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Error estimates for any single fit are given by taking the square root of the diagonal elements of the covariance matrix, which in turn is estimated as the inverse Hessian of the -log-likelihood. Note that the definition of the confidence interval corresponds to a specified change in the log-likelihood along a given direction in parameter space. The estimates obtained from the inverse Hessian are only accurate insofar as the likelihood surface at the local minimum can be accurately represented as a quadratic function of the model parameters. The error estimates reported below are averaged over each set of Monte Carlo trials.

Binned Analysis

Counts maps for the Crab_Pulsar, the three anticenter sources, and extragalactic diffuse tests are prepared for the following geometry:
E min = 30, E max = 3e5 MeV, 39 bins, logrithmically spaced
RA center = 83 o, eighty 0.5 o pixels
Dec center = 22 o, eighty 0.5 o pixels

A single point source: Crab_Pulsar

Prefactor

 

 

Index

 

 

true +/- err. est.value

MC dist

true +/- err. est.

KS prob

true value

MC dist

KS probMC

27.00 +/- 1.86

27.21 +/- 1.92

4.14e-03

-2.19 +/- 0.05

-2.16 +/- 0.06

1.59e-26

Three strong sources in the Galactic anticenter region: PKS 0528+134, Crab, Geminga

Here is a FITS image of the count map, summed over energies, used in these fits.

  • PKS0528+134

    Prefactor

     

     

    Index

     

     

    true value

    MC dist

    KS prob

    true value

    MC dist

    KS prob

    true +/- err. est.

    MC

    true +/- err. est.

    MC

    13.65 +/- 1.68

    14.37 +/- 1.70

    6.31e-25

    -2.46 +/- 0.09

    -2.55 +/- 0.13

    1.87e-73

  • Crab

    Prefactor

     

     

    Index

     

     

    true +/- err. est.value

    MC dist

    KS prob

    true +/- err. est.value

    MC dist

    KS prob

    27.00 +/- 2.14

    26.74 +/- 2.19

    9.48e-03

    -2.19 +/- 0.05

    -2.15 +/- 0.07

    3.61e-52

  • Geminga

    Prefactor

     

     

    Index

     

     

    true +/- err. est.value

    MC dist

    KS prob

    true +/- err. est.value

    MC dist

    KS prob

    23.29 +/- 1.73

    23.62 +/- 1.88

    1.96e-07

    -1.66 +/- 0.02

    -1.66 +/- 0.04

    1.69e-02

Unbinned Analysis

These analyses use this ROI file.

Crab_Pulsar

Prefactor

 

 

Index

 

 

true +/- err. est.value

MC dist

KS prob

true +/- err. est.value

MC dist

KS prob

27.00 +/- 1.78

28.19 +/- 1.84

3.55e-62

-2.19 +/- 0.05

-2.22 +/- 0.05

1.39e-60

Markov Chain Monte Carlo (MCMC)

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PKS 0528+134, Crab, & Geminga

  • PKS0528p134

    Prefactor

     

     

    Index

     

     

    true +/- err. est.value

    MC dist

    KS prob

    true +/- err. est.value

    MC dist

    KS prob

    13.65 +/- 1.76

    14.62 +/- 1.75

    3.13e-40

    -2.46 +/- 0.11

    -2.52 +/- 0.11

    5.13e-40

  • Crab

    Prefactor

     

     

    Index

     

     

    true valuetrue +/- err. est.

    MC dist

    true +/- err. est.

    KS prob

    true value

    MC dist

    KS probMC

    27.00 +/- 2.02

    28.10 +/- 2.03

    7.68e-42

    -2.19 +/- 0.05

    -2.22 +/- 0.06

    1.63e-42

  • Geminga

    Prefactor

     

     

    Index

     

     

    true +/- err. est.value

    MC dist

    KS prob

    true +/- err. est.value

    MC dist

    KS prob

    23.29 +/- 1.68

    24.38 +/- 1.74

    4.84e-59

    -1.66 +/- 0.03

    -1.68 +/- 0.03

    4.37e-58

MCMC results for a single trial

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Extragalactic Diffuse

The ROI file.

Prefactor

 

 

Index

 

 

true +/- err. est.value

MC dist

true +/- err. est.

KS prob

true value

MC dist

KS probMC

1.45

1.48 +/- 0.06

1.48 +/- 0.0602e-55

-2.10 +/- 0.03

-2.10 +/- 0.03

5.79e-08