| Commit message (Collapse) | Author | Age | Files | Lines |
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Handy liner to help debugging Makefile.
Credit: http://blog.jgc.org/2015/04/the-one-line-you-should-add-to-every.html
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* Mask the regions where the dust absorption is too high to well
determine the true Halpha absorption.
There are regions (e.g., Galactic plane) have too large dust
absorption which cause float overflow when applying absorption
correction to the Halpha map.
* Fix a bug on the wrong parameter passed to "_calc_ratio_a()" method
in "_simulate_frequency()"
* Move "_correct_dust_absorption()" invokation from "simulate()"
to "_simulate_frequency()"
Already tested and OK!
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* healpix2hpx(), hpx2healpix(): Remove the "header" parameter, thus the
"data" parameter can only be either the filename or a HDU;
* healpix2hpx(): Remove the check on "ORDERING", since
"read_fits_healpix()" always return the HEALPix data in RING ordering;
* Small updates to the log messages and comments.
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* bin/fg21sim: check the "common/components" config to simulate the
enabled components;
* bin/fg21sim: add Galactic free-free component support;
* galactic/freefree.py: fix missing attributes.
NOTE: simulated free-free maps are WRONG!! Need check/debug!
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* New class "galactic.FreeFree" to simulate free-free emission
* Add new config section "galactic/freefree"
NOTE: current untested
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* Merge the upgrade/downgrade resolution w.r.t Nside to the map loading
methods;
* Update the variable names;
* Check the status of smallscales addition.
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The missing pixels in the reprojected HEALPix map are filled with the
averages of their 8 neighboring pixels (excluding the NaN's if any).
Also add the "--inpaint" argument to the executable script.
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Also fix typos
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The mask array has values 0, 1, and 2, which indicate the different
statuses of the reprojected HEALPix pixels.
Also update the executable script to use the new return results.
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The script takes the two ZEA-projected FITS images, reproject them to
the full-sky HEALPix map in Galactic frame with RING ordering.
TODO:
* Add argument "--inpaint" after implement the inpainting function.
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The "zea2healpix()" function reprojects the maps in ZEA
(zenithal/azithumal equal area) projection to HEALPix data in Galactic
frame with RING ordering.
The other two helper functions "_image_to_healpix()" and "_convert_wcs()"
are almost copied from the "reproject" project [1]. Thanks!
TODO:
* Add some more logging
* Implement the "inpaint" argument to inpaint the HEALPix map if exists
missing pixels
[1] reproject: https://github.com/astrofrog/reproject
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* utils/fits.py: hack the dtype to ignore the byteorder (FITS data use
big endianness, e.g., dtype(">f4"))
* utils/healpix.py: explicit convert the dtype and log the dtype
* bin/healpix2hpx, bin/hpx2healpix: remove the --float argument
* other minor fixes/updates
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Also remove a unused variable in "galactic/synchrotron.py"
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This function wraps on the `healpy.read_map()`, but reset the data array
to its original dtype in FITS file, as well as return the FITS header in
`astropy.io.fits.Header` object.
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NOTE:
This "write_fits_healpix()" function only implements the most common
case of the HEALPix FITS style.
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Credits:
* http://doc.pytest.org/en/latest/goodpractices.html
* https://github.com/kennethreitz/requests/blob/master/setup.py
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* Add new executable "bin/fg21sim"
* galactic/synchrotron: update to use "configs.get_path()"
* galactic/synchrotron: create output dir if not exists
* galactic/synchrotron: add logging support
* galactic/synchrotron: append FITS extension to filename
* galactic/synchrotron: pass the basic test
TODO:
* "output()" needs fixes with the FITS header
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This "read_userconfig()" method is specifically used to load the user
configuration file, and record the absolute path of the configuration
file, which allows the use of relative path to specify the input files
(e.g., galactic/synchrotron/template) for simulation within the
configurations.
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NOTE:
these checker functions check on the whole configuration, and have no
relation to the checker functions of the `Validator` class.
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The "frequencies" property will return or calculate the frequency
values of the simulation.
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* The variable "VENV" (default: "venv") defines the virtualenv name and
can be override by the environment.
* Add "devbuild" target to menu.
* Remove the "--user" argument to fix the pip install problem.
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* Add new configs for the [frequency] section
* Use "None" as the default value for some configs
* Fix the syntax of "cosmology/OmegaM0"
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These additional checker functions validate the required configs whether
provided by the user config file, as well as against necessary contexts.
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NOTE: untested
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