<?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>Tables of membership for 43 open clusters (1994 Version)</title>
	<altname type="ADC">1215</altname>
		<altname type="CDS">I/215</altname>
		<altname type="brief">Tables of membership for 43 open clusters</altname>
	<reference>
		<source>
<journal>
	<title>Tables of membership for 43 open clusters (1994 Version)</title>
	<author>
			<initial>J</initial>
			<initial>-L</initial>
			<lastName>Zhao</lastName></author>
	<author>
			<initial>K</initial>
			<initial>P</initial>
			<lastName>Tian</lastName></author>
	<name>Bull. Inf. CDS</name>
	<volume>47</volume>
	<pageno>5</pageno>
		<date>
			<year>1995</year></date>
	<bibcode>1995BICDS..47....5Z</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Clusters_open.html">Clusters, open</keyword>
			<keyword xlink:href="Proper_motions.html">Proper motions</keyword></keywords>
	<descriptions>
				<description>
				<para>
      Relative  proper  motion  data  have  been  widely  used to determine
    membership of open clusters. In view of the fact that  most of  data of
    proper motions had been obtained before Sanders' method was set  up and
    information  on  membership of  open clusters had been mostly published
    without a  statistically  rigorous method available, it is necessary to
    restudy  membership  of  clusters  from  data  by means of the rigorous
    method.  59 pieces of  relative proper motion data for 43 open clusters
    having  been  collected, we, by use of  the improved  Sanders'  method,
    calculate membership  probabilities  of all  the stars  for each field,
    based upon  which  individual member stars are found.  Recently we have
    obtained  proper  motions  and  membership  of  open  clusters  of M67,
    NGC2286 and Orion, which are also included in this new version. All the
    results  concerned are given in the form of catalogue.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="summary">
	<title>List of Clusters</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Seq</name>
			<definition>Order number</definition>
			<units>---</units></field>
		<field>
			<name>Cluster</name>
			<definition>Name of open cluster</definition>
			<units>---</units></field>
		<field>
			<name>File</name>
			<definition>Name of file</definition>
			<units>---</units></field>
		<field>
			<name>Nstars</name>
			<definition>Total number of stars (1st line)</definition>
			<units>---</units></field>
		<field>
			<name>Nmembers</name>
			<definition>Number of cluster member
	<footnote footnoteId="???"><para>number=1</para>
			<para>the next line lists the uncertainty on the parameter
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>pmX(fld)</name>
			<definition>Proper motion of field center in X
	<footnote footnoteId="???"><para>number=1</para>
			<para>the next line lists the uncertainty on the parameter
</para></footnote></definition>
			<units>10mas/yr</units></field>
		<field>
			<name>pmY(fld)</name>
			<definition>Proper motion of field center in Y
	<footnote footnoteId="???"><para>number=1</para>
			<para>the next line lists the uncertainty on the parameter
</para></footnote></definition>
			<units>10mas/yr</units></field>
		<field>
			<name>pmX(cl)</name>
			<definition>Proper motion of cluster center in X
	<footnote footnoteId="???"><para>number=1</para>
			<para>the next line lists the uncertainty on the parameter
</para></footnote></definition>
			<units>10mas/yr</units></field>
		<field>
			<name>pmY(cl)</name>
			<definition>Proper motion of cluster center in Y
	<footnote footnoteId="???"><para>number=1</para>
			<para>the next line lists the uncertainty on the parameter
</para></footnote></definition>
			<units>10mas/yr</units></field>
		<field>
			<name>sdX(fld)</name>
			<definition>Standard deviation in X of field stars
	<footnote footnoteId="???"><para>number=1</para>
			<para>the next line lists the uncertainty on the parameter
</para></footnote></definition>
			<units>10mas/yr</units></field>
		<field>
			<name>sdY(fld)</name>
			<definition>Standard deviation in Y of field stars
	<footnote footnoteId="???"><para>number=1</para>
			<para>the next line lists the uncertainty on the parameter
</para></footnote></definition>
			<units>10mas/yr</units></field>
		<field>
			<name>sd(cl)</name>
			<definition>Standard deviation of cluster stars
	<footnote footnoteId="???"><para>number=1</para>
			<para>the next line lists the uncertainty on the parameter
</para></footnote></definition>
			<units>10mas/yr</units></field>
		<field>
			<name>PA</name>
			<definition>Rotation angle to the major axis
