Published February 21, 2005 | Version v1
Journal article

Model-based analysis of the Galactic Centre with H.E.S.S. during Summer 2003

  • 1. Laboratoire de Physique Nucleaire et de Hautes Energies, IN2P3/CNRS, Universites Paris VI and VII, 4 place Jussieu, F-75252 Paris Cedex 05 (France)

Description

The detection of a very high energy γ-ray source in the direction of the Galactic Centre with the H.E.S.S. array of Cerenkov has been reported in [1]. Another chain of analysis, including different calibration, simulation, image analysis and spectral reconstruction, has been used within the H.E.S.S. collaboration. The results of this model-based analysis are reported

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
745
Journal Issue
1
Journal Page Range
p. 397-402
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
2. international symposium on high energy gamma-ray astronomy
Dates
26-30 Jul 2004
Place
Heidelberg (Germany)

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
36073357
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
CALIBRATION; CHERENKOV COUNTERS; COSMIC GAMMA SOURCES; COSMIC PHOTONS; COSMIC RAY DETECTION; GAMMA ASTRONOMY; IMAGES; SIMULATION; TELESCOPE COUNTERS
Descriptors DEC
ASTRONOMY; BOSONS; COSMIC RADIATION; COSMIC RAY SOURCES; DETECTION; ELEMENTARY PARTICLES; IONIZING RADIATIONS; MASSLESS PARTICLES; MEASURING INSTRUMENTS; PHOTONS; RADIATION DETECTION; RADIATION DETECTORS; RADIATIONS

Optional Information

Notes
(c) 2005 American Institute of Physics
Collaborations
H.E.S.S. Collaboration