<?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>Far-ultraviolet stellar photometry: a field in Monoceros</title>
	<altname type="ADC">J/ApJ/408/484</altname>
		<altname type="CDS">J/ApJ/408/484</altname>
		<altname type="brief">Far-UV photometry of a field in Monoceros</altname>
	<reference>
		<source>
<journal>
	<title>Far-ultraviolet stellar photometry: a field in Monoceros</title>
	<author>
			<initial>E</initial>
			<initial>G</initial>
			<lastName>Schmidt</lastName></author>
	<author>
			<initial>G</initial>
			<initial>R</initial>
			<lastName>Carruthers</lastName></author>
	<name>Astrophys. J.</name>
	<volume>408</volume>
	<pageno>484</pageno>
		<date>
			<year>1993</year></date>
	<bibcode>1993ApJ...408..484S</bibcode></journal></source>
	<related>
			<holding role="similar">J/ApJS/89/259 :  another observation in a field in Orion<xlink:simple href="J/ApJS/89/259"/></holding></related></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Photometry_ultraviolet.html">Photometry, ultraviolet</keyword></keywords>
	<descriptions>
				<description>
				<para>
   FUV photometry of stars in a field in Monoceros in the wavelength range
   from 1230 to 1600 A has been carried out using data from an
   electrographic Schmidt camera carried on a sounding rocket. Ultraviolet
   magnitudes were extracted for 602 objects in the field. Fifty-eight
   percent were tentatively identified with visible stars using the SIMBAD
   data base while another 25 percent are blends of objects too close
   together to separate with the resolution used.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1">
	<title>Objects detected in the UV</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>No</name>
			<definition>Number of the star</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right Ascension 1950 (hours)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right Ascension 1950 (minutes)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right Ascension 1950 (seconds)</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination 1950 (sign)</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination 1950 (degrees)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination 1950 (minutes)</definition>
			<units>arcmin</units></field>
		<field>
			<name>m1367</name>
			<definition>Far UV magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>Name</name>
			<definition>Identification (from SIMBAD) of the star</definition>
			<units>---</units></field>
		<field>
			<name>mag</name>
			<definition>V or P magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>n_mag</name>
			<definition>P if mag is photographic</definition>
			<units>---</units></field>
		<field>
			<name>Sp</name>
			<definition>Spectral type</definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Francois Ochsenbein</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1993</year><month>Dec</month><day>23</day></date><acknowledgement>Edward Schmidt (eschmidt@unlinfo.unl.edu)</acknowledgement></ingest>
		</history>
	<identifier>J_ApJ_408_484.xml</identifier></dataset>
