<?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>Triton stellar occultation candidates 1992-1994</title>
	<altname type="ADC">J/AJ/104/862</altname>
		<altname type="CDS">J/AJ/104/862</altname>
		<altname type="brief">Stellar occultation candidates</altname>
	<reference>
		<source>
<journal>
	<title>Triton stellar occultation candidates 1992-1994</title>
	<author>
			<initial>S</initial>
			<initial>W</initial>
			<lastName>McDonald</lastName></author>
	<author>
			<initial>J</initial>
			<initial>L</initial>
			<lastName>Elliot</lastName></author>
	<name>Astron. J.</name>
	<volume>104</volume>
	<pageno>862</pageno>
		<date>
			<year>1992</year></date>
	<bibcode>1992AJ....104..862M</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Occultations.html">Occultations</keyword>
			<keyword xlink:href="Positional_data.html">Positional data</keyword></keywords>
	<descriptions>
				<description>
				<para>
    A search for Triton stellar occultation candidates for the period
    1992-1994 has been completed with CCD strip-scanning observations. The
    search reached an R magnitude of about 17.4 and found 129 candidates
    within 1.5arcsec of Triton's ephemeris during this period. Of these
    events, we expect around 30 occultations to be visible from the Earth,
    indicating that a number of Triton occultation events should be
    visible from major observatories. Even the faintest of our candidate
    events could produce useful occultation data if observed with a large
    enough telescope. Our astrometric accuracy is inadequate to identify
    which of these appulse events will produce occultations on the Earth;
    further astrometry is needed to refine the predictions for positive
    occultation identification. To aid in selecting candidates for
    additional astrometric and photometric studies, we include finder
    charts and Earth-based visibility charts for each event.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table2">
	<title>Possible occultations by Triton</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>ID</name>
			<definition>Star name</definition>
			<units>---</units></field>
		<field>
			<name>AppDate</name>
			<definition>Date of the closest approach</definition>
			<units>"DD/MM/YY"</units></field>
		<field>
			<name>Apph</name>
			<definition>UT time of the closest approach</definition>
			<units>h</units></field>
		<field>
			<name>Appm</name>
			<definition>UT time of the closest approach</definition>
			<units>min</units></field>
		<field>
			<name>SepMin</name>
			<definition>Minimum separation of the closest approach</definition>
			<units>arcsec</units></field>
		<field>
			<name>PA</name>
			<definition>Position angle of Triton relative to the star
                                  at the time of the closest approach</definition>
			<units>deg</units></field>
		<field>
			<name>Rmag</name>
			<definition>CCD magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>Vel</name>
			<definition>Shadow velocity</definition>
			<units>km/s</units></field>
		<field>
			<name>Dist</name>
			<definition>Angular distance between Triton and the Sun</definition>
			<units>deg</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension (J2000) of the star</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension (J2000) of the star</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension (J2000) of the star</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination (J2000) of the star
	<footnote footnoteId="???"><para>number=1</para>
			<para>The declination is also the sub-Earth latitude of the star.
</para></footnote></definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination (J2000) of the star
	<footnote footnoteId="???"><para>number=1</para>
			<para>The declination is also the sub-Earth latitude of the star.
</para></footnote></definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination (J2000) of the star
	<footnote footnoteId="???"><para>number=1</para>
			<para>The declination is also the sub-Earth latitude of the star.
</para></footnote></definition>
			<units>arcsec</units></field>
		<field>
			<name>GLON</name>
			<definition>Sub-Earth longitude of the star</definition>
			<units>deg</units></field>
		<field>
			<name>Strip</name>
			<definition>Strip numbers on which an image of the
                                  candidate star was measured</definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>James Marcout, Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1995</year><month>May</month><day>10</day></date></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para> Keypunched at CDS</para></revision></revisions></history>
	<identifier>J_AJ_104_862.xml</identifier></dataset>
