J/A+A/489/911  Polarimetric measures of selected variable stars   (Elias+, 2008)

Polarimetric measures of selected variable stars. Elias N.M.II, Koch R.H., Pfeiffer R.J. <Astron. Astrophys. 489, 911 (2008)> =2008A&A...489..911E 2008A&A...489..911E
ADC_Keywords: Stars, variable ; Polarization Keywords: polarization - binaries: close - Cepheids - circumstellar matter - accretion, accretion disks - dust, extinction Abstract: The purpose of this paper is to summarize and interpret unpublished optical polarimetry for numerous program stars that were observed over the past decades at the Flower and Cook Observatory (FCO), University of Pennsylvania. We also make the individual calibrated measures available for long-term comparisons with new data. We employ three techniques to search for intrinsic variability within each dataset. First, when the observations for a given star and filter are numerous enough and when a period has been determined previously via photometry or spectroscopy, the polarimetric measures are plotted versus phase. If a statistically significant pattern appears, we attribute it to intrinsic variability. Second, we compare means of the FCO data to means from other workers. If they are statistically different, we conclude that the object exhibits long-term intrinsic variability. Third, we calculate the standard deviation for each program star and filter and compare it to the standard deviation estimated from comparable polarimetric standards. If the standard deviation of the program star is at least three times the value estimated from the polarimetric standards, the former is considered intrinsically variable. All of these statements are strengthened when variability appears in multiple filters. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file stars.dat 57 39 Stars positions (from Simbad) table12.dat 84 71 *The weighted means of the normalized linear and circular polarisations, together with the reduced standard deviations and numbers of observations table.dat 58 670 Polarization observations of close binary and β Cep stars from the polarization program at the Flower and Cook Observatory, University of Pennsylvania. -------------------------------------------------------------------------------- Note on table12.dat: Normalized Linear / Circular Stokes parameters. The reduced standard deviations must be multiplied by the square root of the number of measurements to compare them with the standard-deviation equations. -------------------------------------------------------------------------------- Byte-by-byte Description of file: stars.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Star Simbad star name 11- 12 I2 h RAh Simbad Hour of Right Ascension (J2000.0) 14- 15 I2 min RAm Simbad Minute of Right Ascension (J2000.0) 17- 20 F4.1 s RAs Simbad Second of Right Ascension (J2000.0) 22 A1 --- DE- Simbad Sign of the Declination (J2000.0) 23- 24 I2 deg DEd Simbad Degree of Declination (J2000.0) 26- 27 I2 arcmin DEm Simbad Arcminute of Declination (J2000.0) 29- 30 I2 arcsec DEs Simbad Arcsecond of Declination (J2000.0) 33- 38 F6.3 mag Bmag ? Simbad B band magnitude 40- 44 F5.3 mag Vmag Simbad V band magnitude 46- 57 A12 --- SpType Simbad MK spectral type -------------------------------------------------------------------------------- Byte-by-byte Description of file: table12.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 --- Name Star name 13- 21 A9 --- Star Other name (HD name if exist) 23- 24 A2 --- Filt [UBVRB1B2 -] Filter (G1) 26- 32 F7.4 % q Weighted mean q Stokes parameter 34- 39 F6.4 % e_q ? rms uncertainty on q 41- 46 F6.3 % u Weighted mean u Stokes parameter 48- 52 F5.3 % e_u ? rms uncertainty on u 54- 55 I2 --- Nl Number of observations for linear polarisation 57- 63 F7.4 % v ? Weighted mean v Stokes parameter 65- 70 F6.4 % e_v ? rms uncertainty on v 72- 73 I2 --- Nc Number of observations for circular polarisation 75- 84 A10 --- Note Note on observation -------------------------------------------------------------------------------- Byte-by-byte Description of file: table.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Star Name (HD name if exist) 10- 11 A2 --- n_Star [-6 ] Multiplicity index for the binary HD 036485-6 13- 23 F11.3 d HJD Heliocentric Julian date 25 A1 --- Filt [UBVR-] Filter (G1) 27- 32 F6.3 % q Normalized linear q Stokes parameter (NLSP) 34- 39 F6.3 % u Normalized linear u Stokes parameter (NLSP) 41- 45 F5.3 % e_q ? Normalized rms uncertainty on q and u (NLSP error) 47- 52 F6.3 % v ? Normalized circular v Stokes parameter (NCSP) 54- 58 F5.3 % e_v ? Normalized rms uncertainty on v (NCSP error) (2) -------------------------------------------------------------------------------- Note (2): No data for v parameter indicates no concurrent NCSP measurement with the NLSP measurement. -------------------------------------------------------------------------------- Global notes: Note (G1): - for unfiltered (≃ wide-band green). -------------------------------------------------------------------------------- Acknowledgements: Nicholas Elias,
(End) Patricia Vannier [CDS] 03-Oct-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