papers

Publications (39)

astro-ph.HE2010

Discovery of VHE gamma-rays from the BL Lac object PKS 0548-322

H. E. S. S. collaboration, :, F. Aharonian +168

PKS 0548-322 (z=0.069) is a ``high-frequency-peaked'' BL Lac object and a candidate very high energy (VHE, E>100 GeV) gamma-ray emitter, due to its high X-ray and radio flux. Obser…

astro-ph1999

VHE Gamma Rays from PKS 2155-304

P. M. Chadwick, K. Lyons, T. J. L. McComb +5

The X-ray selected BL Lac PKS 2155-304 has been observed using the University of Durham Mark 6 very high energy gamma ray telescope during 1998. We find no evidence for TeV emissio…

astro-ph.HE2010

H.E.S.S. constraints on Dark Matter annihilations towards the Sculptor and Carina Dwarf Galaxies

HESS Collaboration, A. Abramowski, F. Acero +192

The Sculptor and Carina Dwarf spheroidal galaxies were observed with the H.E.S.S. Cherenkov telescope array between January 2008 and December 2009. The data sets consist of a total…

astro-ph1999

Correlation between the TeV gamma ray and X-ray emission from an accreting X-ray binary

P. M. Chadwick, K. Lyons, T. J. L. McComb +6

This paper has been withdrawn by the authors.

astro-ph.HE2011

H.E.S.S. observations of the globular clusters NGC 6388 and M 15 and search for a Dark Matter signal

HESS Collaboration, A. Abramowski, F. Acero +195

Observations of the globular clusters NGC 6388 and M 15 were carried out by the H.E.S.S. array of Cherenkov telescopes for a live time of 27.2 and 15.2 hours respectively. No gamma…

astro-ph.HE2011

Very-high-energy gamma-ray emission from the direction of the Galactic globular cluster Terzan 5

HESS Collaboration, A. Abramowski, F. Acero +194

The H.E.S.S. very-high-energy (VHE, E > 0.1 TeV) gamma-ray telescope system has discovered a new source, HESS J1747-248. The measured integral flux is (1.2 +/- 0.3) \times 10^-12 c…

astro-ph.HE2011

HESS J1943+213: a candidate extreme BL Lacertae object

H. E. S. S. Collaboration, :, A. Abramowski +200

We report on a newly detected point-like source, HESS J1943+213 located in the Galactic plane. This source coincides with an unidentified hard X-ray source IGR J19443+2117, which w…

astro-ph1999

TeV Measurements of Young Pulsars and Supernova Remnants

P. M. Chadwick, K. Lyons, T. J. L. McComb +6

Observations have been made with the University of Durham Mark 6 telescope of a number of supernova remnants and young pulsars (Vela pulsar, PSR B1055-52, PSR J1105-6107, PSR J0537…

astro-ph.HE2011

Search for Lorentz Invariance breaking with a likelihood fit of the PKS 2155-304 flare data taken on MJD 53944

HESS Collaboration, A. Abramowski, F. Acero +193

Several models of Quantum Gravity predict Lorentz Symmetry breaking at energy scales approaching the Planck scale (10^{19} GeV). With present photon data from the observations of d…

astro-ph1999

Geomagnetic Effects on the Performance of Atmospheric Cerenkov Telescopes

P. M. Chadwick, K. Lyons, T. J. L. McComb +5

Atmospheric Cerenkov telescopes are used to detect electromagnetic showers from primary gamma rays of energy > 300 GeV and to discriminate these from cascades due to hadrons using…

astro-ph.HE2012

Discovery of VHE γ-ray emission and multi-wavelength observations of the BL Lac object 1RXS J101015.9-311909

HESS Collaboration, A. Abramowski, F. Acero +191

1RXS J101015.9-311909 is a galaxy located at a redshift of z=0.14 hosting an active nucleus belonging to the class of bright BL Lac objects. Observations at high (HE, E > 100 MeV)…

astro-ph.HE2011

Search for a Dark Matter annihilation signal from the Galactic Center halo with H.E.S.S

