New Features:
- Moved old `LsstErrorModel` to `LsstErrorModelV1`
- Created new `LsstErrorModelV2` (which is also aliased as `LsstErrorModel`). This model features the latest throughputs (including all silver mirror coatings), system noise measurements, and more accurate values for quantities like the median seeing and sky brightness. This model assumes a single 38s exposure for the _u_ band and single 30s exposures for the _grizy_ bands. The visit distribution matches the `u 1.2` OpSim run.
- Now requires python >= 3.10
Bug fixes:
- Fixed incorrect calculation of the effect of varying `tvis` by adding a `dCmInf` parameter, and distinguishing `msky` and `mskyDark`
- Fixed bug where FWHM was not being scaled by airmass for extended source error calculations
Relevant issues/pull requests
- PR 13
- PR 14