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ING Instrumentation Options 2007B


This page gives an overview of the instrumentation available on the WHT and INT, and on the TNG as part of the Italian, NL and UK TNG-WHT timeshare programme. It is revised bi-annually to reflect the options offered in each semester; a summary of the time allocation process is also available.

Please email the instrument contact, listed in the tables, if you require further information about any instrument; important notes regarding specific instruments and procedures are given at the bottom of this page.



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 0.26-1.81 (Red+)
0.11-1.63 (EEV12)
4' Red: Red+
Blue: EEV12
Spectro- and/or
Imaging Polarimetry
LIRIS (§)
Michael Schirmer ]
9000-24000Å R=1000-3000 4.2' HgCdTe(1024x1024) Long-Slit and
multi-object
AUTOFIB2/WYFFOS
Romano Corradi ]
3500-10000Å R=100-3000 (ref.)
R=7500 (ech.)
1.6" fibres 2EEV Up to 150 objects
NAOMI/OASIS
Sam Rix ]
4000-10000 Å 1000 < R < 4000 2.7x3.7" to 7.4x10.3" field imaged
onto 1100 lenslets
MIT/LL (2048x4096) IFS,available with and without AO
2.5-m Isaac Newton Telescope      
IDS Spectrograph (§)
Javier Licandro ]
3000-10000Å 0.24-3.67 3.3' EEV10 235mm Camera
TNG-WHT Timeshare
3.6-m Telescopio Nazionale Galileo      
TNG/SARG
Ernesto Oliva ]
3700-10000 Å 29000 < R < 164000 Up to 30-arcsec 2EEV Echelle
TNG/NICS
Ernesto Oliva ]
9000-25000Å 50 < R < 2500 4-arcmin HgCdTe(1024x1024) Low, Medium Res
TNG/DOLORES
Ernesto Oliva ]
3000-10000Å 300 < R < 3000 Multi-slit 9'.4 FoV Loral 2K x 2K Multi-slit Low-Res


Imaging
Instrument/Contact Detector Filters Scale ("/pixel) Field-of-View
4.2-m William Herschel Telescope        
Prime Focus Mosaic CCD camera
Pierre Leisy ]
2EEV see database 0.24 16'.2 x 16'.2
Aux Port Imager (§)
Dan Bramich ]
Tek2 UBVRI default 0.11 1'.8
NAOMI/INGRID
Ian Skillen ]
HgCdTe(1024x1024) ZJHKK_s
and 10 narrow-band
0.04 42"
NAOMI/INGRID/OSCA
Ian Skillen ]
HgCdTe(1024x1024) ZJHKK_s
and 10 narrow-band
0.04 27"
LIRIS
Michael Schirmer ]
HgCdTe(1024x1024) ZJHK_s
and 8 narrow-band
0.25 4'.27
2.5-m Isaac Newton Telescope        
Wide Field Camera (§)
Romano Corradi ]
4 of 4k x 2k EEV see database 0.33 33'.8 x 33'.8


Visitor Instruments (§)
Instrument Institute 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


§ Important Notes
  • Applicants wishing to submit proposals to use a visitor instrument should contact the relevant Instrument Contact in the first instance. Applicants wishing to submit a proposal based on a new (to ING) visitor instrument should follow these instructions.
  • LIRIS slit-mask preparation and manufacture takes approximately two months; PIs awarded time in multi-slit mode are strongly encouraged to initiate the design of slit masks at the earliest opportunity. Details on slit-mask design and timelines are available; please email queries to Mischa Schirmer (mischa@ing.iac.es).
  • AUX port imaging is permanently available using CuSO4-U and Harris-BVRI filters only. Changes to other filters are permitted for runs scheduled specifically for Aux Port Imager.
  • The INT WFC is offered in rotator angle 180 degrees only. When there is compelling scientific justification, other rotator angles (0, 90 or 270-degrees) can be offered for the duration of the run; changes to the rotator angle within a run are not permitted.
  • IDS is offered on the INT with the EEV detector and 235mm camera only, but with the full range of gratings.
  • Specifications and technical details of all CCDs current at the ING are given on the ING Detectors technical page.
  • Full details of all ING filters are given in the Filter Home Page.
  • SIGNAL can be used to calculate exposure times for any telescope/instrument/detector combination.


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Last modified: 20 February 2026

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