Image Details

Choose export citation format:

TIC 322208686: An Eclipsing System with γ Doradus Pulsations and a Third Component on a Wider Orbit

  • Authors: Jae Woo Lee, Kyeongsoo Hong, Min-Ji Jeong, Jang-Ho Park, Pakakaew Rittipruk, Hye-Young Kim

Jae Woo Lee et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 7.

Light curve residuals from the W-D model fit to the TESS data. The lower panel is a zoomed-in view of the residuals shown in the inset box in the upper panel. The red solid line represents the synthetic curve computed from the 11 frequency fit to the out-of-eclipse data. The residuals from the frequency fit are offset from zero by +20 mmag for clarity and are plotted as the blue symbols. The vertical solid and dotted lines indicate the primary and secondary minimum epochs, respectively.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse