36450
2011
2011
eng
193
316
124
3
32
article
Springer
Dordrecht
CTA Consortium
1
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Design concepts for the Cherenkov Telescope Array CTA an advanced facility for ground-based high-energy gamma-ray astronomy
Ground-based gamma-ray astronomy has had a major breakthrough with the impressive results obtained using systems of imaging atmospheric Cherenkov telescopes. Ground-based gamma-ray astronomy has a huge potential in astrophysics, particle physics and cosmology. CTA is an international initiative to build the next generation instrument, with a factor of 5-10 improvement in sensitivity in the 100 GeV-10 TeV range and the extension to energies well below 100 GeV and above 100 TeV. CTA will consist of two arrays (one in the north, one in the south) for full sky coverage and will be operated as open observatory. The design of CTA is based on currently available technology. This document reports on the status and presents the major design concepts of CTA.
Experimental astronomy : an international journal on astronomical instrumentation and data analysis
10.1007/s10686-011-9247-0
0922-6435
1572-9508
wos:2011-2013
WOS:000300769700001
Hofmann, W (reprint author), Heidelberg Univ, CTA Project Off, D-69117 Heidelberg, Germany., Werner.Hofmann@mpi-hd.mpg.de; martinez@ifae.es
Ministerio de Ciencia, Tecnologia e Innovacion Productiva (MinCyT);
Comision Nacional de Energia Atomica (CNEA); Consejo Nacional de
Investigaciones Cientificas y Tecnicas (CONICET) Argentina; State
Committee of Science of Armenia; Ministry for Research, France;
CNRS-INSU, France; CNRS-IN2P3, France; CEA, France; Max Planck Society,
Germany; BMBF, Germany; DESY, Germany; Helmholtz Association, Germany;
MIUR, Italy; Netherlands Research School for Astronomy (NOVA);
Netherlands Organization for Scientific Research (NWO); Ministry of
Science and Higher Education, Poland; National Centre for Research and
Development, Poland; MICINN; CPAN, Spain; MultiDark Consolider-Ingenio
programme, Spain; Swedish Research Council, Sweden; Royal Swedish
Academy of Sciences, Sweden; Swiss National Science Foundation (SNSF),
Switzerland; Leverhulme Trust, UK; Royal Society, UK; Science and
Technologies Facilities Council, UK; Durham University, UK; National
Science Foundation; Department of Energy; Argonne National Laboratory;
University of California; University of Chicago; Iowa State University;
Institute for Nuclear and Particle Astrophysics (INPAC-MRPI); Washington
University McDonnell Center for the Space Sciences, USA
M. Actis
G. Agnetta
Felix A. Aharonian
A. G. Akhperjanian
J. Aleksic
E. Aliu
D. Allan
I. Allekotte
F. Antico
L. A. Antonelli
P. Antoranz
A. Aravantinos
T. Arlen
H. Arnaldi
S. Artmann
K. Asano
H. G. Asorey
J. Baehr
A. Bais
C. Baixeras
S. Bajtlik
D. Balis
A. Bamba
C. Barbier
M. Barcelo
Anna Barnacka
Jürgen Barnstedt
U. Barres de Almeida
J. A. Barrio
S. Basso
D. Bastieri
C. Bauer
J. Becerra Gonzalez
Yvonne Becherini
K. C. Bechtol
J. Becker
Volker Beckmann
W. Bednarek
B. Behera
M. Beilicke
M. Belluso
M. Benallou
W. Benbow
J. Berdugo
K. Berger
T. Bernardino
K. Bernlöhr
A. Biland
S. Billotta
T. Bird
E. Birsin
E. Bissaldi
S. Blake
O. Blanch Bigas
A. A. Bobkov
L. Bogacz
M. Bogdan
Catherine Boisson
J. Boix Gargallo
J. Bolmont
G. Bonanno
A. Bonardi
T. Bonev
Janett Borkowski
O. Botner
A. Bottani
M. Bourgeat
C. Boutonnet
A. Bouvier
S. Brau-Nogue
I. Braun
T. Bretz
M. S. Briggs
Pierre Brun
L. Brunetti
H. Buckley
V. Bugaev
R. Buehler
Tomasz Bulik
G. Busetto
S. Buson
K. Byrum
M. Cailles
R. A. Cameron
R. Canestrari
S. Cantu
E. Carmona
A. Carosi
John Carr
P. H. Carton
M. Casiraghi
H. Castarede
O. Catalano
S. Cavazzani
S. Cazaux
B. Cerruti
M. Cerruti
M. Chadwick
J. Chiang
M. Chikawa
M. Cieslar
M. Ciesielska
A. N. Cillis
C. Clerc
P. Colin
J. Colome
M. Compin
P. Conconi
V. Connaughton
Jan Conrad
J. L. Contreras
P. Coppi
M. Corlier
P. Corona
O. Corpace
D. Corti
J. Cortina
H. Costantini
G. Cotter
B. Courty
S. Couturier
S. Covino
J. Croston
G. Cusumano
M. K. Daniel
F. Dazzi
A. Deangelis
E. de Cea del Pozo
E. M. de Gouveia Dal Pino
O. de Jager
I. de la Calle Perez
G. De La Vega
B. De Lotto
M. de Naurois
E. de Ona Wilhelmi
V. de Souza
B. Decerprit
C. Deil
E. Delagnes
G. Deleglise
C. Delgado
T. Dettlaff
A. Di Paolo
F. Di Pierro
C. Diaz
J. Dick
H. Dickinson
S. W. Digel
D. Dimitrov
G. Disset
A. Djannati-Ataï
M. Doert
W. Domainko
D. Dorner
M. Doro
J. -L. Dournaux
D. Dravins
L. Drury
F. Dubois
R. Dubois
G. Dubus
C. Dufour
D. Durand
J. Dyks
M. Dyrda
E. Edy
Kathrin Egberts
C. Eleftheriadis
S. Elles
D. Emmanoulopoulos
R. Enomoto
J. -P. Ernenwein
M. Errando
A. Etchegoyen
A. D. Falcone
K. Farakos
C. Farnier
S. Federici
F. Feinstein
D. Ferenc
E. Fillin-Martino
D. Fink
C. Finley
J. P. Finley
R. Firpo
D. Florin
C. Foehr
E. Fokitis
Ll. Font
G. Fontaine
A. Fontana
A. Foerster
L. Fortson
N. Fouque
C. Fransson
G. W. Fraser
L. Fresnillo
C. Fruck
Y. Fujita
Y. Fukazawa
S. Funk
W. Gaebele
S. Gabici
A. Gadola
N. Galante
Y. Gallant
B. Garcia
R. J. Garcia Lopez
D. Garrido
L. Garrido
D. Gascon
C. Gasq
M. Gaug
J. Gaweda
N. Geffroy
C. Ghag
A. Ghedina
M. Ghigo
E. Gianakaki
S. Giarrusso
G. Giavitto
B. Giebels
E. Giro
P. Giubilato
T. Glanzman
J. -F. Glicenstein
M. Gochna
V. Golev
M. Gomez Berisso
A. Gonzalez
F. Gonzalez
F. Granena
R. Graciani
J. Granot
R. Gredig
A. Green
T. Greenshaw
O. Grimm
J. Grube
M. Grudzinska
J. Grygorczuk
V. Guarino
L. Guglielmi
F. Guilloux
S. Gunji
G. Gyuk
D. Hadasch
D. Haefner
R. Hagiwara
J. Hahn
A. Hallgren
S. Hara
M. J. Hardcastle
T. Hassan
T. Haubold
M. Hauser
M. Hayashida
R. Heller
G. Henri
G. Hermann
A. Herrero
James Anthony Hinton
D. Hoffmann
W. Hofmann
P. Hofverberg
D. Horns
D. Hrupec
H. Huan
B. Huber
J. -M. Huet
G. Hughes
K. Hultquist
T. B. Humensky
J. -F. Huppert
A. Ibarra
J. M. Illa
J. Ingjald
S. Inoue
Y. Inoue
K. Ioka
C. Jablonski
A. Jacholkowska
M. Janiak
P. Jean
H. Jensen
T. Jogler
I. Jung
P. Kaaret
S. Kabuki
J. Kakuwa
C. Kalkuhl
R. Kankanyan
M. Kapala
A. Karastergiou
M. Karczewski
S. Karkar
N. Karlsson
J. Kasperek
H. Katagiri
K. Katarzynski
N. Kawanaka
B. Kedziora
E. Kendziorra
B. Khelifi
D. Kieda
T. Kifune
T. Kihm
S. Klepser
W. Kluzniak
J. Knapp
A. R. Knappy
T. Kneiske
J. Knoedlseder
F. Koeck
K. Kodani
K. Kohri
K. Kokkotas
N. Komin
A. Konopelko
K. Kosack
R. Kossakowski
P. Kostka
J. Kotula
G. Kowal
J. Koziol
T. Kraehenbuehl
J. Krause
H. Krawczynski
F. Krennrich
A. Kretzschmann
H. Kubo
V. A. Kudryavtsev
J. Kushida
N. La Barbera
V. La Parola
G. La Rosa
A. Lopez
G. Lamanna
P. Laporte
C. Lavalley
T. Le Flour
A. Le Padellec
J. -P. Lenain
L. Lessio
B. Lieunard
E. Lindfors
A. Liolios
T. Lohse
S. Lombardi
A. Lopatin
E. Lorenz
P. Lubinski
O. Luz
E. Lyard
M. C. Maccarone
T. Maccarone
G. Maier
P. Majumdar
S. Maltezos
P. Malkiewicz
C. Mana
A. Manalaysay
G. Maneva
A. Mangano
P. Manigot
J. Marin
M. Mariotti
S. Markoff
G. Martinez
M. Martinez
A. Mastichiadis
H. Matsumoto
S. Mattiazzo
D. Mazin
T. J. L. McComb
N. McCubbin
I. McHardy
C. Medina
D. Melkumyan
A. Mendes
P. Mertsch
M. Meucci
J. Michalowski
P. Micolon
T. Mineo
N. Mirabal
F. Mirabel
J. M. Miranda
R. Mirzoyan
T. Mizuno
B. Moal
R. Moderski
E. Molinari
I. Monteiro
A. Moralejo
C. Morello
K. Mori
G. Motta
F. Mottez
E. Moulin
R. Mukherjee
P. Munar
H. Muraishi
K. Murase
A. Stj. Murphy
S. Nagataki
T. Naito
T. Nakamori
K. Nakayama
C. L. Naumann
D. Naumann
P. Nayman
D. Nedbal
A. Niedzwiecki
J. Niemiec
A. Nikolaidis
K. Nishijima
S. J. Nolan
N. Nowak
P. T. O'Brien
I. Ochoa
Y. Ohira
M. Ohishi
H. Ohka
A. Okumura
C. Olivetto
R. A. Ong
R. Orito
M. Orr
J. P. Osborne
M. Ostrowski
L. Otero
A. N. Otte
E. Ovcharov
I. Oya
A. Ozieblo
S. Paiano
J. Pallota
J. L. Panazol
D. Paneque
M. Panter
R. Paoletti
G. Papyan
J. M. Paredes
G. Pareschi
R. D. Parsons
M. Paz Arribas
G. Pedaletti
A. Pepato
M. Persic
P. O. Petrucci
B. Peyaud
W. Piechocki
S. Pita
G. Pivato
L. Platos
R. Platzer
L. Pogosyan
Martin Pohl
G. Pojmanski
J. D. Ponz
W. Potter
E. Prandini
R. Preece
H. Prokoph
G. Puehlhofer
M. Punch
E. Quel
A. Quirrenbach
P. Rajda
R. Rando
M. Rataj
M. Raue
C. Reimann
O. Reimann
A. Reimer
O. Reimer
M. Renaud
S. Renner
J. -M. Reymond
W. Rhode
M. Ribo
M. Ribordy
J. Rico
F. Rieger
P. Ringegni
J. Ripken
P. Ristori
S. Rivoire
L. Rob
S. Rodriguez
U. Roeser
P. Romano
G. E. Romero
S. Rosier-Lees
A. C. Rovero
F. Roy
S. Royer
B. Rudak
C. B. Rulten
J. Ruppel
F. Russo
F. Ryde
B. Sacco
A. Saggion
V. Sahakian
