Strong pulses detected from a rotating radio transient J18191458
arXiv:1104.3256 · doi:10.1051/0004-6361/201015953
Abstract
We analyze individual pulses detected from RRAT J18191458. From April 2007 to April 2010, we carried out observations using the Nanshan 25-m radio telescope of Urumqi Observatory at a central frequency of 1541.25 MHz. We obtain a dispersion measure pc cm^{-3} by analyzing all the 423 detected bursts. The tri-band pattern of arrival time residuals is confirmed by a single pulse timing analysis. Twenty-seven bimodal bursts located in the middle residual band are detected, and, profiles of two typical bimodal bursts and two individual single-peak pulses are presented. We determine the statistical properties of SNR and W of bursts in different residual bands. The W variation with SNR shows that the shapes of bursts are quite different from each other. The cumulative probability distribution of intensity for a possible power law with index is inferred from the number of those bursts with and high intensities.
6 pages, 8 figures, 1 table, accepted for publication in A&A
References in corpus (17)
- TEMPO2, a new pulsar timing package. I: Overview
- The strongest cosmic magnets: Soft Gamma-ray Repeaters and Anomalous X-ray Pulsars
- The Magnificent Seven: Magnetic fields and surface temperature distributions
- Pulsar Nulling and Mode Changing
- On the birthrates of Galactic neutron stars
- Is pulsar B0656+14 a very nearby RRAT source?
- Discovery of Pulsations and a Possible Spectral Feature in the X-ray Emission from Rotating Radio Transient J1819-1458
- A tale of two populations: Rotating Radio Transients and X-ray Dim Isolated Neutron Stars
- Simultaneous multi-frequency single-pulse properties of AXP XTE J1810-197
- Pulsar radiation belts and transient radio emission
- Bright Giant Pulses from the Crab Nebula Pulsar: Statistical Properties, Pulse Broadening and Scattering due to the Nebula
- Discovery of extended X-ray emission around the highly magnetic RRAT J1819-1458
- Radio polarization measurements from RRAT J1819-1458
- A Study of Giant Pulses from PSR J1824-2452A
- Timing observations of RRAT J1819-1458 at Urumqi Observatory
- A search for optical bursts from the rotating radio transient J1819-1458 with ULTRACAM
- Chandra Smells a RRAT: X-ray Detection of a Rotating Radio Transient