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Overview of the EUSO-SPB2 Target of Opportunity program using the Cherenkov Telescope
High Energy Astrophysical Phenomena · Submitted 18 Oct 2023
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim With the launch of the EUSO-SPB2 payload on the 13th May 2023, this summarizes the ToO program status and preliminary data, as available.
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During the Extreme Universe Space Observatory on a Super Pressure Balloon 2 (EUSO-SPB2) mission, we planned Target of Opportunity (ToO) operations to follow up on possible sources of $\gtrsim 10 \, {\rm PeV}$ neutrinos. The original plan before flight was to point the onboard Cherenkov Telescope (CT) to catch the source's path on the sky just below Earth's horizon. By using the Earth as a tau-neutrino to tau-lepton converter, the CT would then be able to look for optical extensive air shower signals induced by tau-lepton decays in the atmosphere. The CT had a field of view of $6.4^\circ$ vertical $\times$ $12.8^\circ$ horizontal. Possible neutrino source candidates include gamma ray bursts, tidal disruption events and other bursting or flaring sources. In addition, follow-ups of binary neutron star mergers would have been possible after the start of the O4 observation run from LIGO-Virgo-KAGRA. The resulting exposure is modeled using the NuSpaceSim framework in ToO mode. With the launch of the EUSO-SPB2 payload on the 13th May 2023, this summarizes the ToO program status and preliminary data, as available.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | During the Extreme Universe Space Observatory on a Super Pressure Balloon 2 (EUSO-SPB2) mission, we planned Target of Opportunity (ToO) operations to follow up on possible sources of $\gtrsim 10 \, {\rm PeV}$ neutrinos. | contribution 0.83 | 0.83 | 0.07 | asserted 0.99 |
| s1 | The original plan before flight was to point the onboard Cherenkov Telescope (CT) to catch the source's path on the sky just below Earth's horizon. | method 0.94 | 0.55 | 0.03 | asserted 1.00 |
| s2 | By using the Earth as a tau-neutrino to tau-lepton converter, the CT would then be able to look for optical extensive air shower signals induced by tau-lepton decays in the atmosphere. | method 0.98 | 0.15 | 0.05 | asserted 0.52 |
| s3 | The CT had a field of view of $6.4^\circ$ vertical $\times$ $12.8^\circ$ horizontal. | method 1.00 | 0.50 | 0.02 | asserted 1.00 |
| s4 | Possible neutrino source candidates include gamma ray bursts, tidal disruption events and other bursting or flaring sources. | background 0.76 | 0.12 | 0.03 | hedged possibility 0.82 |
| s5 | In addition, follow-ups of binary neutron star mergers would have been possible after the start of the O4 observation run from LIGO-Virgo-KAGRA. | contribution 0.37 | 0.13 | 0.03 | hedged possibility 0.99 |
| s6 | The resulting exposure is modeled using the NuSpaceSim framework in ToO mode. | method 1.00 | 0.74 | 0.04 | asserted 0.99 |
| s7 | With the launch of the EUSO-SPB2 payload on the 13th May 2023, this summarizes the ToO program status and preliminary data, as available. | contribution 0.76 | 0.64 | 0.11 | asserted 0.93 |
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The paper
Original abstract
During the Extreme Universe Space Observatory on a Super Pressure Balloon 2 (EUSO-SPB2) mission, we planned Target of Opportunity (ToO) operations to follow up on possible sources of $\gtrsim 10 \, {\rm PeV}$ neutrinos. The original plan before flight was to point the onboard Cherenkov Telescope (CT) to catch the source's path on the sky just below Earth's horizon. By using the Earth as a tau-neutrino to tau-lepton converter, the CT would then be able to look for optical extensive air shower signals induced by tau-lepton decays in the atmosphere. The CT had a field of view of $6.4^\circ$ vertical $\times$ $12.8^\circ$ horizontal. Possible neutrino source candidates include gamma ray bursts, tidal disruption events and other bursting or flaring sources. In addition, follow-ups of binary neutron star mergers would have been possible after the start of the O4 observation run from LIGO-Virgo-KAGRA. The resulting exposure is modeled using the NuSpaceSim framework in ToO mode. With the launch of the EUSO-SPB2 payload on the 13th May 2023, this summarizes the ToO program status and preliminary data, as available.
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References
How the literature uses it
3 arXiv papers cite this in 4 sentences
Papers citing it · 3 sentences without a confident label
Uses its method or tool 1 paper
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In addition, a modular and open-source software, NuTS[https://pypi.org/project/too-nuts/] [ref] , has been developed to monitor alerts and develop a catalog of potential very-high energy neutrino sources.
POEMMA-Balloon with Radio: A multi-messenger, multi-detector balloon payload · Expectation for Neutrino search from Targets of Opportunity · 0.93
What it cites · 2 sentences without a confident label
Uses the method or tool of 3 papers
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The result of this search can be turned into a limit on the neutrino flux using a Feldman-Cousins 90% confidence level upper limit [ref] .
A Unified Approach to the Classical Statistical Analysis of Small Signals · Introduction · 1.00
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A prioritization scheme for the sources is implemented, based on flux predictions from models, distance of the source from Earth and relative occurrence rate in the local universe [ref] .
POEMMA's Target of Opportunity Sensitivity to Cosmic Neutrino Transient Sources · Source types and creating a schedule · 0.81
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A prioritization scheme for the sources is implemented, based on flux predictions from models, distance of the source from Earth and relative occurrence rate in the local universe [ref] .
High-energy neutrino transients and the future of multi-messenger astronomy · Source types and creating a schedule · 0.81
Cites as support 1 paper
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During the time period we were pointing above the limb, several bifocal cosmic-ray candidate events have been observed, showing that the camera was functional and capable of detecting such signals [ref] .
Modeling of the Tau and Muon Neutrino-induced Optical Cherenkov Signals from Upward-moving Extensive Air Showers · In flight performance · 0.97
Cites as background 1 paper
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The Target of Opportunity (ToO) program was devised as a way to collect interesting source candidates that produce neutrino-induced extensive air shower events and determine possible neutrino sources observed from the Extreme Universe Space Observatory on a Super Pressure Balloon 2 (EUSO-SPB2) [ref] .
Science and mission status of EUSO-SPB2 · Introduction · 0.80
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