Photometric system Choose among the available photometric systems:
2MASS + Spitzer (IRAC+MIPS)
2MASS + Spitzer (IRAC+MIPS) + WISE
2MASS JHK s
OGLE + 2MASS + Spitzer (IRAC+MIPS)
2MASS+Spitzer+WISE+Washington+DDO51
UBVRIJHK (cf. Maiz-Apellaniz 2006 + Bessell 1990)
UBVRIJHKLMN (cf. Bessell 1990 + Bessell & Brett 1988)
AKARI
BATC
CFHT Megacam + Wircam (all ABmags)
CFHT Wircam
CFHT/Megacam u*g'r'i'z'
CIBER
DECAM (ABmags)
DECAM ugrizY (ABmags) + VISTA ZYJHK s (Vegamags)
DENIS
DMC 14 filters
DMC 15 filters
ESO/EIS (WFI UBVRIZ + SOFI JHK )
ESO/WFI
ESO/WFI2
Euclid/NISP (ABmags)
GALEX FUV+NUV (Vegamag) + SDSS ugriz (ABmags)
GALEX FUV+NUV + Johnson's UBV (Maiz-Apellaniz version), all Vegamags
Gaia DR1 + Tycho2 + 2MASS (all Vegamags)
Gaia DR2 + Tycho2 + 2MASS (all Vegamags, Gaia passbands from Evans et al. 2018)
Gaia DR2 + Tycho2 + 2MASS (all Vegamags, Gaia passbands from Weiler 2018)
Gaia's DR1 G, G_BP and G_RP (Vegamags)
Gaia's DR2 G, G_BP and G_RP (Vegamags, Gaia passbands from Evans et al. 2018)
Gaia's DR2 G, G_BP and G_RP (Vegamags, Gaia passbands from Maiz-Apellaniz and Weiler 2018)
Gaia's DR2 G, G_BP and G_RP (Vegamags, Gaia passbands from Weiler 2018)
HST+GALEX+Swift/UVOT UV filters
HST/ACS HRC
HST/ACS WFC
HST/NICMOS AB
HST/NICMOS Vega
HST/STIS imaging mode, Vegamag
HST/WFC3 all W+LP+X filters (UVIS1+IR, final throughputs)
HST/WFC3 long-pass and extremely wide filters (UVIS1, final throughputs)
HST/WFC3 medium filters (UVIS1+IR, final throughputs)
HST/WFC3 wide filters (UVIS1+IR, final throughputs)
HST/WFPC2 (Vegamag, cf. Holtzman et al. 1995)
INT/WFC (Vegamag)
IPHAS
JWST MIRI wide filters, Vegamags
JWST NIRCam wide+verywide filters, Vegamags
JWST NIRCam wide+verywide+medium filters, Vegamags
Kepler + SDSS griz + DDO51 (in ABmags)
Kepler + SDSS griz + DDO51 (in ABmags) + 2MASS (~Vegamag)
LBT/LBC (Vegamag)
LSST (ABmags) + WFIRST proposed filters (Vegamags)
LSST ugrizY, March 2012 total filter throughputs (all ABmags)
NOAO/CTIO/MOSAIC2 (Vegamag)
OGLE-II
Pan-STARRS1
S-PLUS (Vegamags), revised on Nov. 2017
SDSS ugriz
SDSS ugriz + 2MASS JHK s
SDSS ugriz + UKIDSS ZYJHK
SWIFT/UVOT UVW2, UVM2, UVW1,u (Vegamag)
SkyMapper (ABmags)
Spitzer IRAC+MIPS
Stroemgren-Crawford
Subaru/Suprime-Cam (ABmags)
TESS + 2MASS (Vegamags)
TESS + 2MASS (Vegamags) + Kepler + SDSS griz + DDO51 (in ABmags)
UKIDSS ZYJHK (Vegamag)
UVIT (all ABmags)
VISIR
VISTA ZYJHK s (Vegamag)
VPHAS+ (ABmags)
VST/OMEGACAM (ABmag)
Vilnius
WFIRST proposed filters, Vegamags
Washington CMT1 T2 + DDO51
deltaa (Paunzen) + UBV (Maiz-Apellaniz), in Vegamags
They are briefly described here .
Warning: the following options will not work for PARSEC+COLIBRI tracks, which adopt, by default, a mix between ATLAS9 ODFNEW and Aringer et al. (2016) for O-rich stars, and an updated version of Aringer et al. (2009) for C-rich stars (see details in Marigo et al. (2017) ).
Sets of bolometric corrections to be applied to "normal stars": NBC as described on Chen et al. (2014) , based on PHOENIX BT-Settl for Teff<4000 K, and on ATLAS9 ODFNEW otherwise
Warning: This will not work for PARSEC+COLIBRI tracks (OBC will be used then).
or on OBC as described on Girardi et al. (2008) , mostly based on ATLAS9 ODFNEW models (see also Marigo et al. (2008) and Girardi et al. (2002) ) For Carbon stars, you can choose bolometric corrections based either on Loidl et al. (2001) (as in Marigo et al. (2008) and Girardi et al. (2008) ) or on Aringer et al. (2009) (updated to include new spectra from Aringer et al. (2016) )