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When Neutrinos Don't Point the Way: A Blazar Mystery
**Introduction:**
* This episode discusses the search for the sources of high-energy neutrinos using the example of the blazar B3 2247+381.
* The IceCube Neutrino Observatory detects astrophysical neutrinos, and scientists are working to find their origins by looking for correlations between neutrino alerts and electromagnetic radiation from objects like blazars.
**The IceCube Alert and B3 2247+381:**
* IceCube detected a multiplet of muon neutrino events, which appeared to be coming from the direction of the blazar B3 2247+381 between May and November 2022.
* This triggered a multiwavelength observational campaign, including observations by the VERITAS telescope.
* The Gamma-ray Follow-Up (GFU) program is a method used by IceCube to enable follow up investigations of known gamma-ray sources for which IceCube has detected a cluster of candidate neutrino events.
**VERITAS and Multiwavelength Observations:**
* VERITAS did not detect B3 2247+381 during the time period of the neutrino alert.
* The source was in a low-flux state in the optical, ultraviolet, and gamma-ray bands during the neutrino event.
* B3 2247+381 was detected in the hard X-ray band with NuSTAR during this time.
* Data from Swift-XRT, Swift-UVOT, ASAS-SN, ATLAS, and the 48” optical telescope at the FLWO were also used in this study.
* The multiwavelength spectral energy distribution (SED) was modeled using a one-zone leptonic synchrotron self-Compton (SSC) radiation model.
**Analysis and Findings:**
* The observed neutrino excess had a significance of 3.2σ but was likely not fully corrected for trials. The corresponding false alert rate was 0.0355 per year.
* The neutrino events associated with B3 2247+381 had energies primarily between 0.5 TeV and 6 TeV, making them likely to be atmospheric neutrino background.
* The lack of detection by VERITAS, combined with the low multiwavelength flux levels during the neutrino alert period, suggests that B3 2247+381 is an unlikely source of the IceCube multiplet.
* The neutrino excess is likely a background fluctuation.
* The study highlights some of the challenges in searching for neutrino-emitting blazars, such as the limited localization precision of the IceCube Observatory and the effect of weather on IACT observations.
* The one-zone leptonic model reasonably fits the SED, suggesting that no hadronic component is needed to explain the data.
**Conclusion:**
* This study is an example of a follow-up to an IceCube alert within the framework of the GFU program.
* Further multiwavelength observations, especially during flaring periods, and improved understanding of instrument uncertainties, are needed to identify neutrino sources.
* Future neutrino detectors are expected to improve sensitivity to high-energy neutrino events.
**Reference:**
* Acharyya, A., et al. "VERITAS and multiwavelength observations of the Blazar B3 2247+381 in response to an IceCube neutrino alert." *Draft version February 7, 2025*
Acknowledements: Podcast prepared with Google/NotebookLM. Illustration credits: CfA/Rick Peterson
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By Astro-COLIBRI**Introduction:**
* This episode discusses the search for the sources of high-energy neutrinos using the example of the blazar B3 2247+381.
* The IceCube Neutrino Observatory detects astrophysical neutrinos, and scientists are working to find their origins by looking for correlations between neutrino alerts and electromagnetic radiation from objects like blazars.
**The IceCube Alert and B3 2247+381:**
* IceCube detected a multiplet of muon neutrino events, which appeared to be coming from the direction of the blazar B3 2247+381 between May and November 2022.
* This triggered a multiwavelength observational campaign, including observations by the VERITAS telescope.
* The Gamma-ray Follow-Up (GFU) program is a method used by IceCube to enable follow up investigations of known gamma-ray sources for which IceCube has detected a cluster of candidate neutrino events.
**VERITAS and Multiwavelength Observations:**
* VERITAS did not detect B3 2247+381 during the time period of the neutrino alert.
* The source was in a low-flux state in the optical, ultraviolet, and gamma-ray bands during the neutrino event.
* B3 2247+381 was detected in the hard X-ray band with NuSTAR during this time.
* Data from Swift-XRT, Swift-UVOT, ASAS-SN, ATLAS, and the 48” optical telescope at the FLWO were also used in this study.
* The multiwavelength spectral energy distribution (SED) was modeled using a one-zone leptonic synchrotron self-Compton (SSC) radiation model.
**Analysis and Findings:**
* The observed neutrino excess had a significance of 3.2σ but was likely not fully corrected for trials. The corresponding false alert rate was 0.0355 per year.
* The neutrino events associated with B3 2247+381 had energies primarily between 0.5 TeV and 6 TeV, making them likely to be atmospheric neutrino background.
* The lack of detection by VERITAS, combined with the low multiwavelength flux levels during the neutrino alert period, suggests that B3 2247+381 is an unlikely source of the IceCube multiplet.
* The neutrino excess is likely a background fluctuation.
* The study highlights some of the challenges in searching for neutrino-emitting blazars, such as the limited localization precision of the IceCube Observatory and the effect of weather on IACT observations.
* The one-zone leptonic model reasonably fits the SED, suggesting that no hadronic component is needed to explain the data.
**Conclusion:**
* This study is an example of a follow-up to an IceCube alert within the framework of the GFU program.
* Further multiwavelength observations, especially during flaring periods, and improved understanding of instrument uncertainties, are needed to identify neutrino sources.
* Future neutrino detectors are expected to improve sensitivity to high-energy neutrino events.
**Reference:**
* Acharyya, A., et al. "VERITAS and multiwavelength observations of the Blazar B3 2247+381 in response to an IceCube neutrino alert." *Draft version February 7, 2025*
Acknowledements: Podcast prepared with Google/NotebookLM. Illustration credits: CfA/Rick Peterson