Three New Light Curves and Updated Transit Timings of WASP-135 b
Kristine Kate Torres, Isabela G. Huckabee, Patrizia Phem Odo, Danielle Baldono, Riana Gabrielle Gamboa, Ma. Francelen Rose Molod, Michelle Dote, Dave Justine Bantilan, Juan Migelle Ferido, Zachary Lacuesta, Mark Erickson Calunod, Franchesca Margarette Visitacion

TL;DR
This paper refines the orbital parameters of exoplanet WASP-135 b using new ground-based transit observations, significantly reducing timing uncertainties and enhancing future observation planning.
Contribution
It introduces three new transit light curves analyzed with the EXOTIC pipeline, improving the ephemeris accuracy for WASP-135 b and demonstrating citizen science's role in exoplanet monitoring.
Findings
Mid-transit time uncertainty reduced by 92%
Refined orbital period to 1.4013776 days
Improved transit forecast precision through 2030
Abstract
We present updated transit timing measurements for the hot Jupiter WASP-135 b using three new ground-based transit observations obtained with Leia, a 0.6-meter telescope operated by NASA's Exoplanet Watch at the Table Mountain Facility. These observations, conducted as part of Exoplanet Watch citizen science initiative, were analyzed with the EXOplanet Transit Interpretation Code (EXOTIC) pipeline to generate high-quality light curves and extract precise mid-transit times. By combining our new data with previously published observations, we refined the planet's ephemeris, reducing uncertainties in both the orbital period and mid-transit time. Our final mid-transit value is 2460585.6563426 +/- 0.00001908 BJD_TDB and the final period value is 1.4013776 +/- 0.0000002 days. Our updated timing solution demonstrates a 92% reduction in mid-transit time uncertainty compared to the original…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Astro and Planetary Science
