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Override Programmes

Before proposing an override programme, please visit the Applying for Telescope Time web pages.
  1. For Override Teams
  2. For Observers at the Telescope
  3. Allocations
  4. Conflict Resolution

1. For Override Teams

Vignetting at low elevation

The WHT lower dome shutter is currently (and probably until July 2013) out of action, and observations at elevation <25 deg will be vignetted (plot).

Step 1: CHECK

Before triggering, find your programme in the override-allocations table below and check:

  • Which programmes you can override and which instruments you can use, by checking what is scheduled for the night on the ING schedules.
  • The observations made so far of your programme and the limits for the semester.
  • The visibility of your targets (sky brightness, moon distance, airmass, telescope limits).
Overrides can only be triggered by a member of an Override Team (see the allocations table below for nominated members).

Step 2: PHONE

The 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. This phone call will establish precedence in the event of more programmes being activated that night.

Contact Phone
WHT Control Room +34 922 405 559
INT Control Room +34 922 405 640

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: EMAIL

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: +34 922 405 646 and let the observers know.

2. For Observers at the Telescope

Step 1: CHECK

Look for the triggering programme in the allocations table below and check the following:
  • Whether the observers' programme can be overridden, can be overridden only at the observers' discretion or cannot be overridden at all.
  • The maximum allowed duration of the override, including the overheads.
  • That the observing plan was correctly received from the Override Team, it is clear and it can be carried out.
If everything is fine then please acknowledge the triggering email from the Override Team replying to the sender and all copied recipients (including triggering.iac.es) and proceed to the next step. If anything is not clear, check the conflict resolution rules below and contact the Override Team as soon as possible.

Step 2: OBSERVE

Please 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: REPORT

Whether the attempt has been successful or not, always and immediately submit the “Night Report” below  right after obtaining the target data. The same night report can be edited and submitted later on with any remaining calibration frames, but the immediate submission of the night report  is critical for communicating the results, sending the data and taking any further observing decisions. The night report is also essential for recording the override programme's used time and triggers.

Override Report

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:

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)
ftp> cd whtguest/20110801
ftp> bin
ftp> prompt
ftp> passive
ftp> mget *
ftp> bye

The prompt and the passive commands should set the interactive and the transfer modes on respectively.

Or browsing 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/*

3. Allocations

Override Programmes Semester 2013A

WHT
Ref.ProgrammePITitleIf triggered, it overrides...Allowed triggers and observations made
any of these
instruments [1]
these programmes (see abbreviations)CommentsWho can
trigger
EmailsMaximum
individual
duration
(incl.
overheads)
hh:mm
Triggers
observed /
 Allowed
this
semester
Time
Observed /
 Allowed
this
semester
(incl.
overheads)
hh:mm
Dates
observed
neveronly at
the discretion
of the
observer
always
P27W/2013A/27Levan The diverse nature of GRBs and their role as probesACAM
ISIS
LIRIS
PFIP
ULTRACAM
P6 (Hasswell)
P9 (Watson)
P41 (Page)
P42 (Evans)

Comm#
C#
N#
S, S/D, D
P#
[1] Late-time overrides for outbursts of age greater than ten days are restricted to S or S/D nights, but may proceed on scheduled nights at observer's discretion.
[2] Defers to P3 (Dhillon) on scheduled nights irrespective of which triggers first.
[3] Both can be executed on S or S/D nights.
Levan
Tanvir
Wiersema
Rol
Gorosabel
a.j.levan@warwick.ac.uk
kw113@leicester.ac.uk
nrt3@star.le.ac.uk
jgu@iaa.es
02:00
3 / Any
05:56 / 15:002013-04-30
2013-06-06
2013-06-17
P3W/2013A/03Dhillon Optical spectroscopy of LOFAR transientsACAMP6 (Hasswell)
P9 (Watson)
P41 (Page)
P42 (Evans)

Comm#
C#
N#
S, S/D, D
P#
[1] Takes precedence over P27 (Levan) on scheduled nights irrespective of which triggers first.
[2] Both can be executed on S or S/D nights.
Dhillon
Jonker
Wijnands
Daw
Fender
Stappers
vik.dhillon@sheffield.ac.uk
p.jonker@sron.nl
r.a.m.j.wijers@uva.nl
r.fender@soton.ac.uk
01:30
0 / 3
00:00 / 04:30
C105105-MULT-4/13AEderoclite Spectro-Photometric Target Of Opportunity Follow-up of Classical NovaeACAMC6 (Martinez)
C34 (Bouy)
C51 (Miles)
C72 (Ferre)
CAT DDT

