model

jaxon.model.model(n_temps, phase, time, y, yerr, eclipse_numpy, filt_wavelength, filt_trans, a_rs, a_rp, T_s, rprs, mstar, mass, period, rstar, nus=DeviceArray([1818.18181818, 1944.85110876, 2080.34520939, 2225.27892789, 2380.30990462, 2546.14159646, 2723.52646881, 2913.26940993, 3116.23138311, 3333.33333333, 6060.60606061, 6327.21029671, 6605.54237289, 6896.11819332, 7199.47635661, 7516.17915418, 7846.81361247, 8191.99258105, 8552.35586855, 8928.57142857, 10309.27835052, 11552.98203449, 12946.72520725, 14508.60852131, 16258.91627843, 18220.3798635, 20418.47295879, 22881.74237266, 25642.17877926, 28735.63218391], dtype=float64), wav=DeviceArray([348., 389.98246156, 437.0296561, 489.75258925, 548.83597789, 615.04714267, 689.2459732, 772.39609553, 865.57738687, 970., 1120., 1169.26846283, 1220.70423051, 1274.40264213, 1330.4632307, 1388.98990769, 1450.09115559, 1513.88022898, 1580.47536451, 1650., 3000., 3209.00432946, 3432.56959549, 3671.71023102, 3927.51134262, 4201.13363415, 4493.81867354, 4806.89452639, 5141.78178214, 5500.], dtype=float64), Parr=DeviceArray([1.00000000e-05, 1.42252931e-05, 2.02358965e-05, 2.87861559e-05, 4.09491506e-05, 5.82513671e-05, 8.28642773e-05, 1.17876863e-04, 1.67683294e-04, 2.38534401e-04, 3.39322177e-04, 4.82695744e-04, 6.86648845e-04, 9.76778110e-04, 1.38949549e-03, 1.97659807e-03, 2.81176870e-03, 3.99982340e-03, 5.68986603e-03, 8.09400122e-03, 1.15139540e-02, 1.63789371e-02, 2.32995181e-02, 3.31442475e-02, 4.71486636e-02, 6.70703561e-02, 9.54095476e-02, 1.35722878e-01, 1.93069773e-01, 2.74647411e-01, 3.90693994e-01, 5.55773659e-01, 7.90604321e-01, 1.12465782e+00, 1.59985872e+00, 2.27584593e+00, 3.23745754e+00, 4.60537826e+00, 6.55128557e+00, 9.31939576e+00, 1.32571137e+01, 1.88586328e+01, 2.68269580e+01, 3.81621341e+01, 5.42867544e+01, 7.72244995e+01, 1.09854114e+02, 1.56270698e+02, 2.22299648e+02, 3.16227766e+02], dtype=float64), dParr=DeviceArray([2.97026788e-06, 4.22529313e-06, 6.01060334e-06, 8.55025945e-06, 1.21629947e-05, 1.73022165e-05, 2.46129102e-05, 3.50125862e-05, 4.98064302e-05, 7.08511070e-05, 1.00787777e-04, 1.43373567e-04, 2.03953101e-04, 2.90129265e-04, 4.12717384e-04, 5.87102577e-04, 8.35170626e-04, 1.18805470e-03, 1.69004263e-03, 2.40413519e-03, 3.41995278e-03, 4.86498308e-03, 6.92058104e-03, 9.84472939e-03, 1.40044161e-02, 1.99216925e-02, 2.83391915e-02, 4.03133307e-02, 5.73468946e-02, 8.15776386e-02, 1.16046582e-01, 1.65079665e-01, 2.34830662e-01, 3.34053501e-01, 4.75200897e-01, 6.75987206e-01, 9.61611617e-01, 1.36792071e+00, 1.94590731e+00, 2.76811019e+00, 3.93771789e+00, 5.60151913e+00, 7.96832517e+00, 1.13351761e+01, 1.61246203e+01, 2.29377451e+01, 3.26296147e+01, 4.64165835e+01, 6.60289506e+01, 9.39281178e+01], dtype=float64), stellar_spectrum=array([3.94835270e-05, 8.37888264e-05, 1.04370654e-04, 1.20768349e-04, 1.30886013e-04, 1.39983365e-04, 1.44604439e-04, 1.45003233e-04, 1.41159012e-04, 1.38223319e-04, 1.30975061e-04, 1.31039635e-04, 1.28658677e-04, 1.25976784e-04, 1.23719116e-04, 1.20262273e-04, 1.13975015e-04, 1.14419132e-04, 1.11605388e-04, 1.07100378e-04, 3.91213347e-05, 3.47755868e-05, 3.08216410e-05, 2.72207739e-05, 2.40589281e-05, 2.06023406e-05, 1.87621349e-05, 1.65296140e-05, 1.45468362e-05, 1.28310704e-05]), res=68.41495182127963, predict=False)[source]

The full joint model passed to numpyro.

Parameters

  • n_temps (int) – Number of temperatures in the T-P profile

  • phase (numpy.ndarray) – Phase of the planetary orbit

  • time (numpy.ndarray) – Time in BJD

  • y (numpy.ndarray) – Normalized flux in ppm

  • yerr (numpy.ndarray) – Normalized flux error in ppm

  • eclipse_numpy (numpy.ndarray) – Normalized eclipse vector

  • filt_wavelength (numpy.ndarray) – Filter transmittance wavelength array

  • filt_trans (numpy.ndarray) – Filter transmittance array

  • a_rs (float) – Semimajor axis normalized by stellar radius

  • a_rp (float) – Semimajor axis normalized by the planetary radius

  • T_s (float) – Stellar effective temperature

  • rprs (float) – Radius ratio

  • mstar (float) – Stellar mass in solar masses

  • mass (float) – Planet mass in Jupiter masses

  • period (float) – Orbital period [d]

  • rstar (float) – Stellar radius in solar radii

  • nus (numpy.ndarray) – Frequencies sampled in the spectrum

  • wav (numpy.ndarray) – Wavelengths sampled in the spectrum

  • Parr (numpy.ndarray) – Pressure array at each temperature in the T-P profile

  • dParr (numpy.ndarray) – Delta pressure array at each temperature in the T-P profile

  • stellar_spectrum_vis (numpy.ndarray) – Spectrum of the star

  • res (float) – Spectral resolution

  • predict (bool) – Turn on or off the gaussian process predict features