= Spectrum Analysis =

The differential flux \(\phi(E)\) per area, time and energy interval is defined as
\[\phi(E) = \frac{dN}{dA\cdot dt\cdot dE}\]

Often \(\phi(E)\) is also referred to as \(\frac{dN}{dE}\) as observation time and effective collection area is a constant. The effective Area is then defined as \(A_\textrm{eff}(E)=\epsilon(E)\cdot A_0\). Note that at large distances the efficiency vanishes, so that the effective area is an (energy dependent) constant while \(A_0\) and the efficiency \(\epsilon(E)\) are mutually dependent.

For an observation with an effective observation time (\\Delta T\), this yields:
\[\phi(E) = \frac{1}{A_0\cdot \Delta T}\frac{dN}{d\epsilon(E)\cdot dE}\]



== Define Binnings ==

== Get Data File List ==

== Get Observation Time ==

== Get Monte Carlo File List ==

== Get Zenith Angle Histogram ==

== Analyze Data ==

== Analyze Monte Carlo Data ==

== Summarize Corsika Production ==

== Result (Spectrum) ==

== Result (Threshold) ==

== Result (Migration) ==