- A. K. Gautam, T. Do, A. M. Ghez, et al. An Adaptive Optics Survey of Stellar Variability at the Galactic Center
Journal Link: ApJ, 871:103, 2019 | Open Access: arXiv:1811.04898
- S. Jia, et al. The Galactic Center: Improved Relative Astrometry for Velocities, Accelerations, and Orbits near the Supermassive Black Hole
Journal Link: ApJ, 873:9, 2019 | Open Access: arXiv:1902.02491
- S. Sakai, et al. The Galactic Center: An Improved Astrometric Reference Frame for Stellar Orbits around the Supermassive Black Hole
Journal Link: ApJ, 873:65, 2019 | Open Access: arXiv:1901.08685
- D. S. Chu, et al. Investigating the Binarity of S0-2
Journal Link: ApJ, 854:12, 2018 | Open Access: arXiv:1709.04890
Conference talks and proceedings
- A. K. Gautam, T. Do, A. M. Ghez, et al. Photometric detection of a candidate low-mass giant binary system at the Milky Way Galactic Center
AAS 231, 2018 January
- A. K. Gautam, T. Do, A. M. Ghez, et al. Constraining the Variability and Binary Fraction of Galactic Center Young Stars
IAU Symposium 322, 2016 July
- A. K. Gautam, A. Siemion, E. J. Korpela, et al. SETI Searches for Radio Transients from Kepler Field Planets and Astropulse Candidates
AAS 224, 2014 June
Stellar and dynamical environment
of the Milky Way Galactic center
My graduate thesis research projects primarily study the stellar population and dynamical environment of the Milky Way Galactic center (GC). My projects largely use near-infrared adaptive optics imaging data of the Galactic center taken using the Keck II telescope. Through my projects, I’ve developed a methodology to extract precise photometry from the UCLA Galactic Center Group’s 12 year AO imaging dataset. Precise photometry of the GC stars presents a valuable way to understand the nature of the stars at the Galactic center and the environment they inhabit.
One way I’m using photometry data is detecting binary star systems to help answer some open questions about the GC stars and dynamical history. The GC has a surprising collection of young stars in close proximity to the central black hole, and a distribution of old stars that don’t quite match theoretical expectations. Binary star systems are valuable ways to help us better understand both open questions: the birth of binary star systems can tell us about star formation, and the survival of binary star systems tells us about what kinds of dynamical environments they have encountered over their lifetimes.
I worked on several projects to search for transients in radio data with the Berkeley SETI Research Center (BSRC). This included radio observations of Kepler Objects of Interest (KOI) in the Kepler Field, re-observations of candidates from the Astropulse survey, and millimeter observations of the galactic center. The goal was to search for SETI signals and signals from natural radio transients such as pulsars, FRBs, and RRATs.
(2011 – 2014)
Analysis of the Guitar Nebula and PSR B2224+65
I worked on analyzing multiple epochs of radio, optical, and x-ray data of the region surrounding the pulsar B2224+65 with Professor Jim Cordes and Dr. Shami Chatterjee at Cornell University. This included the very interesting bow-shock nebula created by the pulsar known as the Guitar Nebula. The work was conducted at Cornell University’s 2012 Astronomy REU Program.
Sgr A* VLBI Calibration
I worked on calibration work for VLBI (Very Long Baseline Interferometry) observations of Sgr A* at millimeter wavelengths with Dr. Melvyn Wright at UC Berkeley.