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Home > Astronomy > Override Programmes |
Override Programmes
IMPORTANT: Trigger information
Step 1: CHECKBefore triggering, find your programme in the override-allocations table below and check:
Step 2: PHONEThe Override Team must make phone contact with the observers prior to execution of the observations in order to obtain an email address where to send the request and find out about the instrument setups and modes currently available. This phone call will establish precedence in the event of more programmes being activated that night.
If the phone numbers above are unavailable, please phone the Residencia (+34 922 405 500) and ask for the relevant control room; or call the OSA mobile phone (+34 616 97 45 13), available only from 19:30 (summer) or 18:30 (winter) until sunrise every night. Step 3: TRIGGEROverrides can only be triggered by a member of an Override Team (see the allocations table below for nominated members). Email the override request template to the observer and to triggering.iac.es. This will automatically forward the communication to the Observing Support Assistants (OSAs), Support Astronomers (SAs) and Override Programme Manager. If bounced, then please fax the request to WHT's control room: +34 922 425 448 and let the observers know. We recommend triggers are emailed as soon as possible. Our email template allows specifying the night when observations are requested. Delaying a trigger can result in unnecesary time losses and inconvenience when setting up for the night, while an early trigger helps planning the night better. Step 1: CHECKLook for the triggering programme in the allocations table below and check the following:
If anything is not clear (instrument setups, number of overrides allowed per night), check the conflict resolution rules below and contact the Override Team as soon as possible. Copy messages to the Override Manager at overrideing.iac.es. Step 2: OBSERVEPlease observe at the earliest opportunity on the timescale requested by the Override Team. For example, prompt reaction to rapid-response GRB programmes is important and target acquisition should commence immediately on receipt of the alert if so requested by the GRB team. For other GRB triggers target acquisition should commence no later than thirty minutes after the phone request, unless a more relaxed observation timeline is confirmed by the GRB team.Non-ACAM observers undertaking an ACAM override should seek advice from the OSA about how to configure and use the instrument, and if the Override Team submitted a specific ACAM observing sequence, then proceed to execute. Step 3: REPORTWhether the attempt has been successful or not, always and immediately submit the Override Report below right after obtaining the data. The same report can be edited and resubmitted later with any remaining calibration frames, for instance, but the immediate submission of the report is critical for communicating the results, sending the data to the override team and taking any further observing decisions. This report is also essential for recording the override programme's used time and triggers.
Only if the above form is not available (the form is only available at the ING intranet) or the file upload failed, then follow these alternative instructions: The data should be copied promptly to the appropriate directory in the anonymous ftp area. For example, as user whtguest (replace wht by int below for INT observers) on any public linux PC (for instance, WHTDRPC1 or INTDRPC1):
mkdir /obsdata/outgoing/whtguest/20110801
cp /obsdata/whta/20110801/files /obsdata/outgoing/whtguest/20110801 gzip /obsdata/outgoing/whtguest/20110801/*
chmod 555 /obsdata/outgoing/whtguest/20110801/* Then the data can be retrieved from the ING ftp server as follows:
user> ftp ftp.ing.iac.es (login as anonymous, password your email address) (The prompt and the passive commands should set the interactive and the transfer modes on respectively. Or you can also browse the data as an anonymous user:
ftp://ftp.ing.iac.es/whtguest/20110801/ Please email the downloading instructions and their description promptly to the override team and to the Override Programme Manager (overrideing.iac.es). Delete the files once downloaded: rm /obsdata/outgoing/whtguest/20110801/* Step 4: FURTHER ACTIONS The Spanish CAT time-allocation committee requests from the observers some other actions, please visit CAT override programmes. |
WHT | ||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Reference (PI) Programme "Title" | If triggered, it overrides... | Allowed triggers and observations made | ||||||||||||||
any of these instruments [1] | these programmes (see abbreviations) | Comments | Who can trigger | Maximum individual duration (incl. overheads) hh:mm |
Triggers observed / total allowed | Time observed / total allowed (incl. overheads) hh:mm | ||||||||||
never | only at the discretion of the observer | always | ||||||||||||||
Notes: [1] Any of the listed instruments if scheduled (ie. shown in the instrument column of the ING schedules). Please note that ACAM is always available when observing at Cassegrain, and not necessarily it is scheduled. |
INT | ||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Reference (PI) Programme "Title" | If triggered, it overrides... | Allowed triggers and observations made | ||||||||||||||
