CALBLOCK-PV-007: Early-release observations¶
Observation configuration file¶
Not applicable
Scheduling¶
Early-release observations (ERO) of several targets, whenever they fit into the PV plan.
In case of failure: These observations are target-specific, and the target might have a very limited visibility; in this case it should not be repeated, and the remaining PV plan should not be disturbed. If the target has perennial visibility and has high scientific value, it could be appended at the end of PV phase.
Time-critical¶
No.
Dependencies¶
CALBLOCK-F-001: Self Calibration
CALBLOCK-F-007: VIS Nonlinearity, PTC, BFE and NISP LED flats
Objective¶
Early-release targets show-case Euclid’s potential as a survey telescope. The list of potential targets must be safe for Euclid to observe, and should cover a broad range of ecliptic longitudes and latitudes to accomodate launch date uncertainties.
Observations¶
Good image quality is essential, but we don’t need weak lensing performance, nor fulfill the CalCD-B requirements. Yet the fluxing of all data should be consistent across the focal planes to make the data scientifically valuable. Only the ROS is permitted as an observing sequence.
VIS Cycling: The VIS ROS-inline calibrations follow the nominal wide-survey cycling, as described in ROS: inline VIS calibrations and cadences.
Targets and pointing constraints¶
Pointing: Straylight suppression as per MOCDA-SYS-003.
# ID |
R.A. |
Dec |
Comment |
Undisclosed |
TBD |
TBD |
TBD |
Instrument configuration¶
Instrument: Wide survey
Methodology / Uplink procedure¶
Entity: NISP, VIS
Commanding Method: NISP: Observation, VIS: Science
Dither Sequence: ROS
Inter-operability constraints¶
None
In-orbit duration¶
In-orbit Duration: 24 h
Data volume¶
20*ROS = 99620 MB, assuming 20 executions of the ROS or 5 targets doable in 24 h.
Processing input¶
Ground Processing Input Data: All baseline calibration products, can be from ground
Data Description: Standard ROS data
Processing method¶
Standard SGS processing.
Processing output¶
Color images for the general public, and potentially photometric catalogs.
Processing tools¶
L1 pipelines
Validation¶
At the least good image quality.
Recovery¶
None.
Quality control parameters¶
DataModel: https://gitlab.euclid-sgs.uk/
Contact person¶
Survey Scientist (Roberto Scaramella), Calibration lead