Changelog

Todo

  • (!) allow to abort the continuum fitting with CTRL-C

  • run_crude_snr_maps: compute proper S/N for bright stars (not <>/std !)

  • enable minorticks in colorbars (see astropy bug [8126])

  • set the color of NaN pixels in plots … (see astropy bug [8165])

  • when drawing contours in run_skysub(), show the actual pixel edges

  • allow for an automated selection of the sky areas -> requires a better snr estimate ?

  • (?) use config.parser to feed in the parameters, instead of YAML

  • (?) add scalebar to plots … tricky: what if pix scale not uniform, North not up, etc …

v2019.08.3: F.P.A. Vogt - continued with pylint a bit more … re-ouch … - added PyYAML to the list of required packages in setup.py - fixed MANIFEST.in to include the .yaml setup files!

v2019.08.2: F.P.A. Vogt - improved the WCS function, to minimize memory use in crowded fields. - full restructuration of the high-level operation of the code, with proper entry point, via a new run() function - split the WCS correction function, so that it can also be used (potentially) as a stand-alone tool for 2D images. - started using pylint … ouch! - worked on the plotting routines, to make them more robust and uniform.

v2019.08.1: F.P.A Vogt - improved the WCS adjustment step, in case the reference pixel is not in the middle of the image (found by J. Suherli with OCam data). - added automatic inclusion of code version in setup.py - added a proper brutifus entry point from the console.

v2019.07.1: F.P.A. Vogt - added courtesy function to create the execution files, via python -m brutifus –setup. - added a proper entry point, so this can be run as brutifus –setup. - carry over the full original headers when adjusting the WCS values. - fixed a bug in the WCS adjustment function that led to an error of 0.5 pixel for odd array sizes

v2019.02.3: F.P.A. Vogt

  • following the suggestion from Nick Whyborn, use image convolution to find the best spatial shift required to anchor the cube WCS on Gaia.

  • removed all references to aplpy

v2019.02.2: F.P.A. Vogt

  • added photutils to the list of required packages

  • fixed all docstrings

  • cleaned up code of all old brutus bits not (yet) ported to brutifus.

  • started working on documentation

  • first public release!

v2019.02.1: F.P.A. Vogt

  • added run_BWplot step

  • aded WCS correction step

  • worked a bit on refactoring the docstrings

v2019.01.1: F.P.A. Vogt

  • revived the reddening module

v2018.11.1: F.P.A. Vogt

  • added the ‘raw_cube’ name to fn_list for easy access

v2018.11.0: F.P.A. Vogt

  • ported brutus to python 3, renamed it to brutifus (available pip name)

  • removed ppxf from brutifus (focus on SNRs for now)

  • removed pyqz from brutifus (outdated)

  • added sky-subtraction step

  • initial upload to Github, initial upload to pip