The allowed mass range is between 0.1 M and 15.0 M. Masses not in the original grids will be calculated by interpolation. To download single track of a given mass, select the grid, metallicity and select the mass from the options or just type the required mass in solar units. In case of multiple mass requests, type Mass1--Mass2, step all in solar units. For example, typing 0.9--1.4, 0.05 will produce as output 11 tracks with masses equal to 0.90, 0.95... 1.35, 1.40 M. The minimum allowed mass step is 0.0001 M

 

For reasons of computational time, the maximum number of tracks downloadable in one go is 60. If a photometric system is not selected, the HR-diagram is provided by default. Interpolation in metallicity is available for Z and [Fe/H] with the following condition:

Pre-computed tracks for available photometric systems can be downloaded after the selection of Heavy element mixture, Available grids, and metallicity. In this cases, all masses are included in the file.

The photometric systems for wich we computed bolometric corrections. Given are also the source form the response curves and reference zero-points.

Photometric systemCalibrationPassbandsZero-points
2MASS Vegamag Cohen et al. (2003) Cohen et al. (2003)
DECam ABmag CTIOa 0
Euclid (VIS + NISP) ABmag Euclid mission databaseb 0
Gaia DR1 Vegamag Jordi et al. (2010)c Jordi et al. (2010)
Gaia DR2 Vegamag Maíz-Apellániz & Weiler (2018)dMaíz-Apellániz & Weiler (2018)
Gaia EDR3 Vegamag Brown, A.G.A. et al. (Gaia Collaboration) (2020)eBrown, A.G.A. et al. (Gaia Collaboration) (2020)
GALEX ABmag NASAf 0
Hipparcos + Tycho ABmag Bessell & Murphy (2012) Bessell & Murphy (2012)
HST (WFPC2) Vegamag SYNPHOT SYNPHOT
HST (WFC3) Vegamag SYNPHOT SYNPHOT
HST (ACS) Vegamag SYNPHOT SYNPHOT
J-PLUS ABmag J-PLUS collaboration g 0
JWST (NIRCam) Vegamag JWST User Documentationh SYNPHOT
JWST (NIRISS) Vegamag JWST User Documentation h SYNPHOT
Kepler ABmag Kepler collaborationi 0
PanSTARSS1 ABmag Tonry et al. (2012) 0
SAGE ABmag SAGE collaboration 0
Skymapper ABmag Bessell (2011) 0
Sloan ABmag Doi et al. (2010)Dotter et al. (2008)
Spitzer (IRAC) Vegamag NASAj Groenewegen (2006)
Strömgren Vegamag Maíz-Apellániz (2006) Maíz-Apellániz (2006)
Subaru (HSC) ABmag HSC collaborationk 0
SWIFT (UVOT) Vegamag NASAl Poole et al. (2008)
TESS ABmag NASAm 0
UBVRIJHKLM Vegamag Bessell & Brett (1988); Bessell (1990) Bessell et al. (1998)
UVIT (FUV+NUV+VIS) ABmag UVIT collaboration n Tandon et al. (2017)
Vera C. Rubin ObservatoryABmag LSST collaboration o 0
VISTA Vegamag ESOp Rubele et al. (2012)
WFIRST (WFI) Vegamag WFIRST reference information q SYNPHOT
WISE Vegamag WISE collaborationr Wright et al. (2010)
  • [a] ctio.noao.edu
  • [b] euclid.esac.esa.int
  • [c] The nominal G passband curve has been corrected following the post-DR1 correction provided by Maiz-Apellaniz17
  • [d] Two different GBP passbands are provided for sources brighter and fainter than G=10.87, respectively.
  • [e]EDR3
  • [f]Galex
  • [g] www.j-plus.es
  • [h] jwst-docs.stsci.edu
  • [i] keplergo.arc.nasa.gov
  • [j] irsa.ipac.caltech.edu
  • [k] hsc-release.mtk.nao.ac.jp
  • [l] heasarc.gsfc.nasa.gov
  • [m] heasarc.gsfc.nasa.gov
  • [n] uvit.iiap.res.in
  • [o] github.com/lsst
  • [p] www.eso.org
  • [q] wfirst.gsfc.nasa.gov
  • [r] wise2.ipac.caltech.edu