Comm#
N#
P#
C#S, S/D, DEderocliteaederocl@cefca.es
00:18
0 / 4
00:00 / 01:12
C29029-MULT-5/13AGorosabel Sub-proposal II, 3 telescopes for 3 sharp GRB science cases: the WHT to study short GRBs, the LTLIRIS
ISIS
ACAM
C6 (Martinez)
C10 (Maiz)
C14 (Jimenez)
C34 (Bouy)
C51 (Miles)
C63 (Allende)
C72 (Ferre)
C123 (Seidel)
C130 (Murgas)
CAT DDT

Comm#
N#
P#
S, S/D, D
C#
Gorosabel
Castro-Tirado
Levan
Rol
Tanvir
jgu@iaa.es
a.j.levan@warwick.ac.uk
nrt3@star.le.ac.uk
01:00
0 / 3
00:00 / 03:00
N9W13AN009Hartoog Gamma Ray Bursts : Their Nature and Use as Cosmological ProbesACAM
ISIS
LIRIS
ULTRACAM
N5 (Jonker)
N7 (Kuijken)
N8 (Mahony)
N10 (Brinchmann)
N14 (Birkby)
N15 (Brogi)

Comm#
C#
P#
S, S/D, D
N#
[1] Late-time overrides for outbursts of age greater than ten days are restricted to S or S/D nights, but may proceed on scheduled nights at the discretion of the observer.
[2] Defers to N1 (Jonker) on scheduled nights irrespective of which triggers first.
[3] Both can be executed on S or S/D nights.
Hartoog
Rol
Kamble
Wiersema
Tanvir
Levan
O.E.Hartoog@uva.nl
kw113@leicester.ac.uk
kamble@uwm.edu
nrt3@star.le.ac.uk
A.J.Levan@warwick.ac.uk
02:00
4 / Any
07:09 / 15:002013-02-15
2013-05-08
2013-05-16
2013-06-03
N1W13AN001Jonker WHT/ACAM optical spectroscopy of LOFAR transientsACAMN5 (Jonker)
N8 (Mahony)
N14 (Birkby)
N15 (Brogi)

Comm#
C#
P#
S, S/D, D
N#
[1] Takes precedence over N9 (Hartoog) on scheduled nights irrespective of which triggers first.
[2] Both can be executed on S or S/D nights.
Jonker
Wijnands
Fender
Wijers
Dhillon
Torres
p.jonker@sron.nl
vik.dhillon@sheffield.ac.uk
r.a.d.wijnands@uva.nl
r.fender@soton.ac.uk
r.a.m.j.wijers@uva.nl
01:30
0 / 3
00:00 / 04:30
INT
Ref.ProgrammePITitleIf triggered, it overrides...Allowed triggers and observations made
any of these
instruments [1]
these programmes (see abbreviations)CommentsWho can
trigger
EmailsMaximum
individual
duration
(incl.
overheads)
hh:mm
Triggers
observed /
 Allowed
this
semester
Time
Observed /
 Allowed
this
semester
(incl.
overheads)
hh:mm
Dates
observed
neveronly at
the discretion
of the
observer
always
C29029-MULT-5/13AGorosabel Sub-proposal II, 3 telescopes for 3 sharp GRB science cases: the WHT to study short GRBs, the LT to monitor long GRBs, and the INT to identify FERMI GRBs.WFCC4 (Casares)
C12 (Bouy)
C18 (Cornelisse)
C156 (Damian)

INO#
NEON
N#
P#
CAT S
C#
D
Gorosabel
Castro-Tirado
Levan
Rol
Tanvir
jgu@iaa.es
nrt3@star.le.ac.uk
a.j.levan@warwick.ac.uk
01:00
0 / 1
00:00 / 01:00

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.


Semester:


4. Conflict Resolution

4.1. For visiting astronomers: overrides on scheduled nights

Only 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. 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.

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 nights

There is no limit on the number of override programmes that can be observed on a service night or discretionary night (WHT S, S/D and D nights and INT CAT S and D nights).

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. 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 precedence, except if service Target-of-Opportunity and/or Time-Critical observations, 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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Contact:  (Override Manager)
Last modified: 04 June 2013