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OSEM LED Selection Measurements: Intensity Noise and Angular Distribution

OSEM LED Selection Measurements: Intensity Noise and Angular Distribution. NAOJ VIS Meeting, April 29 nd , 2014. Results from OSEMs last November (1/2). LIGO papers have shown that OP232 LED intensity noise varies from batch to batch. Results from OSEMs last November (1/2).

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OSEM LED Selection Measurements: Intensity Noise and Angular Distribution

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  1. OSEM LED Selection Measurements:Intensity Noise and Angular Distribution NAOJ VIS Meeting, April 29nd, 2014

  2. Results from OSEMs last November (1/2) LIGO papers have shown that OP232 LED intensity noise varies from batch to batch

  3. Results from OSEMs last November (1/2) In addition, LIGO papers show different angular distribution and peak locations for different LEDs

  4. Measurement set-up Determined with the first (!) fully assembled OSEM what current to run the LED, now with collimator, to have -12V on UTIA output: Rs,LED = 300W ULED = 8V ILED ≈ 25mA For fast comparative measurement, LED is runin a simple set-up at 25 mA and ASD on theUTIA signal is taken First, a dependence of intensity noise on theLED intensity magnitude is investigated

  5. Intensity noise LED current dependence

  6. Intensity noise first batch of LEDs

  7. Comparison between batches

  8. Measurement set-up Lens (f = 8mm) LED CCD Camera OSEM optics Replace for trans-lation stage

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