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Lesgourgues, J.; Pastor, S. Neutrino Mass from Cosmology 2012 Advances in High Energy Physics 2012 608515 - 34pp details   doi
Pierre Auger Collaboration (Abreu, P. et al); Pastor, S. Ultrahigh Energy Neutrinos at the Pierre Auger Observatory 2013 Advances in High Energy Physics 2013 708680 - 18pp details   doi
Pierre Auger Collaboration (Abreu, P. et al); Pastor, S. Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter 2010 Astroparticle Physics 34 314-326 details   doi
Pierre Auger Collaboration (Abreu, P. et al); Pastor, S. The exposure of the hybrid detector of the Pierre Auger Observatory 2011 Astroparticle Physics 34 368-381 details   doi
Pierre Auger Collaboration (Abraham, J. et al); Pastor, S. A study of the effect of molecular and aerosol conditions in the atmosphere on air fluorescence measurements at the Pierre Auger Observatory 2010 Astroparticle Physics 33 108-129 details   doi
Pierre Auger Collaboration (Abreu, P. et al); Pastor, S. Search for first harmonic modulation in the right ascension distribution of cosmic rays detected at the Pierre Auger Observatory 2011 Astroparticle Physics 34 627-639 details   doi
Pierre Auger Collaboration (Abreu, P. et al); Pastor, S. The Lateral Trigger Probability function for the Ultra-High Energy Cosmic Ray showers detected by the Pierre Auger Observatory 2011 Astroparticle Physics 35 266-276 details   doi
Pierre Auger Collaboration (Abreu, P. et al); Pastor, S. Search for signatures of magnetically-induced alignment in the arrival directions measured by the Pierre Auger Observatory 2012 Astroparticle Physics 35 354-361 details   doi
Pierre Auger Collaboration (Abreu, P. et al); Pastor, S. Description of atmospheric conditions at the Pierre Auger Observatory using the Global Data Assimilation System (GDAS) 2012 Astroparticle Physics 35 591-607 details   doi
Pierre Auger Collaboration (Abreu, P. et al); Pastor, S. Identifying clouds over the Pierre Auger Observatory using infrared satellite data 2013 Astroparticle Physics 50-52 92-101 details   doi
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