Find the haystacks, then look for needles: The rate of strongly lensed transients in galaxy-galaxy strong gravitational lenses
Ana Sainz de Murieta, Thomas E. Collett, Mark R. Magee, Justin D. R., Pierel, Wolfgang J. R. Enzi, Martine Lokken, Alex Gagliano, Dan, Ryczanowski

TL;DR
This paper estimates the rate of strongly lensed supernovae and their hosts in upcoming surveys, highlighting their potential for cosmological measurements and the importance of identifying lens systems beforehand.
Contribution
It provides rate predictions for lensed supernovae and hosts in LSST and Euclid, and discusses their use in cosmology and lens identification strategies.
Findings
LSST will discover about 88 glSNe annually.
Approximately 54% of these will have a strongly lensed host.
Most golden sample glSNe will be identifiable in Euclid data.
Abstract
The time delay between appearances of multiple images of a gravitationally lensed supernova (glSN) is sensitive to the Hubble constant, . As well as time delays, a lensed host galaxy is needed to enable precise inference of . In this work we investigate the connection between discoverable lensed transients and their host galaxies. We find that LSST will discover 88 glSNe per year, of which will also have a strongly lensed host. The rates can change by approximately 30 percent uncertainty depending primarily on the choice of unlensed SN population and uncertainties in the redshift evolution of the deflector population, but the fraction of glSNe with a lensed host is consistently around a half. LSST will discover 20 glSNe per year in systems that could plausibly have been identified by Euclid as galaxy-galaxy lenses before the discovery of the glSN. Such systems have…
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Taxonomy
TopicsAdaptive optics and wavefront sensing · Astronomy and Astrophysical Research · Galaxies: Formation, Evolution, Phenomena
