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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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    "description": "<p>Image cubes, self-calibrated visibilities, and self-calibration and imaging scripts for data from Huang et al., 2020, &quot;Large-scale CO spirals and complex kinematics associated with the T Tauri star RU Lup,&quot; accepted for publication by The Astrophysical Journal, arXiv:2007.02974&nbsp;</p>\n\n<p>The raw ALMA data can be found at the ALMA archive under program ID 2018.1.01201.S (PI: Jane Huang).</p>\n\n<p><strong>Scripts:</strong></p>\n\n<p>selfcal_C43-5.py, selfcal_C43-2.py, selfcal_ACA.py: self-calibration scripts for observation of RU Lup in various ALMA configurations</p>\n\n<p>imaging.py: imaging script used for all lines</p>\n\n<p>reductionutils.py can be downloaded from&nbsp;<a href=\"https://zenodo.org/record/3628656\">https://zenodo.org/record/3628656</a></p>\n\n<p><strong>Measurement sets:</strong></p>\n\n<p>RULupcontinuum.ms.tgz: Continuum visibilities for &quot;RULupallcontinuum.image.pbcor.fits&quot; (the high-resolution ALMA continuum data can be found on the <a href=\"https://bulk.cv.nrao.edu/almadata/lp/DSHARP/\">DSHARP</a> page)</p>\n\n<p>RULup_12CO.ms.contsub.tgz: Continuum-subtracted visibilities for the <sup>12</sup>CO J=2-1 line toward RU Lup</p>\n\n<p>RULup_12CO_nocontsub.ms.tgz: Visibilities for the <sup>12</sup>CO J=2-1 line (no continuum subtraction) toward RU Lup, used to make the &#39;RULup_12COpeakintensity.fits&#39; file.</p>\n\n<p>RULup_13CO.ms.contsub.tgz: Continuum-subtracted visibilities for the <sup>13</sup>CO J=2-1 line toward RU Lup</p>\n\n<p>RULup_C18O.ms.contsub.tgz: Continuum-subtracted visibilities for the C<sup>18</sup>O J=2-1 line toward RU Lup</p>\n\n<p>RULup_DCOp.ms.contsub.tgz: Continuum-subtracted visibilities for the&nbsp; DCO<sup>+</sup> J=3-2 line toward RU Lup</p>\n\n<p><strong>Images: </strong></p>\n\n<p>RULup12CO.1sigcut.pbcor.mom0.fits: Integrated intensity map of <sup>12</sup>CO J=2-1 appearing in Fig. 1</p>\n\n<p>RULup12CO.pbcor.mom1.fits: <sup>12</sup>CO J=2-1 intensity-weighted velocity map appearing in Fig. 1</p>\n\n<p>RULup13CO.pbcor.mom0.fits: Integrated intensity map of <sup>13</sup>CO J=2-1 appearing in Fig. 1</p>\n\n<p>RULup13CO.pbcor.mom1.fits: <sup>13</sup>CO J=2-1 intensity-weighted velocity map appearing in Fig. 1</p>\n\n<p>RULupC18O.pbcor.mom0.fits: Integrated intensity map of C<sup>18</sup>O J=2-1 appearing in Fig. 1</p>\n\n<p>RULupC18O.pbcor.mom1.fits: C<sup>18</sup>O J=2-1 intensity-weighted velocity map appearing in Fig. 1</p>\n\n<p>RULup12CO.image.pbcor.fits: <sup>12</sup>CO J=2-1 image cube appearing in Fig. 2</p>\n\n<p>RULupC18O.image.pbcor.fits: C<sup>18</sup>O J=2-1 image cube appearing in Fig. 2</p>\n\n<p>RULup13CO.image.pbcor.fits: <sup>12</sup>CO J=2-1 image cube appearing in Fig. 3</p>\n\n<p>RULup_12COpeakintensity.fits: Peak intensity image of <sup>12</sup>CO used to make Figure 4</p>\n\n<p>RULupDCOp.pbcor.mom0.fits: Integrated intensity map of DCO<sup>+</sup> J=3-2 appearing in Fig. 10</p>\n\n<p>RULupDCOp.image.pbcor.fits: DCO<sup>+</sup> J=3-2 image cube appearing in Fig. 11</p>\n\n<p>RULupallcontinuum.image.pbcor.fits: Continuum image appearing in Fig. 12</p>\n\n<p>RULup12COinitial.mask.image.fits: <sup>12</sup>CO CLEAN mask shown in Fig. 13</p>\n\n<p>&nbsp;</p>", 
    "language": "eng", 
    "title": "Data from \"Large-scale CO spirals and complex kinematics associated with the T Tauri star RU Lup\"", 
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    "publication_date": "2020-07-07", 
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