# The double-peaked radio light curve of PTF11qcj

## TL;DR

This paper reports on extended radio observations of supernova PTF11qcj, revealing a double-peaked light curve that suggests complex circumstellar interactions or an off-axis gamma-ray burst, with implications for understanding supernova progenitors.

## Contribution

It provides the first detailed radio light curve analysis of PTF11qcj over five years, proposing models for the double-peak profile and discussing the possible presence of an off-axis GRB.

## Key findings

- Radio light curve shows a double-peak profile.
- Modeling indicates a flatter CSM density profile and higher progenitor mass-loss rate.
- Off-axis GRB scenario remains plausible but requires unusual parameters.

## Abstract

We present continued radio follow-up observations of PTF11qcj, a highly energetic broad-lined Type Ic supernova (SN), with a radio peak luminosity comparable to that of the $\gamma$-ray burst (GRB) associated SN 1998bw. The latest observations, carried out with the Karl G. Jansky Very Large Array (VLA), extend up to $\sim$5 years after the PTF11qcj optical discovery. The radio light curve shows a double-peak profile, possibly associated with density variations in the circumstellar medium (CSM), or with the presence of an off-axis GRB jet. Optical spectra of PTF11qcj taken during both peaks of the radio light curve do not show the broad H$\alpha$ features typically expected from H-rich circumstellar interaction. Modeling of the second radio peak within the CSM interaction scenario requires a flatter density profile and an enhanced progenitor mass-loss rate compared to those required to model the first peak. Although our radio data alone cannot rule out the alternative scenario of an off-axis GRB powering the second radio peak, the implied off-axis GRB parameters are unusual compared to typical values found for cosmological long GRBs. Deep X-ray observations carried out around the time of the second radio peak could have helped distinguish between the density variation and off-axis GRB scenarios. Future VLBA measurements of the PTF11qcj radio ejecta may unambiguously rule out the off-axis GRB jet scenario.