Supported instrument modes
Here we list each of the available instrument modes.
Spectroscopic
Hubble STIS gratings : ‘HST_STIS_G430L’, ‘HST_STIS_G750L’Hubble WFC3 grisms : ‘HST_WFC3_G280p1’, ‘HST_WFC3_G280n1’, ‘HST_WFC3_G102’,‘HST_WFC3_G141’JWST NIRSpec : ‘JWST_NIRSpec_Prism’, ‘JWST_NIRSpec_G395H’, ‘JWST_NIRSpec_G395M’,‘JWST_NIRSpec_G235H’, ‘JWST_NIRSpec_G235M’, ‘JWST_NIRSpec_G140H’,‘JWST_NIRSpec_G140M-f100’, ‘JWST_NIRSpec_G140H-f070’, ‘JWST_NIRSpec_G140M-f070’JWST NIRISS : ‘JWST_NIRISS_SOSSo1’, ‘JWST_NIRISS_SOSSo2’JWST NIRCam : ‘JWST_NIRCam_F322W2’, ‘JWST_NIRCam_F444’JWST MIRI : ‘JWST_MIRI_LRS’
Note for the WFC3 G280 grism the p1 and n1 signify the positive 1st order spectrum and negative 1st order spectrum for the UVIS grism.

Photometric
Spitzer IRAC : ‘Spitzer_IRAC_Ch1’, ‘Spitzer_IRAC_Ch2’TESS : ‘TESS’
Note for Spitzer Ch1 is the 3.6 micron channel and Ch2 is the 4.5 microns channel.

Custom
Custom profile : ‘custom’
See the custom throughput tutorial.