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CHIME/FRB Outriggers: Design Overview

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arxiv 2504.05192 v1 pith:QDG335PD submitted 2025-04-07 astro-ph.HE astro-ph.IM

classification astro-ph.HEastro-ph.IM
keywords chimeoutriggersfrbsdesignprojectfastlocalizationoverview
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abstract

The Canadian Hydrogen Intensity Mapping Experiment (CHIME) has emerged as the world's premier facility for studying fast radio bursts (FRBs) through its fast transient search backend CHIME/FRB\@. The CHIME/FRB Outriggers project will augment this high detection rate of 2--3 FRBs per day with the ability to precisely localize them using very long baseline interferometry (VLBI). Using three strategically located stations in North America and deploying recently developed synoptic VLBI observing techniques, the Outriggers will provide $\sim 50$~milliarcsecond localization precision for the majority of detected FRBs. This paper presents an overview of the design and implementation of the Outriggers, covering their geographic distribution, structural design, and observational capabilities. We detail the scientific objectives driving the project, including the characterization of FRB populations, host galaxy demographics, and the use of FRBs as cosmological probes. We also discuss the calibration strategies available to mitigate ionospheric and instrumental effects, ensuring high-precision localization. With two stations currently in science operations, and the third in commissioning, the CHIME/FRB Outriggers project is poised to become a cornerstone of the FRB field, offering unprecedented insights into this enigmatic cosmic phenomenon.

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Cited by 8 Pith papers

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

  1. Measurement of angular cross-correlation between the cosmological dispersion measure and the thermal Sunyaev--Zeldovich effect

    astro-ph.CO 2025-11 conditional novelty 7.0 of 10

    First detection of an angular cross-correlation between FRB dispersion measure and the thermal SZ y-map: amplitude A≈2 relative to the fiducial halo-model prediction (4.0σ for Planck, 1.5σ for ACT).

  2. A Correlation Between FRB Dispersion Measure and Foreground Large-Scale Structure

    astro-ph.CO 2025-06 conditional novelty 7.0 of 10

    FRB dispersion measures are positively correlated with foreground galaxy density at 4.2 sigma, and sightlines avoiding halos imply at least 69% of cosmic baryons reside outside virial radii.

  3. Modelling Radio Frequency Interference on the Lunar Farside

    astro-ph.IM 2026-07 conditional novelty 6.0 of 10

    Planned lunar satellites will increasingly contaminate the farside radio band; under this model, ≥30 dB uniform UEMR shielding is required to keep peak RFI below LFT3-like sensitivity.

  4. Testing the Isotropy of the Universe with the CHIME/FRB Catalog I

    astro-ph.HE 2026-07 conditional novelty 6.0 of 10

    A 536-burst CHIME FRB sample shows no statistically significant directional anisotropy, though the test's constraining power is limited.

  5. Discovery and Localization of the Swift-Observed FRB 20241228A in a Star-forming Host Galaxy

    astro-ph.HE 2025-06 conditional novelty 6.0 of 10

    FRB 20241228A is localized to a star-forming galaxy at z=0.1614, with a stringent X-ray limit from Swift follow-up 112 seconds after the burst.

  6. Measurement of the Dispersion$\unicode{x2013}$Galaxy Cross-Power Spectrum with the Second CHIME/FRB Catalog

    astro-ph.CO 2025-06 conditional novelty 6.0 of 10

    FRB dispersion and foreground galaxy density are spatially correlated at 5.1 sigma, with a fitted plasma clustering cutoff near 0.9 Mpc, measured from 2,873 CHIME FRBs and about 6 million DESI galaxies.

  7. Testing the Young FRB Progenitor Hypothesis: A Crossmatch of Catalog-1 CHIME Bursts with Historic Local Universe Supernovae

    astro-ph.HE 2025-06 accept novelty 6.0 of 10

    A systematic cross-match of 886 local supernovae with 241 CHIME FRBs finds no statistically significant associations, and a rate model implies steep magnetar burst-rate decay with age.

  8. The FRB--Galaxy Overdensity Cross-Correlation Statistic in Dispersion Space

    astro-ph.CO 2026-07 conditional novelty 5.0 of 10

    A dispersion-binned FRB–galaxy cross-correlation contains the DM–galaxy cross-correlation as a moment, giving strictly more information and forecasted SNR gains for CHIME and CHORD.

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