Circe is a parametrisation of guinea-pig output written by T. Ohl in 1997. It provides a faster way to generate beamstrahlung beam data, and the function it uses as a parametrisation of the spectrum is often used as a fitting function for linear collider luminosity spectra (cf. Ref [1Monig reconstruct paper].)
The fitting function used is of the form:
(equ.
1.)
where f(x) represents the luminosity spectrum ∂L/∂√S,
x is the √S/√Snominal, the ratio of center of mass energy to beam energy,
and a0 ...a3 are the four fitting parameters—one of which is usually be found by normalisation of the spectrum.