| Cosmology intertwined: A review of the particle physics, astrophysics, and cosmology associated with the cosmological tensions and anomalies E Abdalla, GF Abellán, A Aboubrahim, A Agnello, Ö Akarsu, Y Akrami, ... Journal of High Energy Astrophysics 34, 49-211, 2022 | 257 | 2022 |
| Exploring cosmic origins with CORE: Inflation F Finelli, M Bucher, A Achúcarro, M Ballardini, N Bartolo, D Baumann, ... Journal of Cosmology and Astroparticle Physics 2018 (04), 016, 2018 | 165 | 2018 |
| Exploring cosmic origins with CORE: Cosmological parameters E Di Valentino, T Brinckmann, M Gerbino, V Poulin, FR Bouchet, ... Journal of Cosmology and Astroparticle Physics 2018 (04), 017, 2018 | 143 | 2018 |
| Generating PBHs and small-scale GWs in two-field models of inflation M Braglia, DK Hazra, F Finelli, GF Smoot, L Sriramkumar, AA Starobinsky Journal of Cosmology and Astroparticle Physics 2020 (08), 001, 2020 | 139 | 2020 |
| Primordial features due to a step in the inflaton potential DK Hazra, M Aich, RK Jain, L Sriramkumar, T Souradeep Journal of Cosmology and Astroparticle Physics 2010 (10), 008, 2010 | 121 | 2010 |
| BINGO: A code for the efficient computation of the scalar bi-spectrum DK Hazra, L Sriramkumar, J Martin Journal of Cosmology and Astroparticle Physics 2013 (05), 026, 2013 | 105 | 2013 |
| Wiggly whipped inflation DK Hazra, A Shafieloo, GF Smoot, AA Starobinsky Journal of Cosmology and Astroparticle Physics 2014 (08), 048, 2014 | 94 | 2014 |
| Sharp inflaton potentials and bi-spectra: Effects of smoothening the discontinuity J Martin, L Sriramkumar, DK Hazra Journal of Cosmology and Astroparticle Physics 2014 (09), 039, 2014 | 87 | 2014 |
| Primordial power spectrum from Planck DK Hazra, A Shafieloo, T Souradeep Journal of Cosmology and Astroparticle Physics 2014 (11), 011, 2014 | 83 | 2014 |
| Probing primordial features with the stochastic gravitational wave background M Braglia, X Chen, DK Hazra Journal of Cosmology and Astroparticle Physics 2021 (03), 005, 2021 | 74 | 2021 |
| Oscillations in the inflaton potential: Complete numerical treatment and comparison with the recent and forthcoming CMB datasets M Aich, DK Hazra, L Sriramkumar, T Souradeep Physical Review D 87 (8), 083526, 2013 | 70 | 2013 |
| Inflation with whip-shaped suppressed scalar power spectra DK Hazra, A Shafieloo, GF Smoot, AA Starobinsky Physical Review Letters 113 (7), 071301, 2014 | 64 | 2014 |
| Primordial features and Planck polarization DK Hazra, A Shafieloo, GF Smoot, AA Starobinsky Journal of Cosmology and Astroparticle Physics 2016 (09), 009, 2016 | 60* | 2016 |
| Reconstruction of broad features in the primordial spectrum and inflaton potential from Planck DK Hazra, A Shafieloo, GF Smoot Journal of Cosmology and Astroparticle Physics 2013 (12), 035, 2013 | 49 | 2013 |
| Primordial power spectrum: a complete analysis with the WMAP nine-year data DK Hazra, A Shafieloo, T Souradeep Journal of Cosmology and Astroparticle Physics 2013 (07), 031, 2013 | 45 | 2013 |
| On the scalar consistency relation away from slow roll V Sreenath, DK Hazra, L Sriramkumar Journal of Cosmology and Astroparticle Physics 2015 (02), 029, 2015 | 44 | 2015 |
| Ruling out the power-law form of the scalar primordial spectrum DK Hazra, A Shafieloo, GF Smoot, AA Starobinsky Journal of Cosmology and Astroparticle Physics 2014 (06), 061, 2014 | 43 | 2014 |
| Metastable dark energy with radioactive-like decay A Shafieloo, DK Hazra, V Sahni, AA Starobinsky Monthly Notices of the Royal Astronomical Society 473 (2), 2760-2770, 2018 | 39 | 2018 |
| Cosmological parameter estimation with free-form primordial power spectrum DK Hazra, A Shafieloo, T Souradeep Physical Review D 87 (12), 123528, 2013 | 34 | 2013 |
| Probing features in inflaton potential and reionization history with future CMB space observations DK Hazra, D Paoletti, M Ballardini, F Finelli, A Shafieloo, GF Smoot, ... Journal of Cosmology and Astroparticle Physics 2018 (02), 017, 2018 | 30 | 2018 |
Arman ShafielooPrincipal Researcher, Korea Astronomy and Space Science Institute (KASI)Verified email at kasi.re.kr
