<?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>B and V photometry of faint stars in the Large Magellanic Cloud</title>
	<altname type="ADC">J/A+AS/73/37</altname>
		<altname type="CDS">J/A+AS/73/37</altname>
		<altname type="brief">LMC faint stars BV photometry</altname>
	<reference>
		<source>
<journal>
	<title>B and V photometry of faint stars in the Large Magellanic Cloud</title>
	<author>
			<initial>P</initial>
			<lastName>Linde</lastName></author>
	<author>
			<initial>A</initial>
			<lastName>Ardeberg</lastName></author>
	<author>
			<initial>H</initial>
			<lastName>Lindgren</lastName></author>
	<author>
			<initial>G</initial>
			<lastName>Lynga</lastName></author>
	<name>Astron. Astrophys. Suppl. Ser.</name>
	<volume>73</volume>
	<pageno>37</pageno>
		<date>
			<year>1988</year></date>
	<bibcode>1988A&amp;AS...73...37L</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Magellanic_Clouds.html">Magellanic Clouds</keyword>
			<keyword xlink:href="Photometry.html">Photometry</keyword>
			<keyword xlink:href="Stars_faint.html">Stars, faint</keyword></keywords>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="electronography.html">electronography</keyword>
			<keyword xlink:href="image_crowding.html">image crowding</keyword>
			<keyword xlink:href="image_processing.html">image processing</keyword>
			<keyword xlink:href="Magellanic_Clouds.html">Magellanic Clouds</keyword>
			<keyword xlink:href="photometry_BV.html">photometry, BV</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
    Photometric data on the Johnson BV system are given for 947 stars in a
    field close to the bar of the Large Magellanic Cloud. The data have
    been determined from electronographs calibrated through photoelectric
    photometry. The visual magnitudes of the programme stars range from
    V=14.63 to V=23.13.</para></abstract>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1">
	<title>Data for the measured stars.</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Seq</name>
			<definition>Star sequential number
	<footnote footnoteId="???"><para>number=1</para>
			<para>Remark: Stars Nos. 90, 721, 751 and 835 have the following
                  photoelectrically measured magnitudes:
                        No.     V       B-V
                         90     16.63   1.74
                        721     15.25   0.62
                        751     13.56   0.72
                        835     17.35   1.40</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension (1950)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension (1950)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension (1950)</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination (1950)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination (1950)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination (1950)</definition>
			<units>arcsec</units></field>
		<field>
			<name>Xpos</name>
			<definition>X position
	<footnote footnoteId="???"><para>number=2</para>
			<para>1 pix = 0.144".</para></footnote></definition>
			<units>pix</units></field>
		<field>
			<name>Ypos</name>
			<definition>Y position
	<footnote footnoteId="???"><para>number=2</para>
			<para>1 pix = 0.144".</para></footnote></definition>
			<units>pix</units></field>
		<field>
			<name>Vmag</name>
			<definition>V magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>B-V</name>
			<definition>B-V colour index</definition>
			<units>mag</units></field>
		<field>
			<name>o_Vmag</name>
			<definition>Number of observations in V magnitude</definition>
			<units>---</units></field>
		<field>
			<name>n_Vmag</name>
			<definition>Note on Vmag
	<footnote footnoteId="???"><para>number=3</para>
			<para>An * marks that the magnitude has been measured at an unusual
           intensity, in most cases lower than normal.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>o_Bmag</name>
			<definition>Number of observations in B magnitude</definition>
			<units>---</units></field>
		<field>
			<name>n_Bmag</name>
			<definition>Note on Bmag
	<footnote footnoteId="???"><para>number=3</para>
			<para>An * marks that the magnitude has been measured at an unusual
           intensity, in most cases lower than normal.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>e_Vmag</name>
			<definition>rms uncertainty on V magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>e_Bmag</name>
			<definition>rms uncertainty on B magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>q_Vmag</name>
			<definition>Quality factor on V magnitude
	<footnote footnoteId="???"><para>number=4</para>
			<para>5 denotes a perfect fit with no noticeable residuals and
          1 a fit estimated as unsatisfactory.
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>q_Bmag</name>
			<definition>Quality factor on B magnitude
	<footnote footnoteId="???"><para>number=4</para>
			<para>5 denotes a perfect fit with no noticeable residuals and
          1 a fit estimated as unsatisfactory.
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>DeltaD</name>
			<definition>Measure of positional accuracy</definition>
			<units>arcsec</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Marie-Jose Wagner, Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1997</year><month>Apr</month><day>18</day></date></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para> Prepared via OCR at CDS.</para></revision></revisions></history>
	<identifier>J_A+AS_73_37.xml</identifier></dataset>
