Pranav Charvu

ORCID: 0000-0003-2342-2866
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About
Contact & Profiles
Research Areas
  • Gamma-ray bursts and supernovae
  • Cosmology and Gravitation Theories
  • Space Science and Extraterrestrial Life
  • Galaxies: Formation, Evolution, Phenomena
  • Astrophysical Phenomena and Observations
  • Big Data Technologies and Applications
  • Stellar, planetary, and galactic studies
  • History and Developments in Astronomy
  • Italy: Economic History and Contemporary Issues

Duke University
2022

We present constraints on cosmological parameters from the Pantheon+ analysis of 1701 light curves 1550 distinct Type Ia supernovae (SNe Ia) ranging in redshift $z=0.001$ to 2.26. This work features an increased sample size, span, and improved treatment systematic uncertainties comparison original Pantheon results a factor two improvement constraining power. For Flat$\Lambda$CDM model, we find $\Omega_M=0.334\pm0.018$ SNe alone. Flat$w_0$CDM measure $w_0=-0.90\pm0.14$ alone, H$_0=73.5\pm1.1$...

10.3847/1538-4357/ac8e04 article EN cc-by The Astrophysical Journal 2022-10-01

Here we present 1701 light curves of 1550 spectroscopically confirmed Type Ia supernovae (SNe Ia) that will be used to infer cosmological parameters as part the Pantheon+ SN analysis and SH0ES (Supernovae H0 for Equation State dark energy) distance-ladder analysis. This effort is one a series works perform an extensive review redshifts, peculiar velocities, photometric calibration, intrinsic-scatter models SNe Ia. The total number curves, which are compiled across 18 different surveys,...

10.3847/1538-4357/ac8b7a article EN cc-by The Astrophysical Journal 2022-10-01

We present constraints on cosmological parameters from the Pantheon+ analysis of 1701 light curves 1550 distinct Type Ia supernovae (SNe Ia) ranging in redshift $z=0.001$ to 2.26. This work features an increased sample size, span, and improved treatment systematic uncertainties comparison original Pantheon results a factor two improvement constraining power. For Flat$Λ$CDM model, we find $Ω_M=0.334\pm0.018$ SNe alone. Flat$w_0$CDM measure $w_0=-0.90\pm0.14$ alone, H$_0=73.5\pm1.1$ km...

10.48550/arxiv.2202.04077 preprint EN cc-by arXiv (Cornell University) 2022-01-01

Here we present 1701 light curves of 1550 spectroscopically confirmed Type Ia supernovae (SNe Ia) that will be used to infer cosmological parameters as part the Pantheon+ SN analysis and SH0ES (Supernovae H0 for Equation State dark energy) distance-ladder analysis. This effort is one a series works perform an extensive review redshifts, peculiar velocities, photometric calibration, intrinsic-scatter models SNe Ia. The total number curves, which are compiled across 18 different surveys,...

10.48550/arxiv.2112.03863 preprint EN other-oa arXiv (Cornell University) 2021-01-01
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