H. E. S. S. Collaboration, :, A. Abramowski +193

A search for a very-high-energy (VHE; >= 100 GeV) gamma-ray signal from self-annihilating particle Dark Matter (DM) is performed towards a region of projected distance r ~ 45-150 p…

astro-ph.HE2010

Revisiting the Westerlund 2 Field with the H.E.S.S. Telescope Array

The HESS Collaboration, A. Abramowski, F. Acero +194

Aims. Previous observations with the H.E.S.S. telescope array revealed the existence of extended very-high-energy (VHE; E>100 GeV) γ-ray emission, HESS J1023-575, coincident with…

astro-ph1999

TeV Gamma Ray Emission from Cen X-3

P. M. Chadwick, K. Lyons, T. J. L. McComb +5

Cen X-3 is a well-studied high-mass accreting X-ray binary and a variable source of high energy gamma rays from 100 MeV to 1 TeV. The object has been extensively monitored with the…

astro-ph.HE2011

A new SNR with TeV shell-type morphology: HESS J1731-347

HESS Collaboration, A. Abramowski, F. Acero +195

The recent discovery of the radio shell-type supernova remnant (SNR), G353.6-0.7, in spatial coincidence with the unidentified TeV source HESS J1731-347 has motivated further obser…

astro-ph1998

The Uuniversity of Durham Mark 6 Gamma Ray Telescope

P. Armstrong, P. M. Chadwick, P. J. Cottle +18

The design, construction and operation of the University of Durham ground-based gamma ray telescope is discussed. The telescope has been designed to detect gamma rays in the < 200…

astro-ph1999

Correlation between the X-ray and TeV Gamma Ray Emission from an Accreting X-ray Binary

P. M. Chadwick, K. Lyons, T. J. L. McComb +6

This paper has been withdrawn by the authors.

astro-ph.HE2010

Multi-wavelength Observations of H 2356-309

HESS Collaboration, A. Abramowski, F. Acero +184

AIMS: The properties of the broad-band emission from the high-frequency peaked BL Lac H 2356-309 (z=0.165) are investigated. METHODS: Very High Energy (VHE; E > 100 GeV) observatio…

astro-ph.HE2011

Discovery of extended VHE γ-ray emission from the vicinity of the young massive stellar cluster Westerlund 1

HESS Collaboration, A. Abramowski, F. Acero +198

Results obtained in very-high-energy (VHE; E > 100 GeV) γ-ray observations performed with the H.E.S.S. telescope array are used to investigate particle acceleration processes in t…

astro-ph.HE2010

Discovery and follow-up studies of the extended, off-plane, VHE gamma-ray source HESS J1507-622

H. E. S. S. Collaboration, F. Acero, F. Aharonian +167

Context: The detection of gamma-rays in the very-high-energy (VHE) range (100 GeV-100 TeV) offers the possibility of studying the parent population of ultrarelativistic particles f…

astro-ph.HE2011

Simultaneous multi-wavelength campaign on PKS 2005-489 in a high state

The H. E. S. S. Collaboration, the Fermi LAT Collaboration, : +345

The high-frequency peaked BL Lac object PKS 2005-489 was the target of a multi-wavelength campaign with simultaneous observations in the TeV gamma-ray (H.E.S.S.), GeV gamma-ray (Fe…

astro-ph.HE2010

First detection of VHE gamma-rays from SN 1006 by H.E.S.S

HESS Collaboration, F. Acero, F. Aharonian +175

Recent theoretical predictions of the lowest very high energy (VHE) luminosity of SN 1006 are only a factor 5 below the previously published H.E.S.S. upper limit, thus motivating f…

astro-ph2001

Very high energy gamma-rays from Centaurus X-3: indications and implications

A. M. Atoyan, P. M. Chadwick, M. K. Daniel +7

A timing analysis of VHE gamma-ray observations of Cen X-3 taken with the University of Durham Mark 6 telescope was performed, using both Rayleigh and Bayesian statistics. Data fro…

astro-ph1999

A Search for VHE Gamma Rays from AGNs Visible from the Southern Hemisphere

P. M. Chadwick, K. Lyons, T. J. L. McComb +5

Observations have been made, using the University of Durham Mark 6 gamma ray telescope, of the very high energy gamma ray emission from a number of active galactic nuclei visible f…

astro-ph1998

VHE Gamma Rays from PKS 2155-304

P. M. Chadwick, K. Lyons, T. J. L. McComb +6

The close X-ray selected BL Lac PKS 2155-304 has been observed using the University of Durham Mark 6 very high energy (VHE) gamma ray telescope during 1996 September/October/Novemb…

astro-ph1999

The energy spectra of TeV sources measured with the Durham Mark 6 Telescope

P. M. Chadwick, K. Lyons, T. J. L. McComb +5

A programme of detailed simulations of the response of the Durham Mark 6 atmospheric Cherenkov telescope is in progress. The effective collecting area for triggering by gamma-ray s…

