[HTML][HTML] Quantum gravity phenomenology at the dawn of the multi-messenger era—A review

A Addazi, J Alvarez-Muniz, RA Batista… - Progress in Particle and …, 2022 - Elsevier
The exploration of the universe has recently entered a new era thanks to the multi-
messenger paradigm, characterized by a continuous increase in the quantity and quality of …

High-energy neutrino transients and the future of multi-messenger astronomy

C Guépin, K Kotera, F Oikonomou - Nature Reviews Physics, 2022 - nature.com
The discovery of high-energy astrophysical neutrinos and the first hints of coincident
electromagnetic and neutrino emissions opened new opportunities in multi-messenger …

IceCube-Gen2: the window to the extreme Universe

MG Aartsen, R Abbasi, M Ackermann… - Journal of Physics G …, 2021 - iopscience.iop.org
The observation of electromagnetic radiation from radio to γ-ray wavelengths has provided a
wealth of information about the Universe. However, at PeV (10 15 eV) energies and above …

[HTML][HTML] High-energy and ultra-high-energy neutrinos: A Snowmass white paper

M Ackermann, M Bustamante, L Lu, N Otte… - Journal of high energy …, 2022 - Elsevier
Astrophysical neutrinos are excellent probes of astroparticle physics and high-energy
physics. With energies far beyond solar, supernovae, atmospheric, and accelerator …

Leptohadronic single-zone models for the electromagnetic and neutrino emission of TXS 0506+ 056

M Cerruti, A Zech, C Boisson, G Emery… - Monthly Notices of …, 2019 - academic.oup.com
While active galactic nuclei with relativistic jets have long been prime candidates for the
origin of extragalactic cosmic rays and neutrinos, the BL Lac object TXS 0506+ 056 is the …

[HTML][HTML] ASTRI Mini-Array core science at the Observatorio del Teide

S Vercellone, C Bigongiari, A Burtovoi… - Journal of High Energy …, 2022 - Elsevier
Abstract The ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana) Project led by
the Italian National Institute for Astrophysics (INAF) is developing and will deploy at the …

TXS 0506+ 056, the first cosmic neutrino source, is not a BL Lac

P Padovani, F Oikonomou… - Monthly Notices of …, 2019 - academic.oup.com
We present evidence that TXS 0506+ 056, the first plausible non-stellar neutrino source,
despite appearances, is not a blazar of the BL Lac type but is instead a masquerading BL …

Leptohadronic blazar models applied to the 2014–2015 flare of TXS 0506+ 056

X Rodrigues, S Gao, A Fedynitch… - The Astrophysical …, 2019 - iopscience.iop.org
We investigate whether the emission of neutrinos observed in 2014–2015 from the direction
of the blazar TXS 0506+ 056 can be accommodated with leptohadronic multiwavelength …

[HTML][HTML] Association of IceCube neutrinos with radio sources observed at Owens Valley and Metsähovi Radio Observatories

T Hovatta, E Lindfors, S Kiehlmann… - Astronomy & …, 2021 - aanda.org
Context. Identifying the most likely sources for high-energy neutrino emission has been one
of the main topics in high-energy astrophysics ever since the first observation of high-energy …

Cascading constraints from neutrino-emitting blazars: the case of TXS 0506+ 056

A Reimer, M Böttcher, S Buson - The Astrophysical Journal, 2019 - iopscience.iop.org
We present a procedure to generally constrain the environments of neutrino-producing sites
in photomeson production models of jetted active galactic nuclei (AGNs) where any origin of …