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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 4.

V-band images of KSP-OT-202104a. Panel (a) is a quiescent phase image made by stacking 549 60 s exposures obtained during MJD = 58795.27–59298.86 before the superoutburst. Panel (b) is the first detection image at MJD = 59313.40; (c) is a near-peak image of the superoutburst at MJD = 59314.01; and (d) is the last image during the declining part at MJD = 59339.05. The labels (a)–(d) coincide with those in the light curve in Figure 1. North is up, and east is to the left. Crosshairs mark the position of KSP-OT-202104a. Horizontal bars of 5″ are shown in the bottom-left corners.

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