Abstract
Atomic resolution in c ryo-electron microscopy was first demonstrated six years ago. This was
accomplished using 300 kV electron microscopes equipped with new hardware that provided
narrower energy spread , aberration correction, and energy filtering. Here, we report the
achievement of 1.24 Å atomic resolution on an upgraded 200 kV electron microscope featuring a
cold field emission gun, a high-resolution objective lens polepiece, and an energy filter. These
components transform the instrument into a cost-effective single particle cryo-EM platform with
performance comparable to that of significantly more expensive 300 kV systems. The microscope
can also be operated at 100 kV and by using a high-speed hybrid-pixel detector we were able to
reach sub-2 Å resolution.
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1. Introduction
The cryo-EM “resolution revolution” has been ongoing for more than a decade. It reached a major
milestone in 2020 with the demonstration of atomic resolution by two independent teams
(Nakane et al., 2020; Yip et al., 2020). According to the current consensus in X-ray crystallography,
“atomic resolution” is defined as 1.2 Å or better (Dauter, 2003) , based on a criterion of non -
overlapping atomic densities proposed by Sheldrick (Sheldrick, 1990).
The first atomic resolution cryo-EM results were obtained using well-behaved, highly symmetric
heavy-chain apoferritin, which has served as the gold standard test specimen for cryo-EM single-
particle performance since its introduction by Russo and Passmore (Russo & Passmore, 2014)
and its subsequent improvement to a heavy -chain variant (Danev et al., 2019). The two atomic
resolution teams used upgraded 300 kV microscopes : one featured a cold field -emission gun
(CFEG) and a newly developed energy filter (Nakane et al., 2020), and the other a monochromator
and a spherical aberration corrector (Yip et al., 2020). Since these reports, other groups have also
presented atomic resolution results on 300 kV instruments, almost all equipped with CFEG
sources (Fujita et al., 2023; Zhang et al., 2020; Maki-Yonekura et al., 2023; Küçükoğlu et al., 2024).
In 2020, we tested the newly installed Titan Krios G4 (Thermo Fisher Scientific, Waltham, USA)
300 kV electron microscope at the University of Tokyo equipped with a Schottky FEG (SFEG) and
the dataset reached 1.31 Å (Danev et al., 2021). At present, 300 kV microscopes offer the best
cryo-EM performance for both single-particle analysis and cryo -tomography. However, they are
expensive to purchase, costly to maintain, heavy in electricity consumption, and require a large
installation space.
The cryo-EM capabilities of 200 kV microscopes have been extensively evaluated over the years
with remarkable results (Herzik et al., 2017; Wu et al., 2020; Merk et al., 2020; Hamdi et al., 2020;
Kayama et al., 2021; Feathers et al., 2021; Gerle et al., 2022; Thangaratnarajah et al., 2022; Koh
et al. , 2022; Jia et al. , 2024) . Surprisingly, despite the ir excellent performance, only ~10 % of
deposited maps with resolution s better than 6 Å in the E lectron Microscopy Data bank (EMDB)
come from 200 kV microscopes. Currently, 200 kV machines are widely used as a cost-effective
alternative to 300 kV instruments at universities, research institutions, and industrial facilities for
sample screening and data collection, with the understanding that the achievable resolution may
not be as high but is often sufficient to answer most research questions.
In the past few years, 100 kV microscopes were shown to hold substantial promise as “people’s
cryo-microscopes” , offering sufficient performance for sample screening and exploratory data
collection at an affordable cost and with minimal installation requirements (Naydenova et al.,
2019; McMullan et al., 2023; Chan et al., 2024; Venugopal et al., 2025; Karia et al., 2025). However,
achieving high resolution results on current commercially available 100 kV instruments remains
challenging, as evidenced by the fact that there are fewer than fifty maps at resolutions better
than 6 Å in the EMDB, the majority of which are test samples.
