by Alice Harding, Matthew Kerr, Marco Ajello, Denis Bernard, Harsha Blumer, Isabelle Grenier, Sylvain Guiriec, Francesco Longo, Antonios Manousakis, Pablo Saz-Parkinson, Chanda Prescod-Weinstein, Zorawar Wadiasingh, George Younes, Silvia Zane, and Bing Zhang
Published onMay 31, 2019
Prospects for Pulsar Studies at MeV Energies
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Abstract
Enabled by the Fermi Large Area Telescope, we now know that pulsars fill the gamma-ray sky, and we are beginning to understand their emission mechanism and their distribution throughout the Galaxy. To address key questions calls for a sensitive, wide-field MeV telescope, which can detect the population of MeV-peaked pulsars hinted at by Fermi.
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