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Zooming into the broad line region of the gravitationally lensed quasar QSO 2237+0305 equivalent to the Einstein Cross III. Determination of the size and structure of the C-IV and C-III] emitting regions using microlensing

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Zooming into the broad line region of the gravitationally lensed quasar QSO 2237+0305 equivalent to the Einstein Cross III. Determination of the size and structure of the C-IV and C-III] emitting regions using microlensing

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The DESI Survey Validation: Results from Visual Inspection of Bright Galaxies, Luminous Red Galaxies, and Emission-line Galaxies

Constraining quasar structure using high-frequency microlensing variations and continuum reverberation

Do the majority of stars form as gravitationally unbound?

J1721+8842: a gravitationally lensed binary quasar with a proximate damped Lyman-alpha absorber

A machine learning approach to correct for mass resolution effects in simulated halo clustering statistics

Single-Mode Emission in InP Microdisks on Si Using Au Antenna

The Pristine survey IX. CFHT ESPaDOnS spectroscopic analysis of 115 bright metal-poor candidate stars

Microlensing Analysis for the Gravitational Lens Systems SDSS0924+0219, Q1355-2257, and SDSS1029+2623

Time-delay Cosmography with Strongly Lensed Quasars

Constraining the primordial magnetic field with dwarf galaxy simulations

Measuring accretion disk sizes of lensed quasars with microlensing time delay in multi-band light curves

Testing the evolution of correlations between supermassive black holes and their host galaxies using eight strongly lensed quasars

A Microlensing Accretion Disk Size Measurement in the Lensed Quasar WFI 2026-4536

TDCOSMO. IV. Hierarchical time-delay cosmography - joint inference of the Hubble constant and galaxy density profiles

The GOGREEN survey: Internal dynamics of clusters of galaxies at redshift 0.9-1.4

COSMOGRAIL: XIX. Time delays in 18 strongly lensed quasars from 15 years of optical monitoring star

The formation of the milky way halo and its dwarf satellites: a NLTE-1D abundance analysis. IV. Segue 1, Triangulumii, and Coma Berenices UFDs