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-Gal\'an, Avinash Singh, Adam A., Miller, Charles D. Kilpatrick, K-Ryan Hinds, Chang Liu, Steve Schulze, Jesper, Sollerman, Theophile Jegou du Laz, Tom\'as Ahumada, Katie Auchettl, S. J., Brennan, Michael W. Coughlin, Christoffer Fremling

TL;DR
This paper reports on the rapid, autonomous follow-up observations of the nearby Type IIP supernova 2024jlf, revealing early interaction features and constraining the progenitor's mass-loss history using new automated programs.
Contribution
Introduction of the BTSbot-nearby program for autonomous, rapid follow-up of nearby transients, enabling early-time spectroscopy and detailed progenitor analysis.
Findings
SN 2024jlf brightened faster than 90% of Type II SNe.
Detected short-lived flash ionization features indicating recent mass loss.
Constrained progenitor's mass-loss rate to between 10^{-4} and 10^{-3} solar masses per year.
Abstract
We present observations of the Type IIP supernova (SN) 2024jlf, including spectroscopy beginning just 0.7 days (17 hours) after first light. Rapid follow-up was enabled by the new program, which involves autonomously triggering target-of-opportunity requests for new transients in Zwicky Transient Facility data that are coincident with nearby ( Mpc) galaxies and identified by the 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 90% of Type II SNe. Early spectra reveal weak flash ionization features: narrow, short-lived () emission lines of H, He II, and C IV. Assuming a wind velocity of km s, these properties indicate that the red supergiant progenitor exhibited…
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Taxonomy
TopicsGamma-ray bursts and supernovae
