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A New WZ Sagittae-type Dwarf Nova KSP-OT-202104a Near the Period Minimum from the KMTNet Supernova Program

  • Authors: Sang Chul Kim, Youngdae Lee, Dae-Sik Moon, Hong Soo Park, Yuan Qi Ni, Nan Jiang, Hyobin Im

Sang Chul Kim et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 5.

(a) Results of PDM analysis and (b) phase-folded profile. In panel (a), the black solid line is median Θ and the shaded area presents 90% confidence range from 1,000 bootstrap resampling. In panel (b), blue, green, and red colors indicate B, V, and I band, respectively. The black dashed curve is a sine curve fitted to the data with the period of 71.7 minutes.

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