|
par1–6 | Chebyshev polynomial coefficients |
par7 | H density (cm) |
par8 | abundance wrt to Solar |
par9 | Redshift |
par10 | Switch (0 = calculate using mekal model, 1 = interpolate using mekal model, 2 = use AtomDB data, 3 = use SPEX data). |
norm | Normalization |
For vexpcheb6 the parameters are:
par1–6 | Chebyshev polynomial coefficients |
par7 | H density (cm) |
par8–21 | Abundances of He, C, N, O, Ne, Na, Mg, Al, Si, S, Ar, Ca, Fe, Ni wrt Solar (defined by the abund command) |
par22 | Redshift |
par23 | Switch (0 = calculate using mekal model, 1 = interpolate using mekal model, 2 = use AtomDB data, 3 = use SPEX data). |
norm | Normalization |
For bexpcheb6 the parameters are:
par1–6 | Chebyshev polynomial coefficients |
par7 | H density (cm) |
par8 | abundance wrt to Solar |
par9 | Redshift |
par10 | Gaussian sigma for velocity broadening (km/s) (switch=2 or 3 only) |
par11 | Switch (0 = calculate using mekal model, 1 = interpolate using mekal model, 2 = use AtomDB data, 3 = use SPEX data). |
norm | Normalization |
For bvexpcheb6 the parameters are:
par1–6 | Chebyshev polynomial coefficients |
par7 | H density (cm) |
par8–21 | Abundances of He, C, N, O, Ne, Na, Mg, Al, Si, S, Ar, Ca, Fe, Ni wrt Solar (defined by the abund command) |
par22 | Redshift |
par23 | Gaussian sigma for velocity broadening (km/s) (switch=2 or 3 only) |
par24 | Switch (0 = calculate using mekal model, 1 = interpolate using mekal model, 2 = use AtomDB data, 3 = use SPEX data). |
norm | Normalization |
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Last modified: Friday, 23-Aug-2024 13:20:40 EDT
HEASARC Staff Scientist Position - Applications are now being accepted for a Staff Scientist with significant experience and interest in the technical aspects of astrophysics research, to work in the High Energy Astrophysics Science Archive Research Center (HEASARC) at NASA Goddard Space Flight Center (GSFC) in Greenbelt, MD. Refer to the AAS Job register for full details.