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by Abdalla, H and Abramowski, A and Aharonian, F and Benkhali, F. Ait and Angüner, E. O and Arakawa, M and Arrieta, M and Aubert, P and Backes, M and Balzer, A and Barnard, M and Becherini, Y and Tjus, J. Becker and Berge, D and Bernhard, S and Bernlöhr, K and Blackwell, R and Böttcher, M and Boisson, C and Bolmont, J and Bonnefoy, S and Bordas, P and Bregeon, J and Brun, F and Brun, P and Bryan, M and Büchele, M and Bulik, T and Capasso, M and Carrigan, S and Caroff, S and Carosi, A and Casanova, S and Cerruti, M and Chakraborty, N and Chaves, R. C. G and Chen, A and Chevalier, J and Colafrancesco, S and Condon, B and Conrad, J and Davids, I. D and Decock, J and Deil, C and Devin, J and deWilt, P and Dirson, L and Djannati-Ataï, A and Domainko, W and Donath, A and Drury, L. O’C and Dutson, K and Dyks, J and Edwards, T and Egberts, K and Eger, P and Emery, G and Ernenwein, J.-P and Eschbach, S and Farnier, C and Fegan, S and Fernandes, M. V and Fiasson, A and Fontaine, G and Förster, A and Funk, S and Füßling, M and Gabici, S and Gallant, Y. A and Garrigoux, T and Gast, H and Gaté, F and Giavitto, G and Giebels, B and Glawion, D and Glicenstein, J. F and Gottschall, D and Grondin, M.-H and Hahn, J and Haupt, M and Hawkes, J and Heinzelmann, G and Henri, G and Hermann, G and Hinton, J. A and Hofmann, W and Hoischen, C and Holch, T. L and Holler, M and Horns, D and Ivascenko, A and Iwasaki, H and Jacholkowska, A and Jamrozy, M and Jankowsky, D and Jankowsky, F and Jingo, M and Jouvin, L and Jung-Richardt, I and Kastendieck, M. A and ... and H E S S Collaboration and H.E.S.S. Collaboration
Astronomy and astrophysics (Berlin), ISSN 1432-0746, 04/2018, Volume 612, p. A1
Journal Article
by F. Aharonian and A. G. Akhperjanian and K. -M. Aye and A. R. Bazer-Bachi and M. Beilicke and W. Benbow and D. Berge and P. Berghaus and K. Bernlöhr and C. Boisson and O. Bolz and C. Borgmeier and I. Braun and F. Breitling and A. M. Brown and J. Bussons Gordo and P. M. Chadwick and L. -M. Chounet and R. Cornils and L. Costamante and B. Degrange and A. Djannati-Ataï and L. O'C. Drury and G. Dubus and T. Ergin and P. Espigat and F. Feinstein and P. Fleury and G. Fontaine and S. Funk and Y. A. Gallant and B. Giebels and S. Gillessen and P. Goret and C. Hadjichristidis and M. Hauser and G. Heinzelmann and G. Henri and G. Hermann and J. A. Hinton and W. Hofmann and M. Holleran and D. Horns and O. C. de Jager and I. Jung and B. Khélifi and Nu. Komin and A. Konopelko and I. J. Latham and R. Le Gallou and A. Lemière and M. Lemoine and N. Leroy and T. Lohse and A. Marcowith and C. Masterson and T. J. L. McComb and M. de Naurois and S. J. Nolan and A. Noutsos and K. J. Orford and J. L. Osborne and M. Ouchrif and M. Panter and G. Pelletier and S. Pita and G. Pühlhofer and M. Punch and B. C. Raubenheimer and M. Raue and J. Raux and S. M. Rayner and I. Redondo and A. Reimer and O. Reimer and J. Ripken and L. Rob and L. Rolland and G. Rowell and V. Sahakian and L. Saugé and S. Schlenker and R. Schlickeiser and C. Schuster and U. Schwanke and M. Siewert and H. Sol and R. Steenkamp and C. Stegmann and J. -P. Tavernet and R. Terrier and C. G. Théoret and M. Tluczykont and D. J. van der Walt and G. Vasileiadis and C. Venter and P. Vincent and B. Visser and H. J. Völk and S. J. Wagner
Science (American Association for the Advancement of Science), ISSN 0036-8075, 3/2005, Volume 307, Issue 5717, pp. 1938 - 1942
Journal Article
