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        <parTitl xml:lang="en">Sunburst Arc Magellan/MagE observations</parTitl>
        <IDNo agency="SND">doi-10-17045-sthlmuni-9907991-0</IDNo>
        <IDNo agency="DOI">https://doi.org/10.17045/STHLMUNI.9907991</IDNo>
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        <producer xml:lang="en" abbr="SND">Swedish National Data Service</producer>
        <producer xml:lang="sv" abbr="SND">Svensk nationell datatjänst</producer>
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      <holdings URI="https://doi.org/10.17045/STHLMUNI.9907991">Landing page</holdings>
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    <citation>
      <titlStmt>
        <titl xml:lang="sv"></titl>
        <parTitl xml:lang="en">Sunburst Arc Magellan/MagE observations</parTitl>
        <IDNo agency="SND">doi-10-17045-sthlmuni-9907991-0</IDNo>
        <IDNo agency="DOI">https://doi.org/10.17045/STHLMUNI.9907991</IDNo>
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        <distrbtr xml:lang="en" abbr="SND" URI="https://snd.se">Swedish National Data Service</distrbtr>
        <distrbtr xml:lang="sv" abbr="SND" URI="https://snd.se">Svensk nationell datatjänst</distrbtr>
        <distDate xml:lang="en" date="2019-09-26" />
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      <holdings URI="https://doi.org/10.17045/STHLMUNI.9907991">Landing page</holdings>
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      <abstract xml:lang="en" contentType="abstract">These are raw data files from the Magellan telescopes, MagE
spectrograph, that are used in Rivera-Thorsen et al. 2019 (Science).  All individual science integrations are included, as well as all the calibration frames: blueflat, redflat, bias, ThAr lamps, order definition flats, and flux calibration stars. Directories include data from three observing runs; the  directory name gives the month and year the observations  were obtained.  All observations are of the galaxy known as the  "Sunburst Arc", discussed in Rivera-Thorsen et al. 2019. 

The slit positions are as follows:- Img 1 / slit H-9 from August 2018
- Img 5 / slit "1" from May 2017
- Img 8   / slit H-2 from April 2018
- Img 10 / slit H-6 from April 2018 
- No LyC   slit H-3 from April 2018

Viewing the data:  Data is stored in the Flexible Image Transport System (FITS) file format[¹], which is designed to store table or binary image data together with an ASCII header containing meta-data stored as a keyword-value pairs, of which some are mandatory and some are optional. 
Multiple software applications exist which can view and analyze FITS files. We recommend either DS9[²], QFitsView[³] or Ginga[⁴] packages, all of which are open source and freely available for both Windows, Mac OS X and GNU/Linux.
Unpacking: The data is compressed in the .tar.gz format, which is natively supported on Mac OS X and GNU/Linux. On Windows, it can be opened with e.g. the 7-Zip software[⁵].
 -------------
[¹]: https://en.wikipedia.org/wiki/FITS[²]: http://ds9.si.edu/site/Home.html[³]: http://www.mpe.mpg.de/~ott/dpuser/qfitsview.html[⁴]: https://ejeschke.github.io/ginga/ 
[⁵]: https://www.7-zip.org/</abstract>
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        <restrctn xml:lang="en">Access to data through an external actor. </restrctn>
        <restrctn xml:lang="sv">Åtkomst till data via extern aktör. </restrctn>
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