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20012026
most citedA direct empirical proof of the existence of dark matter

2.4k citations · 12.9k across the 170 of their papers we have counts for

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Showing astro-ph.COShow all

36 papers · 1 filter

astro-ph.CO2026★ 1 cited

VENUS: Strong-lensing model of MACS J1931.8-2635 -- revealing the farthest multiply imaged supernova

Joseph F. V. Allingham, Adi Zitrin, Vasily Kokorev +42

We present a parametric strong-lensing model for the galaxy cluster MACS J1931.8-2635 (), accompanying the detection of the spectroscopically confirmed SN Eos at $z = 5…

astro-ph.CO2026★ 5 cited

Mapping dark matter in the Bullet Cluster using JWST imaging and spectroscopy

Gregor Rihtaršič, Maruša Bradač, Guillaume Desprez +23

We present an updated gravitational lens model of the Bullet cluster (1E 0657-56) by combining JWST NIRCam imaging and NIRSpec spectroscopy. Although previous lens models relied on…

astro-ph.CO2024

Strong Lensing by Galaxy Clusters

Priyamvada Natarajan, Liliya L. Williams, Marusa Bradac +4

Galaxy clusters as gravitational lenses play a unique role in astrophysics and cosmology: they permit mapping the dark matter distribution on a range of scales; they reveal the pro…

astro-ph.CO2019★ 14 cited

RELICS: A Very Large () Cluster Lens -- RXC J0032.1+1808

Ana Acebron, Adi Zitrin, Dan Coe +38

Extensive surveys with the \textit{Hubble Space Telescope} (HST) over the past decade, targeting some of the most massive clusters in the sky, have uncovered dozens of galaxy-clust…

astro-ph.CO2019★ 2 cited

Unveiling the Phase Transition of the Universe During the Reionization Epoch with Lyman-alpha

Steven L. Finkelstein, Marusa Bradac, Caitlin Casey +15

The epoch of reionization (6 < z < 10) marks the period in our universe when the first large galaxies grew to fruition, and began to affect the universe around them. Massive stars,…

astro-ph.CO2019★ 244 cited

Inferences on the Timeline of Reionization at z~8 From the KMOS Lens-Amplified Spectroscopic Survey

Charlotte A. Mason, Adriano Fontana, Tommaso Treu +12

Detections and non-detections of Lyman alpha (Ly) emission from galaxies ( Gyr after the Big Bang) can be used to measure the timeline of cosmic reionization. Of key i…