K. Saito
T. Saito
N. Sakaki
E. Salazar
A. Salini
F. Sanchez
M. A. Sanchez Conde
A. Santangelo
E. M. Santos
A. Sanuy
L. Sapozhnikov
S. Sarkar
V. Scalzotto
V. Scapin
M. Scarcioffolo
T. Schanz
S. Schlenstedt
R. Schlickeiser
T. Schmidt
J. Schmoll
M. Schroedter
C. Schultz
J. Schultze
A. Schulz
U. Schwanke
S. Schwarzburg
T. Schweizer
J. Seiradakis
S. Selmane
K. Seweryn
M. Shayduk
R. C. Shellard
T. Shibata
M. Sikora
J. Silk
A. Sillanpaa
J. Sitarek
C. Skole
N. Smith
D. Sobczynska
M. Sofo Haro
H. Sol
F. Spanier
D. Spiga
S. Spyrou
V. Stamatescu
A. Stamerra
R. L. C. Starling
L. Stawarz
R. Steenkamp
Christian Stegmann
S. Steiner
N. Stergioulas
R. Sternberger
F. Stinzing
M. Stodulski
U. Straumann
A. Suarez
M. Suchenek
R. Sugawara
K. H. Sulanke
S. Sun
A. D. Supanitsky
P. Sutcliffe
M. Szanecki
T. Szepieniec
A. Szostek
A. Szymkowiak
G. Tagliaferri
H. Tajima
H. Takahashi
K. Takahashi
L. Takalo
H. Takami
R. G. Talbot
P. H. Tam
M. Tanaka
T. Tanimori
M. Tavani
J. -P. Tavernet
C. Tchernin
L. A. Tejedor
Igor O. Telezhinsky
P. Temnikov
C. Tenzer
Y. Terada
R. Terrier
M. Teshima
V. Testa
L. Tibaldo
O. Tibolla
M. Tluczykont
C. J. Todero Peixoto
F. Tokanai
M. Tokarz
K. Toma
D. F. Torres
G. Tosti
T. Totani
F. Toussenel
P. Vallania
G. Vallejo
J. van der Walt
C. van Eldik
J. Vandenbroucke
H. Vankov
G. Vasileiadis
V. V. Vassiliev
I. Vegas
L. Venter
S. Vercellone
C. Veyssiere
J. P. Vialle
M. Videla
P. Vincent
J. Vink
N. Vlahakis
L. Vlahos
P. Vogler
A. Vollhardt
F. Volpe
H. P. Von Gunten
S. Vorobiov
S. Wagner
R. M. Wagner
B. Wagner
S. P. Wakely
P. Walter
R. Walter
R. Warwick
P. Wawer
R. Wawrzaszek
N. Webb
P. Wegner
A. Weinstein
Q. Weitzel
R. Welsing
H. Wetteskind
R. White
A. Wierzcholska
M. I. Wilkinson
D. A. Williams
M. Winde
R. Wischnewski
L. Wisniewski
A. Wolczko
M. Wood
Q. Xiong
T. Yamamoto
K. Yamaoka
R. Yamazaki
S. Yanagita
B. Yoffo
M. Yonetani
A. Yoshida
T. Yoshida
T. Yoshikoshi
V. Zabalza
A. Zagdanski
A. Zajczyk
A. Zdziarski
Alraune Zech
K. Zietara
P. Ziolkowski
V. Zitelli
P. Zychowski
eng
uncontrolled
Ground based gamma ray astronomy
eng
uncontrolled
Next generation Cherenkov telescopes
eng
uncontrolled
Design concepts
Institut für Physik und Astronomie
Referiert
35161
2013
2013
eng
3
18
16
2
43
preprint
Elsevier
Amsterdam
CTA Consortium
1
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Introducing the CTA concept
The Cherenkov Telescope Array (CTA) is a new observatory for very high-energy (VHE) gamma rays. CTA has ambitions science goals, for which it is necessary to achieve full-sky coverage, to improve the sensitivity by about an order of magnitude, to span about four decades of energy, from a few tens of GeV to above 100 TeV with enhanced angular and energy resolutions over existing VHE gamma-ray observatories. An international collaboration has formed with more than 1000 members from 27 countries in Europe, Asia, Africa and North and South America. In 2010 the CTA Consortium completed a Design Study and started a three-year Preparatory Phase which leads to production readiness of CTA in 2014. In this paper we introduce the science goals and the concept of CTA, and provide an overview of the project.
Astroparticle physics
10.1016/j.astropartphys.2013.01.007
0927-6505
1873-2852
wos:2011-2013
WOS:000318126800002
Martinez, M (reprint author), Inst Fis Altes Energies, Barcelona, Spain., martinez@ifae.es
B. S. Acharya
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T. Aghajani
G. Agnetta
J. Aguilar
Felix A. Aharonian
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A. G. Akhperjanian
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I. Allekotte
E. Amato
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A. Aravantinos
T. Arlen
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H. Arnaldi
L. Arrabito
K. Asano
T. Ashton
H. G. Asorey
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A. Babic
N. Baby
J. Baehr
A. Bais
C. Baixeras
S. Bajtlik
M. Balbo
D. Balis
C. Balkowski
A. Bamba
R. Bandiera
A. Barber
C. Barbier
M. Barcelo
Anna Barnacka
Jürgen Barnstedt
U. Barres de Almeida
J. A. Barrio
A. Basili
S. Basso
D. Bastieri
C. Bauer
Anton N. Baushev
J. Becerra Gonzalez
Yvonne Becherini
K. C. Bechtol
J. Becker Tjus
Volker Beckmann
W. Bednarek
B. Behera
M. Belluso
W. Benbow
J. Berdugo
K. Berger
F. Bernard
T. Bernardino
K. Bernlöhr
N. Bhat
S. Bhattacharyya
C. Bigongiari
A. Biland
S. Billotta
T. Bird
E. Birsin
E. Bissaldi
Jonathan Biteau
M. Bitossi
S. Blake
O. Blanch Bigas
P. Blasi
A. A. Bobkov
V. Boccone
Markus Boettcher
L. Bogacz
J. Bogart
M. Bogdan
Catherine Boisson
J. Boix Gargallo
J. Bolmont
G. Bonanno
A. Bonardi
T. Bonev
P. Bonifacio
G. Bonnoli
Pol Bordas
A. W. Borgland
Janett Borkowski
R. Bose
O. Botner
A. Bottani
L. Bouchet
M. Bourgeat
C. Boutonnet
A. Bouvier
S. Brau-Nogue
I. Braun
T. Bretz
M. S. Briggs
T. Bringmann
P. Brook
Pierre Brun
L. Brunetti
T. Buanes
J. H. Buckley
R. Buehler
V. Bugaev
A. Bulgarelli
Tomasz Bulik
G. Busetto
S. Buson
K. Byrum
M. Cailles
R. A. Cameron
J. Camprecios
R. Canestrari
S. Cantu
M. Capalbi
P. A. Caraveo
E. Carmona
A. Carosi
John Carr
P. H. Carton
Sabrina Casanova
M. Casiraghi
O. Catalano
S. Cavazzani
S. Cazaux
M. Cerruti
E. Chabanne
Paula M. Chadwick
C. Champion
Andrew Chen
J. Chiang
L. Chiappetti
M. Chikawa
V. R. Chitnis
F. Chollet
J. Chudoba
M. Cieslar
A. N. Cillis
J. Cohen-Tanugi
Sergio Colafrancesco
P. Colin
J. Calome
S. Colonges
M. Compin
P. Conconi
V. Conforti
V. Connaughton
Jan Conrad
J. L. Contreras
P. Coppi
P. Corona
D. Corti
J. Cortina
L. Cossio
H. Costantini
G. Cotter
B. Courty
S. Couturier
S. Covino
G. Crimi
S. J. Criswell
J. Croston
G. Cusumano
M. Dafonseca
O. Dale
M. Daniel
J. Darling
I. Davids
F. Dazzi
A. De Angelis
V. De Caprio
F. De Frondat
E. M. de Gouveia Dal Pino
I. de la Calle
G. A. De La Vega
R. de los Reyes Lopez
B. De Lotto
A. De Luca
J. R. T. de Mello Neto
M. de Naurois
Y. de Oliveira
E. de Ona Wilhelmi
V. de Souza
G. Decerprit
G. Decock
C. Deil
E. Delagnes
G. Deleglise
C. Delgado
D. Della Volpe
P. Demange
G. Depaola
A. Dettlaff
A. Di Paola
F. Di Pierro
C. Diaz
J. Dick
R. Dickherber
H. Dickinson
V. Diez-Blanco
S. Digel
D. Dimitrov
G. Disset
A. Djannati-Ataï
M. Doert
M. Dohmke
W. Domainko
Dijana Dominis Prester
A. Donat
D. Dorner
M. Doro
J-L. Dournaux
G. Drake
D. Dravins
L. Drury
F. Dubois
R. Dubois
G. Dubus
C. Dufour
D. Dumas
J. Dumm
D. Durand
J. Dyks
M. Dyrda
J. Ebr
E. Edy
Kathrin Egberts
P. Eger
S. Einecke
C. Eleftheriadis
S. Elles
D. Emmanoulopoulos
D. Engelhaupt
R. Enomoto
J-P Ernenwein
M. Errando
A. Etchegoyen
P. Evans
A. Falcone
D. Fantinel
K. Farakos
C. Farnier
G. Fasola
B. Favill
E. Fede
S. Federici
S. Fegan
F. Feinstein
D. Ferenc
P. Ferrando
M. Fesquet
A. Fiasson
E. Fillin-Martino
D. Fink
C. Finley
J. P. Finley
M. Fiorini
R. Firpo Curcoll
H. Flores
D. Florin
W. Focke
C. Foehr
E. Fokitis
L. Font
G. Fontaine
M. Fornasa
A. Foerster
L. Fortson
N. Fouque
A. Franckowiak
C. Fransson
G. Fraser
R. Frei
I. F. M. Albuquerque
L. Fresnillo
C. Fruck
Y. Fujita
Y. Fukazawa
Y. Fukui
S. Funk
W. Gaebele
S. Gabici
R. Gabriele
A. Gadola
N. Galante
D. Gall
Y. Gallant
J. Gamez-Garcia
B. Garcia
R. Garcia Lopez
D. Gardiol
D. Garrido
L. Garrido
D. Gascon
M. Gaug
J. Gaweda
L. Gebremedhin
N. Geffroy
L. Gerard
A. Ghedina
M. Ghigo
E. Giannakaki
F. Gianotti
S. Giarrusso
G. Giavitto
B. Giebels
V. Gika
P. Giommi
N. Girard
E. Giro
A. Giuliani
T. Glanzman
J. -F. Glicenstein
N. Godinovic
V. Golev
M. Gomez Berisso
J. Gomez-Ortega
M. M. Gonzalez
A. Gonzalez
F. Gonzalez
A. Gonzalez Munoz
K. S. Gothe
M. Gougerot
R. Graciani
P. Grandi
F. Granena
J. Granot
G. Grasseau
R. Gredig
A. Green
T. Greenshaw
T. Gregoire
O. Grimm
J. Grube
M. Grudzinska
V. Gruev
S. Gruenewald
J. Grygorczuk
V. Guarino
S. Gunji
G. Gyuk
D. Hadasch
R. Hagiwara
J. Hahn
N. Hakansson
A. Hallgren
N. Hamer Heras
S. Hara
M. J. Hardcastle
J. Harris
T. Hassan
K. Hatanaka
T. Haubold
A. Haupt
T. Hayakawa
M. Hayashida
R. Heller
F. Henault
G. Henri
G. Hermann
R. Hermel
A. Herrero
N. Hidaka
J. Hinton
D. Hoffmann
W. Hofmann
P. Hofverberg
J. Holder
D. Horns
D. Horville
J. Houles
M. Hrabovsky
D. Hrupec
H. Huan
B. Huber
J. -M. Huet
G. Hughes
T. B. Humensky
J. Huovelin
A. Ibarra
J. M. Illa
D. Impiombato
S. Incorvaia
S. Inoue
Y. Inoue
K. Ioka
E. Ismailova
C. Jablonski
A. Jacholkowska
M. Jamrozy
M. Janiak
P. Jean
C. Jeanney
J. J. Jimenez
T. Jogler
T. Johnson
L. Journet
C. Juffroy
I. Jung
P. Kaaret
S. Kabuki
M. Kagaya
J. Kakuwa
