J/AJ/99/1071        1.4 GHz source survey            (Condon+ 1990)

A 1.4 GHz source survey in an area without nearby rich galaxy clusters Condon J.J., Dickey J.M., Salpeter E.E. <Astron. J. 99, 1071 (1990)> =1990AJ.....99.1071C 1990AJ.....99.1071C (SIMBAD/NED BibCode)
ADC_Keywords: Radio sources ; Galaxies, radio Abstract: We report on 1.4GHz continuum observations for 56 contiguous VLA fields, using the D configuration, in a region devoid of nearby, rich galaxy clusters (at z<0.4). 354 continuum sources are tabulated, with fluxes down to about 1.5mJy, in an area of about 12degres+2. Only about seven of the 354 radio sources are associated with known rich galaxy clusters at z>0.4 (tabulated by Gunn, Hoessel, and Oke, 1986ApJ...306...30G 1986ApJ...306...30G). We compare source positions with those from an optical catalog (generated from a POSS plate with the use of the Minnesota Automated Plate Scanner) and find mild correlations on angular scales of order 1arcmin. This suggests some association of radio sources with galaxy groups (sizes of order 200 kpc) at redshifts of order z∼0.1, even though there are no rich galaxy clusters in this redshift range. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 35 56 Center of fields and sensitivity of VLA fields table2.dat 57 354 Radio sources detected by the VLA. table3.dat 48 130 Large optical galaxies from POSS plates table4.dat 64 58 Optical objects coincident with radio sources -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Field Field number 6- 7 I2 h RAh Right Ascension B1950 of field center (hours) 8- 9 I2 min RAm Right Ascension B1950 of field center (minutes) 10- 11 I2 s RAs [0,60] Right Ascension B1950 (seconds) 12 A1 --- DE- Declination B1950 of field center (sign) 13- 14 I2 deg DEd Declination B1950 of field center (degrees) 15- 16 I2 arcmin DEm Declination B1950 of field center (minutes) 20- 23 F4.2 mJy Srms RMS noise flux density 26- 29 F4.2 mJy Sneg ? Flux level for "negative" detections 32- 35 F4.2 mJy Smin Minimum flux level adopted for detection -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- Source Source name 5 A1 --- n_Source ['?] Note on Source (1) 7- 9 I3 --- Field Field whose center is closest to the source 10 A1 --- n_Field [*] Note on Field (2) 12 I1 h RAh Right ascension (1950) 14- 15 I2 min RAm Right ascension (1950) 17- 20 F4.1 s RAs Right ascension (1950) 21 A1 --- DE- Declination sign 22- 23 I2 deg DEd Declination (1950) 25- 26 I2 arcmin DEm Declination (1950) 28- 29 I2 arcsec DEs [0,60] Declination (1950) 31- 35 F5.1 mJy Smax Peak flux at 1.4GHz 37- 41 F5.1 mJy Sint Area integrated flux at 1.4GHz 43- 46 F4.2 --- PBC Primary-beam correction factor (3) -------------------------------------------------------------------------------- Note (1): ? : slightly suspect detections ' : Smax < 2(PBC)Smin Note (2): * : the source is fairly close to the center of a second field Note (3): PBC(t)=exp[10.7t2 + 25.3t4] where t is the distance from the source to the field center in degrees. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Gno Galaxy source Number 6- 7 I2 h RAh Right Ascension B1950 (hours) 8- 9 I2 min RAm Right Ascension B1950 (minutes) 10- 13 F4.1 s RAs Right Ascension B1950 (seconds) 14 A1 --- DE- Declination B1950 (sign) 15- 16 I2 deg DEd Declination B1950 (degrees) 17- 18 I2 arcmin DEm Declination B1950 (minutes) 19- 20 I2 arcsec DEs [0,60] Declination B1950 (seconds) 24- 26 I3 um R65%diam Diameter on red plate at level 65% (1) 29- 31 I3 um R30%diam Diameter on red plate at level 30% (1) 35- 37 I3 um B65%diam Diameter on blue plate at level 65% (1) 40- 42 I3 um B30%diam Diameter on blue plate at level 30% (1) 45- 48 F4.1 mag mZw ? Zwicky magnitude of galaxy -------------------------------------------------------------------------------- Note (1): the levels are defined from the transmission density. Diameters are in microns (1um = 0.067") from the POSS plates 1st epoch -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- Source Source name, as in table2 5 A1 --- u_Source [?] Uncertainty flag 7 A1 --- Otype [Gf] optical Galaxy or faint object (1) 10- 14 F5.2 mJy Smax Peak flux at 1.4GHz 16- 17 I2 h RAh Right Ascension B1950 (hours) 18- 19 I2 min RAm Right Ascension B1950 (minutes) 20- 23 F4.1 s RAs Right Ascension B1950 (seconds) 24 A1 --- DE- Declination B1950 (sign) 25- 26 I2 deg DEd Declination B1950 (degrees) 27- 28 I2 arcmin DEm Declination B1950 (minutes) 29- 30 I2 arcsec DEs [0,60] Declination B1950 (seconds) 34- 36 I3 um R65%diam Diameter on red plate at level 65% (2) 39- 41 I3 um R30%diam Diameter on red plate at level 30% (2) 46- 48 I3 um B65%diam Diameter on blue plate at level 65% (2) 51- 53 I3 um B30%diam Diameter on blue plate at level 30% (2) 57- 58 I2 arcsec Sep Separation between optical and radio sources 62- 64 I3 --- Gno ? Number in table3 (1) -------------------------------------------------------------------------------- Note (1): 'G' indicates a coincidence with a galaxy; when this galaxy was optically identified in table3, its number is listed in the last column. These coincidences are listed in table4a of the publication. 'g' indicates a coincidence with an optical faint or unresolved objet, originally listed in table4b of the publication. Note (2): the levels are defined from the transmission density. Diameters are in microns (1um = 0.067") from the POSS plates 1st epoch -------------------------------------------------------------------------------- Acknowledgements: We thank Heinz Andernach for supplying the tables 1, 3 and 4. History: * 14-Nov-1997: table2 prepared via OCR at CDS. * 14-Dec-1997: an error in R120 declination was detected by H. Andernach and corrected. * 28-Oct-1998: tables 1,3,4 prepared by H. Andernach (catalogue numbered R187 in his list) were added. * 03-Nov-1998: an error in table3 (Gno 115 was labelled Gno 117) was detected by Fabienne Woelfel and corrected
(End) Marie-Jose Wagner, Patricia Bauer, Francois Ochsenbein [CDS] 28-Oct-1998
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