<?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>A photometric study of the open cluster IC 4665</title>
	<altname type="ADC">2194A</altname>
		<altname type="CDS">II/194A</altname>
		<altname type="brief">Photometric study of IC 4665</altname>
	<reference>
		<source>
<journal>
	<title>A photometric study of the open cluster IC 4665</title>
	<author>
			<initial>M</initial>
			<initial>F</initial>
			<initial>S</initial>
			<initial>J</initial>
			<lastName>McCarthy</lastName></author>
	<author>
			<initial>S</initial>
			<initial>S</initial>
			<initial>J</initial>
			<lastName>O'Sullivan</lastName></author>
	<name>Ricerche Astron.</name>
	<volume>7</volume>
	<pageno>483-498</pageno>
		<date>
			<year>1969</year></date>
	<bibcode>1969RA......7..483M</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Clusters_open.html">Clusters, open</keyword>
			<keyword xlink:href="Photographic_catalog.html">Photographic catalog</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
    Photographic observations of the open cluster IC 4665 made on blue
    and yellow sensitive plates with the Vatican 40 cm refractor are
    presented and discussed. Apparent magnitudes were determined for
    200 stars by means of a program of photometric reduction designed
    by BERTIAU. The mean internal errors in the final blue and yellow
    magnitudes average about 0.02 mag. All stars selected for
    measurement of proper motions by VASILEVSKIS on long base-line
    Allegheny plates have been observed here. The forty stars which
    VASILEVSKIS' proper motion measures have shown to be probable
    members constitute a normal main sequence from V = 7 to V = 13.5,
    followed by a gap of 0.2 to 0.3 mag, and a group of 10 stars in
    the subgiant domain. The reality of this gap and the membership
    characteristics of the stars in the subgiant region of the C - M
    diagram are discussed.</para></abstract>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1">
	<title>Standard stars: photoelectric and
                                photographic data compared</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Vno</name>
			<definition>Number on the plate (Vasilevskis)</definition>
			<units>---</units></field>
		<field>
			<name>Kno</name>
			<definition>Number in Kopff</definition>
			<units>---</units></field>
		<field>
			<name>Ano</name>
			<definition>Number in Alcaino</definition>
			<units>---</units></field>
		<field>
			<name>BD</name>
			<definition>Bonner Durchmustering identification</definition>
			<units>---</units></field>
		<field>
			<name>Vpe</name>
			<definition>V photoelectric</definition>
			<units>mag</units></field>
		<field>
			<name>(B-V)pe</name>
			<definition>(B-V) color photoelectric</definition>
			<units>mag</units></field>
		<field>
			<name>Vpg</name>
			<definition>V photographic</definition>
			<units>mag</units></field>
		<field>
			<name>(B-V)pg</name>
			<definition>(B-V) photographic</definition>
			<units>mag</units></field>
		<field>
			<name>Notes</name>
			<definition>Notes as follows:
                                    1 = pe data from Hogg &amp; Kron, AJ 60, 365
                                    2 = pe data from Johnson ApJ 119, 181
                                                        and  ApJ 126, 121
                                    3 = pe data (this paper)
                                    4 = pe data from Coyne (priv. comm.)
                                    5 = not used as yellow standard</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table2">
	<title>General catalogue of stars observed in
                                IC 4665 (Merging of tables 2,3,4)</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Vno</name>
			<definition>Number on the plate (Vasilevskis)</definition>
			<units>---</units></field>
		<field>
			<name>Kno</name>
			<definition>Number in Kopff</definition>
			<units>---</units></field>
		<field>
			<name>Ano</name>
			<definition>Number in Alcaino</definition>
			<units>---</units></field>
		<field>
			<name>BD</name>
			<definition>Bonner Durchmustering identification</definition>
			<units>---</units></field>
		<field>
			<name>B</name>
			<definition>Photographic B</definition>
			<units>mag</units></field>
		<field>
			<name>V</name>
			<definition>photographic V</definition>
			<units>mag</units></field>
		<field>
			<name>(B-V)</name>
			<definition>color</definition>
			<units>mag</units></field>
		<field>
			<name>e_B</name>
			<definition>mean error on B</definition>
			<units>mag</units></field>
		<field>
			<name>e_V</name>
			<definition>mean error on V</definition>
			<units>mag</units></field>
		<field>
			<name>Class</name>
			<definition>1=probable member, 2=Possible member,
                                         3=Less possible member</definition>
			<units>---</units></field>
		<field>
			<name>Notes</name>
			<definition>Notes as follows:
                                   #1 = Less than 6 plates in B determination
                                   #2 = Less than 6 plates in V determination
                                   #3 = Identification from Kopff,
                                        Mitt. Hamburger Sternw. 8, No 52
                                   #4 = Suspected variable
                                   #6 = Photoelectric data from Hogg &amp; Kron,
                                        AJ 60, 365</definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>M.-J. Wagner, James Marcout, Francois Ochsenbein</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1995</year><month>Jun</month><day>12</day></date></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para>  * 02-Jun-1994: Keypunched at CDS, Strasbourg.
         Tables 2, 3 and 4 merged into single file table2.
  * 13-Jun-1995: errors corrected in table2 at CDS
        Star 093   Ano is 25 (instead of 26)
        Star 090   is BD+5 3483 (instead of BD+5 3843)
        Star 105   Ano is 24 (instead of  4)
        Star 033   Kno is 37 (instead of 38)</para></revision></revisions></history>
	<identifier>II_194A.xml</identifier></dataset>
