This repository is meant to accompany the publication "Detection of a Disk Surrounding the Variably Accreting Young Star HBC722" in the Research Notes of the AAS (Volume 4, Number 9).
- The
data
directory contains a.csv
file with the key results from applying 3 rounds of self-calibration (more specifically, 2 rounds of phase self-calibration, followed by 1 round of amplitude self-calibration) to the ALMA 233 GHz continuum observations of the FU Orionis object HBC722. Note that the values are rounded up to 3 decimal places solely for vanity. The raw data is available upon request. disk_mass.ipynb
contains the Jupyter Notebook used to calculate the object's total circumstellar disk mass.Yek_2020.pdf
is a PDF of the final publication, downloaded from the arXiv: https://arxiv.org/abs/2009.08019.- The
src
directory houses the LaTeX source code used to typesetYek_2020.pdf
. utils/continuum_detection_image.pro
is the IDL source code used to create Figure 1 ofYek_2020.pdf
.