collaborators

9 papers

astro-ph.CO2025

Testing Light Unaffiliated Mass Clumps in MACS 0416 on galaxy and galaxy cluster scales using JWST

Marceau Limousin, Derek Perera, Gregor Rihtarsic +2

Light unaffiliated mass clumps (LUMCs), i.e. dark matter (DM) components without any stellar counterparts, have been reported in strong lensing mass reconstructions of MACS 0416, b…

astro-ph.GA2025

Addressing the core-cusp and diversity problem of dwarf and disk galaxies using cold collisionless DARKexp theory

Liliya L. R. Williams, Jens Hjorth, Evan D. Skillman

Dwarf galaxies are observed to have linearly rising rotation curves, which indicate constant density cores in their centers. These do not arise naturally from dark matter only simu…

astro-ph.GA2025

Flashlights: Prospects for constraining the Initial Mass Function around cosmic noon with caustic-crossing events

Ashish Kumar Meena, Sung Kei Li, Adi Zitrin +7

The Flashlights program with the Hubble Space Telescope imaged the six Hubble Frontier Fields galaxy clusters in two epochs and detected twenty transients. These are primarily expe…

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.GA2025

Challenging the LyC-Ly relation: strong Ly emitters without LyC leakage at z 2.3

Annalisa Citro, Claudia M. Scarlata, Kameswara B. Mantha +9

The escape fraction of LyC ionizing radiation () is crucial for understanding reionization, yet difficult to measure at . Recently, studies have focused on ca…

astro-ph.GA2025

Are Models of Strong Gravitational Lensing by Clusters Converging or Diverging?

Derek Perera, John H Miller, Liliya L. R. Williams +4

The increasingly large numbers of multiple images in cluster-scale gravitational lenses have allowed for tighter constraints on the mass distributions of these systems. Most lens m…