Two new classes are introduced. One is called "Site" with telescope information and the field rotation angle fra() function. The other is called "EHT" (probably not the best name) which contains an array of sites.
An usage example is given in "examples/eht.ipynb".
Two new classes are introduced. One is called "Site" with telescope information and the field rotation angle fra() function. The other is called "EHT" (probably not the best name) which contains an array of sites.
An usage example is given in "examples/eht.ipynb".
The part I trust the less is how time is handled.