The cosmic microwave background radiation fluctuations from H i perturbations prior to reionization S Bharadwaj, SS Ali Monthly Notices of the Royal Astronomical Society 352 (1), 142-146, 2004 | 234 | 2004 |
On using visibility correlations to probe the Hi distribution from the dark ages to the present epoch – I. Formalism and the expected signal S Bharadwaj, SK Saiyad Ali Monthly Notices of the Royal Astronomical Society 356 (4), 1519-1528, 2005 | 195 | 2005 |
Testing homogeneity on large scales in the sloan digital sky survey data release one J Yadav, S Bharadwaj, B Pandey, TR Seshadri Monthly Notices of the Royal Astronomical Society 364 (2), 601-606, 2005 | 170 | 2005 |
HI fluctuations at large redshifts: I-visibility correlation S Bharadwaj, SK Sethi Journal of Astrophysics and Astronomy 22, 293-307, 2001 | 155 | 2001 |
Foregrounds for redshifted 21-cm studies of reionization: Giant Meter Wave Radio Telescope 153-MHz observations SS Ali, S Bharadwaj, JN Chengalur Monthly Notices of the Royal Astronomical Society 385 (4), 2166-2174, 2008 | 141 | 2008 |
Using HI to probe large scale structures at z∼ 3 S Bharadwaj, BB Nath, SK Sethi Journal of Astrophysics and Astronomy 22, 21-34, 2001 | 140 | 2001 |
The multifrequency angular power spectrum of the epoch of reionization 21-cm signal KK Datta, TR Choudhury, S Bharadwaj Monthly Notices of the Royal Astronomical Society 378 (1), 119-128, 2007 | 131 | 2007 |
The scale of homogeneity of the galaxy distribution in SDSS DR6 P Sarkar, J Yadav, B Pandey, S Bharadwaj Monthly Notices of the Royal Astronomical Society: Letters 399 (1), L128-L131, 2009 | 130 | 2009 |
Characterizing foreground for redshifted 21 cm radiation: 150 MHz Giant Metrewave Radio Telescope observations A Ghosh, J Prasad, S Bharadwaj, SS Ali, JN Chengalur Monthly Notices of the Royal Astronomical Society 426 (4), 3295-3314, 2012 | 128 | 2012 |
Quantifying the non-Gaussianity in the EoR 21-cm signal through bispectrum S Majumdar, JR Pritchard, R Mondal, CA Watkinson, S Bharadwaj, ... Monthly Notices of the Royal Astronomical Society 476 (3), 4007-4024, 2018 | 110 | 2018 |
On the use of seminumerical simulations in predicting the 21-cm signal from the epoch of reionization S Majumdar, G Mellema, KK Datta, H Jensen, TR Choudhury, ... Monthly Notices of the Royal Astronomical Society 443 (4), 2843-2861, 2014 | 101 | 2014 |
Modeling galaxy halos using dark matter with pressure S Bharadwaj, S Kar Physical Review D 68 (2), 023516, 2003 | 100 | 2003 |
The size of the longest filaments in the universe S Bharadwaj, SP Bhavsar, JV Sheth The Astrophysical Journal 606 (1), 25, 2004 | 90 | 2004 |
Improved foreground removal in GMRT 610 MHz observations towards redshifted 21-cm tomography A Ghosh, S Bharadwaj, SS Ali, JN Chengalur Monthly Notices of the Royal Astronomical Society 418 (4), 2584-2589, 2011 | 80 | 2011 |
Evidence for filamentarity in the Las Campanas redshift survey S Bharadwaj, V Sahni, BS Sathyaprakash, SF Shandarin, C Yess The Astrophysical Journal 528 (1), 21, 2000 | 75 | 2000 |
Probing non-Gaussian features in the H i distribution at the epoch of re-ionization S Bharadwaj, SK Pandey Monthly Notices of the Royal Astronomical Society 358 (3), 968-976, 2005 | 74 | 2005 |
A study of interstellar medium of dwarf galaxies using H i power spectrum analysis P Dutta, A Begum, S Bharadwaj, JN Chengalur Monthly Notices of the Royal Astronomical Society 398 (2), 887-897, 2009 | 68 | 2009 |
The evolution of correlation functions in the zeldovich approximation and its implications for the validity of perturbation theory S Bharadwaj The Astrophysical Journal 472 (1), 1, 1996 | 67 | 1996 |
Estimation of cosmological parameters from neutral hydrogen observations of the<? format?> post-reionization epoch S Bharadwaj, SK Sethi, TD Saini Physical Review D—Particles, Fields, Gravitation, and Cosmology 79 (8), 083538, 2009 | 63 | 2009 |
Visibility-based angular power spectrum estimation in low-frequency radio interferometric observations S Choudhuri, S Bharadwaj, A Ghosh, SS Ali Monthly Notices of the Royal Astronomical Society 445 (4), 4351-4365, 2014 | 61 | 2014 |