C. Kalkuhl
R. Kankanyan
A. Karastergiou
K. Kaercher
M. Karczewski
S. Karkar
Aci. Kasperek
D. Kastana
H. Katagiri
J. Kataoka
K. Katarzynski
U. Katz
N. Kawanaka
B. Kellner-Leidel
H. Kelly
E. Kendziorra
B. Khelifi
D. B. Kieda
T. Kifune
T. Kihm
T. Kishimoto
K. Kitamoto
W. Kluzniak
C. Knapic
J. w Knapp
J. Knoedlseder
F. Koeck
J. Kocot
K. Kodani
J. -H. Koehne
K. Kohri
K. Kokkotas
D. Kolitzus
N. Komin
I. Kominis
Y. Konno
H. Koeppel
P. Korohoda
K. Kosack
G. Koss
R. Kossakowski
P. Kostka
R. Koul
G. Kowal
S. Koyama
J. Koziol
T. Kraehenbuehl
J. Krause
H. Krawzcynski
F. Krennrich
A. Krepps
A. Kretzschmann
R. Krobot
P. Krueger
H. Kubo
V. A. Kudryavtsev
J. Kushida
A. Kuznetsov
A. La Barbera
N. La Palombara
V. La Parola
G. La Rosa
K. Lacombe
G. Lamanna
J. Lande
D. Languignon
J. Lapington
P. Laporte
C. Lavalley
T. Le Flour
A. Le Padellec
S. -H. Lee
W. H. Lee
M. A. Leigui de Oliveira
D. Lelas
J. -P. Lenain
D. J. Leopold
T. Lerch
L. Lessio
B. Lieunard
E. Lindfors
A. Liolios
A. Lipniacka
H. Lockart
T. Lohse
S. Lombardi
A. Lopatin
M. Lopez
R. Lopez-Coto
A. Lopez-Oramas
A. Lorca
E. Lorenz
P. Lubinski
F. Lucarelli
H. Luedecke
J. Ludwin
P. L. Luque-Escamilla
W. Lustermann
O. Luz
E. Lyard
M. C. Maccarone
T. J. Maccarone
G. M. Madejski
A. Madhavan
M. Mahabir
G. Maier
P. Majumdar
G. Malaguti
S. Maltezos
A. Manalaysay
A. Mancilla
D. Mandat
G. Maneva
A. Mangano
P. Manigot
K. Mannheim
I. Manthos
N. Maragos
A. Marcowith
M. Mariotti
M. Marisaldi
S. Markoff
A. Marszalek
C. Martens
J. Marti
J-M. Martin
P. Martin
G. Martinez
F. Martinez
M. Martinez
A. Masserot
A. Mastichiadis
A. Mathieu
H. Matsumoto
F. Mattana
S. Mattiazzo
G. Maurin
S. Maxfield
J. Maya
D. Mazin
L. Mc Comb
N. McCubbin
I. McHardy
R. McKay
C. Medina
C. Melioli
D. Melkumyan
S. Mereghetti
P. Mertsch
M. Meucci
J. Michalowski
P. Micolon
A. Mihailidis
T. Mineo
M. Minuti
N. Mirabal
F. Mirabel
J. M. Miranda
R. Mirzoyan
T. Mizuno
B. Moal
R. Moderski
I. Mognet
E. Molinari
M. Molinaro
T. Montaruli
I. Monteiro
P. Moore
A. Moralejo Olaizola
M. Mordalska
C. Morello
K. Mori
F. Mottez
Y. Moudden
E. Moulin
I. Mrusek
R. Mukherjee
P. Munar-Adrover
H. Muraishi
K. Murase
A. Murphy
S. Nagataki
T. Naito
D. Nakajima
T. Nakamori
K. Nakayama
C. L. Naumann
D. Naumann
M. Naumann-Godo
P. Nayman
D. Nedbal
D. Neise
L. Nellen
V. Neustroev
N. Neyroud
L. Nicastro
J. Nicolau-Kuklinski
A. Niedzwiecki
J. Niemiec
D. Nieto
A. Nikolaidis
K. Nishijima
S. Nolan
R. Northrop
D. Nosek
N. Nowak
A. Nozato
P. O'Brien
Y. Ohira
M. Ohishi
S. Ohm
H. Ohoka
T. Okuda
A. Okumura
J. -F. Olive
R. A. Ong
R. Orito
M. Orr
J. Osborne
M. Ostrowski
L. A. Otero
N. Otte
E. Ovcharov
I. Oya
A. Ozieblo
L. Padilla
S. Paiano
D. Paillot
A. Paizis
S. Palanque
M. Palatka
J. Pallota
K. Panagiotidis
J. -L. Panazol
D. Paneque
M. Panter
R. Paoletti
Alexandros Papayannis
G. Papyan
J. M. Paredes
G. Pareschi
G. Parks
J. -M. Parraud
D. Parsons
M. Paz Arribas
M. Pech
G. Pedaletti
V. Pelassa
D. Pelat
M. D. C. Perez
M. Persic
P-O Petrucci
B. Peyaud
A. Pichel
S. Pita
F. Pizzolato
L. Platos
R. Platzer
L. Pogosyan
M. Pohl
G. Pojmanski
J. D. Ponz
W. Potter
J. Poutanen
E. Prandini
J. Prast
R. Preece
F. Profeti
H. Prokoph
M. Prouza
M. Proyetti
I. Puerto-Gimenez
G. Puehlhofer
I. Puljak
M. Punch
R. Pyziol
E. J. Quel
J. Quinn
A. Quirrenbach
E. Racero
P. J. Rajda
P. Ramon
R. Rando
R. C. Rannot
M. Rataj
M. Raue
P. Reardon
O. Reimann
A. Reimer
O. Reimer
K. Reitberger
M. Renaud
S. Renner
B. Reville
W. Rhode
M. Ribo
M. Ribordy
M. G. Richer
J. Rico
J. Ridky
F. Rieger
P. Ringegni
J. Ripken
P. R. Ristori
A. Riviere
S. Rivoire
L. Rob
U. Roeser
R. Rohlfs
G. Rojas
P. Romano
W. Romaszkan
G. E. Romero
S. Rosen
S. Rosier Lees
D. Ross
G. Rouaix
J. Rousselle
S. Rousselle
A. C. Rovero
F. Roy
S. Royer
B. Rudak
C. Rulten
M. Rupinski
F. Russo
F. Ryde
B. Sacco
E. O. Saemann
A. Saggion
V. Safiakian
K. Saito
T. Saito
Y. Saito
N. Sakaki
R. Sakonaka
A. Salini
F. Sanchez
M. Sanchez-Conde
A. Sandoval
H. Sandaker
E. Sant'Ambrogio
A. Santangelo
E. M. Santos
A. Sanuy
L. Sapozhnikov
S. Sarkar
N. Sartore
H. Sasaki
K. Satalecka
M. Sawada
V. Scalzotto
V. Scapin
M. Scarcioffolo
J. Schafer
T. Schanz
S. Schlenstedt
R. Schlickeiser
T. Schmidt
J. Schmoll
P. Schovanek
M. Schroedter
C. Schultz
J. Schultze
A. Schulz
K. Schure
T. Schwab
U. Schwanke
J. Schwarz
S. Schwarzburg
T. Schweizer
S. Schwemmer
A. Segreto
J. -H. Seiradakis
G. H. Sembroski
K. Seweryn
M. Sharma
M. Shayduk
R. C. Shellard
J. Shi
T. Shibata
A. Shibuya
E. Shum
L. Sidoli
M. Sidz
J. Sieiro
M. Sikora
J. Silk
A. Sillanpaa
B. B. Singh
J. Sitarek
C. Skole
R. Smareglia
A. Smith
D. Smith
J. Smith
N. Smith
D. Sobczynska
H. Sol
G. Sottile
M. Sowinski
F. Spanier
D. Spiga
S. Spyrou
V. Stamatescu
A. Stamerra
R. Starling
L. Stawarz
R. Steenkamp
Christian Stegmann
S. Steiner
N. Stergioulas
R. Sternberger
M. Sterzel
F. Stinzing
M. Stodulski
U. Straumann
E. Strazzeri
L. Stringhetti
A. Suarez
M. Suchenek
R. Sugawara
K. -H. Sulanke
S. Sun
A. D. Supanitsky
T. Suric
P. Sutcliffe
J. Sykes
M. Szanecki
T. Szepieniec
A. Szostek
G. Tagliaferri
H. Tajima
H. Takahashi
K. Takahashi
L. Takalo
H. Takami
C. Talbot
J. Tammi
M. Tanaka
S. Tanaka
J. Tasan
M. Tavani
J. -P. Tavernet
L. A. Tejedor
Igor O. Telezhinsky
P. Temnikov
C. Tenzer
Y. Terada
R. Terrier
M. Teshima
V. Testa
D. Tezier
D. Thuermann
L. Tibaldo
O. Tibolla
A. Tiengo
M. Tluczykont
C. J. Todero Peixoto
F. Tokanai
M. Tokarz
K. Toma
K. Torii
M. Tornikoski
D. F. Torres
M. Torres
G. Tosti
T. Totani
C. Toussenel
G. Tovmassian
P. Travnicek
M. Trifoglio
I. Troyano
K. Tsinganos
H. Ueno
K. Umehara
S. S. Upadhya
T. Usher
M. Uslenghi
J. F. Valdes-Galicia
P. Vallania
G. Vallejo
W. van Driel
C. van Eldik
J. Vandenbrouke
J. Vanderwalt
H. Vankov
G. Vasileiadis
V. Vassiliev
D. Veberic
I. Vegas
S. Vercellone
S. Vergani
C. Veyssiere
J. P. Vialle
A. Viana
M. Videla
P. Vincent
S. Vincent
J. Vink
N. Vlahakis
L. Vlahos
P. Vogler
A. Vollhardt
H. P. von Gunten
S. Vorobiov
C. Vuerli
V. Waegebaert
R. Wagner
R. G. Wagner
S. Wagner
S. P. Wakely
R. Walter
T. Walther
K. Warda
R. Warwick
P. Wawer
R. Wawrzaszek
N. Webb
P. Wegner
A. Weinstein
Q. Weitzel
R. Welsing
M. Werner
H. Wetteskind
R. White
A. Wierzcholska
S. Wiesand
M. Wilkinson
D. A. Williams
R. Willingale
K. Winiarski
R. Wischnewski
L. Wisniewski
M. Wood
A. Woernlein
Q. Xiong
K. K. Yadav
H. Yamamoto
T. Yamamoto
R. Yamazaki
S. Yanagita
J. M. Yebras
D. Yelos
A. Yoshida
T. Yoshida
T. Yoshikoshi
V. Zabalza
M. Zacharias
A. Zajczyk
R. Zanin
A. Zdziarski
Alraune Zech
A. Zhao
X. Zhou
K. Zietara
J. Ziolkowski
P. Ziolkowski
V. Zitelli
C. Zurbach
P. Zychowski
eng
uncontrolled
TeV gamma-ray astronomy
eng
uncontrolled
Air showers
eng
uncontrolled
Cherenkov Telescopes
Institut für Physik und Astronomie
Referiert
35105
2013
2013
eng
14
4
552
article
EDP SCIENCES S A
LES ULIS CEDEX A
HESS Collaboration
1
--
--
--
Discovery of TeV gamma-ray emission from PKS 0447-439 and derivation of
an upper limit on its redshift
Very high-energy gamma-ray emission from PKS 0447-439 was detected with the H. E. S. S. Cherenkov telescope array in December 2009. This blazar is one of the brightest extragalactic objects in the Fermi bright source list and has a hard spectrum in the MeV to GeV range. In the TeV range, a photon index of 3.89 +/- 0.37 (stat) +/- 0.22 (sys) and a flux normalisation at 1 TeV, phi(1) (TeV) = (3.5 +/- 1.1(stat) +/- 0.9(sys)) x 10(-13) cm(-2) s(-1) TeV-1 were found. The detection with H. E. S. S. triggered observations in the X-ray band with the Swift and RXTE telescopes. Simultaneous UV and optical data from Swift UVOT and data from the optical telescopes ATOM and ROTSE are also available. The spectrum and light curve measured with H. E. S. S. are presented and compared to the multi-wavelength data at lower energies. A rapid flare is seen in the Swift XRT and RXTE data, together with a flux variation in the UV band, at a time scale of the order of one day. A firm upper limit of z < 0.59 on the redshift of PKS 0447-439 is derived from the combined Fermi-LAT and H. E. S. S. data, given the assumptions that there is no upturn in the intrinsic spectrum above the Fermi-LAT energy range and that absorption on the extragalactic background light (EBL) is not weaker than the lower limit provided by current models. The spectral energy distribution is well described by a simple one-zone synchrotron self-Compton scenario, if the redshift of the source is less than z less than or similar to 0.4.
