<?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>A Proper-Motion Membership Study of the Old Open Cluster NGC 188</title>
	<altname type="ADC">J/AJ/111/1205</altname>
		<altname type="CDS">J/AJ/111/1205</altname>
		<altname type="brief">Proper-Motion Membership of Open Cluster NGC 188</altname>
	<reference>
		<source>
<journal>
	<title>A Proper-Motion Membership Study of the Old Open Cluster NGC 188</title>
	<author>
			<initial>D</initial>
			<initial>I</initial>
			<lastName>Dinescu</lastName></author>
	<author>
			<initial>T</initial>
			<initial>M</initial>
			<lastName>Girard</lastName></author>
	<author>
			<initial>W</initial>
			<initial>F</initial>
			<lastName>van Altena</lastName></author>
	<author>
			<initial>T</initial>
			<lastName>Yang</lastName></author>
	<author>
			<initial>Y</initial>
			<initial>-W</initial>
			<lastName>Lee</lastName></author>
	<name>Astron. Journ.</name>
	<volume>111</volume>
	<pageno>1205</pageno>
		<date>
			<year>1996</year></date>
	<bibcode>1996AJ....111.1205D</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 motions have been determined for 1127 stars in
  the field of the open cluster NGC 188 from plates spanning a
  60-year interval, taken with the 76-cm Thaw refractor of the
  Allegheny Observatory. Special attention has been paid to the
  corrections for systematic errors as a function of magnitude and
  color.</para><para>  The study is complete to a magnitude B = 16.2. Also some stars
  brighter than B = 12.5 were eliminated from the study because
  of the large uncertainty in estimating the magnitude equation at
  the bright end. The final relative proper motions have an accuracy
  of 0.5 mas/yr for well-exposed stars. From the cluster membership
  probabilities based on proper motions we obtain 360 cluster
  members, enabling us to better define the color-magnitude diagram.</para><para>  We provide a list of highly probable candidate blue stragglers
  in addition to the sample proposed by Eggen &amp; Sandage (1969).</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table.dat">
	<title>Master table</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>ID</name>
			<definition>identification number (AJ 111, 1205)</definition>
			<units>---</units></field>
		<field>
			<name>IDUP</name>
			<definition>identification number (Upgren at al. AJ 77, 74)</definition>
			<units>---</units></field>
		<field>
			<name>IDS</name>
			<definition>identification number (Sandage ApJ 135, 333)</definition>
			<units>---</units></field>
		<field>
			<name>V</name>
			<definition>V magnitudes (calibrated photographic magnitudes)</definition>
			<units>mag</units></field>
		<field>
			<name>B-V</name>
			<definition>B-V colors</definition>
			<units>mag</units></field>
		<field>
			<name>X</name>
			<definition>X coordinate</definition>
			<units>mm</units></field>
		<field>
			<name>Y</name>
			<definition>Y coordinate</definition>
			<units>mm</units></field>
		<field>
			<name>RAh</name>
			<definition>Right Ascension J2000 (h); mean epoch 1983.91</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right Ascension J2000 (minutes)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right Ascension J2000 (seconds)</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination  J2000 (degrees)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination  J2000 (arcminutes)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination  J2000 (arcseconds)</definition>
			<units>arcsec</units></field>
		<field>
			<name>pmX</name>
			<definition>Proper Motion in X (milliarcseconds/yr)</definition>
			<units>mas/yr</units></field>
		<field>
			<name>pmY</name>
			<definition>Proper Motion in Y</definition>
			<units>mas/yr</units></field>
		<field>
			<name>e_pmX</name>
			<definition>Proper-motion error in X</definition>
			<units>mas/yr</units></field>
		<field>
			<name>e_pmY</name>
			<definition>Proper-motion error in Y</definition>
			<units>mas/yr</units></field>
		<field>
			<name>Pc</name>
			<definition>Proper-motion membership probability</definition>
			<units>%</units></field>
		<field>
			<name>Pcx</name>
			<definition>Proper-motion and spatial (combined) membership
                                 probability</definition>
			<units>%</units></field>
		<field>
			<name>N</name>
			<definition>Number of plates on which the object was measured</definition>
			<units>---</units></field>
		<field>
			<name>Notes</name>
			<definition>Explained at the end of the table
	<footnote>
			<para>
  1  - photoelectric standards used in the photometric calibration
       (Sandage 77, 74)
  2  - photometry from McClure and Twarog ApJ 214, 111
  3  - photometry replaced from Caputo et al. AJ 99, 261
  4  - stars with no magnitudes estimates from Lick plates which
       were used for the photometry
  5  - stars with only V magnitudes from the Lick plates
  BS - blue stragglers (Eggen and Sandage ApJ 158, 669)
  ER Cep, ES Cep, V5, V8, V9 - short-period variables
                               (Kaluzny and Shara ApJ 314, 585)
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Paul Kuin</lastName>
				<affiliation>NASA/ADC</affiliation></creator>
	<date>
		<year>1997</year><month>May</month><day>19</day></date></ingest>
		</history>
	<identifier>J_AJ_111_1205.xml</identifier></dataset>
