Characterization and correction of charge-induced pixel shifts in DECam
Characterization and correction of charge-induced pixel shifts in DECam
复制标题
DECam 中电荷引起的像素偏移的表征和校正
DOI:
--
复制
发表时间:
2015
期刊:
影响因子:
--
通讯作者:
Stella Seitz
中科院分区:
文献类型:
--
作者:
Daniel Gruen;Gary M. Bernstein;Mike Jarvis;Barnaby Rowe;V. Vikram;A. Plazas;Stella Seitz
Interaction of charges in CCDs with the already accumulated charge distribution causes both a flux dependence of the point-spread function (an increase of observed size with flux, also known as the brighter/fatter effect) and pixel-to-pixel correlations of the {Poissonian} noise in flat fields. We describe these effects in the Dark Energy Camera (DECam) with charge dependent shifts of effective pixel borders, i.e. the Antilogus et al. (2014) model, which we fit to measurements of flat-field {Poissonian} noise correlations. The latter fall off approximately as a power-law r−2.5 with pixel separation r, are isotropic except for an asymmetry in the direct neighbors along rows and columns, are stable in time, and are weakly dependent on wavelength. They show variations from chip to chip at the 20% level that correlate with the silicon resistivity. The charge shifts predicted by the model cause biased shape measurements, primarily due to their effect on bright stars, at levels exceeding weak lensing science requirements. We measure the flux dependence of star images and show that the effect can be mitigated by applying the reverse charge shifts at the pixel level during image processing. Differences in stellar size, however, remain significant due to residuals at larger distance from the centroid.
DOI:
10.1117/12.926216
发表时间:
2012
期刊:
--
影响因子:
--
作者:
Flaugher B
通讯作者:
Flaugher B
DOI:
10.1111/j.1365-2966.2006.10198.x
发表时间:
2006-05-21
影响因子:
4.8
作者:
Heymans, C;Van Waerbeke, L;Wittman, D
通讯作者:
Wittman, D