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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 2.

Schematic light curve diagram (blue solid curve) of a type D WZ Sge-type DN without rebrightening. Thick gray horizontal line represents the quiescent phase brightness. The beginning points of the four phases—rising, plateau, decline, and tail parts—are marked as 1, 2, 3, and 4, respectively. The short blue dashed line is the extension of the decline part to the quiescent magnitude. “Dp” between points 1 and 5 is the outburst duration above the quiescent magnitude.

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