                                    of the field distribution</definition>
			<units>deg</units></field>
		<field>
			<name>Ref</name>
			<definition>Reference</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="ber58">
	<title>Berkeley 58</title></tableLink>
				<tableLink xlink:href="ic1805">
	<title>IC 1805</title></tableLink>
				<tableLink xlink:href="ic4665">
	<title>IC 4665</title></tableLink>
				<tableLink xlink:href="ic4756">
	<title>IC 4756</title></tableLink>
				<tableLink xlink:href="ngc129a">
	<title>NGC 129</title></tableLink>
				<tableLink xlink:href="ngc129b">
	<title>NGC 129</title></tableLink>
				<tableLink xlink:href="ngc129c">
	<title>NGC 129</title></tableLink>
				<tableLink xlink:href="ngc188">
	<title>NGC 188</title></tableLink>
				<tableLink xlink:href="ngc457">
	<title>NGC 457</title></tableLink>
				<tableLink xlink:href="ngc581a">
	<title>NGC 581</title></tableLink>
				<tableLink xlink:href="ngc581b">
	<title>NGC 581</title></tableLink>
				<tableLink xlink:href="ngc663">
	<title>NGC 663</title></tableLink>
				<tableLink xlink:href="ngc752">
	<title>NGC 752</title></tableLink>
				<tableLink xlink:href="ngc1664">
	<title>NGC 1664</title></tableLink>
				<tableLink xlink:href="ngc1817">
	<title>NGC 1817</title></tableLink>
				<tableLink xlink:href="ngc1912">
	<title>NGC 1912</title></tableLink>
				<tableLink xlink:href="ngc2099a">
	<title>NGC 2099</title></tableLink>
				<tableLink xlink:href="ngc2099b">
	<title>NGC 2099</title></tableLink>
				<tableLink xlink:href="ngc2099c">
	<title>NGC 2099</title></tableLink>
				<tableLink xlink:href="ngc2168a">
	<title>NGC 2168</title></tableLink>
				<tableLink xlink:href="ngc2168b">
	<title>NGC 2168</title></tableLink>
				<tableLink xlink:href="ngc2264">
	<title>NGC 2264</title></tableLink>
				<tableLink xlink:href="ngc2281">
	<title>NGC 2281</title></tableLink>
				<tableLink xlink:href="ngc2286">
	<title>NGC 2286</title></tableLink>
				<tableLink xlink:href="ngc2420">
	<title>NGC 2420</title></tableLink>
				<tableLink xlink:href="ngc2548">
	<title>NGC 2548</title></tableLink>
				<tableLink xlink:href="ngc2682a">
	<title>NGC 2682</title></tableLink>
				<tableLink xlink:href="ngc2682b">
	<title>NGC 2682</title></tableLink>
				<tableLink xlink:href="ngc2682c">
	<title>NGC 2682</title></tableLink>
				<tableLink xlink:href="ngc2682d">
	<title>NGC 2682</title></tableLink>
				<tableLink xlink:href="ngc6611">
	<title>NGC 6611</title></tableLink>
				<tableLink xlink:href="ngc6633">
	<title>NGC 6633</title></tableLink>
				<tableLink xlink:href="ngc6705a">
	<title>NGC 6705</title></tableLink>
				<tableLink xlink:href="ngc6705b">
	<title>NGC 6705</title></tableLink>
				<tableLink xlink:href="ngc6705c">
	<title>NGC 6705</title></tableLink>
				<tableLink xlink:href="ngc6811">
	<title>NGC 6811</title></tableLink>
				<tableLink xlink:href="ngc6819">
	<title>NGC 6819</title></tableLink>
				<tableLink xlink:href="ngc6823">
	<title>NGC 6823</title></tableLink>
				<tableLink xlink:href="ngc6882">
	<title>NGC 6882</title></tableLink>
				<tableLink xlink:href="ngc6885">
	<title>NGC 6885</title></tableLink>
				<tableLink xlink:href="ngc6913">
	<title>NGC 6913</title></tableLink>
				<tableLink xlink:href="ngc6939">
	<title>NGC 6939</title></tableLink>
				<tableLink xlink:href="ngc7062">
	<title>NGC 7062</title></tableLink>
				<tableLink xlink:href="ngc7092a">
	<title>NGC 7092</title></tableLink>
				<tableLink xlink:href="ngc7092b">
	<title>NGC 7092</title></tableLink>
				<tableLink xlink:href="ngc7092c">
	<title>NGC 7092</title></tableLink>
				<tableLink xlink:href="ngc7209">
	<title>NGC 7209</title></tableLink>
				<tableLink xlink:href="ngc7654">
	<title>NGC 7654</title></tableLink>
				<tableLink xlink:href="ngc7788a">
	<title>NGC 7788</title></tableLink>
				<tableLink xlink:href="ngc7788b">
	<title>NGC 7788</title></tableLink>
				<tableLink xlink:href="ngc7790">
	<title>NGC 7790</title></tableLink>
				<tableLink xlink:href="oriona">
	<title>Orion Nebula</title></tableLink>
				<tableLink xlink:href="perh">
	<title>h Per</title></tableLink>
				<tableLink xlink:href="perx">
	<title>chi Per</title></tableLink>
				<tableLink xlink:href="tr1a">
	<title>Trumpler 1</title></tableLink>
				<tableLink xlink:href="tr1b">
	<title>Trumpler 1</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Number</name>
			<definition>The star number</definition>
			<units>---</units></field>
		<field>
			<name>x_mag</name>
			<definition>Filter Indicator
	<footnote footnoteId="???"><para>number=1</para>
			<para>x_mag takes the following values:
    'B' if "mag" column contains the B magnitude
