In each flux file (except for the flux_reference_spectrum):
col.3=wavelength in nm
col.4=frequency nu (s^-1)
col.5=Hnu (erg/cm^2/s/Hz/ster)
col.6=Hcont (erg/cm^2/s/Hz/ster)
col.7=Hnu/Hcont
Hnu is Eddington flux
Flambda=4*Hnu*c/wavelength^2 c=light velocity
SOLAR ABUNDANCES FROM Asplund, Grevesse & Sauval, 2005, ASP Conference Series, Vol. XXX
-----------------------------------------------------------------------------------------
ap00t5777g44377k1asp.asc-ATLAS9 solar model (new ODFs, nover)
fp00t5777g44377k1asp.asc-ATLAS9 solar flux (new ODFs, nover)
ap00t5615g4534k1asp.asc-ATLAS9 solar model for the young Sun (new ODFs, nover)
fp00t5615g4534k1asp.asc-ATLAS9 solar flux for the young Sun (new ODFs, nover)
ap00t5680g4546k1asp.asc-ATLAS9 solar model for the young Sun (new ODFs, nover)
fp00t5680g4546k1asp.asc-ATLAS9 solar flux for the young Sun (new ODFs, nover)
SOLAR ABUNDANCES FROM Grevesse & Sauval, 1998, Space Sci. Rev., 85, 161
-------------------------------------------------------------------------
a) NEW ODF's
asunodfnew.dat-ATLAS9 solar model (new ODFs, nover)
fsunodfnew.dat-ATLAS9 solar flux from ASUNODFNEW.DAT
b) OLD ODF's
asunnover.dat-ATLAS9 solar model with old ODFs and no-overshooting
fsunnover.dat-ATLAS9 solar flux from ASUNNOVER.DAT
c) Holweger-Muller model in ATLAS9 format, meteoritic abundances (Cowley& Castelli, 2002, A&A 387, 595),
hm50meteorat9.dat
Solar reference spectrum (Colina, Bohlin, Castelli, AJ 112, 307 (1996)
----------------------------------------------------------------------
sun_reference_spectrum.asc-