activity
19972025
most citedA new measure for cosmic shear

399 citations · 1.1k across the 12 of their papers we have counts for

collaborators

13 papers

astro-ph.CO2025★ 299 cited

The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics

Eleonora Di Valentino, Jackson Levi Said, Adam Riess +533

The standard model of cosmology has provided a good phenomenological description of a wide range of observations both at astrophysical and cosmological scales for several decades.…

astro-ph.IM2015

The Whole is Greater than the Sum of the Parts: Optimizing the Joint Science Return from LSST, Euclid and WFIRST

B. Jain, D. Spergel, R. Bean +26

The focus of this report is on the opportunities enabled by the combination of LSST, Euclid and WFIRST, the optical surveys that will be an essential part of the next decade's astr…

astro-ph.CO2010★ 26 cited

3D Reconstruction of the Density Field: An SVD Approach to Weak Lensing Tomography

Jake VanderPlas, Andrew Connolly, Bhuvnesh Jain +1

We present a new method for constructing three-dimensional mass maps from gravitational lensing shear data. We solve the lensing inversion problem using truncation of singular valu…

astro-ph.CO2009★ 1 cited

Exploring Dark Energy with Next-Generation Photometric Redshift Surveys

Hu Zhan, Andreas Albrecht, Asantha Cooray +15

The coming decade will be an exciting period for dark energy research, during which astronomers will address the question of what drives the accelerated cosmic expansion as first r…

astro-ph2003★ 15 cited

A weak lensing analysis of a STIS dark-lens candidate

T. Erben, J. M. Miralles, D. Clowe +6

We perform a weak lensing analysis on a previously reported dark-lens candidate on STIS Parallel data (Miralles et al. 2002). New VLT-data indicate that the reported signal origina…

astro-ph2002★ 197 cited

Weak Lensing Results from the 75 Square Degree CTIO Survey

M. Jarvis, G. Bernstein, B. Jain +4

We measure seeing-corrected ellipticities for 2 x 10^6 galaxies with magnitude R<23 in 12 widely separated fields totalling 75 deg^2 of sky. At angular scales >30\arcmin, elliptici…