Turn-over in pulsar spectra around 1 GHz
arXiv:astro-ph/0611445 · doi:10.1051/0004-6361:20066125
Abstract
The main aim is to investigate the possibility of a high frequency turn-over in the radio spectrum of pulsars. Using the GMRT, multi-frequency flux density measurements of several candidate pulsars have been carried out and their spectra have been extended to lower frequencies. We present the first direct evidence for turn-over in pulsar radio spectra at high frequencies. A total of 3 pulsars (including 2 new ones from this study) are now shown to have a turn-over frequency > 1 GHz, and one is shown to have a turn-over at ~600 MHz.
4 pages, to be published in Astronomy & Astrophysics
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