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The SABRE South Experiment at the Stawell Underground Physics Laboratory

The SABRE South Experiment at the Stawell Underground Physics Laboratory

Direct Detection, MetrologyFleur Morrison31 October 2025Publication

Search for nonvirialized axions with 3.3 − 4.2 μ⁢eV mass at selected resolving powers

Search for nonvirialized axions with 3.3 − 4.2 μ⁢eV mass at selected resolving powers

Direct DetectionFleur Morrison16 October 2025Publication

Search for Axion Dark Matter from 1.1 to 1.3 GHz with ADMX

Search for Axion Dark Matter from 1.1 to 1.3 GHz with ADMX

Direct DetectionFleur Morrison30 September 2025Publication

Photomultiplier requirements and pre-calibration for the SABRE South Liquid Scintillator Veto

Photomultiplier requirements and pre-calibration for the SABRE South Liquid Scintillator Veto

Direct DetectionFleur Morrison31 July 2025Publication

Characterisation of Hamamatsu R11065-20 PMTs for use in the SABRE South NaI(Tl) Crystal Detectors

Characterisation of Hamamatsu R11065-20 PMTs for use in the SABRE South NaI(Tl) Crystal Detectors

Direct DetectionFleur Morrison31 July 2025Publication

Dark Matter in the Coma cluster

Dark Matter in the Coma cluster

TheoryFleur Morrison31 July 2025Publication

Tidal adaptive softening and artificial fragmentation in cosmological simulations

Tidal adaptive softening and artificial fragmentation in cosmological simulations

TheoryFleur Morrison28 July 2025Publication

Euclid: IV. The NISP Calibration Unit

Euclid: IV. The NISP Calibration Unit

Fleur Morrison28 July 2025Publication

Ending the Hubble tension

Ending the Hubble tension

TheoryFleur Morrison28 June 2025Publication

Near-quantum-limited axion dark matter search with the ORGAN experiment around 26 μ⁢eV

Near-quantum-limited axion dark matter search with the ORGAN experiment around 26 μ⁢eV

Direct DetectionFleur Morrison31 May 2025Publication

Improved receiver noise calibration for ADMX axion search: 4.54 to 5.41 μeV

Improved receiver noise calibration for ADMX axion search: 4.54 to 5.41 μeV

Direct DetectionFleur Morrison31 May 2025Publication

Data acquisition and trigger system for the SABRE South dark matter experiment

Data acquisition and trigger system for the SABRE South dark matter experiment

Direct Detection, MetrologyFleur Morrison30 April 2025Publication

The SABRE South Experiment: Simulation and analysis of the target NaI(Tl) Crystals

The SABRE South Experiment: Simulation and analysis of the target NaI(Tl) Crystals

Direct Detection, MetrologyFleur Morrison30 April 2025Publication

Dark matter genesis

Dark matter genesis

TheoryFleur Morrison30 April 2025Publication

Euclid preparation: LXVI. Impact of line-of-sight projections on the covariance between galaxy cluster multi-wavelength observable properties: insights from hydrodynamic simulations

Euclid preparation: LXVI. Impact of line-of-sight projections on the covariance between galaxy cluster multi-wavelength observable properties: insights from hydrodynamic simulations

Fleur Morrison28 April 2025Publication

Euclid preparation: LXX. Forecasting detection limits for intracluster light in the Euclid Wide Survey

Euclid preparation: LXX. Forecasting detection limits for intracluster light in the Euclid Wide Survey

Fleur Morrison28 April 2025Publication

Euclid preparation

Euclid preparation

Fleur Morrison28 April 2025Publication

Euclid preparation: LXIX. The impact of relativistic redshift-space distortions on two-point clustering statistics from the Euclid wide spectroscopic survey

Euclid preparation: LXIX. The impact of relativistic redshift-space distortions on two-point clustering statistics from the Euclid wide spectroscopic survey

Fleur Morrison28 March 2025Publication

ADMX Axion Dark Matter Bounds around 3.3 μ⁢eV with Dine-Fischler-Srednicki-Zhitnitsky Discovery Ability

ADMX Axion Dark Matter Bounds around 3.3 μ⁢eV with Dine-Fischler-Srednicki-Zhitnitsky Discovery Ability

Direct DetectionFleur Morrison16 March 2025Publication

The SABRE South Experiment at the Stawell Underground Physics

The SABRE South Experiment at the Stawell Underground Physics

Direct DetectionFleur Morrison28 February 2025Publication