activity
20152026
most citedKiDS-450 + 2dFLenS: Cosmological parameter constraints from weak gravitational lensing tomography and overlapping redshift-space galaxy clustering

296 citations · 1.6k across the 28 of their papers we have counts for

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12 papers · 1 filter

astro-ph.IM20235 cited

The Dark Energy Survey Six-Year Calibration Star Catalog

E. S. Rykoff, D. L. Tucker, D. L. Burke +64

This Technical Note presents a catalog of calibrated reference stars that was generated by the Forward Calibration Method (FGCM) pipeline (arXiv:1706.01542) as part of the FGCM pho…

astro-ph.IM2023

Simulating image coaddition with the Nancy Grace Roman Space Telescope: II. Analysis of the simulated images and implications for weak lensing

Masaya Yamamoto, Katherine Laliotis, Emily Macbeth +16

One challenge for applying current weak lensing analysis tools to the Nancy Grace Roman Space Telescope is that individual images will be undersampled. Our companion paper presente…

astro-ph.IM2023

Simulating image coaddition with the Nancy Grace Roman Space Telescope: I. Simulation methodology and general results

Christopher M. Hirata, Masaya Yamamoto, Katherine Laliotis +16

The upcoming Nancy Grace Roman Space Telescope will carry out a wide-area survey in the near infrared. A key science objective is the measurement of cosmic structure via weak gravi…

astro-ph.IM2021

The Dark Energy Survey Data Release 2

DES Collaboration, T. M. C. Abbott, M. Adamow +132

We present the second public data release of the Dark Energy Survey, DES DR2, based on optical/near-infrared imaging by the Dark Energy Camera mounted on the 4-m Blanco telescope a…

astro-ph.IM2020

Reducing ground-based astrometric errors with Gaia and Gaussian processes

W. F. Fortino, G. M. Bernstein, P. H. Bernardinelli +64

Stochastic field distortions caused by atmospheric turbulence are a fundamental limitation to the astrometric accuracy of ground-based imaging. This distortion field is measurable…

astro-ph.IM202012 cited

Noise from Undetected Sources in Dark Energy Survey Images

K. Eckert, G. M. Bernstein, A. Amara +66

For ground-based optical imaging with current CCD technology, the Poisson fluctuations in source and sky background photon arrivals dominate the noise budget and are readily estima…