|
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 vcheb6 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 bcheb6 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 only) |
par11 | Switch (0 = calculate using mekal model, 1 = interpolate using mekal model, 2 = use AtomDB data, 3 = use SPEX data). |
norm | Normalization |
For bvcheb6 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 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