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STUDY SUMMARY - IPMU

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<strong>SUMMARY</strong> REPORT<br />

WIDE FIELD FIBER-FED OPTICAL<br />

MULTI-OBJECT SPECTROMETER (WFMOS)<br />

Figure 3.14-1: Control Hierarchy<br />

Science<br />

Subaru Telescope<br />

PHSC<br />

Guide Stars<br />

Subaru TCS<br />

PHSC hexapod<br />

Instrument rotator<br />

Calibration<br />

lamps<br />

STARS Archive<br />

SOSS<br />

WFMOS Control System<br />

Observer<br />

Light:<br />

Science<br />

Guide<br />

Calibration<br />

Control<br />

signals<br />

Data<br />

WFMOS Data<br />

Handling and<br />

Pipeline System<br />

WFC + ADC<br />

Autoguider<br />

Metrology Detector<br />

Positioner<br />

Fibres<br />

Fiducial<br />

lamps<br />

Slit block 1<br />

Slit block 2<br />

Slit block 3<br />

Positioner lamp 1<br />

Positioner lamp 2<br />

Positioner lamp 3<br />

Spectrograph 1<br />

Spectrograph 2<br />

Spectrograph 3<br />

Science Detector 1<br />

Science Detector 2<br />

Science Detector 3<br />

Figure 3.14-2: Block Diagram. Subaru infrastructure is shown in green, Subaru-supplied<br />

components are shown in cyan, and WFMOS-supplied components are shown in yellow.<br />

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