On building a cluster watchlist for identifying strongly lensed supernovae, gravitational waves and kilonovae. Issue 2 (9th May 2020)

• Record Type: Journal Article
• Authors: Ryczanowski, Dan; Smith, Graham P; Bianconi, Matteo; Massey, Richard; Robertson, Andrew; Jauzac, Mathilde
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 495:Issue 2(2020)
• Page Start: 1666
• Page End: 1671
• Publication Date: 2020-05-09
• Subjects: gravitational lensing: strong -- gravitational waves; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/staa1274
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: Motivated by discovering strongly lensed supernovae, gravitational waves, and kilonovae in the 2020s, we investigate whether to build a watchlist of clusters based on observed cluster properties (i.e. lens-plane selection) or on the detectability of strongly lensed background galaxies (i.e. source-plane selection). First, we estimate the fraction of high-redshift transient progenitors that reside in galaxies that are themselves too faint to be detected as being strongly lensed. We find ∼15–50 per cent of transient progenitors reside in z = 1 − 2 galaxies too faint to be detected in surveys that reach AB ≃ 23, such as the Dark Energy Survey. This falls to ≲10 per cent at depths that will be probed by early data releases of LSST (AB ≃ 25). Secondly, we estimate a conservative lower limit on the fraction of strong-lensing clusters that will be missed by magnitude-limited searches for multiply imaged galaxies and giant arcs due to the faintness of such images. We find that DES-like surveys will miss ∼75 per cent of 10 15 M⊙ strong-lensing clusters, rising to ∼100 per cent of 10 14 M⊙ clusters. Deeper surveys, such as LSST, will miss ∼40 per cent at 10 15 M⊙ and ∼95 per cent at 10 14 M⊙ . Our results motivate building a cluster watchlist for strongly lensed transients that includes those found by the lens-plane selection.