<?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>Spectrophotometric Scans</title>
	<altname type="ADC">3048B</altname>
		<altname type="CDS">III/48B</altname>
		<altname type="brief">Spectrophotometric Scans</altname>
	<reference>
		<source>
<journal>
	<title>Spectrophotometric Scans</title>
	<author>
			<initial>M</initial>
			<lastName>Breger</lastName></author>
	<name>ApJS</name>
	<volume>32</volume>
	<pageno>7</pageno>
		<date>
			<year>1976</year></date>
	<bibcode>1976ApJS...32....7B</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Spectrophotometry.html">Spectrophotometry</keyword></keywords>
	<descriptions>
				<description>
				<para>
   This data set contains 937 sets of spectrophotometric observations of
   stellar continuua made in the 3200-12000A region.  The data were
   transformed to the Hayes and Latham (1975) calibration of Alpha
   Lyrae. Bandpasses vary between 10 and 100A.  An analysis of the
   errors in the catalog appears in Breger (1976).  Note that scans of
   the southern stars observed by Gutierrez-Moreno et al. (1968) are
   NOT corrected for the right ascension effects discussed in Breger
   (1976).</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="catalog.dat">
	<title>Catalog Data</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>StarName</name>
			<definition>Star name</definition>
			<units>---</units></field>
		<field>
			<name>Cat</name>
			<definition>Catalogue number, usually a Harvard Revised
                                     (HR) = Yale Bright Star (YBS) or Henry Draper
                                     (HD) number.</definition>
			<units>---</units></field>
		<field>
			<name>B-V</name>
			<definition>(B-V) color
	<footnote>
			<para>
  (B-V) color taken from the Blanko et al. (1970) UBV Catalogue, the Bright
  Star Catalogue or the original spectrophotometric source.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Sp</name>
			<definition>Spectral type as taken from the same sources
                                     as the B-V color.</definition>
			<units>---</units></field>
		<field>
			<name>BW</name>
			<definition>Bandpass width used; sometimes two
                                     bandpass widths are given and are separated
                                     by a slash ( / )</definition>
			<units>0.1nm</units></field>
		<field>
			<name>Obscode</name>
			<definition>Observer code - (right justified).</definition>
			<units>---</units></field>
		<field>
			<name>Num</name>
			<definition>The number(N) of wavelength (0.1nm)- magnitude
                                     pairs given. If this is less than the maximum
                                     value of 35 the remainder of each logical
                                     record is filled with zeroes.</definition>
			<units>---</units></field>
		<field>
			<name>WaveLen</name>
			<definition>Wavelength</definition>
			<units>0.1nm</units></field>
		<field>
			<name>Mag</name>
			<definition>Magnitude
	<footnote>
			<para>
  The magnitude refers to the conventional magnitude per unit frequency.
</para></footnote></definition>
			<units>mag</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>C.-H. Joseph Lyu</lastName>
				<affiliation>Hughes STX/NASA</affiliation></creator>
	<date>
		<year>1995</year><month>Jun</month><day>22</day></date></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para>  The Catalog of Spectrophotometric Scans of Stars (Breger, M.
  1976, Ap.J. Supp., 32, 7.) was received in machine-readable form
  from Dr. S. Parsons (University of Texas) on March 11, 1976.
  The version as received consisted of a 7-track 800 bpi magnetic
  tape with two files.  The first file contained the analysis
  program as written for the CDC 6600 computer and the second file
  represents the original data.  The analysis program was then
  converted to run on the IBM S/360 at NASA/GSFC and the data was
  processed.  Some corrections to the original analysis program
  had to be made due to the differences in the computers, but since
  the result of the analysis was a listing of the data as given in
  the above reference - checks were possible at every step of the
  analysis.  The output was then reformatted so that the data would
  be in a format that allowed easy access to the data.  As the
  catalogue was checked out, a number of star name errata were noticed.

  A list of Corrected errata in catalogue
  HR Number           Page    Published        Fixed machine-
  Name              Number    Catalogue        readable record
  HR    718             14       X12    CET     XI2 CET
  HR    984             17   EPSILON    ERI    ZETA ERI
  HR    5843            58        XI    SER     CHI SER
  HR    6493            63     55 XI    SER       blank
  KAPPA VEL             40        HR   3731      HR 3734
  HR    3659            39     ALPHA    CAR       a  CAR
  HR    8937            85      BETA    SCI    BETA  SCL
  HR    8937            85      BETA    SCI    BETA  SCL
  DELTA ORI             27        HR 1851-2      HR 1851
  XI    SCO             59        HR 5977/8      HR 5977
  Note: A lower case a was used for star HR 3659 (a CAR)
--------------------------------------------------------------------------------</para></revision></revisions></history>
	<identifier>III_48B.xml</identifier></dataset>
