哥伦比亚大学巴纳德学院物理与天文学系导师教师师资介绍简介-Reshmi Mukherjee

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Reshmi Mukherjee


Helen Goodhart Altschul Professor of Physics & Astronomy?

Department


Physics & Astronomy

Office


Office Hours ALT 514
Wednesday 12:00-1:00pm

Altschul 506

Contact


212-854-5101

rmukherj@barnard.edu


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Reshmi Mukherjee joined the Barnard faculty in 1997. Her teaching assignments include such courses as "Introductory Physics (Mechanics)," "Experimental Methods in Physics, " "Supervised Individual Research," and "Quantum Physics."
Professor Mukherjee's research interests are in high-energy astrophysics and astroparticle physics. She uses ground-based atmospheric Cherenkov telescopes to study galactic and extragalactic high-energy gamma-ray sources.
One of her current projects is VERITAS (Very Energetic Radiation Imaging Telescope Array System), located in southern Arizona. VERITAS is a major ground-based gamma-ray observatory that enables the study of extragalactic and galactic high energy gamma-ray sources. The VERITAS collaboration uses an array of mirrors at night to detect the quick flashes of blue Cherenkov light that result from gamma-ray air showers.
Professor Mukherjee is also involved with the study of active galaxies, thought to be powered by super-massive black holes at their centers, and unidentified high-energy gamma-ray sources.

BS, Presidency College, University of Calcutta
MA, MPhil, PhD, Columbia


Experimental astrophysics


"Discovery of Very High Energy Gamma-ray Radiation from the BL Lac1ES0806+524," with V.Acciari, et al., The Astrophysical Journal690L, 126 (2009).
"Search for dark matter annihilation in Draco with the Solar Tower AtmosphericCherenkovEffect Experiment," withD.D. Driscoll, et al., Physical ReviewVol. 78, No. 8 (2008): 7101.
"On the Origin ofTeVGamma-ray Emission from HESSJ1834-087," with V.Gotthelfand J. P.Halpern, The Astrophysical Journal (2008).
"Transient X-ray sources in the field of the Unidentified Gamma-Ray SourceTeVJ2032+4130 in Cygnus," with E. V.Gotthelfand J. P.Halpern, Proceedings of the Conference The Multi-Messenger Approach to High-Energy Gamma-ray Sources, Barcelona/Spain (2006).
"Chandra Observation of the UnidentifiedTeVGamma-Ray Source HESSJ1303-631in the Galactic Plane," with J. P.Halpern, The Astrophysical Journal 629, 1017 (2005).
"MultifrequencyStrategies for the Identification of Gamma-Ray Sources," with J. P.Halpern, Cosmic Gamma-ray Sources, K. S. Cheng and G. E. Romeroeds. (KluwerAcademic Press, 2004).
"Search for a Point-Source Counterpart of the Unidentified Gamma-Ray SourceTeVJ2032+4130 in Cygnus," with J. P.Halpern, E. V.Gotthelf, M.Eracleous, and N.Mirabal, The Astrophysical Journal 589, 487 (2003).
"Predictions of the High-Energy Emission from BL Lac Objects: The Case of WComae," with M.Boettcherand A.Reimer, The Astrophysical Journal 581, 143 (2002).
"A Statistical Detection of Gamma-ray Emission from Galaxy Clusters: Implications for the Gamma-ray Background and Structure Formation," with C.Scharf, The Astrophysical Journal 580, 154 (2002).





In The News



Professor Reshmi Mukherjee Publishes New Research on Observations of an Active Galaxy during an Elevated Gamma-Ray state


July 14, 2022


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August 21, 2020


Professor Reshmi Mukherjee and Colleagues Help Prove Viability of Prototype Gamma-Ray Telescope


June 8, 2020