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

	Commit message (Collapse)	Author	Age	Files	Lines
*	Add bin/update_manifest.py with support of "repro" products	Aaron LI	2017-05-25	1	-0/+68
\| \| \| \|	TODO: support updating other products to manifest.yaml
*	chandra_genspcreg.sh: Give default values for reg_in and reg_out	Aaron LI	2017-03-06	1	-0/+2
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*	make_sbprofile_reg.py: do not set default background file	Aaron LI	2017-03-06	1	-7/+2
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*	manifest: Add logging support; avoid print messages	Aaron LI	2017-03-05	2	-0/+10
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*	Add 'calc_pb_flux.py' to calculate the particle background	Aaron LI	2017-03-04	1	-0/+47
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*	clean_evt2.py: Show a warning with solution for GTI creation in ChIPS	Aaron LI	2017-03-04	1	-0/+3
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*	clean_evt2.py: Add 'reg_sources' and 'gti' to manifest	Aaron LI	2017-03-04	1	-1/+7
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*	Add make_sbprofile.reg.py supporting various arguments	Aaron LI	2017-03-03	1	-0/+282
\| \| \| \|	To replace 'scripts/chandra_gensbpreg.sh'
*	Minor changes	Aaron LI	2017-03-03	2	-3/+4
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*	calc_centroid.py: Do not need to use tempfile	Aaron LI	2017-03-03	1	-9/+6
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*	Add repro_acis.py: reprocess ACIS level=1 data and build manifest.yaml	Aaron LI	2017-03-01	1	-0/+99
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*	make_expmap.py: Add "BUNIT" raw keyword after 'dmimgcalc'	Aaron LI	2017-02-26	1	-1/+6
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*	Add extract_sbprofile.py: Extract SBP from binned image	Aaron LI	2017-02-26	1	-0/+182
\| \| \| \|	To replace 'ciao_sbp.sh' and 'chandra_ccdgap_rect.py'
*	Add correct_exposure.py: Create exposure-corrected image	Aaron LI	2017-02-24	1	-0/+127
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*	make_expmap.py: Threshold-cut the exposure map (cut=1.5%)	Aaron LI	2017-02-24	1	-4/+33
\| \| \| \| \|	* Copy several keywords from instrument map (as 'fluximage' does) * Set the merged expmap has block name "EXPMAP" (as 'fluximage' does)
*	Split 'get_xygrid()' from 'make_expmap.py' to 'acispy/image.py'	Aaron LI	2017-02-24	1	-17/+3
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*	Add make_expmap.py: Make spectral-weighted exposure map	Aaron LI	2017-02-23	1	-0/+247
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*	event2image.py: Use 'logging' instead of 'print'	Aaron LI	2017-02-23	1	-12/+13
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*	Add calc_spectral_weights.py (for spectral-weighted exposure map)	Aaron LI	2017-02-23	1	-0/+118
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*	clean_evt2.py: Update "DETNAM" keyword after filter out chips	Aaron LI	2017-02-23	1	-0/+4
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*	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