Lecture 4 Flashcards

1
Q

Active pixel sensors

A

is a detector in which individual pixels contain photosensitive material and an amplifier

each pixel can be read out individually

no moving charge about like in a CCD

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2
Q

CCD or CMOS - Electronic Noise

A

CMOS preferred with low electronic noise, dynamic range is also improved

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3
Q

CCD or CMOS - Quantum Efficiency

A

CCD preferred for low operation at low light levels, but CMOS catching up fast

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4
Q

CCD or CMOS - Readout rate

A

CMOS has a faster readout rate but it is usually unimportant

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5
Q

CCD or CMOS - Blooming

A

CMOS preferred but ‘anti-blooming’ techniques help in CCDs

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6
Q

CCD or CMOS - Flat Field

A

CCD is preferred can be made very uniform. Single substrate, single readout process

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7
Q

CCD or CMOS - Dark Current

A

CCD currently marginally better

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8
Q

CCD or CMOS - Spectral Coverage

A

CCD better outside the optical range. But CMOS can count individual high energy photons

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9
Q

CCD or CMOS - Flexibility

A

CCD readout needs circuits and CMOS readout needs software & computing power

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10
Q

CCD or CMOS - Power

A

Low power means CMOS preferred for space. But few space qualified CMOS detectors

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11
Q

Converting DN into physical units

A
  1. Convert DN to photo-electrons per pixel
  2. Convert photo-electrons per pixel to photons per pixel and CCD illumination
  3. Convert illumination to flux arriving at telescope
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12
Q

Converting DN to photo-electrons per pixel (formula)

A

N = n/g ± σ

N = DN read out

n = number of photo-electrons

g = gain

σ = readout noise

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13
Q

the photon-counting noise is given by (formula)

A

σn = √Ng

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14
Q

gain calibration (formula)

A

σ^2(N) = σ^2 + N/g

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15
Q

from photo-electrons to CCD illumination (formula)

A

nij = Nij g

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16
Q

The number of photons incident at that pixel is (formula)

A

nph = nij/Q

17
Q

the mean wavelength of the photons detected is (formula)

A

λmean = ∫ P(λ)s(λ)λdλ /
∫P(λ)s(λ)dλ

18
Q

the pixel illumination (formula)

A

J = nph h vmean/Apix Δt

19
Q

from CCD illumination to flux

A

J = F/θ^2 (D/f)^2

20
Q

so a pixel of dimension y subtends

A

θ = y/f