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Field nameContentExamples
Scheduler

Type of scheduling to use. Default is to use the dynamic scheduler, so scheduling units are picked up automatically, but it is possible to specify fixed time scheduling.

Dynamic
Fixed time

time atRun observations at this specific time. Only use this if really required, e.g., the target is also observed with another telescope. Specifying this option circumvents priority scheduling and should be used with care.
time after

Minimum start time of this scheduling unit. Default: start of cycle

(info) Observations will by default also be scheduled only in the cycles connected to the project.

2021-06-01 00:00:00
time beforeMaximum end time of this scheduling unit. Default: end of cycle2021-11-30 23:59:59
time betweenOnly schedule within the time windows specified here. More time-windows can be specified by pressing the + button below. This can be used to distinguish observations that should run monthly be specifying a few days where these observations could run.From: 2021-07-08 00:00:00
Until:
2021-07-10 23:00:00
time not betweenDo not schedule within the time windows specified here. More time-windows can be specified by pressing the + button below.From: 2021-07-08 00:00:00
Until:
2021-07-10 23:00:00
Daily

require_day : Day time observations. Run when the sun is higher than 10 degrees above the horizon at the Superterp.

require_night : Night time observations. Run when the sun is lower than 10 degrees above the horizon at the Superterp.

avoid_twilight : Avoid sunrise and sunset. Run when the sun is higher than 10 degrees above the horizon at the Superterp, or lower than 10 degress below the horizon.


transit_offsetOffset in (UTC) seconds from transit for all target beams in the observation. Alternatively, use you can specify the reference pointing as the reference for transit. When the observation is split into shorted chunks to be observed at different LST ranges. Please take into account a one minute gap between subsequent observations.from -7200 to 7200
from -7200 to -3600
from 3600 to 7200
min_distance

Minimum distance to the Sun, Moon and Jupiter (latter mostly relevant below 30 MHz) in degrees (backend uses radians).

Current default 30, or 28.64 degrees

Sun: 30
Moon: 30
Jupiter: 30 (< 40 MHz ) else 15
min_elevation.targetMinimum elevation for all SAPs in the target observations
min_elevation.calibratorMinimum elevation for the SAP of all calibrator observations
Reference pointing

If true, will be used for scheduling calculations taking into account the transit_offset

Note: If used, the reference pointing direction should be identical to the tile beam pointing direction (for HBA).

enabled=false

enabled=true
pointing.angle1=12h30m00s
pointing.angle2=50d00m00s
pointing.reference_frame=J2000
pointing.target = LST=12.5

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Task ParameterPresent in these strategiesDescriptionExamples
Duration All except BF FE - Ionospheric Scintillation and FE RT TestObservation duration in hour:min:sec. For HBA strategies there are additional duration fields for the calibrators and/or additional targets/beam pointing. Similarly some modes have Target Duration which is given in seconds.

00:02:00 (hour:min:sec)

28800 (sec)

Observation Description All except BF FE - Ionospheric Scintillation and FE RT TestUsually target (and/or calibrator) name

OOO.O _Target_name_

FRB YYYYMMDDA

Paaa+01 & Paaa+02

Pipeline Description All except BF FE - Ionospheric Scintillation and FE RT TestUsually target pipeline (and/or calibrator pipeline) name

oOOO.O _Target_name_

FRB YYYYMMDDA/pulp

Paaa+01/TP

Target Pointing All except BF FE - Ionospheric Scintillation and FE RT TestDefine pointing to target(s and/or calibrator(s)) given in Angle 1 (RA), Angle 2 (DEC), Reference frame (J2000) and target name

Angle 1: 02h31m49.09s

Angle 2: 89d15m50.8s

Reference frame: J2000

Target: _Target_name_

Digifil optionsBF CV FRB

Relevant options for siggle-pulse searches

DM: 0.0001

Nr of Frequency Channels: 320

Coherent Dedispersion: true

Integration time: 4

Raw outputBF CV FRB and BF CV Timing ScintillationWhether to include the raw data in each output data product

false

true

Sub-band per fileBF CV FRB and BF CV Timing Scintillation

The maximum number of sub-bands to write in each output data product.


20

Optimize period and DM

BF CV Timing Scintillation and BF Pulsar Timing

false

true

Sub-integration time

BF CV Timing Scintillation and BF Pulsar Timing
10

Frequency channel per file

BF CV Timing ScintillationNumber of frequency channels per part (multiple of subbands per part).120
Duration FE (1..4)
BF FE - Ionospheric Scintillation, FE RT Test and Solar CampaignDuration of (one of the) the fly's eye (FE) observation in seconds. Needs to fit within the overall SU duration.
300 (sec)
Description FE (1..4)
Solar Campaign
IPS FE1
Pointing FE (1..4)
Solar CampaignDefine FE pointing given in Angle 1 (RA), Angle 2 (DEC), Reference frame (J2000) and IPS name

Angle 1: 02h31m49.09s

Angle 2: 89d15m50.8s

Reference frame: J2000

Target: _Target_name_IPS

FrequencyIM HBA 1 beam and IM LBA 1 beamFrequency range of the observation, i.e. bandwidth covered.

LBA: 21.4-69.0

HBA: 120.2-126.7,126.9-131.9,132.1-135.3 etc.

Sub-bandsIM HBA 1 beam and IM LBA 1 beamSub-band numbers specification (alternative to frequency). For Range enter Start and End separated by 2 dots. Multiple ranges can be separated by comma. Minimum should be 0 and maximum should be 511. For example 11..20, 30..50

false

true


HBA: 104..136,138..163,165..180,182..184,187..209,212..213, etc.

Run adderIM HBA 1 beam, IM LBA 1 beam, IM HBA LoTSS 2 beam and IM LBA LoDSS 5 beamDo/Don't create plots from the QA file from the observation

false

true

Tile BeamIM HBA LoTSS 2 beamHBA Only, insert pointing of the tile beam given in Angle 1 (RA), Angle 2 (DEC), Reference frame (J2000) and target name. Should be between (average of) the SAP pointings.

Angle 1: 02h31m49.09s

Angle 2: 89d15m50.8s

Reference frame: J2000

Target: Paaa+01Paaa+02REF

FilterIM LBA 1 beamBandpass filter applied

LBA_10_90

HBA_110_190

Antenna setIM LBA 1 beamSelect the antenna mode to observe with

LBA_SPARSE_EVEN

HBA_DUAL_INNER

Time averaging steps

IM LBA 1 beam, IM LBA 1 beam and IM LBA Survey 3 beamFactor used to average the data in time2

Freq averaging steps

IM LBA 1 beam, IM LBA 1 beam and IM LBA Survey 3 beamFactor used to average the data in frequency3
Demix pipelineIM LBA 1 beam and IM LBA Survey 3 beam.Given in several drop-down menus per target/calibrator where the user can select what sources to demix. Note that the time step and frequency step in this menu have to be multiples of the previously defined averaging steps.

Sources: CasA, CygA, HerA, HydraA, TauA, VirA

Time step: 8

Ignore Target: false

Frequency step: 64

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