Hello everyone,
I have a few questions regarding flux calibrations performed by LSST, specifically:
- Does the current LSST flux calibration work well for extended sources?
- Is flux calibration already applied to cut-out images?
- Does LSST provide a standard first-level calibration, such as a direct conversion from counts to flux (e.g., x counts = y Jy)?
Any clarification or further details on how flux calibration is handled for these specific use cases would be greatly appreciated!
Thanks in advance for your help!