Here, we evaluated the performance of an upgraded 200 kV microscope equipped with a CFEG,
a narrow gap objective lens polepiece, and an omega-type energy filter. We collected apoferritin
test datasets at accelerating voltages of 200 and 100 kV using a latest generation direct detection
camera and a high-speed hybrid-pixel detector respectively. The results are presented below.
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2. Materials and methods
2.1 Microscope configuration
The experiments were performed on a CRYO ARM 200 II (JEM-Z200CA, JEOL Ltd., Tokyo, Japan)
electron cryo-microscope upgraded with a narrow-gap high-resolution objective lens polepiece.
This reduced the spherical and chromatic aberration coefficients from the regular CS = 2.7 mm
and CC = 2.8 mm to CS = 1.5 mm and CC = 1.8 mm. The microscope is equipped as standard with
a CFEG , a three -lens condenser system, and an omega -type energy filter. The system also
featured a Gatan K3 (Gatan, Pleasanton, USA) direct electron detector and an electrostatic dose
modulator (EDM), which was used as a fast electrostatic shutter. For the 100 kV experiments, the
camera was replaced with a DECTRIS SINGLA (DECTRIS Ltd., Baden-Daettwil, Switzerland) high-
speed hybrid-pixel detector.
2.2 Sample preparation
Mouse heavy chain apoferritin was expressed and purified as described previously (Danev et al.,
2021). Cryo-EM samples were prepared by applying 3 μl of 1.9 mg/ml sample solution on
UltrAuFoil R 0.6/1 300 mesh (200 kV experiment s) or UltrAuFoil R1.2 /1.3 300 mesh (100 kV
experiments) grids (Russo & Passmore, 2016) (Quantifoil Micro Tools GmbH, Jena, Germany) and
plunge-freezing in liquid ethane on a Vitrobot Mark IV (Thermo Fisher Scientific, Waltham, USA),
blot time 20 s (R0.6/1.0 grids) or 10 s (R1.2/1.3 grids), chamber temperature 4 oC, 100 % humidity.
2.3 Data collection
The datasets were collected automatically by SerialEM software (Schorb et al., 2019) using its
built-in single-particle automation routines. The main acquisition parameters are summarized in
Supplementary Table S1.
For the 200 kV dataset, t he microscope was set up at an indicated magnification of 150,000 x,
calibrated pixel size 0.3056 Å pix el
-1, spot size 3, convergence angle 3, condenser aperture 100
μm, beam diameter ~ 0.95 μm, no objective aperture, zero -loss energy filtering with 20 eV slit,
target defocus -0.5 μm. The detector was operated in counting (non-super-resolution) correlated
double sampling (CDS) mode, with an exposure time of 1.51 s, an exposure rate of 3.3 e pixel-1 s-
1, a total exposure of 53.4 e Å-2, a frame time of 0.0185 s, 81 frames, and an exposure per frame of
0.66 e Å-2. In total, 13,654 movies were collected in 56 hours with an average through put of 244
movies per hour using a beam -tilt compensated 3x3 x1 image shift acquisition pattern with a
single image in the center of each hole.
For the 100 kV dataset, t he microscope was set up at an indicated magnification of 5 00,000x,
calibrated pixel size 1.17 Å pixel-1, spot size 6, convergence angle 3, condenser aperture 70 μm,
beam diameter ~ 0.53 μm, objective aperture 250 μm, zero-loss energy filtering with 20 eV slit,
and target defocus -0.45 μm to -0.55 μm. The movies were recorded in HDF5 format at the raw
framerate of the detector of 4,500 frames s-1, with an exposure time of 3.0 s, an exposure rate of
23.8 e pixel-1 s -1, a total exposure of 5 2.2 e Å -2, 13,500 total frames, an exposure per frame of
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0.0039 e Å-2. In total, 17,424 movies were collected in 49.5 hours with an average throughput of
352 movies per hour using a beam -tilt compensated 3x3x4 image shift acquisition pattern with
four images in each hole.
