<?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>Two-Micron Sky Survey</title>
	<altname type="ADC">2002B</altname>
		<altname type="CDS">II/2B</altname>
		<altname type="brief">Two-Micron Sky Survey</altname>
	<reference>
		<source>
<other>
	<title>Two-Micron Sky Survey</title>
	<author>
			<initial>G</initial>
			<lastName>Neugebauer</lastName></author>
	<author>
			<initial>R</initial>
			<initial>B</initial>
			<lastName>Leighton</lastName></author>
	<name>NASA SP-3047</name>
	<publisher>???</publisher>
	<city>???</city>
	
		<date>
			<year>1969</year></date>
	<bibcode>1969tmss.book.....N</bibcode></other></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Photometry_infrared.html">Photometry, infrared</keyword>
			<keyword xlink:href="Surveys.html">Surveys</keyword></keywords>
	<descriptions>
				<description>
				<para>
   The catalog, giving sources of emission in the 2.2-micrometer region for
   more than 5000 stars, represents a systematic survey of the Northern
   Hemisphere for stars brighter than third magnitude.  The survey was 
   carried out with a telescope at Mount Wilson, California, having a 
   62-inch diameter and an f/l aluminized epoxy mirror mounted 
   equatorially.  Radiation at an effective wavelength of 2.2 micrometers 
   was detected by a lead sulfide photoconductive cell cooled by liquid 
   nitrogen.  In addition to the 2.2-micrometer detector array, radiation 
   at an effective wavelength of 0.84 micrometers was detected by a simple 
   silicon photovoltaic cell.  The catalog includes right ascension and 
   declination (B1950.0), K and I magnitudes, number of measurements, 
   V magnitude, spectral types, cross identifications to the numbering 
   systems of the General Catalogue, the Durchmusterung catalogs, the 
   Bright Star Catalogue, and star names.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="catalog.dat">
	<title>Catalog Data</title></tableLink>
				<tableLink xlink:href="rasort.dat">
	<title>Catalog Data by RA</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>ID</name>
			<definition>Two-Micron Sky Survey number (TMSS)</definition>
			<units>---</units></field>
		<field>
			<name>n_ID</name>
			<definition>Remark
	<footnote>
			<para>
   = 1, if there is a remark; = 0, otherwise</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension 1950 (hours)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension 1950 (minutes)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension 1950 (seconds)</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Sign of declination  </definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination 1950 (degrees)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination 1950 (arc minutes)</definition>
			<units>arcmin</units></field>
		<field>
			<name>u_RAs</name>
			<definition>Right ascension 1950 uncertainty</definition>
			<units>---</units></field>
		<field>
			<name>RAs_X2</name>
			<definition>Right ascension chi-square</definition>
			<units>s</units></field>
		<field>
			<name>u_DEm</name>
			<definition>Declination 1950 uncertainty</definition>
			<units>---</units></field>
		<field>
			<name>DEm_X2</name>
			<definition>Declination chi-square</definition>
			<units>arcmin</units></field>
		<field>
			<name>Kmag</name>
			<definition>K magnitude
	<footnote>
			<para>
   Ignore if byte 76 = 3 or 4.</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>e_Kmag</name>
			<definition>K error (ignore if byte 76 = 3 or 4)</definition>
			<units>mag</units></field>
		<field>
			<name>Kmag_X2</name>
			<definition>K chi-square
	<footnote>
			<para>
   Ignore if byte 76 = 3 or 4.</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>Imag</name>
			<definition>I magnitude
	<footnote>
			<para>
   Ignore if I magnitude > 14.0 and/or ignore if byte 76 = 2 or 4.</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>e_Imag</name>
			<definition>I error
	<footnote>
			<para>
   Ignore if I magnitude > 14.0 and/or ignore if byte 73 = 1 and/or
   ignore if byte 76 = 2 or 4.</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>Imag_X2</name>
			<definition>I chi-square
	<footnote>
			<para>
   Ignore if I magnitude > 14.0 and/or ignore if byte 73 = 1 and/or
   ignore if byte 76 = 2 or 4.</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>n_Imag</name>
			<definition>I magnitude questionable
	<footnote>
			<para>
   = 1, if I magnitude is questionable; = 0, otherwise</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>KIX2</name>
			<definition>I and K chi-square excess
	<footnote>
			<para>
   = 1, if chi-square is not excessive
   = 2, if I chi-square is excessive
   = 3, if K chi-square is excessive
   = 4, if I and K chi-square are excessive</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>n_KIX2</name>
