<?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>New Luyten Catalogue of stars with proper motions larger than two tenths
of an arcsecond (NLTT)</title>
	<altname type="ADC">1098A</altname>
		<altname type="CDS">I/98A</altname>
		<altname type="brief">NLTT Catalogue</altname>
	<reference>
		<source>
<other>
	<title>New Luyten Catalogue of stars with proper motions larger than two tenths
of an arcsecond (NLTT)</title>
	<author>
			<initial>W</initial>
			<initial>J</initial>
			<lastName>Luyten</lastName></author>
	<name>Minneapolis, University of Minnesota</name>
	<publisher>???</publisher>
	<city>???</city>
	
		<date>
			<year>1979</year></date>
	<bibcode>1979</bibcode></other>
<other>
	<title>New Luyten Catalogue of stars with proper motions larger than two tenths
of an arcsecond (NLTT)</title>
	<author>
			<initial>W</initial>
			<initial>J</initial>
			<lastName>Luyten</lastName></author>
	<author>
			<initial>H</initial>
			<initial>S</initial>
			<lastName>Hughes</lastName></author>
	<name>Proper Motion Survey with the Forty-Eight inch Schmidt Telescope LV</name>
	<publisher>???</publisher>
	<city>???</city>
	
		<date>
			<year>1980</year></date>
	<bibcode>1980LP.....55....1L</bibcode></other></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Proper_motions.html">Proper motions</keyword></keywords>
	<descriptions>
				<description>
				<para>
    The NLTT catalog is a collection of stars with proper motions
    exceeding 0.18"/yr found by Luyten and his coworkers. The First
    Supplement to the NLTT catalog is the result of continued plate
    analysis and contains data for 398 stars with proper motions
    greater than 0.179"/yr. A number of corrections to the data in the
    published catalog have been entered in the machine-readable
    version, including the omission of duplicate entries and those
    stars later determined to show no motion. The catalog contains, in
    addition to the proper motions, 1950 equatorial coordinates, a
    flag indicating the approximate accuracy of the positions,
    estimated red and photographic magnitudes, spectral types, and
    flags indicating a change from the published volume and the
    presence of the star in the supplement.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="catalog.dat">
	<title>The NLTT Catalogue and 1st Supplement</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Star designation
	<footnote footnoteId="???"><para>number=1</para>
			<para>Identifiers without prefixes are DM (Bonner and Cordoba
    Durchmusterungen, written with a colon), or Luyten numbers from the
    Bruce Proper Motion Survey (L numbers) or the Luyten-Palomar Survey
    (LP numbers), the former in zones -45 to -89 deg and the latter in
    zones +89 to -44 deg. Other miscellaneous identifiers (Oxf = Oxford AC,
    Grw = Greenwich AC; U = Upgren; R = Ross, etc...).
    An asterisk (*) in the identification field indicates that a not
    exists in the "notes" file of the catalog.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Hours RA, equinox B1950.0</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Minutes RA, equinox B1950.0</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Seconds RA, equinox B1950.0</definition>
			<units>s</units></field>
		<field>
			<name>RAm2</name>
			<definition>Right ascension, equinox B1950.0,
                                     minutes only</definition>
			<units>min</units></field>
		<field>
			<name>n_RAs</name>
			<definition>Flag on RA: 1 = RA originally
                                     reported in 0.1min</definition>
			<units>---</units></field>
		<field>
			<name>DE-</name>
			<definition>Sign Dec, equinox B1950.0</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Degrees Dec, equinox B1950.0</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Minutes Dec, equinox B1950.0</definition>
			<units>arcmin</units></field>
		<field>
			<name>Rmag</name>
			<definition>Estimated red magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>n_Rmag</name>
			<definition>Flag on Rmag
	<footnote footnoteId="???"><para>number=2</para>
			<para>
    ':' indicates a larger uncertainty
    '+' indicates a mag fainter than reported value
    'v' indicates a known variability</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Ptg</name>
			<definition>Estimated photographic magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>n_Ptg</name>
			<definition>'+' Flag on Ptg
	<footnote footnoteId="???"><para>number=2</para>
			<para>
    ':' indicates a larger uncertainty
    '+' indicates a mag fainter than reported value
    'v' indicates a known variability</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>SpType</name>
			<definition>Spectral type; lowercase letters represent
                                     estimated color classes or ranges.</definition>
			<units>---</units></field>
		<field>
			<name>pm</name>
			<definition>Relative proper motion, equinox B1950.0
	<footnote footnoteId="???"><para>number=3</para>
			<para>
    The total proper motion is reported. The RA/DE proper motions can
    be computed with the formulae
    pmRA = pm.sin(pmPA)             pmDE = pm.cos(pmPA)
</para></footnote></definition>
			<units>arcsec/yr</units></field>
		<field>
			<name>u_pm</name>
			<definition>':' if proper motion is uncertain</definition>
			<units>---</units></field>
		<field>
			<name>pmPA</name>
			<definition>Position angle of PM vector
	<footnote footnoteId="???"><para>number=3</para>
			<para>
    The total proper motion is reported. The RA/DE proper motions can
    be computed with the formulae
    pmRA = pm.sin(pmPA)             pmDE = pm.cos(pmPA)
</para></footnote></definition>
			<units>deg</units></field>
		<field>
			<name>u_pmPA</name>
			<definition>':' if position angle is uncertain</definition>
			<units>---</units></field>
		<field>
			<name>ModFlag</name>
			<definition>'A' indicates data have been changed
                                     (see Appendix A of adc.doc or adc.tex)</definition>
			<units>---</units></field>
		<field>
			<name>SupplFlag</name>
			<definition>'1' indicates a star from First
                                     Supplement (Luyten and Hughes, 1980)</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="remarks.dat">
	<title>Remarks for NLTT stars</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Star designation in one of many catalogs</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Hours RA, equinox B1950.0</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Minutes RA, equinox B1950.0</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Seconds RA, equinox B1950.0</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Sign Dec, equinox B1950.0</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Degrees Dec, equinox B1950.0</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Minutes Dec, equinox B1950.0</definition>
			<units>arcmin</units></field>
		<field>
			<name>Text</name>
			<definition>Note for star in free-form text</definition>
			<units>---</units></field></fields></tableHead>
	
			<textFile xlink:href="adc.doc"><name>adc.doc</name><description><para>Documentation  by Warren et al. (ascii)</para></description></textFile>
			<textFile xlink:href="doc.tex"><name>doc.tex</name><description><para>Documentation  by Warren et al. (LaTeX)</para></description></textFile>
	<history>
		<ingest>
	
			<creator>
				<lastName>Francois Ochsenbein</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1995</year><month>Jun</month><day>27</day></date></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para>  * A large number of corrections were performed at ADC, see section 3
    of "adc.doc" or "doc.tex" files
  * From the "Selected Astronomical Catalogs" Vol. 1 CD-ROM (1992), directory
         /astrom/nltt
  * 30-Jun-1995: bad decimal point (blank or dashed) corrected in records
     9694 (LP 198-153), column DEm
    37692 (LP 381- 80), column pm
    38236 (CD-68:1403), column Rmag
    52719 (LP 983- 71), column DEm</para></revision></revisions></history>
	<identifier>I_98A.xml</identifier></dataset>
