snr_check.py ΒΆ
Computes the SNRs on the secondary eclipses of all TRAPPIST-1 planets in the 15 micron JWST MIRI filter. This is used for benchmarking the code. The benchmarked values are
planetplanet analytic ratio b: 4.250 4.488 0.947 c: 2.752 2.950 0.933 d: 0.931 0.978 0.953 e: 0.863 0.900 0.958 f: 0.652 0.691 0.942 g: 0.502 0.539 0.931 h: 0.117 0.122 0.958
Note that the planetplanet estimates are lower than the analytic estimates by a few percent because the latter neglects thermal/background noise.