Wide-band, low-frequency pulse profiles of 100 radio pulsars with LOFAR
© ESO, 2016. Context. LOFAR offers the unique capability of observing pulsars across the 10-240 MHz frequency range with a fractional bandwidth of roughly 50%. This spectral range is well suited for studying the frequency evolution of pulse profile morphology caused by both intrinsic and extrinsic e...
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
---|---|
Format: | Journal Article |
Published: |
2016
|
Online Access: | http://hdl.handle.net/20.500.11937/39406 |