WE PROPOSE MONITORING OBSERVATIONS OF THE YOUNG HIGHLY ENERGETIC PULSARS PSR J1838-0655 AND PSR J1846-0258. THESE SOURCES ARE ONLY EASILY DETECTABLE AS PULSARS AT X-RAY ENERGIES WHICH MAKES NICER THE IDEAL INSTRUMENT TO CONDUCT THE NECESSARY OBSERVATIONS.
$37,477FY2021National Aeronautics and Space AdministrationNASA
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