- Apr 11, 2025
-
-
Michal Dovčiak authored
* KYNBB was updated to resolve an undefined behaviour when input energy array is changed.
-
- Oct 07, 2024
-
-
Michal Dovčiak authored
-
- Aug 07, 2024
-
-
Michal Dovčiak authored
-
Michal Dovčiak authored
-
Michal Dovčiak authored
* extended corona geometry was also added.
-
- Nov 15, 2023
-
-
Michal Dovčiak authored
- Nov 14, 2023
-
-
Michal Dovčiak authored
-
- May 10, 2021
-
-
Michal Dovčiak authored
-
Michal Dovčiak authored
-
Michal Dovčiak authored
* in the KYNBB model, the colour correction is computed according to Done et al. (2012) MNRAS 420, 1848 for parameter f_col=-1
-
- Apr 03, 2021
-
-
Michal Dovčiak authored
* xside - flat space approximation above 1000rg added * kynbb & kynphebb - radius can be up to 100000 rg or infinite * kynbb - the accretion rate definition in Medd added * Q/I and U/I added as an output for polarization in kynbb, kynphebb and kynlpcr * kynlpcr - the orientation angle added
-
- Oct 13, 2018
-
-
Michal Dovčiak authored
according to the XFLT0001 keyword. * Add definition of the KYNBB and KYNPHEBB model output according to the XFLT0001 keyword of the SPECTRUM extension of the data file. * Speed up KYNBB and KYNPHEBB model when using the same parameters (e.g. when using several data sets of the same source) by remembering the output from the last computation.
-
- Sep 20, 2018
-
-
Michal Dovčiak authored
* Add system orientation angle. * Add negative inclination for opposite system rotation.
-
- Mar 13, 2018
-
- Oct 30, 2017
-
-
Michal Dovčiak authored
-
Michal Dovčiak authored
-
Michal Dovčiak authored
-
Michal Dovčiak authored
* Add obscuration of primary X-ray source * Add q^2 from axis to the observer to lamp tables to compute impact parameter beta of the lamp needed for primary obscuration and change of observed polarisation angle of the primary radiation * Rename lamp tables to 'KBHlamp80.fits' * Add polarisation in KYNlpcr with polarised primary * Add polarisation in KYNbb and KYNphebb * Create 'goosmann.fits' with local polarisation properties of thermal disc radiation for different tau computed with Stokes by Rene Goosmann * In KYNbb and KYNphebb, compute contribution of outer disc only if rout >= 1000 GM/c^2 * Add possibility to use Garcia's xillverD-4.fits tables where density dependence of the reflection spectra is included (for radial power-law profile of the disc density and for constant ionisation of the disc) * Add photon flux as output in XSPEC for parameter Stokes=1 when polarisation computations are switched on * Update documentation
-
- Sep 22, 2017
-
-
Michal Dovčiak authored
-
Michal Dovčiak authored
-
Michal Dovčiak authored
* Change the definition of Np:Nr and luminosity towards the observer or towards the disc in KYNlpcr, KYNrefionx and KYNxillver * Add direct definition of ionisation of the disc in KYNrefionx and KYNxillver, i.e. instead of indirect definition by specifying the density * Update definition of shifted Ecut in KYNrefionx * Add possibility to define cut-off energy in the observer's reference frame in KYNxillver * Update KYNxillver for the newest XILLVER tables (note the definition order of the previous ones has been changed) * Correct error in interpolation of local emission angle in KYNxillver * Correct small error in using local energy in incomplete Gamma function in KYNxillver
- Aug 08, 2016
-
-
Michal Dovčiak authored
-
Michal Dovčiak authored
-
Michal Dovčiak authored
-
- Aug 07, 2016
-
-
Michal Dovčiak authored
-
Michal Dovčiak authored
-
- Aug 05, 2016
-
-
Michal Dovčiak authored
-
- Aug 04, 2016
-
-
Michal Dovčiak authored
-