Allowed filters in ARIADNE

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