2.4 Data processing
The data were processed with CryoSPARC (Punjani et al. , 2017) (Structura Biotechnology,
Toronto, Canada).
The 200 kV dataset processing workflow is summarized in Supplementary Fig. S1. Briefly, 13,654
movies were subjected to patch motion correction and patch CTF estimation followed by
exposure curation with CTF fit resolution selection range between 2 and 4 Å , retaining 10,189
micrographs. The micrographs were split into nine exposure groups based on their image shift.
Particles were picked with 20 Å low -pass filtered templates generated from a previous 3D
apoferritin map, resulting in 927k picks after selecti on with NCC score > 0.4 and local power
between 600 and 900. E xtraction with a 160 pixel box at 1.57 Å pix el-1 produced 652k particles
that were subjected to 2D classification with 100 classes . Manual 2D class selection left 635k
particles that were run through ab-initio 3D reconstruction with two classes . The 3D reference
and 622k particles from the larger class were used for further processing. Initial 3D homo
refinement hit Nyquist at 3.23 Å . The particles were re -extracted with 400 pix el box at 0.627 Å
pixel-1 and another 3D homo refinement reached 1.56 Å. The particles were then split into hour-
wise exposure groups for a total of 504 exposure groups, followed by a 3D homo refinement which
reached 1.35 Å. A round of reference -based motion correction and 3D homo refinement
improved the map to 1.26 Å. A 3D heterogeneous refinement with three classes reduced the
particle stack to 615k, followed by another round of reference-based motion correction and 3D
homo refinement to produce the final map at 1.24 Å.
The 100 kV dataset processing workflow is summarized in Supplementary Fig . S2. Briefly, the
17,654 HDF5 hardware frame stacks were subjected to 2x super -resolution electron counting
(Zambon, 2023) with a GPU -accelerated software tool provided by DECTRIS ( DECTRIS Ltd.,
Baden-Daettwil, Switzerland) and were fractionated with 225 hardware frames per fraction into
60 frame MRC movies. The mov ies were renamed with a Python script according to image shift
group specifications in summed MRC images that were saved separately by SerialEM during
acquisition. The renamed super-resolution MRC movies were imported into CryoSPARC and were
subjected to patch motion correction with 3/4 Fourier crop and patch CTF estimation followed by
exposure curation with CTF fit resolution selection range between 2 .5 and 5 Å, retaining 9, 123
micrographs. Particles were picked with 20 Å low -pass filtered templates generated from a
previous 3D apoferritin map, resulting in 477k picks after selection with NCC score > 0.4 and local
power between 8*106 and 13*106. Extraction with a 15 0 pixel box at 1.4 Å pixel-1 produced 350k
particles that were subjected to 2D classification with 200 classes. Manual 2D class selection
left 322k particles that were run through ab -initio 3D reconstruction with t hree classes. The 3D
Reference
and 321k particles from the large st class were used for further processing. Initial 3D
homo refinement reached 2.9 Å. The particles were re- extracted with a 250 pixel box at 0.936 Å
pixel-1 and split into 36 exposure groups according to image shift. A nother 3D homo refinement
reached 2.01 Å. A reference -based motion correction was attempted but did not improve the
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resolution while exhibiting unexpectedly smooth particle tracks and an anomalous overweighting
of high-resolution spectral components in later movie frames. To circumvent that, patch motion
correction of the movies was performed again by using only the first 30 frames. Particles were re-
extracted from the limited-frame micrographs and a 3D homo refinement reached 2.0 Å. A round
of reference-based motion correction and 3D homo refinement improved the map resolution to
1.93 Å. Splitting the particles into hour -wise exposure groups and further exposure curation
reduced the particle stack to 250k pa rticles and improved the 3D homogeneous refinement
resolution to 1.91 Å.
