Early-phase simultaneous multiband observations of the Type II supernova SN 2024ggi with Mephisto

Abstract

We present early-phase good-cadence (hour-to-day) simultaneous multiband ($ugi$ and $vrz$ bands) imaging of the nearby supernova SN~2024ggi, which exploded in the nearby galaxy, NGC 3621. A quick follow-up was conducted within less than a day after the explosion and continued $\sim$23 days. The $uvg$ band light curves display a rapid rise ($\sim$1.4 mag day${}^{-1}$) to maximum in $\sim$4 days and absolute magnitude $M_g\sim$--17.75 mag. The post-peak decay rate in redder bands is $\sim$0.01 mag day${}^{-1}$. Different colors (e.g., $u-g$ and $v-r$) of SN~2024ggi are slightly redder than SN 2023ixf. A significant rise ($\sim$12.5 kK) in black-body temperature (optical) was noticed within $\sim$2 days after the explosion, which successively decreased, indicating shock break out inside a dense circumstellar medium (CSM) surrounding the progenitor. Using semianalytical modeling, the ejecta mass and progenitor radius were estimated as 1.2 $M_{\odot }$ and $\sim$550 $R_{\odot }$. The archival deep images ($g,r,iandz$ bands) from the Dark Energy Camera Legacy Survey were examined, and a possible progenitor was detected in each band ($\sim$22--22.5 mag) and had a mass range of 14--17 $M_{\odot }$.

Pages 12, Table 1, Figures 7