| Cosmology with tachyon field as dark energy JS Bagla, HK Jassal, T Padmanabhan Physical Review D 67 (6), 063504, 2003 | 683 | 2003 |
| WMAP constraints on low redshift evolution of dark energy HK Jassal, JS Bagla, T Padmanabhan Monthly Notices of the Royal Astronomical Society: Letters 356 (1), L11-L16, 2005 | 438 | 2005 |
| Gamma-ray bursts from stellar remnants: probing the Universe at high redshift RAMJ Wijers, JS Bloom, JS Bagla, P Natarajan Monthly Notices of the Royal Astronomical Society 294 (1), L13-L17, 1998 | 360 | 1998 |
| Observational constraints on low redshift evolution of dark energy:<? format?> How consistent are different observations? HK Jassal, JS Bagla, T Padmanabhan Physical Review D—Particles, Fields, Gravitation, and Cosmology 72 (10), 103503, 2005 | 260 | 2005 |
| TreePM: A code for cosmological N-body simulations JS Bagla Journal of Astrophysics and Astronomy 23, 185-196, 2002 | 236 | 2002 |
| Fractal dimension as a measure of the scale of homogeneity JK Yadav, JS Bagla, N Khandai Monthly Notices of the Royal Astronomical Society 405 (3), 2009-2015, 2010 | 145 | 2010 |
| Understanding the origin of CMB constraints on dark energy HK Jassal, JS Bagla, T Padmanabhan Monthly Notices of the Royal Astronomical Society 405 (4), 2639-2650, 2010 | 133* | 2010 |
| HI as a probe of the large-scale structure in the post-reionization universe JS Bagla, N Khandai, KK Datta Monthly Notices of the Royal Astronomical Society 407 (1), 567-580, 2010 | 123 | 2010 |
| Crisis in Cosmology: Observational Constraints on Omega and H_0 JS Bagla, T Padmanabhan, JV Narlikar arXiv preprint astro-ph/9511102, 1995 | 110 | 1995 |
| Non-linear evolution of density perturbations using the approximate constancy of the gravitational potential JS Bagla, T Padmanabhan Monthly Notices of the Royal Astronomical Society 266 (1), 227-237, 1994 | 103 | 1994 |
| Cosmological N-body simulation: Techniques, scope and status JS Bagla Current science, 1088-1100, 2005 | 96 | 2005 |
| Evolution of galaxy clustering JS Bagla Monthly Notices of the Royal Astronomical Society 299 (2), 417-424, 1998 | 83 | 1998 |
| Transfer of power in non-linear gravitational clustering JS Bagla, T Padmanabhan Monthly Notices of the Royal Astronomical Society 286 (4), 1023-1031, 1997 | 75 | 1997 |
| CosmologicalN-body simulations JS Bagla, T Padmanabhan Pramana 49, 161-192, 1997 | 72 | 1997 |
| Atomic hydrogen in star-forming galaxies at intermediate redshifts A Bera, N Kanekar, JN Chengalur, JS Bagla The Astrophysical Journal Letters 882 (1), L7, 2019 | 62 | 2019 |
| Comments on the size of the simulation box in cosmological N-body simulations JS Bagla, S Ray Monthly Notices of the Royal Astronomical Society 358 (3), 1076-1082, 2005 | 61 | 2005 |
| Performance characteristics of TreePM codes JS Bagla, S Ray New Astronomy 8 (7), 665-677, 2003 | 61 | 2003 |
| Gravitational lensing of gravitational waves: wave nature and prospects for detection AK Meena, JS Bagla Monthly Notices of the Royal Astronomical Society 492 (1), 1127-1134, 2020 | 54 | 2020 |
| The observed evolution of galaxy clustering versus epoch-dependent biasing models M Magliocchetti, JS Bagla, SJ Maddox, O Lahav Monthly Notices of the Royal Astronomical Society 314 (3), 546-556, 2000 | 54 | 2000 |
| Effects of the size of cosmological N-body simulations on physical quantities – I. Mass function JS Bagla, J Prasad Monthly Notices of the Royal Astronomical Society 370 (2), 993-1002, 2006 | 52 | 2006 |
T. PadmanabhanDistinguished Professor, IUCAA在 iucaa.in 的电子邮件经过验证
