activity
20132026
most citedThe cosmic-ray positron energy spectrum measured by PAMELA

308 citations · 1.4k across the 42 of their papers we have counts for

collaborators

42 papers

astro-ph.IM2026

The General Antiparticle Spectrometer (GAPS) Antarctic Balloon Payload

The GAPS Collaboration, Kazutaka Aoyama, Tsuguo Aramaki +65

The General Antiparticle Spectrometer (GAPS) is an Antarctic stratospheric balloon mission designed to provide unmatched sensitivity to low-energy (<0.25 GeV/n) cosmic-ray antiprot…

astro-ph.HE2026

The JEM-EUSO Collaboration: Contributions to the 39th International Cosmic Ray Conference (ICRC2025)

M. Abdullahi, M. Abrate, J. H. Adams +163

This is a collection of papers presented by the JEM-EUSO Collaboration at the 39th International Cosmic Ray Conference (ICRC 2025) (Geneva, Switzerland, July 14--24, 2025).

astro-ph.IM2026

POEMMA-Balloon with Radio: A multi-messenger, multi-detector balloon payload

J. Adams, J. Alfaro, D. Allard +123

A review of the current status of the field of Ultra-High-Energy Cosmic Ray (UHECR) including a summary of remaining open questions was presented in the white paper "Ultra-High Ene…

astro-ph.IM2024★ 4 cited

The Wide Field Monitor (WFM) of the China-Europe eXTP (enhanced X-ray Timing and Polarimetry) mission

Margarita Hernanz, Marco Feroci, Yuri Evangelista +58

The eXTP mission is a major project of the Chinese Academy of Sciences (CAS), with a large involvement of Europe. Its scientific payload includes four instruments: SFA, PFA, LAD an…

astro-ph.HE2023

GAPS contributions to the 38th International Cosmic Ray Conference (Nagoya 2023)

T. Aramaki, M. Boezio, S. E. Boggs +55

Compilation of papers presented by the GAPS Collaboration at the 38th International Cosmic Ray Conference (ICRC), held July 26 through August 3, 2023 in Nagoya, Japan.

astro-ph.HE2023★ 6 cited

Current status and new perspectives on cosmic ray deuterons

Diego Mauricio Gomez-Coral, Cory Gerrity, Riccardo Munini +1

Deuterons are the most abundant secondary cosmic ray species in the Galaxy, but their study has been severely limited due to experimental challenges. In an era with new experiments…