ESI Electronics Group Training
2001 May 16
Below is the outline of a presentation to the Electronics Group done on 2001 May 16.

Overview

  • Mid-resolution echelle spectrograph
  • Very low-resolution prism spectrograph
  • Imager

Science drivers

  • Echelle mode
    • kinematics of galaxies and galaxy clusters
    • QSO intervening gas studies
    • "long slit" kinematics of gaseous nebulae
    • stellar metallicities
  • Low-D mode
    • High throughput survey work: quasars, radio and X-ray sources, etc.
      (redshifts, continuum shapes, identifications)
  • Imaging mode
    • narrow-band QSO imaging
    • small field of view surveys
    • benefits from seeing < 0.5 arcsec

LRIS Similarities

  • Cassegrain instrument

  • Optical spectrograph (3900 Å - 1.1 µm, like LRIS-R)

  • Imaging mode
  • Choice of two resolutions (LRIS has many)
  • Slit masks possible, though little used
    • smaller field of view
    • not a commissioned mode
    • only 3 or 4 slots available for masks

HIRES Similarities

  • Cross-dispersed echelle (also like NIRSPEC high-resolution mode)
  • Can use slit masks

Novel features

  • "Space frame" design to isolate structure from environment and minimize flexure
  • Open-loop flexure compensation control
    • simple formula predicts image movement
    • high-precision active collimator controls compensate

Also different

  • Active servo mechanisms with "optical" (~8500 Å) encoder tapes.

  • New control interface design ("Dashboard")
    • tcl/tk
    • highly customizable, although we don't use this feature much
  • "Sealed" hatch and spectrograph body with positive air pressure to keep optics clean

Design Walkthrough

Following the light path from the telescope to the detector:

  • entrance window and cover (AIR operated)
  • triple wheel (SERVO)
    • only upper wheel in focus
    • five slots per wheel
    • holders (one per slot) can have one, two, or three filters or slit masks
    • special 9-position echelle slit mask with "dekker" in middle wheel to select active slit
  • offset mirror for guide/acquisition field

Guider path:

  • 8-position filter wheel (HIRES_style holders) (SERVO)
  • remote camera focus
  • PXL 2K x 2K CCD

Science path:

  • Collimator (SERVO)
    • Three legs with ± 25 mm travel, encoded to 5 µm
    • Focus and flexure compensation
  • Cross-dispersion prism #1 OR imaging fold mirror (AIR)
  • Fixed cross-dispersion prism (#2)
  • Echelle grating OR low-D fold mirror (AIR)
  • Camera shutter (AIR)
    • "curtain shutter" design with 3 states: left, open, and right
  • Camera lens
    • fluid-filled gaps between some elements
  • Dewar
    • ion pump
    • 2K x 4K MIT/Lincoln Labs CCD

Instrument Walkaround

  • Electronics boxes

  • hatch
  • cryo fill port
  • access panels

Electronics and Computers

  • Galil motor controllers (2); Renishaw encoder tapes

  • Leach II CCD controller
  • Ion pump controller (a la HIRES)
  • Lantronics terminal server
  • Separate CCD computer (esi5cb; UNIX)
  • Low-level interface control (koki; UNIX)
  • Instrument computer (kanaha; UNIX)

Interface demonstration

  • Startup

  • Features of GUI

    • Control
    • Detail panels
    • Low-level diagnostic panels
  • Log file
  • Configuration tool (replacement not created yet)
  • Other tools
    • xshow
    • cshow
    • testAll
    • ct

 

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