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B. Daniel

38 papers hereh-index 3910.5k citations85 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author4
  • last author3

Across the 8 of 38 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE26
  • astro-ph.IM10
  • hep-ex1
  • physics.ins-det1
same name
  • B. Daniel — 19 papers
  • B. Daniel — 1 paper, h 1
  • B. Daniel — 1 paper, h 1
  • B. Daniel — 1 paper, h 4
  • B. Daniel — 1 paper

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20102019
most citedObservation of a Large-scale Anisotropy in the Arrival Directions of Cosmic Rays above 8×1018 eV

409 citations · 3.1k across the 36 of their papers we have counts for

collaborators
Showing 2017 · astro-ph.HEShow all

3 papers · 2 filters

astro-ph.HE2017

Inferences on Mass Composition and Tests of Hadronic Interactions from 0.3 to 100 EeV using the water-Cherenkov Detectors of the Pierre Auger Observatory

The Pierre Auger Collaboration, A. Aab, P. Abreu +403

We present a new method for probing the hadronic interaction models at ultra-high energy and extracting details about mass composition. This is done using the time profiles of the…

astro-ph.HE2017★ 1 cited

The Pierre Auger Observatory: Contributions to the 35th International Cosmic Ray Conference (ICRC 2017)

The Pierre Auger Collaboration, A. Aab, P. Abreu +394

Contributions of the Pierre Auger Collaboration to the 35th International Cosmic Ray Conference (ICRC 2017), 12-20 July 2017, Bexco, Busan, Korea.

astro-ph.HE2017★ 409 cited

Observation of a Large-scale Anisotropy in the Arrival Directions of Cosmic Rays above 8×1018 eV

The Pierre Auger Collaboration, A. Aab, P. Abreu +404

Cosmic rays are atomic nuclei arriving from outer space that reach the highest energies observed in nature. Clues to their origin come from studying the distribution of their arriv…

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