<?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>Stellar Distribution Near the Selected Areas 127, 141 and 189</title>
	<altname type="ADC">2121</altname>
		<altname type="CDS">II/121</altname>
		<altname type="brief">Stellar Distribution Near SA 127, SA 141, SA 189</altname>
	<reference>
		<source>
<other>
	<title>Stellar Distribution Near the Selected Areas 127, 141 and 189</title>
	<author>
			<initial>K</initial>
			<initial>U</initial>
			<lastName>Ratnatunga</lastName></author>
	<name>Ph.D. Dissertation, The Australian National University, Canberra</name>
	<publisher>???</publisher>
	<city>???</city>
	
		<date>
			<year>1983</year></date>
	<bibcode>1993</bibcode></other></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Selected_areas.html">Selected areas</keyword>
			<keyword xlink:href="Stellar_distribution.html">Stellar distribution</keyword></keywords>
	<descriptions>
				<description>
				<para>
    Photographic photometry and 1950 coordinates were determined using
    Automated Image location on 50 micron aperture PDS scans of the
    regions on UKSTU Schmidt plates. Galaxy contamination, which is
    small at these relatively bright apparent magnitudes, has not been
    removed from the images located. The image locating algorithm does
    not locate faint stars within 9 seconds of arc of an image of a
    brighter star on the plate. Assuming uniform random distributions,
    the estimated incompleteness is 0.5% at magnitude 15 and 2.2% at
    17.5.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="sa127.dat">
	<title>SA 127 field</title></tableLink>
				<tableLink xlink:href="sa141.dat">
	<title>SA 141 field</title></tableLink>
				<tableLink xlink:href="sa189.dat">
	<title>SA 189 field</title></tableLink></tableLinks>
	<fields>
		<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)
	<footnote>
			<para>
  In numerous records the seconds are equal to 60
</para></footnote></definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination 1950 (sign)</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination 1950 (degrees)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination 1950 (minutes)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination 1950 (seconds)</definition>
			<units>arcsec</units></field>
		<field>
			<name>J</name>
			<definition>Photographic J magnitude = V + 0.841*(B-V)</definition>
			<units>mag</units></field>
		<field>
			<name>F</name>
			<definition>Photographic F magnitude = V - 0.605*(B-V)</definition>
			<units>mag</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>C.-H. Lyu</lastName>
				<affiliation>Hughes STX/NASA</affiliation></creator>
			<creator>
				<lastName>and Francois Ochsenbein</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1995</year><month>May</month><day>25</day></date></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para>    Data format modified at the Astronomical Data Center (ADC)/NASA GSFC,
    1991 October...Wayne H. Warren Jr.
    Data description (prepared at the ADC/NASA GSFC from separate descriptions
    supplied by K. U. Ratnatunga, with format description added,
    1991 November...WHW).</para></revision>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para>  Remarks on  Plate Information:
     -----------------------------------------------------------------------------
     J  = IIIa-J KODAK emulsion + 2mm GG395 Schott glass filter  = V + 0.841*(B-V)
     F  = IIIa-F KODAK emulsion + 3mm RG630 Schott glass filter  = V - 0.605*(B-V)
     -----------------------------------------------------------------------------

     ----------------------------------------------------------------------------
     SA  Plate   Observation Air   Exposure  Min Image   Sky    Back    Limiting
         Number     Date     Mass            Diameter   Bright Density  Magnitude
                                   (min)    (microns)  (mag)            (mag)
     ----------------------------------------------------------------------------
     127 J7438S  05-JAN-1982 1.05    15         60       20.5   1.27     19.5
     127 R7407S  20-DEC-1981 1.22    30         85       20.0   0.90     17.7
     141 J7168S  03-JAN-1981 1.00    15         50       21.2   0.44     19.5
     141 R6856S  14-NOV-1980 1.17    12         60       21.3   0.40     17.4
     189 J7227S  30-SEP-1981 1.14    15         35       21.3   0.34     19.5
     189 R7215S  22-SEP-1981 1.16    30         50       20.2   0.74     18.2
     ----------------------------------------------------------------------------

  Remarks on Field Information:
      ------------------------------------------------------------
      SA   l   b   Field            RA   (1950)   Dec    No. stars
           d   d  (sq.deg)    h  m     h  m    d      d
      ------------------------------------------------------------
      127 272 +38   20.9     11 00 to 11 20  -20 to -16    35786
      141 245 -86   22.5     01 00 to 01 20  -32 to -37    13612
      189 277 -50   20.9     02 50 to 03 30  -62 to -58    31088
      ------------------------------------------------------------

    Coordinate calibration used positions of SAO stars.

    Estimated rms accuracy for Best Magnitude range 13.5 &lt; V &lt; 16.0:
        Visual magnitude 0.05 mag
        (B-V)  color     0.07 mag
        Positions        1    second of arc

    *** magnitudes brighter than 12 and fainter than 17.5 inaccurate ***</para></revision></revisions></history>
	<identifier>II_121.xml</identifier></dataset>
