<?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>Moderate-resolution spectral standards from 560 to 900 nm</title>
	<altname type="ADC">J/AJ/109/1379</altname>
		<altname type="CDS">J/AJ/109/1379</altname>
		<altname type="brief">Praesepe &amp; M 67 spectral standards</altname>
	<reference>
		<source>
<journal>
	<title>Moderate-resolution spectral standards from 560 to 900 nm</title>
	<author>
			<initial>L</initial>
			<initial>E</initial>
			<lastName>Allen</lastName></author>
	<author>
			<initial>K</initial>
			<initial>M</initial>
			<lastName>Strom</lastName></author>
	<name>Astron. J.</name>
	<volume>109</volume>
	<pageno>1379</pageno>
		<date>
			<year>1995</year></date>
	<bibcode>1995AJ....109.1379A</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="MK_spectral_classification.html">MK spectral classification</keyword>
			<keyword xlink:href="Photometry.html">Photometry</keyword></keywords>
	<descriptions>
				<description>
				<para>
    We present a grid of stellar classification spectra of moderate
    resolution (R~1500) in the range lambda lambda 5600-9000A, compiled
    from high signal-to-noise spectra of 275 stars, most in the open
    clusters Praesepe and M 67. The grid covers dwarfs from types B8
    through M5, giants from G8 through M7, and subgiants from F5 through
    K0. We catalog atomic and molecular absorption features useful for
    stellar classification, and demonstrate the use of
    luminosity-sensitive features to distinguish between late-type dwarf
    and giant stars.</para></description>
                        <details>
	<astroObjects>
		
			<astroObject><name>M 67</name><name>NGC 2682</name><position><ra>08 50.4 </ra><dec>+11 49 </dec></position></astroObject>
			<astroObject><name>M 44</name><name>Praesepe</name><name>NGC 2632</name><position><ra>08 40.4 </ra><dec>+19 40 </dec></position></astroObject></astroObjects></details></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1">
	<title>Spectral standards in Praesepe</title></tableLink>
				<tableLink xlink:href="table2">
	<title>Spectral standards in M 67</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>ID</name>
			<definition>Identification number
	<footnote footnoteId="???"><para>number=1</para>
			<para>In table1, ID from Jones and Stauffer (1991AJ....102.1080J)
          In table2, ID from Sanders (1977A&amp;AS...27...89S)</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>n_ID</name>
			<definition>* when spectrum plotted
	<footnote footnoteId="???"><para>number=2</para>
			<para>*: spectrum plotted in Figure 3 for table1, in Figure 5 for table2.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension (1950)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension (1950)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension (1950)</definition>
			<units>s</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination (1950)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination (1950)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination (1950)</definition>
			<units>arcsec</units></field>
		<field>
			<name>Sp</name>
			<definition>Adopted spectral type</definition>
			<units>---</units></field>
		<field>
			<name>Vmag</name>
			<definition>V magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>B-V</name>
			<definition>B-V color index</definition>
			<units>mag</units></field>
		<field>
			<name>V-I</name>
			<definition>V-I color index</definition>
			<units>mag</units></field>
		<field>
			<name>Prob</name>
			<definition>Probability of membership
	<footnote footnoteId="???"><para>number=3</para>
			<para>In table1, Prob from Jones and Stauffer (1991AJ....102.1080J)
          In table2, Prob from Girard et al. (1989AJ.....98..227G)</para></footnote></definition>
			<units>%</units></field>
		<field>
			<name>r_Vmag</name>
			<definition>BVI photometry reference
	<footnote footnoteId="???"><para>number=4</para>
			<para>0: BVI photometry from Jones and Stauffer (1991AJ....102.1080J)
          1: BV photometry from Girard et al. (1989AJ.....98..227G)
          2: BVI photometry from Montgomery et al. (1993) &lt;J/AJ/106/181></para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Notes</name>
			<definition>Notes
	<footnote footnoteId="???"><para>number=5</para>
			<para>In table1:
            Ab = Abt (1986PASP...98..307A)
            Ba = Barbier (1963POHP....6...36B)
            BB = Boesgaard and Budge (1988ApJ...332..410B)
            Bi = Bidelman (1956PASP...68..318B)
            Bo = Bolte (1991ApJ...376..514B)
            CB = Crawford and Barnes (1969AJ.....74..818C)
          CGal = Corbally and Garrison (1986AJ.....92...90C)
           CGb = Corbally and Garrison (1983JRASC..77...28C)
            Jo = Johnson (1952ApJ...116..640J)
            Po = Popper (1948ApJ...108..490P)
            Re = Rebeirot (1966POHP....8...24R)
            RS = Randich and Schmitt (1994) Cat. &lt;J/A+A/298/115>
            SS = Soderblom and Stauffer (1984AJ.....89.1543S)
            St = Stauffer (1982PASP...94..678S)
            Up = Upgren et al. (1979AJ.....84.1586U)
            Wi = Wilson (1963ApJ...138..832W)
          In table2:
            Identification cross references:
                     F: Fagerholm ID (1906ArMAF...2s...1F)
                   RGO: Royal Greenwich Observatory ID
                     S: Sandage ID
            Previously published spectral types from:
                    BB: Burbidge and Burbidge (1959ApJ...129..513B)
                    Pe: Pesch (1967ApJ...148..781P)
                    Po: Popper (1954AJ.....59..445P)
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table3">
	<title>Additional giants</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Star name</definition>
			<units>---</units></field>
		<field>
			<name>n_Name</name>
			<definition>* when spectrum plotted in Figure 3</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension (1950)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension (1950)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension (1950)</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination (1950)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination (1950)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination (1950)</definition>
			<units>arcsec</units></field>
		<field>
			<name>Sp</name>
			<definition>Spectral type</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table4">
	<title>Spectral features</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Lambda</name>
			<definition>Wavelength</definition>
			<units>0.1nm</units></field>
		<field>
			<name>n_Lambda</name>
			<definition>Separator, '-' for interval</definition>
			<units>---</units></field>
		<field>
			<name>Lambda2</name>
			<definition>Second wavelength</definition>
			<units>0.1nm</units></field>
		<field>
			<name>n_Lambda2</name>
			<definition>Separator</definition>
			<units>---</units></field>
		<field>
			<name>Lambda3</name>
			<definition>Third wavelength</definition>
			<units>0.1nm</units></field>
		<field>
			<name>Ident</name>
			<definition>Identification</definition>
			<units>---</units></field>
		<field>
			<name>Notes</name>
			<definition>Notes</definition>
			<units>---</units></field>
		<field>
			<name>Ref</name>
			<definition>References
	<footnote footnoteId="???"><para>number=1</para>
			<para>1: Torre-Dodgen &amp; Weaver (1993)  &lt;III/181>
          2: Kirkpatrick et al. (1991ApJS...77..417K)
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>James Marcout, Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1996</year><month>Oct</month><day>01</day></date></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para> Prepared via OCR at CDS.</para></revision></revisions></history>
	<identifier>J_AJ_109_1379.xml</identifier></dataset>
