Transit Analysis Package: An IDL Graphical User Interface for Exoplanet Transit Photometry

Table 1

Analysis of Johnson et al., [34] WASP-10b light curve.

Parameter	Value
	Johnson et al. [34]	TAP: no red noise	TAP
Period [days]	3.0927616	⋯	⋯
Inclination [deg]	88.49^+0.22−0.17	88.44^+0.25−0.21	88.50^+0.34−0.25
𝑎/𝑅𝑠	11.65^+0.09−0.13	11.60±0.14	11.64±0.16
𝑅𝑝/𝑅𝑠	0.1592^+0.0005−0.0012	0.1593±0.0012	0.1588^+0.0014−0.0017
𝑇mid [HJD since 2454664.0]	0.037295±0.000082	0.03731±0.000066	0.037312±0.000087

A comparison between the analysis originally published by [17] and our TAP analysis. The results indicate that TAP reproduces the derived parameters and that the light curve contains no significant red noise contamination. For all analyses, orbital period (𝑃=3.0927616 days) and eccentricity parameters (𝑒=0.051,𝜔=2.67 radians) were locked to values derived by [17] using RV data from [10].