Welcome.

Cosmology, Galaxy Clusters, Dynamics

I am Alex Rodriguez, a 6th-year astronomy PhD student at the University of Michigan and a Caltech/IPAC Visiting Research Fellow studying galaxy cluster dynamics, weak lensing, and the expansion history of the Universe.

Research Overview

From dynamics to cosmology.

01

Phase-space dynamics

Galaxy redshifts define a projected radius-velocity space. The fastest galaxies trace the energy scale needed to escape the cluster potential.

02

Weak lensing and structure

Galaxy shear maps projected mass. I use weak lensing to study cluster substructure and identify candidate cosmic-web filaments.

03

Cosmological acceleration

Escape from a cluster depends on mass and on the accelerated expansion of the background universe.

Phase-Space Dynamics

The fastest cluster galaxies measure the potential.

The escape edge is the outer boundary of the radius-velocity diagram. More massive clusters have deeper potentials, so their fastest galaxies reach higher velocities. Sparse sampling lowers the measured edge.

less massive more massive
less sampling more sampling
Measured edge 82% of true profile
Focused AS1063 mass comparison figure

AS1063

Escape Velocity Mass of AS1063

A disturbed massive cluster where the escape-velocity mass agrees with lensing and SZ estimates.

Rodriguez et al. 2024
Weak-lensing mass versus escape-velocity mass figure

Cluster Sample

Weak Lensing and Escape-Velocity Concordance

A larger cluster sample showing strong agreement between independent lensing and escape-velocity mass estimates.

Rodriguez & Miller 2025
Predicted velocity bias for 45 clusters from simulations

Velocity Dispersions

Galaxy Velocity Bias in Galaxy Cluster Observations

We measure \(\sigma_v\) for 45 clusters in observations and measure the predicted velocity bias to be at the same level as relative differences in cosmological simulations.

Rodriguez et al. 2026a (in prep)

Cosmology

A dynamical probe of dark energy.

The escape velocity profile is affected by the expansion of the background, making it the only known dynamical probe of cosmology, complementary to distance-based probes.

This is particularly attractive when analyzing the expansion history of our universe through probes like \(q(z)\), where recent DESI results have hinted at decelerating cosmologies. Rodriguez 2026b, in prep.

less expansion more expansion
less sampling more sampling
Measured edge 82% of true profile
Lensing and Dynamics

Projection, redshifts, and orbital structure.

My lensing and earlier dynamics work ask how gravitational systems assemble, from galactic nuclei to cluster-scale filaments.

Subaru HSC color image of MACSJ0600 with weak-lensing convergence contours

MACSJ0600

Mapping a cosmic-web node

Subaru/HSC shear shows projected mass structure around MACS J0600.1-2008. Magellan/IMACS spectroscopy will test whether those features are genuine cluster-connected filaments.

Rodriguez et al. 2026c (in prep)

Eccentricity evolution for an ideal eccentric nuclear disk and an isolated disk

Nuclear Dynamics

Eccentric nuclear disks

Eccentric nuclear disks with a secondary SMBH can induce slowed secular evolution, along with eccentricity oscillations, aligning the disk and enhancing TDE rates.

Rodriguez, Generozov & Madigan 2021
Teaching and Outreach

Astronomy for classrooms, museums, and the public.

Science Communication Fellowship

Scientist Spotlight

Designed a hands-on demo for children explaining how galaxies can escape from galaxy clusters.

Alexander Rodriguez leading an interactive demo with a child at Scientist Spotlight

Planetarium

Museum of Natural History

Served for two years as a planetarium presenter, designing and giving interactive astronomy shows for the public.

Audience watching a star-filled planetarium show

Lead Instructor

ASTRO 127: Naked Eye Astronomy

Led four semesters and eight mini-terms as part of the Michigan Graduate Teaching Cerificate (GTC) requirements, designing lectures, labs, assignments, and projects on the Sun, Moon, planets, stars, comets, meteors, and the motion of the sky.

Quantitative Finance

Astronomy methods for financial markets.

I interned at Wells Fargo in Summer 2025 as a Quantitative Analyst in Market and Counterparty Risk Analytics, where I modeled correlated default structure in global portfolios using unsupervised learning and multi-factor regressions. I am interested in alpha research at the intersection of Bayesian inference, variational methods, entropy-based modeling, and unsupervised learning. My astrophysics research has trained me to extract weak signals from noisy, incomplete, high-dimensional data, and I am excited to apply that background to latent market structure, systematic trading signals, and market prediction.

Finance resume