<?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>F5 and Later Stars in Selected Areas 28, 54, 106, 107</title>
	<altname type="ADC">3012A</altname>
		<altname type="CDS">III/12A</altname>
		<altname type="brief">F5 and Later Stars in SA28, 54, 106, 107</altname>
	<reference>
		<source>
<journal>
	<title>F5 and Later Stars in Selected Areas 28, 54, 106, 107</title>
	<author>
			<initial>A</initial>
			<initial>R</initial>
			<lastName>Upgren</lastName>
			<suffix>Jr.</suffix></author>
	<author>
			<initial>R</initial>
			<initial>T</initial>
			<lastName>Staron</lastName></author>
	<name>Astrophys. J. Suppl.</name>
	<volume>19</volume>
	<pageno>367</pageno>
		<date>
			<year>1970</year></date>
	<bibcode>1970ApJS...19..367U</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Selected_areas.html">Selected areas</keyword></keywords>
	<descriptions>
				<description>
				<para>
  The catalog is an objective-prism survey of 2181 stars later than
  spectral class F2; the earlier stars are in catalog ADC# 3011A.  The
  limiting magnitude is about 11.5.  Four regions of intermediate
  galactic latitude are included in this survey.  Each region is
  centered on one of the Selected Areas 28, 54, 106, and 107 and
  consists of a square 7 degrees on a side or about 50 square degrees
  in area.  The fields, 4 x 4 degrees in size, were each photographed
  on two IIa-O emulsion plates, one with an exposure time of three
  minutes on which bright stars could be classified and one with an
  exposure time of 40 minutes extending to faint stars.  The plates
  were taken with the 24-inch Baker-Schmidt telescope of the Dyer
  Observatory.  The dispersion of the objective prism is about 330
  A/mm at H-gamma.  The stars were classified according to the
  criteria established by Nassau and Seyfert (1946) and Nassau and van
  Albada (1947). Photographic magnitudes were found from direct IIa-O
  plates taken with the 8-inch Ross camera of the Yale University
  Observatory. The catalog includes BD numbers, magnitudes, and
  spectral classes for BD stars.  For non BD stars, the BD number
  listed in bytes 1-3 indicates a nearby BD star from which the star
  listed is offset by the values in bytes 5-12 and 15-17 given in
  minutes of arc.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="bdstars.dat">
	<title>catalog data for BD stars</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>AreaNum</name>
			<definition>Selected Area number</definition>
			<units>---</units></field>
		<field>
			<name>BD</name>
			<definition>BD number</definition>
			<units>---</units></field>
		<field>
			<name>PhotoMag</name>
			<definition>Photographic magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>u_PhotoMag</name>
			<definition>Colon for uncertainty in photographic
                                   magnitude</definition>
			<units>---</units></field>
		<field>
			<name>SpTemp</name>
			<definition>Spectral type, temperature class and subclass</definition>
			<units>---</units></field>
		<field>
			<name>u_SpTemp</name>
			<definition>Colon for uncertainty in temperature
                                   class/subclass</definition>
			<units>---</units></field>
		<field>
			<name>LumCl</name>
			<definition>luminosity class</definition>
			<units>---</units></field>
		<field>
			<name>u_LumCl</name>
			<definition>Colon for uncertainty in luminosity class</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="nonbd.dat">
	<title>data for non-BD stars</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>AreaNum</name>
			<definition>Selected Area number</definition>
			<units>---</units></field>
		<field>
			<name>BD</name>
			<definition>BD number of nearby star</definition>
			<units>---</units></field>
		<field>
			<name>RAoffset</name>
			<definition>Right ascension offset from BD star given in
                                    bytes 5-12, minutes of arc</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEoffset</name>
			<definition>Declination offset from BD star given in
                                    bytes 5-12, minutes of arc</definition>
			<units>arcmin</units></field>
		<field>
			<name>PhotoMag</name>
			<definition>Photographic magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>u_PhotoMag</name>
			<definition>Colon for uncertainty in photographic
                                    magnitude</definition>
			<units>---</units></field>
		<field>
			<name>SpTemp</name>
			<definition>Spectral type, temperature class and subclass</definition>
			<units>---</units></field>
		<field>
			<name>u_SpTemp</name>
			<definition>Colon for uncertainty in temperature
                                    class/subclass</definition>
			<units>---</units></field>
		<field>
			<name>LumCl</name>
			<definition>luminosity class</definition>
			<units>---</units></field>
		<field>
			<name>u_LumCl</name>
			<definition>Colon for uncertainty in luminosity class</definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>C.-H. Joseph Lyu</lastName>
				<affiliation>Hughes STX/NASA</affiliation></creator>
	<date>
		<year>1995</year><month>Jun</month><day>10</day></date></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para>  This survey is part of a study of stellar densities with a view
  toward determining the inclination to the galactic plane of
  surfaces of equal stellar density.
  Data format modified at the Astronomical Data Center (ADC)/NASA GSFC,
  1988 June...WHW</para></revision></revisions></history>
	<identifier>III_12A.xml</identifier></dataset>
