Image Details
Caption: Figure 2.
Left panel: the fit to σ of the PS with the best parameters derived from the sigmoid function. The best-fit parameters to this function are noted in the first row of Table 1. Right panel: the fit to σ of the CS with the best parameters derived from a piecewise function. The data points below zcut = 3.01 are best fit with a fourth-order polynomial, while the data points above zcut are best fit with a sigmoid. The best-fit parameters to these functions are noted in the second and third rows of Table 1.
© 2025. The Author(s). Published by the American Astronomical Society.