<?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>Cross identifications in the region of cluster NGC 1502</title>
	<altname type="ADC">J/AJ/114/222</altname>
		<altname type="CDS">J/AJ/114/222</altname>
		<altname type="brief">Cross identifications in NGC 1502</altname>
	<reference>
		<source>
<journal>
	<title>Cross identifications in the region of cluster NGC 1502</title>
	<author>
			<initial>A</initial>
			<initial>J</initial>
			<lastName>Weitenbeck</lastName></author>
	<name>Astron. J.</name>
	<volume>114</volume>
	<pageno>222</pageno>
		<date>
			<year>1997</year></date>
	<bibcode>1997AJ....114..222W</bibcode></journal></source>
	<related>
			<holding role="similar">I/220 : The HST Guide Star Catalog (Lasker+ 1992)<xlink:simple href="I/220"/></holding></related></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="Cross_identifications.html">Cross identifications</keyword></keywords>
	<descriptions>
				<description>
				<para>
    In studying this region Purgathofer (1964AnWie..26...37P) [the SIMBAD
    numbering], Hoag et al.(1961PUSNO..17..343H), and Dombrovskii and
    Hagen-Thorn (1964TrLen..20...75D) each set up their own numbering
    system; subsequent authors used one or another of those or variants or
    combinations.
    The region covered is 2 degrees in diameter, centered at:
    (2000) RA 04 04 53.28 dec +62 19 20.7.
    This is about 15' west of the cluster, the position of HD 25290.</para></description>
                        <details>
	<astroObjects>
		
			<astroObject><name>NGC 1502</name><name>C 0403+622</name><position><ra>04 07.8 </ra><dec>+62 20 </dec></position></astroObject></astroObjects></details></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1">
	<title>Cross Identifications near NGC 1502 by GSC number</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>GSC</name>
			<definition>GSC zone (Cat. &lt;I/220>)</definition>
			<units>---</units></field>
		<field>
			<name>ID</name>
			<definition>Identification number</definition>
			<units>---</units></field>
		<field>
			<name>mag</name>
			<definition>Magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension (J2000.0)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension (J2000.0)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension (J2000.0)</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination (J2000.0)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination (J2000.0)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination (J2000.0)</definition>
			<units>arcsec</units></field>
		<field>
			<name>Name</name>
			<definition>Other name
	<footnote footnoteId="???"><para>number=1</para>
			<para>Designations of the form NGC 1502 NN are from
           Purgathofer (1964AnWie..26...37P), those of the form
           HoagNN and DHNN are from Hoag et al. (1961PUSNO..17..343H) and
           Dombrovskii and Hagen-Thorn (1964TrLen..20...75D).
           Hoag et al. (1961PUSNO..17..343H) give a table of 26 numbered
           stars with photoelectric photometry, and a second, longer,
           unnumbered table of stars with photographic photometry, which
           includes the stars in the other table.  Reiman and Pfau
           (1987AN....308..111R) numbered the stars in the second table
           by continuing the numbering from the first table, calling the
           first star in the second table 27; this system is used here.</para></footnote></definition>
			<units>----</units></field>
		<field>
			<name>Name2</name>
			<definition>Other name
	<footnote footnoteId="???"><para>number=1</para>
			<para>Designations of the form NGC 1502 NN are from
           Purgathofer (1964AnWie..26...37P), those of the form
           HoagNN and DHNN are from Hoag et al. (1961PUSNO..17..343H) and
           Dombrovskii and Hagen-Thorn (1964TrLen..20...75D).
           Hoag et al. (1961PUSNO..17..343H) give a table of 26 numbered
           stars with photoelectric photometry, and a second, longer,
           unnumbered table of stars with photographic photometry, which
           includes the stars in the other table.  Reiman and Pfau
           (1987AN....308..111R) numbered the stars in the second table
           by continuing the numbering from the first table, calling the
           first star in the second table 27; this system is used here.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Name3</name>
			<definition>Other name
	<footnote footnoteId="???"><para>number=1</para>
			<para>Designations of the form NGC 1502 NN are from
           Purgathofer (1964AnWie..26...37P), those of the form
           HoagNN and DHNN are from Hoag et al. (1961PUSNO..17..343H) and
           Dombrovskii and Hagen-Thorn (1964TrLen..20...75D).
           Hoag et al. (1961PUSNO..17..343H) give a table of 26 numbered
           stars with photoelectric photometry, and a second, longer,
           unnumbered table of stars with photographic photometry, which
           includes the stars in the other table.  Reiman and Pfau
           (1987AN....308..111R) numbered the stars in the second table
           by continuing the numbering from the first table, calling the
           first star in the second table 27; this system is used here.</para></footnote></definition>
			<units>----</units></field>
		<field>
			<name>Name4</name>
			<definition>Other name
	<footnote footnoteId="???"><para>number=1</para>
			<para>Designations of the form NGC 1502 NN are from
           Purgathofer (1964AnWie..26...37P), those of the form
           HoagNN and DHNN are from Hoag et al. (1961PUSNO..17..343H) and
           Dombrovskii and Hagen-Thorn (1964TrLen..20...75D).
           Hoag et al. (1961PUSNO..17..343H) give a table of 26 numbered
           stars with photoelectric photometry, and a second, longer,
           unnumbered table of stars with photographic photometry, which
           includes the stars in the other table.  Reiman and Pfau
           (1987AN....308..111R) numbered the stars in the second table
           by continuing the numbering from the first table, calling the
           first star in the second table 27; this system is used here.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Note</name>
			<definition>Note
	<footnote footnoteId="???"><para>number=2</para>
			<para>4067-862 and 4067-873: The 1855 coordinates for BD +61 649 lies almost
           exactly halfway between these two GSC stars. Additionally, 4067-414
           10.8mag, is about 2.6' from the position
          4068-347: This is evidently DH97, though DH do not give a BD number.
           There are no other stars of similar brightness in the vicinity in
           the GSC or on the Palomar Sky Survey.
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table2">
	<title>Cross Identifications near NGC 1502 by cluster
                                member number</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>NGC1502</name>
			<definition>NGC 1502 (1964AnWie..26...37P) identification
                                   number
	<footnote footnoteId="???"><para>number=1</para>
			<para>NGC 1502 1 and 2: There is some confusion in the literature over
           identification of these two similar stars. In SIMBAD the lower
           HD number HD25638 = 1 is east of HD25639 = 2, and all the other
           identifications given there are consistent with this. PPM and DH
           are two of the places with the reverse of SIMBAD.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>m_NGC1502</name>
			<definition>Multiplicity index on NGC1502</definition>
			<units>---</units></field>
		<field>
			<name>Hoag</name>
			<definition>Hoag (1961PUSNO..17..343H) number
	<footnote footnoteId="???"><para>number=2</para>
			<para>These Hoag et al. stars are not in the GSC:
           24, 45, 58, 59, 63, 67, 69, 71, 80, 83, 85, 87, 88, 89, 92, 93, 94.
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Tapia</name>
			<definition>Tapia (1991MNRAS.253..649T) number</definition>
			<units>---</units></field>
		<field>
			<name>DH</name>
			<definition>DH (1964TrLen..20...75D) number</definition>
			<units>---</units></field>
		<field>
			<name>GSC</name>
			<definition>GSC 4068- (Cat. &lt;I/220>) number</definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1997</year><month>Nov</month><day>18</day></date></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para>    It is a pleasure to thank Anthony J. Weitenbeck &lt;ajw@sal.wisc.edu>
    who kindly supplied a copy of this table.</para></revision></revisions></history>
	<identifier>J_AJ_114_222.xml</identifier></dataset>
