Measurements of the Crab Pulsar’s Giant Radio Pulse Amplitude Power-law Index Using Low-frequency Arecibo and Green Bank Telescope Observations

We report two low-frequency measurements of the power-law index for the amplitudes of giant radio pulses from the Crab pulsar. The two observations were taken with the Arecibo and Green Bank radio telescopes at center frequencies of 327 MHz and 350 MHz, respectively. We find best-fit values for the...

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Main Authors: Fronefield Crawford, T. Joseph W. Lazio, Alexander McEwen, Julia S. Deneva, James M. Cordes, Laura Spitler, Ryan F. Trainor
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/acca7f
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author Fronefield Crawford
T. Joseph W. Lazio
Alexander McEwen
Julia S. Deneva
James M. Cordes
Laura Spitler
Ryan F. Trainor
author_facet Fronefield Crawford
T. Joseph W. Lazio
Alexander McEwen
Julia S. Deneva
James M. Cordes
Laura Spitler
Ryan F. Trainor
author_sort Fronefield Crawford
collection DOAJ
description We report two low-frequency measurements of the power-law index for the amplitudes of giant radio pulses from the Crab pulsar. The two observations were taken with the Arecibo and Green Bank radio telescopes at center frequencies of 327 MHz and 350 MHz, respectively. We find best-fit values for the differential power-law index β (where ${dN}/{dS}\propto {S}^{\beta }$ and S is the pulse amplitude) of −2.63 ± 0.05 and −3.6 ± 0.5 from the Arecibo and Green Bank data sets, respectively. Both values are broadly consistent with other values previously measured for the Crab pulsar at low radio frequencies. These reported values may be useful in future giant pulse studies of the Crab pulsar.
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spelling doaj.art-a1acd4ef7eae457ca564f6cb353e8ba02023-09-03T14:28:02ZengIOP PublishingThe Astrophysical Journal1538-43572023-01-0194814610.3847/1538-4357/acca7fMeasurements of the Crab Pulsar’s Giant Radio Pulse Amplitude Power-law Index Using Low-frequency Arecibo and Green Bank Telescope ObservationsFronefield Crawford0https://orcid.org/0000-0002-2578-0360T. Joseph W. Lazio1Alexander McEwen2https://orcid.org/0000-0001-5481-7559Julia S. Deneva3https://orcid.org/0000-0003-1226-0793James M. Cordes4https://orcid.org/0000-0002-4049-1882Laura Spitler5https://orcid.org/0000-0002-3775-8291Ryan F. Trainor6https://orcid.org/0000-0002-6967-7322Department of Physics and Astronomy, Franklin and Marshall College , P.O. Box 3003, Lancaster, PA 17604, USA ; fcrawfor@fandm.eduJet Propulsion Laboratory, California Institute of Technology , 4800 Oak Grove Dr., M/S 67-201, Pasadena, CA 91107, USACenter for Gravitation, Cosmology and Astrophysics, Department of Physics, University of Wisconsin-Milwaukee , P.O. Box 413, Milwaukee, WI 53201, USAGeorge Mason University , 4400 University Dr., Fairfax, VA 22030, USACornell Center for Astrophysics and Planetary Science, and Department of Astronomy, Cornell University , Ithaca, NY 14853, USAMax-Planck-Institut für Radioastronomie (MPIfR) , Auf dem Hügel 69, D-53121, Bonn, GermanyDepartment of Physics and Astronomy, Franklin and Marshall College , P.O. Box 3003, Lancaster, PA 17604, USA ; fcrawfor@fandm.eduWe report two low-frequency measurements of the power-law index for the amplitudes of giant radio pulses from the Crab pulsar. The two observations were taken with the Arecibo and Green Bank radio telescopes at center frequencies of 327 MHz and 350 MHz, respectively. We find best-fit values for the differential power-law index β (where ${dN}/{dS}\propto {S}^{\beta }$ and S is the pulse amplitude) of −2.63 ± 0.05 and −3.6 ± 0.5 from the Arecibo and Green Bank data sets, respectively. Both values are broadly consistent with other values previously measured for the Crab pulsar at low radio frequencies. These reported values may be useful in future giant pulse studies of the Crab pulsar.https://doi.org/10.3847/1538-4357/acca7fPulsarsRadio transient sources
spellingShingle Fronefield Crawford
T. Joseph W. Lazio
Alexander McEwen
Julia S. Deneva
James M. Cordes
Laura Spitler
Ryan F. Trainor
Measurements of the Crab Pulsar’s Giant Radio Pulse Amplitude Power-law Index Using Low-frequency Arecibo and Green Bank Telescope Observations
The Astrophysical Journal
Pulsars
Radio transient sources
title Measurements of the Crab Pulsar’s Giant Radio Pulse Amplitude Power-law Index Using Low-frequency Arecibo and Green Bank Telescope Observations
title_full Measurements of the Crab Pulsar’s Giant Radio Pulse Amplitude Power-law Index Using Low-frequency Arecibo and Green Bank Telescope Observations
title_fullStr Measurements of the Crab Pulsar’s Giant Radio Pulse Amplitude Power-law Index Using Low-frequency Arecibo and Green Bank Telescope Observations
title_full_unstemmed Measurements of the Crab Pulsar’s Giant Radio Pulse Amplitude Power-law Index Using Low-frequency Arecibo and Green Bank Telescope Observations
title_short Measurements of the Crab Pulsar’s Giant Radio Pulse Amplitude Power-law Index Using Low-frequency Arecibo and Green Bank Telescope Observations
title_sort measurements of the crab pulsar s giant radio pulse amplitude power law index using low frequency arecibo and green bank telescope observations
topic Pulsars
Radio transient sources
url https://doi.org/10.3847/1538-4357/acca7f
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