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

Abstract We present a new set of 35 transit light curves of the hot Jupiter WASP-43 b, obtained through the SPEARNET network. These datasets were analyzed together with previously published ground-based observations, as well as space-based data from TESS, Hubble Space Telescope (HST), and JWST, to refine the planetary parameters of WASP-43 b. A total of 188 midtransit times, measured with TransitFit , were analyzed for potential timing variations. The transit timing variations do not show any significant evidence of orbital decay. Atmospheric retrievals using HST/WFC3 G141 transmission spectra suggest that higher-temperature solutions are associated with higher water abundances. However, when these data are combined with observations from ground-based telescopes, TESS, and JWST, the increased modeling complexity across the broad wavelength baseline presents significant challenges for atmospheric characterization. These results highlight that high-precision, multi-instrument datasets will be necessary to break existing degeneracies in the atmospheric modeling of this target in the future.

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Publication Details

Journal
The Astronomical Journal
Published
2026-05-01
DOI
https://doi.org/10.3847/1538-3881/ae5b78
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
0.00

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article

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

Vik. S. Dhillon, Smanchan Chandaiam, Ronnakrit Rattanamala, O. Tasuya et al.
The Astronomical Journal
Stellar, planetary, and galactic studies
article

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

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

Abstract

Abstract We present a new set of 35 transit light curves of the hot Jupiter WASP-43 b, obtained through the SPEARNET network. These datasets were analyzed together with previously published ground-based observations, as well as space-based data from TESS, Hubble Space Telescope (HST), and JWST, to refine the planetary parameters of WASP-43 b. A total of 188 midtransit times, measured with TransitFit , were analyzed for potential timing variations. The transit timing variations do not show any significant evidence of orbital decay. Atmospheric retrievals using HST/WFC3 G141 transmission spectra suggest that higher-temperature solutions are associated with higher water abundances. However, when these data are combined with observations from ground-based telescopes, TESS, and JWST, the increased modeling complexity across the broad wavelength baseline presents significant challenges for atmospheric characterization. These results highlight that high-precision, multi-instrument datasets will be necessary to break existing degeneracies in the atmospheric modeling of this target in the future.

The Astronomical JournalVol. 171(5)
Centre National de la Recherche Scientifique (FR), National Science and Technology Development Agency (TH), University of Turku (FI), The Open University (GB), National Tsing Hua University (TW), Commissariat à l'Énergie Atomique et aux Énergies Alternatives (FR), Université Paris-Saclay (FR), Aryabhatta Research Institute of Observational Sciences (IN), University of Manchester (GB), Astrophysique, Instrumentation et Modélisation (FR), CEA Paris-Saclay (FR), Instituto de Astrofísica de Canarias (ES), Nakhon Ratchasima Rajabhat University (TH), Institut de Recherche sur les Lois Fondamentales de l'Univers (FR), Chiang Mai University (TH), Suranaree University of Technology (TH), National Astronomical Research Institute of Thailand (TH), University of Sheffield (GB)
National Astronomical Research Institute of Thailand, Thailand Science Research and Innovation
Openalex Percentile: Top 7%
Stellar, planetary, and galactic studies
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