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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 8.

Differences in power-law indices (αλ) between the V and i bands (x-axis) and the B and V bands (y-axis) shown in colored crosses: red for early-red, blue for early-blue, and gold for early-yellow events. The three black open symbols represent the error-bar-weighted means for each population. (KSN-2018ku and KSN-2021V are included in the early-red population as green crosses; see the text). The power-law rise of the events in the four labeled quadrants separated by horizontal and vertical dashed lines evolve in B − V and V − i as follows: (I) blueward in both colors; (II) blueward in B − V and redward in V − i; (III) redward in both colors; and (IV) redward in B − V and blueward in V − i.

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