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Triggering WEAVE Targets of OpportunityIMPORTANT: For operational reasons, triggering of WEAVE ToOs is temporarily suspended. When WEAVE operations resume, we will let you know. What can be triggeredThe observing strategy at execution must match what was requested and approved in the proposal, and triggers must not exceed the allocated time (see table below). ING anticipates executing at most one ToO trigger per night, on a first-come, first-served basis.WhenAt present, ING supports next day triggers: for an event scheduled to be observed on a given night, the trigger must be received by the Observatory no later than 12:00 noon on the preceding day. ING will strive to execute ToO programmes on a shorter timescale on a best-effort basis.Who can triggerPIs of allocated ToO-programmes can trigger if the ToO programme is currently active and time remains for triggers. The following table lists the currently active programmes, their allocations and time remaining. |
| WEAVE ToO programmes currently active | ||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Programme | Mode | Principal investigator | Title | Allocation incl. overheads | Band | Trimesters | OBs | Science time | ||||||
| SW2026a09 (WS2026A2-009) | LIFU LR_BR | Peter Jonker | Rapid WEAVE/LIFU redshift and host characteristics of Fast X-ray Transients | 15.2h | A | 26A2-26B1 | COMPLETE:0 | NEW:0 NEW_active:0 | OBSERVED: 0.0h | ALLOCATED: 12.0h | REMAINING: 12.0h | |||
| SW2026a11 (WS2026A2-011) | LIFU LR_BR | Jan van Roestel | Rapid followup of transients in the nearby Galaxy found by BlackGEM | 7.4h | A | 26A2-26B1 | COMPLETE:0 | NEW:0 NEW_active:0 | OBSERVED: 0.0h | ALLOCATED: 6.0h | REMAINING: 6.0h | |||
How to triggerStep 1: Prepare a CSV catalogueSee instructions on how to prepare a CSV catalogue at WEAVE Open-Time Phase 2: The Short Guide. An example of a CSV catalogue follows.
filename: [eg: WS2026A2-010_target_list.csv]
Use PROGTEMP and OBSTEMP builders. IFU_DITHER can be 0 for no dithering or 3,4,5 or 6 for point ditehring. Note that number of exposures per OB and dithering points must match. We can only provide the standard values for position angle, ie. 0° for declinations south of +28.7° and 180° for north of +28.7°. Step 2: Fill out the template below, attach CSV catalogue and emailFollow instructions in square brackets.
Step 3: Preparation of OBs and observingThe ING trigger team will make the requested OBs and ingest into the observing queue. Observations will be attempted at the earliest opportunity, following the provided instructions.Data retrievalAllow for a one or few days before the data are reduced and L1 products are made available on the WEAVE Operational Repository (login with the programme's credentials). If urgent assessment of the data is requested, then the observers will upload the data to the ING ftp server.Conflict resolutionIf multiple programmes trigger on the same night, unless precedence rules have been set, then the programme which was triggered first takes priority.Triggers are limited to a maximum of two hours' duration per night including all overheads, unless . If competing teams trigger for the same target and instrument setup, the observations will be attempted for the team whose request was received first. However, in these circumstances the teams may elect to share the data. In this event, the time used will be accounted on a 50% basis to the teams involved, and the duration of the override will be limited to two hours, including overheads. |
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