To generate the Rosenthal-Henderson plot (Rosenthal & Henderson, 2003) for the 200 kV dataset,
random particle subsets from the final particle stack were 3D homo refined independently and
the results were plotted in a reciprocal squared resolution versus logarithm of the number of
particles. The B -factor was calculated as 2 *(slope of linear fit) -1 from the linear regression fits
through the data points in these coordinates.
Evaluation of the effect of radiation damage by pre-exposure on the achievable resolution was
performed by using the first 1,000 movies containing 58k particles from the 200 kV dataset,
running motion correction jobs with omission of a varying number of initial movie frames
(Supplementary Table S2), extracting the particles from the aligned micrographs, and performing
a 3D homogeneous refinement with defocus, nine image- shift exposure group beam tilt, and
Ewald sphere correction. Reference -based motion correction and higher -order aberration
refinements were not used during this processing.
2.5 Numerical estimation of the effect of pre-exposure on resolution
To quantify the resolution decrease as a function of pre-exposure, we must estimate the spectral
signal-to-noise ratio (SNR) and dampen it with a resolution-dependent radiation damage model.
It is not necessary to know the absolute but rather the relative spectral SNR, which can be
calculated from the B -factor fit of the Rosenthal -Henderson plot. Assuming that particles
represent independent measurements, the SNR is inversely proportional to the square root of the
number of particles necessary to reach a given resolution. Therefore, having a 3D refinement
without pre-exposure, the relative SNR of lower resolution shells can be calculated as the square
root of the particle number ratio. Then, by applying a resolution- dependent radiation damage
model, the exposure needed to attenuate the relative SNR of a given resolution shell to 1 can be
estimated. This will correspond to the exposure that will limit the 3D reconstruction to the
resolution of that shell.
Using this approach and the empirical radiation damage model by Grant and Grigorieff (Grant &
Grigorieff, 2015) adjusted for 200 kV by reducing the critical exposure by 25% (as suggested in the
paper), we estimated the resolution vs pre -exposure. The calculations were performed in
Wolfram Mathematica (Wolfram Research, Champaign, USA).
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2.6 Model refinement and visualization
The initial model (PDB-7A4M) was rigid-body fitted in Coot (Casañal et al., 2020), followed by
reciprocal-space refinement using Servalcat (Yamashita et al., 2021) against unsharpened half
maps. The model was interactively adjusted in Coot using the sharpened map and Fo − Fc
difference map, which included the positioning of polar hydrogen atoms. Finally, a hydrogen
omit Fo − Fc difference map was calculated using Servalcat. The models were validated using
MolProbity (Chen et al., 2010).
3D images of the maps and model for the figures were created using UCSF Chimera (Pettersen
et al., 2004) and UCSF Chimera X (Meng et al., 2023).
3. Results
Fig. 1 shows normalized histograms of the resolution of Electron Microscopy Data Bank (EMDB)
depositions from 300 kV and 200 kV microscopes in the last six years. The ratio of 200 kV to 300
kV depositions is approximately 1:9 (3,058 vs 27,825). Log-normal fits of the histograms indicate
a 0.25 Å higher median resolution at 300 kV . The rather moderate resolution advantage on its own
cannot explain the big disparity in the number of depositions. Nevertheless, a closer look at the
histograms shows that 300 kV is ~1.7 times more prolific in the 2.5 –3.0 Å range, and ~3.3 times
more prolific in the 2.0 –2.5 Å r ange. These resolution ranges , and especially the latter, are of
increasing importance in cryo-EM studies because they enable more accurate modeling of
sidechains, identification and pose assignment of small molecules, and high- confidence
detection of water molecules.
