PoS - Proceedings of Science
Volume 444 - 38th International Cosmic Ray Conference (ICRC2023) - Gamma-ray Astronomy (GA)
Observation the UHE Gamma-ray emission from the J1959+2850 with LHAASO
Y. Yu
Full text: pdf
Pre-published on: January 09, 2024
Published on:
Abstract
We report the discovery of an extended $\gamma-$ray source around the high spin-down power Fermi-LAT pulsar - 4FGL J1958+2846 with Large High-Altitude Air Shower Observatory (LHAASO), which is also resolved from previous public source LHAASO J1956+2845. The significance is 16.5 standard deviations above 25 TeV. The best-fit location is R.A. = 299.68$^\circ \pm$ 0.05$^\circ$ and decl. = 28.84$^\circ \pm$ 0.04$^\circ$, and the extension is $\sim$ 0.30$^\circ$.
DOI: https://doi.org/10.22323/1.444.0621
How to cite

Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in "proceeding" format which is more detailed and complete.

Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.