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Investigations of Faraday Rotation Maps of Extended Radio Sources ...

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82 CHAPTER 4. PACMAN – A NEW RM MAP MAKING ALGORITHM<br />

where ⃗ ∇RM(⃗x) and ⃗ ∇ϕ 0 (⃗x) are the gradients <strong>of</strong> RM and ϕ 0 . A map pair, which was<br />

constructed from a set <strong>of</strong> independent random polarisation angle maps ϕ(k), will give<br />

a V ≥ −1. A map pair without any correlated noise will give a V ≈ 0. Hence, the<br />

statistic V is suitable to detect especially correlated small scale pixel noise.<br />

The denominator in Eq. (4.9) is the normalisation and enables the comparison <strong>of</strong> V<br />

for RM maps <strong>of</strong> different sources, since V is proportional to the fraction <strong>of</strong> gradients<br />

which are artefacts. Since, the comparision <strong>of</strong> the quality between maps calculated for<br />

the same source using the two different algorithms is desired, it is useful to introduce<br />

the unnormalised quantity<br />

∫<br />

Ṽ = d 2 x ∇RM(⃗x) ⃗ · ⃗∇ϕ 0 (⃗x). (4.10)<br />

The quantity Ṽ gives the absolute measure <strong>of</strong> correlation between the gradient alignments<br />

<strong>of</strong> RM and ϕ 0 . The smaller this value is the smaller is the total level <strong>of</strong> correlated<br />

noise in the maps.<br />

4.4.2 Error Under or Over Estimation<br />

One problem, one is faced with is the possibility that the measurement errors are under<br />

or overestimated. Such a hypothesis can be tested by performing a reduced χ 2 ν test<br />

which is considered to be a measure for the goodness <strong>of</strong> each least squares fit and<br />

calculates as follows<br />

] 2<br />

χ 2 ν ij<br />

= 1 f∑<br />

[ϕ obsij (k) − (RM ij λ 2 k + ϕ0 ij )<br />

ν<br />

σ 2 = s2 ij<br />

, (4.11)<br />

k=1<br />

k ij<br />

〈σ kij 〉 k<br />

where ν = f −n c is the number <strong>of</strong> degrees <strong>of</strong> freedom and f is the number <strong>of</strong> frequencies<br />

used and n c is the number <strong>of</strong> model parameters (here n c = 2). The parameter s 2 is<br />

the variance <strong>of</strong> the fit and 〈σ kij 〉 k is the weighted average <strong>of</strong> the individual variances:<br />

⎡<br />

〈σ kij 〉 k = ⎣ 1 f<br />

f∑<br />

k=1<br />

⎤−1<br />

1<br />

⎦<br />

σk 2 ij<br />

(4.12)<br />

If one believes in the assumption <strong>of</strong> Gaussian noise, that the data are not corrupted<br />

and that the linear fit is an appropriate model then any statistical deviation from unity<br />

<strong>of</strong> the map average χ 2 ν <strong>of</strong> this value indicates an under or over error estimation. For<br />

a χ 2 ν > 1, the errors have been underestimated and for a χ 2 ν < 1, they have been<br />

overestimated.<br />

Unfortunately this analysis does not reveal in its simple form at which frequency<br />

the errors might be under or overestimated. However, one can test for the influence <strong>of</strong><br />

single frequencies by leaving out the appropriate frequency for the calculation <strong>of</strong> the<br />

RM map and comparing the resulting χ 2 ν ij<br />

values with the original one.<br />

It is advisable to evaluate the reduced χ 2 ν ij<br />

-maps in order to locate regions <strong>of</strong> too<br />

high or too low values for χ 2 ν by eye.

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