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- Jan 28, 2020, 2:03:32 PM (6 years ago)
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trunk/doc/release.2015/ps1.calibration/calibration.tex
r41210 r41239 490 490 the isoplanetic patch size. We note that, in the typical conditions 491 491 at the \PSONE\ site, if the seeing is due to low-lying atmospheric 492 layers, the isoplanetic patch scale will be a most a few arcminutes492 layers, the isoplanetic patch scale will be at most a few arcminutes 493 493 \citep{1988ESOC...30..693B}, and smaller when the seeing comes from 494 494 higher altitudes.} … … 871 871 \cite{2012ApJ...756..158S}. This analysis is performed by the group 872 872 at Harvard, loading data from the raw detection files into their instance 873 of the Large SurveyDatabase \citep[LSD,][]{2011AAS...21743319J}, a873 of the Large \textmod{Survey} Database \citep[LSD,][]{2011AAS...21743319J}, a 874 874 system similar to DVO used to manage the detections and determine the 875 875 calibrations.
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