Saved in:
Bibliographic Details
Main Authors: Abbott, Thomas C., Zwaniga, Andrew V., Brar, Charanjot, Kaspi, Victoria M., Petroff, Emily, Bhardwaj, Mohit, Boyle, P. J., Cook, Amanda M., Joseph, Ronny C., Masui, Kiyoshi W., Pandhi, Ayush, Pleunis, Ziggy, Scholz, Paul, Shin, Kaitlyn, Tendulkar, Shriharsh
Format: Preprint
Published: 2024
Subjects:
Online Access:https://arxiv.org/abs/2410.22468
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1866917822321393664
author Abbott, Thomas C.
Zwaniga, Andrew V.
Brar, Charanjot
Kaspi, Victoria M.
Petroff, Emily
Bhardwaj, Mohit
Boyle, P. J.
Cook, Amanda M.
Joseph, Ronny C.
Masui, Kiyoshi W.
Pandhi, Ayush
Pleunis, Ziggy
Scholz, Paul
Shin, Kaitlyn
Tendulkar, Shriharsh
author_facet Abbott, Thomas C.
Zwaniga, Andrew V.
Brar, Charanjot
Kaspi, Victoria M.
Petroff, Emily
Bhardwaj, Mohit
Boyle, P. J.
Cook, Amanda M.
Joseph, Ronny C.
Masui, Kiyoshi W.
Pandhi, Ayush
Pleunis, Ziggy
Scholz, Paul
Shin, Kaitlyn
Tendulkar, Shriharsh
contents We present frb-voe, a publicly available software package that enables radio observatories to broadcast fast radio burst (FRB) alerts to subscribers through low-latency virtual observatory events (VOEvents). We describe a use-case of frb-voe by the Canadian Hydrogen Intensity Mapping Experiment Fast Radio Burst (CHIME/FRB) Collaboration, which has broadcast thousands of FRB alerts to subscribers worldwide. Using this service, observers have daily opportunities to conduct rapid multi-wavelength follow-up observations of new FRB sources. Alerts are distributed as machine-readable reports and as emails containing FRB metadata, and are available to the public within approximately 13 seconds of detection. A sortable database and a downloadable JSON file containing FRB metadata from all broadcast alerts can be found on the CHIME/FRB public webpage. The frb-voe service also provides users with the ability to retrieve FRB names from the Transient Name Server (TNS) through the frb-voe client user interface (CLI). The frb-voe service can act as a foundation on which any observatory that detects FRBs can build its own VOEvent broadcasting service to contribute to the coordinated multi-wavelength follow-up of astrophysical transients.
format Preprint
id arxiv_https___arxiv_org_abs_2410_22468
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle frb-voe: A Real-time Virtual Observatory Event Alert Service for Fast Radio Bursts
Abbott, Thomas C.
Zwaniga, Andrew V.
Brar, Charanjot
Kaspi, Victoria M.
Petroff, Emily
Bhardwaj, Mohit
Boyle, P. J.
Cook, Amanda M.
Joseph, Ronny C.
Masui, Kiyoshi W.
Pandhi, Ayush
Pleunis, Ziggy
Scholz, Paul
Shin, Kaitlyn
Tendulkar, Shriharsh
Instrumentation and Methods for Astrophysics
We present frb-voe, a publicly available software package that enables radio observatories to broadcast fast radio burst (FRB) alerts to subscribers through low-latency virtual observatory events (VOEvents). We describe a use-case of frb-voe by the Canadian Hydrogen Intensity Mapping Experiment Fast Radio Burst (CHIME/FRB) Collaboration, which has broadcast thousands of FRB alerts to subscribers worldwide. Using this service, observers have daily opportunities to conduct rapid multi-wavelength follow-up observations of new FRB sources. Alerts are distributed as machine-readable reports and as emails containing FRB metadata, and are available to the public within approximately 13 seconds of detection. A sortable database and a downloadable JSON file containing FRB metadata from all broadcast alerts can be found on the CHIME/FRB public webpage. The frb-voe service also provides users with the ability to retrieve FRB names from the Transient Name Server (TNS) through the frb-voe client user interface (CLI). The frb-voe service can act as a foundation on which any observatory that detects FRBs can build its own VOEvent broadcasting service to contribute to the coordinated multi-wavelength follow-up of astrophysical transients.
title frb-voe: A Real-time Virtual Observatory Event Alert Service for Fast Radio Bursts
topic Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2410.22468