Sherpa

Latest version: v4.17.0

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4.8.0

This version of Sherpa introduces 'wstat' statistics which is an extension
of 'cstat' with Poisson background data. It also provides the ability to include
background data with the 'user statistics'.

Many changes were aimed at improving the Xspec extension by making it more
robust, intuitive, and by fixing several bugs. Sherpa 4.8.0 supports Xspec 12.9.0d
and was also tested against versions 12.8.2e, 12.8.2l, and 12.8.2q.

Most of the codebase was reviewed and cleaned up, in particular to remove the
use of deprecated functionality and to comply with Python's PEP8 standard.
More tests were added to the test suite, and
a new testing infrastructure was put in place in order to simplify writing and
running tests, and to measure the test suite code coverage.

More details below (infrastructure changes are not shown):

32: Fix segfault from CRATES update in 4.8b1. Since v4.8b1 CRATES returns
variable length arrays by default, rather than the zero-padded fixed length
ones it used to return. Sherpa manipulated the arrays so to remove the
zero-padding and obtaining variable length arrays. The change in the CRATES
API resulted in Sherpa segfaulting when trying to manipulate the data coming
from CRATES. In the patch, we use a new API offered by CRATES to get the
old-style fixed-length arrays instead of the new default ones. In the future,
we may want to update the Sherpa code to deal with the new arrays directly.

44: `save_quality` now correctly outputs 'QUALITY' as the column name,
instead of 'GROUPS'.

48: Fix up several issues seen in plot labels - titles and Y-axis labels -
for commands such as `sherpa.ui.plot_data`, `sherpa.ui.plot_fit_resid`, and
`sherpa.ui.plot_chisqr`.

59: Fix bug 38 (grouping twice gives an IndexError exception). An un-handled
corner case in one of the Sherpa internal methods (`utils.create_expr`) was
triggering an `IndexError` when two `group_counts` operations were performed
back to back. The fix handles the case so that applying `group_counts` twice
does not result in an Exception.

77: Replace `==` and `!=` comparisons to `None` with `is` and `is not`.

78: OutOfBoundErr exceptions in some sherpa.utils
functions are properly caught. There were several places where screen output
used either `print` or `sys.stderr.write`.

81: Ensure that XSPEC models which fail - for instance, because a data file
it needs is missing - return 0's for all bins, rather than random values. This
should make it more obvious that something has gone wrong (for instance if the
XSPEC chatter level is low enough not to show any error messages, as is the
case for the default setting used by Sherpa, namely 0).

82: The XSpec "spectrum number" value is now set to 1 rather than 0, as this
value is 1-based in Xspec.

83: Removed S-Lang scripts, files, and references in the code.

84: Clarified error messages in Xspec extension. Also, changed the class of
the exception from `RuntimeError` to more appropriate exception types, in
particular `LookupError`, `ValueError`, `KeyError`. This is a
backwards-incompatible change, in that code that caught the `RuntimeError`
will not catch the new error.

87: Some methods in `sherpa/fit.py` assigned mutable objects to default
arguments. This has now been fixed. More instances of this issue have been
identified (Bug 95) and will removed in the future.

90: Added background data to the UserStat class.

94: Implement wstat statistic as described at the following url:
https://heasarc.gsfc.nasa.gov/xanadu/xspec/manual/XSappendixStatistics.html

96: Remove the unused myoptfct module.

99: Correct the documentation for the `set_exposure` function.

100 Fix bug 97, whereby the save_all function would not create the necessary
`set_source()` line. This does not fix all cases, but it does the simple PHA
case such as


load_pha('src.pi')
set_source(xsphabs.gal * powlaw1d.pl)
save_all('test.out).


It also ensures that files created by `save_all`
can be run using IPython's %run directive, by explicitly importing the
`sherpa.astro.ui` module.

101: Fix handling of non-contiguous bins in Xspec - i.e. when a model is
called with both xlo and xhi arguments but the bins do not fully cover the
energy, or wavelenth, range. This fixes 62 (for XSPEC 12.8.2; switching to
XSPEC 12.9.0 should also fix it) and 56. It also fixes an (un-reported)
problem with handling of non-contiguous grids when using a table model, where
a crash was likely. When an XSPEC model is called with both low and high
values for the grid - i.e. with two arguments - then the two arrays are
checked to have the same length, and a ValueError is raised if this condition
does not hold. This is a breaking change, but the results are not guaranteed
to be correct if the two arrays are not the same length. The experimental
interface for XSPEC convolution models has changed, so that the function call
takes pars, fluxes, xlo, with optional xhi whereas before it was pars, xlo,
xhi, fluxes. This is a breaking change, but this is in the low-level API that
is not documented to users, and adds useful functionality (the ability to have
xhi be optional). The cpflux convolution model has been added. Note that these
models do not have Python classes associated with them as they are still an
experimental interface. The test suite has been updated to test the new and
changed functionality in this PR. The choice of models is made so as to avoid
known problematic models (with a version check where relevant). It is
believed that the changes in this PR fixes 42, although this is hard to prove
conclusively given the erratic nature of the bug.

110: Update the sherpa.astro.datastack module documentation to include information from the
CIAO ahelp documentation and to match the style used by the sherpa.astro.ui module.

111: Update the documentation to include more information about the pyBLoCXS code.

Caveats

These caveats are being fixed for the 4.8.1 release.

