

I'm a graduate student pursuing my PhD in Astronomy at New Mexico State University, with a B.S. in Physics. My research interests focus on galaxy clusters and high-redshift galaxies.
I started as a National Science Foundation Research Experiences for Undergraduates (NSF REU) intern at the Maria Mitchell Association during the summer of 2024. Since then I have continued working with Dr. Mónica Relaño, with whom I collaborated with there. I have been studying the interplay between dust, gas, and stars in high-redshift galaxies as part of the CRISTAL survey ([CII] Resolved ISM in Star-forming Galaxies with ALMA). This survey investigates the gas, dust, and stars in representative sample of star-forming galaxies at redshifts of z ~ 4-5 on kiloparsec-spatially resolved scales. Specifically, I utilized JWST observations to create emission line maps for two galaxies within this sample. To analyze these maps, I processed the data in Python and performed Gaussian fiting to extract emission lines. based on these emission line maps, I derived estimates of the gas, dust, and star distributions within the galaxies, all through Python. Our findings are currently being prepared for publication.
I started as a National Science Foundation Research Experiences for Undergradutes (NSF REU) intern at the University of Utah during the summer of 2023. Since then I have continued working with Dr. Daniel Wik, with whom I collaborated with there. I used NuSTAR observations of 10 relaxed galaxy clusters to measure their temperatures and compared them with measurements from Chandra and XMM-Newton in identical regions. This process involved NuSTAR observations using light curve filtering, background characterization, and global spectral extraction/fitting. All of this work was done in IDL and Xspec (spectral fitting program). Our findings are currently being submitted for publication.
I was in a group of undergraduate students, led by Dr. Rolan Allen, which explored the potential evidence for a dark matter particle with second-gauge couplings. I contributed in calculating the cross-section of the proposed particle using Monte Carlo integration in Python.




Department of Astronomy
New Mexico State University
Las Cruces, NM 88001
fl@nmsu.edu