<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE dataset SYSTEM "http://tarantella.gsfc.nasa.gov/xml/dataset_048.dtd">
<dataset subject="astronomy" xmlns:xlink="http://www.w3.org/XML/XLink/0.9">
	<title>Linear polarimetry of Ap stars. V. A general catalogue of measurements</title>
	<altname type="ADC">J/A+AS/114/79</altname>
		<altname type="CDS">J/A+AS/114/79</altname>
		<altname type="brief">Polarimetry of Ap stars: general catalogue</altname>
	<reference>
		<source>
<journal>
	<title>Linear polarimetry of Ap stars. V. A general catalogue of measurements</title>
	<author>
			<initial>J</initial>
			<initial>L</initial>
			<lastName>Leroy</lastName></author>
	<name>Astron. Astrophys. Suppl. Ser.</name>
	<volume>114</volume>
	<pageno>79</pageno>
		<date>
			<year>1995</year></date>
	<bibcode>1995A&amp;AS..114...79L</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="catalogs.html">catalogs</keyword>
			<keyword xlink:href="polarization.html">polarization</keyword>
			<keyword xlink:href="stars_chemically_peculiar.html">stars: chemically peculiar</keyword>
			<keyword xlink:href="stars_magnetic_fields.html">stars: magnetic fields</keyword></keywords>
	<descriptions>
				<description>
				<para>
    A systematic program of broadband linear polarimetry, bearing on 55 Ap
    stars, has been developed during the 4 last years, at the Pic du Midi
    Observatory. While separate data have been already published, we
    present in this paper a complete catalogue of our observational
    material, including more than 400 measurements. We complement these
    data with another 100 measurements, obtained previously by other
    authors, so as to get a synthetic view of the phenomenon. Most of the
    observations have been dedicated to a small number (15) of stars,
    which show conspicuous changes of the linear polarization, so that it
    is possible to know accurately the time variation of the Stokes
    parameters: we expect that these new data will really improve our
    knowledge of the magnetic configuration, after a proper analysis which
    is currently being developed. For the other 40 stars, the polarization
    is either too small, or strongly contaminated by the interstellar
    polarization, so that broadband polarimetry is not very effective.
    Anyway, this first systematic investigation on the linear polarization
    of Ap stars will be a useful starting point for future measurements
    which should be made with higher spectral resolution. Finally, our
    measurements have provided new determinations of the rotation period
    for several stars.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="polariz.dat">
	<title>Polarization data (polariz.dat 1 to 68)</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Star</name>
			<definition>Star name
	<footnote footnoteId="???"><para>number=1</para>
			<para>HD 11502 = {gamma} Ari S
          HD 11503 = {gamma} Ari N</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Filter</name>
			<definition>Filter
	<footnote footnoteId="???"><para>number=2</para>
			<para>B   : B filter
          Ba  : B filter; Piirola and Tuominen 1981
          Bb  : B filter; Breger et al. 1989
          Bc  : B filter; Berdyugin et al. 1992
          exB : extended-B filter; Kemp and Wolstencroft 1974
          L   : {lambda}=4200A filter
          L5  : {lambda}=5200A filter
          LB  : {lambda}=4200A or B filter
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>JD</name>
			<definition>Julian Date</definition>
			<units>d</units></field>
		<field>
			<name>Pol</name>
			<definition>Polarization degree</definition>
			<units>%</units></field>
		<field>
			<name>Theta</name>
			<definition>Polarization orientation</definition>
			<units>deg</units></field>
		<field>
			<name>Q/I</name>
			<definition>Reduced Stokes parameter Q/I</definition>
			<units>%</units></field>
		<field>
			<name>U/I</name>
			<definition>Reduced Stokes parameter U/I</definition>
			<units>%</units></field>
		<field>
			<name>e_Q/I</name>
			<definition>Standard deviation on Q/I and U/I</definition>
			<units>%</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table69">
	<title>Fourier coefficients of the Q/I and U/I
                                 expansion</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Star</name>
			<definition>Star name</definition>
			<units>---</units></field>
		<field>
			<name>ZQ</name>
			<definition>Fourier coefficient Z_Q_</definition>
			<units>---</units></field>
		<field>
			<name>AQ</name>
			<definition>Fourier coefficient A_Q_</definition>
			<units>---</units></field>
		<field>
			<name>BQ</name>
			<definition>Fourier coefficient B_Q_</definition>
			<units>---</units></field>
		<field>
			<name>CQ</name>
			<definition>Fourier coefficient C_Q_</definition>
			<units>---</units></field>
		<field>
			<name>DQ</name>
			<definition>Fourier coefficient D_Q_</definition>
			<units>---</units></field>
		<field>
			<name>EQ</name>
			<definition>Fourier coefficient E_Q_</definition>
			<units>---</units></field>
		<field>
			<name>FQ</name>
			<definition>Fourier coefficient F_Q_</definition>
			<units>---</units></field>
		<field>
			<name>GQ</name>
			<definition>Fourier coefficient G_Q_</definition>
			<units>---</units></field>
		<field>
			<name>HQ</name>
			<definition>Fourier coefficient H_Q_</definition>
			<units>---</units></field>
		<field>
			<name>IQ</name>
			<definition>Fourier coefficient I_Q_</definition>
			<units>---</units></field>
		<field>
			<name>JQ</name>
			<definition>Fourier coefficient J_Q_</definition>
			<units>---</units></field>
		<field>
			<name>ZU</name>
			<definition>Fourier coefficient Z_U_</definition>
			<units>---</units></field>
		<field>
			<name>AU</name>
			<definition>Fourier coefficient A_U_</definition>
			<units>---</units></field>
		<field>
			<name>BU</name>
			<definition>Fourier coefficient B_U_</definition>
			<units>---</units></field>
		<field>
			<name>CU</name>
			<definition>Fourier coefficient C_U_</definition>
			<units>---</units></field>
		<field>
			<name>DU</name>
			<definition>Fourier coefficient D_U_</definition>
			<units>---</units></field>
		<field>
			<name>EU</name>
			<definition>Fourier coefficient E_U_</definition>
			<units>---</units></field>
		<field>
			<name>FU</name>
			<definition>Fourier coefficient F_U_</definition>
			<units>---</units></field>
		<field>
			<name>GU</name>
			<definition>Fourier coefficient G_U_</definition>
			<units>---</units></field>
		<field>
			<name>HU</name>
			<definition>Fourier coefficient H_U_</definition>
			<units>---</units></field>
		<field>
			<name>IU</name>
			<definition>Fourier coefficient I_U_</definition>
			<units>---</units></field>
		<field>
			<name>JU</name>
			<definition>Fourier coefficient J_U_</definition>
			<units>---</units></field>
		<field>
			<name>Chi2/nu</name>
			<definition>Ratio of Chi-squared to the number of degrees
                                  of freedom</definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Simona Mei</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1995</year><month>Jul</month><day>05</day></date></ingest>
		</history>
	<identifier>J_A+AS_114_79.xml</identifier></dataset>
