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minor typo fixes in changelog
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CHANGELOG.md

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@@ -41,7 +41,7 @@ to describe zenith driftscan data that have no w-projections applied.
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- The `MirParser` class has been significantly overhauled, which significantly reduces
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memory usage and improves processing speed.
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- Updated minimum dependency versions: numpy>=1.19, scipy>=1.3, optional dependencies:
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python-casacore>=3.3, pyyam>=5.1, astropy-healpix>=0.6
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python-casacore>=3.3, pyyaml>=5.1, astropy-healpix>=0.6
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- `UVBase` object now require that individual attribute names match that given in
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`UVParameter._name`.
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- `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
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- Added the `_make_flex_pol` and `remove_flex_pol` methods to `UVData`, which allows for
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one to convert a standard `UVData` object to one with "flexible-polarization".
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- Added a new method to `MirParser` called `_apply_tsys`, which will convert MIR visibility data
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from correlation coefficiencts to pseudo-Jy.
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from correlation coefficients to pseudo-Jy.
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- Added a method to `Mir` called `_init_from_mir_parser`, which allows for one to pass
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a `MirParser` object to be coverted into a UVData object (rather than reading from
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a `MirParser` object to be converted into a UVData object (rather than reading from
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a file on disk).
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- Added the `flex_spw` attribute to the `UVCal` class, which can be set to True by using
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the new `_set_flex_spw` method.

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