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Strongly Lensed Transient Sources: A Review

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arxiv 2207.13489 v2 pith:T2KYYXXC submitted 2022-07-18 astro-ph.HE astro-ph.CO

Strongly Lensed Transient Sources: A Review

classification astro-ph.HE astro-ph.CO
keywords lenseddetectiontransientbandsburstsgravitationalreviewsources
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The past decades have witnessed a lot of progress in gravitational lensing with two main targets: stars and galaxies (with active galactic nuclei). The success is partially attributed to the continuous luminescence of these sources making the detection and monitoring relatively easy. With the running of ongoing and upcoming large facilities/surveys in various electromagnetic and gravitational-wave bands, the era of time-domain surveys would guarantee constant detection of strongly lensed explosive transient events, for example, supernovae in all types, gamma ray bursts with afterglows in all bands, fast radio bursts and even gravitational waves. Lensed transients have many advantages over the traditional targets in studying the Universe and magnification effect helps to understand the transients themselves at high redshifts. In this review article, basing on the recent achievements in the literature, we summarize the methods of searching for different kinds of lensed transient signals, the latest results on detection and their applications in fundamental physics, astrophysics and cosmology. At the same time, we give supplementary comments as well as prospects of this emerging research direction that may help readers who are interested in entering this field.

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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Improved Identification of Strongly Lensed Gravitational Waves with Host Galaxy Locations

    astro-ph.CO 2025-12 unverdicted novelty 6.0

    A two-step Bayesian reweighting scheme using Euclid galaxy locations boosts the Bayes factor for true lensed GW pairs by a factor of about 10 while lowering it for unlensed coincidences.

  2. Multi-wavelength Constraints on the Transient EP250905a

    astro-ph.HE 2026-07 conditional novelty 5.0

    EP250905a is best explained as a mildly off-axis structured-jet afterglow at z=2.714, possibly weakly magnified by a foreground galaxy at z=0.374.

  3. Probing Dark Matter Substructure with Image Number Anomaly in Strong Lensing Systems

    astro-ph.CO 2025-11 unverdicted novelty 5.0

    Null detection of extra lensed images in 3500 mock systems constrains PBH abundance to ≲0.04-0.125% and excludes FDM masses below 0.4-3.5×10^{-22} eV at 95% CL depending on angular resolution.

  4. Effects of formation channels and gravitational lensing on stochastic gravitational wave background

    gr-qc 2026-05 unverdicted novelty 4.0

    Using HBI on GWTC-4 data the authors compute lensed SGWBs for ABHs and PBHs and conclude that LIGO and ET can distinguish the two formation channels in specific frequency ranges, with ET offering broader coverage.