applicationContext = Production

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.

MAGIC discoveries

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, some of which are described below:

Peak values from the Crab Pulsar

In the Crab Pulsar, MAGIC detected the most energetic pulsed gamma radiation ever measured in a star: The pulses reached energy peak values of up to 1.5 teraelectronvolts. It is still unclear what mechanism accelerates charged particles to such high energy levels.

Sky lab for blazars

Together with other instruments such as the Fermi-LAT satellite, VERITAS and H.E.S.S., MAGIC is scanning the electromagnetic spectra of the nearby Markarian 421 and Markarian 501 blazars. These are a kind of "testing lab" for finding distant active galactic nuclei.

Record emissions from galaxies

Violent processes around black holes in the center of galaxies emit far higher levels of energy than previously assumed, as revealed by observations of the galaxies PKS 1441+25 and QSO B0218+357. They are the most distant galaxies emitting gamma rays at very high energies and allow researchers to study the transparency of the universe. QSO B0218+357 is the first source of radiation discovered at very high energies discovered through gravitational lensing.

Information on the MAGIC Group

News releases

The MAGIC telescope system at the Roque de los Muchachos Observatory, La Palma, Canary Islands, Spain (Photo: G. Ceribella/MAGIC Collaboration)

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...

Read more

MAGIC telescopes observes most violent gamma-ray burst to date

Gamma-ray burst with ultra power

Künstlerische Darstellung eines Gammablitzes mit Jet

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...

Read more
The MAGIC telescopes in the Roque de los Muchachos observatory on the Canary island of La Palma

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...

Read more
The MAGIC telescopes at the Roque de los Muchachos observatory on the canary island La Palma (Photo: T. Dettlaff/MPP)

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...

Read more
The supernova remains Cassiopeia A generates too little energy for it to come into question as an accelerator for cosmic radiation.

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...

Read more
Die MAGIC-Teleskope auf der Kanareninsel La Palma

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...

Read more

The Crab Pulsar has set a new record: The neutron star in the Crab Nebula is sending out the most energetic light radiation that has ever been measured from a star. This observation could challenge our current understanding of pulsars. Moreover, a new mechanism, little understood up to now, appears...

Read more

For the first time, scientists have observed gamma radiation from a well-known distant galaxy. In the center of the active galaxy PKS 1441+25 resides a massive black hole, which is surrounded by a luminous disk of matter. The latest observation leads not only to a better understanding of active...

Read more

The Instituto de Astrofísica de Canaria (IAC) on Tenerife was honored by a visit of Felipe VI, King of Spain. The king was the VIP guest at the ceremony for IAC’s 30th anniversary. The next day, the monarch visited also the MAGIC telescopes on the island of La Palma, where he gained insight into...

Read more

Turbulent processes take place close to supermassive black holes, which lurk in the centres of nearly all galaxies. They swallow up matter flowing in from the outside while at the same time producing so-called gas jets which shoot out into space in two opposite directions. Researchers at the Max...

Read more

Group members

name function extension office www

Besenrieder, Jürgen

Engineering 224 125

Ceribella, Giovanni

PhD-Student 259 233

Chai, Yating

PhD-Student 312 236

Green, David, Dr.

Postdoc 289 235

Hahn, Alexander

PhD-Student 421 234

Heckmann, Lea

PhD-Student 259 233

Huetten, Moritz, Dr.

Postdoc 289 235

Ishio, Kazuma

PhD-Student 421 235

Mazin, Daniel, Dr.

Scientist 255 110

Mirzoyan, Razmik, Dr.

Scientist 328 232

Ohtani, Yoshiki

PhD-Student 213 015C

Paneque, David, Dr.

Scientist 349 231

Pihet, Marine

Student 485 128

Sakurai, Shunsuke

Student 213 015C

Schmuckermaier, Felix

Student 485 128

Schweizer, Thomas, Dr.

Scientist 227 224

Strom, Derek, Dr.

Engineering 422 332

Suda, Yusuke, Dr.

Postdoc 575 222

Teshima, Masahiro, Dr.

Director 301 217

Werner, Diana

Secretary 364 215

Will, Martin, Dr.

Postdoc 291 222

van Scherpenberg, Juliane

PhD-Student 421 234

Events and meetings

Currently, there are no events or meetings.

Key publications

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

Teraelectronvolt pulsed emission from the Crab Pulsar detected by MAGIC
MAGIC Collaboration
Astronomy & Astrophysics, Volume 585 (January 2016)

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