|
par1 = | line wavelength in Angstrom |
par2 = | line width in km/s |
Norm = K | total photons/cm/s in the line |
For zvagauss the corresponding formula is:
and the parameters are:
par1 = | line wavelength in Angstrom |
par2 = | line width in km/s |
par3 = z | redshift |
Norm = K | total photons/cm/s in the line |
The line is truncated at the point that the integrated flux under the line is within a critical value of the total flux. This critical value can be changed using xset LINECRITLEVEL. The default critical value is .
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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.