The Astrophysics Science Division (ASD) at NASA's Goddard Space Flight Center (GSFC) seeks a creative, innovative individual with strong teamwork and leadership skills to serve as Director of the High Energy Astrophysics Science Archive Research Center (HEASARC). This will be a permanent civil servant position. + Learn more.
kdblur2: convolve with the laor2 model shape
A convolution model to smooth a spectrum by relativistic effects from an
accretion disk around a rotating black hole. The accretion disk has a
broken-power law emissivity profile. Uses Ari Laor's calculation
including GR effects (Laor 1991). Modified from laor2 model by
Andy Fabian and Roderick Johnstone.
Note that due to the energy binning the convolution process can
produce spurious structures around sharp features in the spectrum
being convolved. We strongly recommend testing for this by using the
energies command to change the binning.
par1 |
Index: power law dependence of emissivity (scales as ) |
par2 |
inner radius (units of ) |
par3 |
outer radius (units of ) |
par4 |
inclination (degrees) |
par5 |
radius at which emissivity power-law index changes |
par6 |
Emissivity power-law index for radii >par6 |
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Last modified: Friday, 23-Aug-2024 13:20:40 EDT
The Astrophysics Science Division (ASD) at NASA's Goddard Space Flight Center (GSFC) seeks a creative, innovative individual with strong teamwork and leadership skills to serve as Director of the High Energy Astrophysics Science Archive Research Center (HEASARC). This will be a permanent civil servant position. + Learn more.
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