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ING Instrumentation Options 2003B
This page gives an overview of the instrumentation available on the WHT and INT. It is revised bi-annually to reflect the options offered in each semester. Full information on all the listed instruments is indexed in the Manuals Home Page, and information on older instruments can be found on-line in the Obsolete Instruments section of the Manuals Home Page.

Change to UK PATT Submission Deadlines

Following the recent review of PATT, PPARC has agreed to move the deadlines for UK proposal submission earlier by two weeks to 15th March for B Semesters, and 15th September for A Semesters. This change will take place with immediate effect; the deadline for receipt of UK proposals for Semester 2003B will be midnight GMT on 15th March, 2003.

UK applications must be submitted on the current version of the PATT2 form, version 02/2003.

NAOMI/INGRID and OSCA

Prospective NAOMI/INGRID applicants should read the most recent performance summary.
Prospective applicants wishing to use the coronograph OSCA with NAOMI/INGRID should read its homepage.

Use of the INT and JKT

Due to the impact of cost savings at ING, IDS is no longer offered as a common-user instrument. The INT service programme, in which service observations are carried out by observatory personnel, has been discontinued.

Also for reasons of cost savings, the JKT is no longer offered as a general-user facility.

TNG Timeshare

As part of a continuing collaboration between ING and TNG, 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 spectroscopic mode only
  • The multi-object low-resolution optical spectrograph, DOLORES
Five nights are available, and NL and UK applicants should submit proposals on their standard application forms to the NFRA PC and UK PATT respectively.

Spectroscopy
Instrument/Contact Wavelength Range (Å) Dispersion (Å/pixel) Slit Length Detector Comments
4.2-m William Herschel Telescope




ISIS Spectrograph
Javier Licandro
3000-10000Å 0.19-2.90 (Tek4)
0.11-1.63 (EEV12)
4' Red: Marconi2
Blue: EEV12
Spectro- and/or
Imaging Polarimetry
AUTOFIB2/WYFFOS
Romano Corradi
3500-10000Å R=100-3000 (ref.)
R=7500 (ech.)
1.6" fibres Tek6 (§) Up to 150 objects


Imaging
Instrument/Contact Detector Filters Scale ("/pixel) Field-of-View
4.2-m William Herschel Telescope        
Prime Focus Mosaic CCD camera
Almudena Zurita
2EEV see database 0.24 16'.2 x 16'.2
Aux Port Imager (§)
Chris Benn
Tek2 UBVRI default 0.11 1'.8
INGRID (Cass)
Almudena Zurita
HgCdTe (1024x1024) ZJHKK_s
and 10 narrow-band
0.24 4'.1
NAOMI/INGRID
Chris Benn
HgCdTe (1024x1024) ZJHKK_s
and 10 narrow-band
0.04 42"
NAOMI/INGRID/OSCA
Sebastian Els
HgCdTe (1024x1024) ZJHKK_s
and 10 narrow-band
0.04 42"
2.5-m Isaac Newton Telescope        
Wide Field Camera
Robert Greimel
4 of 4k x 2k EEV see database 0.33 33'.8 x 33'.8


The following instruments have visitor instrument status at the ING. Applicants wishing to submit proposals to use a visitor instrument should contact the relevant Instrument Contact in the first instance.

Visitor Instruments
Instrument Institute Instrument Contact
4.2-m William Herschel Telescope    
Integral IAC Evencio Mediavilla
PN.S Kapteyn Nigel Douglas
SAURON Lyon/Leiden/Durham Tim de Zeeuw
S-CAM ESA Michael Perryman
Ultracam Sheffield Vik Dhillon

§ Notes


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Last Updated: 6 February 2003
Ian Skillen