Prof. Dr. rer. nat. Burkhardt Funk

Professor - aktiv

Jahrgang
1968
Universität
Leuphana Universität Lüneburg
Fachbereich
Fakultät II – Wirtschafts-, Verhaltens- und Rechtswissenschaften
Arbeitsbereiche
E-Business
Land
Deutschland
Ort / PLZ
21339 Lüneburg
Strasse
Volgershall 1
Telefon
04131-677-180
Sekretariat
04131-677-147
FAX
04131-677-140

Veröffentlichungen

Als Hauptautor

An upper limit on the infrared background density from HEGRA data on Mkn 501
B. Funk et al.
Astroparticle Physics 9, 97-103 (1998).

Search for gamma-ray bursts above 20 TeV with the HEGRA AIROBICC Cherenkov array.
L. Padilla, B. Funk et al.
Astronomy and Astrophysics 337, 43-50 (1998).

The gamma ray burst rate at high photon energies.
K. Mannheim, D. Hartmann, and B. Funk,
Astrophysical Journal 467, 532-536 (1996).

Design and performance of the lead-concrete Geiger tower array within the HEGRA experiment.
W. Rhode et al.,
Nuclear Instruments and Methods A 378, 399-409 (1996).

Separating gamma- and hadron-induced cosmic ray air showers with feed-forward neural networks using the charged particle information
S. Westerhoff, B. Funk, A. Lindner et al.
ASTROPARTICLE PHYSICS, Volume 4, Issue 2, p. 119-132.
Search for Gamma-Ray Bursts with Energies above 1 TeV
V. Matheis, B. Funk, H. Meyer et al.
Astrophysics and Space Science, v. 231, p. 303-306 (1995).


Als Coautor

Measurement of the flux, spectrum, and variability of TeV gamma-rays from Mkn 501 during a state of high activity.
F.A. Aharonian et al. (The HEGRA Collaboration),
Astronomy and Astrophysics 327, L5-L8 (1997).

Detection of gamma-rays above 1.5 TeV from Mkn 501 .
S.M. Bradbury et al. (The HEGRA Collaboration),
Astronomy and Astrophysics 320, L5-L8 (1997).

First results on the performance of the HEGRA IACT array.
A. Daum et al. (The HEGRA Collaboration),
Astroparticle Physics 8, 1-11 (1997).

Detection of VHE gamma-rays from Mkn 421 with the HEGRA Cherenkov telescopes.
D. Petry et al. (The HEGRA Collaboration),
Astronomy and Astrophysics 311, L13-L16 (1996).

Search for very high energy gamma radiation from the radio bright region DR4 of the SNR G78.2+2.1.
C. Prosch et al. (The HEGRA Collaboration),
Astronomy and Astrophysics 314, 275-280 (1996).

An optimized method for the reconstruction of the direction of air showers for scintillator arrays .
H. Krawczynski et al. (The HEGRA Collaboration),
Nuclear Instruments And Methods A 383, 431-440 (1996).

Search for Isotropic Gamma Radiation in the Cosmological Window between 65-TeV and 200-Tev
A. Karle, S. Martinez, R. Plaga et al. (The HEGRA Collaboration)
Phys. Lett. B, 347, 161 (1995).

A Search for Gamma Radiation above 24-TeV Energy from Cosmic Point Sources
A. Karle, F. Arqueros, K.H. Becker et al. (The HEGRA Collaboration)
Astropart. Phys., 4, 1 (1995).


Konferenzbeiträge

e-Yield Management: Ertragschance für Veranstalter?
B. Söder, B. Funk
Ticketmanagement-Kongress, Bonn (2001)

What can we Learn from Tev-Astronomy with Respect to GRBs?
B. Funk
Very High Energy Phenomena in the Universe, Morion Workshop, Editions Frontieres, p.83 (1997)

GRB and their high energy tails.
B. Funk and H. Krawczynski,
Cosmic-ray Astrophysics, Erice (Italy), 16-23 June 1996.
World Scientific, p. 141-147 (1998).

Status of the high energy grb counterpart search with the HEGRA experiment.
B. Funk et al. (The HEGRA Collaboration)
3rd Huntsville Symposium on GRB, Huntsville, AL (USA), 25-27 Oct 1995, AIP Conf. Proc., No. 384 (1996).

Search for TeV gamma-rays from evaporating primordial black holes.
B. Funk et al. (The HEGRA Collaboration),
Paper OG 2.2.5, Vol. 2, p. 104. (ICRC 95).

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