No detectable radio emission from the magnetar-like pulsar in Kes 75
arXiv:0805.1448 · doi:10.1086/591661
Abstract
The rotation-powered pulsar PSR J1846-0258 in the supernova remnant Kes 75 was recently shown to have exhibited magnetar-like X-ray bursts in mid-2006. Radio emission has not yet been observed from this source, but other magnetar-like sources have exhibited transient radio emission following X-ray bursts. We report on a deep 1.9 GHz radio observation of PSR J1846-0258 with the 100-m Green Bank Telescope in late 2007 designed to search for radio pulsations or bursts from this target. We have also analyzed three shorter serendipitous 1.4 GHz radio observations of the source taken with the 64-m Parkes telescope during the 2006 bursting period. We detected no radio emission from PSR J1846-0258 in either the Green Bank or Parkes datasets. We place an upper limit of 4.9 μJy on coherent pulsed emission from PSR J1846-0258 based on the 2007 November 2 observation, and an upper limit of 27 μJy around the time of the X-ray bursts. Serendipitously, we observed radio pulses from the nearby RRAT J1846-02, and place a 3σconfidence level upper limit on its period derivative of 1.7 * 10^{-13}, implying its surface dipole magnetic field is less than 2.6 * 10^{13} G.
15 pages, 2 figures, submitted to ApJ
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- The Third Fermi Large Area Telescope Catalog of Gamma-ray Pulsars
- A Magnetar-like Outburst from a High-B Radio Pulsar
- The soft gamma-ray pulsar population: an high-energy overview
- The fundamental plane for radio magnetars
- The Fermi LAT detection of magnetar-like pulsar PSR J1846-0258 at high-energy gamma-rays
- Emission mechanism of GeV-quiet soft gamma-ray pulsars; A case for peculiar geometry?
- Reactivation of the high-magnetic field pulsar PSR J1846--0258 with magnetar-like bursts
- High Frequency Radio Observations of Two Magnetars, PSR J16224950 and 1E 1547.05408
- Upper Limits on Pulsed Radio Emission from the 6.85 s X-ray Pulsar XTE J0103-728 in the Small Magellanic Cloud
- Spatio-spectral-temporal Modelling of Two Young Pulsar Wind Nebulae