S. Funk
University of Erlangen-Nuremberg
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Publication
Featured researches published by S. Funk.
web science | 2005
F. Aharonian; A. G. Akhperjanian; V. Borrel; A. R. Bazer-Bachi; M. Beilicke; W. Benbow; Y. Fuchs; D. Berge; K. Bernlöhr; O. Bolz; C. Boisson; J.F. Glicenstein; F. Breitling; A. M. Brown; H.J. Dickinson; P. M. Chadwick; I. Braun; L.-M. Chounet; R. Cornils; L. Costamante; B. Degrange; A. Djannati-Ataï; L. O'c. Drury; D. Emmanoulopoulos; P. Espigat; F. Feinstein; G. Dubus; G. Fontaine; S. Funk; Y.A. Gallant
We report the detection of TeV
The Astrophysical Journal | 2012
F. Giordano; M. Naumann-Godo; J. Ballet; K. Bechtol; S. Funk; J. Lande; M. N. Mazziotta; S. Rainò; T. Tanaka; O. Tibolla; Y. Uchiyama
\gamma
Science | 2009
Eveline A. Helder; J. Vink; C.G. Bassa; Aya Bamba; J. A. M. Bleeker; S. Funk; Parviz Ghavamian; K. J. van der Heyden; F. Verbunt; Ryo Yamazaki
-rays from the shell-type supernova remnant RX J0852.0-4622 with data of 3.2 h of live time recorded with H.E.S.S. in February 2004. An excess of (700
Astroparticle Physics | 2004
S. Funk; German Hermann; J. A. Hinton; D. Berge; K. Bernlöhr; W. Hofmann; P. Nayman; F. Toussenel; P. Vincent
\pm
The Astrophysical Journal | 2010
Y. Uchiyama; R. D. Blandford; S. Funk; Hiroyasu Tajima; T. Tanaka
60) events from the whole remnant with a significance of 12
The Astrophysical Journal | 2012
J. Lande; Markus Ackermann; A. Allafort; J. Ballet; K. Bechtol; T. H. Burnett; J. Cohen-Tanugi; Alex Drlica-Wagner; S. Funk; F. Giordano; Marie-Hélène Grondin; Matthew Kerr; M. Lemoine-Goumard
\sigma
web science | 2005
F. Aharonian; A. G. Akhperjanian; K.-M. Aye; A. R. Bazer-Bachi; M. Beilicke; W. Benbow; D. Berge; P. Berghaus; K. Bernlöhr; C. Boisson; O. Bolz; C. Borgneier; I. Bruan; F. Breitling; A. M. Brown; J. Bussons Gordo; P. M. Chadwick; L.-M. Chounet; R. Cornils; L. Costamante; B. Degrange; A. Djannati-Ataï; L. O'c. Drury; G. Dubus; T. Ergin; P. Espigat; F. Feinstein; P. Fleury; G. Fontaine; S. Funk
was found. The observed emission region is clearly extended with a radius of the order of 1 degree and the spatial distribution of the signal correlates with X-ray observations. The spectrum in the energy range between 500 GeV and 15 TeV is well described by a power law with a photon index of
Physics of the Dark Universe | 2015
Daniel A. Bauer; James Henry Buckley; M. Cahill-Rowley; Randel Cotta; A. Drlica-Wagner; Jonathan L. Feng; S. Funk; JoAnne L. Hewett; Dan Hooper; A. Ismail; Manoj Kaplinghat; Alexander Kusenko; K. Matchev; D. N. McKinsey; T. Rizzo; William Shepherd; Tim M. P. Tait; Alexander M. Wijangco; M. Wood
\Gamma=2.1 \pm 0.1_{stat} \pm 0.2_{syst}
Monthly Notices of the Royal Astronomical Society | 2011
A. Charbonnier; Vi-Vii Paris U.; C. Combet; U Leicester; M. Daniel; U Durham; S. Funk; Menlo Park Kipac; J.A. Hinton; D. Maurin; Grenoble Lpsc; Inst. Astrophys. Paris; C. Power; Trieste Ictp; J.I. Read; S. Sarkar; M.G. Walker; U Cambridge; Harvard-Smithsonian Ctr. Astrophys.; M.I. Wilkinson
and a differential flux at 1 TeV of
Astronomy and Astrophysics | 2005
F. Aharonian; A. G. Akhperjanian; K.-M. Aye; A. R. Bazer-Bachi; M. Beilicke; W. Benbow; D. Berge; P. Berghaus; K. Bernlöhr; C. Boisson; O. Bolz; I. Braun; F. Breitling; A. M. Brown; J. Bussons Gordo; P. M. Chadwick; L.-M. Chounet; R. Cornils; L. Costamante; B. Degrange; A. Djannati-Ataï; L. O'c. Drury; G. Dubus; D. Emmanoulopoulos; P. Espigat; F. Feinstein; P. Fleury; G. Fontaine; Y. Fuchs; S. Funk
\varphi
