One of the main reasons I want to be at a liberal arts college is that undergraduates can do real research here, and be the first author on it. My work is computational, which makes it a good fit: a student needs a laptop and a willingness to learn Python, not a beam line or a telescope allocation. The Nirvana catalog contains models of over a thousand barred galaxies, and there are more good questions to ask of it than I will ever get to on my own.

Student Projects

Four students have worked with me so far, two at Colby and two at Swarthmore.

  • Wilber Valente-Gutierrez (Swarthmore, 2026) — How do bars in spiral galaxies affect shear measurements in kinematic weak lensing? Bars produce non-circular motions that can mimic a lensing signal. Wilber is using the Nirvana bar models to quantify how much that biases a kinematic shear measurement.
  • Josephine Tuft (Swarthmore, 2026) — The effect of bisymmetric motions on Tully-Fisher scatter. Josephine is testing whether galaxies with strong second-order motions sit systematically off the Tully-Fisher relation, extending Nico Flota-Sanchez's earlier project to the full catalog.
  • Zora Lewis (Colby, 2023-2024) — Stellar population gradients in barred galaxies. Zora measured stellar population gradients across kinematically-identified bars to test whether radial mixing within the bar flattens them. This work is part of a paper in preparation.
  • Nico Flota-Sanchez (Colby, 2023-2024) — The effect of kinematic asymmetries on Tully-Fisher scatter. Nico looked at whether asymmetric galaxies scatter off the Tully-Fisher relation because our rotation models describe them badly, or because they genuinely follow a different relation.

How I Run a Project

I try to scope projects so that a student can finish something in the time they actually have — an academic year or a summer, around their coursework. That usually means handing them a well-defined question against an existing dataset rather than asking them to build infrastructure from scratch.

Most of my students arrive with one Python course or none. I spend the first few weeks on the same kind of hands-on data work I used to teach in my scientific computing class and the Lamat REU bootcamp: load the data, look at it, plot it, fit something to it. I meet with research students at least daily over summers to ensure that they're never stuck too long on a single bug.

Projects I'd Like to Start

If you are a student reading this, these are the questions I have sitting on the shelf. All of them are open, computational, and sized for an undergraduate.

  • Fitting a parametric model to bar rotation curves. There is no accepted functional form for the radial flows inside a bar. We have over a thousand nonparametric curves; someone should fit candidate models to all of them and see which wins.
  • Looking for outflows. Nirvana currently assumes gas is neither flowing in nor out. Relaxing that assumption would turn it into a tool for finding obscured AGN.
  • Bars at high redshift. JWST is producing resolved spectroscopy of distant galaxies. Do their bars look like nearby ones?
  • Bar strength and environment. MaNGA galaxies have environment measurements. Do galaxies in dense environments have stronger bisymmetric motions?