sunbather.RT

Functions

FinFout(sim, wavsAA, species[, numrays, ...])	Calculates a transit spectrum in units of in-transit flux / out-of-transit flux (i.e., Fin/Fout).
FinFout2RpRs(FinFout)	Converts the Fin/Fout (i.e., flux in-transit / flux out-of-transit) to Rp/Rs (i.e., the apparent size of the planet relative to the star).
RpRs2FinFout(RpRs)	Converts the Fin/Fout (i.e., flux in-transit / flux out-of-transit) to Rp/Rs (i.e., the apparent size of the planet relative to the star).
air2vac(wavs_air)	Converts air wavelengths to vacuum.
avg_limbdark_quad(ab)	Average of the quadratic limb darkening I(mu) over the stellar disk.
calc_cum_tau(x, ndens, Te, vx, nu, nu0, m, ...)	Calculates cumulative optical depth using Eq.
calc_tau(x, ndens, Te, vx, nu, nu0, m, sig0, ...)	Calculates optical depth using Eq.
constantR_wavs(wav_lower, wav_upper, R)	Returns an array of wavelengths at a constant spectral resolution.
convolve_spectrum_R(wavs, flux, R[, verbose])	Convolves a spectrum with a Gaussian filter down to a lower spectral resolution.
limbdark_quad(mu, ab)	Quadratic limb darkening law from Claret & Bloemen (2011).
project_1D_to_2D(r1, q1, Rp[, numb, ...])	Projects a 1D sub-stellar solution onto a 2D grid.
read_NIST_lines(species[, wavlower, wavupper])	Reads a tabular file of spectral line coefficients from the NIST database.
tau_12D(sim, wavAA, species[, width_fac, ...])	Maps out the optical depth at one specific wavelength.
tau_1D(sim, wavAA, species[, width_fac, v_turb])	Maps out the optical depth at one specific wavelength.
tau_to_FinFout(b_edges, tau, Rs[, bp, ab, ...])	Takes in optical depth values and calculates the Fin/Fout transit spectrum, using the stellar radius and optional limb darkening and transit phase parameters.
vac2air(wavs_vac)	Converts vacuum wavelengths to air.