Fig. 2 contains a plot of the theoretical temporal coherence contrast transfer function (CTF)
envelope (eq. 6.42 in (Reimer & Kohl, 2010)) for a number of cryo-microscope configurations. The
top-of-the-line CRYO ARM 300 II (JEOL Ltd., Tokyo, Japan) and Krios 5 (Thermo Fisher Scientific,
Waltham, USA) (green solid line) 300 kV machines have demonstrated atomic resolution in the
past (Nakane et al. , 2020; Yip et al. , 2020; Maki -Yonekura et al. , 2023) and are currently the
highest optical performance commercially available cryo -microscopes. The CRYO ARM 200 II
(pink solid line) used in this study is a close second and is currently the top performing 200 kV
instrument. Other CFEG 200 kV microscopes, such as the CRYO ARM 200 (JEOL Ltd., Tokyo,
Japan) and Glacios 2 (Thermo Fisher Scientific, Waltham, USA) ( blue solid line), follow next.
Remarkably, the recently presented “Dublin lens” design for 100 keV (Alves et al., 2025) (gray solid
line) with a very low chromatic aberration coefficient of CC = 1.0 mm, if coupled with a CFEG will
perform on par with the CRO ARM 200 and Glacios 2. S FEG-equipped instruments, such as the
Krios, Glacios (Thermo Fisher Scientific, Waltham, USA), the “Dublin lens” , and Tundra (Thermo
Fisher Scientific, Waltham, USA) come next in terms of theoretical optical quality.
To experimentally test the overall optical performance of the CRYO ARM 200 II, we collected high-
magnification (200,000x) images of oriented single crystal (100) gold test specimen (AGS135,
Agar Scientific, Rotherham, UK). The Fourier transform of one of the best images is shown in Fig.
3. It contains spots up to lattice plane (046) with spacing 0.566 Å along the sample stage tilt axis
and up to lattice plane (044) with spacing 0.721 Å perpendicular to the tilt axis. This confirms the
excellent optical performance of the microscope going beyond 1 Å in all directions. It also
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indicates that it may have been slightly affected by mechanical disturbances. The instrument is
installed in a room that is on the ground floor of a building but was not specially designed for high-
resolution electron microscopy with considerations and measures to minimize floor vibrations.
The data acquisition scheme and exemplary micrograph from the 200 kV apoferritin dataset are
presented in Fig s. 4 a, b . To minimize beam- induced sample motion w e prepared the 200 kV
sample on 0.6 μm holes gold foil grid and collected a single image in the center of each hole with
the beam illuminating uniformly the hole edge all -around (Fig. 4a). To maximize the camera’s
detective quantum efficiency (DQE) performance over the target resolution range, the 200 kV data
was collected at a relatively high indicated magnification of 150,000x with a pixel size of 0.3056 Å
pix-1 (Fig. 4b, Supplementary Table S1). The resolution of the final 3D map corresponds to ~49%
of the physical Nyquist limit of the camera.
The 100 kV dataset was also collected on a gold foil grid but to maximize data acquisition
throughput we used a grid with 1.2 μm holes and acquired four images per hole (Fig. 4c). In
previous experiments using such acquisition strategy on this and other microscopes, we have
reached resolutions far below 2 Å (Danev et al. , 2021) and therefore do not expect it to be a
limiting factor in this test. Due to the much larger physical pixel of the D ECTRIS SINGLA camera
(75 μ m vs 5 μ m of the Gatan K3) we had to collect at even higher magnification of 500,000x
(Supplementary Table S1 ). This presented some practical challenges in terms of microscope
alignment and operation in the ultra-high magnification range, which is not typically used in cryo-
EM. Fig. 4d contains an exemplary image from the 100 kV dataset illustrating the gap (horizontal
stripe in the middle of the image) between the two modules of the detector which is interpolated
in software to facilitate cryo-EM data processing.
