To find and download HEASARC data in the cloud, you can use astroquery.heasarc or download our new tool, hark.
The HEASARC and NuSTAR teams are greatly saddened by the sudden passing of Katja Pottschmidt. Most recently Katja was the lead scientist for the NuSTAR Guest Observer Facility (GOF), a role she had supported for many years. During her science career she worked on many other high energy astrophysics missions and played an integral role in advancing our knowledge of the universe. She was a wonderful colleague and friend and will be keenly missed by all who knew her.
Next: expdec: exponential decay Up: Additive Model Components Previous: equil, vequil, bequil, bvequil: Contents
expcheb6, vexpcheb6, bexpcheb6, bvexpcheb6: differential emission
measure using exponential of a 6-order Chebyshev polynomial
expcheb6 is a multi-temperature collisional-ionization equilibrium model using the exponential of a sixth-order Chebyshev polynomial for the differential emission measure. The switch parameter determines whether spectrum is calculated by running the mekal code, by interpolating on a pre-calculated mekal table, using the AtomDB data, or using the SPEX data. The final two options is now preferred. See the cie model for further information and options. The reference for this model is Singh et al. (1996, ApJ, 456, 766).
Velocity broadening can only be used with switch=2.
For expcheb6 the parameters are:
| 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 |
Next: expdec: exponential decay Up: Additive Model Components Previous: equil, vequil, bequil, bvequil: Contents