July 7, 2020 Dataset Open Access

Jane Huang

DataCite XML Export

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  <identifier identifierType="DOI">10.5281/zenodo.3928862</identifier>
  <creators>
    <creator>
      <creatorName>Jane Huang</creatorName>
      <affiliation>Center for Astrophysics | Harvard &amp; Smithsonian</affiliation>
    </creator>
  </creators>
  <titles>
    <title>Data from "Large-scale CO spirals and complex kinematics associated with the T Tauri star RU Lup"</title>
  </titles>
  <publisher>Zenodo</publisher>
  <publicationYear>2020</publicationYear>
  <subjects>
    <subject>ALMA</subject>
    <subject>protoplanetary disks</subject>
    <subject>RU Lup</subject>
  </subjects>
  <dates>
    <date dateType="Issued">2020-07-07</date>
  </dates>
  <language>en</language>
  <resourceType resourceTypeGeneral="Dataset"/>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://zenodo.org/record/3928862</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.5281/zenodo.3928861</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="https://creativecommons.org/licenses/by/4.0/legalcode">Creative Commons Attribution 4.0 International</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">&lt;p&gt;Image cubes, self-calibrated visibilities, and self-calibration and imaging scripts for data from Huang et al., 2020, &amp;quot;Large-scale CO spirals and complex kinematics associated with the T Tauri star RU Lup,&amp;quot; accepted for publication by The Astrophysical Journal, arXiv:2007.02974&amp;nbsp;&lt;/p&gt;

&lt;p&gt;The raw ALMA data can be found at the ALMA archive under program ID 2018.1.01201.S (PI: Jane Huang).&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;Scripts:&lt;/strong&gt;&lt;/p&gt;

&lt;p&gt;selfcal_C43-5.py, selfcal_C43-2.py, selfcal_ACA.py: self-calibration scripts for observation of RU Lup in various ALMA configurations&lt;/p&gt;

&lt;p&gt;imaging.py: imaging script used for all lines&lt;/p&gt;

&lt;p&gt;reductionutils.py can be downloaded from&amp;nbsp;&lt;a href="https://zenodo.org/record/3628656"&gt;https://zenodo.org/record/3628656&lt;/a&gt;&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;Measurement sets:&lt;/strong&gt;&lt;/p&gt;

&lt;p&gt;RULupcontinuum.ms.tgz: Continuum visibilities for &amp;quot;RULupallcontinuum.image.pbcor.fits&amp;quot; (the high-resolution ALMA continuum data can be found on the &lt;a href="https://bulk.cv.nrao.edu/almadata/lp/DSHARP/"&gt;DSHARP&lt;/a&gt; page)&lt;/p&gt;

&lt;p&gt;RULup_12CO.ms.contsub.tgz: Continuum-subtracted visibilities for the &lt;sup&gt;12&lt;/sup&gt;CO J=2-1 line toward RU Lup&lt;/p&gt;

&lt;p&gt;RULup_12CO_nocontsub.ms.tgz: Visibilities for the &lt;sup&gt;12&lt;/sup&gt;CO J=2-1 line (no continuum subtraction) toward RU Lup, used to make the &amp;#39;RULup_12COpeakintensity.fits&amp;#39; file.&lt;/p&gt;

&lt;p&gt;RULup_13CO.ms.contsub.tgz: Continuum-subtracted visibilities for the &lt;sup&gt;13&lt;/sup&gt;CO J=2-1 line toward RU Lup&lt;/p&gt;

&lt;p&gt;RULup_C18O.ms.contsub.tgz: Continuum-subtracted visibilities for the C&lt;sup&gt;18&lt;/sup&gt;O J=2-1 line toward RU Lup&lt;/p&gt;

&lt;p&gt;RULup_DCOp.ms.contsub.tgz: Continuum-subtracted visibilities for the&amp;nbsp; DCO&lt;sup&gt;+&lt;/sup&gt; J=3-2 line toward RU Lup&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;Images: &lt;/strong&gt;&lt;/p&gt;

&lt;p&gt;RULup12CO.1sigcut.pbcor.mom0.fits: Integrated intensity map of &lt;sup&gt;12&lt;/sup&gt;CO J=2-1 appearing in Fig. 1&lt;/p&gt;

&lt;p&gt;RULup12CO.pbcor.mom1.fits: &lt;sup&gt;12&lt;/sup&gt;CO J=2-1 intensity-weighted velocity map appearing in Fig. 1&lt;/p&gt;

&lt;p&gt;RULup13CO.pbcor.mom0.fits: Integrated intensity map of &lt;sup&gt;13&lt;/sup&gt;CO J=2-1 appearing in Fig. 1&lt;/p&gt;

&lt;p&gt;RULup13CO.pbcor.mom1.fits: &lt;sup&gt;13&lt;/sup&gt;CO J=2-1 intensity-weighted velocity map appearing in Fig. 1&lt;/p&gt;

&lt;p&gt;RULupC18O.pbcor.mom0.fits: Integrated intensity map of C&lt;sup&gt;18&lt;/sup&gt;O J=2-1 appearing in Fig. 1&lt;/p&gt;

&lt;p&gt;RULupC18O.pbcor.mom1.fits: C&lt;sup&gt;18&lt;/sup&gt;O J=2-1 intensity-weighted velocity map appearing in Fig. 1&lt;/p&gt;

&lt;p&gt;RULup12CO.image.pbcor.fits: &lt;sup&gt;12&lt;/sup&gt;CO J=2-1 image cube appearing in Fig. 2&lt;/p&gt;

&lt;p&gt;RULupC18O.image.pbcor.fits: C&lt;sup&gt;18&lt;/sup&gt;O J=2-1 image cube appearing in Fig. 2&lt;/p&gt;

&lt;p&gt;RULup13CO.image.pbcor.fits: &lt;sup&gt;12&lt;/sup&gt;CO J=2-1 image cube appearing in Fig. 3&lt;/p&gt;

&lt;p&gt;RULup_12COpeakintensity.fits: Peak intensity image of &lt;sup&gt;12&lt;/sup&gt;CO used to make Figure 4&lt;/p&gt;

&lt;p&gt;RULupDCOp.pbcor.mom0.fits: Integrated intensity map of DCO&lt;sup&gt;+&lt;/sup&gt; J=3-2 appearing in Fig. 10&lt;/p&gt;

&lt;p&gt;RULupDCOp.image.pbcor.fits: DCO&lt;sup&gt;+&lt;/sup&gt; J=3-2 image cube appearing in Fig. 11&lt;/p&gt;

&lt;p&gt;RULupallcontinuum.image.pbcor.fits: Continuum image appearing in Fig. 12&lt;/p&gt;

&lt;p&gt;RULup12COinitial.mask.image.fits: &lt;sup&gt;12&lt;/sup&gt;CO CLEAN mask shown in Fig. 13&lt;/p&gt;

&lt;p&gt;&amp;nbsp;&lt;/p&gt;</description>
  </descriptions>
</resource>