activity
19992023
most citedThe Repeating Fast Radio Burst FRB 121102 as Seen on Milliarcsecond Angular Scales

417 citations · 1.1k across the 21 of their papers we have counts for

collaborators

21 papers

astro-ph.IM2023★ 2 cited

Point Source C-Band Mueller Matrices for the Green Bank Telescope

Paul Fallon, Derck P Smits, Tapasi Ghosh +2

C-Band Mueller matrices for the Green Bank Telescope are presented here which enable on-sky Stokes parameters for point sources at the beam center to be determined. Standard calibr…

astro-ph.IM2022

Regular Solar Radio Imaging at Arecibo: Space Weather Perspective of Evolution of Active Regions

Periasamy K. Manoharan, Christopher J. Salter, Christiano M. Brum +7

The sudden release of magnetic energy on the Sun drives powerful solar flares and coronal mass ejections. The key issue is the difficulty in predicting the occurrence time and loca…

astro-ph.EP2022

Probing the Plasma Tail of Interstellar Comet 2I/Borisov

P K Manoharan, Phil Perillat, C J Salter +8

We present an occultation study of compact radio sources by the plasma tail of interstellar Comet 2I/Borisov (C/2019 Q4) both pre- and near-perihelion using the Arecibo and Green B…

hep-ph2021★ 6 cited

Dedicated Triggers for Displaced Jets using Timing Information from Electromagnetic Calorimeter at HL-LHC

Biplob Bhattacherjee, Tapasi Ghosh, Rhitaja Sengupta +1

In this paper, we study the prospect of ECAL barrel timing to develop triggers dedicated to long-lived particles decaying to jets, at the level-1 of HL-LHC. We construct over 20 ti…

astro-ph.IM2021★ 10 cited

The Future Of The Arecibo Observatory: The Next Generation Arecibo Telescope

D. Anish Roshi, N. Aponte, E. Araya +71

The Arecibo Observatory (AO) is a multidisciplinary research and education facility that is recognized worldwide as a leading facility in astronomy, planetary, and atmospheric and…

astro-ph.GA2019

Radio Recombination Line Observations Toward the Massive Star Forming Region W51 IRS1

Mishaal. I. Jan, D. Anish Roshi, M. E. Lebrón +6

We observed radio recombination lines (RRLs) toward the W51 molecular cloud complex, one of the most active star forming regions in our Galaxy. The UV radiation from young massive…