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| Autori principali: | , , , , , , , , , , , , , , , , , |
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| Natura: | Preprint |
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2026
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| Soggetti: | |
| Accesso online: | https://arxiv.org/abs/2604.05570 |
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| _version_ | 1866914451476709376 |
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| author | A-thano, Napaporn Awiphan, Supachai Kerins, Eamonn Priyadarshi, Akshay McDonald, Iain Tasuya, Orarik Rattanamala, Ronnakrit Jiang, Ing-Guey Joshi, Yogesh C. Yang, Fan Janiak, Ida Munsaket, Patcharawee Qadir, Yasir Abdul Chandaiam, Smanchan Choonhakit, Boonyarit Wutsang, Suwanit Soonthornthum, Boonrucksar Dhillon, Vik S |
| author_facet | A-thano, Napaporn Awiphan, Supachai Kerins, Eamonn Priyadarshi, Akshay McDonald, Iain Tasuya, Orarik Rattanamala, Ronnakrit Jiang, Ing-Guey Joshi, Yogesh C. Yang, Fan Janiak, Ida Munsaket, Patcharawee Qadir, Yasir Abdul Chandaiam, Smanchan Choonhakit, Boonyarit Wutsang, Suwanit Soonthornthum, Boonrucksar Dhillon, Vik S |
| contents | WASP-11~b/HAT-P-10~b is an inflated hot Jupiter, which has a low density that makes it a good target for atmospheric studies using the transmission spectroscopy technique. In this work, we present 31 new transit light curves of WASP-11~b/HAT-P-10~b, obtained through the SPEARNET network. These data were analyzed along with previously published ground-based observations and space-based data from \texttt{TESS}. We refine the planetary parameters of WASP-11~b/HAT-P-10~b and perform a transit timing analysis using data spanning 16 years. The updated ($O-C$) diagram shows no significant evidence of orbital decay. The TTV analysis reveals no significant signals indicative of additional planets. Atmospheric analysis using multi-band optical observations indicates a strong Rayleigh scattering slope in the transmission spectra, which may originate from the planetary atmosphere itself or be influenced by contamination such as stellar activity or light from the companion star. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2604_05570 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Investigation of Transit Timing and an Optical Transmission Spectrum of the Hot Jupiter WASP-11 b A-thano, Napaporn Awiphan, Supachai Kerins, Eamonn Priyadarshi, Akshay McDonald, Iain Tasuya, Orarik Rattanamala, Ronnakrit Jiang, Ing-Guey Joshi, Yogesh C. Yang, Fan Janiak, Ida Munsaket, Patcharawee Qadir, Yasir Abdul Chandaiam, Smanchan Choonhakit, Boonyarit Wutsang, Suwanit Soonthornthum, Boonrucksar Dhillon, Vik S Earth and Planetary Astrophysics WASP-11~b/HAT-P-10~b is an inflated hot Jupiter, which has a low density that makes it a good target for atmospheric studies using the transmission spectroscopy technique. In this work, we present 31 new transit light curves of WASP-11~b/HAT-P-10~b, obtained through the SPEARNET network. These data were analyzed along with previously published ground-based observations and space-based data from \texttt{TESS}. We refine the planetary parameters of WASP-11~b/HAT-P-10~b and perform a transit timing analysis using data spanning 16 years. The updated ($O-C$) diagram shows no significant evidence of orbital decay. The TTV analysis reveals no significant signals indicative of additional planets. Atmospheric analysis using multi-band optical observations indicates a strong Rayleigh scattering slope in the transmission spectra, which may originate from the planetary atmosphere itself or be influenced by contamination such as stellar activity or light from the companion star. |
| title | Investigation of Transit Timing and an Optical Transmission Spectrum of the Hot Jupiter WASP-11 b |
| topic | Earth and Planetary Astrophysics |
| url | https://arxiv.org/abs/2604.05570 |