Figure 10 from

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF

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 10.

The best-fit transmission spectrum model of WASP-43 b, calculated for the combined dataset including ground-based observations (gray circles), TESS (light-blue circles), HST processed with Iraclis (pink circles), HST processed with TransitFit (dark-red circles), and JWST (green circles). The synthetic model generated by TauREx is shown as a solid blue line, with the corresponding 1σ confidence region indicated by the blue shading. The binned best-fit model values are shown as blue squares. Note that the five outlier transit depths in the optical wavelength range correspond to the R, I, ﹩{z}^{{\prime} }﹩, H, and K filters, respectively.

Copyright and Terms & Conditions

Additional terms of reuse

Other Images in This Article

Copyright and Terms & Conditions