Max E. Lee
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View article: The effect of intrinsic alignments on weak lensing statistics in hydrodynamical simulations
The effect of intrinsic alignments on weak lensing statistics in hydrodynamical simulations Open
The next generation of weak gravitational lensing surveys has the potential to place stringent constraints on cosmological parameters. However, their analysis is limited by systematics such as the intrinsic alignments of galaxies, which al…
View article: Cosmological and Astrophysical Parameter Inference from Stacked Galaxy Cluster Profiles Using CAMELS-zoomGZ
Cosmological and Astrophysical Parameter Inference from Stacked Galaxy Cluster Profiles Using CAMELS-zoomGZ Open
We present a study on the inference of cosmological and astrophysical parameters using stacked galaxy cluster profiles. Utilizing the CAMELS-zoomGZ simulations, we explore how various cluster properties—such as X-ray surface brightness, ga…
View article: Cosmological and Astrophysical Parameter Inference from Stacked Galaxy Cluster Profiles Using CAMELS-zoomGZ
Cosmological and Astrophysical Parameter Inference from Stacked Galaxy Cluster Profiles Using CAMELS-zoomGZ Open
We present a study on the inference of cosmological and astrophysical parameters using stacked galaxy cluster profiles. Utilizing the CAMELS-zoomGZ simulations, we explore how various cluster properties--such as X-ray surface brightness, g…
View article: Zooming by in the CARPoolGP Lane: New CAMELS-TNG Simulations of Zoomed-in Massive Halos
Zooming by in the CARPoolGP Lane: New CAMELS-TNG Simulations of Zoomed-in Massive Halos Open
Galaxy formation models within cosmological hydrodynamical simulations contain numerous parameters with nontrivial influences over the resulting properties of simulated cosmic structures and galaxy populations. It is computationally challe…
View article: Zooming by in the CARPoolGP lane: new CAMELS-TNG simulations of zoomed-in massive halos
Zooming by in the CARPoolGP lane: new CAMELS-TNG simulations of zoomed-in massive halos Open
Galaxy formation models within cosmological hydrodynamical simulations contain numerous parameters with non-trivial influences over the resulting properties of simulated cosmic structures and galaxy populations. It is computationally chall…
View article: Comparing weak lensing peak counts in baryonic correction models to\n hydrodynamical simulations
Comparing weak lensing peak counts in baryonic correction models to\n hydrodynamical simulations Open
Next-generation weak lensing (WL) surveys, such as by the Vera Rubin\nObservatory's LSST, the $\\textit{Roman}$ Space Telescope, and the\n$\\textit{Euclid}$ space mission, will supply vast amounts of data probing\nsmall, highly nonlinear s…
View article: Redundant-baseline calibration of the hydrogen epoch of reionization array
Redundant-baseline calibration of the hydrogen epoch of reionization array Open
In 21-cm cosmology, precision calibration is key to the separation of the neutral hydrogen signal from very bright but spectrally smooth astrophysical foregrounds. The Hydrogen Epoch of Reionization Array (HERA), an interferometer speciali…