Predoc List

Zolal Ayazpour, Atomic and Molecular Physics
Advisor: Gonzalo Gonzalez Abad
Ernesto Camacho Iniguez, Optical and Infrared
Advisor: Igor Chilingaryan
Bore Gao, Optical and Infrared
Johns Hopkins University
Advisor: Catherine Zucker
Claire Hinrichs, Optical and Infrared
Dartmouth College
Advisor: Wystan Benbow
Xing Pan, Radio and Geoastronomy
Nanjing University
Advisor: Qizhou Zhang
Emily Silich, High Energy Astrophysics
Advisor: John ZuHone
Crisel Suarez
Crisel Suarez Bustamante, High Energy Astrophysics
Advisor: Christopher Moore

Crisel Suarez is a graduate student at Vanderbilt University where she is currently pursuing her Ph.D in Physics. She is interested in studying the physical properties of the solar corona by comparing different types of observations to numerical models. Her research focuses on analyzing solar flare observations from the Miniature X-ray Solar Spectrometer (MinXSS) Cubesats and using the hydrodynamic numerical simulations (HYDRAD) to better understand the emission, temperature and elemental abundances of the solar corona during flares. While at the CfA, Crisel is working with Dr. Christopher Moore to better understand the signature of Quasi-Periodic Pulsations (QPP) in solar flares by using a data constrained successive reconnection model.

Santiago Ubach Ramirez, High Energy Astrophysics
Advisor: Jack Steiner

Santi is a PhD student at Autonomous University of Barcelona (UAB) under the supervision of Dr. Gaug and Dr. Font in the high energy astrophysics group. Specially, Santi is focused on the detection of Quasi-Periodic Oscillations (QPOs) in the Very High Energy (VHE) regime inside the MAGIC collaboration to try to understand the origin of these QPOs. Such QPOs appear in stellar-mass Black Hole Binary (BHB) systems but also in Active Galactic Nucleus (AGN). At CfA and under the supervision of Dr. James Steiner, will study the Dynamic Accretion onto Stellar-Mass Black Holes, measuring the spin of black hole systems, modeling QPOs in black hole systems and relating QPO changes to spectral evolution of the BH system, modeling the geometrical and spectral characteristics during a black hole outburst, and using the premier Magellan telescopes to measure orbital characteristics and determine the masses of quiescent black hole systems. Outside of research, he enjoys reading science fiction and training for an Ironman, watching Japanese animations, and working as a field hockey coach. You can also find him playing field hockey or working extra hours.

Noah Vowell, Solar, Stellar, and Planetary Sciences
Michigan State University
Advisor: Samuel Quinn
Josephine Wong, High Energy Astrophysics
Stanford University
Advisor: Michael McCollough