[KDR2018] LS1 , the SIMBAD biblio

[KDR2018] LS1 , the SIMBAD biblio (16 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST02:57:27

Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2018NatAs...2..324R 81           X         2 24 47 Two peculiar fast transients in a strongly lensed host galaxy. RODNEY S.A., BALESTRA I., BRADAC M., et al.
2018NatAs...2..334K 6797       S   X C       167 8 116 Extreme magnification of an individual star at redshift 1.5 by a galaxy-cluster lens. KELLY P.L., DIEGO J.M., RODNEY S., et al.
2019A&A...625A..84D 694           X C       16 11 46 The Universe at extreme magnification. DIEGO J.M.
2018ATel11708....1K 161           X         4 2 ~ Detection of a Microlensing Event of a Magnified Star at Redshift z = 1.5. KELLY P., DIEGO J.M., WILLIAMS L., et al.
2018ATel11724....1K 80           X         2 2 ~ No Bright, Early June 2018 Microlensing Event in MACS1149 Galaxy-Cluster Field. KELLY P., WILLIAM L. and FILIPPENKO A.
2020AJ....159...49D 245       D     X         6 3 71 Gravitational lensing signatures of axion dark matter minihalos in highly magnified stars. DAI L. and MIRALDA-ESCUDE J.
2021MNRAS.506.1595G 84           X         2 19 ~ Hamilton's Object - a clumpy galaxy straddling the gravitational caustic of a galaxy cluster: constraints on dark matter clumping. GRIFFITHS R.E., RUDISEL M., WAGNER J., et al.
2022A&A...665A.127D 298           X         7 6 ~ Fast algorithm for simulating light curves of stars at extreme magnification affected by microlensing. DIEGO J.M.
2023A&A...679A..31D 218           X         5 5 ~ JWST's PEARLS: Mothra, a new kaiju star at z = 2.091 extremely magnified by MACS0416, and implications for dark matter models. DIEGO J.M., SUN B., YAN H., et al.
2024ApJ...969...54W 45           X         1 26 ~ Sp1149. I. Constraints on the Balmer L-σ Relation for H II Regions in a Spiral Galaxy at Redshift z = 1.49 Strongly Lensed by the MACS J1149 Cluster. WILLIAMS H., KELLY P., CHEN W., et al.
2024A&A...689A.167D 134           X         3 9 ~ Imaging dark matter at the smallest scales with z ≈ 1 lensed stars. DIEGO J.M., KEI LI S., AMRUTH A., et al.
2025MNRAS.536.1579M 65       D     X         2 17 ~ Limits on dark matter compact objects implied by supermagnified stars in lensing clusters. MULLER C.V. and MIRALDA-ESCUDE J.
2025ApJ...987...94Z 140           X         3 2 ~ The Magnified Waltz: Simulating Light Curves of Binary Stars Passing Through Microcaustics in Strong Lensing Galaxy Clusters. ZHENG W., FU X., CHEN Y., et al.
2025ApJ...988..178L 140           X         3 7 ~ Constraining the z ∼ 1 Initial Mass Function with HST and JWST Lensed Stars in MACS J0416.1-2403. LI S.K., DIEGO J.M., MEENA A.K., et al.
2025ApJ...993..226S 93           X         2 23 ~ Is Earendel a Star? Investigating the Sunrise Arc Using JWST Strong and Weak Gravitational Lensing Analyses. SCOFIELD Z.P., JEE M.J., CHA S., et al.
2026ApJ...996..105W 50           X         1 7 ~ JWST's PEARLS: Temperatures of Nine Highly Magnified Stars in a Galaxy at Redshift 0.94 and Simulated Stellar Population Dependence on Stellar Metallicity and the Initial Mass Function. WILLIAMS H., KELLY P.L., WINDHORST R.A., et al.

goto View the references in ADS