v1.2.0

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