Very-high-energy particle acceleration powered by the jets of the microquasar SS 433
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J. C. Arteaga-Velázquez | S. BenZvi | I. Taboada | S. Westerhoff | J. Wood | G. Yodh | R. Springer | M. Castillo | G. Kunde | J. García-González | B. Dingus | R. Ellsworth | A. Smith | M. Rosenberg | K. Engel | H. A. Solares | C. Brisbois | H. Fleischhack | J. P. Harding | A. Albert | A. Iriarte | L. Villaseñor | P. Hüntemeyer | L. Nellen | A. Zepeda | A. Sandoval | E. Belmont-Moreno | H. L. Vargas | R. Arceo | G. Sinnis | R. Lauer | R. Alfaro | C. Hui | M. Mostafá | K. Caballero-Mora | M. DuVernois | S. Casanova | M. González | R. López-Coto | O. Tibolla | K. Malone | A. Abeysekara | P. Kar | G. Vianello | C. Álvarez | J. Álvarez | T. Capistrán | A. Carramiñana | U. Cotti | J. Cotzomi | C. D. León | E. D. L. Fuente | S. Dichiara | N. Fraija | F. Garfias | Z. Hampel-Arias | S. Hernández | B. Hona | F. Hueyotl-Zahuantitla | A. Jardin-Blicq | S. Kaufmann | A. Longinotti | G. Luis-Raya | S. Marinelli | O. Martinez | I. Martinez-Castellanos | J. Martínez-Castro | P. Miranda-Romagnoli | E. Moreno | A. Nayerhoda | M. Newbold | M. Nisa | R. Noriega-Papaqui | J. Pretz | E. Pérez-Pérez | Z. Ren | C. Rho | C. Rivière | E. Ruiz-Velasco | F. Greus | M. Arroyo | P. Surajbali | I. Torres | T. Weisgarber | T. Yapici | H. Zhou | F. Werner | H. Schoorlemmer | C. Espinoza | Michael Schneider | J. Linnemann | J. Matthews | S. León | A. Galván-Gámez | M. U. Nisa | J. Hinton | D. Rojas | D. Rosa-González | V. Joshi | J. Goodman | J. C. Diaz-Velez | Ke Fang | William H. Lee | Hui Li | A. González-Muñoz | K. Tollefson | Haocheng Zhang | J. C. Díaz-Vélez | H. Solares
[1] J. C. Arteaga-Velázquez,et al. Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth , 2017, Science.
[2] S. BenZvi,et al. Effect of the diffusion parameters on the observed γ -ray spectrum of sources and their contribution to the local all-electron spectrum: The EDGE code , 2017, Astroparticle Physics.
[3] P. Kar,et al. VERITAS Observations of High-Mass X-Ray Binary SS 433 , 2017, 1708.04967.
[4] Landessternwarte,et al. Constraints on particle acceleration in SS433/W50 from MAGIC and H.E.S.S. observations , 2017, 1707.03658.
[5] J. A. Garc'ia-Gonz'alez,et al. The 2HWC HAWC Observatory Gamma-Ray Catalog , 2017, 1702.02992.
[6] O. Tibolla,et al. Observation of the Crab Nebula with the HAWC Gamma-Ray Observatory , 2017, 1701.01778.
[7] Merate,et al. UvA-DARE ( Digital Academic Repository ) Relativistic Jets in Active Galactic Nuclei and , 2016 .
[8] James Michael Burgess,et al. The Multi-Mission Maximum Likelihood framework , 2016 .
[9] A. Panferov. Jets of SS 433 on scales of dozens of parsecs , 2016, 1607.02043.
[10] E. Pueschel,et al. EXCEPTIONALLY BRIGHT TEV FLARES FROM THE BINARY LS I +61° 303 , 2016, 1601.01812.
[11] J. Gladstone,et al. WATCHDOG: A COMPREHENSIVE ALL-SKY DATABASE OF GALACTIC BLACK HOLE X-RAY BINARIES , 2015, 1512.00778.
[12] H. A. Solares,et al. A high-level analysis framework for HAWC , 2015, 1508.07479.
[13] Andrew J A C Smith. HAWC: Design, Operation, Reconstruction and Analysis , 2015, 1508.05826.
[14] S. Fabrika,et al. Supercritical accretion disks in ultraluminous X-ray sources and SS 433 , 2015, Nature Physics.
[15] F. Aharonian,et al. DETECTION OF PERSISTENT GAMMA-RAY EMISSION TOWARD SS433/W50 , 2014, 1411.7413.
