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Instrument Concepts

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GMT conceptual design review February 2006 ... Four catadioptric cameras. 4k x 6.5k to 6k x 8k CCDs (15 m pixels) UV: 299 to 389 nm ... – PowerPoint PPT presentation

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Title: Instrument Concepts


1
Instrument Concepts
Instrument Function l range (microns) Resolution FOV
GMACS Optical Multi-Object Spectrometer 0.35-1.0 250-4000 36-144 arcmin2
NIRMOS Near-IR Multi-Object Spectrometer 1.0-2.5 Up to 4000 49 arcmin2
QSpec Optical High Resolution Spectrometer 0.3-1.05 30K 1 slit 3 fibre mode
SHARPS (G-CLEF) Optical High Resolution (Doppler) Spectrometer 0.4-0.7 150K 7 x 1 fibers
GMTNIRS Near-IR High-Resolution Spectrometer 1.2- 5.0 25K-100K Single object
MIISE Mid-IR Imaging Spectrometer 3.0-25.0 1500 30
HRCam Near-IR AO Imager 0.9-5.0 5-5000 30
GMTIFS NIR AO-fed IFU 0.9-2.5 3000-5000 3
2
History
GMT instrument conceptual design studies
2005 Internal to GMT consortium (at that
time) GMT conceptual design review February
2006 Subsequent work by project, with partner
participation Integration of seeing-limited
instruments Reconfiguration of instrument
platform AO relay Meetings Seeing-limited
instruments workshop Adaptive optics workshop
Planet RV workshop Science with GMT (Canberra)
March 2008 Before proceeding, need to resolve
instrument-AO interface
3
GMT Instrument Design Studies
  • Request letters of intent (e.g. Sep 2008)
  • Select list for design studies ( 6?) (Nov
    2008)
  • Request for proposals released
  • for each instrument (Jan 2009)
  • Proposals due (Mar 2009)
  • Award contracts for design studies (May 2009)
  • Negotiate study contracts,
  • contract start (Jul 2009)
  • Finish design studies and review (Dec 2010)
  • Select first light instruments,
  • start instrument development (2011)

4
Some Issues
Intention of design studies is to form actual
instrument teams across (and beyond) partner
institutions Design study funding project
in-kind (probably not telescope time too
sensitive) Evaluation Internal hard to avoid
some conflicts External
5
(No Transcript)
6
GMACS
  • Resolving power w/ 0.7 arcsec slit
  • R 1400 in blue
  • R 2700 in red
  • (for accurate sky subtraction)
  • cross-over at 6500 Ã…
  • Separate 8 x 9 arcmin imaging
  • channel
  • Multi-object, multi-slit spectrograph
  • 4x spectrographs, each with
  • red and blue arms, VPH gratings
  • Field of view 8 x 18 arcmin
  • Wavelength range 0.36 1.02 µm
  • Collimated beam diameter 300 mm

7
GMACS Optical Layout x4
8
NIRMOS
  • Wavelength range 0.85 2.5 µm
  • Imaging Mode
  • 7 x 7 arcmin field of view
  • 0.067 arcsec/pixel
  • 6kx6k detector
  • Spectroscopy Mode
  • Multi-slits 140 x 3 arcsec long,
  • full wavelength coverage
  • 5 x 7 arcmin field of view
  • R 3000 with 0.5 arcsec slits
  • Augmented by GLAO

9
GMACS, NIRMOS MIISE
10
QSpec
  • Four beam instrument
  • 450 mm beam diameter
  • R4 echelle gratings (x2)
  • 200 x 1600 mm
  • Rf 30,000 arcsecs
  • ?? 300 nm to 1.07 µm
  • (in four channels)
  • 2-pix resolution R125,000
  • Pupil anamorphism
  • White pupil design
  • VPH grating cross-dispersion
  • Four catadioptric cameras
  • 4k x 6.5k to 6k x 8k CCDs
  • (15 µm pixels)

11
SHARPS
  • Planet Doppler spectroscopy
  • Fiber-fed 7x(obj,sky,cal) x 1.0 ?
  • Resolving power 150,000
  • Wavelength gt 4400 6700 Ã…
  • White pupil spectrograph design
  • CCD mosaic detector
  • Deep depletion CCDs for red orders
  • Vacuum-enclosed spectrograph
  • High-stability thermal environment
  • Bulky enclosure

12
MIISE Mid-IR Imaging Spectrometer
  • Wavelength range 3 - 25 µm
  • Field of view 30 40 arcsec
  • Resolving power R 1500
  • Modes
  • Imaging
  • Spectroscopy
  • Nulling (8-25 µm)
  • Coronography (3-5 µm)
  • Short wavelength channel 3-5µ,
  • 0.010 arcsec/pixel
  • Long wavelength channel 8-25µ,
  • 0.030 arcsec/pixel

3-5 µm detector
8-25 µm detector
input from AO feed
dichroic
nulling channel
2 micron phase sensor
long wavelength imaging channel
13
GMTIFS GMT Integral Field Spectrograph
  • Single-object, AO-corrected, integral-field
    spectroscopy
  • Wavelength range 1.0 2.5 µm
  • Resolving power 4000 5000
  • Range of spatial sampling and fields of view
  • Galaxy dynamics 0.05-0.10 arcsec sampling, 2-3
    arcsec FOV
  • Black hole masses Diffraction-limited sampling,
    small FOV

Spaxel size along slit (arcsec) 0.008 0.016 0.032 0.054
Slitlet width (arcsec) 0.020 0.040 0.080 0.135
Field of view (arcsec) 0.80 1.6 3.2 5.4
F-converter
Tel focus
slicer
fold
collimator
detector
grating
camera
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