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author | Aaron LI <aaronly.me@outlook.com> | 2015-06-16 16:46:23 +0800 |
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committer | Aaron LI <aaronly.me@outlook.com> | 2015-06-16 16:46:23 +0800 |
commit | 9c7782686fd607fd4e38038ed44f0307da0cd8c7 (patch) | |
tree | f4c3d7167f9f86974f0b3ff19ce910a4feb88cbb /astro/fits | |
parent | 4b96527999e0b63917efa68ddfdffa57122c22cf (diff) | |
download | atoolbox-9c7782686fd607fd4e38038ed44f0307da0cd8c7.tar.bz2 |
Updated astro tools.
* fit_betasbp_cut.py
- fixed 'dof' calculation with 'n-p-1'
- fixed 'par_eps' calculation/configuration
- added 'fit_model_bounds' using 'scipy.optimize.minimize' to
perform function minimization with bounds
- split the data cut section to function 'cut_data'
- added argument 'options' to 'fit_model_bounds'
* marx_pntsrc.py
Run MARX simulation on a given list of point sources, merge the
output simulation results, and finally convert into FITS image.
* blanksky_add_time.py
Add a time column for the chandra blanksky event file.
The time data are generated with a uniform distribution
between TSTART and TSTOP.
Diffstat (limited to 'astro/fits')
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