ASTRONOMY & ASTROPHYSICS
10.1051/0004-6361/201321108
0004-6361
wos:2011-2013
A118
WOS:000317912000117
Zech, A (reprint author), Univ Paris Diderot, CNRS, Observ Paris, LUTH, 5 Pl Jules Janssen, F-92190 Meudon, France.
, Bagmeet.Behera@desy.de; Andreas.Zech@obspm.fr
Attila Abramowski
F. Acero
A. G. Akhperjanian
Gisela Anton
Shangkari Balenderan
Arnim Balzer
Anna Barnacka
Yvonne Becherini
J. Becker Tjus
B. Behera
K. Bernlöhr
E. Birsin
Jonathan Biteau
A. Bochow
Catherine Boisson
J. Bolmont
Pol Bordas
J. Brucker
Francois Brun
Pierre Brun
Tomasz Bulik
Svenja Carrigan
Sabrina Casanova
M. Cerruti
Paula M. Chadwick
Ryan C. G. Chaves
A. Cheesebrough
Sergio Colafrancesco
Gabriele Cologna
Jan Conrad
C. Couturier
M. Dalton
M. K. Daniel
I. D. Davids
B. Degrange
C. Deil
P. deWilt
H. J. Dickinson
A. Djannati-Ataï
W. Domainko
L. O&rsquo Drury
C.
G. Dubus
K. Dutson
J. Dyks
M. Dyrda
Kathrin Egberts
P. Eger
P. Espigat
L. Fallon
C. Farnier
S. Fegan
F. Feinstein
M. V. Fernandes
D. Fernandez
A. Fiasson
G. Fontaine
A. Foerster
Matthias Fussling
M. Gajdus
Y. A. Gallant
T. Garrigoux
H. Gast
B. Giebels
J. F. Glicenstein
B. Glueck
D. Goering
M. -H. Grondin
M. Grudzinska
S. Haeffner
J. D. Hague
J. Hahn
D. Hampf
J. Harris
S. Heinz
G. Heinzelmann
G. Henri
G. Hermann
A. Hillert
James Anthony Hinton
W. Hofmann
P. Hofverberg
M. Holler
D. Horns
A. Jacholkowska
C. Jahn
M. Jamrozy
I. Jung
M. A. Kastendieck
K. Katarzynski
U. Katz
S. Kaufmann
B. Khelifi
S. Klepser
D. Klochkov
W. Kluzniak
T. Kneiske
D. Kolitzus
Nu Komin
K. Kosack
R. Kossakowski
F. Krayzel
P. P. Krueger
H. Laffon
G. Lamanna
J. Lefaucheur
M. Lemoine-Goumard
J. -P. Lenain
D. Lennarz
T. Lohse
A. Lopatin
C. -C. Lu
V. Marandon
A. Marcowith
J. Masbou
G. Maurin
N. Maxted
M. Mayer
T. J. L. McComb
M. C. Medina
J. Mehault
U. Menzler
R. Moderski
M. Mohamed
E. Moulin
C. L. Naumann
M. Naumann-Godo
M. de Naurois
D. Nedbal
N. Nguyen
J. Niemiec
S. J. Nolan
S. Ohm
E. de Ona Wilhelmi
B. Opitz
M. Ostrowski
I. Oya
M. Panter
R. D. Parsons
M. Paz Arribas
N. W. Pekeur
G. Pelletier
J. Perez
P. -O. Petrucci
B. Peyaud
S. Pita
G. Puehlhofer
M. Punch
A. Quirrenbach
S. Raab
M. Raue
A. Reimer
O. Reimer
M. Renaud
R. de los Reyes
F. Rieger
J. Ripken
L. Rob
S. Rosier-Lees
G. Rowell
B. Rudak
C. B. Rulten
V. Sahakian
David M. Sanchez
A. Santangelo
R. Schlickeiser
A. Schulz
U. Schwanke
S. Schwarzburg
S. Schwemmer
F. Sheidaei
J. L. Skilton
H. Sol
G. Spengler
L. Stawarz
R. Steenkamp
Christian Stegmann
F. Stinzing
K. Stycz
Iurii Sushch
A. Szostek
J. -P. Tavernet
R. Terrier
M. Tluczykont
C. Trichard
K. Valerius
C. van Eldik
G. Vasileiadis
C. Venter
A. Viana
P. Vincent
H. J. Voelk
F. Volpe
S. Vorobiov
M. Vorster
S. J. Wagner
M. Ward
R. White
A. Wierzcholska
D. Wouters
M. Zacharias
A. Zajczyk
A. A. Zdziarski
Alraune Zech
H. -S. Zechlin
D. Pelat
eng
uncontrolled
galaxies: active
eng
uncontrolled
BL Lacertae objects: individual: PKS 0447-439
eng
uncontrolled
radiation mechanisms: non-thermal
eng
uncontrolled
gamma rays: galaxies
34578
2013
2013
eng
12
10
88
article
American Physical Society
College Park
HESS Collaboration
1
--
--
--
Constraints on axionlike particles with HESS from the irregularity of the PKS 2155-304 energy spectrum
Axionlike particles (ALPs) are hypothetical light (sub-eV) bosons predicted in some extensions of the Standard Model of particle physics. In astrophysical environments comprising high-energy gamma rays and turbulent magnetic fields, the existence of ALPs can modify the energy spectrum of the gamma rays for a sufficiently large coupling between ALPs and photons. This modification would take the form of an irregular behavior of the energy spectrum in a limited energy range. Data from the H. E. S. S. observations of the distant BL Lac object PKS 2155 - 304 (z = 0.116) are used to derive upper limits at the 95% C. L. on the strength of the ALP coupling to photons, g(gamma a) < 2.1 x 10(-11) GeV-1 for an ALP mass between 15 and 60 neV. The results depend on assumptions on the magnetic field around the source, which are chosen conservatively. The derived constraints apply to both light pseudoscalar and scalar bosons that couple to the electromagnetic field.
Physical review : D, Particles, fields, gravitation, and cosmology
10.1103/PhysRevD.88.102003
1550-7998
1550-2368
wos:2011-2013
102003
WOS:000327214000001
Abramowski, A (reprint author), Univ Hamburg, Inst Expt Phys, Luruper Chaussee 149, D-27761 Hamburg, Germany., pierre.brun@cea.fr; denis.wouters@cea.fr
German Ministry for Education and Research (BMBF); Max Planck Society;
German Research Foundation (DFG); French Ministry for Research;
CNRS-IN2P3; Astroparticle Interdisciplinary Program of the CNRS; United
Kingdom Science and Technology Facilities Council (STFC); IPNP of the
Charles University; Czech Science Foundation; Polish Ministry of Science
and Higher Education; South African Department of Science and
Technology; National Research Foundation; University of Namibia;
European Community [ERC-StG-259391]
Attila Abramowski
F. Acero
Felix A. Aharonian
Faical Ait Benkhali
A. G. Akhperjanian
Ekrem Oǧuzhan Angüner
Gisela Anton
Shangkari Balenderan
Arnim Balzer
Anna Barnacka
Yvonne Becherini
J. Becker Tjus
K. Bernlöhr
E. Birsin
E. Bissaldi
Jonathan Biteau
Catherine Boisson
J. Bolmont
Pol Bordas
J. Brucker
Francois Brun
Pierre Brun
Tomasz Bulik
Svenja Carrigan
Sabrina Casanova
M. Cerruti
Paula M. Chadwick
R. Chalme-Calvet
Ryan C. G. Chaves
A. Cheesebrough
M. Chretien
Sergio Colafrancesco
Gabriele Cologna
Jan Conrad
C. Couturier
M. Dalton
M. K. Daniel
I. D. Davids
B. Degrange
C. Deil
P. deWilt
H. J. Dickinson
A. Djannati-Ataï
W. Domainko
L. O'C. Drury
G. Dubus
K. Dutson
J. Dyks
M. Dyrda
T. Edwards
Kathrin Egberts
P. Eger
P. Espigat
C. Farnier
S. Fegan
F. Feinstein
M. V. Fernandes
D. Fernandez
A. Fiasson
G. Fontaine
A. Foerster
M. Fuessling
M. Gajdus
Y. A. Gallant
T. Garrigoux
H. Gast
B. Giebels
J. F. Glicenstein
D. Goering
M. -H. Grondin
M. Grudzinska
S. Haeffner
J. D. Hague
J. Hahn
J. Harris
G. Heinzelmann
G. Henri
G. Hermann
O. Hervet
A. Hillert
James Anthony Hinton
W. Hofmann
P. Hofverberg
Markus Holler
D. Horns
A. Jacholkowska
C. Jahn
M. Jamrozy
M. Janiak
F. Jankowsky
I. Jung
M. A. Kastendieck
K. Katarzynski
U. Katz
S. Kaufmann
B. Khelifi
M. Kieffer
S. Klepser
D. Klochkov
W. Kluzniak
T. Kneiske
D. Kolitzus
Nu. Komin
K. Kosack
S. Krakau
F. Krayzel
P. P. Krueger
H. Laffon
G. Lamanna
J. Lefaucheur
M. Lemoine-Goumard
J-P. Lenain
D. Lennarz
T. Lohse
A. Lopatin
C-C. Lu
V. Marandon
A. Marcowith
R. Marx
G. Maurin
N. Maxted
M. Mayer
T. J. L. McComb
M. C. Medina
J. Mehault
U. Menzler
M. Meyer
R. Moderski
M. Mohamed
E. Moulin
T. Murach
C. L. Naumann
M. de Naurois
D. Nedbal
J. Niemiec
S. J. Nolan
L. Oakes
S. Ohm
E. de Ona Wilhelmi
B. Opitz
M. Ostrowski
I. Oya
M. Panter
R. D. Parsons
M. Paz Arribas
N. W. Pekeur
G. Pelletier
J. Perez
P-O. Petrucci
B. Peyaud
S. Pita
H. Poon
G. Puehlhofer
M. Punch
A. Quirrenbach
S. Raab
M. Raue
A. Reimer
O. Reimer
M. Renaud
R. de los Reyes
F. Rieger
L. Rob
S. Rosier-Lees
G. Rowell
B. Rudak
C. B. Rulten
V. Sahakian
David M. Sanchez
A. Santangelo
R. Schlickeiser
F. Schuessler
A. Schulz
U. Schwanke
S. Schwarzburg
S. Schwemmer
H. Sol
G. Spengler
F. Spiess
L. Stawarz
R. Steenkamp
Christian Stegmann
F. Stinzing
K. Stycz
Iurii Sushch
A. Szostek
J-P. Tavernet
R. Terrier
M. Tluczykont
C. Trichard
K. Valerius
C. van Eldik
G. Vasileiadis
C. Venter
A. Viana
P. Vincent
H. J. Voelk
F. Volpe
M. Vorster
S. J. Wagner
P. Wagner
M. Ward
M. Weidinger
Q. Weitzel
R. White
A. Wierzcholska
P. Willmann
A. Woernlein
D. Wouters
M. Zacharias
A. Zajczyk
A. A. Zdziarski
Alraune Zech
H-S. Zechlin
Institut für Physik und Astronomie
Referiert
34607
2013
2013
eng
11
559
article
EDP SCIENCES S A
LES ULIS CEDEX A
HESS Collaboration
1
--
--
--
Discovery of very high energy gamma-ray emission from the BL Lacertae
object PKS0301-243 with HESS
The active galactic nucleus PKS 0301-243 (z = 0.266) is a high-synchrotron-peaked BL Lac object that is detected at high energies (HE, 100 MeV < E < 100 GeV) by Fermi/LAT. This paper reports on the discovery of PKS 0301-243 at very high energies (E > 100 GeV) by the High Energy Stereoscopic System (H.E.S.S.) from observations between September 2009 and December 2011 for a total live time of 34.9 h. Gamma rays above 200 GeV are detected at a significance of 9.4 sigma. A hint of variability at the 2.5 sigma level is found. An integral flux I(E > 200GeV) = (3.3 +/- 1.1(stat) +/- 0.7(syst)) x 10(-12) ph cm(-2) s(-1) and a photon index Gamma = 4.6 +/- 0.7(stat) +/- 0.2(syst) are measured. Multi-wavelength light curves in HE, X-ray and optical bands show strong variability, and a minimal variability timescale of eight days is estimated from the optical light curve. A single-zone leptonic synchrotron self-Compton scenario satisfactorily reproduces the multi-wavelength data. In this model, the emitting region is out of equipartition and the jet is particle dominated. Because of its high redshift compared to other sources observed at TeV energies, the very high energy emission from PKS 0301-243 is attenuated by the extragalactic background light (EBL) and the measured spectrum is used to derive an upper limit on the opacity of the EBL.
