activity
20242026
most citedTowards -cm intensity mapping at with uGMRT using the tapered gridded estimator -- IV. Wideband analysis

9 citations · 11 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.CO2026

Forest without Trees is still Fruitful: Constraints on the thermal state of the neutral IGM at with the 21-cm forest power spectrum

Tomáš Šoltinský, Arnab Chakraborty, Girish Kulkarni +10

Neutral regions of the intergalactic medium (IGM) during the Epoch of Reionization (EoR) remain largely unexplored due to the limitations of existing probes. Owing to discoveries o…

astro-ph.CO2026

Intensity fluctuations of radio halo in galaxy cluster: Insights from power spectrum estimation

Srijita Pal, Nirupam Roy, Sameer Salunkhe +3

Non-thermal synchrotron emissions from radio halo allow us to study mechanisms of particle (re)acceleration, magnetic field distribution, merger history, and turbulence in the intr…

astro-ph.GA2026

Detection of non-thermal radio emission components from the Orion Nebula: stellar jets, cloud collision or feedback from stellar winds?

Md Rashid, Nirupam Roy, Prasun Dutta +5

The Orion Nebula is the closest high-mass star-forming region, making it an ideal laboratory to investigate physical processes in complex star-forming environments. At radio freque…

astro-ph.HE2025

ELAIS-N1 deep field uGMRT Band-2: constraints on diffuse Galactic synchrotron emission power spectrum

Rashmi Sagar, Abhirup Datta, Arnab Chakraborty +13

We present high sensitivity, low radio frequency continuum observations of the ELAIS-N1 field with 32 hours of observations of the uGMRT Band-2 ( MHz) covering $5.86\,\tex…

astro-ph.CO2025

Deep uGMRT observations for enhanced calibration of 21 cm arrays -- I. First image and source catalogue

Khandakar Md Asif Elahi, Samir Choudhuri, Nirupam Roy +3

Radio-interferometric arrays require very precise calibration to detect the Epoch of Reionization 21-cm signal. A remarkably complete and accurate sky model is therefore needed in…

astro-ph.CO2025

Calibration requirements for Epoch of Reionization 21-cm signal observations -- IV. Bias and variance with time and frequency correlated residual gains

Saikat Gayen, Jais Kumar, Prasun Dutta +3

Observation of multifrequency angular power spectrum of the redshifted 21-cm brightness temperature fluctuation from the neutral hydrogen holds the key to understand the structure…

astro-ph.IM2024

Reliability of in-band and broadband spectral index measurement: systematic study of the effect of signal to noise for uGMRT data

Md Rashid, Nirupam Roy, J. D. Pandian +4

Low radio frequency spectral index measurements are a powerful tool to distinguish between different emission mechanisms and, in turn, to understand the nature of the sources. Besi…

astro-ph.CO2024★ 9 cited

Towards -cm intensity mapping at with uGMRT using the tapered gridded estimator -- IV. Wideband analysis

Khandakar Md Asif Elahi, Somnath Bharadwaj, Srijita Pal +8

We present a Wideband Tapered Gridded Estimator (TGE), which incorporates baseline migration and variation of the primary beam pattern for neutral hydrogen (${\rm H\hspace{0.5mm}}{…

astro-ph.IM2024★ 2 cited

Calibration requirement for Epoch of Reionization 21-cm signal observation -- III. Bias and variance in uGMRT ELAIS-N1 field power spectrum

Saikat Gayen, Rashmi Sagar, Sarvesh Mangla +6

Power spectrum of \HI 21-cm radiation is one of the promising probes to study large scale structure of the universe and understand galaxy formation and evolution. The presence of f…