SatAndLight
2.2.2-hubble
Simulation toolkit for space telescopes
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This program is designed to produce a source SpecTime object. More...
Functions | |
int | main (int argc, char *argv[]) |
Produce a source SpecTime object. More... | |
This program is designed to produce a source SpecTime object.
int main | ( | int | argc, |
char * | argv[] | ||
) |
Produce a source SpecTime object.
A SpecTime object captures both the light curve and the energy spectrum of an astrophysical source. It is a 2-dimensional function \({\cal{F}}(E,t)\) which measures the particle "on-axis" flux as a function of energy and time. This program generates the SpecTime object as a TH2F object saved in a ROOT file. The horizontal axis is binned in time \([\mathrm{ms}]\). The vertical axis is binned in energy \([\mathrm{keV}]\). Each bin is given the flux value in \([\mathrm{keV}^{-1}\mathrm{ms}^{-1}\mathrm{mm}^{-2}]\).
[in] | argc | Number of arguments. |
[in] | argv | List of arguments. |