5 citations · 10 across the 3 of their papers we have counts for
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Mitigation of the Brighter-Fatter Effect in the LSST Camera
Alex Broughton, Yousuke Utsumi, Andrés Plazas Malagón +8
Thick, fully depleted charge-coupled devices (CCDs) are known to exhibit non-linear behavior at high signal levels due to the dynamic behavior of charges collecting in the potentia…
The Brighter-Fatter Effect in the JWST MIRI Si:As IBC detectors I. Observations, impact on science, and modelling
Ioannis Argyriou, Craig Lage, George H. Rieke +10
The Mid-Infrared Instrument (MIRI) on board the James Webb Space Telescope (JWST) uses three Si:As impurity band conduction (IBC) detector arrays. The output voltage level of each…
Laboratory Measurements of Instrumental Signatures of the LSST Camera Focal Plane
Adam Snyder, Aurelien Barrau, Andrew Bradshaw +19
Electro-optical testing and characterization of the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) Camera focal plane, consisting of 205 charge-coupled devices (C…
Physical and electrical analysis of LSST sensors
Craig Lage
Removing systematic effects from astronomical images taken with CCDs requires a detailed understanding of the physics of the imaging process. To aid in this understanding, we have…
Linearity and correction of the BF effect in LSST sensors
Craig Lage
The Brighter-Fatter (hereafter BF) effect in CCD sensors causes increases in the image size of bright objects due to electrostatic repulsion of collected charges. Correcting this e…
Characterization of LSST CCDs Using Realistic Images, Before First Light
Andrew K. Bradshaw, Craig Lage, J. Anthony Tyson
The 3.2 gigapixel LSST camera, an array of 189 thick fully-depleted CCDs, will repeatedly image the southern sky and accomplish a wide variety of science goals. However, its trove…