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# Spectrum Analysis

The differential flux

per area, time and energy interval is defined asOften

is also referred to as as observation time and effective collection area is a constant. The effective area is then defined as . Note that at large distances the efficiency vanishes, so that the effective area is an (energy dependent) constant while and the efficiency are mutually dependent.For an observation with an effective observation time

, this yields in a given Energy interval :For simplicity, in the following,

will be replaced by just but always refers to to a given energy interval.The total area

and the corresponding efficiency are of course only available for simulated data. For simulated data, is the production area and the corresponding energy dependent efficiency of the analysis chain. For a given energy bin, the efficiency is then defined as

where

is the number of simulated events in this energy bin and the number of *excess* events that are produced by the analysis chain.Note that the exact calculation of the efficiency

depends on prior knowledge of the correct source spectrum . Therefore, it is strictly speaking only correct if the simulated spectrum and the real spectrum are identical. As the real spectrum is unknown, special care has to be taken of the systematic introduced by the assumption of .### Excess

The number of excess events, for data and simulations, is defined as

where

is the number of events identified as potential gammas from the source direction ('on-source') and the number of gamma-like events measured 'off-source'. Note that for Simulations, is not necessarily zero for wobble-mode observations as an event can survive the analysis for on- and off-events, if this is not protected by the analysis chain.The average number of background events

is the total number of background events from all off-regions times the corresponding weight . For five off-regions, this yields

### Theta and Spectral Weights

While the source spectrum

is of course independent of the zenith angle of the observation, the efficiency is not, so that

In addition, the observed differential flux depends on the zenith angle, so that

That means that for a correct calculation of the efficiency, the number of simulated events per zenith angle interval has to match the observation time distribution. This can be achieved by applying zenith angle dependent weights

to each simulated event. Similarly, the discussed requirement of the match between result spectrum and simulated spectrum can be achieved applying energy dependent weights .As the simulated energy spectrum is independent of zenith angle, it can be expressed as

with the differential energy spectrum

and the zenith angle distribution , for the total production range to and to

and

the total number of generated Monte Carlo events. For the generated number of events in the energy interval and zenith angle interval this is

with the weights chosen such that the sum over all intervals

## 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)

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