Corrigendum: A large light-mass component of cosmic rays at 1017-1017.5 electronvolts from radio observations.
Nature Nature Publishing Group 537:7621 (2016) 572
Abstract:
In this Letter, we omitted to cite preliminary results from the low-energy extension of the Pierre Auger Observatory, as presented at the International Cosmic Ray Conference 2015 (ref. 1). Figure 1 of this Corrigendum shows measurements of the average value of Xmax for the Low Frequency Array (LOFAR), and earlier experiments using different techniques, now including the data from the Pierre Auger Observatory1 , specifically the contribution of A. Porcelli. Our values are in agreement with those of ref. 1 within systematic uncertainties.Low-radio-frequency eclipses of the redback pulsar J2215+5135 observed in the image plane with LOFAR
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 459:3 (2016) 2681-2689
New methods to constrain the radio transient rate: results from a survey of four fields with LOFAR
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 459:3 (2016) 3161-3174
On Type IIn/Ia-CSM supernovae as exemplified by SN 2012ca
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 459:3 (2016) 2721-2740