I am using the following output command in the parameter file of my fits, however, I don't see an option in the manual for an output of the intrinsic/unattenuated SED. Is there a way to add this feature, as I am looking to derive the xi_ion_unatt_stellar value manually.
****
* PRINTED OUTPUT ***
****
RESULTS DIRECTORY = $BEAGLE_RESULTS/JESCO-tests/
MOCK CATALOGUE NAME =
PRINT PHOTOMETRY = T
PRINT SPECTRUM = T
PRINT SPECTRAL INDICES = T
PRINT SF AND ChE HISTORIES = T
PRINT CONTINUUM = T
Also, the manual describes the folder structure for BEAGLE as including an emission template + attenuation in the dust folder, however I seem to only have the attenuation models. Would a greybody or other radiative transfer models be accessible?
Hi Jacopo,
I am using the following output command in the parameter file of my fits, however, I don't see an option in the manual for an output of the intrinsic/unattenuated SED. Is there a way to add this feature, as I am looking to derive the xi_ion_unatt_stellar value manually.
****
* PRINTED OUTPUT ***
****
RESULTS DIRECTORY = $BEAGLE_RESULTS/JESCO-tests/
MOCK CATALOGUE NAME =
PRINT PHOTOMETRY = T PRINT SPECTRUM = T PRINT SPECTRAL INDICES = T PRINT SF AND ChE HISTORIES = T PRINT CONTINUUM = T
Also, the manual describes the folder structure for BEAGLE as including an emission template + attenuation in the dust folder, however I seem to only have the attenuation models. Would a greybody or other radiative transfer models be accessible?