J/A+A/340/371       Quasar polarization                (Hutsemekers+ 1998)

Polarization properties of a sample of broad absorption line and gravitationally lensed quasars Hutsemekers D., Lamy H., Remy M. <Astron. Astrophys. 340, 371 (1998)> =1998A&A...340..371H 1998A&A...340..371H
ADC_Keywords: QSOs ; Polarization Keywords: polarization - galaxies: quasars: absorption lines - galaxies: quasars: general - cosmology: gravitational lensing Description: Table 2 contains optical (V) polarimetric measurements for 42 optically selected QSOs including 29 broad absorption line QSOs. Table 3 contains a series of spectral indices characterizing the broad absorption line QSOs. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 67 42 Polarimetric results table3.dat 68 29 BAL QSO spectral characteristics -------------------------------------------------------------------------------- See also: J/A+A/332/410 : Quasar polarization (Hutsemekers 1998) J/A+AS/142/451 : Optical Polarization of 47 QSOs (Lamy+, 2000) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Quasar name (from 1950 position) 11- 15 F5.3 --- z Redshift 17 I1 --- Type [1/6] Object type (G1) 18 I1 --- Note [0/1] 1 for objects identified as true or possible gravitationally lensed QSOs 20- 24 F5.2 % Q Normalized Stokes parameter Q 26- 29 F4.2 % e_Q Uncertainty of Normalized Stokes parameter Q 31- 35 F5.2 % U Normalized Stokes parameter U 37- 40 F4.2 % e_U Uncertainty of Normalized Stokes parameter U 42- 45 F4.2 % Pol Polarization degree 47- 50 F4.2 % e_Pol Uncertainty of polarization degree 52- 55 F4.2 % Pold Debiased polarization degree 57- 60 F4.2 % Poli Interstellar polarization 62- 64 I3 deg PA Polarization position angle 66- 67 I2 deg e_PA ? Uncertainty of polarization position angle -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Quasar name (from 1950 position) 11 I1 --- Type [1/6] Object type (G1) 12 I1 --- Note [0/1] 1 for objects identified as true or possible gravitationally lensed QSOs 14- 18 I5 km/s BI Balnicity index (2) 20- 24 F5.2 --- DI Detachment index (3) 26- 29 I4 km/s HWHM(CIV) ? CIV Half Width at Half Maximum 31- 34 I4 km/s HWHM(CIII) ? CIII] Half Width at Half Maximum 36- 39 F4.1 0.1nm EW(CIV) ? CIV equivalent width 41- 44 F4.1 0.1nm EW(CIII) ? CIII] equivalent width 46- 50 F5.2 0.1nm EW(FeII2400) ? FeII 2400 equivalent width 52- 56 F5.2 0.1nm EW(FeII2070) ? FeII 2070 equivalent width 58- 62 F5.2 --- Bcont Continuum slope B 64- 67 F4.2 --- Rcont Continuum slope R -------------------------------------------------------------------------------- Note (2): The balnicity index is a modified velocity equivalent width of the C IV broad absorption line. See Weymann et al., 1991ApJ...373...23W 1991ApJ...373...23W. Note (3): The detachment index is the degree of detachment of the absorption line relative to the emission one. See Weymann et al. (1991ApJ...373...23W 1991ApJ...373...23W) -------------------------------------------------------------------------------- Global Notes: Note (G1): Object Type is numbered as follows: 1 = non-BAL QSOs + one intermediate object 2 = HIBAL QSOs 3 = Strong LIBAL QSOs 4 = Weak LIBAL QSOs 5 = Marginal LIBAL QSOs 6 = unclassified BAL QSOs Acknowledgements: Damien Hutsemekers
(End) Hutsemekers [Liege University], Patricia Bauer [CDS] 13-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