13 New Light Curves and Updated Mid-Transit Time and Period for Hot Jupiter WASP-104 b with EXOTIC
Heather B. Hewitt, Federico Noguer, Suber Corley, James Ball, Claudia, Chastain, Richard Cochran-White, Kendall Collins, Kris Ganzel, Kimberly, Merriam Gray, Mike Logan, Steve Marquez-Perez, Chyna Merchant, Matthew, Pedone, Gina Plumey, Matthew Rice, Zachary Ruybal

TL;DR
This study used small ground-based telescopes and citizen science data to accurately update the orbital parameters of exoplanet WASP-104 b, demonstrating the value of amateur contributions in exoplanet research.
Contribution
The paper presents a method for amateur astronomers to effectively contribute to exoplanet ephemeris updates using small telescopes and open-source software.
Findings
13 new light curves of sufficient accuracy were obtained.
Updated mid-transit time: 2457805.170208 +/- 0.000036 BJD_TBD.
Updated orbital period: 1.75540644 +/- 0.00000016 days.
Abstract
Using the EXOplanet Transit Interpretation Code (EXOTIC), we reduced 52 sets of images of WASP-104 b, a Hot Jupiter-class exoplanet orbiting WASP-104, in order to obtain an updated mid-transit time (ephemeris) and orbital period for the planet. We performed this reduction on images taken with a 6-inch telescope of the Center for Astrophysics | Harvard & Smithsonian MicroObservatory. Of the reduced light curves, 13 were of sufficient accuracy to be used in updating the ephemerides for WASP-104 b, meeting or exceeding the three-sigma standard for determining a significant detection. Our final mid-transit value was 2457805.170208 +/- 0.000036 BJD_TBD and the final period value was 1.75540644 +/- 0.00000016 days. The true significance of our results is in their derivation from image sets gathered over time by a small, ground-based telescope as part of the Exoplanet Watch citizen science…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Stellar, planetary, and galactic studies · Astronomical Observations and Instrumentation