Incompatibility with matplotlib 1.5: Sherpa 4.8.0 is not compatible with matplotlib 1.5. Unfortunately, this version is currently the default package installed by conda. Users should install sherpa with matplotlib=1.4 numpy=1.9.

Test requirements are not installed automatically: sherpa_test does not work out of the box. Users should issue "pip install pytest-cov" in order for sherpa_test to run.

SAO DS9 issue on Ubuntu 14.04: the ds9 binaries shipped with Ubuntu and installed through apt-get install do not seem to work as expected. Binaries downloaded directly from the SAO ds9 page seem to work instead.

4.7

Release Notes

This standalone release is based on CIAO Sherpa v4.7.

Release notes for this baseline version can be found at the following link:
http://cxc.harvard.edu/ciao/releasenotes/ciao_4.7_release.html#Sherpa

Additionally, the present release includes some changes listed below:
- Standalone Sherpa and CIAO sherpa now look for different configuration files in the $HOME directory. For standalone this is `$HOME/.sherpa-standalone.rc`. If this file is not present, Sherpa falls back to the internal configuration file. This file has defaults better suited for the standalone mode: `pyfits` and `pylab` are set as backends, and the stack trace is not silenced. Users can still override the configuration file location by exporting the `SHERPARC` environment variable, as supported by previous versions of Sherpa and CIAO.
- All source files now have copyright and licensing information. A summary is included upfront in the repository main directory.
- Orphan code that was not actually used has been removed.
- Fixed code triggering deprecation warnings from Numpy 1.9.
- Fixed code triggering compiler warnings.
- Added documentation (README, ipython notebook).
- The version string (`sherpa.__version__`) depends on the git commit/tag, unlike in CIAO where it is fixed to 40701.
- Some classes from the template module were not exposed by `__all__`, and template models were not imported in the sherpa session. Now they are.

Known issues
- the datastack module is not imported if no plotting packages are available. Installing `matplotlib` in the same environment as Sherpa fixes the issue.

3.10

One of the tests fails in Python 3.10 because the error message has been changed.

1493 - Remove deprecated distutils.version.LooseVersion
The distutils.version.LooseVersion class is now marked as deprecated so remove its
use when building Sherpa and when importing the Sherpa XSPEC module.

1494 - Update AX_PYTHON_DEVEL.m4 from serial 17 to 25
This update covers the cleanup of distutils in the configure files for grplib (and
stklib in the case of standalone sherpa).

1495 - Note that we support Python 3.10
Note that Sherpa can be built using Python 3.10 and add two Python 3.10 CI test runs.

1496 - DS9 update from 8.2.1 to 8.3
Update to use ds9 v8.3 since v8.2.1 is no longer available

1497 - Tests: ensure matplotlib windows are closed after all tests are run
Ensure that our tests can run on CI cleanly.

3.4

Matplotlib 3.4 changes how the drawstyle argument is handled in some functions.
This change removes the use of this argument for those functions.

1126 - Tweak plot docs
Adds a new notebook that shows off a number of plots created with matplotlib and
exports the ScatterPlot, TracePlot, CDFPlot, PDFPlot, and LRHistogram classes from
sherpa.plot.

1130: Fix save_data when the output file exists
Fix problems when save_data is used with clobber=False but the output file already
exists. Fixes 1071

1132 - Update XQuartz for GH Actions workflow
Updates the xQuartz download location and version for the GitHub Actions Conda tests

1139 - Fix typo in Zenodo test that made it fail
Fixed a typo in the zenodo test which gets only run via the --runzenodo flag

1142 - Add instruction for source build on Mac
Add instruction for source building on Mac that were previously only part of the
internal release notes.

2.0

Internal code changes to improve support for NumPy 2.0.

1874 - save_all improvements for set_psf and load_xstable_model
Ensure that save_all includes set_psf calls, supports XSPEC table models,
and improve the support for data sets created with load_arrays or
dataspace1d/dataspace2d. Fixes 1873.

1877 - un-whitelist deprecation warnings
Cleaned up deprecation warning exceptions from test white list

1878 - Tests: better handle case where both astropy and crates are available
Fix up tests that would fail when both astropy and crates packages were
installed and the pyfits backend was chosen (the tested functionality was
not wrong, just they were testing the wrong things).

1.19

Compatibility updates for numpy v1.19 with regards to numpy.distutils and tostring deprecation

781 - Docs: fix typo in docstring for calc_kcorr
Fixed a typo in docstring for calc_kcorrFix a typo in the documentation
for calc_kcorr: change "0." to "0.5" in one of the examples.

759 - revert PR 444 (caching)
Revert the ARF cache added in 444, as well as some of the related code
changes, as they caused problems with Analysis in wavelength space
(e.g. 746)

756 - calculate_photon_flux/calculate_energy_flux fix and improvement
Bug fixes and improvements for calculate_photon_flux and calculate_energy_flux:
- address flux and flux-density calculation issues discussed (fix 619)
- fix documentation of the lo and hi arguments (fix 308)
- add model parameter to calc_photon/energy_flux which allows users to
easily calculate "unabsorbed" fluxes

747 - reworked regrid to eval usr grid, but 0 every where else
Modifies the 1D grid implementation to evaluate over the user-supplied
range, anything outside that is set to 0

745 - ensure that min/max limits are applied to linked parameters before use
Enforce parameter restrictions (they must lie within their min/max range)
even when the parameter is linked to another (which has a different range).

739 - Post 4.12.0 Updates
Update readme to include DOI for 4.12.0

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