Sky Variability in the y Band at the LSST Site
F. William High, Christopher W. Stubbs, Brian Stalder, David Kirk, Gilmore, John L. Tonry

TL;DR
This study measures spatial and temporal variability in the y band sky brightness at the LSST site, revealing atmospheric gravity wave effects and significant flux fluctuations that impact observational strategies.
Contribution
It provides the first detailed characterization of y band sky variability at the LSST site, highlighting atmospheric effects and implications for imaging strategies.
Findings
3%-4% rms spatial sky flux variability on 2-degree scales
Up to a factor of 2 temporal flux variability over a night
Coherent wave structures caused by atmospheric gravity waves
Abstract
We have measured spatial and temporal variability in the y band sky brightness over the course of four nights above Cerro Tololo near Cerro Pachon, Chile, the planned site for the Large Synoptic Survey Telescope (LSST). Our wide-angle camera lens provided a 41 deg field of view and a 145 arcsec pixel scale. We minimized potential system throughput differences by deploying a deep depletion CCD and a filter that matches the proposed LSST y_3 band (970 nm-1030 nm). Images of the sky exhibited coherent wave structure, attributable to atmospheric gravity waves at 90 km altitude, creating 3%-4% rms spatial sky flux variability on scales of about 2 degrees and larger. Over the course of a full night the y_3 band additionally showed highly coherent temporal variability of up to a factor of 2 in flux. We estimate the mean absolute sky level to be approximately y_3 = 17.8 mag (Vega), or y_3 =…
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