Release Notes¶
5.0.0 (2024-07-03)¶
potentially breaking change: xspec: in BXA v5, priors now use min/max soft parameter limits instead of hard parameter limits. That is, among “min, bottom, top, and max”, BXA<5 used min and max, while BXA>=5 uses bottom and top.
xspec: compute fluxes for multi-source and multi-spectrum cases (thanks @DaKalt)
sherpa: smooth interpolation in CDF prior file interpolation
add eROSITA background file
4.1.4 (2024-05-26)¶
fix in BXA/sherpa PCA background fitting. Previously, emission lines were never added.
This means that versions before 4.1.3 and after will give different background fits
The old behaviour can be recovered with auto_background(max_lines=0).
add Bayesian workflow tutorial
4.0.0 (2021-01-06)¶
Make ultranest default, remove multinest.
3.4 (2019-05-26)¶
3.3 (2020-01-28)¶
3.2 (2020-01-12)¶
circumvent xspec numerical interpolation issues (Lepsilon parameter)
3.1 (2019-10-21)¶
Make multinest optional, allow ultranest
3.0 (2019-10-15)¶
2.10 (2019-06-12)¶
Added PCA background models
2.9 (2019-06-11)¶
2.8 (2019-05-31)¶
2.7 (2019-05-31)¶
2.6 (2019-05-21)¶
replace outdated progressbar with tqdm
2.5 (2019-04-08)¶
added PCA background model
added galactic absorption fetcher
added generic AGN fitting script
2.4 (2015-06-17)¶
2.3 (2015-06-09)¶
added Chandra background model
added Swift background model
2.0.0 (2015-06-05)¶
Python 3 support
added corner plots
added more convenience functions for plotting
added Chandra background model
added acceleration of models
1.0.0 (2013-12-01)¶
simple multinest interfaces for xspec and sherpa based on pyblocxs code