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Infant Type Ia Supernovae from the KMTNet. I. Multicolor Evolution and Populations

  • Authors: Yuan Qi Ni, Dae-Sik Moon, Maria R. Drout, Youngdae Lee, Patrick Sandoval, Jeehye Shin, Hong Soo Park, Sang Chul Kim, Kyuseok Oh

Yuan Qi Ni et al 2025 The Astrophysical Journal 983 .

  • Provider: AAS Journals

Caption: Figure 6.

Projection of the color evolution in Figure 5 onto B − V (top) and V − i (bottom) axes. The black dashed line in the top panel separates red and blue objects of SET18 based on B − V color, which approximately correspond to early-red and early-blue in this work. The green shaded region represents the gap in the observations of KSN-2018ku from  ∼0.5–2.0 days, showing the 1σ uncertainties of its interpolated colors, which are particularly large due to its rapid color evolution in infancy prior to the gap within  ≲0.5 day.

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