ASTRONOMY & ASTROPHYSICS
10.1051/0004-6361/201321639
0004-6361
1432-0746
wos:2011-2013
A136
WOS:000327847200136
Wouters, D (reprint author), CEA Saclay, DSM Irfu, F-91191 Gif Sur Yvette, France.
, jlenain@lpnhe.in2p3.fr; denis.wouters@cea.fr
German Ministry for Education and Research (BMBF); Max Planck Society;
German Research Foundation (DFG); French Ministry for Research;
CNRS-IN2P3; Astroparticle Interdisciplinary Programme of the CNRS; U.K.
Science and Technology Facilities Council (STFC); IPNP of the Charles
University; Czech Science Foundation; Polish Ministry of Science and
Higher Education; South African Department of Science and Technology;
National Research Foundation; University of Namibia
Attila Abramowski
F. Acero
Felix A. Aharonian
Faical Ait Benkhali
A. G. Akhperjanian
Ekrem Oǧuzhan Angüner
Gisela Anton
Shangkari Balenderan
Arnim Balzer
Anna Barnacka
Yvonne Becherini
J. Becker Tjus
K. Bernlöhr
E. Birsin
E. Bissaldi
Jonathan Biteau
Markus Boettcher
Catherine Boisson
J. Bolmont
Pol Bordas
J. Brucker
Francois Brun
Pierre Brun
Tomasz Bulik
Svenja Carrigan
Sabrina Casanova
M. Cerruti
Paula M. Chadwick
R. Chalme-Calvet
Ryan C. G. Chaves
A. Cheesebrough
M. Chretien
Sergio Colafrancesco
Gabriele Cologna
Jan Conrad
C. Couturier
M. Dalton
M. K. Daniel
I. D. Davids
B. Degrange
C. Deil
P. deWilt
H. J. Dickinson
A. Djannati-Ataï
W. Domainko
L. O&rsquo Drury
C.
G. Dubus
K. Dutson
J. Dyks
M. Dyrda
T. Edwards
Kathrin Egberts
P. Eger
P. Espigat
C. Farnier
S. Fegan
F. Feinstein
M. V. Fernandes
D. Fernandez
A. Fiasson
G. Fontaine
A. Foerster
M. Fuessling
M. Gajdus
Y. A. Gallant
T. Garrigoux
B. Giebels
J. F. Glicenstein
M. -H. Grondin
M. Grudzinska
S. Haeffner
J. D. Hague
J. Hahn
J. Harris
G. Heinzelmann
G. Henri
G. Hermann
O. Hervet
A. Hillert
James Anthony Hinton
W. Hofmann
P. Hofverberg
M. Holler
D. Horns
A. Jacholkowska
C. Jahn
M. Jamrozy
M. Janiak
F. Jankowsky
I. Jung
M. A. Kastendieck
K. Katarzynski
U. Katz
S. Kaufmann
B. Khelifi
M. Kieffer
S. Klepser
D. Klochkov
W. Kluzniak
T. Kneiske
D. Kolitzus
Nu. Komin
K. Kosack
S. Krakau
F. Krayzel
P. P. Krueger
H. Laffon
G. Lamanna
J. Lefaucheur
M. Lemoine-Goumard
J. -P. Lenain
D. Lennarz
T. Lohse
A. Lopatin
C. -C. Lu
V. Marandon
A. Marcowith
R. Marx
G. Maurin
N. Maxted
M. Mayer
T. J. L. McComb
M. C. Medina
J. Mehault
U. Menzler
M. Meyer
R. Moderski
M. Mohamed
E. Moulin
T. Murach
C. L. Naumann
M. de Naurois
D. Nedbal
J. Niemiec
S. J. Nolan
L. Oakes
S. Ohm
E. de Ona Wilhelmi
B. Opitz
M. Ostrowski
I. Oya
M. Panter
R. D. Parsons
M. Paz Arribas
N. W. Pekeur
G. Pelletier
J. Perez
P. -O. Petrucci
B. Peyaud
S. Pita
H. Poon
G. Puehlhofer
M. Punch
A. Quirrenbach
S. Raab
M. Raue
A. Reimer
O. Reimer
M. Renaud
R. de los Reyes
F. Rieger
L. Rob
S. Rosier-Lees
G. Rowell
B. Rudak
C. B. Rulten
V. Sahakian
David M. Sanchez
A. Santangelo
R. Schlickeiser
F. Schuessler
A. Schulz
U. Schwanke
S. Schwarzburg
S. Schwemmer
H. Sol
G. Spengler
F. Spies
L. Stawarz
R. Steenkamp
Christian Stegmann
F. Stinzing
K. Stycz
Iurii Sushch
A. Szostek
J. -P. Tavernet
R. Terrier
M. Tluczykont
C. Trichard
K. Valerius
C. van Eldik
G. Vasileiadis
C. Venter
A. Viana
P. Vincent
H. J. Voelk
F. Volpe
M. Vorster
S. J. Wagner
P. Wagner
M. Ward
M. Weidinger
Q. Weitzel
R. White
A. Wierzcholska
P. Willmann
A. Woernlein
D. Wouters
M. Zacharias
A. Zajczyk
A. A. Zdziarski
Alraune Zech
H. -S. Zechlin
eng
uncontrolled
galaxies: active
eng
uncontrolled
BL Lacertae objects: general
eng
uncontrolled
BL Lacertae objects: individual: PKS 0301-243
eng
uncontrolled
gamma rays: galaxies
eng
uncontrolled
radiation mechanisms: non-thermal
36122
2012
2012
eng
18
2
746
article
IOP Publ. Ltd.
Bristol
HESS Collaboration, MAGIC Collaboration, VERITAS Collaboration
1
--
--
--
The 2010 very high energy gamma-ray flare and 10 years ofmulti-wavelength oservations of M 87
The giant radio galaxy M 87 with its proximity (16 Mpc), famous jet, and very massive black hole ((3-6) x 10(9) M-circle dot) provides a unique opportunity to investigate the origin of very high energy (VHE; E > 100 GeV) gamma-ray emission generated in relativistic outflows and the surroundings of supermassive black holes. M 87 has been established as a VHE gamma-ray emitter since 2006. The VHE gamma-ray emission displays strong variability on timescales as short as a day. In this paper, results from a joint VHE monitoring campaign on M 87 by the MAGIC and VERITAS instruments in 2010 are reported. During the campaign, a flare at VHE was detected triggering further observations at VHE (H.E.S.S.), X-rays (Chandra), and radio (43 GHz Very Long Baseline Array, VLBA). The excellent sampling of the VHE gamma-ray light curve enables one to derive a precise temporal characterization of the flare: the single, isolated flare is well described by a two-sided exponential function with significantly different flux rise and decay times of tau(rise)(d) = (1.69 +/- 0.30) days and tau(decay)(d) = (0.611 +/- 0.080) days, respectively. While the overall variability pattern of the 2010 flare appears somewhat different from that of previous VHE flares in 2005 and 2008, they share very similar timescales (similar to day), peak fluxes (Phi(>0.35 TeV) similar or equal to (1-3) x 10(-11) photons cm(-2) s(-1)), and VHE spectra. VLBA radio observations of 43 GHz of the inner jet regions indicate no enhanced flux in 2010 in contrast to observations in 2008, where an increase of the radio flux of the innermost core regions coincided with a VHE flare. On the other hand, Chandra X-ray observations taken similar to 3 days after the peak of the VHE gamma-ray emission reveal an enhanced flux from the core (flux increased by factor similar to 2; variability timescale <2 days). The long-term (2001-2010) multi-wavelength (MWL) light curve of M 87, spanning from radio to VHE and including data from Hubble Space Telescope, Liverpool Telescope, Very Large Array, and European VLBI Network, is used to further investigate the origin of the VHE gamma-ray emission. No unique, common MWL signature of the three VHE flares has been identified. In the outer kiloparsec jet region, in particular in HST-1, no enhanced MWL activity was detected in 2008 and 2010, disfavoring it as the origin of the VHE flares during these years. Shortly after two of the three flares (2008 and 2010), the X-ray core was observed to be at a higher flux level than its characteristic range (determined from more than 60 monitoring observations: 2002-2009). In 2005, the strong flux dominance of HST-1 could have suppressed the detection of such a feature. Published models for VHE gamma-ray emission from M 87 are reviewed in the light of the new data.
The astrophysical journal : an international review of spectroscopy and astronomical physics
10.1088/0004-637X/746/2/151
0004-637X
wos:2011-2013
151
WOS:000300406300037
Abramowski, A (reprint author), Univ Hamburg, Inst Expt Phys, Luruper Chaussee 149, D-22761 Hamburg, Germany., martin.raue@desy.de; stawarz@astro.isas.jaxa.jp; colin@mppmu.mpg.de; mazin@ifae.es; beilicke@physics.wustl.edu; cmhui@physics.utah.edu
Namibian authorities; German Ministry for Education and Research (BMBF);
Max Planck Society; French Ministry for Research; CNRS-IN2P3; CNRS; U.K.
