The Canon Magazine 101
Our signal to noise test measures clarity,
specifically the ratio of the image ‘data’
you want capture, versus the image noise
you don’t want, but will be visible when
shooting at higher ISOs. The higher
the score the better
Canon’s sensor and processing tweaks
for the EOS Ra have noticeably improved
dynamic range. It manages to record
around 1 stop of extra dynamic over the
standard EOS R range right across the
ISO sensitivity range
RAW* SIGNAL-TO-NOISE RATIO
RAW* DYNAMIC RANGE
50
10
12
14
30
6
20
4
10
2
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200
200
ISO100
ISO100
400
400
800
800
1600
1600
3200
3200
6400
6400
1280025600
1280025600
40
8
30
30
28
0 51015 20 25
It’s no surprise that the 30Mp EOS Ra
manages to resolve excellent fine detail,
plus the EOS Ra scores are identical to
the regular EOS R in this test
RAW* RESOLUTION (AT ISO200)
EOS R
EOS R
EOS Ra
EOS R
EOS ra
EOS ra
picture height x100Line widths per^35
EOS Ra vs EOS R
*Ra
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variant, which is almost certainly
going to be used on a tripod or an
equatorial mount.
We have complained about the
heavy 4K video crop in the past,
but this will only affect
astrophotography if you need an
ultra-wide view of the sky. The 1.7x
crop means that your RF and EF
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Interestingly, Canon says you
can use the EOS Ra for regular
photography too, but warns that its
extended infra-red sensitivity can
lead to some colors looking strange
compared to what we see with the
naked eye.
Key features
Apart from its astrophotography
adaptations, the EOS Ra is
essentially the same as the EOS R.
It has a full-frame 30.3Mp CMOS
sensor and a phase-detection AF
system with 5655 focus positions
covering 88% of the frame
horizontally and 100% vertically.
The EOS Ra does not have
in-body image stabilisation (IBIS),
unlike rival full-frame mirrorless
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regular EOS R, but not for this
Shot on the EOS
Ra with RF 85mm
F1.2L USM lens at
f/1.8, 30 secs,
ISO1600
FULL TEST Canon EOS Ra
The AF system
is sensitive down to
an impressive -6EV,
more than enough for
very dark skies
The EOS Ra has impressive high ISO noise control and noise
only really becomes an issue at values of 3200 and higher
ISO3200
ISO25600