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Development and Initial Testing of XR-based Fence Diagrams for Polar Science

N. Tack; N. Holschuh; S. Sharma; R. Williams; D. Engel (July 2023, IEEE International Geoscience and Remote Sensing Symposium)

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First measurement of the total inelastic cross section of positively charged kaons on argon at energies between 5.0 and 7.5 GeV

https://doi.org/10.1103/PhysRevD.110.092011

Abud, A Abed; Abi, B; Acciarri, R; Acero, M A; Adames, M R; Adamov, G; Adamowski, M; Adams, D; Adinolfi, M; Adriano, C; et al (November 2024, Physical Review D)

ProtoDUNE Single-Phase (ProtoDUNE-SP) is a 770-ton liquid argon time projection chamber that operated in a hadron test beam at the CERN Neutrino Platform in 2018. We present a measurement of the total inelastic cross section of charged kaons on argon as a function of kaon energy using 6 and $7 GeV / c$ beam momentum settings. The flux-weighted average of the extracted inelastic cross section at each beam momentum setting was measured to be $380 \pm 26 mbarns$ for the $6 GeV / c$ setting and $379 \pm 35 mbarns$ for the $7 GeV / c$ setting. Published by the American Physical Society2024
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Open Data from the Third Observing Run of LIGO, Virgo, KAGRA, and GEO

https://doi.org/10.3847/1538-4365/acdc9f

Abbott, R.; Abe, H.; Acernese, F.; Ackley, K.; Adhicary, S.; Adhikari, N.; Adhikari, R. X.; Adkins, V. K.; Adya, V. B.; Affeldt, C.; et al (July 2023, The Astrophysical Journal Supplement Series)

Abstract The global network of gravitational-wave observatories now includes five detectors, namely LIGO Hanford, LIGO Livingston, Virgo, KAGRA, and GEO 600. These detectors collected data during their third observing run, O3, composed of three phases: O3a starting in 2019 April and lasting six months, O3b starting in 2019 November and lasting five months, and O3GK starting in 2020 April and lasting two weeks. In this paper we describe these data and various other science products that can be freely accessed through the Gravitational Wave Open Science Center at https://gwosc.org . The main data set, consisting of the gravitational-wave strain time series that contains the astrophysical signals, is released together with supporting data useful for their analysis and documentation, tutorials, as well as analysis software packages.
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