chandra-acis-analysis.git - Chandra ACIS analysis tools and documents

	Commit message (Collapse)	Author	Age	Files	Lines
*	Print more information	Aaron LI	2017-02-23	2	-4/+11
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*	event2image.py: Update keyword "DETNAM" of the created image	Aaron LI	2017-02-23	1	-0/+4
\| \| \| \| \| \| \| \|	The "DETNAM" keyword of the created image is updated to show the actually available chips. Therefore, there won't be issues when this image is corrected for exposure by dividing the exposure map. And the exposure-corrected image will have correct "DETNAM" value instead of "Merged".
*	Update to use 'cosmo_calc.py'	Aaron LI	2017-02-22	3	-3/+3
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*	Remove calc_coolfunc.sh (replaced by calc_coolfunc_{table,profile}.py)	Aaron LI	2017-02-21	1	-113/+0
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*	fit_{mass,sbp}.sh: Update to use 'calc_coolfunc_{table,profile}.py'	Aaron LI	2017-02-21	2	-6/+17
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*	Update to use 'cosmo_calc.py' instead of 'cosmo_calc'	Aaron LI	2017-02-21	2	-2/+2
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*	Add calc_coolfunc_profile.py: calculate cooling function proifle	Aaron LI	2017-02-21	1	-0/+67
\| \| \| \| \| \| \|	Calculate cooling function profile w.r.t. temperature profile by interpolating previously calculated cooling function table. This tool replaces the 'calc_coolfunc.sh' and 'calc_coolfunc_bands.sh'
*	Add calc_coolfunc_table.py: to speed up the repeated CF calculations	Aaron LI	2017-02-21	1	-0/+177
\| \| \| \| \| \| \| \| \|	Calculate the cooling function table with respect to the specified temperature range, using the XSPEC model 'wabs*apec' with the provided arguments. Later, the cooling function profile w.r.t. a temperature profile can be quickly derived by interpolating this cooling function table.
*	Move various Python tools from 'scripts/' to 'bin/'	Aaron LI	2017-02-21	11	-0/+1118
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*	Move shell/python scripts from 'mass_profile/' to 'bin/'	Aaron LI	2017-02-20	12	-0/+1406