{% extends "base.html" %} {% block content %}
{{ js|indent(4)|safe }} {{ css|indent(4)|safe }} {{ script|safe }} {{ filt_script|safe }}The Limb Darkening calculates limb-darkening coefficients for a specified stellar model, plotting results versus intensity ratio and wavelength. It uses high spectral resolution stellar atmospheric models, which are a neccesisty given JWST's expected precision.
Teff | {{ form.teff.data }} |
log(g) | {{ form.logg.data }} |
Fe/H | {{ form.feh.data }} |
Bandpass | {{ form.bandpass.data }} |
Profiles |
{% for prof in form.profiles.data %}
{{ prof }} {% endfor %} |
Models | {{ form.modeldir.data }} |
Transit Duration | {{ form.transit_duration.data }} |
Orbital Period | {{ form.orbital_period.data }} |
Rp/R* | {{ form.rp_rs.data }} |
a/R* | {{ form.a_rs.data }} |
Inclination | {{ form.inclination.data }} |
Eccentricity | {{ form.eccentricity.data }} |
\( \omega \) | {{ form.omega.data }} |