<?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>UBVRI Photometric Standard Stars Around the Celestial Equator</title>
	<altname type="ADC">2118</altname>
		<altname type="CDS">II/118</altname>
		<altname type="brief">UBVRI Photometric Standard Stars, Celestial Equator</altname>
	<reference>
		<source>
<journal>
	<title>UBVRI Photometric Standard Stars Around the Celestial Equator</title>
	<author>
			<initial>A</initial>
			<initial>U</initial>
			<lastName>Landolt</lastName></author>
	<name>AJ</name>
	<volume>88</volume>
	<pageno>439</pageno>
		<date>
			<year>1983</year></date>
	<bibcode>1983AJ.....88..439L</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Photometry_UBVRI.html">Photometry, UBVRI</keyword>
			<keyword xlink:href="Stars_standard.html">Stars, standard</keyword>
			<keyword xlink:href="Stars_equatorial.html">Stars, equatorial</keyword></keywords>
	<descriptions>
				<description>
				<para>
   The catalog contains UBVRI photoelectric observations of 223 stars,
   mostly in an approximately 2-degree zone centered on the celestial
   equator. The catalog is intended to provide a uniform set of new
   standards, available to various sizes of telescopes in both hemispheres,
   on an internally consistent, homogeneous system. Most of the stars are
   in Selected Areas 92-115 and fall in the magnitude range of about 7 to
   12.5 in V and color range -0.3 to +2.0 in B-V. The data include
   equatorial coordinates, photoelectric magnitudes and colors, numbers of
   observations, and computed internal errors.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="standard.dat">
	<title>Catalog Data</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>cat</name>
			<definition>Catalog abbreviation</definition>
			<units>---</units></field>
		<field>
			<name>ID</name>
			<definition>Number in catalog</definition>
			<units>---</units></field>
		<field>
			<name>supp</name>
			<definition>BD supplement letter (Barnard star)</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension hours (1985.0)
	<footnote>
			<para>
   Positions are for equinox 1985 at epoch. However, proper motions have
   been accounted for in computing the 1985 coordinates for the large
   proper-motion stars, so these positions are given for equinox and epoch
   1985.0.</para></footnote></definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension minutes (1985.0)
	<footnote>
			<para>
   Positions are for equinox 1985 at epoch. However, proper motions have
   been accounted for in computing the 1985 coordinates for the large
   proper-motion stars, so these positions are given for equinox and epoch
   1985.0.</para></footnote></definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension seconds (1985.0)
	<footnote>
			<para>
   Positions are for equinox 1985 at epoch. However, proper motions have
   been accounted for in computing the 1985 coordinates for the large
   proper-motion stars, so these positions are given for equinox and epoch
   1985.0.</para></footnote></definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Sign of declination</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination degrees (1985.0)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination degrees (1985.0)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination degrees (1985.0)</definition>
			<units>arcsec</units></field>
		<field>
			<name>V</name>
			<definition>V magnitude
	<footnote>
			<para>
   Weighted V magnitude on the UBVRI photometric system, as defined by
   stars in Landolt (1973) and Cousins (1976). The colors are similar
   weighted means.</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>B-V</name>
			<definition>B-V color</definition>
			<units>mag</units></field>
		<field>
			<name>U-B</name>
			<definition>U-B color</definition>
			<units>mag</units></field>
		<field>
			<name>V-R</name>
			<definition>V-R color</definition>
			<units>mag</units></field>
		<field>
			<name>R-I</name>
			<definition>R-I color</definition>
			<units>mag</units></field>
		<field>
			<name>V-I</name>
			<definition>V-I color</definition>
			<units>mag</units></field>
		<field>
			<name>o_V</name>
			<definition>Number of observations in weighted means</definition>
			<units>---</units></field>
		<field>
			<name>no_V</name>
			<definition>Number of nights on which star was observed</definition>
			<units>---</units></field>
		<field>
			<name>e_V</name>
			<definition>Mean error of V
	<footnote>
			<para>
   The mean error of a single observation of V or a color can be found by
   multiplying the appropriate error of the mean by the square root of n.</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>e_B-V</name>
			<definition>Mean error of B-V</definition>
			<units>mag</units></field>
		<field>
			<name>e_U-B</name>
			<definition>Mean error of U-B</definition>
			<units>mag</units></field>
		<field>
			<name>e_V-R</name>
			<definition>Mean error of V-R</definition>
			<units>mag</units></field>
		<field>
			<name>e_R-I</name>
			<definition>Mean error of R-I</definition>
			<units>mag</units></field>
		<field>
			<name>e_V-I</name>
			<definition>Mean error of V-I</definition>
			<units>mag</units></field>
		<field>
			<name>n_V</name>
			<definition>Note flag(s)
	<footnote>
			<para>
   Number(s) referring to notes given at the top of the remarks file. These
   notes are distinct from the additional information given in Appendix I,
   which follows the "Notes" section in notes.txt.
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	
			<textFile xlink:href="doc.txt"><name>doc.txt</name><description><para>ASCII version of ADC doc. (more detailed)</para></description></textFile>
			<textFile xlink:href="doc.tex"><name>doc.tex</name><description><para>LaTeX version of ADC document</para></description></textFile>
			<textFile xlink:href="notes.txt"><name>notes.txt</name><description><para>Remarks</para></description></textFile>
	<history>
		<ingest>
	
			<creator>
				<lastName>N. G. Roman</lastName>
				<affiliation>SSDOO/ADC</affiliation></creator>
	<date>
		<year>1997</year><month>May</month><day>27</day></date><acknowledgement>Warren expressed appreciation to A. U. Landolt for providing the catalog
   on magnetic tape and for reviewing and commenting on a preliminary
   version of this document prior to its finalization for distribution with
   the machine-readable catalog. This document has been derived from
   doc.txt.</acknowledgement></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para>   The machine-readable data table UBVRI Photometric Standards Around the
   Celestial Equator was received on magnetic tape from Dr. Arlo U. Landolt
   on 15 April 1986. Various modifications were made by Wayne. H. Warren at
   the ADC in order to effect a uniformly formatted data file, to isolate
   the table notes from the data, and to add the additional information
   contained in Appendix I of the published paper.</para></revision></revisions></history>
	<identifier>II_118.xml</identifier></dataset>
