AMI Full Frame Fractional Throughput
Abstract
Observations will be made of a standard star in regular full frame imaging and then with the NRM in the beam to calibrate the fractional throughput of the mask for photometric calibration purposes. A similar program is planned for the SUB80 sub-array, but that uses brighter targets than can be observed in full frame imaging.
This calibration program is provisional and may change in response to system developments and the final science program.- Publication:
-
JWST Proposal. Cycle 1
- Pub Date:
- October 2019
- Bibcode:
- 2019jwst.prop.1506V