Priyanka Chakraborty
Affiliation confirmed via AI analysis of OpenAlex, ORCID, and web sources.
Assistant professor of Astrophysics
Also affiliated: Smithsonian Institution (2024); University of Kentucky (2018–2022); Smithsonian Astrophysical Observatory (2023–2024); Presidency University (2018); Center for Astrophysics Harvard & Smithsonian (2022–2026)
Research Areas
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Biography and Research Information
OverviewAI-generated summary
Priyanka Chakraborty is an assistant professor of Astrophysics at the University of Arkansas at Fayetteville. Her research focuses on astrophysical phenomena and the development of observational tools. Chakraborty has contributed to studies examining the mass-metallicity relation in the early universe, utilizing data from instruments like the James Webb Space Telescope (JWST/NIRSpec). She is also involved in the development of software for astronomical observations, including the Line Emission Mapper (LEM) and Cloudy, which probe the physics of cosmic ecosystems. Her earlier work includes research on materials science, specifically investigating the properties of sol-gel indium tin oxide films and porous silica coatings. Chakraborty has a publication record of 76 articles and a citation count of 1,264, with an h-index of 16. She has a significant collaboration history with Arnab Sarkar at the University of Arkansas at Fayetteville, with whom she shares 25 publications.
Metrics
- h-index: 14
- Publications: 60
- Citations: 625
Positions
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Assistant professor of Astrophysics 2025–presentUniversity of Arkansas at Fayetteville Physics ORCID
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Astrophysicist 2024–2025Center for Astrophysics Harvard & Smithsonian ORCID
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Postdoctoral researcher 2021–2024Center for Astrophysics Harvard & Smithsonian ORCID
Selected Publications
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Rubin J122659.4+090236: An Extremely Low Surface Brightness Galaxy Candidate Discovered in the Rubin LSST Early Data Preview 2 (2026)
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XRISM Reveals a Kinematically Coherent Core System of the Nearby Cool-Core Cluster Abell 2199 (2026)arXiv (Cornell University) OpenAlex
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XRISM Reveals a Kinematically Coherent Core System of the Nearby Cool-Core Cluster Abell 2199 (2026)
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Swift J2037.2+4151: An absorbed symbiotic X-ray binary in the Galactic plane (2026)
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Metallicity Gradients in Modern Cosmological Simulations. II. The Role of Bursty versus Smooth Feedback at High Redshift (2026)
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Detection of new galaxy candidates at <i>z</i> &gt; 11 in the JADES field using <i>JWST</i> NIRCam (2025)
Collaboration Network
Top Collaborators
- Metallicity Gradients in Modern Cosmological Simulations. II. The Role of Bursty versus Smooth Feedback at High Redshift
- Detection of new galaxy candidates at <i>z</i> &gt; 11 in the JADES field using <i>JWST</i> NIRCam
- Metallicity Gradients in Modern Cosmological Simulations. II. The Role of Bursty versus Smooth Feedback at High Redshift
- Metallicity Gradients in Modern Cosmological Simulations. II. The Role of Bursty versus Smooth Feedback at High Redshift
- Metallicity Gradients in Modern Cosmological Simulations. II. The Role of Bursty versus Smooth Feedback at High Redshift
- Metallicity Gradients in Modern Cosmological Simulations. II. The Role of Bursty versus Smooth Feedback at High Redshift
- Metallicity Gradients in Modern Cosmological Simulations. II. The Role of Bursty versus Smooth Feedback at High Redshift
- Metallicity Gradients in Modern Cosmological Simulations. II. The Role of Bursty versus Smooth Feedback at High Redshift
- Metallicity Gradients in Modern Cosmological Simulations. II. The Role of Bursty versus Smooth Feedback at High Redshift
- Metallicity Gradients in Modern Cosmological Simulations. II. The Role of Bursty versus Smooth Feedback at High Redshift
- Metallicity Gradients in Modern Cosmological Simulations. II. The Role of Bursty versus Smooth Feedback at High Redshift
- Metallicity Gradients in Modern Cosmological Simulations. II. The Role of Bursty versus Smooth Feedback at High Redshift
- Metallicity Gradients in Modern Cosmological Simulations. II. The Role of Bursty versus Smooth Feedback at High Redshift
- Metallicity Gradients in Modern Cosmological Simulations. II. The Role of Bursty versus Smooth Feedback at High Redshift
- Metallicity Gradients in Modern Cosmological Simulations. II. The Role of Bursty versus Smooth Feedback at High Redshift
- Metallicity Gradients in Modern Cosmological Simulations. II. The Role of Bursty versus Smooth Feedback at High Redshift
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