any of these instruments [1] | these programmes (see abbreviations) | Comments | Who can trigger | Maximum individual duration (incl. overheads) hh:mm |
Triggers observed / total allowed | Time observed / total allowed (incl. overheads) hh:mm | ||||||||||
never | only at the discretion of the observer | always | ||||||||||||||
C30 (de la Fuente) 030-MULT-2/24A "Tweaking Synthetic Tracking as a Discovery Tool of Near Earth Asteroids" | WFC Default setup: | C# ITP# N# P# | CAT S D | Raul de la Fuente Marcos (rauldelafuentemarcos@gmail.com) | 01:50 / 05:00 Nights and | |||||||||||
C102 (Castro) 102-MULT-4/24A "GTC follow-up of gravitational radiation sources in the Multi-messenger Era" | WFC Default setup: | C# ITP# N# P# | CAT S D | Alberto Javier Castro Tirado (ajct@iaa.es) | 00:00 / 30:00 | |||||||||||
N2 (Vaduvescu) ING.NL.24A.002 "Detection of Near Earth Asteroids Using Synthetic Tracking" | WFC Default setup: | C# CAT S ITP# N# P# | D | Ovidiu Vaduvescu ovidiu.vaduvescu@gmail.com | 00:15 / 02:00 Nights and | |||||||||||
Notes: [1] Any of the listed instruments if scheduled (ie. shown in the instrument column of the ING schedules). Please note that ACAM is always available when observing at Cassegrain, and not necessarily it is scheduled. |
4.1. For visiting astronomers: overrides on scheduled nightsOnly one authorised programme can override a scheduled programme per night. If multiple override programmes were triggered on the same night, please check the observing priorities in the column 'Comments' of the allocations table. If no priority was specified there, then give priority to the programme which was triggered first.Overrides by a given programme are limited to a maximum of two hours' duration per night including all overheads, distributed in no more than two distinct slots, unless a maximum duration is indicated for that specific programme (see allocations table). For example precursor imaging observations followed by spectroscopic observations if quick-look analysis of the imaging data indicates that this is merited, or subsequent override being requested by the same team within the night for a different target. In general, longer observations could proceed at the discretion of the scheduled observer. Overrides which require a switch of focal station from that scheduled are permitted, but changes to the configuration of a specific instrument (e.g. filter-wheel content, dichroic or grating changes) may only be made with the permission of the observer affected and only if qualified ING staff are available to make such a change, and a observer is trained. Please note that some changes, for instance, from GRACE to ACAM, might be longer than others (~10-15 minutes), given the particular instrument setups, and any resulting overheads will be charged to the overriden time. Nights scheduled with adaptive optics allocations are usually annotated as Reference+S/D in the schedules. In these cases, 'S/D' refers to the allocated backup programme for non-AO conditions. These nights can be overridden in the same way as other programmes, as described in the allocations table and in the present section. 4.2. For support astronomers: overrides on service and discretionary nightsThe number of override programmes that can be observed on a service or discretionary night (WHT's S, S/D and D nights and INT's CAT S and D nights) is restricted to 2, unless time is shorter than one night, in which case it is restricted to only 1. Overrides by a given programme are limited to a maximum of two hours' duration per night including all overheads, distributed in no more than two distinct slots, unless a maximum duration is indicated for that specific programme (see allocations table). For example precursor imaging observations followed by spectroscopic observations if quick-look analysis of the imaging data indicates that this is merited, or subsequent override being requested by the same team within the night for a different target. In general, longer observations could proceed at the discretion of the scheduled observer. Overrides take always precedence, except if target-of-opportunity and/or time-critical service observations can never be overriden (see allocations table for details), or uninterruptable discretionary tasks are being done. Those service or discretionary observations must be completed before attempting the override programme. Only if the override request is for the same target as the one being observed as part of the service target-of-opportunity or time-critical proposal, then the override programme takes precedence over the service observations, and the data must be made available to the override team only. If more than one override programme is triggered, then all overrides should be queued according to whom triggered first, except if precedence rules were set (see allocations table) or if the triggering team has set observing constraints, as airmass, seeing, etc. If one override programme triggers while another override programme of lower-precedence is being observed, observations should be completed before attempting the higher-precedence programme. If the observations are for the same target, they should be delivered to whoever triggered the observations first. If competing override programmes trigger an override for the same target and instrumentation on a service night, the override 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 in the override 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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