Priyanka Chakraborty
- Neutron Stars and White Dwarfs
- Spectroscopy
- Atomic & Molecular Data
- Black Holes
- Variable Stars and Binaries
- Elemental Abundances
- Galaxy Clusters
- Intergalactic Medium
- Jets, Outflows and Shocks
- Large Scale Structure
- Computational Astrophysics
- Cosmology
- Extragalactic Astronomy
- Laboratory Astrophysics
- Stellar Astronomy
- The Energetic Universe
About
The primary focus of Priyanka's research is high-resolution X-ray spectroscopy. She uses data from high-resolution spectral data from telescopes such as Chandra, XMM-Newton, and Hitomi to addresses fundamental inquiries surrounding accretion disk winds, relativistic jets in X-ray binaries (XRBs), properties of the Intra-cluster medium, (ICM), and the growth of galaxy clusters. Priyanka is a member of the XRISM team, and serving as PI and Co-I, she has obtained over $600,000 in NASA observational grants, including fundings from Chandra, XRISM, and NuSTAR. She is an expert in modeling both collisionally-ionized and photoionized plasma, and has been an active developer of the spectral synthesis codes - AtomDB and Cloudy for several years. Priyanka's expertise extends to multiwavelength studies, spanning microwave, optical, and near-infrared bands, utilizing Planck SZ observations for galaxy groups and SDSS data to probe quasar distribution within dark matter halos.
For detailed information on Priyanka's work, refer to the following link:
Education
PhD from University of Kentucky
Press releases
NASAs Chandra Finds Galaxy Cluster Collision on a "WHIM"
https://www.nasa.gov/missions/chandra/nasas-chandra-finds-galaxy-cluster-collision-on-a-whim/
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