Published February 4, 2025
| Version v1
Data paper
Open
Results from the KOREL code used in the Disentangling Method for Cygnus X-1
Authors/Creators
-
1.
Czech Academy of Sciences, Astronomical Institute
- 2. Faculty of mathematics and physics, Charles University
- 3. Astronomical Institute of the Czech Academy of Sciences
Description
The .zip file contains the output of the KOREL code from the Disentangling Method, in the hard and soft X-ray spectral states of the high-mass X-ray binary Cygnus X-1, for the hydrogen and helium lines. The .dat files contain the input parameters for the Disentangling. The .par files control the calculation in KOREL using the initial parameters from the .dat file. The .res files contain the output values after calculation. See "Disentangling of spectra - theory and practice" from P. Hadrava for a more detailed description.
Files
aa509100-24_paper_dataset.zip
Files
(770.0 kB)
| Name | Size | Download all |
|---|---|---|
|
md5:a7eaf92867616bc75456077a139f9329
|
770.0 kB | Preview Download |
Additional details
Funding
- Charles University
- Charles Univeersity Grant Agency 102323
References
- Disentangling of spectra - theory and practice, Hadrava, 2009, https://doi.org/10.48550/arXiv.0909.0172
- Disentangling of the Spectra of Binary Stars – Principles, Results and Future Development, Hadrava, 2005, https://doi.org/10.1007/s10509-006-9153-5
- KOREL – User's guide, Hadrava, 2004, https://ui.adsabs.harvard.edu/abs/2004PAICz..92...15H
- Relative line photometry of eclipsing binaries., Hadrava, 1997, https://ui.adsabs.harvard.edu/link_gateway/1997A&AS..122..581H/doi:10.1051/aas:1997102