<?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>uvby-beta photometry of all stars earlier than G0 and brighter than
m_pg = 10.3 mag in Selected Area 194</title>
	<altname type="ADC">J/A+AS/104/9</altname>
		<altname type="CDS">J/A+AS/104/9</altname>
		<altname type="brief">uvby-beta photometry of all stars earlier than G0</altname>
	<reference>
		<source>
<journal>
	<title>uvby-beta photometry of all stars earlier than G0 and brighter than
m_pg = 10.3 mag in Selected Area 194</title>
	<author>
			<initial>G</initial>
			<initial>A</initial>
			<initial>P</initial>
			<lastName>Franco</lastName></author>
	<name>Astron. Astrophys. Suppl. Ser.</name>
	<volume>104</volume>
	<pageno>9</pageno>
		<date>
			<year>1994</year></date>
	<bibcode>1994A&amp;AS..104....9F</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="dust_extinction.html">dust, extinction</keyword>
			<keyword xlink:href="ISM_clouds.html">ISM: clouds</keyword>
			<keyword xlink:href="ISM_individual_(Southern_Coalsack).html">ISM: individual (Southern Coalsack)</keyword>
			<keyword xlink:href="surveys.html">surveys</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
   Four-colour and H{beta} photometry is introduced for 594 stars earlier than
   G0 in the Kapteyn's Selected Area 194. The results give V, b-y, m_1_, c_1_,
   and {beta} on the standard systems, with overall rms errors for one
   observation of one star of 0.009mag, 0.004mag, 0.006mag, 0.009mag, and
   0.009mag, respectively. The data cover an area of about 5deg x 5deg and is
   intended for an investigation of the distribution of the interstellar
   medium toward the northern part of the Southern Coalsack and its
   surroundings. A comparison to earlier results obtained by other authors has
   shown that the c_1_ indices obtained for the late type stars were
   underestimated, in average, by 0.020mag. Since such difference may account
   for an error of little more than 10% in the estimated stellar distances, a
   correction was applied to the c_1_ index of these stars.</para></abstract>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1">
	<title>uvby-beta photometry of 594 stars in SA 194</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Star identification in the Potsdam-Spektral
                                   Durchmusterung of the Kapteyn's SA 194</definition>
			<units>---</units></field>
		<field>
			<name>HD</name>
			<definition>HD number</definition>
			<units>---</units></field>
		<field>
			<name>MK</name>
			<definition>Michigan two dimensional classification
	<footnote footnoteId="???"><para>number=1</para>
			<para>
 Houk N. &amp; Cowley A.P. 1975, Univeresity of Michigan Catalogue of
  Two-Dimensional Spectrl Types for HD Stars, Univ. of Michigan,
  Ann Arbor, Vol.1
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right Ascension 1900.0</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right Ascension 1900.0</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right Ascension 1900.0</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination 1900.0</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination 1900.0</definition>
			<units>arcmin</units></field>
		<field>
			<name>V</name>
			<definition>computed V magnitude on the Johnson system</definition>
			<units>mag</units></field>
		<field>
			<name>e_V</name>
			<definition>mean error of V</definition>
			<units>0.001mag</units></field>
		<field>
			<name>n_V</name>
			<definition>When *, the star is probably variable</definition>
			<units>---</units></field>
		<field>
			<name>(b-y)</name>
			<definition>(b-y) colour index</definition>
			<units>mag</units></field>
		<field>
			<name>e_(b-y)</name>
			<definition>mean error of (b-y)</definition>
			<units>0.001mag</units></field>
		<field>
			<name>m1</name>
			<definition>colour indices difference m1</definition>
			<units>mag</units></field>
		<field>
			<name>e_m1</name>
			<definition>mean error of m1</definition>
			<units>0.001mag</units></field>
		<field>
			<name>c1</name>
			<definition>colour indices difference c1</definition>
			<units>mag</units></field>
		<field>
			<name>e_c1</name>
			<definition>mean error of c1</definition>
			<units>0.001mag</units></field>
		<field>
			<name>o_ubvy</name>
			<definition>Number of observations in uvby</definition>
			<units>---</units></field>
		<field>
			<name>Hbeta</name>
			<definition>Hbeta index</definition>
			<units>mag</units></field>
		<field>
			<name>e_Hbeta</name>
			<definition>mean error of Hbeta</definition>
			<units>0.001mag</units></field>
		<field>
			<name>o_Hbeta</name>
			<definition>Number of observations in Hbeta</definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1994</year><month>Mar</month><day>21</day></date></ingest>
		</history>
	<identifier>J_A+AS_104_9.xml</identifier></dataset>
