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1. Full Text Observational constraints on energetic particle diffusion in young supernovae remnants: Amplified magnetic field and maximum energy
by Parizot, E and Marcowith, A and Ballet, J and Gallant, Y.A
Astronomy and Astrophysics, ISSN 0004-6361, 2006, Volume 453, Issue 2, pp. 387 - 395
Constraints on the diffusion and acceleration parameters in five young supernova remnants (SNRs) are derived from the observed thickness of their X-ray rims,... 
ISM: supernova remnants | Acceleration of particles | Magnetic fields | Cosmic rays | ISM : supernova remnants | DISTANCE | magnetic fields | COSMIC-RAY ACCELERATION | SHELL | acceleration of particles | CASSIOPEIA-A | SN-1006 | SHOCK ACCELERATION | AMPLIFICATION | cosmic rays | ASTRONOMY & ASTROPHYSICS | EXPANSION | EMISSION
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2. Full Text Multi-messenger Observations of a Binary Neutron Star Merger
by Scholten, Olaf and van den Berg, Aiaan and Las Cumbres Observatory Grp and ATCA Australia Telescope and LIGO Sci Collaboration & Virgo and KU Collaboration and GROUND and RIMAS RATIR and AGILE Team and ASKAP Australian SKA Pathfinder and IPN Collaboration and LOFAR Collaboration and Salt Grp and VINROUGE Collaboration and Nordic Optical Telescope and MAXI Team and Fermi GBM and Fermi Large Area Telescope and J-GEM and IceCube Collaboration and BOOTES Collaboration and Pi Sky Collaboration and Pan-STARRS and LWA Long Wavelength Array and SKA South Africa MeerKAT and CALET Collaboration and AstroSat Cadmium Zinc Telluride and HAWC Collaboration and GROWTH JAGWAR CALTECH and ATLAS and ePESSTO and DFN Desert Fireball Network and Insight-Hxmt Collaboration and Texas Tech Univ and MASTER Collaboration and TZAC Consortium and Dark Energy Camera GW-EM and GRAWITA GRAvitational Wave and INTERGRAL and Toros Transient Robotic Observat and Chandra Team McGill Univ and H E S S Collaboration and Swift Collaboration and Pierre Auger Collaboration and OzGrav DWF Deeper Wider Faster and IKI-GW Follow-up Collaboration and Euro VLBI Team and High Time Resolution Universe and ANTARES Collaboration and DLT40 Collaboration and ALMA Collaboration and The 1M2H Team and MWA Murchison Widefield Array and The Insight-HXMT Collaboration and The MAXI Team and The Swift Collaboration and The Fermi Large Area Telescope Collaboration and GROND and TOROS: Transient Robotic Observatory of the South Collaboration and Texas Tech University and OzGrav, DWF (Deeper, Wider, Faster program), AST3, and CAASTRO Collaborations and MWA: Murchison Widefield Array and GROWTH, JAGWAR, Caltech-NRAO, TTU-NRAO, and NuSTAR Collaborations and INTEGRAL and RIMAS and RATIR and Pi of the Sky Collaboration and The Chandra Team at McGill University and LWA: Long Wavelength Array and The DLT40 Collaboration and DFN: Desert Fireball Network and LIGO Scientific Collaboration and Virgo Collaboration and ASKAP: Australian SKA Pathfinder and AstroSat Cadmium Zinc Telluride Imager Team and The BOOTES Collaboration and The Pierre Auger Collaboration and ATCA: Australia Telescope Compact Array and SALT Group and H.E.S.S. Collaboration and The Dark Energy Camera GW-EM Collaboration and the DES Collaboration and High Time Resolution Universe Survey and Las Cumbres Observatory Group and GRAWITA: GRAvitational Wave Inaf TeAm and The VINROUGE Collaboration and The CALET Collaboration and SLAC National Accelerator Lab., Menlo Park, CA (United States) and Brookhaven National Lab. (BNL), Upton, NY (United States) and Los Alamos National Lab. (LANL), Los Alamos, NM (United States) and Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States) and Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States) and Lawrence Berkeley National Laboratory-National Energy Research Scientific Computing Center (NERSC) and Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States) and Fysikum and Naturvetenskapliga fakulteten and Institutionen för astronomi and Stockholms universitet and Oskar Klein-centrum för kosmopartikelfysik (OKC)
Astrophysical Journal Letters, ISSN 2041-8205, 10/2017, Volume 848, Issue 2, p. L12
On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational... 
Stars: neutron | Gravitational waves | GAMMA-RAY BURST | NEARBY SUPERNOVA RATES | AFTERGLOW | PULSAR | stars: neutron | EVOLUTION | GRAVITATIONAL-WAVES | ASTRONOMY & ASTROPHYSICS | gravitational waves | REDSHIFT | IMAGER | NUCLEOSYNTHESIS | HOST GALAXY | Astrofísica | Astrophysics | Ones gravitacionals | Astronomia i astrofísica | Astronomia | Raigs gamma | Astronomy | Àrees temàtiques de la UPC | Física | Gamma ray astronomy | ASTRONOMY AND ASTROPHYSICS | Fysik | Physical Sciences | Naturvetenskap | Natural Sciences
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3. Full Text Acceleration of petaelectronvolt protons in the Galactic Centre
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 and Linnéuniversitetet and Institutionen för fysik och elektroteknik (IFE) and Fakulteten för teknik (FTK)
Nature, ISSN 0028-0836, 03/2016, Volume 531, Issue 7595, pp. 476 - 478
Galactic cosmic rays reach energies of at least a few petaelectronvolts(1) (of the order of 1015 electronvolts). This implies that our Galaxy contains... 
ORIGIN | GAMMA-RAY EMISSION | MOLECULAR CLOUDS | SUPERNOVA-REMNANTS | MULTIDISCIPLINARY SCIENCES | CENTER REGION | X-RAY | CENTER RIDGE | MASSIVE BLACK-HOLE | MAGNETIC-FIELD | COSMIC-RAYS | Protons | Usage | Particle accelerators | Properties | Cosmic rays | Astrophysics | Supernovae | Stars & galaxies | Physics - High Energy Astrophysical Phenomena | Physics | High Energy Astrophysical Phenomena | Fysik | Physical Sciences | Astronomi, astrofysik och kosmologi | Naturvetenskap | Astroparticle Physics | Natural Sciences | Astronomy, Astrophysics and Cosmology | Astropartikelfysik
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4. Full Text Multimessenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A
by Aartsen, M.G and Ackermann, M and Adams, J and Aguilar, J.A and Ahlers, M and Ahrens, M and Al Samarai, I and Altmann, D and Andeen, K and Anderson, T and Ansseau, I and Anton, G and Argüelles, C and Auffenberg, J and Axani, S and Bagherpour, H and Bai, X and Barron, J.P and Barwick, S.W and Baum, V and Bay, R and Beatty, J.J and Becker Tjus, J and Becker, K.-H and Benzvi, S and Berley, D and Bernardini, E and Besson, D.Z and Binder, G and Bindig, D and Blaufuss, E and Blot, S and Bohm, C and Börner, M and Bos, F and Böser, S and Botner, O and Bourbeau, E and Bourbeau, J and Bradascio, F and Braun, J and Brenzke, M and Bretz, H.-P and Bron, S and Brostean-Kaiser, J and Burgman, A and Busse, R.S and Carver, T and Cheung, E and Chirkin, D and Christov, A and Clark, K and Classen, L and Coenders, S and Collin, G.H and Conrad, J.M and Coppin, P and Correa, P and Cowen, D.F and Cross, R and Dave, P and Day, M and de André, J.P.A.M and De Clercq, C and Delaunay, J.J and Dembinski, H and De Ridder, S and Desiati, P and de Vries, K.D and de Wasseige, G and de With, M and Deyoung, T and Díaz-Vélez, J.C and Di Lorenzo, V and Dujmovic, H and Dumm, J.P and Dunkman, M and Dvorak, E and Eberhardt, B and Ehrhardt, T and Eichmann, B and Eller, P and Evenson, P.A and Fahey, S and Fazely, A.R and Felde, J and Filimonov, K and Finley, C and Flis, S and Franckowiak, A and Friedman, E and Fritz, A and Gaisser, T.K and Gallagher, J and Gerhardt, L and Ghorbani, K and Glauch, T and Glüsenkamp, T and Goldschmidt, A and Gonzalez, J.G and ... and VERITAS and HESS and Kapteyn and ASAS-SN and IceCube Collaboration and