activity
20092018
most citedPerformance of the MAGIC stereo system obtained with Crab Nebula data

245 citations · 3.8k across the 69 of their papers we have counts for

collaborators

70 papers

quant-ph2018★ 6 cited

Towards a standard procedure for the measurement of the multi-photon component in a CW telecom heralded single-photon source

E. Rebufello, F. Piacentini, M. López +8

Single-photon sources are set to be a fundamental tool for metrological applications as well as for quantum information related technologies. Because of their upcoming widespread d…

astro-ph.HE2018★ 28 cited

The detection of the blazar S4 0954+65 at very-high-energy with the MAGIC telescopes during an exceptionally high optical state

MAGIC Collaboration, M. L. Ahnen, S. Ansoldi +169

The very-high-energy (VHE, GeV) -ray MAGIC observations of the blazar S4 0954+65, were triggered by an exceptionally high flux state of emission in the optical. Th…

astro-ph.HE2017★ 43 cited

Indirect dark matter searches in the dwarf satellite galaxy Ursa Major II with the MAGIC Telescopes

MAGIC Collaboration, M. L. Ahnen, S. Ansoldi +142

The dwarf spheroidal galaxy Ursa Major II (UMaII) is believed to be one of the most dark-matter dominated systems among the Milky Way satellites and represents a suitable target fo…

astro-ph.HE2017★ 45 cited

Constraining Lorentz invariance violation using the Crab Pulsar emission observed up to TeV energies by MAGIC

MAGIC Collaboration, M. L. Ahnen, S. Ansoldi +142

Spontaneous breaking of Lorentz symmetry at energies on the order of the Planck energy or lower is predicted by many quantum gravity theories, implying non-trivial dispersion relat…

astro-ph.IM2017★ 1 cited

Performance of the MAGIC telescopes under moonlight

D. Guberman, P. Colin

MAGIC, a system of two imaging atmospheric Cherenkov telescopes, achieves its best performance under dark conditions, i.e. in absence of moonlight or twilight. Since operating the…

astro-ph.HE2017★ 11 cited

MAGIC observations of the microquasar V404 Cygni during the 2015 outburst

M. L. Ahnen, S. Ansoldi, L. A. Antonelli +142

The microquasar V404 Cygni underwent a series of outbursts in 2015, June 15-31, during which its flux in hard X-rays (20-40 keV) reached about 40 times the Crab Nebula flux. Becaus…

astro-ph.HE2017★ 6 cited

Observation of the Black Widow B1957+20 millisecond pulsar binary system with the MAGIC telescopes

MAGIC Collaboration, M. L. Ahnen, S. Ansoldi +145

B1957+20 is a millisecond pulsar located in a black widow type compact binary system with a low mass stellar companion. The interaction of the pulsar wind with the companion star w…

astro-ph.IM2017★ 87 cited

Performance of the MAGIC telescopes under moonlight

MAGIC Collaboration, M. L. Ahnen, S. Ansoldi +143

MAGIC, a system of two imaging atmospheric Cherenkov telescopes, achieves its best performance under dark conditions, i.e. in absence of moonlight or twilight. Since operating the…

astro-ph.HE2017★ 33 cited

First Multi-wavelength Campaign on the Gamma-ray-loud Active Galaxy IC 310

M. L. Ahnen, S. Ansoldi, L. A. Antonelli +160

The extragalactic VHE gamma-ray sky is rich in blazars. These are jetted active galactic nuclei viewed at a small angle to the line-of-sight. Only a handful of objects viewed at a…

astro-ph.HE2017★ 20 cited

MAGIC detection of very high energy gamma-ray emission from the low-luminosity blazar 1ES 1741+196

MAGIC Collaboration, M. L. Ahnen, S. Ansoldi +159

We present the first detection of the nearby (z=0.084) low-luminosity BL Lac object 1ES 1741+196 in the very high energy (VHE: E100 GeV) band. This object lies in a triplet of i…

physics.ins-det2017★ 21 cited

A measurement of the ionization efficiency of nuclear recoils in silicon

F. Izraelevitch, D. Amidei, A. Aprahamian +26

We have measured the ionization efficiency of silicon nuclear recoils with kinetic energy between 1.8 and 20 keV. We bombarded a silicon-drift diode with a neutron beam to perform…

astro-ph.HE2016★ 67 cited

Multiband variability studies and novel broadband SED modeling of Mrk 501 in 2009

M. L. Ahnen, S. Ansoldi, L. A. Antonelli +290

We present an extensive study of the BL Lac object Mrk 501 based on a data set collected during the multi-instrument campaign spanning from 2009 March 15 to 2009 August 1 which inc…

astro-ph.HE2016★ 34 cited

Observations of Sagittarius A* during the pericenter passage of the G2 object with MAGIC