astro-ph1998

PKS 2155-304 - a source of VHE gamma-rays

P. M. Chadwick, K. Lyons, T. J. L. McComb +7

The close X-ray selected BL Lac PKS 2155--304 has been observed using the University of Durham Mark 6 very high energy (VHE) gamma ray telescope during 1996 September/October/Novem…

astro-ph1998

Centaurus X-3 - A Source of High Energy Gamma Rays

P. M. Chadwick, M. R. Dickinson, N. A. Dipper +8

Centaurus X-3 is a well-studied high-mass accreting X-ray binary and a variable source of high energy gamma rays with energies from 100 MeV to 1 TeV. Previous results have suggeste…

astro-ph1998

TeV gamma rays from PSR 1706-44

P. M. Chadwick, M. R. Dickinson, N. A. Dipper +9

Observations made with the University of Durham Mark 6 atmospheric Cerenkov telescope confirm that PSR B1706-44 is a very high energy gamma-ray emitter. There is no indication from…

astro-ph.HE2013

Search for Dark Matter Annihilation Signals from the Fornax Galaxy Cluster with H.E.S.S

HESS Collaboration, A. Abramowski, F. Acero +195

The Fornax galaxy cluster was observed with the High Energy Stereoscopic System (H.E.S.S.) for a total live time of 14.5 hours, searching for very-high-energy (VHE, E>100 GeV) gamm…

astro-ph1999

Measurements of Flux Limits for TeV Emission from AGNs

P. M. Chadwick, K. Lyons, T. J. L. McComb +6

The University of Durham Mark 6 Telescope has been used to make observations of a number of AGNs visible from the Southern Hemisphere. Results are presented for limits to VHE gamma…

astro-ph.CO2012

The 2010 very high energy gamma-ray flare & 10 years of multi-wavelength observations of M 87

The H. E. S. S. Collaboration, :, A. Abramowski +442

Abridged: The giant radio galaxy M 87 with its proximity, famous jet, and very massive black hole provides a unique opportunity to investigate the origin of very high energy (VHE;…

astro-ph.HE2010

VHE gamma-ray emission of PKS 2155-304: spectral and temporal variability

HESS Collaboration, A. Abramowski, F. Acero +185

Observations of very high energy gamma-rays from blazars provide information about acceleration mechanisms occurring in their innermost regions. Studies of variability in these obj…

astro-ph.HE2011

Discovery of the source HESS J1356-645 associated with the young and energetic PSR J1357-6429

HESS Collaboration, A. Abramowski, F. Acero +195

Several newly discovered very-high-energy (VHE; E > 100 GeV) gamma-ray sources in the Galaxy are thought to be associated with energetic pulsars. Among them, middle-aged (> 1E+4 yr…

astro-ph.HE2011

Detection of very-high-energy gamma-ray emission from the vicinity of PSR B1706-44 and G343.1-2.3 with H.E.S.S

H. E. S. S. Collaboration, :, A. Abramowski +198

The gamma-ray pulsar PSR B1706-44 and the adjacent supernova remnant (SNR) candidate G343.1-2.3 were observed by H.E.S.S. during a dedicated observation campaign in 2007. As a resu…

astro-ph.HE2012

A multiwavelength view of the flaring state of PKS 2155-304 in 2006

HESS Collaboration, A. Abramowski, F. Acero +208

Multiwavelength (MWL) observations of the blazar PKS 2155-304 during two weeks in July and August 2006, the period when two exceptional flares at very high energies (VHE, E>= 100 G…

astro-ph.HE2012

Discovery of VHE emission towards the Carina arm region with the H.E.S.S. telescope array: HESS J1018-589

HESS Collaboration, A. Abramowski, F. Acero +195

The observational coverage with HESS of the Carina region in VHE gamma-rays benefits from deep exposure (40 h) of the neighboring open cluster Westerlund 2. The observations have r…

astro-ph1999

Geomagnetic effects on atmospheric Cerenkov images

P. M. Chadwick, K. Lyons, T. J. L. McComb +6

Atmospheric Cerenkov telescopes are used to detect electromagnetic showers from primary gamma rays of energy ~300 GeV - ~10 TeV and to discriminate these from cascades due to hadro…

astro-ph.HE2012

Discovery of hard-spectrum γ-ray emission from the BL Lac object 1ES 0414+009

The HESS Collaboration, A. Abramowski, F. Acero +199

1ES 0414+009 (z = 0.287) is a distant high-frequency-peaked BL Lac object, and has long been considered a likely emitter of very-high energy (VHE, E>100 GeV) gamma-rays due to its…