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TOI-7154b: A Close-in Massive Brown Dwarf in an Eccentric Orbit

  • Authors: Rohan Ch. Das, Churchil Dwivedi, Rishikesh Sharma, Hareesh G. Bhaskar, K.J. Nikitha, Allyson Bieryla, Boris S. Safonov, Shubhendra N. Das, Abhijit Chakraborty, Lalthakimi Zadeng, David W. Latham, Neelam J.S.S.V. Prasad, Kapil K. Bharadwaj, Kevikumar A. Lad, Ashirbad Nayak

Rohan Ch. Das et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 3.

The GLS periodogram for the combined PARAS-2 and TRES RVs, the residuals RVs, and the spectral window function of TOI-7154 are shown in panels (1)–(3) (top to bottom), respectively. The periodogram shows prominent peaks at ∼0.89 days (teal solid line) and ∼8.5 days (teal dashed line). The ∼8.5 days periodicity is consistent with the TESS transit period (P ∼ 8.86 days) and represents the true orbital signal, while the ∼0.89 day peak is an alias. After removing the 8.5 day signal, no significant periodicities are found. The FAP levels corresponding to 0.1%, 1%, and 10% are shown as horizontal gray, pink, and red dashed lines, respectively.

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