<?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>Catalogue of early-type stars measured in a narrow-band photometric system</title>
	<altname type="ADC">2026A</altname>
		<altname type="CDS">II/26A</altname>
		<altname type="brief">Narrow-band photometry of Early-type stars</altname>
	<reference>
		<source>
<journal>
	<title>Catalogue of early-type stars measured in a narrow-band photometric system</title>
	<author>
			<initial>N</initial>
			<lastName>Morguleff</lastName></author>
	<author>
			<initial>M</initial>
			<lastName>Gerbaldi</lastName></author>
	<name>Astron. Astrophys. Suppl. Ser.</name>
	<volume>19</volume>
	<pageno>189</pageno>
		<date>
			<year>1975</year></date>
	<bibcode>1975A&amp;AS...19..189M</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Photometry.html">Photometry</keyword>
			<keyword xlink:href="Stars_early-type.html">Stars, early-type</keyword></keywords>
	<descriptions>
				<description>
				<para>
    A compilation of the photoelectric measurements in the Barbier-Morguleff
    system is presented for 773 stars of spectral types O8 to F6.
    706 stars have been measured at least twice.
    The passbands (in Angstroems) and the mean photometric errors
    of the indexes C(j)-C(2) (in magnitudes) are:
        -----------------------
        Band  Interval    m.e.
        -----------------------
        C(1)  6000-5900  0.0318
        C(2)  5000-4900   ---
        C(3)  4905-4815  0.0073
        C(4)  4380-4310  0.0100
        C(5)  4070-4010  0.0102
        C(6)  3965-3925  0.0201
        C(7)  3780-3720  0.0195
        C(8)  3650-3575  0.0189
        -----------------------</para><para>  Regarding the catalog Pass Bands Morguleff and Gerbaldi (1975) note
  the following:</para><para>     These spectral intervals permit the determination of certain
     physical characteristics .... The pass bands 1 and 5 lead us
     to calculate red and blue gradients. The equivalent widths
     of the H(beta), H(gamma) lines of hydrogen and the K lines of
     Ca II are derived from band 3, 4, and 6. Bands 7 and 8 measure
     the Balmer jump.</para><para>  Listed in the catalog file are the normalized magnitudes corresponding
  to the above pass bands. The normalized magnitude of a pass band,
  C(j), is defined as the color index of the magnitude in the band minus
  the magnitude of the second band, C(2).</para><para>  See Morguleff and Gerbaldi (1975) for a brief discussion of
  conservation of the system and mean errors across all stars.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="catalog.dat">
	<title>The catalogue</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>HD or BD (if starting with a + sign)
                                    identification
	<footnote>
			<para>
  HD or BD number of the object. Only the last two objects have
  BD rather than HD numbers.</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  HD or BD number of the object. Only the last two objects have
  BD rather than HD numbers.</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  The normalized magnitudes in seven of the eight pass bands (see "Pass
  Bands"). C(2) is always equal to zero, by definition.</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Number of measurements contributing to the above values.
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Var</name>
			<definition>'V' indicates a variable star
	<footnote footnoteId="???"><para>number=</para>
			<para>
  HD or BD number of the object. Only the last two objects have
  BD rather than HD numbers.</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  The normalized magnitudes in seven of the eight pass bands (see "Pass
  Bands"). C(2) is always equal to zero, by definition.</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Number of measurements contributing to the above values.
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>c1</name>
			<definition>Index C(1)-C(2).
	<footnote>
			<para>
  The normalized magnitudes in seven of the eight pass bands (see "Pass
  Bands"). C(2) is always equal to zero, by definition.</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  HD or BD number of the object. Only the last two objects have
  BD rather than HD numbers.</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  The normalized magnitudes in seven of the eight pass bands (see "Pass
  Bands"). C(2) is always equal to zero, by definition.</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Number of measurements contributing to the above values.
</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>c3</name>
			<definition>Index C(3)-C(2).
	<footnote footnoteId="???"><para>number=</para>
			<para>
  HD or BD number of the object. Only the last two objects have
  BD rather than HD numbers.</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  The normalized magnitudes in seven of the eight pass bands (see "Pass
  Bands"). C(2) is always equal to zero, by definition.</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Number of measurements contributing to the above values.
</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>c4</name>
			<definition>Index C(4)-C(2).
	<footnote footnoteId="???"><para>number=</para>
			<para>
  HD or BD number of the object. Only the last two objects have
  BD rather than HD numbers.</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  The normalized magnitudes in seven of the eight pass bands (see "Pass
  Bands"). C(2) is always equal to zero, by definition.</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Number of measurements contributing to the above values.
</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>c5</name>
			<definition>Index C(5)-C(2).
	<footnote footnoteId="???"><para>number=</para>
			<para>
  HD or BD number of the object. Only the last two objects have
  BD rather than HD numbers.</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  The normalized magnitudes in seven of the eight pass bands (see "Pass
  Bands"). C(2) is always equal to zero, by definition.</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Number of measurements contributing to the above values.
</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>c6</name>
			<definition>Index C(6)-C(2).
	<footnote footnoteId="???"><para>number=</para>
			<para>
  HD or BD number of the object. Only the last two objects have
  BD rather than HD numbers.</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  The normalized magnitudes in seven of the eight pass bands (see "Pass
  Bands"). C(2) is always equal to zero, by definition.</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Number of measurements contributing to the above values.
</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>c7</name>
			<definition>Index C(7)-C(2).
	<footnote footnoteId="???"><para>number=</para>
			<para>
  HD or BD number of the object. Only the last two objects have
  BD rather than HD numbers.</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  The normalized magnitudes in seven of the eight pass bands (see "Pass
  Bands"). C(2) is always equal to zero, by definition.</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Number of measurements contributing to the above values.
</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>c8</name>
			<definition>Index C(8)-C(2).
	<footnote footnoteId="???"><para>number=</para>
			<para>
  HD or BD number of the object. Only the last two objects have
  BD rather than HD numbers.</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  The normalized magnitudes in seven of the eight pass bands (see "Pass
  Bands"). C(2) is always equal to zero, by definition.</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Number of measurements contributing to the above values.
</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>Obs</name>
			<definition>Number of measurements
	<footnote>
			<para>
  Number of measurements contributing to the above values.
</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  HD or BD number of the object. Only the last two objects have
  BD rather than HD numbers.</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  The normalized magnitudes in seven of the eight pass bands (see "Pass
  Bands"). C(2) is always equal to zero, by definition.</para></footnote>
	<footnote footnoteId="???"><para>number=</para>
			<para>
  Number of measurements contributing to the above values.
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>e_c1</name>
			<definition>Mean error on c1
	<footnote footnoteId="???"><para>number=1</para>
			<para>the mean error is only computed if Obs>1</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>e_c3</name>
			<definition>Mean error on c3
	<footnote footnoteId="???"><para>number=1</para>
			<para>the mean error is only computed if Obs>1</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>e_c4</name>
			<definition>Mean error on c4
	<footnote footnoteId="???"><para>number=1</para>
			<para>the mean error is only computed if Obs>1</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>e_c5</name>
			<definition>Mean error on c5
	<footnote footnoteId="???"><para>number=1</para>
			<para>the mean error is only computed if Obs>1</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>e_c6</name>
			<definition>Mean error on c6
	<footnote footnoteId="???"><para>number=1</para>
			<para>the mean error is only computed if Obs>1</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>e_c7</name>
			<definition>Mean error on c7
	<footnote footnoteId="???"><para>number=1</para>
			<para>the mean error is only computed if Obs>1</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>e_c8</name>
			<definition>Mean error on c8
	<footnote footnoteId="???"><para>number=1</para>
			<para>the mean error is only computed if Obs>1</para></footnote></definition>
			<units>mag</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Francois Ochsenbein</lastName>
				<affiliation>CDS</affiliation></creator>
			<creator>
				<lastName>and N. Paul Kuin</lastName>
				<affiliation>ADC/SSDOO/NASA</affiliation></creator>
	<date>
		<year>1995</year><month>Mar</month><day>29</day></date></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para>  * Catalogue received at CDS in 1975 (punched cards)
  * January 1995: standardised description, added 'V' symbol for
    variable stars listed in the paper.
  * March 1995: included pertinent information from original ADC
    documentation to the catalog by N. Paul Kuin.</para></revision></revisions></history>
	<identifier>II_26A.xml</identifier></dataset>
