residual voltage it is possible to reconstruct photo-
signals that would otherwise exceed the pixel FWC
for a given integration whilst preserving linearity. Re-
cent implementations include a 16×16 pixel on 20 µm
pitch at 121 dB DR [7] and 96×128 pixel on 25 µm
pitch at 125 dB DR [8]. Fill factors are 13.1% and
10% respectively. A key advantage is the continu-
ous SNR increase with photosignal, however the low
fill factor, large pitch and small array sizes can be a
challenge for use in scientific imaging.
Multiple exposure is a commonly employed tech-
nique to increase DR without the need for additional
circuitry. Dual exposure involves acquiring two im-
ages at different integration times Tlong and Tshort
with the DR extension equal to Tlong/Tshort [9][10].
There exists an SNR dip in regions corresponding to
saturation in the short exposure, as the photosignal
here is only sampled for a fraction of the total inte-
gration time. The use of multiple shorter integrations
can lower the resulting SNR dip [11].
Non-destructive readout (NDR) operates by sam-
pling the signal many times during the integration
time without affecting the built up photocharge. The
CIS is read with up-the-ramp sampling, as widely
used on IR photodiode arrays for DR increase [12][13]
and for cosmic ray rejection [14].
Coded rolling shutter [15] works by spatially vary-
ing exposure per row, achieving a DR increase up
to the ratio of longest and shortest exposure times.
Image reconstruction is needed as vertical spatial in-
formation may be lost, however, due to the encoded
temporal information, high speed video and optical
flow can be extracted [16][17]. Interleaved multiple
gain readout has been used to achieve a DR of 120 dB
[18]. Work in this area is limited by commercial CIS
devices often being addressable row-wise only, pixel-
wise coded exposure could be achieved with full X-Y
addressability [16].
Pixel-wise control of integration times builds on
row-wise coded exposure by the addition of control
over an additional spatial dimension. Recent ad-
vances in 3D stacked CIS devices haven enabled a
pixel-parallel architecture, typically based on Cu-Cu
interconnects between the sensing and logic layers
[19]. A similar method is to control exposure for a
block of pixels, as shown in [20][21]. In [22] a 512×512
array with 4.6 µm pitch on a 3D-IC achieves 127 dB
DR by combining dual conversion gain with time-
to-saturation detection. Key advantages are the high
spatial fidelity achieved with a pixel-parallel readout,
however there is non-continuity in the SNR response
due to the three photosensing regimes.
In this paper a row-wise coded exposure scheme
is proposed which varies exposure locally depending
on the illumination, with multiple sub-exposures oc-
curring in said regions to exceed the SNR limit im-
posed by the FWC of the pixel. A hardware demon-
stration on a Teledyne e2v (Te2v) SIRIUS CIS115
[23] results in extended DR and peak signal-to-noise
ratio (PSNR). This is achieved thanks to the abil-
ity to randomly address and read out rows. A fu-
ture implementation of this technique is for actively
controlled spectroscopy [24], as both high signal cal-
ibration spectral lines and science spectral lines fall
on the focal plane [25][26]. Other applications may
include multi-ROI imaging at varying sub-exposures
and other areas, where high DR and SNR images are
of interest. The ability for CMOS image sensors to
operate in such way has been recognised by others
[27][28], but to our knowledge has not been imple-
mented in scientific imaging applications.
2 Dynamic range
A scene’s dynamic range is given by the upper and
lower limits of its luminance range. It is desirable for
a CIS to have a high dynamic range as this means it
can faithfully quantify both the high and low signal
regions in the scene. For a sensor with a linear full
well capacity of Qwell (e−), exposure time t(s), aver-
age dark current Idc (e−/s) and read noise variance
σ2
read (e2), the DR is the ratio of maximum (Imax)
and minimum (Imin) detectable photocurrents as in
equation 1. The maximum detectable signal is lim-
ited by Qwell minus the dark signal (which is sub-
tracted from a reference image taken in darkness),
whilst the noise floor (assuming correlated double
sampling and fixed pattern noise correction) is de-
termined by the read noise and dark current signal
noise.
2