CALPRODUCT-VS-014: VIS LED Pixel Response Non-uniformity (PRNU)

Parent requirement

Scheduling

Once, during PV phase, and on a regular basis during the ROS.

Time-critical

No

Objective

For each LED wavelength, obtain the zero-signal PRNU, i.e. corrected for contrast reduction due to CALPRODUCT-VS-004: VIS Brighter-fatter Effect (BFE). This can be achieved by extrapolation to zero signal, and / or BFE correction.

Flag cold/dead pixels, as well as hot pixels.

Fulfilled by

CALBLOCK-PV-022: VIS PRNU and Brighter-fatter Effect

CALBLOCK-PV-029: VIS Photon Transfer Curve and CTI/EPER (also)

CALBLOCK-F-006: Wide Survey

Data volume

Data Volume under study; compression ratio varies by a large factor depending on the fluence.

Processing input

Ground Processing Input Data: BPM, ground-based QE

Data Description: Flat-field and QE cubes

Processing output

Effective flat fields for each LED. Trend analysis

Required accuracy, constraints

Expected flux levels within TBD%, stable within TBD%, spatial irradiance as expected (within requirement, ground-based measurements)

Processing tools

OU-VIS LED PRNU Processing Element

Quality control parameters

DataModel: https://gitlab.euclid-sgs.uk/

Contact person

VIS instrument scientist