@@ -41,7 +41,7 @@ to describe zenith driftscan data that have no w-projections applied.
4141- The ` MirParser ` class has been significantly overhauled, which significantly reduces
4242memory usage and improves processing speed.
4343- Updated minimum dependency versions: numpy>=1.19, scipy>=1.3, optional dependencies:
44- python-casacore>=3.3, pyyam >=5.1, astropy-healpix>=0.6
44+ python-casacore>=3.3, pyyaml >=5.1, astropy-healpix>=0.6
4545- ` UVBase ` object now require that individual attribute names match that given in
4646` UVParameter._name ` .
4747- ` UVData.fix_phase ` now raises a warning when called.
@@ -106,9 +106,9 @@ along with an option to force them to be real-only if non-zero imaginary compone
106106- Added the ` _make_flex_pol ` and ` remove_flex_pol ` methods to ` UVData ` , which allows for
107107 one to convert a standard ` UVData ` object to one with "flexible-polarization".
108108- Added a new method to ` MirParser ` called ` _apply_tsys ` , which will convert MIR visibility data
109- from correlation coefficiencts to pseudo-Jy.
109+ from correlation coefficients to pseudo-Jy.
110110- Added a method to ` Mir ` called ` _init_from_mir_parser ` , which allows for one to pass
111- a ` MirParser ` object to be coverted into a UVData object (rather than reading from
111+ a ` MirParser ` object to be converted into a UVData object (rather than reading from
112112 a file on disk).
113113- Added the ` flex_spw ` attribute to the ` UVCal ` class, which can be set to True by using
114114the new ` _set_flex_spw ` method.
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