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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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  <dc:creator>Jane Huang</dc:creator>
  <dc:date>2020-07-07</dc:date>
  <dc:description>Image cubes, self-calibrated visibilities, and self-calibration and imaging scripts for data from Huang et al., 2020, "Large-scale CO spirals and complex kinematics associated with the T Tauri star RU Lup," accepted for publication by The Astrophysical Journal, arXiv:2007.02974 

The raw ALMA data can be found at the ALMA archive under program ID 2018.1.01201.S (PI: Jane Huang).

Scripts:

selfcal_C43-5.py, selfcal_C43-2.py, selfcal_ACA.py: self-calibration scripts for observation of RU Lup in various ALMA configurations

imaging.py: imaging script used for all lines

reductionutils.py can be downloaded from https://zenodo.org/record/3628656

Measurement sets:

RULupcontinuum.ms.tgz: Continuum visibilities for "RULupallcontinuum.image.pbcor.fits" (the high-resolution ALMA continuum data can be found on the DSHARP page)

RULup_12CO.ms.contsub.tgz: Continuum-subtracted visibilities for the 12CO J=2-1 line toward RU Lup

RULup_12CO_nocontsub.ms.tgz: Visibilities for the 12CO J=2-1 line (no continuum subtraction) toward RU Lup, used to make the 'RULup_12COpeakintensity.fits' file.

RULup_13CO.ms.contsub.tgz: Continuum-subtracted visibilities for the 13CO J=2-1 line toward RU Lup

RULup_C18O.ms.contsub.tgz: Continuum-subtracted visibilities for the C18O J=2-1 line toward RU Lup

RULup_DCOp.ms.contsub.tgz: Continuum-subtracted visibilities for the  DCO+ J=3-2 line toward RU Lup

Images: 

RULup12CO.1sigcut.pbcor.mom0.fits: Integrated intensity map of 12CO J=2-1 appearing in Fig. 1

RULup12CO.pbcor.mom1.fits: 12CO J=2-1 intensity-weighted velocity map appearing in Fig. 1

RULup13CO.pbcor.mom0.fits: Integrated intensity map of 13CO J=2-1 appearing in Fig. 1

RULup13CO.pbcor.mom1.fits: 13CO J=2-1 intensity-weighted velocity map appearing in Fig. 1

RULupC18O.pbcor.mom0.fits: Integrated intensity map of C18O J=2-1 appearing in Fig. 1

RULupC18O.pbcor.mom1.fits: C18O J=2-1 intensity-weighted velocity map appearing in Fig. 1

RULup12CO.image.pbcor.fits: 12CO J=2-1 image cube appearing in Fig. 2

RULupC18O.image.pbcor.fits: C18O J=2-1 image cube appearing in Fig. 2

RULup13CO.image.pbcor.fits: 12CO J=2-1 image cube appearing in Fig. 3

RULup_12COpeakintensity.fits: Peak intensity image of 12CO used to make Figure 4

RULupDCOp.pbcor.mom0.fits: Integrated intensity map of DCO+ J=3-2 appearing in Fig. 10

RULupDCOp.image.pbcor.fits: DCO+ J=3-2 image cube appearing in Fig. 11

RULupallcontinuum.image.pbcor.fits: Continuum image appearing in Fig. 12

RULup12COinitial.mask.image.fits: 12CO CLEAN mask shown in Fig. 13

 </dc:description>
  <dc:identifier>https://zenodo.org/record/3928862</dc:identifier>
  <dc:identifier>10.5281/zenodo.3928862</dc:identifier>
  <dc:identifier>oai:zenodo.org:3928862</dc:identifier>
  <dc:language>eng</dc:language>
  <dc:relation>doi:10.5281/zenodo.3928861</dc:relation>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>https://creativecommons.org/licenses/by/4.0/legalcode</dc:rights>
  <dc:subject>ALMA</dc:subject>
  <dc:subject>protoplanetary disks</dc:subject>
  <dc:subject>RU Lup</dc:subject>
  <dc:title>Data from "Large-scale CO spirals and complex kinematics associated with the T Tauri star RU Lup"</dc:title>
  <dc:type>info:eu-repo/semantics/other</dc:type>
  <dc:type>dataset</dc:type>
</oai_dc:dc>
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