with flux density estimates available at the two frequencies. -------------------------------------------------------------------------------- Remarks and Modifications: This galactic supernova remnant catalogue was made machine-readable at the Goddard Space Flight Center. The data is from the paper "A study of Galactic Supernova Remnants, Based on Molonglo-Parkes Observational Data" by D. H. Clark and J. L. Caswell (Mon. Not. Royal Astronomical Society, 1976, 174, 267-305 = 1976MNRAS.174..267C 1976MNRAS.174..267C). Acknowledgements: The original ADC documentation by Theresa A. Nagy (1979) was used to generate this ReadMe file.
(End) C.-H. Joseph Lyu [Hughes STX/NASA] 08-Apr-1996
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