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Searches for Fast Radio Transients

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arxiv astro-ph/0304364 v3 pith:X73N7FPC submitted 2003-04-21 astro-ph

Searches for Fast Radio Transients

J. M. Cordes & M. A. McLaughlin This is my paper
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keywords radioastrophysicalfastsourcestransientsaccountanalysisapplies
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We discuss optimal detection of fast radio transients from astrophysical objects while taking into account the effects of propagation through intervening ionized media, including dispersion, scattering and scintillation.Our analysis applies to the giant-pulse phenomenon exhibited by some pulsars, for which we show examples, and to radio pulses from other astrophysical sources, such as prompt radio emission from gamma-ray burst sources and modulated signals from extra-terrestrial civilizations.

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Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

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    astro-ph.HE 2025-12 conditional novelty 8.0

    The central compact object 1E 1207.4-5209 emits pulsed radio waves at its 0.4-second spin period, revealing it as a faint radio pulsar.

  2. VAPOLA -- A multi-year, multi-band polarization survey of AGN and Sgr A* at mm wavelengths with ALMA I. Survey Overview and Science-Ready Archival Products

    astro-ph.GA 2026-07 accept novelty 6.0

    An automated pipeline and web portal deliver science-ready, full-polarization ALMA data products from VLBI campaigns for AGN and Sgr A* across Bands 3, 6, and 7.

  3. The Southern-sky MWA Rapid Two-metre (SMART) pulsar survey--IV. Survey update and an atlas of 205 non-recycled southern pulsars

    astro-ph.HE 2026-07 accept novelty 6.0

    Atlas of 205 non-recycled southern pulsars at 140–170 MHz from MWA SMART data, with profiles, DMs, RMs, fluxes and public data products for SKA-Low.

  4. Debiasing the Observed Fast Radio Burst Population with the CHIME/FRB Selection Function

    astro-ph.HE 2026-06 unverdicted novelty 4.0

    Analysis of CHIME/FRB Catalog 2 with synthetic injections and a multidimensional selection function yields evidence for a slight downturn in the intrinsic scattering timescale distribution, though flat or rising distr...

  5. Searching for links between energetic millisecond pulsars and repeating fast radio bursts

    astro-ph.HE 2026-05 unverdicted novelty 4.0

    Wideband observations show M28A giant pulses differ from FRB 20200120E bursts in duration, luminosity, timing statistics, and spectral structure, yielding no strong evidence for a direct link.