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Field name | Content | Examples |
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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 |
time at | Run 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 Observations will by default also be scheduled only in the cycles connected to the project. | 2021-06-01 00:00:00 |
time before | Maximum end time of this scheduling unit. Default: end of cycle | 2021-11-30 23:59:59 |
time between | Only 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 between | Do 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_offset | Offset 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.target | Minimum elevation for all SAPs in the target observations | |
min_elevation.calibrator | Minimum 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 |
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Task Parameter | Present in these strategies | Description | Examples |
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Duration | All except BF FE - Ionospheric Scintillation and FE RT Test | Observation 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 Test | Usually 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 Test | Usually 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 Test | Define 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 options | BF CV FRB | Relevant options for siggle-pulse searches | DM: 0.0001 Nr of Frequency Channels: 320 Coherent Dedispersion: true Integration time: 4 |
Raw output | BF CV FRB and BF CV Timing Scintillation | Whether to include the raw data in each output data product | false true |
Sub-band per file | BF 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 Scintillation | Number of frequency channels per part (multiple of subbands per part). | 120 |
Duration FE (1..4) | BF FE - Ionospheric Scintillation, FE RT Test and Solar Campaign | Duration 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 Campaign | Define 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 |
Frequency | IM HBA 1 beam and IM LBA 1 beam | Frequency 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-bands | IM HBA 1 beam and IM LBA 1 beam | Sub-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 adder | IM HBA 1 beam, IM LBA 1 beam, IM HBA LoTSS 2 beam and IM LBA LoDSS 5 beam | Do/Don't create plots from the QA file from the observation | false true |
Tile Beam | IM HBA LoTSS 2 beam | HBA 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 |
Filter | IM LBA 1 beam | Bandpass filter applied | LBA_10_90 HBA_110_190 |
Antenna set | IM LBA 1 beam | Select 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 beam | Factor used to average the data in time | 2 |
Freq averaging steps | IM LBA 1 beam, IM LBA 1 beam and IM LBA Survey 3 beam | Factor used to average the data in frequency | 3 |
Demix pipeline | IM 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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