by Acciari, V.A and Aliu, E and Arlen, T and Bautista, M and Beilicke, M and Benbow, W and Bradbury, S.M and Buckley, J.H and Bugaev, V and Butt, Y and Byrum, K and Cannon, A and Celik, O and Cesarini, A and Chow, Y.C and Ciupik, L and Cogan, P and Cui, W and Dickherber, R and Fegan, S.J and Finley, J.P and Fortin, P and Fortson, L and Fumiss, A and Gall, D and Gillanders, G.H and Grube, J and Guenette, R and Gyuk, G and Hanna, D and Holder, J and Horan, D and Hui, C.M and Humensky, T.B and Imran, A and Kaaret, P and Karlsson, N and Kieda, D and Kildea, J and Konopelko, A and Krawczynski, H and Krennrich, F and Lang, M.J and LeBohec, S and Maier, G and McCann, A and McCutcheon, M and Millis, J and Moriarty, P and Ong, R.A and Otte, A.N and Pandel, D and Perkins, J.S and Petry, D and Pohl, M and Quinn, J and Ragan, K and Reyes, L.C and Reynolds, P.T and Roache, E and Roache, E and Rose, H.J and Schroedter, M and Sembroski, G.H and Smith, A.W and Swordy, S.P and Theiling, M and Toner, J.A and Varlotta, A and Vincent, S and Wakely, S.P and Ward, J.E and Weekes, T.C and Weinstein, A and Williams, D.A and Wissel, S and Wood, M and Waiker, R.C and Davies, F and Hardee, P.E and Junor, W and Ly, C and Aharonian, F and Akhperjanian, A.G and Anton, G and De Almeida, U. Barres and Bazer-Bachi, A.R and Becherini, Y and Behera, B and Bemlöhr, K and Bochow, A and Boisson, C and Bolmont, J and Borrel, V and Brucker, J and Brun, F and Brun, P and Bühler, R and Bulik, T and Büsching, I and ... and VERITAS Collaboration and HESS Collaboration and MAGIC Collaboration and VLBA 43 Ghz M87 Monitoring Team and H.E.S.S. Collaboration and VLBA 43 GHz M87 Monitoring Team and the MAGIC Collaboration and The VERITAS Collaboration and the VLBA 43 GHz M87 Monitoring Team and the H.E.S.S. Collaboration
Science (American Association for the Advancement of Science), ISSN 0036-8075, 7/2009, Volume 325, Issue 5939, pp. 444 - 448
Journal Article
by Abdalla, H and Aharonian, F and Benkhali, F. Ait and Angüner, E. O and Arakawa, M and Arcaro, C and Armand, C and Arrieta, M and Backes, M and Barnard, M and Becherini, Y and Tjus, J. Becker and Berge, D and Bernhard, S and Bernlöhr, K and Blackwell, R and Böttcher, M and Boisson, C and Bolmont, J and Bonnefoy, S and Bordas, P and Bregeon, J and Brun, F and Brun, P and Bryan, M and Büchele, M and Bulik, T and Bylund, T and Capasso, M and Caroff, S and Carosi, A and Cerruti, M and Chakraborty, N and Chandra, S and Chaves, R. C. G and Chen, A and Colafrancesco, S and Condon, B and Davids, I. D and Deil, C and Devin, J and deWilt, P and Dirson, L and Djannati-Ataï, A and Dmytriiev, A and Donath, A and Doroshenko, V and Drury, L. O’C and Dyks, J and Egberts, K and Emery, G and Ernenwein, J.-P and Eschbach, S and Fegan, S and Fiasson, A and Fontaine, G and Funk, S and Füßling, M and Gabici, S and Gallant, Y. A and Gaté, F and Giavitto, G and Glawion, D and Glicenstein, J. F and Gottschall, D and Grondin, M.-H and Hahn, J and Haupt, M and Heinzelmann, G and Henri, G and Hermann, G and Hinton, J. A and Hofmann, W and Hoischen, C and Holch, T. L and Holler, M and Horns, D and Huber, D and Iwasaki, H and Jacholkowska, A and Jamrozy, M and Jankowsky, D and Jankowsky, F and Jouvin, L and Jung-Richardt, I and Kastendieck, M. A and Katarzyński, K and Katsuragawa, M and Katz, U and Kerszberg, D and Khangulyan, D and Khélifi, B and King, J and Klepser, S and Kluźniak, W and Komin, Nu and Kosack, K and Krakau, S and Kraus, M and Krüger, P. P and ... and H.E.S.S. Collaboration
The Astrophysical journal, ISSN 1538-4357, 01/2019, Volume 870, Issue 2, p. 93
The blazar Mrk 501 (z = 0.034) was observed at very-high-energy (VHE, E ≳ 100 GeV) gamma-ray wavelengths during a bright flare on the night of 2014 June 23–24... 
astroparticle physics | BL Lacertae objects: individual (Mrk 501) | gamma rays: galaxies | Gamma rays | Confidence intervals | Time dependence | Wavelengths | Energy | Night | Telescopes | Attenuation | Photons | Spectra | Invariance | Power law | Physics - High Energy Astrophysical Phenomena
Journal Article
by Abramowski, A and Acero, F and Aharonian, F and Akhperjanian, A.G and Anton, G and Balenderan, S and Balzer, A and Barnacka, A and Becherini, Y and Becker Tjus, J and Bernlöhr, K and Birsin, E and Biteau, J and Bochow, A and Boisson, C and Bolmont, J and Bordas, P and Brucker, J and Brun, F and Brun, P and Bulik, T and Carrigan, S and Casanova, S and Cerruti, M and Chadwick, P.M and Chaves, R.C.G and Cheesebrough, A and Colafrancesco, S and Cologna, G and Conrad, J and Couturier, C and Dalton, M and Daniel, M.K and Davids, I.D and Degrange, B and Deil, C and Dewilt, P and Dickinson, H.J and Djannati-Ataï, A and Domainko, W and Drury, L.O'C and Dubus, G and Dutson, K and Dyks, J and Dyrda, M and Egberts, K and Eger, P and Espigat, P and Fallon, L and Farnier, C and Fegan, S and Feinstein, F and Fernandes, M.V and Fernandez, D and Fiasson, A and Fontaine, G and Förster, A and Füßling, M and Gajdus, M and Gallant, Y.A and Garrigoux, T and Gast, H and Giebels, B and Glicenstein, J.F and Glück, B and Göring, D and Grondin, M.-H and Häffner, S and Hague, J.D and Hahn, J and Hampf, D and Harris, J and Heinz, S and Heinzelmann, G and Henri, G and Hermann, G and Hillert, A and Hinton, J.A and Hofmann, W and Hofverberg, P and Holler, M and Horns, D and Jacholkowska, A and Jahn, C and Jamrozy, M and Jung, I and Kastendieck, M.A and Katarzyński, K and Katz, U and Kaufmann, S and Khélifi, B and Klepser, S and Klochkov, D and Kluåniak, W and Kneiske, T and Komin, Nu and Kosack, K and Kossakowski, R and Krayzel, F and Krüger, P.P and ... and HESS Collaboration
Physical review letters, ISSN 0031-9007, 01/2013, Volume 110, Issue 4, pp. 041301 - 041301
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... 
Physics, Multidisciplinary | Physical Sciences | Physics | Science & Technology
Journal Article
by Abdalla, H and Abramowski, A and Aharonian, F and Benkhali, F. Ait and Akhperjanian, A. G and Andersson, T and Angüner, E. O and Arrieta, M and Aubert, P and Backes, M and Balzer, A and Barnard, M and Becherini, Y and Tjus, J. Becker and Berge, D and Bernhard, S and Bernlöhr, K and Blackwell, R and Böttcher, M and Boisson, C and Bolmont, J and Bordas, P and Bregeon, J and Brun, F and Brun, P and Bryan, M and Bulik, T and Capasso, M and Carr, J and Casanova, S and Cerruti, M and Chakraborty, N and Chalme-Calvet, R and Chaves, R. C.G and Chen, A and Chevalier, J and Chrétien, M and Colafrancesco, S and Cologna, G and Condon, B and Conrad, J and Cui, Y and Davids, I. D and Decock, J and Degrange, B and Deil, C and Devin, J and deWilt, P and Dirson, L and Djannati-Ataï, A and Domainko, W and Donath, A and Drury, L.O’C and Dubus, G and Dutson, K and Dyks, J and Edwards, T and Egberts, K and Eger, P and Ernenwein, J.-P and Eschbach, S and Farnier, C and Fegan, S and Fernandes, M. V and Fiasson, A and Fontaine, G and Förster, A and Fukuyama, T and Funk, S and Füßling, M and Gabici, S and Gajdus, M and Gallant, Y. A and Garrigoux, T and Giavitto, G and Giebels, B and Glicenstein, J. F and Gottschall, D and Goyal, A and Grondin, M.-H and Hadasch, D and Hahn, J and Haupt, M and Hawkes, J and Heinzelmann, G and Henri, G and Hermann, G and Hervet, O and Hinton, J. A and Hofmann, W and Hoischen, C and Holler, M and Horns, D and Ivascenko, A and Jacholkowska, A and Jamrozy, M and Janiak, M and Jankowsky, D and Jankowsky, F and Jingo, M and ... and H E S S Collaboration and H.E.S.S. Collaboration
Astronomy and astrophysics (Berlin), ISSN 1432-0746, 04/2018, Volume 612, p. A6
Journal Article
by Abramowski, A and Aharonian, F and Benkhali, F. Ait and Akhperjanian, A.G and Anguner, E.O and Backes, M and Balzer, A and Becherini, Y and Tjus, J. Becker and Berge, D and Bernhard, S and Bernlohr, K and Birsin, E and Blackwell, R and Bottcher, M and Boisson, C and Bolmont, J and Bordas, P and Bregeon, J and Brun, F and Brun, P and Bryan, M and Bulik, T and Carr, J and Casanova, S and Chakraborty, N and Chalme-Calvet, R and Chaves, R.C.G and Chen, A and Chretien, M and Colafrancesco, S and Cologna, G and Conrad, J and Couturier, C and Cui, Y and Davids, I.D and Degrange, B and Deil, C and DeWilt, P and Djannati-Atai, A and Domainko, W and Donath, A and Drury, L.O and Dubus, G and Dutson, K and Dyks, J and Dyrda, M and Edwards, T and Egberts, K and Eger, P and Ernenwein, J.-P and Espigat, P and Farnier, C and Fegan, S and Feinstein, F and Fernandes, M.V and Fernandez, D and Fiasson, A and Fontaine, G and Forster, A and Fusling, M and Gabici, S and Gajdus, M and Gallant, Y.A and Garrigoux, T and Giavitto, G and Giebels, B and Glicenstein, J.F and Gottschall, D and Goyal, A and Grondin, M.-H and Grudzińska, M and Hadasch, D and Haffner, S and Hahn, J and Hawkes, J and Heinzelmann, G and Henri, G and Hermann, G and Hervet, O and Hillert, A and Hinton, J.A and Hofmann, W and Hofverberg, P and Hoischen, C and Holler, M and Horns, D and Ivascenko, A and Jacholkowska, A and Jamrozy, M and Janiak, M and Jankowsky, F and Jung-Richardt, I and Kastendieck, M.A and Katarzyński, K and Katz, U and Kerszberg, D and Khelifi, B and Kieffer, M and Klepser, S and ... and HESS Collaboration
Nature (London), ISSN 1476-4687, 03/2016, Volume 531, Issue 7595, pp. 476 - 479
Galactic cosmic rays reach energies of at least a few petaelectronvolts(1) (of the order of 1015 electronvolts). This implies that our Galaxy contains... 
Science & Technology - Other Topics | Multidisciplinary Sciences | Science & Technology | Protons | Usage | Particle accelerators | Properties | Cosmic rays | Astrophysics | Supernovae | Stars & galaxies | Physics - High Energy Astrophysical Phenomena | Physics | High Energy Astrophysical Phenomena
Journal Article