output
19922026
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations

Showing astro-ph.SRShow all

267 papers · 1 filter

astro-ph.SR2026

The location and propagation of fine structures in type II solar radio bursts

S. Normo, K. Bhandari, A. Nadiger +1

Solar eruptions such as coronal mass ejections can drive collisionless shocks that are good particle accelerators. Electrons accelerated by these shocks can be observed remotely vi…

astro-ph.SR2026

AT 2025abao: The fourth luminous red nova in M 31

A. Reguitti, A. Pastorello, G. Valerin +15

We present photometric and spectroscopic observations of the luminous red nova (LRN) AT 2025abao, the fourth discovered in M 31. The LRN, associated to the asymptotic giant branch…

astro-ph.SR2026

Catalogue and statistics of greater than 100 MeV solar proton events during solar cycles 23-25 from SOHO-ERNE observations

M. Jarry, C. Palmroos, E. Lavasa +12

The SPEARHEAD (specification, analysis, and re-calibration of high-energy particle data) project, funded by the European Union Horizon Europe programme, enhances the accuracy and u…

astro-ph.SR2026

Multi-spacecraft constraints on relativistic solar energetic particle transport in the widespread 28 October 2021 event

E. Lavasa, J. T. Lang, A. Papaioannou +6

Aims. We investigated the transport of solar energetic particles (SEPs) during the relativistic widespread event of 28 October 2021, quantifying the role of parallel and perpendicu…

astro-ph.SR2026

In-flight calibration of RADEM, the JUICE mission radiation monitor

Marco Pinto, Francisca Santos, António Gomes +7

The RADiation-hard Electron Monitor (RADEM) aboard the Jupiter Icy Moons Explorer (JUICE), launched on 14 April 2023, measures high-energy protons and electrons during the cruise p…

astro-ph.SR2026

SN 2017ati: A luminous type IIb explosion from a massive progenitor

Z. -H. Peng, S. Benetti, Y. -Z. Cai +21

We present optical photometric and spectroscopic observations of the Type~IIb supernova (SN)~2017ati. It reached the maximum light at about 27~d after the explosion and the light c…