<?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>Photometric and spectroscopic studies of cool stars discovered in EXOSAT
X-ray images. III. Photometric properties</title>
	<altname type="ADC">J/A+AS/115/41</altname>
		<altname type="CDS">J/A+AS/115/41</altname>
		<altname type="brief">UBV</altname>
	<reference>
		<source>
<journal>
	<title>Photometric and spectroscopic studies of cool stars discovered in EXOSAT
X-ray images. III. Photometric properties</title>
	<author>
			<initial>G</initial>
			<lastName>Cutispoto</lastName></author>
	<author>
			<initial>G</initial>
			<lastName>Tagliaferri</lastName></author>
	<author>
			<initial>R</initial>
			<lastName>Pallavicini</lastName></author>
	<author>
			<initial>L</initial>
			<lastName>Pasquini</lastName></author>
	<author>
			<initial>M</initial>
			<lastName>Rodono</lastName></author>
	<name>Astron. Astrophys. Suppl. Ser.</name>
	<volume>115</volume>
	<pageno>41</pageno>
		<date>
			<year>1996</year></date>
	<bibcode>1996A&amp;AS..115...41C</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Photometry_UBVRI.html">Photometry, UBVRI</keyword>
			<keyword xlink:href="Stars_late-type.html">Stars, late-type</keyword>
			<keyword xlink:href="X-ray_sources.html">X-ray sources</keyword></keywords>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="stars_activity.html">stars: activity</keyword>
			<keyword xlink:href="stars_late-type.html">stars: late-type</keyword>
			<keyword xlink:href="stars_variables_general.html">stars: variables: general</keyword>
			<keyword xlink:href="X-rays_stars.html">X-rays: stars</keyword></keywords>
	<descriptions>
				<description>
				<para>
    We present high-precision UBV(RI)_c_ photometry for a sample of active
    stars detected serendipitously by the EXOSAT satellite. Fourteen
    objects, out of 47 likely optical counterparts, turned out to be
    clearly variable, with periods in the range 1-8 days, including a
    newly discovered eclipsing binary. For most of them the optical
    variability is consistent with the presence of photospheric cool
    spots. We have used our multicolour photometry to estimate spectral
    classifications and distances. The derived distances indicate that
    some of the observed stars are previously unidentified nearby
    (d&lt;=25pc) M dwarfs. When combined with the results of high resolution
    spectroscopy, our photometric observations allow us to investigate the
    stellar content of the selected X-ray sample. Young stars and RS
    CVn-type binaries appear to constitute a large fraction of the
    selected sample. For a description of the UBV and (RI)c photometric
    systems, see e.g.
    &lt;http://obswww.unige.ch/gcpd/ph01.html> and
    &lt;http://obswww.unige.ch/gcpd/ph54.html>.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table2">
	<title>Photometric data for the observed stars</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Id</name>
			<definition>Identification number</definition>
			<units>---</units></field>
		<field>
			<name>Name</name>
			<definition>EXOSAT name (Catalogue &lt;VI/43>)</definition>
			<units>---</units></field>
		<field>
			<name>ObsSeason</name>
			<definition>Code for the observing season
	<footnote footnoteId="???"><para>number=1</para>
			<para>The code is composed by the initial of the month followed
           by the two last numbers of the year.
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>n_ObsSeason</name>
			<definition>When "o": data from Paper I:
                                  Cutispoto G. et al 1991</definition>
			<units>---</units></field>
		<field>
			<name>Vmax</name>
			<definition>V magnitude at maximum luminosity</definition>
			<units>mag</units></field>
		<field>
			<name>U-B</name>
			<definition>U-B color index</definition>
			<units>mag</units></field>
		<field>
			<name>B-V</name>
			<definition>B-V color index</definition>
			<units>mag</units></field>
		<field>
			<name>V-Rc</name>
			<definition>V-R_c_ color index (Cousins)</definition>
			<units>mag</units></field>
		<field>
			<name>V-Ic</name>
			<definition>V-I_c_ color index (Cousins)</definition>
			<units>mag</units></field>
		<field>
			<name>Qual</name>
			<definition>Quality of the data</definition>
			<units>---</units></field>
		<field>
			<name>Var</name>
			<definition>Variability flag</definition>
			<units>---</units></field>
		<field>
			<name>n_Var</name>
			<definition>Uncertainty on variability flag</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table3">
	<title>Photometric data</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Id</name>
			<definition>Identification number</definition>
			<units>---</units></field>
		<field>
			<name>EXOSAT</name>
			<definition>EXOSAT name</definition>
			<units>---</units></field>
		<field>
			<name>Other</name>
			<definition>Other catalogue number</definition>
			<units>---</units></field>
		<field>
			<name>Sp</name>
			<definition>Spectral type</definition>
			<units>---</units></field>
		<field>
			<name>Dist</name>
			<definition>Distance</definition>
			<units>pc</units></field>
		<field>
			<name>n_Dist</name>
			<definition>Uncertainty on distance</definition>
			<units>---</units></field>
		<field>
			<name>Var</name>
			<definition>Variability flag</definition>
			<units>---</units></field>
		<field>
			<name>Period</name>
			<definition>Period of variability</definition>
			<units>d</units></field>
		<field>
			<name>n_Period</name>
			<definition>Uncertainty on period of variability</definition>
			<units>---</units></field>
		<field>
			<name>l_DeltaV</name>
			<definition>Limit flag on amplitude in V-band</definition>
			<units>---</units></field>
		<field>
			<name>DeltaV</name>
			<definition>Amplitude in the V-band</definition>
			<units>mag</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Simona Mei</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1995</year><month>Sep</month><day>25</day></date></ingest>
		</history>
	<identifier>J_A+AS_115_41.xml</identifier></dataset>