M. L. Ahnen, S. Ansoldi, L. A. Antonelli +153

Context. We present the results of a multi-year monitoring campaign of the Galactic Center (GC) with the MAGIC telescopes. These observations were primarily motivated by reports th…

astro-ph.HE2016★ 39 cited

A search for spectral hysteresis and energy-dependent time lags from X-ray and TeV gamma-ray observations of Mrk 421

A. U. Abeysekara, S. Archambault, A. Archer +220

Blazars are variable emitters across all wavelengths over a wide range of timescales, from months down to minutes. It is therefore essential to observe blazars simultaneously at di…

astro-ph.HE2016★ 89 cited

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

MAGIC Collaboration, M. L. Ahnen, S. Ansoldi +151

Context. QSO B0218+357 is a gravitationally lensed blazar located at a redshift of 0.944. The gravitational lensing splits the emitted radiation into two components, spatially indi…

astro-ph.GA2016★ 46 cited

Long-term multi-wavelength variability and correlation study of Markarian 421 from 2007 to 2009

MAGIC Collaboration, M. L. Ahnen, S. Ansoldi +176

We study the multi-band variability and correlations of the TeV blazar Mrk 421 on year time scales, which can bring additional insight on the processes responsible for its broadban…

astro-ph.HE2016★ 29 cited

Super-orbital variability of LS I +61°303 at TeV energies

MAGIC Collaboration, M. L. Ahnen, S. Ansoldi +150

The gamma-ray binary LS I +61303 is a well established source from centimeter radio up to very high energy (VHE; E100 GeV). Its broadband emission shows a periodicity…

astro-ph.HE2016★ 62 cited

Deep observation of the NGC 1275 region with MAGIC: search of diffuse gamma-ray emission from cosmic rays in the Perseus cluster

MAGIC Collaboration, M. L. Ahnen, S. Ansoldi +154

Clusters of galaxies are expected to be reservoirs of cosmic rays (CRs) that should produce diffuse gamma-ray emission due to their hadronic interactions with the intra-cluster med…

astro-ph.HE2015★ 143 cited

Multiwavelength Study of Quiescent States of Mrk 421 with Unprecedented Hard X-Ray Coverage Provided by NuSTAR in 2013

M. Baloković, D. Paneque, G. Madejski +305

We present coordinated multiwavelength observations of the bright, nearby BL Lac object Mrk 421 taken in 2013 January-March, involving GASP-WEBT, Swift, NuSTAR, Fermi-LAT, MAGIC, V…

astro-ph.GA2015★ 117 cited

Very-high-energy gamma-rays from the Universe's middle age: detection of the z=0.940 blazar PKS 1441+25 with MAGIC

MAGIC Collaboration, M. L. Ahnen, S. Ansoldi +246

The flat-spectrum radio quasar PKS 1441+25 at a redshift of z = 0.940 is detected between 40 and 250 GeV with a significance of 25.5 σ using the MAGIC telescopes. Together with the…

astro-ph.HE2015★ 143 cited

Teraelectronvolt pulsed emission from the Crab pulsar detected by MAGIC

MAGIC Collaboration, S. Ansoldi, L. A. Antonelli +139

Aims: To investigate the extension of the very-high-energy spectral tail of the Crab pulsar at energies above 400 GeV. Methods: We analyzed 320 hours of good quality data of…

physics.ins-det2015★ 1 cited

Status of the DAMIC direct dark matter search experiment

DAMIC Collaboration, A. Aguilar-Arevalo, D. Amidei +31

The DAMIC experiment uses fully depleted, high resistivity CCDs to search for dark matter particles. With an energy threshold 50 eV, and excellent energy and spatial r…

astro-ph.HE2015★ 32 cited

Very-high-energy γ-ray observations of novae and dwarf novae with the MAGIC telescopes

MAGIC Collaboration, M. L. Ahnen, S. Ansoldi +148

Context. In the last five years the Fermi Large Area Telescope (LAT) instrument detected GeV γ-ray emission from five novae. The GeV emission can be interpreted in terms of an inve…

astro-ph.HE2015★ 1 cited

Feasibility of VHE gamma ray detection by an array of imaging atmospheric Cherenkov telescopes using the fluorescence technique

J. L. Contreras, J. Rosado, F. Arqueros +3

The last 20 years have seen the development of new techniques in Astroparticle Physics providing access to the highest end of the electromagnetic spectrum. It has been shown that s…