Ушбу иш иқтибос қилган ишлар
72 та иш
Иш: Depth of maximum of air-shower profiles above <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:msup> <mml:mn>10</mml:mn> <mml:mn>17.7</mml:mn> </mml:msup> <mml:mtext> </mml:mtext> <mml:mtext> </mml:mtext> <mml:mi>eV</mml:mi> </mml:math> measured with the fluorescence detector of the Pierre Auger Observatory
<tt>emcee</tt>: The MCMC Hammer
Daniel Foreman-Mackey, David W. Hogg, Dustin Lang +1
Мақола2013127 иқтибосABIDepth of maximum of air-shower profiles at the Pierre Auger Observatory. I. Measurements at energies above<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mn>1</mml:mn><mml:msup><mml:mrow><mml:mn>0</mml:mn></mml:mrow><mml:mrow><mml:mn>17.8</mml:mn></mml:mrow></mml:msup><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:mrow></mml:math>
A. Aab, P. Abreu, M. Aglietta +97
Мақола201412 иқтибосABIMeasurement of the cosmic-ray energy spectrum above<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mn>2.5</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mn>18</mml:mn></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:math>using the Pierre Auger Observatory
A. Aab, P. Abreu, M. Aglietta +97
Мақола202010 иқтибосABIThe offline software framework of the Pierre Auger Observatory
S. Argirò, S. L. C. Barroso, J. G. González +7
Мақола20078 иқтибосABIHadronic interaction model sibyll 2.3d and extensive air showers
Felix Riehn, R. Engel, Anatoli Fedynitch +2
Мақола20207 иқтибосABIThe fluorescence detector of the Pierre Auger Observatory
J. Abraham, P. Abreu, M. Aglietta +97
Мақола20106 иқтибосABIThe exposure of the hybrid detector of the Pierre Auger Observatory
P. Abreu, M. Aglietta, E. J. Ahn +96
Мақола20105 иқтибосABIMeasurement of the Depth of Maximum of Extensive Air Showers above<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mn>10</mml:mn><mml:mn>18</mml:mn></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:math>
J. Abraham, P. Abreu, M. Aglietta +96
Мақола20104 иқтибосABIThe surface detector system of the Pierre Auger Observatory
I. Allekotte, A.F. Barbosa, P. Bauleo +17
Мақола20074 иқтибосABIOne-dimensional hybrid approach to extensive air shower simulation
T BERGMANN, R. Engel, D. Heck +5
Мақола20064 иқтибосABIInference of the Mass Composition of Cosmic Rays with Energies from <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mn>10</mml:mn><mml:mn>18.5</mml:mn></mml:msup></mml:math> to <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mn>10</mml:mn></mml:mrow><mml:mrow><mml:mn>20</mml:mn></mml:mrow></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:mrow></mml:math> Using the Pierre Auger Observatory and Deep Learning
Adila Abdul Halim, P. Abreu, M. Aglietta +97
ABI