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CHIME/FRB Outriggers: Design Overview

  • Authors: Mandana Amiri, Bridget C. Andersen, Shion Andrew, Kevin Bandura, Mohit Bhardwaj, Kalyani Bhopi, Vadym Bidula, P. J. Boyle, Charanjot Brar, Mark Carlson, Tomas Cassanelli, Alyssa Cassity, Shami Chatterjee, Jean-François Cliche, Alice P. Curtin, Rachel Darlinger, David R. DeBoer, Matt Dobbs, Fengqiu Adam Dong, Gwendolyn Eadie, Emmanuel Fonseca, B. M. Gaensler, Nina Gusinskaia, Mark Halpern, Ian Hendricksen, Jason Hessels, Ronniy C. Joseph, Jane Kaczmarek, Victoria M. Kaspi, Kholoud Khairy, T. L. Landecker, Adam E. Lanman, Albert Wai Kit Lau, Mattias Lazda, Calvin Leung, Robert A. Main, Kiyoshi W. Masui, Ryan Mckinven, Juan Mena-Parra, Bradley W. Meyers, Daniele Michilli, Nikola Milutinovic, Kenzie Nimmo, Gavin Noble, Ayush Pandhi, Aaron B. Pearlman, Jeffrey B. Peterson, Emily Petroff, Ziggy Pleunis, Alexander W. Pollak, Masoud Rafiei-Ravandi, Andre Renard, Mawson W. Sammons, Ketan R. Sand, Pranav Sanghavi, Paul Scholz, Vishwangi Shah, Kaitlyn Shin, Seth R. Siegel, Andrew Siemion, Jonathan L. Sievers, Kendrick Smith, David Spear, Ingrid Stairs, Keith Vanderlinde, Haochen Wang, Jacob P. Willis, Tarik J. Zegmott

Mandana Amiri et al 2025 The Astrophysical Journal 993 .

  • Provider: AAS Journals

Caption: Figure 6.

Localization forecasts for the CHIME/FRB Outriggers. Forecasts are provided as a function of FRB band occupancy (see the text above the left, center, and right panels), and S/N as observed by CHIME. We show three different scenarios for the ionosphere: (1) our fiducial ionospheric prior model where we must fringe-fit for the differential sTEC between targets and calibrators randomly drawn from the field of view; (2) a scenario where we find nearby calibrators that allow us to null 80% of the ionospheric contribution; and (3) a scenario where the ionosphere is 5 times thicker than in our fiducial model widening the prior distribution by a factor of 5. We forecast that we will achieve our localization goal of ∼50 mas precision in both dimensions for all band-filling FRBs except under the most pessimistic assumptions, and that even narrowband FRBs can be localized provided the majority of the ionosphere can be nulled.

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