    'V' if "mag" column contains the V magnitude
    'P' if "mag" column contains a photographic magnitude
    'D' if "mag" column contains a stellar diameter expressed in mm
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>n_mag</name>
			<definition>Note v=very faint f=faint</definition>
			<units>---</units></field>
		<field>
			<name>mag</name>
			<definition>Stellar magnitude or diameter
	<footnote footnoteId="???"><para>number=1</para>
			<para>x_mag takes the following values:
    'B' if "mag" column contains the B magnitude
    'V' if "mag" column contains the V magnitude
    'P' if "mag" column contains a photographic magnitude
    'D' if "mag" column contains a stellar diameter expressed in mm
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>var</name>
			<definition>v=variable</definition>
			<units>---</units></field>
		<field>
			<name>X</name>
			<definition>The measured coordinates in X</definition>
			<units>mm</units></field>
		<field>
			<name>Y</name>
			<definition>The measured coordinates in Y</definition>
			<units>mm</units></field>
		<field>
			<name>pmX</name>
			<definition>Proper motion in X</definition>
			<units>10mas/yr</units></field>
		<field>
			<name>pmY</name>
			<definition>Proper motion in Y</definition>
			<units>10mas/yr</units></field>
		<field>
			<name>Pr</name>
			<definition>Membership probabilities</definition>
			<units>---</units></field>
		<field>
			<name>oriNumber</name>
			<definition>The number in the original data</definition>
			<units>---</units></field>
		<field>
			<name>e_pmX</name>
			<definition>Mean error on pmX</definition>
			<units>10mas/yr</units></field>
		<field>
			<name>e_pmY</name>
			<definition>Mean error on pmY</definition>
			<units>10mas/yr</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="ngc6530">
	<title>NGC 6530</title></tableLink>
				<tableLink xlink:href="ngc654">
	<title>NGC 654</title></tableLink>
				<tableLink xlink:href="orionb">
	<title>Orion Nebula</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Number</name>
			<definition>The star number</definition>
			<units>---</units></field>
		<field>
			<name>x_mag</name>
			<definition>Filter Indicator
	<footnote footnoteId="???"><para>number=1</para>
			<para>x_mag takes the following values:
    'B' if "mag" column contains the B magnitude
    'V' if "mag" column contains the V magnitude
    'P' if "mag" column contains a photographic magnitude
    'D' if "mag" column contains a stellar diameter expressed in mm
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>n_mag</name>
			<definition>Note v=very faint f=faint</definition>
			<units>---</units></field>
		<field>
			<name>mag</name>
			<definition>Stellar magnitude or diameter
	<footnote footnoteId="???"><para>number=1</para>
			<para>x_mag takes the following values:
    'B' if "mag" column contains the B magnitude
    'V' if "mag" column contains the V magnitude
    'P' if "mag" column contains a photographic magnitude
    'D' if "mag" column contains a stellar diameter expressed in mm
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>var</name>
			<definition>v=variable</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right Ascension 1950 (hours)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right Ascension 1950 (minutes)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right Ascension 1950 (seconds)</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination 1950 (sign)</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination 1950 (degrees)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination 1950 (minutes)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination 1950 (seconds)</definition>
			<units>arcsec</units></field>
		<field>
			<name>pmX</name>
			<definition>Proper motion in X</definition>
			<units>10mas/yr</units></field>
		<field>
			<name>pmY</name>
			<definition>Proper motion in Y</definition>
			<units>10mas/yr</units></field>
		<field>
			<name>Pr</name>
			<definition>Membership probabilities</definition>
			<units>---</units></field>
		<field>
			<name>oriNumber</name>
			<definition>The number in the original data</definition>
			<units>---</units></field>
		<field>
			<name>e_pmX</name>
			<definition>Mean error on pmX</definition>
			<units>10mas/yr</units></field>
		<field>
			<name>e_pmY</name>
			<definition>Mean error on pmY</definition>
			<units>10mas/yr</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Francois Ochsenbein, Joseph Florsch</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1995</year><month>Mar</month><day>28</day></date></ingest>
		</history>
	<identifier>I_215.xml</identifier></dataset>
