Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Astrophysical Phenomena and Observations, Galaxies: Formation, Evolution, Phenomena, Astronomy and Astrophysical Research, and Stellar, planetary, and galactic studies.
The Intracluster Light Analysis of the Most Evolved Systems of Galaxies: Fossil Groups
Low-mass Galaxy Interactions Trigger Black Hole Activity
Investigating the Mass of the Black Hole and Possible Wind Outflow of the Accretion Disk in the Tidal Disruption Event AT2021ehb
SDSS J125417.98+274004.6: An X-ray Detected Minor Merger Dual AGN
Prospects for AGN Studies with AXIS: AGN Fueling—Resolving Hot Gas inside Bondi Radius of SMBHs
Post-starburst properties of post-merger galaxies
A Multiwavelength Study of Active Galactic Nuclei in Post-merger Remnants
Two Candidates for Dual AGN in Dwarf-dwarf Galaxy Mergers
AMUSE-Antlia. I. Nuclear X-Ray Properties of Early-type Galaxies in a Dynamically Young Galaxy Cluster
Discovery of Three Candidate Magnetar-powered Fast X-Ray Transients from Chandra Archival Data
Follow-up Observations of the Prolonged, Super-Eddington, Tidal Disruption Event Candidate 3XMM J150052.0+015452: the Slow Decline Continues
An Ultraluminous Supersoft Source in a Dwarf Galaxy of A85: An Intermediate-mass Black Hole Candidate
Three ultraluminous X-ray sources hosted by globular clusters in NGC 1316
Multiwavelength Follow-up of the Hyperluminous Intermediate-mass Black Hole Candidate 3XMM J215022.4−055108
The multiwavelength spectrum of NGC 3115: hot accretion flow properties
Chandra and HST Snapshots of Fossil System Progenitors
A likely decade-long sustained tidal disruption event
Gas Sloshing Regulates and Records the Evolution of the Fornax Cluster
Large decay of X-ray flux in 2XMM J123103.2+110648: evidence for a tidal disruption event
Buoyant AGN Bubbles in the Quasi-isothermal Potential of NGC 1399
Hard X-Ray Emission from the M87 AGN Detected with NuSTAR
Multiwavelength follow-up observations of the tidal disruption event candidate 2XMMi J184725.1−631724
Using Strong Gravitational Lensing to Identify Fossil Group Progenitors
Ultraluminous X-ray bursts in two ultracompact companions to nearby elliptical galaxies
Investigating the Potential Dilution of the Metal Content of Hot Gas in Early-Type Galaxies by Accreted Cold Gas
2016cited by 20position: last
SUZAKU X-RAY OBSERVATIONS OF THE NEAREST NON-COOL CORE CLUSTER, ANTLIA: DYNAMICALLY YOUNG BUT WITH REMARKABLY RELAXED OUTSKIRTS
Flows of X-ray gas reveal the disruption of a star by a massive black hole
THE SCATTER IN THE HOT GAS CONTENT OF EARLY-TYPE GALAXIES
THE MEGASECOND<i>CHANDRA</i>X-RAY VISIONARY PROJECT OBSERVATION OF NGC 3115. III. LUMINOSITY FUNCTIONS OF LMXBS AND DEPENDENCE ON STELLAR ENVIRONMENTS
THE MEGASECOND<i>CHANDRA</i>X-RAY VISIONARY PROJECT OBSERVATION OF NGC 3115. II. PROPERTIES OF POINT SOURCES