You signed in with another tab or window. Reload to refresh your session.You signed out in another tab or window. Reload to refresh your session.You switched accounts on another tab or window. Reload to refresh your session.Dismiss alert
This issue is to implement an optional model of vignetting as a function of position in the focal plane.
Can vignetting be modeled as an achromatic multiplicative throughput factor that depends only on r? Should the model be specified via a tabulated data file or is there a standard parameterization that is flexible enough?
What is the definitive reference for the expected vignetting in DESI? Has the vignetting in eBOSS been measured?
The text was updated successfully, but these errors were encountered:
DESI-2632 is the most detailed look at telescope vignetting. The chromatic effects will be quite small. A larger effect would be the vignetting as a function of the ADC position. This study uses a single ADC position.
This issue is to implement an optional model of vignetting as a function of position in the focal plane.
Can vignetting be modeled as an achromatic multiplicative throughput factor that depends only on r? Should the model be specified via a tabulated data file or is there a standard parameterization that is flexible enough?
What is the definitive reference for the expected vignetting in DESI? Has the vignetting in eBOSS been measured?
The text was updated successfully, but these errors were encountered: