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OST ppm noise floor #30

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rodluger opened this issue Jul 13, 2017 · 2 comments
Closed

OST ppm noise floor #30

rodluger opened this issue Jul 13, 2017 · 2 comments
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@rodluger
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I want to tie in our OST discussion with Figure 14. I argue that if orbital parameters are well known, distinguishing between an airless and a thick atmosphere c requires the sensitivity to a ~80 ppm signal. If the orbital parameters are unconstrained, the signal we're looking for is the asymmetry of the light curve, which is ~10 ppm. Jake, can you calculate what the sensitivity of OST is at 50 microns? I imagine this is just the size of the error bars in ppm, right? That would be the "noise floor" for a 1-sigma detection. We should then calculate how many exposures we would need to stack to get down to 10 ppm. Can you do this?

@jlustigy
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jlustigy commented Jul 14, 2017 via email

@jlustigy
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jlustigy commented Jul 16, 2017 via email

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