Lecture 2 Flashcards
CCDs and CMOS detectors work
via the photoelectric effect in a semiconductor
Semiconductors
In an isolated atom, the atomic energy levels are well spaced out
in solids, atomic levels form blended bands. the low energy bands are filled by electrons up to the fermi level.
in a semiconductor the last filled level is the ‘valence’ band
the valance and higher energy conduction bands are separated in energy by the band gap
electrons must be able to move between energy levels. so full bands cannot participate
electronic conduction arises when an electron moves from the valence band into a higher energy state.
How can a valence electron gain energy and jump the band gap?
Thermally
or from the photoelectric effect
to improve a semiconductors conduction, and help store the charges from the photo-electrons, we use
doped semiconductors
- adding a small amount of a different atom to our semiconductor
p-type
fewer valence electrons so extra hole
n-type
more valence electrons so extra e-
Silicon (MOS) transistor
a thin insulator layer of SiO2 is placed onto the p-type Si and on top of this metal electrode
the positive holes are driven away from the small positive bias voltage near the electrode = depletion region
electrons migrate to near electrode
depletion region
is the region where the positive holes are driven away from the small positive bias voltage near the electrode
full well capacity
maximum number of electrons that can be held before pixel saturates
CCD readout
CCDs are readout by applying sequences of voltages along the columns and down the rows of the CCD, transferring charge from one pixel to the next.
For speed all the columns are shifted at the same time.
Analogue to digital converter:
converts voltage to data numbers (DN)
3 phase read out scheme
each pixel has 3 electrodes connected in parallel at voltages Φ1, Φ2, Φ3
voltage is varied, allowing charge to migrate but also be kept separate
contributions to CCD data numbers (formula)
Xij = Pij + Tij + Eij + Cij
Pij =
contributions from pixel charge due to photons from the astronomical source
Tij =
contribution from pixel charge due to thermal effects (dark current)