[16] G. Richards,et al. MULTIWAVELENGTH OBSERVATIONS OF THE TeV BINARY LS I +61° 303 WITH VERITAS, Fermi-LAT, AND Swift/XRT DURING A TeV OUTBURST , 2013, 1310.7913.
[17] R. Sagdeev,et al. ANALYTIC SOLUTION FOR SELF-REGULATED COLLECTIVE ESCAPE OF COSMIC RAYS FROM THEIR ACCELERATION SITES , 2012, The Astrophysical journal.
[18] C. Dermer,et al. COSMIC-RAY ELECTRON EVOLUTION IN THE SUPERNOVA REMNANT RX J1713.7−3946 , 2012, 1203.4242.
[19] Daniel Foreman-Mackey,et al. emcee: The MCMC Hammer , 2012, 1202.3665.
[20] K. Nishijima,et al. Search for VHE gamma rays from SS433/W50 with the CANGAROO-II telescope , 2009, 0909.0133.
[21] G. E. Romero,et al. Production of gamma rays and neutrinos in the dark jets of the microquasar SS433 , 2008, 0801.2903.
[22] Japan.,et al. XMM-Newton observations of the eastern jet of SS 433 , 2006, astro-ph/0610781.
[23] E. Amato,et al. Non-linear particle acceleration at non-relativistic shock waves in the presence of self-generated turbulence , 2006, astro-ph/0606592.
[24] N Tonello,et al. Variable Very-High-Energy Gamma-Ray Emission from the Microquasar LS I +61 303 , 2006, Science.
[25] A. R. King,et al. The nature of SS433 and the ultraluminous X-ray sources , 2006, astro-ph/0604497.
[26] A. Strong,et al. Dissipation of Magnetohydrodynamic Waves on Energetic Particles: Impact on Interstellar Turbulence and Cosmic-Ray Transport , 2005, astro-ph/0510335.
[27] W. Rhode,et al. TeV gamma-ray observations of SS-433 and a survey of the surrounding field with the HEGRA IACT-system , 2005 .
[28] A. R. Bazer-Bachi,et al. Discovery of Very High Energy Gamma Rays Associated with an X-ray Binary , 2005, Science.
[29] F. Aharonian,et al. Klein-Nishina effects in the spectra of non-thermal sources immersed in external radiation fields , 2005, astro-ph/0504388.
[30] R. Sunyaev,et al. INTEGRAL observations of SS433: Results of a coordinated campaign , 2005, astro-ph/0503352.
[31] K. Gorski,et al. HEALPix: A Framework for High-Resolution Discretization and Fast Analysis of Data Distributed on the Sphere , 2004, astro-ph/0409513.
[32] S. Fabrika,et al. The Jets and Supercritical Accretion Disk in SS433 , 2004 .
[33] S. Migliari,et al. Iron Emission Lines from Extended X-ray Jets in SS 433: Reheating of Atomic Nuclei , 2002, Science.
[34] P. B. Cameron,et al. Twenty Years of Timing SS 433 , 2001, astro-ph/0107296.
[35] I. Mirabel,et al. Mid-Infrared observations of GRS 1915+105 and SS433 , 2000, astro-ph/0011213.
[36] R. Petre,et al. Rossi X-Ray Timing Explorer Observations of the Eastern Lobe of W50 Associated with SS 433 , 1999 .
[37] I. Mirabel,et al. Sources of Relativistic Jets in the Galaxy , 1999, astro-ph/9902062.
[38] R. Cousins,et al. A Unified Approach to the Classical Statistical Analysis of Small Signals , 1997, physics/9711021.
[39] H. Ögelman,et al. ROSAT and ASCA Observations of W50 Associated with the Peculiar Source SS 433 , 1997 .
[40] N. Kawai,et al. ROSAT OBSERVATIONS OF THE W 50/SS 433 SYSTEM , 1996 .
[41] Alan D. Martin,et al. Review of Particle Physics , 2000, Physical Review D.
[42] S. Anderson,et al. Ten Years of SS 433 Kinematics , 1989 .
[43] V. Kornilov,et al. WBVR photometry of SS 433: spectra of the ''normal'' star and the accretion disk , 1982 .
[44] M. Dopita,et al. The interaction between the relativistic jets of SS433 and the interstellar medium , 1980 .
[45] S. S. Wilks. The Large-Sample Distribution of the Likelihood Ratio for Testing Composite Hypotheses , 1938 .
[46] Helmuth Spieler,et al. Big Bang Nucleosynthesis (in "The Review of Particle Properties" 2004) , 2004, astro-ph/0406663.
[47] The 28th International Cosmic Ray Conference 1 , 2003 .
[48] Bruce Margon,et al. Observations of SS 433 , 1984 .