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Pratik Majumdar

Researcher at Saha Institute of Nuclear Physics

Publications -  33
Citations -  561

Pratik Majumdar is an academic researcher from Saha Institute of Nuclear Physics. The author has contributed to research in topics: Fermi Gamma-ray Space Telescope & Blazar. The author has an hindex of 9, co-authored 33 publications receiving 428 citations.

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Journal ArticleDOI

The Blazar TXS 0506+056 Associated with a High-energy Neutrino: Insights into Extragalactic Jets and Cosmic-Ray Acceleration

Stefano Ansoldi, +153 more
TL;DR: In this article, a neutrino with energy similar to 290 TeV was detected in coincidence with the BL Lac object TXS. 0506+056 during enhanced gamma-ray activity, with chance coincidence being rejected at similar to 3 sigma level.
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Multiband variability studies and novel broadband SED modeling of Mrk 501 in 2009

Max Ludwig Ahnen, +315 more
TL;DR: In this paper, the authors present an extensive study of the BL Lac object Mrk 501 based on a data set collected during the multi-instrument campaign spanning from 2009 March 15 to 2009 August 1, which includes, among other instruments, MAGIC, VERITAS, Whipple 10m, and Fermi-LAT to cover the γ-ray range from 0.1 GeV to 20 TeV.
Journal ArticleDOI

Multiband variability studies and novel broadband SED modeling of Mrk 501 in 2009

Max Ludwig Ahnen, +311 more
TL;DR: In this article, an extensive study of the BL Lac object Mrk 501 based on a data set collected during the multi-instrument campaign spanning from 2009 March 15 to 2009 August 1 is presented.
Journal ArticleDOI

Fermi-Large Area Telescope Observations of the Brightest Gamma-Ray Flare Ever Detected from CTA 102

TL;DR: In this article, a multi-wavelength study of the FSRQ CTA 102 using Fermi-LAT and simultaneous Swift-XRT/UVOT observations is presented.
Proceedings ArticleDOI

Discovery of Very High Energy Gamma-Rays from the Distant Flat Spectrum Radio Quasar 3C 279 with the MAGIC Telescope

TL;DR: In this paper, the MAGIC telescope was used to detect a very high energy gamma-ray signal from 3C 279 with a very large redshift of z = 0.536.