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The Transit Timing and Transmission Spectrum of Hot Jupiter WASP-43 b from a Decade of Multiband Transit follow-up Observations

  • Authors: Napaporn A-thano, Supachai Awiphan, Eamonn Kerins, Akshay Priyadarshi, Iain McDonald, Ing-Guey Jiang, Yogesh C. Joshi, Fan Yang, Ida Janiak, Patcharawee Munsaket, Yasir Abdul Qadir, Ronnakrit Rattanamala, Orarik Tasuya, Ekburus Boonsoy, Nuanwan Sanguansak, Rattiyakorn Rattanasai, Thammasorn Padjaroen, Siramas Komonjinda, Sawatkamol Pichadee, Ananpol Sudsap, Smanchan Chandaiam, Boonyarit Choonhakit, Suwanit Wutsang, Vik S Dhillon

Napaporn A-thano et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 7.

Upper mass limit of the perturbing planet in the WASP-43 system. The best ﹩{\rm{\Delta }}{\chi }_{{\rm{red}}}^{2}﹩ values, binned with a period ratio of 0.05, are shown as the black dotted line. The upper mass limits for TTV amplitudes of 5, 15, and 25 s are represented by the blue dashed–dotted, green dashed, and red solid lines, respectively. The white vertical line represents the orbital period of WASP-43 b. The black vertical lines, from left to right, indicate the orbital period resonances of 2:1, 1:2, 1:3, and 1:4. The contour illustrates the ﹩{\rm{\Delta }}{\chi }_{{\rm{red}}}^{2}﹩ values from comparing the best TTV model to the best linear model. The unstable orbit region is shown as the shaded black area.

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