CALPRODUCT-VS-015: VIS Noise Bias Calibration Fields (REPLACED)

Replaced by CHAR-TARGET-003: Noise Bias Calibration Fields.

Parent requirement

Scheduling

Repeatedly throughout the mission duration, until area is covered to the desired depth.

Time-critical

No.

Objective

A sample of about 200000 galaxies shall be obtained with a S/N 6 times that of the wide survey area, obtained from a 40 square degree area constituted by the Euclid Deep Fields (EDF-North, EDF-South, and EDF-Fornax).

Fulfilled by

CALBLOCK-F-002: Noise Bias Fields (Euclid deep fields)

Targets and pointing constraints

Table 13: Noise bias fields. CSV file

# ID

R.A.

Dec

EDF-N

269.733

+66.018

EDF-S

61.241

-48.423

Fornax

52.932

-28.089

In-orbit duration

Processing input

Ground Processing Input Data:

Data Description:

Quality control parameters

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

Contact person

Calibration Lead