The BTSbot-nearby discovery of SN 2024jlf: rapid, autonomous follow-up probes interaction in an 18.5 Mpc Type IIP supernova
Nabeel Rehemtulla, W. V Jacobson-Galán, Avinash Singh, Adam A Miller, Charles D Kilpatrick, K-Ryan Hinds, Chang Liu, Steve Schulze, Jesper Sollerman, Theophile Jegou du Laz, …
We present observations of the Type IIP supernova (SN) 2024jlf, including
spectroscopy beginning just 0.7 days ($\sim$17 hours) after first light. Rapid
follow-up was enabled by the new $\texttt{BTSbot-nearby}$ program, which
involves autonomously triggering target-of-opportunity requests for new
transients in Zwicky Transient Facility data that are coincident with nearby
($D<60$ Mpc) galaxies and identified by the $\texttt{BTSbot}$ machine learning
model. Early photometry and non-detections shortly prior to first light show
that SN 2024jlf initially brightened by $>$4 mag/day, quicker than $\sim$90% of
Type II SNe. Early spectra reveal weak flash ionization features: narrow,
short-lived ($1.3 < \tau ~\mathrm{[d]} < 1.8$) emission lines of H$\alpha$, He
II, and C IV. Assuming a wind velocity of $v_w=50$ km s$^{-1}$, these
properties indicate that the red supergiant progenitor exhibited enhanced
mass-loss in the last year before explosion. We constrain the mass-loss rate to
$10^{-4} < \dot{M}~\mathrm{[M_\odot~yr^{-1}]} < 10^{-3}$ by matching
observations to model grids from two independent radiative hydrodynamics codes.
$\texttt{BTSbot-nearby}$ automation minimizes spectroscopic follow-up latency,
enabling the observation of ephemeral early-time phenomena exhibited by
transients.
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Title
The BTSbot-nearby discovery of SN 2024jlf: rapid, autonomous follow-up probes interaction in an 18.5 Mpc Type IIP supernova