-
Notifications
You must be signed in to change notification settings - Fork 1
New issue
Have a question about this project? Sign up for a free GitHub account to open an issue and contact its maintainers and the community.
By clicking “Sign up for GitHub”, you agree to our terms of service and privacy statement. We’ll occasionally send you account related emails.
Already on GitHub? Sign in to your account
OST ppm noise floor #30
Comments
For a 5 min cadence with our OST setup, I find that 11 stacked observations
reaches 10 ppm precision on the lightcurve.
[image: Inline image 1]
…On Thu, Jul 13, 2017 at 9:38 AM, Rodrigo Luger ***@***.***> wrote:
Assigned #30 <#30> to
@jlustigy <https://github.com/jlustigy>.
—
You are receiving this because you were mentioned.
Reply to this email directly, view it on GitHub
<#30 (comment)>, or mute
the thread
<https://github.com/notifications/unsubscribe-auth/AIeJIhkk3k9tqCPhBgzV9obyLlRWOSeSks5sNkf2gaJpZM4OXQFH>
.
--
Jacob Lustig-Yaeger
Astronomy & Astrobiology Graduate Student
University of Washington
jlustigy.github.io
|
Bad news: I had a bug in my custom filters where I was extrapolating them
far beyond their specified boundaries. So now we would have to observe ~500
(!) events to reach 10 ppm precision. Sorry about that!
But I also made a figure of SNR on an occultation of c by b as a function
of wavelength from ~10-80 microns, which shows a rise up to ~15-20 microns
as the contrast increases, then a decline beyond that as there are fewer
and fewer photons to detect.
[image: Inline image 1]
On Fri, Jul 14, 2017 at 3:15 PM, Jacob Lustig-Yaeger <jlustigy@uw.edu>
wrote:
… For a 5 min cadence with our OST setup, I find that 11 stacked
observations reaches 10 ppm precision on the lightcurve.
[image: Inline image 1]
On Thu, Jul 13, 2017 at 9:38 AM, Rodrigo Luger ***@***.***>
wrote:
> Assigned #30 <#30> to
> @jlustigy <https://github.com/jlustigy>.
>
> —
> You are receiving this because you were mentioned.
> Reply to this email directly, view it on GitHub
> <#30 (comment)>,
> or mute the thread
> <https://github.com/notifications/unsubscribe-auth/AIeJIhkk3k9tqCPhBgzV9obyLlRWOSeSks5sNkf2gaJpZM4OXQFH>
> .
>
--
Jacob Lustig-Yaeger
Astronomy & Astrobiology Graduate Student
University of Washington
jlustigy.github.io
--
Jacob Lustig-Yaeger
Astronomy & Astrobiology Graduate Student
University of Washington
jlustigy.github.io
|
Sign up for free
to join this conversation on GitHub.
Already have an account?
Sign in to comment
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?
The text was updated successfully, but these errors were encountered: