activity
20182026
most citedOn the observability of individual Population III stars and their stellar-mass black hole accretion disks through cluster caustic transits

97 citations · 190 across the 16 of their papers we have counts for

collaborators

17 papers

astro-ph.CO2026

Three-form dark energy: constraints and multi-probe comparison with CDM

Mariam Bouhmadi-López, Hsu-Wen Chiang, Carlos G. Boiza +3

Three-form fields provide a theoretically well-motivated framework for dark energy, arising in higher-dimensional theories and exhibiting a rich cosmological phenomenology. We inve…

astro-ph.GA2026

Extragalactic microlensing through Ultra Diffuse Galaxies

Sung Kei Li, Thomas Broadhurst, Jose M. Diego +4

Stellar microlensing is a powerful method to constrain compact dark matter models, uncover binary stars, and exoplanets during caustic crossing events. At cosmological distances, {…

astro-ph.CO2026

SN 2022riv in RX J2129: Discovery, Spectroscopic Classification, and Microlensing of a Strongly Lensed Type Ia Supernova from JWST and HST Observations

Birendra Dhanasingham, Patrick L. Kelly, Wenlei Chen +27

The multiply imaged SN 2022riv was discovered through a search of galaxy cluster fields as part of a Hubble Space Telescope (HST) SNAP program to find highly magnified stars. The s…

astro-ph.CO2025

Lensed stars in galaxy-galaxy strong lensing -- a JWST prediction for the Cosmic Horseshoe

Sung Kei Li, Luke Weisenbach, Thomas E. Collett +10

We explore for the first time the possibility of detecting lensed star transients in galaxy-galaxy strong lensing systems upon repeated, deep imaging using the {\it James-Webb Spac…

astro-ph.CO2025★ 4 cited

Signatures of Fuzzy Dark Matter Inside Radial Critical Curves

J. M. Palencia, Paloma Morilla, Sung Kei Li +5

We investigate the strong gravitational lensing properties of fuzzy dark matter (FDM) halos, focusing on the magnification properties near radial critical curves (CCs). Using simul…

astro-ph.CO2025★ 1 cited

Transient star B/R ratio and star formation in lensed galaxies

Sung Kei Li, Jose M. Palencia, Jose M. Diego +8

The extreme magnification from galaxy clusters and microlenses therein allows the detection of individual, luminous stars in lensed galaxies as transient events, and hence provides…

astro-ph.CO2025★ 6 cited

Microlensing at Cosmological Distances: Event Rate Predictions in the Warhol Arc of MACS 0416

J. M. Palencia, J. M. Diego, L. Dai +13

Highly magnified stars ( 100) are now outinely identified as transient events at cosmological distances thanks to microlensing by intra-cluster stars near the critical curve…

astro-ph.CO2025

Constraining the z 1 Initial Mass Function with {\it HST} and {\it JWST} Lensed Stars in MACS J0416.1-2403

Sung Kei Li, Jose M. Diego, Ashish K. Meena +19

Our understanding of galaxy properties and evolution is contingent on knowing the initial mass function (IMF), and yet to date, the IMF is constrained only to local galaxies. Indiv…

astro-ph.GA2024★ 1 cited

EPOCHS XI: The Structure and Morphology of Galaxies in the Epoch of Reionization to z ~ 12.5

Lewi Westcott, Christopher J. Conselice, Thomas Harvey +29

We present a structural analysis of 521 galaxy candidates at 6.5 < z < 12.5, with in the F444W filter, taken from the EPOCHS v1 sample, consisting of uniformly reduced…

astro-ph.GA2024★ 8 cited

Galaxy Mergers in the Epoch of Reionization II: Major Merger-Triggered Star Formation and AGN Activities at 4.5-8.5

Qiao Duan, Qiong Li, Christopher J. Conselice +29

Galaxy mergers are a key driver of galaxy formation and evolution, including the triggering of AGN and star formation to a still unknown degree. We thus investigate the impact of g…

astro-ph.GA2024★ 48 cited

Galaxy Mergers in the Epoch of Reionization I: A JWST Study of Pair Fractions, Merger Rates, and Stellar Mass Accretion Rates at

Qiao Duan, Christopher J. Conselice, Qiong Li +30

We present a full analysis of galaxy major merger pair fractions, merger rates, and mass accretion rates, thus uncovering the role of mergers in galaxy formation at the earliest pr…

astro-ph.CO2024★ 3 cited

A high-resolution view of the source-plane magnification near cluster caustics in wave dark matter models

Jose M. Diego, Alfred Amruth, Jose M. Palencia +10

We present the highest resolution images to date of caustics formed by wave dark matter (DM) fluctuations near the critical curves of cluster gravitational lenses. We describe t…

astro-ph.CO2024★ 1 cited

Dark Matter distinguished by skewed microlensing in the "Dragon Arc"

Tom Broadhurst, Sung Kei Li, Amruth Alfred +18

Microlensed stars recently discovered by JWST & HST follow closely the winding critical curve of A370 along all sections of the ``Dragon Arc" traversed by the critical curve. These…

astro-ph.CO2024★ 19 cited

Imaging dark matter at the smallest scales with lensed stars

J. M. Diego, Sung Kei Li, Alfred Amruth +19

Observations of caustic-crossing galaxies at redshift show a wealth of transient events. Most of them are believed to be microlensing events of highly magnified stars. Ea…

astro-ph.CO2024★ 2 cited

Flashlights: Transients among Gravitationally-Lensed Star Clusters in the Dragon Arc. I. Stellar Microlensing vs Stellar Outbursts

Sung Kei Li, Jose M. Diego, Patrick L. Kelly +8

We report the discovery of transients among star clusters in a distant galaxy that is gravitationally lensed by a foreground galaxy cluster, and explore whether these transients co…

astro-ph.GA2024

Identification of 40 gravitationally magnified stars in a galaxy at redshift of 0.725

Yoshinobu Fudamoto, Fengwu Sun, Jose M. Diego +44

Strong gravitational magnifications enable to detect faint background sources, resolve their internal structures, and even identify individual stars in distant galaxies. Highly mag…

astro-ph.GA2018★ 97 cited

On the observability of individual Population III stars and their stellar-mass black hole accretion disks through cluster caustic transits

Rogier A. Windhorst, F. X. Timmes, J. Stuart B. Wyithe +8

We summarize panchromatic Extragalactic Background Light data to place upper limits on the integrated near-infrared surface brightness (SB) that may come from Population III stars…