ING ANNOUNCEMENT OF OPPORTUNITY FOR OBSERVING TIME IN 2003A
Contents
1. ING Instrumentation in Semester 2003A
2. Time-share Agreement with TNG for NL and UK Observers
3. Withdrawal of IDS
4. Discontinuation of the INT Service Programme
5. Withdrawal of the JKT from normal service
6. Telescope Support
1. ING Instrumentation in Semester 2003A
----------------------------------------
General Information
Detailed information on ING instrumentation offered for the
forthcoming semester can be found in the ING web pages at
http://www.ing.iac.es/Astronomy/observing/instruments.html
and guidelines for proposal submission can be found at
http://www.ing.iac.es/Astronomy/observing/INGinfo_home.html
Applicants should refer to these pages for the latest information,
and are reminded that occasionally highly rated proposals may not
be awarded time due to scheduling constraints.
Prospective NAOMI/INGRID applicants are encouraged to read the
most recent performance summary:
http://www.ing.iac.es/~crb/wht/aoperf.html
and prospective applicants for NAOMI/INGRID with the coronograph
OSCA are encouraged to read:
http://www.ing.iac.es/Astronomy/instruments/osca/
Instrumentation Overview
WHT http://www.ing.iac.es/Astronomy/telescopes/wht/
---
WHT applicants are encouraged to submit proposals for larger time
applications. For the UK community, the PATT2 application form
allows a 2-page scientific justification for proposals for six or
more nights.
The following instrument/detector configurations are available:
Instrument Detector
ISIS BLUE EEV12
ISIS RED MARCONI2
AUX-port TEK1
PRIME 2xEEV Mosaic
AUTOFIB2/WYFFOS TEK6
INGRID 1kx1k HgCdTe
NAOMI/INGRID 1kx1k HgCdTe (shared-risks)
NAOMI/INGRID/OSCA 1kx1k HgCdTe (shared-risks)
Notes
NAOMI: Observations will be carried out in service mode.
AUTOFIB2: The large fibres module has been withdrawn.
It is also expected that a new camera will be
commissioned by mid-semester 2003A. AF2 runs in
2003A which use the new camera will therefore
be shared-risk.
INTEGRAL This will not be offered as a common user instrument.
WHT visitor-instrument contacts are:
PN.S Nigel Douglas, ndouglas@astro.rug.nl
SAURON Tim de Zeeuw, tim@strw.leidenuniv.nl
S-CAM Michael Perryman, mperryma@astro.estec.esa.nl
Ultracam Vik Dhillon, vik.dhillon@sheffield.ac.uk
INT - http://www.ing.iac.es/Astronomy/telescopes/int/
---
The following instrument/detector configurations are available:
Instrument Detector
WFC 4xEEV
IDS 235/500 EEV10 or TEK5
INT visitor instrument contacts are:
CIRSI Richard McMahon, rgm@ast.cam.ac.uk
Observing time is allocated in blocks of one week on average,
and observing programmes shorter than *4* nights are not
accepted, unless explicitly agreed in advance by the Head of
Astronomy or the Director of ING.
JKT - http://www.ing.iac.es/Astronomy/telescopes/jkt/
---
Only one instrument/detector configuration is available:
Instrument Detector
Direct imaging 2kx2k SITe2
The JKT only supports one common-user instrument, and private
instruments are not accepted. Although there is no formal limit
on the duration of observing runs on the JKT, short proposals
are discouraged, and observing time is usually allocated in
blocks of ~1 week.
2. Time-share Agreement with TNG for NL and UK Observers
-------------------------------------------------------
The time-share agreement with the TNG proved to be very
successful in semester 2002B, and continues in semester
2003A. In this scheme, NL and UK observers may apply to use
three TNG instruments. These are:
+ The high resolution spectrograph, SARG
+ The near infrared camera-spectrometer, NICS, in non-AO
spectroscopy mode only
+ The multi-object low-resolution optical spectrograph, DOLORES
A minimum of five nights is available in total in semester
2003A to the NL and UK communities, and in return the Italian
community obtains access to the WHT for the same number of
nights. More than five nights may be exchanged if such demand is
balanced between both telescopes.
For further details on the TNG observing guidelines and for
instrumentation details, refer to:
http://www.tng.iac.es/
Select "instruments" for detailed information on SARG, NICS and
DOLORES.
Please note that NL and UK applicants for SARG, NICS or DOLORES
should apply using their standard PATT/NL form and should send
these to their own national TAGs. DO NOT APPLY DIRECTLY TO TNG.
(CAT observers should apply for TNG time in the usual way).
Successful NL and UK applicants to TNG will qualify for EC funding
under the auspices of the EC's Access to Research Infrastructures
Programme to cover travel, accommodation and subsistence costs,
assuming they meet the criteria for eligibility. For further
details of this general scheme see:
http://www.otri.iac.es/eno/
3. Withdrawal of IDS
--------------------
Prospective applicants to the INT are reminded that due to the
impact of cost savings at ING, semester 2003A will be the last
semester in which the Intermediate Dispersion Spectrograph, IDS,
is offered.
4. Discontinuation of the INT Service Programme
-----------------------------------------------
Due to the impact of cost savings at ING, the scheme of service
observing on the INT carried out by observatory personnel will be
discontinued at the end of Semester 2003A.
5. Withdrawal of the JKT from normal service
--------------------------------------------
Due to the impact of cost savings at ING, the JKT will be taken
out of normal service at the end of semester 2003A. The JKT may
continue in operation beyond 2003A as a special-purpose telescope
with external funding, but 2003A will be the final semester in which
it is offered as a general-user facility.
6. Telescope Support
--------------------
Astronomical support is provided on the first night of each run
on the WHT, INT and JKT. Telescope Operator (TO) support is
provided for each night of all WHT runs. INT Wide Field Camera
runs have TO support for the first two nights only, and INT IDS
runs of six or more nights will have TO support for the first three
nights only. TO support is not provided on the JKT.
Observers are reminded that filter and/or grating changes within
a run will be accommodated provided that they have been explicitly
requested in the telescope proposal. However, due to limited human
resources, additional changes to the instrumental configuration
may not be accommodated.
D.Lennon
Sept. 2002
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