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ING Instrumentation Options 2002A
This page gives an overview of the instrumentation available on the WHT, INT and JKT. 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.

NAOMI applicants are encouraged to check the NICMOS data archive before submitting applications.

Email links to the instrument specialists are given; please contact them directly if you require further information about any instrument.

SIGNAL can be used to calculate exposure times for any telescope/instrument/detector combination.

  • INGRID will be unavailable until late March
  • INTEGRAL will be available in the first half of the semester only
  • NAOMI will be available in the second half of the semester only
  • INGRID will be unavailable at Cass when in use with NAOMI in GHRIL
  • UES may be unavailable towards the end of the semester

As part of a collaboration between ING and TNG, NL and UK observers may apply to use the TNG high resolution spectrograph, SARG. Up to seven 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
Begoña Garcia
3000-10000Å 0.19-2.90 (Tek4)
0.11-1.63 (EEV12)
4' Red: Tek4
Blue: EEV12
Spectro- and/or
Imaging Polarimetry
UES Echelle Spectrograph (§)
Danny Lennon
3000-10000Å R=80,000=3.7km/s (2EEV)
R=54000=5.4km/s (SITe1)
3"-5' 2EEV
or SITe1

AUTOFIB2/WYFFOS (§)
Romano Corradi
3500-10000Å R=100-3000 (ref.)
R=7500 (ech.)
1.6" fibres Tek6 Up to 150 objects
INTEGRAL/WYFFOS
Begoña Garcia
3500-10000Å R=100-3000 (ref.)
R=6000 (ech.)
0".45-2".70 fibres
Up to 30" square FoV
Tek6 Area Spectroscopy/Imaging
2.5-m Isaac Newton Telescope




IDS spectrograph
Begoña Garcia
3500-10500Å 0.09-3.66 (EEV10)
0.17-6.50 (Tek5)
4' EEV10
or Tek5


Imaging
Instrument/Contact Detector Filters Scale ("/pixel) Field-of-View
4.2-m William Herschel Telescope        
Prime Focus Mosaic CCD camera
Thomas Augusteijn
2EEV see database 0.24 16'.2 x 16'.2
Aux Port Imager (§)
Thomas Augusteijn
Tek1 UBVRI only 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"
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
1.0-m Jacobus Kapteyn Telescope        
CCD Imager
Thomas Augusteijn
SITe2 see database 0.33 10' x 10'


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    
LDSS2 Durham Richard Bower
SAURON Lyon/Leiden/Durham Tim de Zeeuw
S-CAM ESA Michael Perryman
TAURUS IoA Richard McMahon
2.5-m Isaac Newton Telescope    
CIRSI IoA Richard McMahon
MUSICOS (§) ESA Bernard Foing

§ Notes

Previous Semesters
2001B
2001A
2000B

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Last Updated: 6 September 2001
Ian Skillen