Advanced

Distant Quasar Sets Gamma-Ray Record ⚡ экспресс

Original: "First detection of VHE gamma-ray signal from the FSRQ TON 0599"
· MAGIC Collaboration, K. Abe, S. Abe, J. Abhir, A. Abhishek, V. A. Acciari, A. Aguasca-Cabot, I. Agudo, T. Aniello, S. Ansoldi, L. A. Antonelli, A. Arbet Engels, C. Arcaro, K. Asano, A. Babić, U. Barres de Almeida, J. A. Barrio, L. Barrios-Jiménez, I. Batković, J. Baxter, J. Becerra González, W. Bednarek, E. Bernardini, J. Bernete, A. Berti, J. Besenrieder, C. Bigongiari, A. Biland, O. Blanch, G. Bonnoli, Ž. Bošnjak, E. Bronzini, I. Burelli, A. Campoy-Ordaz, A. Carosi, R. Carosi, M. Carretero-Castrillo, A. J. Castro-Tirado, D. Cerasole, G. Ceribella, Y. Chai, A. Cifuentes, J. L. Contreras, J. Cortina, S. Covino, G. D'Amico, P. Da Vela, F. Dazzi, A. De Angelis, B. De Lotto, R. de Menezes, M. Delfino, J. Delgado, C. Delgado Mendez, F. Di Pierro, R. Di Tria, L. Di Venere, A. Dinesh, D. Dominis Prester, A. Donini, D. Dorner, M. Doro, L. Eisenberger, D. Elsaesser, J. Escudero, L. Foffano, L. Font, S. Fröse, S. Fukami, Y. Fukazawa, M. Garczarczyk, S. Gasparyan, M. Gaug, J. G. Giesbrecht Paiva, N. Giglietto, F. Giordano, P. Gliwny, N. Godinović, T. Gradetzke, R. Grau, D. Green, J. G. Green, P. Günther, D. Hadasch, A. Hahn, T. Hassan, L. Heckmann, J. Herrera Llorente, D. Hrupec, R. Imazawa, D. Israyelyan, I. Jiménez Martínez, J. Jiménez Quiles, J. Jormanainen, S. Kankkunen, D. Kerszberg, M. Khachatryan, J. Konrad, P. M. Kouch, H. Kubo, J. Kushida, M. Láinez, A. Lamastra, E. Lindfors, S. Lombardi, F. Longo, R. López-Coto, M. López-Moya, A. López-Oramas, S. Loporchio, A. Lorini, L. Lulić, E. Lyard, P. Majumdar, M. Makariev, G. Maneva, M. Manganaro, S. Mangano, K. Mannheim, M. Mariotti, M. Martínez, P. Maruševec, A. Mas-Aguilar, D. Mazin, S. Menchiari, S. Mender, D. Miceli, J. M. Miranda, R. Mirzoyan, M. Molero González, E. Molina, H. A. Mondal, A. Moralejo, T. Nakamori, C. Nanci, V. Neustroev, L. Nickel, C. Nigro, L. Nikolić, K. Nilsson, K. Nishijima, K. Noda, S. Nozaki, Y. Ohtani, A. Okumura, J. Otero-Santos, L. Pacciani, S. Paiano, D. Paneque, R. Paoletti, J. M. Paredes, M. Peresano, M. Persic, M. Pihet, F. Podobnik, P. G. Prada Moroni, E. Prandini, G. Principe, M. Ribó, J. Rico, C. Righi, N. Sahakyan, T. Saito, F. G. Saturni, K. Schmitz, F. Schmuckermaier, J. L. Schubert, A. Sciaccaluga, G. Silvestri, J. Sitarek, D. Sobczynska, A. Stamerra, J. Strišković, Y. Suda, H. Tajima, M. Takahashi, R. Takeishi, F. Tavecchio, P. Temnikov, K. Terauchi, T. Terzić, M. Teshima, A. Tutone, S. Ubach, J. van Scherpenberg, S. Ventura, G. Verna, I. Viale, A. Vigliano, C. F. Vigorito, V. Vitale, I. Vovk, R. Walter, F. Wersig, M. Will, T. Yamamoto, J. A. Acosta-Pulido, G. A. Borman, W. Boschin, V. Bozhilov, M. I. Carnerero, D. Carosati, C. Casadio, W. Chamani, W. P. Chen, G. Damljanovic, S. A. Ehgamberdiev, K. E. Ergashev, M. Giroletti, T. S. Grishina, M. A. Gurwell, M. K. Hallum, E. Järvelä, H. E. Jermak, S. G. Jorstad, M. D. Jovanovic, E. N. Kopatskaya, K. Kuratov, O. M. Kurtanidze, S. O. Kurtanidze, A. Lähteenmäki, E. G. Larionova, L. V. Larionova, V. M. Larionov, H. C. Lin, N. Marchili, A. P. Marscher, C. McCall, M. Minev, D. O. Mirzaqulov, I. Myserlis, M. G. Nikolashvili, T. Pursimo, C. M. Raiteri, I. Reva, S. Righini, A. C. Sadun, S. S. Savchenko, E. Semkov, P. S. Smith, I. A. Steele, M. Tornikoski, Yu. V. Troitskaya, I. S. Troitskiy, A. A. Vasilyev, M. Villata, O. Vince, Z. R. Weaver
arXiv:2601.03873v2 · 2026-01-07 · CC BY · ⏱ 1 min · High Energy
The MAGIC telescopes caught a record-breaking gamma-ray burst from a black hole that lived 7 billion years ago.
Abstract

