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First multi-redshift limits on post-Epoch of Reionization (post-EoR) 21 cm signal from z = 1.96 - 3.58 using uGMRT, , , , , , , , , and 1 other author(s). (2020)cite arxiv:2012.04674Comment: Accepted for publication in the Astrophysical Journal Letters (APJL).Constraints on dark matter annihilation in dwarf spheroidal galaxies from low frequency radio observations, , , , and . (2019)cite arxiv:1907.00979Comment: 6 pages, 2 Figures, accepted in Physical Review D.Three- and two-point spatial correlations of intergalactic medium at $z2$ using projected quasar triplets, , , , , , and . (2019)cite arxiv:1907.02086Comment: 28 pages, 20 figures. Submitted to MNRAS.Lyman-$\alpha$ emitters gone missing: evidence for late reionization?, , , and . (2014)cite arxiv:1412.4790Comment: 17 pages, submitted to MNRAS.VoIgt profile Parameter Estimation Routine (VIPER): H I photoionization rate at z<0.5, , , and . (2016)cite arxiv:1610.06572Comment: 16 pages, 10 figures.Patchy reionization bias on the primordial gravitational wave signal: Better to be sure than sorry, , , and . (2022)cite arxiv:2209.12672Comment: Submitted to MNRAS.Bubble mapping with the Square Kilometer Array - I. Detecting galaxies with Euclid, JWST, WFIRST and ELT within ionized bubbles in the intergalactic medium at z>6, , , , , , , , , and 9 other author(s). (2019)cite arxiv:1905.00437Comment: 17 pages, 7 figures, submitted to MNRAS.Detailed study of ELAIS N1 field with the uGMRT -- II. Source Properties and Spectral Variation Of Foreground Power Spectrum from 300-500 MHz Observations, , , , , , , , , and 1 other author(s). (2019)cite arxiv:1908.10380Comment: There are 14 figures. The revised draft after getting the first favourable comments and resubmitted for publication in MNRAS.CMB constraints on a physical model of reionization, , and . (2020)cite arxiv:2007.03705Comment: 5 pages.Constraining the reionization and thermal history of the Universe using a semi-numerical photon-conserving code SCRIPT, and . (2022)cite arxiv:2204.05268Comment: submitted to MNRAS.