On-sky measurements of the transverse electric fields' effects in the Dark Energy Camera CCDs
arXiv:1403.6127 · doi:10.1086/677682
Abstract
Photo-generated charge in thick, back-illuminated, fully-depleted CCDs is transported by electric fields from the silicon substrate to the collecting well at the front gate of the CCDs. However, electric fields transverse to the surface of the CCD -with diverse origins such as doping gradients, guard rings around the imaging area of the sensor, and physical stresses on the silicon lattice- displace this charge, effectively modifying the pixel area and producing noticeable signals in astrometric and photometric measurements. We use data from the science verification period of the Dark Energy Survey (DES) to characterize these effects in the Dark Energy Camera (DECam) CCDs. The transverse fields mainly manifest as concentric rings ("tree rings") and bright stripes near the boundaries of the detectors ("edge distortions") with relative amplitudes of about 1% and 10% in the flat-field images, respectively. Their nature as pixel size variations is confirmed by comparing their photometric and astrometric signatures. Using flat-field images from DECam, we derive templates in the five DES photometric bands (grizY) for the tree rings and the edge distortions as a function of their position in each DECam detector. These templates can be directly incorporated into the derivation of photometric and astrometric solutions, helping to meet the DES photometric and astrometric requirements.
Accepted for publication in the Publications of the Astronomical Society of the Pacific (PASP, issue August 2014)
References in corpus (3)
Cited by in corpus (19)
- Overview of the DESI Legacy Imaging Surveys
- The Dark Energy Camera
- Gravitational Lensing Analysis of the Kilo Degree Survey
- Pan-STARRS Photometric and Astrometric Calibration
- The DES Science Verification Weak Lensing Shear Catalogues
- Dark Energy Survey Year 3 Results: Weak Lensing Shape Catalogue
- The DECam Plane Survey: Optical photometry of two billion objects in the southern Galactic plane
- Dark Energy Survey Year 3 Results: Point-Spread Function Modeling
- The Third Data Release of the Beijing-Arizona Sky Survey
- Point spread function modelling for astronomical telescopes: a review focused on weak gravitational lensing studies
- Poisson_CCD: A dedicated simulator for modeling CCDs
- A framework for modeling the detailed optical response of thick, multiple segment, large format sensors for precision astronomy applications
- Sensor Distortion Effects in Photon Monte Carlo Simulations
- Precision Projector Laboratory: Detector Characterization with an Astronomical Emulation Testbed
- Intra-pixel response characterization of a HgCdTe near infrared detector with a pronounced crosshatch pattern
- Consequences of CCD imperfections for cosmology determined by weak lensing surveys: From laboratory measurements to cosmological parameter bias
- Dark Energy Survey Year 6 Results: Intra-Cluster Light from Redshift 0.2 to 0.5
- Dark Energy Survey Year 1 Results: Photometric Data Set for Cosmology
- The Multiband Imaging Survey for High-Alpha PlanetS (MISHAPS) I: Preliminary Constraints on the Occurrence Rate of Hot Jupiters in 47 Tucanae