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WSClean version 2.4
===================
Released 2017-05-28
Summary: Version 2.4 mostly contains small improvements on various points. Improved source component output allows better integration with (DD and DI) self-calibration pipelines, and continued work on the integration with IDG is aiming towards a fast, full A-correction imager.
New features:
* Option ``-save-source-list`` to save a component list including Gaussians for multi-scale components. The output format is supported by DPPP. Old option ``-save-component-list`` has been removed.
* Source lists can be primary-beam corrected by combining ``-save-source-list`` with ``-apply-primary-beam`` (SF #111).
* Added keywords ``TELESCOP``, ``OBSERVER`` and ``OBJECT`` to fits output (SF #112).
* Fitting a Gaussian to the PSF is now more stable, and deals better with border cases (reported by G . Heald).
* Multi-frequency cleaning will now properly take channel weights into account during spectral fitting and peak finding (SF #109)
* Flux density values are now reported with sensible units, and units can be given on the cmdline (SF #104).
* WSClean will by default now stop deconvolution after 20 major iterations, which can be changed with the new option ``-nmiter`` (SF #117, requested by N. Hurley Walker).
* Option ``-save-psf-pb`` to be able to get a corrected PSF.
* Option ``-circularbeam`` now properly performs a constrained fit (SF #55).
* Option ``-multiscale-convolution-padding`` to change the default padding.
* WSClean now reports the reason for stopping cleaning.
* Slight increase of gridding speed, because X and Y dimensions of gridding kernel are now stored separately. Larger oversampling rates are now also supported.
Bugfixes:
* Parameter ``-stopnegative`` was ignored since the new generalized cleaning algorithm was implemented (reported by N. Hurley-Walker and C. Tremblay).
* In multi-scale, joined polarizations mode, WSClean could not determine scale sizes when last channel has no unflagged visibilities (Reported by R. van Weeren).
* In joined polarization mode, WSClean could continuously perform further major iterations without improving the residuals any further (reported by N. Hurley-Walker).
* Deprecated parameter name ``-rms-background``, which was renamed to ``-local-rms``.
* Fixes for IDG gridding; CPU and GPU gridding & cleaning with IDG works.
* Version information now includes availability of IDG.
* More unit tests.
* Support proper displaying of negative angles.
* Refactoring of primary beam correction code.
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