			<definition>I and K scale
	<footnote>
			<para>
   = 1, if I and K both on scale
   = 2, if I off scale
   = 3, if K off scale
   = 4 if both I and K off scale</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>ct_Kmag</name>
			<definition>Number of K measurements</definition>
			<units>ct</units></field>
		<field>
			<name>ct_Imag</name>
			<definition>Number of I measurements</definition>
			<units>ct</units></field>
		<field>
			<name>n_ctmag</name>
			<definition>Remark on K and I counts
	<footnote>
			<para>
   = 1, if there is a remark; = 0, otherwise</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>obs_dates</name>
			<definition>Observational timetable
	<footnote>
			<para> 
   Range of days on which observations were made starting with 
   January 30, 1965, and running through April 7, 1968.</para></footnote></definition>
			<units>d</units></field>
		<field>
			<name>Vmag</name>
			<definition>V magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>SpType</name>
			<definition>Spectral type</definition>
			<units>---</units></field>
		<field>
			<name>Lum</name>
			<definition>Luminosity class
	<footnote>
			<para>
   = 2, luminosity class I and II
   = 3, luminosity class III
   = 4, luminosity class IV
   = 5, luminosity class V
   = 6, luminosity class c
   = 7, luminosity class g 
   = 8, luminosity class d</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>BCS3</name>
			<definition>HR/BS number
	<footnote>
			<para>
   The HR/BS number is provided if identified in the Yale Catalog 
   of Bright Stars, Third edition (1964).</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>GC</name>
			<definition>GC number
	<footnote>
			<para>
   The GC number is provided if identified in the Boss General
   Catalog of 33342 Stars for the Epoch 1950 (1937).</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>SAO</name>
			<definition>DM number
	<footnote>
			<para>
   The DM number is provided if identified in the Smithsonian
   Astrophysical Observatory (SAO) Star Catalog (1966).</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>GCVS</name>
			<definition>Star name
	<footnote>
			<para>
   The star name is provided if identified in the General Catalog 
   of Variable Stars, Volumes 1 and 2 (1958).</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>RAs_SAO</name>
			<definition>RA difference (seconds)
	<footnote>
			<para>
   These are the position differences, infrared catalog-SAO Star Catalog or,
   if no SAO identification is avalable, the position difference, infrared
   catalog-variable star catalog.
   Note:  
   The data file ordered by increasing right ascension (rasort.dat) is 
   also available.

      Declination Zones (degrees)                  Sequential Record Number

            -33 to -25                                        1-472
            -25 to -15                                     473-1116
            -15 to - 5                                    1117-1725
            - 5 to + 5                                    1726-2262
            + 5 to +15                                    2263-2807
            +15 to +25                                    2808-3365
            +25 to +35                                    3366-3887
            +35 to +45                                    3888-4435
            +45 to +55                                    4436-4919
            +55 to +65                                    4920-5353
            +65 to +75                                    5354-5555
            +75 to +81                                    5556-5612
</para></footnote></definition>
			<units>s</units></field>
		<field>
			<name>DEm_dif</name>
			<definition>Declination difference (arc min)</definition>
			<units>arcmin</units></field>
		<field>
			<name>RArad</name>
			<definition>Right ascension 1950 (radians)</definition>
			<units>rad</units></field>
		<field>
			<name>DErad</name>
			<definition>Declination 1950 (radians)</definition>
			<units>rad</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="chisq.dat">
	<title>Chi-square Excess</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>ID</name>
			<definition>Two-Micron Sky Survey number (TMSS)</definition>
			<units>---</units></field>
		<field>
			<name>o_ID</name>
			<definition>Total number of obs. of this star
	<footnote>
			<para>
   Up to three observations are listed in one logical record.  This
   number is repeated in each record containing data for this star.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Kmag</name>
			<definition>K magnitude of star</definition>
			<units>mag</units></field>
		<field>
			<name>std_Kmag</name>
			<definition>Standard deviation of K magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>Imag</name>