Science and Technology Facilities Council (STFC); IPNP of the Charles
University; Polish Ministry of Science and Higher Education; South
African Department of Science and Technology; National Research
Foundation; University of Namibia; German BMBF; German MPG; Italian
INFN; Swiss National Fund SNF; Spanish MICINN; Bulgarian NSF
[CSD2007-00042, CSD2009-00064, DO02-353]; Academy of Finland [127740];
YIP of the Helmholtz Gemeinschaft; DFG Cluster of Excellence "Origin and
Structure of the Universe,"; DFG Collaborative Research Centers
[SFB823/C4, SFB876/C3]; Polish MNiSzW [745/N-HESS-MAGIC/2010/0]; US
Department of Energy Office of Science; US National Science Foundation;
Smithsonian Institution; NSERC in Canada; Science Foundation Ireland
(SFI) [10/RFP/AST2748]; STFC in the UK; Istituto Nazionale di
Astrofisica in Italy; Centre National d'Etudes Spatiales in France; NASA
[GO0-11120X]; Associated Universities, Inc.; European Community [227290]
Attila Abramowski
F. Acero
Felix A. Aharonian
A. G. Akhperjanian
Gisela Anton
Arnim Balzer
Anna Barnacka
U. Barres de Almeida
Yvonne Becherini
J. Becker
B. Behera
K. Bernlöhr
E. Birsin
Jonathan Biteau
A. Bochow
Catherine Boisson
J. Bolmont
Pol Bordas
J. Brucker
Francois Brun
Pierre Brun
Tomasz Bulik
I. Buesching
Svenja Carrigan
Sabrina Casanova
M. Cerruti
Paula M. Chadwick
A. Charbonnier
Ryan C. G. Chaves
A. Cheesebrough
A. C. Clapson
G. Coignet
Gabriele Cologna
Jan Conrad
M. Dalton
M. K. Daniel
I. D. Davids
B. Degrange
C. Deil
H. J. Dickinson
A. Djannati-Ataï
W. Domainko
L. O'C. Drury
G. Dubus
K. Dutson
J. Dyks
M. Dyrda
Kathrin Egberts
P. Eger
P. Espigat
L. Fallon
C. Farnier
S. Fegan
F. Feinstein
M. V. Fernandes
A. Fiasson
G. Fontaine
A. Foerster
M. Fuessling
Y. A. Gallant
H. Gast
L. Gerard
D. Gerbig
B. Giebels
J. F. Glicenstein
B. Glueck
P. Goret
D. Goering
S. Haeffner
J. D. Hague
D. Hampf
M. Hauser
S. Heinz
G. Heinzelmann
G. Henri
G. Hermann
James Anthony Hinton
A. Hoffmann
W. Hofmann
P. Hofverberg
M. Holler
D. Horns
A. Jacholkowska
O. C. de Jager
C. Jahn
M. Jamrozy
I. Jung
M. A. Kastendieck
K. Katarzynski
U. Katz
S. Kaufmann
D. Keogh
D. Khangulyan
B. Khelifi
D. Klochkov
W. Kluzniak
T. Kneiske
Nu. Komin
K. Kosack
R. Kossakowski
H. Laffon
G. Lamanna
D. Lennarz
T. Lohse
A. Lopatin
C. -C. Lu
V. Marandon
A. Marcowith
J. Masbou
D. Maurin
N. Maxted
M. Mayer
T. J. L. McComb
M. C. Medina
J. Mehault
R. Moderski
E. Moulin
C. L. Naumann
M. Naumann-Godo
M. de Naurois
D. Nedbal
D. Nekrassov
N. Nguyen
B. Nicholas
J. Niemiec
S. J. Nolan
S. Ohm
E. de Ona Wilhelmi
B. Opitz
M. Ostrowski
I. Oya
M. Panter
M. Paz Arribas
G. Pedaletti
G. Pelletier
P. -O. Petrucci
S. Pita
G. Puehlhofer
M. Punch
A. Quirrenbach
M. Raue
S. M. Rayner
A. Reimer
O. Reimer
M. Renaud
R. de los Reyes
F. Rieger
J. Ripken
L. Rob
S. Rosier-Lees
G. Rowell
B. Rudak
C. B. Rulten
J. Ruppel
V. Sahakian
David M. Sanchez
A. Santangelo
R. Schlickeiser
F. M. Schoeck
A. Schulz
U. Schwanke
S. Schwarzburg
S. Schwemmer
F. Sheidaei
J. L. Skilton
H. Sol
G. Spengler
L. Stawarz
R. Steenkamp
Christian Stegmann
F. Stinzing
K. Stycz
Iurii Sushch
A. Szostek
J. -P. Tavernet
R. Terrier
M. Tluczykont
K. Valerius
C. van Eldik
G. Vasileiadis
C. Venter
J. P. Vialle
A. Viana
P. Vincent
H. J. Voelk
F. Volpe
S. Vorobiov
M. Vorster
S. J. Wagner
M. Ward
R. White
A. Wierzcholska
M. Zacharias
A. Zajczyk
A. A. Zdziarski
Alraune Zech
H. -S. Zechlin
J. Aleksic
L. A. Antonelli
P. Antoranz
Michael Backes
J. A. Barrio
D. Bastieri
J. Becerra Gonzalez
W. Bednarek
A. Berdyugin
K. Berger
E. Bernardini
A. Biland
O. Blanch Bigas
R. K. Bock
A. Boller
G. Bonnoli
D. Borla Tridon
I. Braun
T. Bretz
A. Canellas
E. Carmona
A. Carosi
P. Colin
E. Colombo
J. L. Contreras
J. Cortina
L. Cossio
S. Covino
F. Dazzi
A. De Angelis
E. De Cea del Pozo
B. De Lotto
C. Delgado Mendez
A. Diago Ortega
M. Doert
A. Dominguez
Dijana Dominis Prester
D. Dorner
M. Doro
D. Elsaesser
D. Ferenc
M. V. Fonseca
L. Font
C. Fruck
R. J. Garcia Lopez
M. Garczarczyk
D. Garrido
G. Giavitto
N. Godinovic
D. Hadasch
D. Haefner
A. Herrero
D. Hildebrand
D. Hoehne-Moench
J. Hose
D. Hrupec
B. Huber
T. Jogler
S. Klepser
T. Kraehenbuehl
J. Krause
A. La Barbera
D. Lelas
E. Leonardo
E. Lindfors
S. Lombardi
M. Lopez
E. Lorenz
M. Makariev
G. Maneva
N. Mankuzhiyil
K. Mannheim
L. Maraschi
M. Mariotti
M. Martinez
D. Mazin
M. Meucci
J. M. Miranda
R. Mirzoyan
H. Miyamoto
J. Moldon
A. Moralejo
P. Munar
D. Nieto
K. Nilsson
R. Orito
I. Oya
D. Paneque
R. Paoletti
S. Pardo
J. M. Paredes
S. Partini
M. Pasanen
F. Pauss
M. A. Perez-Torres
M. Persic
L. Peruzzo
M. Pilia
J. Pochon
F. Prada
P. G. Prada Moroni
E. Prandini
I. Puljak
I. Reichardt
R. Reinthal
W. Rhode
M. Ribo
J. Rico
S. Ruegamer
A. Saggion
K. Saito
T. Y. Saito
M. Salvati
K. Satalecka
V. Scalzotto
V. Scapin
C. Schultz
T. Schweizer
M. Shayduk
S. N. Shore
A. Sillanpaa
J. Sitarek
D. Sobczynska
F. Spanier
S. Spiro
A. Stamerra
B. Steinke
J. Storz
N. Strah
T. Suric
L. Takalo
H. Takami
F. Tavecchio
P. Temnikov
T. Terzic
D. Tescaro
M. Teshima
M. Thom
O. Tibolla
D. F. Torres
A. Treves
H. Vankov
P. Vogler
R. M. Wagner
Q. Weitzel
V. Zabalza
F. Zandanel
R. Zanin
T. Arlen
T. Aune
M. Beilicke
W. Benbow
A. Bouvier
S. M. Bradbury
J. H. Buckley
V. Bugaev
K. Byrum
A. Cannon
A. Cesarini
L. Ciupik
M. P. Connolly
W. Cui
R. Dickherber
C. Duke
M. Errando
A. Falcone
J. P. Finley
G. Finnegan
L. Fortson
A. Furniss
N. Galante
D. Gall
S. Godambe
S. Griffin
J. Grube
G. Gyuk
D. Hanna
J. Holder
H. Huan
C. M. Hui
P. Kaaret
N. Karlsson
M. Kertzman
Y. Khassen
D. Kieda
H. Krawczynski
F. Krennrich
M. J. Lang
S. LeBohec
G. Maier
S. McArthur
A. McCann
P. Moriarty
R. Mukherjee
P. D. Nunez
R. A. Ong
M. Orr
A. N. Otte
N. Park
J. S. Perkins
A. Pichel
Martin Pohl
H. Prokoph
K. Ragan
L. C. Reyes
P. T. Reynolds
E. Roache
H. J. Rose
J. Ruppel
M. Schroedter
G. H. Sembroski
G. D. Sentuerk
Igor O. Telezhinsky
G. Tesic
M. Theiling
S. Thibadeau
A. Varlotta
V. V. Vassiliev
M. Vivier
S. P. Wakely
T. C. Weekes
D. A. Williams
B. Zitzer
U. Barres de Almeida
M. Cara
C. Casadio
C. C. Cheung
W. McConville
F. Davies
A. Doi
G. Giovannini
M. Giroletti
K. Hada
P. Hardee
D. E. Harris
W. Junor
M. Kino
N. P. Lee
C. Ly
J. Madrid
F. Massaro
C. G. Mundell
H. Nagai
E. S. Perlman
I. A. Steele
R. C. Walker
D. L. Wood
eng
uncontrolled
galaxies: active
eng
uncontrolled
galaxies: individual (M 87)
eng
uncontrolled
galaxies: jets
eng
uncontrolled
galaxies: nuclei
eng
uncontrolled
gamma rays: galaxies
eng
uncontrolled
radiation mechanisms: non-thermal
Institut für Physik und Astronomie
Referiert
35174
2013
2013
eng
7
551
article
EDP Sciences
Les Ulis
HESS Collaboration
1
--
--
--
HESS observations of the binary system PSR B1259-63/LS 2883 around the 2010/2011 periastron passage
Aims. We present very high energy (VHE; E > 100 GeV) data from the gamma-ray binary system PSR B1259-63/LS 2883 taken around its periastron passage on 15th of December 2010 with the High Energy Stereoscopic System (H. E. S. S.) of Cherenkov Telescopes. We aim to search for a possible TeV counterpart of the GeV flare detected by the Fermi LAT. In addition, we aim to study the current periastron passage in the context of previous observations taken at similar orbital phases, testing the repetitive behaviour of the source.
Methods. Observations at VHEs were conducted with H.E.S.S. from 9th to 16th of January 2011. The total dataset amounts to similar to 6 h of observing time. The data taken around the 2004 periastron passage were also re-analysed with the current analysis techniques in order to extend the energy spectrum above 3 TeV to fully compare observation results from 2004 and 2011.
Results. The source is detected in the 2011 data at a significance level of 11.5 sigma revealing an averaged integral flux above 1 TeV of (1.01 +/- 0.18(stat) +/- 0.20(sys)) x 10(-12) cm(-2) s(-1). The differential energy spectrum follows a power-law shape with a spectral index Gamma = 2.92 +/- 0.30(stat) +/- 0.20(sys) and a flux normalisation at 1 TeV of N-0 = (1.95 +/- 0.32(stat) +/- 0.39(sys)) x 10(-12) TeV-1 cm(-2) s(-1). The measured light curve does not show any evidence for variability of the source on the daily scale. The re-analysis of the 2004 data yields results compatible with the published ones. The differential energy spectrum measured up to similar to 10 TeV is consistent with a power law with a spectral index Gamma = 2.81 +/- 0.10(stat) +/- 0.20(sys) and a flux normalisation at 1 TeV of N-0 = (1.29 +/- 0.08(stat) +/- 0.26(sys)) x 10(-12) TeV-1 cm(-2) s(-1).
Conclusions. The measured integral flux and the spectral shape of the 2011 data are compatible with the results obtained around previous periastron passages. The absence of variability in the H.E.S.S. data indicates that the GeV flare observed by Fermi LAT in the time period covered also by H.E.S.S. observations originates in a different physical scenario than the TeV emission. Moreover, the comparison of the new results to the results from the 2004 observations made at a similar orbital phase provides a stronger evidence of the repetitive behaviour of the source.
