Astronomy 920 Commissioning of the Prime Focus Imaging Spectrograph - PowerPoint PPT Presentation

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Astronomy 920 Commissioning of the Prime Focus Imaging Spectrograph

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Commissioning of the Prime Focus Imaging Spectrograph. Meeting 2. Intro; VPH Grating Spectroscopy ... Why Large Telescope Spectrographs are Big. VPH Gratings ... – PowerPoint PPT presentation

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Title: Astronomy 920 Commissioning of the Prime Focus Imaging Spectrograph


1
Astronomy 920Commissioning of the Prime Focus
Imaging Spectrograph
  • Meeting 2
  • Intro VPH Grating Spectroscopy
  • Ken Nordsieck

2
Optics Layout
3
VPH Gratings
4
Throughput
5
NIR Upgrade Path
  • NIR upgrade path preserved by collimator allowing
    full 320 nm 1.7 µ wavelength range support
    structure

6
Assembly and Integration
7
Slitmask Cutter
  • Commercial laser
  • MOS custom slits cut in carbon-fiber
  • Longslit stainless steel, tilted and polished
    for viewing by SALTICAM/ slitviewer optics
  • PI planning tool produces slitmask file for
    inclusion in proposal

8
Grating Optics
  • Grating Equation
  • Resolution
  • Why Large Telescope Spectrographs are Big
  • VPH Gratings

9
Grating Equation and Resolution
  • m ? / ? sin a sin ß 2 sin a (Littrow)
  • d? / dß (?/m) cos ß
  • angular size of monochromatic slit
  • ?a ?? Dtel / Dcol
  • ?ß ?a cos a / cos ß
  • ?? (slit) (?/m) cos a ?? Dtel / Dcol
  • at Littrow
  • R ?/?? (slit) 2 (Dcol / Dtel) tan a / ??

Dtel dia of primary Dcol dia of collimated
beam ? spacing of grating grooves ? angle in
sky a angle of incidence ß angle of
diffraction m order of diffraction
10
Resolution
  • R ?/?? (slit) 2 (Dcol / Dtel) tan a / ??
  • Does not depend on
  • diffraction order (!)
  • grating groove density (!)
  • For fixed seeing, improve only by
  • going to higher grating angle (eg Echelle)
  • increasing the size of your collimated beam ()
  • Note for small telescopes, also worry about
    grating diffraction limit Rdif Dgrat /?
  • For SALT/ PFIS Dcol 150 mm, Dtel / Dcol
    73.3
  • R 5640 for 1 arcsec slit, 45 deg grating angle

11
VPH Gratings
  • Created by exposing holograph material (DCG) to
    interference pattern from laser
  • Index of refraction of DCG is modulated in space
  • Large inexpensive custom design efficient at
    high groove density

12
PFIS VPH
  • 1300 gr/ mm VPH (? 769 nm)

13
Tunable Blaze
  • Peak efficiency is at Littrow gt Blaze angle
    changes with a
  • If increase ß as tilt grating, can use grating at
    large range of central wavelengths gt change
    camera angle a ß
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