Hi! I’m Gilberto Garcia. I am a first-generation graduate student at the University of Oklahoma's Department of Physics and Astronomy. I am currently based in Norman, Oklahoma but was born and raised in Chicago, Illinois. I completed my undergraduate education at Wesleyan University, earning a degree in Astronomy and Physics and working as an Astronomy research assistant. With this experience, I am pursuing a career as an Astrophysicist. You can learn more about my research in my research page.
Because of my background, I am deeply invested in STEM outreach and education, specifically working towards minimizing the education access gap and providing resources to underserved student populations. Because of this, I have actively participated in STEM outreach programs and tutoring positions in Norman, Chicago, and Middletown. To learn more about my work, you can take a look at my CV page
Outside of academics, I am a huge soccer fan. I have enjoyed watching and playing it since I was a kid, and played for school, club, and travel teams. Along with soccer, I like to keep myself active nowadays with running, cycling, and hiking.
DNA in a non-helical structure, like a in a hairpin, are at fault for various genetic disorders. It is known that the formation of these non-helical structures in DNA is induced from crowded cellular enviornments, but the dynamics and stability of the hairpin within these crowded envirnments is not well studied. Using single-molecule Forster resonance energy (FRET) microscopy, I am examining these parameters for a set of DNA with trinucleotide repeats under various crowding conditions.
I am also studying the effects of internal loops on the stability of DNA's helical structure by looking at the temperature-dependent changes in the UV absorbance of DNA.
I will be presenting this work at the National Meeting of the Biophysical Society in February 2022.
Constraints on the duty cycle and duration of accretion episodes in active galactic nuclei (AGNs) are vital for establishing how most AGNs are fueled, which is essential for a complete picture of black hole/galaxy co-evolution. Perhaps the best handle we have on these activity parameters is provided by AGNs that have displayed dramatic, persistent changes in their bolometric luminosities. Given that X-ray emission is directly linked to black-hole accretion, X-ray source catalogs should provide a straightforward means of identifying AGNs that have undergone dramatic changes in their accretion states. However, it appears that such events are very rare, so observations separated in time by many years are needed to maximize discovery rates.
In this project, we cross-correlated the Einstein IPC Two-Sigma Catalog with the Chandra Source Catalog to identify a sample of soft X-ray sources that varied by factors of at least 10 over timescales of 20 or more years. Most of the extremely variable sources revealed via this technique were dimmer in the Chandra era, owing to the lower sensitivity and modest exposures associated with Einstein. Optical spectra from the Sloan Digital Sky Survey indicated that many of the variable sources were radio-quiet AGNs with broad emission lines — not "changing-look" objects that have more subtle AGN signatures in their spectra. We created long-term X-ray light curves for the sources by combining the Einstein and CSC fluxes with those obtained from serendipitous pointed observations by ROSAT.
This work resulted in an undergraduate thesis that was awarded high honors and was presented at various conferences. You can find my thesis and my presentations in the bibliography and presentations section of my CV page.
Some highlights of my academic career so far.
Some fun pictures I have taken of the sky.
You can reach or follow me at the following: