Gamma Ray Astrophysics at the NSSTC

BATSE Pulsars

4U0115+634 Flux/Frequency History (recent)

This source has a period near the the Nyquist limit of 2.048s for the DISCLA data used by the Monitor, so that these measurements lose some power due to aliasing. The flux has been corrected by a factor of 1.15 to obtain the values plotted.

Monitor Parameters ASCII File Typical Pulse Profile PS File

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4U0115+634 Flux/Frequency History (recent)

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