Astronomy and astrophysics : an international weekly journal
10.1051/0004-6361/201220612
0004-6361
wos:2011-2013
A94
WOS:000316460600094
de Naurois, M (reprint author), Ecole Polytech, CNRS, IN2P3, Lab Leprince Ringuet, F-91128 Palaiseau, France., denauroi@in2p3.fr; yusushch@physik.hu-berlin.de
German Ministry for Education and Research (BMBF); Max Planck Society;
French Ministry for Research; CNRS-IN2P3; Astroparticle
Interdisciplinary Programme of the CNRS; UK Particle Physics and
Astronomy Research Council (PPARC); IPNP of the Charles University;
South African Department of Science and Technology; National Research
Foundation; University of Namibia
Attila Abramowski
F. Acero
Felix A. Aharonian
A. G. Akhperjanian
Gisela Anton
Shangkari Balenderan
Arnim Balzer
Anna Barnacka
Yvonne Becherini
J. Becker Tjus
K. Bernlöhr
E. Birsin
Jonathan Biteau
Catherine Boisson
J. Bolmont
Pol Bordas
J. Brucker
Francois Brun
Pierre Brun
Tomasz Bulik
Svenja Carrigan
Sabrina Casanova
M. Cerruti
Paula M. Chadwick
Ryan C. G. Chaves
A. Cheesebrough
Sergio Colafrancesco
Gabriele Cologna
Jan Conrad
C. Couturier
M. Dalton
M. K. Daniel
I. D. Davids
B. Degrange
C. Deil
P. deWilt
H. J. Dickinson
A. Djannati-Ataï
W. Domainko
L. O'C. Drury
G. Dubus
K. Dutson
J. Dyks
M. Dyrda
Kathrin Egberts
P. Eger
P. Espigat
L. Fallon
C. Farnier
S. Fegan
F. Feinstein
M. V. Fernandes
D. Fernandez
A. Fiasson
G. Fontaine
A. Foerster
M. Fuessling
M. Gajdus
Y. A. Gallant
T. Garrigoux
H. Gast
B. Giebels
J. F. Glicenstein
B. Glueck
D. Goering
M. -H. Grondin
M. Grudzinska
S. Haeffner
J. D. Hague
J. Hahn
D. Hampf
J. Harris
S. Heinz
G. Heinzelmann
G. Henri
G. Hermann
A. Hillert
James Anthony Hinton
W. Hofmann
P. Hofverberg
Markus Holler
D. Horns
A. Jacholkowska
C. Jahn
M. Jamrozy
I. Jung
M. A. Kastendieck
K. Katarzynski
U. Katz
S. Kaufmann
B. Khelifi
S. Klepser
D. Klochkov
W. Kluzniak
T. Kneiske
D. Kolitzus
Nu Komin
K. Kosack
R. Kossakowski
F. Krayzel
P. P. Krueger
H. Laffon
G. Lamanna
J. Lefaucheur
M. Lemoine-Goumard
J. -P. Lenain
D. Lennarz
T. Lohse
A. Lopatin
C. -C. Lu
V. Marandon
A. Marcowith
J. Masbou
G. Maurin
N. Maxted
M. Mayer
T. J. L. McComb
M. C. Medina
J. Mehault
U. Menzler
R. Moderski
M. Mohamed
E. Moulin
C. L. Naumann
M. Naumann-Godo
M. de Naurois
D. Nedbal
N. Nguyen
J. Niemiec
S. J. Nolan
L. Oakes
S. Ohm
E. de Ona Wilhelmi
B. Opitz
M. Ostrowski
I. Oya
M. Panter
R. D. Parsons
M. Paz Arribas
N. W. Pekeur
G. Pelletier
J. Perez
P. -O. Petrucci
B. Peyaud
S. Pita
G. Puehlhofer
M. Punch
A. Quirrenbach
S. Raab
M. Raue
A. Reimer
O. Reimer
M. Renaud
R. de los Reyes
F. Rieger
J. Ripken
L. Rob
S. Rosier-Lees
G. Rowell
B. Rudak
C. B. Rulten
V. Sahakian
David M. Sanchez
A. Santangelo
R. Schlickeiser
A. Schulz
U. Schwanke
S. Schwarzburg
S. Schwemmer
F. Sheidaei
J. L. Skilton
H. Sol
G. Spengler
L. Stawarz
R. Steenkamp
Christian Stegmann
F. Stinzing
K. Stycz
Iurii Sushch
A. Szostek
J. -P. Tavernet
R. Terrier
M. Tluczykont
C. Trichard
K. Valerius
C. van Eldik
G. Vasileiadis
C. Venter
A. Viana
P. Vincent
H. J. Voelk
F. Volpe
S. Vorobiov
M. Vorster
S. J. Wagner
M. Ward
R. White
A. Wierzcholska
P. Willmann
D. Wouters
M. Zacharias
A. Zajczyk
A. A. Zdziarski
Alraune Zech
H. -S. Zechlin
eng
uncontrolled
gamma rays: general
eng
uncontrolled
pulsars: individual: PSR B1259-63
eng
uncontrolled
X-rays: binaries
eng
uncontrolled
stars: individual: LS 2883
Institut für Physik und Astronomie
Referiert
35257
2013
2013
eng
6
4
110
article
American Physical Society
College Park
HESS Collaboration
1
--
--
--
Search for Photon-Linelike Signatures from Dark Matter Annihilations with H.E.S.S.
Gamma-ray line signatures can be expected in the very-high-energy (E-gamma > 100 GeV) domain due to self-annihilation or decay of dark matter (DM) particles in space. Such a signal would be readily distinguishable from astrophysical gamma-ray sources that in most cases produce continuous spectra that span over several orders of magnitude in energy. Using data collected with the H. E. S. S. gamma-ray instrument, upper limits on linelike emission are obtained in the energy range between similar to 500 GeV and similar to 25 TeV for the central part of the Milky Way halo and for extragalactic observations, complementing recent limits obtained with the Fermi-LAT instrument at lower energies. No statistically significant signal could be found. For monochromatic gamma-ray line emission, flux limits of (2 x 10(-7)-2 x 10(-5)) m(-2)s(-1)sr(-1) and (1 x 10(-8)- 2 x 10(-6)) m(-2)s(-1)sr(-1) are obtained for the central part of the Milky Way halo and extragalactic observations, respectively. For a DM particle mass of 1 TeV, limits on the velocity- averaged DM annihilation cross section <sigma upsilon >(chi chi ->gamma gamma) reach similar to 10(-27)cm(3)s(-1), based on the Einasto parametrization of the Galactic DM halo density profile. DOI: 10.1103/PhysRevLett.110.041301
Physical review letters
10.1103/PhysRevLett.110.041301
0031-9007
wos:2011-2013
041301
WOS:000313951300004
Abramowski, A (reprint author), Univ Hamburg, Inst Expt Phys, Luruper Chaussee 149, D-22761 Hamburg, Germany., Daniil.Nekrassov@mpi-hd.mpg.de; Christopher.van.Eldik@physik.uni-erlangen.de
German Ministry for Education and Research (BMBF); Max Planck Society;
French Ministry for Research; CNRS-IN2P3; Astroparticle
Interdisciplinary Programme of the CNRS; U.K. Science and Technology
Facilities Council (STFC); IPNP of the Charles University; Polish
Ministry of Science and Higher Education; South African Department of
Science and Technology; National Research Foundation; University of
Namibia; European Community [ERC-StG-259391]
Attila Abramowski
F. Acero
Felix A. Aharonian
A. G. Akhperjanian
Gisela Anton
Shangkari Balenderan
Arnim Balzer
Anna Barnacka
Yvonne Becherini
J. Becker Tjus
K. Bernlöhr
E. Birsin
Jonathan Biteau
A. Bochow
Catherine Boisson
J. Bolmont
Pol Bordas
J. Brucker
Francois Brun
Pierre Brun
Tomasz Bulik
Svenja Carrigan
Sabrina Casanova
M. Cerruti
Paula M. Chadwick
Ryan C. G. Chaves
A. Cheesebrough
Sergio Colafrancesco
Gabriele Cologna
Jan Conrad
C. Couturier
M. Dalton
M. K. Daniel
I. D. Davids
B. Degrange
C. Deil
P. deWilt
H. J. Dickinson
A. Djannati-Ataï
W. Domainko
L. O'C. Drury
G. Dubus
K. Dutson
J. Dyks
M. Dyrda
Kathrin Egberts
P. Eger
P. Espigat
L. Fallon
C. Farnier
S. Fegan
F. Feinstein
M. V. Fernandes
D. Fernandez
A. Fiasson
G. Fontaine
A. Foerster
Matthias Fussling
M. Gajdus
Y. A. Gallant
T. Garrigoux
H. Gast
B. Giebels
J. F. Glicenstein
B. Glueck
D. Goering
M. -H. Grondin
S. Haeffner
J. D. Hague
J. Hahn
D. Hampf
J. Harris
S. Heinz
G. Heinzelmann
G. Henri
G. Hermann
A. Hillert
James Anthony Hinton
W. Hofmann
P. Hofverberg
M. Holler
D. Horns
A. Jacholkowska
C. Jahn
M. Jamrozy
I. Jung
M. A. Kastendieck
K. Katarzynski
U. Katz
S. Kaufmann
B. Khelifi
S. Klepser
D. Klochkov
W. Kluzniak
T. Kneiske
Nu Komin
K. Kosack
R. Kossakowski
F. Krayzel
P. P. Krueger
H. Laffon
G. Lamanna
J. Lefaucheur
M. Lemoine-Goumard
J. -P. Lenain
D. Lennarz
T. Lohse
A. Lopatin
C. -C. Lu
V. Marandon
A. Marcowith
J. Masbou
G. Maurin
N. Maxted
M. Mayer
T. J. L. McComb
M. C. Medina
J. Mehault
U. Menzler
R. Moderski
M. Mohamed
E. Moulin
C. L. Naumann
M. Naumann-Godo
M. de Naurois
D. Nedbal
D. Nekrassov
N. Nguyen
J. Niemiec
S. J. Nolan
S. Ohm
E. de Ona Awilhelmi
B. Opitz
M. Ostrowski
I. Oya
M. Panter
R. D. Parsons
M. Paz Arribas
N. W. Pekeur
G. Pelletier
J. Perez
P. -O. Petrucci
B. Peyaud
S. Pita
G. Puehlhofer
M. Punch
A. Quirrenbach
M. Raue
A. Reimer
O. Reimer
M. Renaud
R. de los Reyes
F. Rieger
J. Ripken
L. Rob
S. Rosier-Lees
G. Rowell
B. Rudak
C. B. Rulten
V. Sahakian
David M. Sanchez
A. Santangelo
R. Schlickeiser
A. Schulz
U. Schwanke
S. Schwarzburg
S. Schwemmer
F. Sheidaei
J. L. Skilton
H. Sol
G. Spengler
L. Stawarz
R. Steenkamp
Christian Stegmann
F. Stinzing
K. Stycz
Iurii Sushch
A. Szostek
J. -P. Tavernet
R. Terrier
M. Tluczykont
C. Trichard
K. Valerius
C. van Eldik
G. Vasileiadis
C. Venter
A. Viana
P. Vincent
H. J. Voelk
F. Volpe
S. Vorobiov
M. Vorster
S. J. Wagner
M. Ward
R. White
A. Wierzcholska
D. Wouters
M. Zacharias
A. Zajczyk
A. A. Zdziarski
Alraune Zech
H. -S. Zechlin
Institut für Physik und Astronomie
Referiert
35175
2013
2013
eng
8
551
article
EDP SCIENCES S A
LES ULIS CEDEX A
HESS Collaboration
1
--
--
--
Search for very-high-energy gamma-ray emission from Galactic globular
clusters with HESS
Context. Globular clusters (GCs) are established emitters of high-energy (HE, 100 MeV < E < 100 GeV) gamma-ray radiation which could originate from the cumulative emission of the numerous millisecond pulsars (msPSRs) in the clusters’ cores or from inverse Compton (IC) scattering of relativistic leptons accelerated in the GC environment. These stellar clusters could also constitute a new class of sources in the very-high-energy (VHE, E > 100 GeV) gamma-ray regime, judging from the recent detection of a signal from the direction of Terzan 5 with the H.E.S.S. telescope array. Aims. To search for VHE gamma-ray sources associated with other GCs, and to put constraints on leptonic emission models, we systematically analyzed the observations towards 15 GCs taken with the H. E. S. S. array of imaging atmospheric Cherenkov telescopes. Methods. We searched for point-like and extended VHE gamma-ray emission from each GC in our sample and also performed a stacking analysis combining the data from all GCs to investigate the hypothesis of a population of faint emitters. Assuming IC emission as the origin of the VHE gamma-ray signal from the direction of Terzan 5, we calculated the expected gamma-ray flux from each of the 15 GCs, based on their number of millisecond pulsars, their optical brightness and the energy density of background photon fields. Results. We did not detect significant VHE gamma-ray emission from any of the 15 GCs in either of the two analyses. Given the uncertainties related to the parameter determinations, the obtained flux upper limits allow to rule out the simple IC/msPSR scaling model for NGC6388 and NGC7078. The upper limits derived from the stacking analyses are factors between 2 and 50 below the flux predicted by the simple leptonic scaling model, depending on the assumed source extent and the dominant target photon fields. Therefore, Terzan 5 still remains exceptional among all GCs, as the VHE gamma-ray emission either arises from extra-ordinarily efficient leptonic processes, or from a recent catastrophic event, or is even unrelated to the GC itself.
