You signed in with another tab or window. Reload to refresh your session.You signed out in another tab or window. Reload to refresh your session.You switched accounts on another tab or window. Reload to refresh your session.Dismiss alert
In the bottom of docs/stardis.bib, in the "Opacity Data" section, there are several papers that contain data for cross-sections, gaunt factors, or hydrogenic bf/ff departure coefficients. The papers are also in the TARDIS Zotero in the STARDIS/Stellar Opacity Data subfolder. A few guidelines for the cross-section files (as the readers for the others haven't been built yet, see #42):
No column or row headers.
# is for comments.
If there is no temperature dependence, wavelength is the first column and cross-section is the second column.
If there is temperature dependence, wavelength is the first column and temperature is the first row. Leave the top left entry blank, though. The cross-sections then are filled in according to their wavelength and temperature.
The reader does flat extrapolation beyond the min/max wavelength/temperature, so if you want the opacity to be zero beyond a certain wavelength/temperature, you need to include that in the table.
Wavelengths must be in Angstrom, temperatures in Kelvin, and cross-sections in the appropriate CGS units.
In the bottom of
docs/stardis.bib
, in the "Opacity Data" section, there are several papers that contain data for cross-sections, gaunt factors, or hydrogenic bf/ff departure coefficients. The papers are also in the TARDIS Zotero in theSTARDIS/Stellar Opacity Data
subfolder. A few guidelines for the cross-section files (as the readers for the others haven't been built yet, see #42):#
is for comments.However, see #61 as these guidelines may change.
We will want these in the refdata repo (either
tardis/refdata
or a newstardis/refdata
) eventually.The text was updated successfully, but these errors were encountered: