Releases: RadioAstronomySoftwareGroup/pyuvdata
Version 2.2.3
This version fixes a few minor bugs that were breaking Conda builds and adds OVRO-LWA to our known telescopes.
Automatically generated details below:
What's Changed
- Fixing automatically generated catalog IDs by @kartographer in #1067
- Add OVRO-LWA to known telescopes by @rlbyrne in #1060
- Increase the tolerance on uvbeam real_if_close call by @bhazelton in #1066
- Putting in a workaround for astroquery/JPL-Horizons related error by @kartographer in #1069
Full Changelog: v2.2.2...v2.2.3
Version 2.2.2
This version add a Measurement Set write method to UVData objects (UVData.write_ms) and methods to easily set data, nsamples and flags for baselines (set_data, set_flags, and set_nsamples) paralleling the popular get methods for these arrays. It also adds a new from_file class method for UVData and UVBeam objects to support one-line file reading into these objects.
Other improvements and bug fixes are detailed in the changelog.
Version 2.2.1
This version has an updated __eq__ method on the UVBase object which includes an allowed_failures keyword to specify parameters which are allowed to be unequal without causing the overall equality check to fail. For UVData, this keyword defaults to include the filename attribute.
Version 2.2.0
This release dramatically improves how phasing is done on UVData objects and adds support for multiple phase centers and non-sidereal phase centers. Reading and writing out data with multiple phase centers is supported for UVH5, UVFITS, MIR, and MIRIAD files. It also adds support for a filename attribute on UVData objects and support for getting and selecting data on UVData objects using LSTs.
Other improvements and bug fixes are detailed in the changelog.
Version 2.1.5
This release adds optional Van Vleck correction for MWA correlator files, a method for reordering frequencies on UVData objects and support for converting UVData objects to use the future array shapes to allow users to upgrade their code before the shapes change.
Other additions and bug fixes are detailed in the changelog.
Version 2.1.4
This release includes a major improvement in memory usage for reading MWA correlator FITS files and speed and memory improvements for finding and handling redundant baseline groups. See the changelog for full details of other bug fixes and improvements.
Version 2.1.3
This release includes significant upgrades to the UVCal object, including metadata-only reading and a copy method. Other changes are detailed in the changelog.
Version 2.1.2
This version adds support for "flexible spectral windows" for UVData objects, which allows for storing multiple spectral windows into a single UVData object, and improves support for MWA correlator files. Writing multiple spectral windows is supported in UVH5, UVFITS, MIR, and MIRIAD files. All changes are detailed in the changelog.
Version 2.1.1
This version adds support for the Submillimeter Array's MIR file format. See the changelog for other changes.
Version 2.1
v2.1.0 Update the changelog for the new version