https://doi.org/10.1051/epjconf/202531903002
Multi-messenger emission from astrophysical sources hidden in γ-rays
1 Department of Physics, Ariel University, Ariel, Israel
2 Ruhr University Bochum, Faculty of Physics and Astronomy, Astronomical Institute (AIRUB), Universitätsstraße 150, 44801 Bochum, Germany
3 Istituto Nazionale di Fisica Nucleare, Sezione di Roma, P. le Aldo Moro 2, I-00185 Rome, Italy
4 Dipartimento di Fisica dell’Università La Sapienza, P. le Aldo Moro 2, I-00185 Rome, Italy
5 Department of Physics, University of Florida, Gainesville, FL 32611-8440, USA
* e-mail: dafneguetta@gmail.com
Published online: 6 March 2025
Over the last decade, choked jets have attracted particular attention as potential sources of high-energy cosmic neutrinos. Testing this hypothesis is challenging because of the missing gamma-ray counterpart; hence the identification of other electromagnetic signatures is crucial. Extended H envelopes surrounding collapsing massive stars might choke launched jets. In addition, the same progenitors are expected to produce a shock breakout signal in the ultraviolet (UV) and optical lasting several days. Early UV radiation, in particular, will carry important information about the presence and nature of choked jets. While UV observations of core-collapse supernovae have so far been limited, the full potential of observations in this spectral band will soon be transformed by the ULTRASAT satellite mission with its unprecedented field of view. Here, we investigate the detection prospects of choked jet progenitors by ULTRASAT, in relation to their visibility in the optical band by the currently operating telescope ZTF. We find that ULTRASAT will double the volume of sky currently visible by ZTF for the same emitting sources, enlarging the sample of observed Type II supernovae by ∼ 60%. For optimised multi-messenger detections, the delay between neutrinos produced at the shock breakout (during the jet propagation inside the stellar envelope) and ULTRASAT observations should be of ∼4(5) days, with subsequent follow-up by instruments like ZTF about one week after.
© The Authors, published by EDP Sciences, 2025
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
