IOC-MIPS_120a |
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10190C,10590C |
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Title: |
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Calibration of MIPS Stimulators Against Celestial Sources at 24um |
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Objective: |
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Measure the output of the MIPS stimulators against the output of known stars. |
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This template tests the stimulator response at 24um. Longer wavelengths done separately. |
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Description: |
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Photometry mode data on a standard star will be collected interspersed with stim flashes |
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recorded using a 24um stim flash IER. |
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including flow / state diagram |
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Stimulator calibration at 24um. |
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1) Observe the star using photometry mode with 3 second integrations and small field dither. |
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2) Observe the stimulator. |
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3) Repeat 1 and 2 five times. |
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Place in Schedule: |
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After aperture door is opened. |
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(relative to water shed events) |
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Required Conditions: |
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MIPS detector aliveness tests must have been performed. |
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MIPS aperture position must be known well enough to place a star in the FOV. |
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Backgrounds must be less than the equivalent of 300,000 photons/sec: |
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24um test at |
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3.6E-05 |
W/m^2/sr |
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or T<43K |
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These values are predicated on the 24um flood illuminator providing 250,000 photons/s at FPA |
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Resources: |
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duration (best estimate) |
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30 min |
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real time downlink (Y / N) |
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no |
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special post event actions (Y / N) |
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no |
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Part 1=16DCEs |
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Part 2=3DCEs |
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Total=5x(16+3)=95DCEs |
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Outcome: |
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description |
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The conversion factor between instrument units and physical units will |
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be available for stimulator observations. |
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can proceed in parallel with other activity |
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no, requires dedicated pointing. |
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must outcome be confirmed before next event / test /activity |
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no |
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method of confirmation (sensor TLM, data analysis, etc.) |
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data analysis |
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estimate of data turn around if required for confirmation |
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N/A |
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Unique or included in planned AOT? |
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Uses photometry AOT and IER for stimulator flashes. |
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Contingency Plan: |
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"What if..." |
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If the test fails, it must be repeated |
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IOC Critical |
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Y |
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References: |
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Template last updated: |
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9/6/99 |
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M.Rieke |
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