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ING Instrumentation Options


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; 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/Contacts Wavelength Range (Å) Dispersion (Å/pixel) Slit Length Detector Comments
4.2-m William Herschel Telescope
Manager: Benn
     
ISIS
Specialist: Hrudkova / Skillen
3000-10000Å 0.26-1.81 (Red+)
0.11-1.63 (EEV12)
4' Red: Red+
Blue: EEV12
Blue or Red: Qucam2, Qucam3
Long-slit spectroscopy, spectro and imaging polarimetry, and fast spectroscopy
LIRIS (§)
Specialist: Karjalainen / Domínguez
9000-24000Å R=1000-3000 4.2' HgCdTe(1024x1024) Long-slit and multi-object spectroscopy, and spectro and imaging polarimetry
ACAM (§)
Specialist: Benn / Domínguez  
3500-9400Å R~400 6' AUXCAM Long-slit spectroscopy
AUTOFIB2/WYFFOS
Specialist: Skillen / Dominguez
3500-10000Å R=100-3000 (ref.)
R=9500 (ech.)
1.6" fibres 2EEV Up to 150 objects
NAOMI/OASIS
Specialist: Benn / Skillen
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
Manager: Karjalainen
     
IDS (§)
Specialist: Vaduvescu / Benn
3000-10000Å 0.24-3.67 3.3' EEV10
Red+2
Long-slit spectroscopy with 235mm camera


Imaging
Instrument/Contacts Detector Filters Scale ("/pixel) Field-of-View
4.2-m William Herschel Telescope
Manager: Benn
       
Prime Focus Camera
Specialist: Vaduvescu / Karjalainen
2EEV see database 0.24 16'.2 x 16'.2
ACAM (§)
Specialist: Benn / Domínguez  
AUXCAM UBVRIZ + narrow-band 0.25 8'.3
NAOMI/INGRID
Specialist: Skillen / Benn
HgCdTe(1024x1024) ZJHKK_s
and 10 narrow-band
0.04 42"
NAOMI/INGRID/OSCA
Specialist: Skillen / Benn
HgCdTe(1024x1024) ZJHKK_s
and 10 narrow-band
0.04 27"
LIRIS
Specialist: Karjalainen / Domínguez
HgCdTe(1024x1024) ZJHK_s
and 8 narrow-band
0.25 4'.27
2.5-m Isaac Newton Telescope
Manager: Karjalainen
       
Wide Field Camera (§)
Specialist: Vaduvescu / Hrudková
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
Manager: Benn
   
GHaFaS IAC John Beckman
Joan Font
INTEGRAL IAC Evencio Mediavilla
PN.S Kapteyn Nigel Douglas
SAURON Lyon/Leiden/Durham SAURON Team
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 eleven weeks; 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 given here; please email queries to Raine Karjalainen (rk@ing.iac.es).
  • ACAM is permanently available except when prime focus is deployed.
  • 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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Telescope Schedules Manager
Last modified: 01 November 2011