J/ApJS/98/33      First Caltech-Jodrell Bank VLBI Survey. II. (Thakkar+ 1995)

The First Caltech-Jodrell Bank VLBI Survey. II. Lambda = 18 Centimeter Observations of 25 Sources Thakkar D.D., Xu W., Readhead A.C.S., Pearson T.J., Taylor G.B., Vermeulen R.C., Polatidis A.G., Wilkinson P.N. <Astrophys. J. Suppl. Ser. 98, 33 (1995)> =1995ApJS...98...33T 1995ApJS...98...33T
ADC_Keywords: VLBI ; QSOs ; Radio sources Keywords: quasars: general - radio continuum: galaxies - surveys - techniques: interferometric Abstract: We report lambda-18 cm VLBI observations made in 1991 September of a further 25 objects from the first Caltech-Jodrell Bank VLBI Survey (the CJ1 survey). The CJ1 sample is a complete, flux-density limited sample of 135 radio sources with total flux density at lambda-6cm between 0.7 and 1.3Jy. These observations complete the lambda-18cm part of the survey. Together with the results of Paper I (Polatidis et al., J/ApJS/98/1), we have now observed 81 CJ1 sources at lambda-18cm. Later papers in the series will present lambda-6cm observations and the analysis and interpretation of the results. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 74 24 Map parameters table3 53 44 Gaussian models fig/* . 51 Maps -------------------------------------------------------------------------------- See also: J/ApJS/98/1 : First Caltech-Jodrell Bank VLBI Survey. I (Polatidis+ 1995) J/ApJS/99/297 : First Caltech-Jodrell Bank VLBI Survey. III (Xu+ 1995) J/ApJS/95/345 : Second Caltech-Jodrell Bank VLBI Survey. I. (Taylor+ 1994) J/ApJS/100/1 : Second Caltech-Jodrell Bank VLBI Survey. II (Henstock+ 1995) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- CJ1 B1950 source name according to IAU convention 10- 13 I4 yr OBSy Date of VLBI observation (year) 15- 16 I2 --- OBSm Date of VLBI observation (year) 18- 20 A3 --- Samp VLBI sample (CJ1 or PR) source belongs to 22- 26 F5.2 mas a18cmn FWHM of major axis of the restoring beam 28- 32 F5.2 mas b18cmn FWHM of minor axis of the restoring beam 34- 37 I4 deg PA18cmn [-89/32] Position angle of major axis, north through east 39- 42 I4 mJy S18cmn *Peak flux density, naturally weighted map 44- 47 F4.2 mJy e_S18cmn *Off source rms, naturally weighted map 49- 53 F5.2 mas a18cmt FWHM of major axis of tapered map restoring beam 55- 59 F5.2 mas b18cmt FWHM of minor axis of tapered map restoring beam 61- 64 I4 deg PA18cmt [-60/72] Position angle of major axis, N through E 66- 69 I4 mJy S18cmt *Peak flux density, tapered map 71- 74 F4.2 mJy e_S18cmt *Off source rms, tapered map -------------------------------------------------------------------------------- Note on S18cmn, e_S18cmn, S18cmt, e_S18cmt: Data are in mJy/beam -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- CJ1 B1950 source name according to IAU convention 9- 14 F6.3 Jy S Flux density of component 15- 21 F7.2 mas Rad *Radius of component 22- 28 F7.1 deg Theta *Angle to component 29- 35 F7.2 mas a FWHM of major axis of component 36- 40 F5.2 --- b/a Axial ratio of major to minor axis, b/a 41- 47 F7.1 deg Phi Position angle of major axis, north through east 48- 53 F6.3 --- Chi2 []? Chi-squared between the model and the self-calibrated UV-data -------------------------------------------------------------------------------- Note on Rad: Radius of component, measured from position of first component Note on Theta: Angle to component, measured north through east from the position of the first component -------------------------------------------------------------------------------- Origin: AAS CD-ROM series, Volume 4, 1995 Lee Brotzman [ADS] 10-May-95
(End) [CDS] 14-Oct-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