Multiwavelength observations reveal a faint candidate black hole X-ray binary in IGR J17285-2922

<h2>Reproduction package for the paper "Multiwavelength observations reveal a faint candidate black hole X-ray binary in IGR J17285-2922"</h2><h4>This is a reproduction package with the internal API designation of 'silver'</h4><h4>Monthly Notices of the Royal Astronomical Society, Volume 507, Issue 1, October 2021, Pages 330–349</h4><h4>Authors: <strong>M. Stoop</strong>, J. van den Eijnden, N. Degenaar, A. Bahramian, S. J. Swihart, J. Strader, F. Jiménez-Ibarra, T. Muñoz-Darias, M. Armas Padilla, A. W. Shaw, T. J. Maccarone, R. Wijnands, T. D. Russell, J. V. Hernández Santisteban, J. C. A. Miller-Jones, D. M. Russell, D. Maitra, C. O. Heinke, G. R. Sivakoff, F. Lewis D. M. Bramich</h4><h4>Paper DOI: https://doi.org/10.1093/mnras/stab2127</h4><h4>Zenodo DOI: https://doi.org/10.5281/zenodo.4664505</h4><p>&nbsp;</p><h2>Raw Data</h2><p>&nbsp;</p><p>- Uncalibrated X-ray data is given in ./raw_data</p><p>&nbsp;</p><p>- Radio data is too large in size to be stored on Zenodo. If you want to acquire these images, but can be found under https://data.nrao.edu searching for project code SF8027</p><p>&nbsp;</p><p>- Raw data for the optical spectra can be acquired by contacting J. van den Eijnden</p><p>&nbsp;</p><h2>Software</h2><p>&nbsp;</p><p>- OS: MacOS Big Sur 11.6</p><p>&nbsp;</p><p>Programming languages:</p><p>&nbsp;</p><p>- Python (3.9.7), matplotlib, numpy, pandas, scipy, linmix</p><p>&nbsp;</p><p>- Jupyter Notebook (6.3.0)</p><p>&nbsp;</p><p>NASA HEASARC's Software:</p><p>&nbsp;</p><p>- xrtpipeline (version 0.13.5)</p><p>&nbsp;</p><p>- caldb in the heasoft package (version 6.26.1)</p><p>&nbsp;</p><p>- xselect (version v2.4g)</p><p>&nbsp;</p><p>- xrtmkarf (version 0.6.3)</p><p>&nbsp;</p><p>- xspec (v. 12.10.1f)</p><p>&nbsp;</p><p>- casa pipeline (5.6.2)</p><p>&nbsp;</p><h2>Figures and Tables</h2><p>&nbsp;</p><p>- scripts and data to make the figures and tables can be found in ./figures_tables</p><p>&nbsp;</p><p>- figure 4, 5, 6, and 7 are made by collaborators. Please contact J. van den Eijnden if you would like access to data files or scripts for these figures.</p><p>&nbsp;</p><p>- X-ray lightcurve fit results in Table 3 is done by collaborators. Please contact J. van den Eijnden if you would like access to data files or scripts for this table.</p><p>&nbsp;</p><h2>Intermediate data products &nbsp;</h2><p>&nbsp;</p><p>- Intermediate data products can be found in the directory ./intermediate_data</p><p>&nbsp;</p><p>- This includes the calibrated X-ray data, VLA imaging scripts to determine the flux density and spectral index.</p><p>&nbsp;</p><p>- Scripts can also be found here for intermediate data products for several figures (1, 2, 3, 8)</p><p>&nbsp;</p><h2>Scientific-analysis</h2><p>&nbsp;</p><p>- The directory ./scientific_analysis contains scripts and data to reduce the raw data to the intermediate data products.</p><p>&nbsp;</p><p>- ./Xray_files how to calibrate the Swift X-ray spectra</p><p>&nbsp;</p><p>- ./Xray_spectral_evolution contains how the intermediate data products for figure 3</p><p>&nbsp;</p><p>- ./VLA_data_reduction how to reduce the VLA data and determine flux densities and spectral indices</p><p>&nbsp;</p><p>- ./Radio_Xray_Coupling contains the intermediate data products for figure 2</p><p>&nbsp;</p><p>- ./Xray_lightcurve_fitting contains intermediate data products for Table 3 and fitting performed in section 3.4</p><p>&nbsp;</p><p>- ./Orbital_Period contains intermediate data products for Table 4 and Figure 8</p><p>&nbsp;</p><p>- ./xray contains backup files related to the x-ray spectra</p><p>&nbsp;</p><p>- ./radio contains backup files related to the radio data</p><p>&nbsp;</p><p>- the main results (intermediate data products) are the .txt files in this directory</p>