Astrophysics (Index)About

CCD

(charge-coupled device)
(type of electronic device to detect light)

A CCD (for charge-coupled device ) is a type of electronic device generally used to detect light, in such cases, incorporating an array of tiny electronic light sensors. It provides a mechanism for unloading the sensor-data, so as to capture an image focused on the sensors as digital data. Generally, such arrays are implemented as integrated circuits. The development and adoption of such electronic light-sensing arrays constituted a revolution in astronomy: they are used in telescopes (as well as many digital cameras) where they provide the data in electronic digital form, convenient for image storage and processing, and offering the possibility of automating the whole observation process. They have improved the efficiency of astronomical observation, vastly increasing the number of images captured and their use is advantageous for remote operation of telescopes, including space probes, and for fully-automated surveys.

The term CCD actually refers to the mechanism for unloading the data: it consists of a string of (basically) identical circuit elements that each sense and store a pixel, and are coupled together such that they that can pass their data to a neighbor in lock-step (shifting the data), so after a number of such steps, all the data has been output. The typical CCD circuit is a row of these strings in parallel, on a single chip, laid out in a grid. This technology and name ("CCD") were initially designed for data storage, but the technology to charge an electronic circuit element from incident EMR was already known and easily incorporated. Unloading a CCD's data takes some time, and faster means have been developed at the expense of more complex circuitry: such faster sensors are not termed CCDs (though undoubtedly people sometimes refer to one as a "CCD"), e.g., some fall under the term CMOS sensor. Such ability to unload data faster allows more time to collect data and more frequent unloading and resetting the device, which offers a number of benefits such as allowing a faster cadence to avoid saturation.


(instrument type,EMR)
Further reading:
https://en.wikipedia.org/wiki/Charge-coupled_device
https://en.wikipedia.org/wiki/Active-pixel_sensor
https://www.mssl.ucl.ac.uk/www_detector/ccdgroup/optheory/ccdoperation.html
https://mcdonaldobservatory.org/research/instruments/charged-coupled-devices
https://hamamatsu.magnet.fsu.edu/articles/ccdanatomy.html
http://spiff.rit.edu/classes/phys445/lectures/ccd1/ccd1.html
https://noirlab.edu/science/sites/default/files/media/archives/presentations/scipresentation0472-en.pdf

Referenced by pages:
ACIS
angular differential imaging (ADI)
aperture masking interferometry (AMI)
aperture photometry
back end instrument
cadence
Canada-France-Hawaii Telescope (CFHT)
Chandra X-ray Observatory (CXO)
color-color diagram (CCD)
commensal mode
cross dispersion spectrograph
DAOPHOT
data cube
Digitized Sky Survey (DSS)
drift scan
ESO Schmidt Telescope
Euclid
exposure time
fiber positioner
field curvature
flux
focal plane
focal plane array (FPA)
focal plane tilt
front end instrument
GaiaNIR
griz photometric system
HATNet
hot pixel
image stabilization
imaging Fourier transform spectroscopy (IFTS)
integration time
International Liquid Mirror Telescope (ILMT)
KELT
Kepler Telescope
KID
Lowell Discovery Telescope (LDT)
Magellan Telescopes
Mercator Telescope
microchannel array
NGTS
noise-equivalent power (NEP)
Palomar 48 Inch Telescope (P48)
Palomar high-redshift quasar surveys
parts per million (PPM)
passband
photocathode
photometer
photometry
photomultiplier tube (PMT)
photon counting
Pi of the Sky
plate
plate scale
point source sensitivity
prime focus
quantum efficiency (QE)
QUEST
real image
sensitivity function (S)
Shane Telescope
shift-and-add
signal-to-noise ratio (SNR)
sky subtraction
Sloan 2.5m Telescope
spaxel
spectrograph
spectrometer
spectropolarimetry
spectroscope
starshade
SUNRISE
Transiting Exoplanet Survey Satellite (TESS)
USNO CCD Astrograph Catalog (UCAC)
USNO Twin Astrograph
Víctor M. Blanco Telescope
WFC3
Zwicky Transient Facility (ZTF)

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