MAGIC Collaboration and Liverpool Telescope and HAWC and Fermi-LAT Collaboration and AGILE and Swift NuSTAR and INTEGRAL and Kanata, Kiso Subaru Observing Te and VLA 17B-403 Team and Subaru and Kanata and Kiso and Fermi-LAT and H.E.S.S and VLA/17B-403 teams and MAGIC and Swift/NuSTAR and The IceCube Collaboration and SLAC National Accelerator Lab., Menlo Park, CA (United States) and Fysikum and Naturvetenskapliga fakulteten and Nordiska institutet för teoretisk fysik (Nordita) and Stockholms universitet and Oskar Klein-centrum för kosmopartikelfysik (OKC)
Science, ISSN 0036-8075, 07/2018, Volume 361, Issue 6398, p. eaat1378
Previous detections of individual astrophysical sources of neutrinos are limited to the Sun and the supernova 1987A, whereas the origins of the diffuse flux of... 
ORIGIN | TELESCOPE | SPECTROGRAPH | PERFORMANCE | MULTIDISCIPLINARY SCIENCES | Sky | Red shift | Atmospheric models | Gravitational waves | Spatial discrimination | Luminosity | Emission | Activation | Waves | Cosmic radiation | Cosmic rays | Energy | Radio sources (astronomy) | Cooperation | Neutrinos | Gravity | Fluctuations | Statistical analysis | Electromagnetic radiation | Blazars | Universe | Photons | Line of sight | Relativistic effects | Emissions | Gamma rays | Observatories | X rays | Wavelengths | Collaboration | Telescopes | Relativism | Acceleration | Astronomy | Tracers | ASTRONOMY AND ASTROPHYSICS | Fysik | Physical Sciences | Naturvetenskap | Natural Sciences
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5. Full Text Search for Dark Matter Annihilations towards the Inner Galactic Halo from 10 Years of Observations with H.E.S.S
by Abdallah, H and Abramowski, A and Aharonian, F and Ait Benkhali, F and Akhperjanian, A.G and Angüner, E and Arrieta, M and Aubert, P and Backes, M and Balzer, A and Barnard, M and Becherini, Y and Becker Tjus, J and Berge, D and Bernhard, S and Bernlöhr, K and Birsin, E 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 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 Couturier, C and Cui, Y and Davids, I.D and Degrange, B and Deil, C and Dewilt, P and Djannati-Ataï, 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 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 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 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 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 Jogler, T and Jouvin, L and ... and HESS Collaboration and H.E.S.S. Collaboration and Linnéuniversitetet and Institutionen för fysik och elektroteknik (IFE) and Fakulteten för teknik (FTK)
Physical Review Letters, ISSN 0031-9007, 09/2016, Volume 117, Issue 11, p. 111301
The inner region of the Milky Way halo harbors a large amount of dark matter (DM). Given its proximity, it is one of the most promising targets to look for DM.... 
ENERGY GAMMA-RAYS | SPECTRUM | PHYSICS, MULTIDISCIPLINARY | EMISSION | Galactic halos | Dark matter | Brackets | Searching | Milky Way Galaxy | Density | Cross sections | Channels | Physics - High Energy Astrophysical Phenomena | Physics | Astrophysics | High Energy Astrophysical Phenomena | Fysik | Physical Sciences | Astronomi, astrofysik och kosmologi | Naturvetenskap | Astroparticle Physics | Natural Sciences | Astronomy, Astrophysics and Cosmology | Astropartikelfysik
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