ARIADNE uses pyphot (https://mfouesneau.github.io/pyphot/libcontent.html) as an interface for photometry, and thus we use the same filter naming convention <facility><instrument><filter>
The allowed filters are (in wavelength order):
- Galex_FUV
- Galex_NUV
- STROMGREN_u
- SkyMapper_u
- SDSS_u
- GROUND_JOHNSON_U
- SkyMapper_v
- STROMGREN_v
- TYCHO_B_MvB
- GROUND_JOHNSON_B
- STROMGREN_b
- SDSS_g
- PS1_g
- SkyMapper_g
- GaiaDR2v2_BP
- TYCHO_V_MvB
- STROMGREN_y
- GROUND_JOHNSON_V
- SkyMapper_r
- SDSS_r
- PS1_r
- PS1_w
- KEPLER_Kp
- GaiaDR2v2_G
- GROUND_COUSINS_R
- NGTS_I
- SDSS_i
- PS1_i
- SkyMapper_i
- GaiaDR2v2_RP
- GROUND_COUSINS_I
- TESS
- PS1_z
- SDSS_z
- SkyMapper_z
- PS1_y
- 2MASS_J
- 2MASS_H
- 2MASS_Ks
- WISE_RSR_W1
- WISE_RSR_W2
- WISE_RSR_W3
- WISE_RSR_W4
- HERSCHEL_PACS_BLUE
- HERSCHEL_PACS_GREEN
- HERSCHEL_PACS_RED
NOTE: WISE W3, W4 and HERSCHEL filters are ONLY available for INFRARED EXCESS VISUALIZATION and NOT for SED FITTING