output
19952026
most citedObservational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

19.6k citations

Showing 2020 · astro-ph.IMShow all

7 papers · 2 filters

astro-ph.IM2020★ 25 cited

Measurement of turbulence profile from defocused ring images

Andrei Tokovinin

A defocused image of a bright single star in a small telescope contains rich information on the optical turbulence, i.e. the seeing. The concept of a novel turbulence monitor based…

astro-ph.IM2020★ 82 cited

Dark Energy Survey Year 3 Results: Point-Spread Function Modeling

M. Jarvis, G. M. Bernstein, A. Amon +79

We introduce a new software package for modeling the point-spread function (PSF) of astronomical images, called Piff (PSFs In the Full FOV), which we apply to the first three years…

astro-ph.IM2020★ 16 cited

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.IM2020★ 36 cited

Unsupervised machine learning for transient discovery in Deeper, Wider, Faster light curves

Sara Webb, Michelle Lochner, Daniel Muthukrishna +7

Identification of anomalous light curves within time-domain surveys is often challenging. In addition, with the growing number of wide-field surveys and the volume of data produced…

astro-ph.IM2020★ 78 cited

Mitigation of LEO Satellite Brightness and Trail Effects on the Rubin Observatory LSST

J. Anthony Tyson, Željko Ivezić, Andrew Bradshaw +8

We report studies on the mitigation of optical effects of bright low-Earth-orbit (LEO) satellites on Vera C. Rubin Observatory and its Legacy Survey of Space and Time (LSST). These…

astro-ph.IM2020★ 12 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…