Statistical properties of giant pulses from the Crab pulsar
arXiv:0704.1197 · doi:10.1051/0004-6361:20066589
Abstract
We have studied the statistics of giant pulses from the Crab pulsar for the first time with particular reference to their widths. We have analyzed data collected during 3.5 hours of observations conducted with the Westerbork Synthesis Radio Telescope operated in a tied-array mode at a frequency of 1200 MHz. The PuMa pulsar backend provided voltage recording of X and Y linear polarization states in two conjugate 10 MHz bands. We restricted the time resolution to 4 microseconds to match the scattering on the interstellar inhomogeneities. In total about 18000 giant pulses (GP) were detected in full intensity with a threshold level of 6 sigma. Cumulative probability distributions (CPD) of giant pulse energies were analyzed for groups of GPs with different effective widths in the range 4 to 65 microseconds. The CPDs were found to manifest notable differences for the different GP width groups. The slope of a power-law fit to the high-energy portion of the CPDs evolves from -1.7 to -3.2 when going from the shortest to the longest GPs. There are breaks in the CPD power-law fits indicating flattening at low energies with indices varying from -1.0 to -1.9 for the short and long GPs respectively. The GPs with a stronger peak flux density were found to be of shorter duration. We compare our results with previously published data and discuss the importance of these peculiarities in the statistical properties of GPs for the heoretical understanding of the emission mechanism responsible for GP generation.
arXiv comment5 pages, 2 figures. Accepted by Astronomy and Astrophysics
References in corpus (12)
- The Brightest Pulses in the Universe: Multifrequency Observations of the Crab Pulsar's Giant Pulses
- Multifrequency Radio Observations of the Crab Pulsar
- Giant Pulses from the Millisecond Pulsar B1821-24
- Giant Pulses from PSR B1937+21 with widths <= 15 nanoseconds and T_b >= 5 x 10^39 K, the Highest Brightness Temperature Observed in the Universe
- The Radio Spectral Index of the Crab Nebula
- High time-resolution observations of the Vela pulsar
- High-resolution single-pulse studies of the Vela Pulsar
- Multifrequency Observations of Giant Radio Pulses from the Millisecond Pulsar B1937+21
- Green Bank Telescope Studies of Giant Pulses from Millisecond Pulsars
- A search for giant pulses in Vela-like pulsars
- Properties and Interpretations of Giant Micropulses and Giant Pulses from Pulsars
- Radio and X-ray Observations of PSR B0540-69
Cited by in corpus (41)
- The surprising Crab pulsar and its nebula: A review
- Repeating behaviour of FRB 121102: periodicity, waiting times and energy distribution
- Fast radio bursts as giant pulses from young rapidly rotating pulsars
- Giant pulses from the Crab pulsar: A wide-band study
- The Crab Pulsar at Centimeter Wavelengths: I. Ensemble Characteristics
- A Giant Sample of Giant Pulses from the Crab Pulsar
- The FRB 20121102A November rain in 2018 observed with the Arecibo Telescope
- Arecibo observations of a burst storm from FRB 20121102A in 2016
- Fast Radio Bursts' emission mechanism: implication from localization
- Bright Giant Pulses from the Crab Nebula Pulsar: Statistical Properties, Pulse Broadening and Scattering due to the Nebula
- Giant Pulses with Nanosecond Time Resolution detected from the Crab Pulsar at 8.5 and 15.1 GHz
- Comprehensive analysis of a dense sample of FRB 121102 bursts
- Intensity Distribution Function and Statistical Properties of Fast Radio Bursts
- Spectral Flattening at Low Frequencies in Crab Giant Pulses
- A detailed study of giant pulses from PSR B1937+21 using the Large European Array for Pulsars
- FRB Energetics and Sources
- Correlation of Fermi photons with high-frequency radio giant pulses from the Crab pulsar
- Radio Properties of Rotating Radio Transients: Single Pulse Spectral and Wait Time Analyses
- Probing pulsar scattering between 120 and 280 MHz with the MWA
- Statistical Studies of Giant Pulse Emission from the Crab Pulsar
- Correlation of Chandra photons with the radio giant pulses from the Crab pulsar
- Short-lived Radio Bursts from the Crab Pulsar
- Observations of Giant Pulses from Pulsar PSR B0950+08 using LWA1
- A Low Frequency Survey of Giant Pulses from the Crab Pulsar
- Hitomi X-ray studies of Giant Radio Pulses from the Crab pulsar
- Long-term study of extreme giant pulses from PSR B0950+08 with AARTFAAC
- Search for a correlation between very-high-energy gamma rays and giant radio pulses in the Crab pulsar
- Repeating Fast Radio Bursts with High Burst Rates by Plate Collisions in Neutron Star Crusts
- A Southern-Hemisphere all-sky radio transient monitor for SKA-Low prototype stations
- Multifrequency Study of Giant Radio Pulses from the Crab Pulsar with the K5 VLBI Recording Terminal
- Simultaneous Observations of Giant Pulses from the Crab Pulsar, with the Murchison Widefield Array and Parkes Radio Telescope: Implications for the Giant Pulse Emission Mechanism
- Statistical and polarization properties of giant pulses of the millisecond pulsar B1937+21
- Spectro-temporal Emission from the Galactic Center Magnetar
- An Arecibo Search for Pulsars and Transient Sources in M33
- Do magnetars really exist?
- An activity transition in FRB 20201124A: methodological rigor, detection of frequency-dependent cessation, and a geometric magnetar model
- Astropulse: A Search for Microsecond Transient Radio Signals Using Distributed Computing. I. Methodology
- Simultaneous Observations of Giant Pulses from Pulsar PSR B0031-07 at 38 MHz and 74 MHz
- Are Pulsar Giant Pulses Induced by Re-emission of Cyclotron Resonance Absorption?
- A Statistical Analysis of Crab Pulsar Giant Pulse Rates
- Energy and waiting time distributions of FRB 121102 observed by FAST