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51. KASCADE-Grande energy reconstruction based on the lateral density distribution using the QGSJet-II.04 interaction model

52. Distribution of the 222Rn decay products from a 226Ra solution in a PTB ampoule – Implications for calibration

53. Latest results from the KASCADE-Grande experiment

54. Identifying clouds over the Pierre Auger Observatory using infrared satellite data

55. Calibration of a low-level anti-Compton underground gamma-spectrometer by experiment and Monte Carlo

56. Studies of radio emission from neutrino induced showers generated in rock salt

57. Lopes-3D - vectorial measurements of radio emission from cosmic ray induced air showers

58. Cosmic ray measurements with LOPES: Status and recent results

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

60. Monte Carlo simulation of air sampling methods for the measurement of radon decay products

61. Revised absolute amplitude calibration of the LOPES experiment

62. Application of GUM Supplement 1 to uncertainty of Monte Carlo computed efficiency in gamma-ray spectrometry

63. Equivalence of computer codes for calculation of coincidence summing correction factors – Part II

64. Cosmic ray energy reconstruction from the S(500) observable recorded in the KASCADE-Grande air shower experiment

65. KASCADE-Grande Review, Recent Results, Future Endeavors

66. A comparison of the cosmic-ray energy scales of Tunka-133 and KASCADE-Grande via their radio extensions Tunka-Rex and LOPES

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

68. Ultrahigh-energy neutrino follow-up of gravitational wave events GW150914 and GW151226 with the Pierre Auger Observatory

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

70. Search for ultrarelativistic magnetic monopoles with the Pierre Auger Observatory

71. KASCADE-Grande experiment measurements of the cosmic ray spectrum and large scale anisotropy

72. Precise measurement and calculation of coincidence summing corrections for point and linear sources

73. On within sample homogeneity testing using gamma-ray spectrometry

74. Radio Propagation Environment Analysis for Neutrino Radio Detection in Salt Mines

75. The cosmic ray energy spectrum in the range 1016–1018 eV measured by KASCADE-Grande

76. Restoring the azimuthal symmetry of lateral distributions of charged particles in the range of the KASCADE-Grande experiment

77. A mobile detector for measurements of the atmospheric muon flux

78. The measurement of the cosmic ray primary energy spectrum at 1016–1018 eV with the KASCADE-Grande experiment

79. New measurements of cosmic ray air showers with the digital radio interferometer LOPES

80. THE EXTENSIVE AIR SHOWER EXPERIMENT KASCADE-GRANDE

81. Muon production height studies with the air shower experiment KASCADE-Grande

82. Improved method for the assessment of 60Co and 134Cs point sources in samples with non-homogeneous matrix

83. A new model calculation of the peak efficiency for HPGe detectors used in assays of radioactive waste drums

84. Application of response functions to make efficient Monte Carlo simulations of germanium detectors

85. Intercomparison of methods for coincidence summing corrections in gamma-ray spectrometry

86. Testing efficiency transfer codes for equivalence

87. Muon Production Height investigated by the Air-Shower Experiment KASCADE-Grande

88. The Air-Shower Experiment KASCADE-Grande

89. Recent results of the LOPES experiment

90. Investigation of cosmic ray muons with the WILLI detector compared with the predictions of theoretical models and with semi-analytical formulae

91. WILLI - EAS - a detection system for investigating the muon charge ratio in Extensive Air Showers

92. Asymmetries of lateral distributions of EAS particles

93. An intercomparison of Monte Carlo codes used in gamma-ray spectrometry

94. A tool for processing decay scheme data that encompasses coincidence summing calculations

95. KASCADE-Grande: An overview and first results

96. WILLI – a scintillator detector setup for studies of the zenith and azimuth variation of charge ratio and flux of atmospheric muons

97. Uncertainties in gamma-ray spectrometry

98. Large scale distribution of ultra high energy cosmic rays detected at the Pierre Auger Observatory with zenith angles up to 80°

99. Muons in air showers at the Pierre Auger Observatory

100. The KASCADE-Grande observatory and the composition of very high-energy cosmic rays

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