The quasar TON 0599 (z=0.7247) is one of the few flat-spectrum radio quasars detected in the very-high-energy gamma-ray range (E > 100 GeV). Observations with the MAGIC telescopes from 15 to 29 December 2017 revealed a flare with a peak flux ~50% of the Crab Nebula above 80 GeV, followed by a decline. The VHE spectrum smoothly connects with simultaneous Fermi-LAT data and shows a break around 50 GeV, indicating the emission region lies beyond the broad-line region. Multiwavelength analysis (optical, near-IR, radio from WEBT, X-ray and optical/UV from Swift) showed strong correlation between bands. The emission is modeled by a one-zone leptonic model, where the high-energy peak is primarily due to external Compton scattering off photons from the dusty torus. This constrains the gamma-ray source location and confirms the role of the environment in particle acceleration.

Links in the knowledge graph 1

📄 Showing the "Simple" version — "Advanced" is not ready yet. Add it to favorites to help prioritize it.

Seven billion years ago, a black hole at the center of a galaxy unleashed a gamma-ray flare — the most energetic form of light — with staggering power. Its light, after crossing cosmic distances, reached the MAGIC telescopes in December 2017. Along the way, the expansion of the Universe stretched the waves, making them longer. But the real surprise was yet to come: the radiation came not from the hole itself, but from the dust ring surrounding it.

The mechanism is like a game of billiards. Particles accelerated by the hole to nearly the speed of light slam into dust grains like target balls. This is how gamma-ray photons — packets of pure energy — are born.

By studying the spectrum (the breakdown of light by energy), astronomers confirmed that the dust acts as the target. A single such gamma-ray photon carries the energy of a mosquito bite, but packed into a volume smaller than an atomic nucleus. Flares like these are windows into the past: they show us how black holes function as particle accelerators when the Universe was half its current age.

🎯 A single gamma-ray photon from this quasar carries energy comparable to a mosquito bite — but concentrated into a volume smaller than an atomic nucleus. If such a photon hit a person, it would knock out a whole cascade of particles.

Scientists
Adam RiessBrian SchmidtEdwin HubbleGeorges LemaîtreMaarten SchmidtSaul Perlmutter
Tags
black hole cosmic dust galaxy expansion of the universe spectroscopy
Laws
Hubble's lawDoppler effectHawking radiationgravitational lensingBekenstein-Hawking entropyEinstein field equations
Original: arXiv:2601.03873v2 · CC BY · bridge42worlds