<?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>Improved CCD Standard Fields</title>
	<altname type="ADC">J/PASP/104/553</altname>
		<altname type="CDS">J/PASP/104/553</altname>
		<altname type="brief">CCD Standard Fields</altname>
	<reference>
		<source>
<journal>
	<title>Improved CCD Standard Fields</title>
	<author>
			<initial>S</initial>
			<initial>C</initial>
			<lastName>Odewahn</lastName></author>
	<author>
			<initial>C</initial>
			<lastName>Bryja</lastName></author>
	<author>
			<initial>R</initial>
			<initial>M</initial>
			<lastName>Humphreys</lastName></author>
	<name>Publ. Astron. Soc. Pac.</name>
	<volume>104</volume>
	<pageno>553</pageno>
		<date>
			<year>1992</year></date>
	<bibcode>1992PASP..104..553O</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Photometry_CCD.html">Photometry, CCD</keyword>
			<keyword xlink:href="Stars_standard.html">Stars, standard</keyword></keywords>
	<descriptions>
				<description>
				<para>
   Multiple nights of CCD observations of NGC 7790, NGC 7006, and NGC 4147 are
   combined in order to establish a deep sequence of photometric standards 
   whose errors have been objectively derived through statistical comparisons.
   In addition to extending these previously studied fields to a fainter limit,
   the range in observed color is increased making the mean sequences more 
   suitable for deriving photometric transformation coefficients.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="tables">
	<title>Tables 2, 3 and 4 (NGC 4147, 7006 and 7790)</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Cluster Name</definition>
			<units>---</units></field>
		<field>
			<name>Star</name>
			<definition>Star Number</definition>
			<units>---</units></field>
		<field>
			<name>X</name>
			<definition>(plate coordinate)</definition>
			<units>pix</units></field>
		<field>
			<name>Y</name>
			<definition>(plate coordinate)</definition>
			<units>pix</units></field>
		<field>
			<name>V</name>
			<definition>V magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>e_V</name>
			<definition>mean error (V)</definition>
			<units>mag</units></field>
		<field>
			<name>o_V</name>
			<definition>Number of observations (V)</definition>
			<units>---</units></field>
		<field>
			<name>(B-V)</name>
			<definition>B-V</definition>
			<units>mag</units></field>
		<field>
			<name>e_(B-V)</name>
			<definition>mean error  (B-V)</definition>
			<units>mag</units></field>
		<field>
			<name>o_(B-V)</name>
			<definition>Number of observations (B-V)</definition>
			<units>---</units></field>
		<field>
			<name>(V-R)</name>
			<definition>V-R</definition>
			<units>mag</units></field>
		<field>
			<name>e_(V-R)</name>
			<definition>mean error  (V-R)</definition>
			<units>mag</units></field>
		<field>
			<name>o_(V-R)</name>
			<definition>Number of observations (V-R)</definition>
			<units>---</units></field></fields></tableHead>
	
			<textFile xlink:href="odewahn.tex"><name>odewahn.tex</name><description><para>ADC Documentation (requires "adc.sty")</para></description></textFile>
	<history>
		<ingest>
	
			<creator>
				<staff/>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1993</year><month>Jul</month><day>28</day></date></ingest>
		</history>
	<identifier>J_PASP_104_553.xml</identifier></dataset>
