J/MNRAS/380/162     Aligned radio polarizations of quasars   (Joshi+, 2007)

A survey of polarization in the JVAS/CLASS flat-spectrum radio source surveys. II. A search for aligned radio polarizations. Joshi S.A., Battye R.A., Browne I.W.A., Jackson N., Muxlow T.W.B., Wilkinson P.N. <Mon. Not. R. Astron. Soc., 380, 162-174 (2007)> =2007MNRAS.380..162J 2007MNRAS.380..162J
ADC_Keywords: Surveys ; QSOs ; Polarization Keywords: polarization - surveys - galaxies: active Abstract: We have used the very large Jodrell Bank VLA Astrometric Survey/Cosmic Lens All-Sky Survey 8.4-GHz surveys of flat-spectrum radio sources to test the hypothesis that there is a systematic alignment of polarization position angle vectors on cosmological scales of the type claimed by Hutsemekers et al. (2005, Cat. J/A+A/441/915). The polarization position angles of 4290 sources with polarized flux density 1mJy have been examined. They do not reveal large-scale alignments either as a whole or when split in half into high-redshift (z≥1.24) and low-redshift subsamples. Nor do the radio sources which lie in the specific areas covered by Hutsemekers et al. (J/A+A/441/915) show any significant effect. We have also looked at the position angles of parsec-scale jets derived from very long baseline interferometry observations and again find no evidence for systematic alignments. Finally, we have investigated the correlation between the polarization position angle and those of the parsec-scale jets. As expected, we find that there is a tendency for the polarization angles to be perpendicular to the jet angles. However, the difference in jet and polarization position angles does not show any systematic trend in different parts of the sky. Description: We make use of the 4290 sources presented in Paper I (Jackson et al., Cat. J/MNRAS/376/371). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 16 1531 VLBI jet angles tablea1.dat 91 52 The 52 common objects in JVAS/CLASS surveys and Hutsemekers et al. sample (Cat. J/A+A/441/915) -------------------------------------------------------------------------------- See also: J/A+A/441/915 : Alignments of quasar polarization vectors (Hutsemekers+ 2005) J/MNRAS/376/371 : Polarisation of flat-spectrum radio sources (Jackson+, 2007) Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 --- Name Name (JHHMM+DDMM or JHHMM+DDMMm) 13- 16 I4 deg JA Jet angle, measured from north through to east -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 h RAh Right ascension (J2000) 4- 5 I2 min RAm Right ascension (J2000) 7- 12 F6.3 s RAs Right ascension (J2000) 14 A1 --- DE- Declination sign (J2000) 15- 16 I2 deg DEd Declination (J2000) 18- 19 I2 arcmin DEm Declination (J2000) 21- 25 F5.2 arcsec DEs Declination (J2000) 27- 33 A7 --- OName Name for some sources 35- 39 I5 mJy F(8.4) Total flux at 8.4GHz 41- 46 F6.3 % P(8.4) Percentage polarized flux at 8.4GHz 48- 52 F5.2 % P(opt) Percentage polarized flux in optical 54- 58 F5.1 deg PA(8.4) Polarization position angle at 8.4GHz 60- 62 I3 deg PA(opt) Polarization position angle in optical 64- 68 F5.1 deg PAdiff Position angle difference, PA(opt)-PA(8.4) 70- 91 A22 --- Name Name (from Hutsemekers et al. (2005, Cat. J/A+A/441/915) -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 22-Jul-2008
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