Astronomical Data Center
ADC/CDS Standard Document for Catalog:
/catalogs/8/8044/
The following is the "ReadMe" document that describes this ADC catalog. You can access the files described here in three ways:
VIII/44 Miyun 232MHz survey (Zhang+ 1997)
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The Miyun 232 MHz survey. II. The main list
Zhang X., Zheng Y., Chen H., Wang S., Cao A., Peng B., Nan R.
<Astron. Astrophys. Suppl. Ser. 121, 59 (1997)>
=1997A&AS..121...59Z (SIMBAD/NED BibCode)
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ADC_Keywords: Radio sources
Keywords: surveys - catalogs - radio continuum: general
Description:
A meter-wave survey of the sky region north of declination +30{deg}
has been carried out with the Miyun Synthesis Radio Telescope
(MSRT), Beijing Astronomical Observatory, at 232MHz. It is a
moderately deep survey. The observations were made between January
1985 and December 1993. The covered sky area is divided into 156
fields of view. Basically all adjacent fields are separated by
8 degree angular distance. Fields #54, #56, #115, #116, have no data
yet. A catalog of 34462 radio sources is given in Table 2. Table3
shows the information on the 152 fields of view.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
fig1.ps 132 864 Arrangement of the fields in the Miyun
232MHz survey
fig2.ps 132 148 Comparisons of flux densities
fig3.ps 132 108 *rms of background fluctuation in RA direction
fig4.ps 132 137 *rms of background fluctuation in DE direction
table2.dat 75 34426 The source-list of the survey
table3.dat 30 152 Information on 152 fields of view
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Note on fig3.ps, fig4.ps: RMSs between the Miyun and the 6C catalog.
Sources used in this measurement are within the range:
RA: 6h to 16h, DE: 30deg to 40deg
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See also:
VIII/18 : 6C Survey at 151MHz (I) (Baldwin+ 1985)
VIII/21 : 6C Survey at 151MHz (II) (Hales+ 1988)
VIII/22 : 6C Survey at 151MHz (III) (Hales+ 1990)
VIII/23 : 6C Survey at 151MHz (IV) (Hales+ 1991)
VIII/24 : 6C Survey at 151MHz (V) (Hales+ 1993)
VIII/25 : 6C Survey at 151MHz (VI) (Hales+ 1993)
Byte-by-byte Description of file: table2.dat
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Bytes Format Units Label Explanations
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4- 14 A11 --- Name Source name (1)
16- 17 I2 h RAh Right ascension 1950.0 of the source
19- 20 I2 min RAm Right ascension 1950.0 of the source
22- 25 F4.1 s RAs Right ascension 1950.0 of the source
28- 29 I2 deg DEd Declination 1950.0 of the source
31- 32 I2 arcmin DEm Declination 1950.0 of the source
34- 37 F4.1 arcsec DEs Declination 1950.0 of the source
40- 47 F8.2 Jy Speak Peak flux density (Jy/beam)
50- 57 F8.2 Jy Sint ? Integrated flux density (Jy/beam)
58- 63 F6.2 --- Factor Factor for correcting the primary beam
64- 70 F7.1 --- S/N Local S/N (2)
73- 75 A3 --- Field Number of the field of view
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Note (1): The name is based on a truncated B1950 position; a suffix
A, B, C or D differentiates sources with identical
truncated positions.
Note (2): Local S/N is calculated in the way of
maximum (peak flux, integral flux)/(local noise)
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Byte-by-byte Description of file: table3.dat
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Bytes Format Units Label Explanations
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1- 3 A3 --- Field Number of the field of view
5- 6 I2 h RAh Right ascension of the field center at OBSdate
8- 9 I2 min RAm Right ascension of the field center at OBSdate
11- 12 I2 s RAs Right ascension of the field center at OBSdate
15- 16 I2 deg DEd Declination of the field center at OBSdate
19- 26 A8 DD/MM/YY OBSdate Observing date
28- 30 I3 mJy Fluct Background fluctuation (mJy/beam)
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Acknowledgements: Xizhen Zhang <zxz@bao01.bao.ac.cn>
References:
Zhang X. et al., 1993A&AS...99..545Z: The Miyun 232 MHz survey. I.
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(End) Patricia Bauer [CDS] 03-Jun-1996
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