MAGIC – Major Atmospheric Gamma Imaging Cherenkov Telescope

With a reflector diameter of 17 meters each, the two MAGIC telescopes are the most sensitive Cherenkov telescopes in the world, especially in the energy range below 200 gigaelectronvolts (GeV). Their line of sight is directed at objects that emit gamma rays ranging from 30 GeV to 100 TeV (teraelectronvolts). This means that MAGIC can cover an enormous energy spectrum.

The twin telescopes are located 2,200 meters above sea level on the Canary Island of La Palma where the clear skies and lack of light pollution make for optimal observing conditions. The Max Planck Institute for Physics (MPP) leads the international collaboration of about 165 astrophysicists from 24 research institutions in eleven countries. Together, they are responsible for the construction, operation and maintenance of the telescopes. MAGIC allows astrophysicists to obtain first class data for gaining scientific insights into enigmatic objects and the most violent processes in the universe.

The MAGIC telescopes have been in operation since 2003 and 2009 respectively. The MPP played a major role in the development and construction of their mechanical structure, imaging cameras and calibration system.

Since the outset, MAGIC has delivered many valuable scientific discoveries.

Information on the MAGIC Group

News releases

08/24/2022

The Max-Planck-Institute for Physics is engaged in fundamental research in particle and astroparticle physics from both experimental and theoretical perspectives. One main research activity is the participation in the ATLAS experiment at the Large Hadron Collider (LHC) at CERN.

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08/11/2022

Julia Summerer has just graduated from high school. She is currently doing an internship at the Max Planck Institute for Physics, more precisely with the "MAGIC" working group. The scientists in this group are working on two large telescopes of an international research collaboration on the Canary…

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04/14/2022

Nova outbursts are apparently a source for cosmic rays

MAGIC telescopes observe nova explosion

The MAGIC telescopes have observed the nova RS Ophiuchi shining brightly in gamma rays at extremely high energy. The Gamma rays emanate from protons that are accelerated to very high energies in the shock front following the explosion. This suggests that novae are also a source of the ubiquitous…

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04/14/2021

Messier M87 is 55 million light years away from Earth. As is the case for probably all galaxies, there is a huge black hole in its center. In 2017, a host of telescopes observed the object over the entire energy spectrum. The spectacular result of this extensive observation campaign was the famous…

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07/18/2020

In 2019, the MAGIC telescopes detected the first Gamma Ray Burst at very high energies. This was the most intense gamma-radiation ever obtained from such a cosmic object. But the GRB data have more to offer: with further analyses, the MAGIC scientists could now confirm that the speed of light is…

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11/20/2019

MAGIC telescopes observes most violent gamma-ray burst to date

Gamma-ray burst with ultra power

The gamma-ray burst recorded by the two MAGIC telescopes on 14 January 2019 was spectacular: Never before have astrophysicists captured a gamma-ray burst with such high energy – hundreds of billions times more intense than that of visible light. MAGIC did not capture the gamma-ray burst until the…

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07/11/2018

For the first time, astrophysicists have localized the source of a high energy cosmic neutrino originating outside the Milky Way. It is highly likely that the neutrino comes from a blazar, an active black hole at the center of a distant galaxy in the Orion constellation. How did the scientists reach…

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06/25/2018

15 years ago, the first MAGIC telescope was inaugurated on La Palma in the Canary Islands. In 2009, it was followed by a second telescope of a similar type. Both instruments study cosmic objects that emit high-energy gamma rays, such as supernovae or massive, active black holes in the center of…

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09/20/2017

What gives the particles of cosmic radiation, which permeate the universe, their high energy? It is suspected that supernova remains might act as naturally occurring particle accelerators. Cassiopeia A is one of a handful of such objects in our galaxy and has therefore long been regarded as a…

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11/03/2016

Never before have astrophysicists measured light of such high energy from a celestial object so far away. Around 7 billion years ago, a huge explosion occurred at the black hole in the center of a galaxy. This was followed by a burst of high-intensity gamma rays. A number of telescopes, MAGIC…

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Group members

E-mail address: e-mail@mpp.mpg.de
Phone number: +49 89 32354-extension
name function e-mail extension office
Arbet-Engels, Axel, Dr. Postdoc aarbet 289 235
Bautista Sierra, Angela Yulieth Student bautista 312 236
Berti, Alessio Postdoc aberti 227 224
Besenrieder, Jürgen Engineering jhose 224 125
Chai, Yating PhD-Student ytchai 312 236
Green, David, Dr. Postdoc damgreen 289 235
Green, Jarred Gershon PhD-Student jgreen 259 233
Hahn, Alexander PhD-Student ahahn 421 234
Heckmann, Lea PhD-Student heckmann 259 233
Jobst, Sophie Elli Student ejobst 312 236
Mazin, Daniel, Dr. Scientist mazin 255 110
Mirzoyan, Razmik, Dr. Scientist razmik 328 232
Nozaki, Seiya, Dr. Postdoc nozaki 227 224
Paneque, David, Dr. Scientist dpaneque 349 231
Pirola, Giorgio PhD-Student gpirola 259 233
Schmuckermaier, Felix PhD-Student fschmuck 485 128
Schweizer, Thomas, Dr. Scientist tschweiz 291 222
Strom, Derek, Dr. Engineering dstrom 422 332
Summerer, Julia Student summerer 291 222
Teshima, Masahiro, Dr. Director mteshima 301 217
Werner, Diana Secretary dwerner 364 215
Will, Martin, Dr. Postdoc mwill 291 222

Key publications

Detection of very high energy gamma-ray emission from the gravitationally-lensed blazar QSO B0218+357 with the MAGIC telescopes
MAGIC Collaboration
arxiv:1609.01095

Teraelectronvolt pulsed emission from the Crab Pulsar detected by MAGIC
MAGIC Collaboration
Astronomy & Astrophysics, Volume 585 (January 2016)
doi:10.1051/0004-6361/201526853

Very high Energy γ-Ray from the universe’s middle age: Detection of the z = 0.940 Blazar PKS 1441+25 with MAGIC
Magic Collaboration
The Astrophysical Journal Letters, 815:L23 (8pp), 2015 December 20
doi:10.1088/2041-8205/815/2L23