<?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>IUE Low-Dispersion Spectra Reference Atlas. I. Normal Stars</title>
	<altname type="ADC">3083</altname>
		<altname type="CDS">III/83</altname>
		<altname type="brief">IUE Low-Dispersion Reference Atlas I, Normal Stars</altname>
	<reference>
		<source>
<journal>
	<title>IUE Low-Dispersion Spectra Reference Atlas. I. Normal Stars</title>
	<author>
			<initial>A</initial>
			<lastName>Heck</lastName></author>
	<author>
			<initial>D</initial>
			<lastName>Egret</lastName></author>
	<author>
			<initial>M</initial>
			<lastName>Jaschek</lastName></author>
	<author>
			<initial>C</initial>
			<lastName>Jaschek</lastName></author>
	<name>Astron. Astrophys. Suppl. Ser.</name>
	<volume>57</volume>
	<pageno>213</pageno>
		<date>
			<year>1984</year></date>
	<bibcode>1984A&amp;AS...57..213H</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Spectrophotometry.html">Spectrophotometry</keyword>
			<keyword xlink:href="Spectra_ultraviolet.html">Spectra, ultraviolet</keyword></keywords>
	<descriptions>
				<description>
				<para>
   The atlas contains the fluxes (2 angstroms/step) of 229 low-dispersion
   stellar spectra collected by the International Ultraviolet Explorer (IUE)
   satellite, compiled for the purpose of establishing reference spectral
   sequences in the ultraviolet range.  The sequences have been constructed
   and the standard stars selected directly from the ultraviolet material,
   staying as far as possible within the general MK frame.  The catalog is
   essentially composed of stars exhibiting normal behaviour in the
   ultraviolet.  A few peculiar objects have, however, been included as an
   illustration of typical abnormalities.  This work clearly pointed out the
   dangers of extrapolating a spectral classification based on a given
   wavelength range to another one, and, in particular, of using the MK
   spectral type alone outside its definition range.</para></description>
                        <details><para><observatory base="space"> IUE</observatory></para></details></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="catalog.dat">
	<title>Calibrated fluxes for each source</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>ID</name>
			<definition>Identification of the star (preferably HD)
	<footnote>
			<para>
   Each star occupies 205 records of the catalog. ID is repeated. For a list
     of the sources in order of appearance in this file, please see
     sources.dat.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Fmax</name>
			<definition>Maximum flux on plot
	<footnote>
			<para>
   Value used as maximum on the y-axis when plotting the spectrum for the
     atlas. Repeated on each line for same star.
   (unit : 10-14 erg cm-2 A-1 s-1)</para></footnote></definition>
			<units>10-17W/m2/A</units></field>
		<field>
			<name>Num</name>
			<definition>Record number for the star</definition>
			<units>---</units></field>
		<field>
			<name>Lambda</name>
			<definition>Wavelength for first flux value in record</definition>
			<units>0.1nm</units></field>
		<field>
			<name>Flux1</name>
			<definition>Calibrated absolute fluxes
                                       (erg s-1 cm-2 A-1)
	<footnote>
			<para>
   Each star has fluxes given for wavelengths 1153A to 3201A stepped by 2A.
     Five fluxes are given per record. The 205 records for each star are
     labeled in the Num field.
</para></footnote></definition>
			<units>mW/m2/A</units></field>
		<field>
			<name>Flux2</name>
			<definition>Flux for ({Lambda} + 2A)</definition>
			<units>mW/m2/A</units></field>
		<field>
			<name>Flux3</name>
			<definition>Flux for ({Lambda} + 4A)</definition>
			<units>mW/m2/A</units></field>
		<field>
			<name>Flux4</name>
			<definition>Flux for ({Lambda} + 6A)</definition>
			<units>mW/m2/A</units></field>
		<field>
			<name>Flux5</name>
			<definition>Flux for ({Lambda} + 8A)</definition>
			<units>mW/m2/A</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="sources.dat">
	<title>List of sources</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>RAh</name>
			<definition>Right Ascension 2000 (hours)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right Ascension 2000 (minutes)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right Ascension 2000 (seconds)</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination 2000 (sign)</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination 2000 (degrees)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination 2000 (minutes)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination 2000 (seconds)</definition>
			<units>arcsec</units></field>
		<field>
			<name>ID</name>
			<definition>Identification of the star
                                            (preferably HD)</definition>
			<units>---</units></field>
		<field>
			<name>Fmax</name>
			<definition>Maximum flux on atlas plot of spectrum</definition>
			<units>10-17W/m2/Angstroem</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Julie Anne Watko</lastName>
				<affiliation>SSDOO/ADC</affiliation></creator>
	<date>
		<year>1997</year><month>Jan</month><day>02</day></date></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para>  Francois Ochsenbein [CDS]   03-Dec-1993
  The original file has been transformed to allow easier computer reading:
  the redundant 1025 wavelength values (1153 to 3201 stepped by 2) were removed,
  floating-point numbers were normalized with the addition of the "E" between
  the mantissa and the exponent.

  Julie Anne Watko [ADC]   02-JAN-1997
  The data file had been formatted with one line per star. The old 10270 byte
  records were difficult to read on some computers. Fluxes were reformatted
  to accommodate an 80 byte logical record length. Running numbers and
  wavelengths were added. sources.dat was created, and the Intro document
  from CDS was updated.

  The 2000-position of stars was added at CDS (F.O., 08-Oct-1997)</para></revision></revisions></history>
	<identifier>III_83.xml</identifier></dataset>
