Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Astrophysical Phenomena and Observations, Pulsars and Gravitational Waves Research, Galaxies: Formation, Evolution, Phenomena, and Astronomy and Astrophysical Research.
WIggle Corrector Kit for NIRSpEc Data: WICKED
Comparing Recent Pulsar Timing Array Results on the Nanohertz Stochastic Gravitational-wave Background
Erratum: “The NANOGrav 15 yr Data Set: Search for Signals from New Physics” (2023, ApJL 951 L11)
NANOGrav 15-year gravitational-wave background methods
The NANOGrav 12.5 yr Data Set: Search for Gravitational Wave Memory
ReveaLLAGN 0: First Look at JWST MIRI Data of Sombrero and NGC 1052
The NANOGrav 12.5 yr Data Set: A Computationally Efficient Eccentric Binary Search Pipeline and Constraints on an Eccentric Supermassive Binary Candidate in 3C 66B
The NANOGrav 15 yr Data Set: Evidence for a Gravitational-wave Background
The NANOGrav 15 yr Data Set: Search for Signals from New Physics
The NANOGrav 15 yr Data Set: Constraints on Supermassive Black Hole Binaries from the Gravitational-wave Background
The NANOGrav 15 yr Data Set: Observations and Timing of 68 Millisecond Pulsars
The NANOGrav 15 yr Data Set: Bayesian Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries
The NANOGrav 15 yr Data Set: Detector Characterization and Noise Budget
The NANOGrav 15 yr Data Set: Search for Anisotropy in the Gravitational-wave Background
Searching for continuous Gravitational Waves in the second data release of the International Pulsar Timing Array
The NANOGrav 12.5 yr Data Set: Bayesian Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries
Hα Reverberation Mapping of the Intermediate-mass Active Galactic Nucleus in NGC 4395
Discrete knot ejection from the jet in a nearby low-luminosity active galactic nucleus, M81∗
Flows of X-ray gas reveal the disruption of a star by a massive black hole
THE RATE OF GAS ACCRETION ONTO BLACK HOLES DRIVES JET VELOCITY
Effects of inclination on measuring velocity dispersion and implications for black holes