CHAR-TARGET-004: Completeness and Purity Calibration (CPC)

Parent requirement

Objective

Generate a spectroscopic sub-sample of at least 120,000 galaxies with 99% purity. The galaxies must be selected with the same selection criteria as in the wide survey. Estimates of the number density of galaxies imply a survey area of at least 40 square degrees.

Observations

The completeness and purity calibration (CPC) is obtained from the EDF-N and the EDF-S, together totaling 43 square deg. The main objective is to observe these field with sufficiently many orientations such that the slitless spectra can be optimally decontaminated.

Each field requires 10 visits that have their own reference angle depending on scheduling, with a minimum separation angle of 5 degrees. In addition, the K-sequence introduces 4 different angles.

The CPC observations are executed with the four red grisms over the full area, and cover at least \(3\times3\) fields with the blue grism during PV phase.

Targets and pointing constraints

Table 17: CPC fields. CSV file

# ID

R.A.

Dec

CPC-N

269.733

+66.018

CPC-S

61.241

-48.423

Instrument configuration

Instrument: Wide survey

Inter-operability constraints

None

Dependencies

Fulfilling

Fulfilled by

CALBLOCK-F-003: Completeness and Purity Calibration (CPC)

Time-critical

No.

Validation

Recovery

In-orbit duration

Processing time

Processing input

Ground Processing Input Data:

Data Description:

Data volume

Processing tools

Processing element

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

Quality control parameters

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

Required accuracy, constraints

Processing method

Processing output

Contact person

Calibration Lead

Status

2026/09/18 - In progress.

FLAG

Priority

Observation record

Comments