How limiting is optical follow-up for fast radio burst applications? Forecasts for radio and optical surveys
Author:
Affiliation:
1. Max-Planck-Institut für Radioastronomie , Auf dem Hügel 69, D-53121 Bonn, Germany
2. Institute for Computational Cosmology, Department of Physics, Science Laboratories, Durham University , South Road, Durham, DH1 3LE, UK
Abstract
Funder
STFC
BEIS
Durham University
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stad1659/50599477/stad1659.pdf
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1. THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY
2. Probabilistic Association of Transients to their Hosts (PATH)
3. THE EIGHTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY: FIRST DATA FROM SDSS-III
4. FAST RADIO BURSTS AS PROBES OF MAGNETIC FIELDS IN THE INTERGALACTIC MEDIUM
5. THE ELEVENTH AND TWELFTH DATA RELEASES OF THE SLOAN DIGITAL SKY SURVEY: FINAL DATA FROM SDSS-III
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