Research Interests

Cosmology

My research in cosmology is centered on understanding the nature of dark energy, the mysterious force driving the accelerated expansion of the universe. I am an active member of several major galaxy survey collaborations, including the Dark Energy Survey (DES), the Hyper Suprime-Cam (HSC) survey, and the Rubin LSST Dark Energy Science Collaboration (DESC). These collaborations are key to probing the large-scale structure of the universe and testing cosmological models. My work involves both the analysis of observational data and the development of theoretical models that can provide insights into the underlying physics of dark energy.

Cosmology with DES

DESY3 cosmological constraints from weak lensing and clusters.

Weak Lensing Systematics

Weak gravitational lensing is a powerful tool for studying the distribution of dark matter in the universe. However, it is also highly sensitive to systematic errors, which can bias our measurements. My research focuses on characterizing and mitigating these systematics to improve the accuracy of weak lensing measurements. This involves detailed studies of the instrumental effects and data analysis pipelines used in surveys like DES and HSC. I am also involved in the Rubin LSST DESC, where I contribute to the development of algorithms that will ensure the robustness of weak lensing studies with LSST.

Tree rings in DECam

Imprint of CCD tree rings on astrometric residuals in DECam.

Strong Lensing Simulations

Strong gravitational lensing provides a unique opportunity to study distant galaxies and the distribution of dark matter on small scales. My work in this area involves creating and analyzing simulations of strong lensing events, which can be used to test theoretical models and to prepare for future observations with the Rubin Observatory. I am a member of the Strong Lensing Collaboration within LSST DESC, where we are developing techniques to identify and study strong lensing systems in the vast LSST dataset.

Strong Lensing Simulation images with skylens3

Simulation of strong gravitational lensing events with different instruments using Skylens.

Instrumentation and detectors

I am deeply interested in the development and use of advanced sensors, including CCDs and near-infrared detectors, to tackle fundamental problems in cosmology, such as understanding dark matter and dark energy, as well as other key physics questions. I proposed and co-organized the Image Sensors for Precision Astronomy conference, which was held at SLAC/KIPAC in March 2024, bringing together experts to explore the latest advancements in sensor technology for astronomy.

Fully-depleted CCDs

I have been actively involved in the electro-optical testing and characterization of fully-depleted, back-illuminated CCDs for astronomical cameras, including the Dark Energy Camera (DECam) and the LSST Camera. These CCDs are critical for capturing high-precision images used in weak lensing and galaxy surveys. My work has focused on understanding and mitigating systematic errors in CCD performance, ensuring that these detectors meet the stringent requirements for cosmological experiments aiming to measure dark energy and dark matter. This experience has contributed to the success of large-scale surveys like the Dark Energy Survey (DES) and the Vera C. Rubin Observatory's Legacy Survey of Space and Time (LSST).

Skipper CCDs

Skipper CCDs are an innovative type of detector that allows for the precise measurement of very low levels of charge, making them ideal for applications in cosmology and particle physics. My research involves both the development and characterization of these detectors, as well as their application to scientific problems such as direct detection of dark matter and low-level light detection in astronomical observations. I work closely with teams developing these detectors and exploring their potential for use in future space missions and ground-based telescopes.

HxRG detectors for Roman and Euclid

Near-infrared (NIR) detectors are crucial for weak lensing science, especially in space-based missions like NASA's Roman Space Telescope and Euclid. These detectors, such as the HgCdTe-based Hawaii-XRG, are used to capture the subtle distortions of distant galaxy shapes caused by dark matter, known as cosmic shear. Precise measurements of these shapes are critical for understanding dark energy and the large-scale structure of the universe. However, systematic effects like the "brighter-fatter" effect, where brighter point sources appear larger due to charge redistribution between pixels, can bias weak lensing measurements. My work focuses on detailed calibration and correction of these systematic effects in NIR detectors to ensure the accuracy of cosmological inferences.

Community and Citizen Science

I am passionate about involving the public in scientific research, and I have led several community science projects. These include studies of the incidence angle and crater counting on planetary surfaces, as well as the formation of the solar system. Through these projects, volunteers are able to contribute to real scientific discoveries while learning about planetary science and the history of our solar system. My work in this area is part of a broader effort to democratize science and make it accessible to everyone, regardless of their background.

Crater counting

Effect of solar incidence angle on crater counting in MoonMappers CosmoquestX project.

Rubin Observatory: Calibration and Community Science

As part of my role at the Rubin Observatory, I am heavily involved in the calibration of the observatory's instruments and the development of tools and resources for the scientific community. This includes ensuring that the data produced by the observatory is accurate and reliable, as well as supporting scientists and citizen scientists who want to use Rubin data for their own research. My work in the Community Science Team is focused on building a vibrant, inclusive community of researchers who are equipped to make the most of the unprecedented data set that the Rubin Observatory will produce.

Publications

Total Publications

More than 410 publications, including those as a builder of the Dark Energy Survey. Citations: 40020. h-index:96. i10-index:373

Complete list of publications

Lead Author Publications

Publications as Coauthor with Substantial Contributions

Publications for Education and Public Outreach