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Data from "Large-scale CO spirals and complex kinematics associated with the T Tauri star RU Lup"

Jane Huang


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        <foaf:name>Jane Huang</foaf:name>
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            <foaf:name>Center for Astrophysics | Harvard &amp; Smithsonian</foaf:name>
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    <dct:title>Data from "Large-scale CO spirals and complex kinematics associated with the T Tauri star RU Lup"</dct:title>
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    <dct:issued rdf:datatype="http://www.w3.org/2001/XMLSchema#gYear">2020</dct:issued>
    <dcat:keyword>ALMA</dcat:keyword>
    <dcat:keyword>protoplanetary disks</dcat:keyword>
    <dcat:keyword>RU Lup</dcat:keyword>
    <dct:issued rdf:datatype="http://www.w3.org/2001/XMLSchema#date">2020-07-07</dct:issued>
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    <dct:description>&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;</dct:description>
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