ASTRONOMY & ASTROPHYSICS
10.1051/0004-6361/201220719
0004-6361
wos:2011-2013
A26
WOS:000316460600026
Eger, P (reprint author), Univ Erlangen Nurnberg, Inst Phys, Erwin Rommel Str 1, D-91058 Erlangen, Germany.
, eger@mpi-hd.mpg.de; Christopher.van.Eldik@physik.uni-erlangen.de
German Ministry for Education and Research (BMBF); Max Planck Society;
German Research Foundation (DFG); French Ministry for Research;
CNRS-IN2P3; Astroparticle Interdisciplinary Programme of the CNRS; U.K.
Science and Technology Facilities Council (STFC); IPNP of the Charles
University; Czech Science Foundation; Polish Ministry of Science and
Higher Education; South African Department of Science and Technology;
National Research Foundation; University of Namibia
Attila Abramowski
F. Acero
Felix A. Aharonian
A. G. Akhperjanian
Gisela Anton
Shangkari Balenderan
Arnim Balzer
Anna Barnacka
Yvonne Becherini
J. Becker Tjus
K. Bernlöhr
E. Birsin
Jonathan Biteau
A. Bochow
Catherine Boisson
J. Bolmont
Pol Bordas
J. Brucker
Francois Brun
Pierre Brun
Tomasz Bulik
Svenja Carrigan
Sabrina Casanova
M. Cerruti
Paula M. Chadwick
Ryan C. G. Chaves
A. Cheesebrough
Sergio Colafrancesco
Gabriele Cologna
Jan Conrad
C. Couturier
M. Dalton
M. K. Daniel
I. D. Davids
B. Degrange
C. Deil
P. deWilt
H. J. Dickinson
A. Djannati-Ataï
W. Domainko
L. O&rsquo Drury
C.
G. Dubus
K. Dutson
J. Dyks
M. Dyrda
Kathrin Egberts
P. Eger
P. Espigat
L. Fallon
C. Farnier
S. Fegan
F. Feinstein
M. V. Fernandes
D. Fernandez
A. Fiasson
G. Fontaine
A. Foerster
M. Fuessling
M. Gajdus
Y. A. Gallant
T. Garrigoux
H. Gast
B. Giebels
J. F. Glicenstein
B. Glueck
D. Goering
M-H. Grondin
M. Grudzinska
S. Haeffner
J. D. Hague
J. Hahn
D. Hampf
J. Harris
S. Heinz
G. Heinzelmann
G. Henri
G. Hermann
A. Hillert
James Anthony Hinton
W. Hofmann
P. Hofverberg
M. Holler
D. Horns
A. Jacholkowska
C. Jahn
M. Jamrozy
I. Jung
M. A. Kastendieck
K. Katarzynski
U. Katz
S. Kaufmann
B. Khelifi
S. Klepser
D. Klochkov
W. Kluzniak
T. Kneiske
D. Kolitzus
Nu. Komin
K. Kosack
R. Kossakowski
F. Krayzel
P. P. Krueger
H. Laffon
G. Lamanna
J. Lefaucheur
M. Lemoine-Goumard
J-P Lenain
D. Lennarz
T. Lohse
A. Lopatin
C-C. Lu
V. Marandon
A. Marcowith
J. Masbou
G. Maurin
N. Maxted
M. Mayer
T. J. L. McComb
M. C. Medina
J. Mehault
U. Menzler
R. Moderski
M. Mohamed
E. Moulin
C. L. Naumann
M. Naumann-Godo
M. de Naurois
D. Nedbal
N. Nguyen
J. Niemiec
S. J. Nolan
S. Ohm
E. de Ona Wilhelmi
B. Opitz
M. Ostrowski
I. Oya
M. Panter
R. D. Parsons
M. Paz Arribas
N. W. Pekeur
G. Pelletier
J. Perez
P-O Petrucci
B. Peyaud
S. Pita
G. Puehlhofer
M. Punch
A. Quirrenbach
S. Raab
M. Raue
A. Reimer
O. Reimer
M. Renaud
R. de los Reyes
F. Rieger
J. Ripken
L. Rob
S. Rosier-Lees
G. Rowell
B. Rudak
C. B. Rulten
V. Sahakian
David M. Sanchez
A. Santangelo
R. Schlickeiser
A. Schulz
U. Schwanke
S. Schwarzburg
S. Schwemmer
F. Sheidaei
J. L. Skilton
H. Sol
G. Spengler
L. Stawarz
R. Steenkamp
Christian Stegmann
F. Stinzing
K. Stycz
Iurii Sushch
A. Szostek
J-P Tavernet
R. Terrier
M. Tluczykont
C. Trichard
K. Valerius
C. van Eldik
G. Vasileiadis
C. Venter
A. Viana
P. Vincent
H. J. Voelk
F. Volpe
S. Vorobiov
M. Vorster
S. J. Wagner
M. Ward
R. White
A. Wierzcholska
D. Wouters
M. Zacharias
A. Zajczyk
A. A. Zdziarski
Alraune Zech
H-S Zechlin
eng
uncontrolled
globular clusters: general
eng
uncontrolled
radiation mechanisms: non-thermal
eng
uncontrolled
pulsars: general
eng
uncontrolled
gamma rays: general
34961
2013
2013
eng
7
6
554
article
EDP Sciences
Les Ulis
HESS Collaboration
1
--
--
--
HESS discovery of VHE gamma-rays from the quasar PKS 1510-089
The quasar PKS 1510-089 (z = 0.361) was observed with the H.E.S.S. array of imaging atmospheric Cherenkov telescopes during high states in the optical and GeV bands, to search for very high energy (VHE, defined as E >= 0.1 TeV) emission. VHE gamma-rays were detected with a statistical significance of 9.2 standard deviations in 15.8 h of H. E. S. S. data taken during March and April 2009. A VHE integral flux of I(0.15 TeV < E < 1.0TeV) = (1.0 +/- 0.2(stat) +/- 0.2(sys)) x 10(-11) cm(-2) s(-1) is measured. The best-fit power law to the VHE data has a photon index of G = 5.4 +/- 0.7(stat) +/- 0.3(sys). The GeV and optical light curves show pronounced variability during the period of H.E.S.S. observations. However, there is insufficient evidence to claim statistically significant variability in the VHE data. Because of its relatively high redshift, the VHE flux from PKS 1510-089 should suffer considerable attenuation in the intergalactic space due to the extragalactic background light (EBL). Hence, the measured gamma-ray spectrum is used to derive upper limits on the opacity due to EBL, which are found to be comparable with the previously derived limits from relatively-nearby BL Lac objects. Unlike typical VHE-detected blazars where the broadband spectrum is dominated by nonthermal radiation at all wavelengths, the quasar PKS 1510-089 has a bright thermal component in the optical to UV frequency band. Among all VHE detected blazars, PKS 1510-089 has the most luminous broad line region. The detection of VHE emission from this quasar indicates a low level of gamma - gamma absorption on the internal optical to UV photon field.
Astronomy and astrophysics : an international weekly journal
10.1051/0004-6361/201321135
0004-6361
wos:2011-2013
A107
WOS:000320444200106
Behera, B (reprint author), DESY, Platanenallee 6, D-15738 Zeuthen, Germany., Bagmeet.Behera@desy.de
Namibian authorities; University of Namibia; German Ministry for
Education and Research (BMBF); Max Planck Society; German Research
Foundation (DFG); French Ministry for Research; CNRS [IN2P3];
Astroparticle Interdisciplinary Programme of the CNRS; UK Science and
Technology Facilities Council (STFC); IPNP of the Charles University;
Czech Science Foundation; Polish Ministry of Science and Higher
Education; South African Department of Science and Technology; National
Research Foundation; International Max Planck Research School (IMPRS)
for Astronomy & Cosmic Physics at the University of Heidelberg
Attila Abramowski
F. Acero
Felix A. Aharonian
A. G. Akhperjanian
Gisela Anton
Shangkari Balenderan
Arnim Balzer
Anna Barnacka
Yvonne Becherini
J. Becker Tjus
B. Behera
K. Bernlöhr
E. Birsin
Jonathan Biteau
A. Bochow
Catherine Boisson
J. Bolmont
Pol Bordas
J. Brucker
Francois Brun
Pierre Brun
Tomasz Bulik
Svenja Carrigan
Sabrina Casanova
M. Cerruti
Paula M. Chadwick
Ryan C. G. Chaves
A. Cheesebrough
Sergio Colafrancesco
Gabriele Cologna
Jan Conrad
C. Couturier
M. Dalton
M. K. Daniel
I. D. Davids
B. Degrange
C. Deil
P. deWilt
H. J. Dickinson
A. Djannati-Ataï
W. Domainko
L. O'C. Drury
G. Dubus
K. Dutson
J. Dyks
M. Dyrda
Kathrin Egberts
P. Eger
P. Espigat
L. Fallon
C. Farnier
S. Fegan
F. Feinstein
M. V. Fernandes
D. Fernandez
A. Fiasson
G. Fontaine
A. Foester
M. Fuessling
M. Gajdus
Y. A. Gallant
T. Garrigoux
H. Gast
B. Giebels
J. F. Glicenstein
B. Glueck
D. Goeing
M. -H. Grondin
M. Grudzinska
S. Haeffner
J. D. Hague
J. Hahn
D. Hampf
J. Harris
M. Hauser
S. Heinz
G. Heinzelmann
G. Henri
G. Hermann
A. Hillert
James Anthony Hinton
W. Hofmann
P. Hofverberg
Markus Holler
D. Horns
A. Jacholkowska
C. Jahn
M. Jamrozy
I. Jung
M. A. Kastendieck
K. Katarzynski
U. Katz
S. Kaufmann
B. Khelifi
S. Klepser
D. Klochkov
W. Kluzniak
T. Kneiske
Nu. Komin
K. Kosack
R. Kossakowski
F. Krayzel
P. P. Krueger
H. Laffon
G. Lamanna
J. Lefaucheur
M. Lemoine-Goumard
J. -P. Lenain
D. Lennarz
T. Lohse
A. Lopatin
C. -C. Lu
V. Marandon
A. Marcowith
J. Masbou
G. Maurin
N. Maxted
M. Mayer
T. J. L. McComb
M. C. Medina
J. Mehault
U. Menzler
R. Moderski
M. Mohamed
E. Moulin
C. L. Naumann
M. Naumann-Godo
M. de Naurois
D. Nedbal
N. Nguyen
J. Niemiec
S. J. Nolan
S. Ohm
E. de Ona Wilhelmi
B. Opitz
M. Ostrowski
I. Oya
M. Panter
R. D. Parsons
M. Paz Arribas
N. W. Pekeur
G. Pelletier
J. Perez
P. -O. Petrucci
B. Peyaud
S. Pita
G. Puehlhofer
M. Punch
A. Quirrenbach
S. Raab
M. Raue
A. Reimer
O. Reimer
M. Renaud
R. de los Reyes
F. Rieger
J. Ripken
L. Rob
S. Rosier-Lees
G. Rowell
B. Rudak
C. B. Rulten
V. Sahakian
David M. Sanchez
A. Santangelo
R. Schlickeiser
A. Schulz
U. Schwanke
S. Schwarzburg
S. Schwemmer
F. Sheidaei
J. L. Skilton
H. Sol
G. Spengler
L. Stawarz
R. Steenkamp
Christian Stegmann
F. Stinzing
K. Stycz
Iurii Sushch
A. Szostek
J. -P. Tavernet
R. Terrier
M. Tluczykont
C. Trichard
K. Valerius
C. van Eldik
G. Vasileiadis
C. Venter
A. Viana
P. Vincent
H. J. Voelk
F. Volpe
S. Vorobiov
M. Vorster
S. J. Wagner
M. Ward
R. White
A. Wierzcholska
D. Wouters
M. Zacharias
A. Zajczyk
A. A. Zdziarski
Alraune Zech
H. S. Zechlin
eng
uncontrolled
gamma rays: galaxies
eng
uncontrolled
quasars: individual: PKS 1510-089
eng
uncontrolled
infrared: diffuse background
Institut für Physik und Astronomie
Referiert