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54 results on '"Lukas Nellen"'

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1. Limits on Diffuse Dark Matter with HAWC

2. Limits on the Diffuse Gamma-Ray Background with HAWC

3. CONSTRAINTS ON THE VERY HIGH ENERGY GAMMA-RAY EMISSION WITH HAWC

4. HAWC results on TeV emitting blazars

5. Studying High-Mass Microquasars with HAWC

6. Modeling the non-flaring VHE emission from M87 as detected by the HAWC gamma ray observatory

7. Study of the eHWC J1825-134 at the Highest Energy with HWAC

8. A GeV to TeV view of shell-type SNRs

9. Follow-up Analysis to Geminga's contribution to the Local Positron Excess with HAWC Gamma-Ray Observatory

10. Galactic Cosmic Ray increase associated to an interplanetary magnetic cloud observed by HAWC

11. Spectral and Energy Morphology Analysis Study of HAWC J2031+415

12. A search for spectral hardening in HAWC sources above 56 TeV

13. Particle Acceleration in the Cygnus Superbubble

14. Characterizing gamma-ray sources with HAL (HAWC Accelerated likelihood) and 3ML

15. Search for TeV decaying dark matter from the Virgo cluster of galaxies

16. The Ultra-High-Energy Source MGRO J1908+06

17. Evidence of 200 TeV photons from HAWC J1825-134

18. HAWC J2227+610 and its association with G106.3+2.7, a new potential Galactic PeVatron

19. Constraining the local burst rate density of primordial black holes with HAWC

20. Combined Dark Matter searches towards dwarf spheroidal galaxies with Fermi-LAT, HAWC, HESS, MAGIC and VERITAS

21. Interplanetary Magnetic Flux Rope Observed at Ground Level by HAWC

22. Search for UHE neutrinos in coincidence with LIGO GW150914 event with the Pierre Auger Observatory

23. Combined Analysis of Cosmic-Ray Anisotropy with IceCube and HAWC

24. Search for very-high-energy emission from Gamma-ray Bursts using the first 18 months of data from the HAWC Gamma-ray Observatory

25. Searching for dark matter sub-structure with HAWC

26. Evidence for a mixed mass composition at the 'ankle' in the cosmic-ray spectrum

27. Search for TeV Gamma-Ray Emission from Point-like Sources in the Inner Galactic Plane with a Partial Configuration of the HAWC Observatory

28. Energy estimation of cosmic rays with the Engineering Radio Array of the Pierre Auger Observatory

29. Measurement of the radiation energy in the radio signal of extensive air showers as a universal estimator of cosmic-ray energy

30. The Pierre Auger Observatory: status, results and outlook

31. Searches for Large-Scale Anisotropy in the Arrival Directions of Cosmic Rays Detected above Energy of $10^{19}$ eV at the Pierre Auger Observatory and the Telescope Array

32. Observation of Small-scale Anisotropy in the Arrival Direction Distribution of TeV Cosmic Rays with HAWC

33. Sensitivity of the High Altitude Water Cherenkov Detector to Sources of Multi-TeV Gamma Rays

34. Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter

35. Limit on the diffuse flux of ultrahigh energy tau neutrinos with the surface detector of the Pierre Auger Observatory

36. The derivation of constraints on the msugra parameter space from the entropy of dark matter halos

37. Correlation of the highest-energy cosmic rays with the positions of nearby active galactic nuclei

38. Constraints on mSUGRA through entropy and abundance criteria

39. The Pierre Auger Observatory—Status and first results

40. Properties and performance of the prototype instrument for the Pierre Auger Observatory

41. Simulations of the surface detector of the Pierre Auger Observatory—Calibration and Monitoring

42. Neutrino production through hadronic cascades in AGN accretion disks

43. Entropy considerations in constraining the mSUGRA parameter space

44. An Optimized Search for Dark Matter in the Galactic Halo with HAWC

45. A Novel Approach towards the Search for Gamma-ray Emission from the Northern Fermi Bubble with HAWC

46. Observing muon decays in water Cherenkov detectors at the Pierre Auger Observatory

47. A Spectacular VHE Gamma-Ray Outburst from PKS 2155-304 in 2006

48. The ANTARES neutrino telescope: a status report

49. Detection of the Cherenkov light diffused by sea water with the ULTRA experiment

50. The AMS-RICH velocity and charge reconstruction

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