<?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>WIYN Open Cluster Study 1: Deep Photometry of NGC 188</title>
	<altname type="ADC">J/AJ/116/1789</altname>
		<altname type="CDS">J/AJ/116/1789</altname>
		<altname type="brief">VI Photometry of NGC 188</altname>
	<reference>
		<source>
<journal>
	<title>WIYN Open Cluster Study 1: Deep Photometry of NGC 188</title>
	<author>
			<initial>T</initial>
			<lastName>von Hippel</lastName></author>
	<author>
			<initial>A</initial>
			<lastName>Sarajedini</lastName></author>
	<name>Astron. J.</name>
	<volume>116</volume>
	<pageno>1789</pageno>
		<date>
			<year>1998</year></date>
	<bibcode>1998AJ....116.1789V</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="Photometry.html">Photometry</keyword></keywords>
	<descriptions>
				<description>
				<para>
     We present V and I broad-band photometry on the Johnson-Kron-Cousins
     (Landolt 1992) system for the central 6.7' x 6.7' field of the old open
     cluster NGC 188.  Only objects with a probability of >= 95% of
     being stellar based on SExtractor (Bertin &amp; Arnouts 1996) analysis of
     0.7" I-band images are presented.  The resulting photometry of 750
     sources spans the range from V = 14 (just above the turn-off) to V =
     26.  We estimate the external accuracy (tie to the Landolt system) to
     be &lt;= 0.01 mag for the brightest stars (V &lt; 17) and &lt;= 0.032 mag for
     the fainter stars blueward of V-I = 2.  Stars redder than V-I = 2
     required an extrapolation of our standard star solution.  Equatorial
     coordinates for equinox J2000 and epoch 1996.10 were kindly derived
     by Imants Platais, Yale University, using 160 reference stars from
     the HST Guide Star Catalog. The standard error of the coordinates is
     0.14", primarily limited by the accuracy of GSC star positions.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="ngc188vi.dat">
	<title>NGC 188 VI photometry data file</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>IAU</name>
			<definition>IAU designation
	<footnote>
			<para>
     The IDs are based on the IAU standard system and include the name of
     our collaboration, WOCS (WIYN Open Cluster Study), followed by J for
     J2000 coordinates, and then the coordinates themselves in RA+Dec
     notation.  For example, our first object is WOCS J0049562+851236 with
     coordinates RA=00:49:56.29 and Dec=+85:12:36.2 (J2000).
-------------------------------------------------------------------------------
References:
   "UBVRI photometric standard stars in the magnitude range 11.5-16.0
   around the celestial equator.", 1992, Landolt, A.U., AJ, 104, 340

   "SExtractor: Software for source extraction.", 1996, Bertin, E.,
   Arnouts, S., 1996, A&amp;AS, 117, 393</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right Ascension hours (J2000)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right Ascension minutes (J2000)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right Ascension seconds (J2000)</definition>
			<units>s</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination degrees (J2000)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination minutes (J2000)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination seconds (J2000)</definition>
			<units>arcsec</units></field>
		<field>
			<name>X</name>
			<definition>CCD X position</definition>
			<units>pix</units></field>
		<field>
			<name>Y</name>
			<definition>CCD Y position</definition>
			<units>pix</units></field>
		<field>
			<name>V</name>
			<definition>V magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>u_V</name>
			<definition>IRAF estimated V magnitude error</definition>
			<units>mag</units></field>
		<field>
			<name>o_V</name>
			<definition>number of V-bandpass measurements</definition>
			<units>---</units></field>
		<field>
			<name>I</name>
			<definition>I magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>u_I</name>
			<definition>IRAF estimated I magnitude error</definition>
			<units>mag</units></field>
		<field>
			<name>o_I</name>
			<definition>number of I-band measurements</definition>
			<units>---</units></field>
		<field>
			<name>prob</name>
			<definition>stellar classification probability</definition>
			<units>%</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Ted von Hippel</lastName>
				<affiliation>NOAO</affiliation></creator>
			<creator>
				<lastName>modified by James E. Gass</lastName>
				<affiliation>SSDOO/ADC</affiliation></creator>
	<date>
		<year>1998</year><month>Oct</month><day>27</day></date></ingest>
		</history>
	<identifier>J_AJ_116_1789.xml</identifier></dataset>
