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Observational Evidence Favors a Static Universe - Journal of ...

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where σi is the uncertainty in yi, εi is the uncertainty in xi and η is described<br />

below. It is apparent that this equation has the basic symmetry in that if η is<br />

zero then interchanging x and y will give the reciprocal <strong>of</strong> the slope b. If all the<br />

ε are zero it has an analytic solution otherwise the minimization can be done<br />

numerically.<br />

A problem arises when the χ 2 value is significantly different from the number<br />

<strong>of</strong> degrees <strong>of</strong> freedom. The case where the value <strong>of</strong> χ 2 is much less than the<br />

number <strong>of</strong> degrees <strong>of</strong> freedom is handled by multiplying the uncertainties by<br />

the square root <strong>of</strong> the ratio <strong>of</strong> χ 2 to the degrees <strong>of</strong> freedom. If the χ 2 is larger<br />

than the number <strong>of</strong> degrees <strong>of</strong> freedom the approach used here is to assume<br />

that there is an additional, unknown contribution which is uncorrelated with<br />

the existing uncertainties. This is a common occurrence when the uncertainties<br />

are measurement errors and may be precise but some other factor makes a<br />

significant contribution the scatter <strong>of</strong> values. the solution is to add a quadratic<br />

term, η 2 , to the denominator and estimate its value by making the χ 2 equal to<br />

the degrees <strong>of</strong> freedom. The prime advantage <strong>of</strong> this technique is that it provides<br />

a smooth transition from the situation where the given uncertainties dominate<br />

to the alternative where they are negligible. The main effect is a change in the<br />

relative weights.<br />

References<br />

Andreon, A., Lobo, C. & Iovino, A., (2004). Extending the Butcher-Oemler<br />

effect up to z 0.7. MNRAS, 349, 889.<br />

Astier, A., Guy, J., Regnault, N., Pain, R., Aubourg, E., Balam, D., Basa, S.,<br />

56

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