			<definition>I magnitude of star
	<footnote>
			<para>
   Ignore if I magnitude > 14.0.</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>std_Imag</name>
			<definition>Standard deviation of I magnitude
	<footnote>
			<para>
   Ignore if I magnitude > 14.0 or if byte 28 = 1.</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>n_Imag</name>
			<definition>I magnitude questionable
	<footnote>
			<para>
   = 1, if I magnitude is questionable; = 0, otherwise
   If I magnitude is 1, then the standard deviation given in bytes 24-27
   should be ignored.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>JD</name>
			<definition>Julian day no. of obs. minus 2430000</definition>
			<units>d</units></field>
		<field>
			<name>Kmag2</name>
			<definition>K magnitude of star
	<footnote>
			<para>
   If more than one observation is included in this record, the format for
   bytes 10-32 is repeated as bytes 34-56.</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>std_Kmag2</name>
			<definition>Standard deviation of K magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>Imag2</name>
			<definition>I magnitude of star
	<footnote>
			<para>
   Ignore if I magnitude > 14.0.</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>std_Imag2</name>
			<definition>Standard deviation of I magnitude
	<footnote>
			<para>
   Ignore if I magnitude > 14.0 or if byte 52 = 1.</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>n_Imag2</name>
			<definition>I magnitude questionable
	<footnote>
			<para>
   = 1, if I magnitude is questionable; = 0, otherwise</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>JD2</name>
			<definition>Julian day no. of obs. minus 2430000</definition>
			<units>d</units></field>
		<field>
			<name>Kmag3</name>
			<definition>K magnitude of star
	<footnote>
			<para>
   If there is a third observation included in this record, the format for
   bytes 10-32 is repeated as bytes 58-80.</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>std_Kmag3</name>
			<definition>Standard deviation of K magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>Imag3</name>
			<definition>I magnitude of star
	<footnote>
			<para>
   Ignore if I magnitude > 14.0.</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>std_Imag3</name>
			<definition>Standard deviation of I magnitude
	<footnote>
			<para>
   Ignore if I magnitude > 14.0 or if byte 76 = 1.</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>n_Imag3</name>
			<definition>I magnitude questionable
	<footnote>
			<para>
   = 1, if I magnitude is questionable; = 0, otherwise
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>JD3</name>
			<definition>Julian day no. of obs. minus 2430000</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="remarks.dat">
	<title>Remarks</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>ID</name>
			<definition>Two-Micron Sky Survey number (TMSS)</definition>
			<units>---</units></field>
		<field>
			<name>n_ID</name>
			<definition>Remarks</definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Melissa C. Larkin</lastName>
				<affiliation>SSDOO/ADC</affiliation></creator>
	<date>
		<year>1997</year><month>May</month><day>27</day></date><acknowledgement>The original ADC documentation (1991) by Theresa A. Nagy was used to
   create this ReadMe file.  She also did the original data reformatting.</acknowledgement></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para>   The Two-Micron Sky Survey Catalogue by G. Neugebauer and R. B. Leighton
      was published in 1969 as a National Aeronautics and Space 
      Administration (NASA) special publication (NASA SP-3047). 
   A computer program was written to perform the following operations on 
      the original version of the catalogue:
        - Convert all "&amp;" to "+"
        - Concatenate left- and right-hand pages into a single data record
            per entry
        - Delete catalogue number from the right-hand page data
        - Add a sequential counter for each record
        - Combine all entries from 12 original files into a single file 
            for data in catalogue
        - Combine all measurements of chi-square excess stars from the
            12 original files into a single sequential file
        - Compute and include right ascension and declination in radians at
            the end of each record in data file
        - Combine all remarks from the 12 original files into a single 
            sequential file
        - Reblock main catalogue from 84 bytes to 17000
        - Change logical record length from 84 to 170 to accommodate 
            re-organization</para></revision></revisions></history>
	<identifier>II_2B.xml</identifier></dataset>