The results from the processing of the 200 kV dataset are presented in Fig.5. The reconstruction
(Fig. 5a) reached 1.24 Å according to the 0.143 gold -standard Fourier Shell Correlation (FSC)
criterion (Fig. 5b). The 3D map shows features consistent with the estimated resolution, such as
atomic bulges at a lower surface threshold and individual blobs for non-hydrogen atoms at a
higher threshold (Fig.5c, gray and blue surfaces ). Furthermore, an F
o–Fc difference density map
calculated in Servalcat (Yamashita et al., 2021) revealed hydrogen atom densities at many of their
expected positions (Fig. 5c, green surfaces).
We quantified the overall experimental performance using a Rosenthal-Henderson B-factor plot
(Rosenthal & Henderson, 2003). Fig. 6 contains B-factor plots for the 200 kV dataset (red symbols
and line) and the Krios G4 (set 1 in (Danev et al., 2021)) apoferritin dataset (blue symbols and line).
The measured B-factors were 39.0 Å2 for the CRYO ARM 200 II and 38.7 Å 2 for the K rios G4. In
practical terms, they are virtually identical. The CRYO ARM 200 II plot was offset vertically towards
slightly higher resolution which indicates a slightly higher overall signal-to-noise ratio of the data.
During data processing, we observed a 0.2 Å improvement in resolution (from 1.56 Å to 1.35 Å)
after splitting the data into hour -wise exposure groups (Supplementary Fig. S 1), indicating that
there was a variation over time of the optical parameters. Supplementary Fig. S3 shows a
temporal trend plot of the refined beam tilt for the nine image -shift exposure groups. The beam
tilt steadily increased by ~0.65 mrad over the course of the experiment. It is not clear what caused
this change. There were no signific ant variations in the room and cooling water temperatures.
One possible explanation is a gradual drift of the optics because the lens degaussing routines
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were disabled to reduce time overhead. The plot also shows that SerialEM’s image shift beam tilt-
compensation performed well by keeping the spread between the nine acquisition areas within
0.1 mrad.
We were curious about the effect of radiation damage on the achievable resolution. To quantify
it, we used the first 1,000 movies and performed independent reconstructions starting from
motion correction by omitting a varying number of initial frames to simulate pre-exposure. The
same set of particle coordinates w as used to extract particles from the aligned micrographs,
followed by a 3D homogeneous refinement job. The results are presented in Fig. 7. Surprisingly,
the reconstruction reached ~2.9 Å resolution even after 20 e Å -2 of pre-exposure. The resolution
dependence on pre- exposure was fitted very well (R2 = 0.997) by a parabola (Fig. 7a, red line ).
Numerical estimation of the resolution vs pre-exposure based on applying an empirical radiation
damage model (Grant & Grigorieff, 2015) produced results that underestimated (larger value) the
achievable resolution (Fig. 7a, black symbols). Using a total exposure value that was 82 % of the
experimentally measured one in the numerical calculation produced results that were much
closer to the experimental ones (Fig. 7a, blue symbols). The difference in the exposure parameter
could be due to various reasons, such as empirical damage model accuracy for this particular
sample and support film, variation of the actual exposure during the experime nt due to CFEG
current decline, or other factors. Fig. 7b contains panels illustrating the decline of 3D map fidelity
with increasing pre-exposure.
The reconstruction of the 100 kV dataset reached a resolution of 1.91 Å (Fig. 8). This corresponds
to 123% of the physical Nyquist frequency of the detector. Map features, such as holes in
aromatic sidechains, confirm the estimated resolution (Fig. 8a). Overall, this is an outstanding
performance at 100 kV that closely matches what was achieved recently at 120 kV on a non-
standard Glacios microscope with a narrow-gap “SP-Twin” objective lens polepiece (C
C = 1.7 mm)
and an Alpine (Gatan, Pleasanton, USA) camera (Chan et al., 2024). This configuration at 120 kV
is expected to perform halfway between the Tundra microscope and the “Dublin lens” (SFEG) in
Fig. 2. Having a CFEG and a narrow-gap polepiece, at 100 kV the CRYO ARM 200 II is expected to
perform better than the Glacios (SFEG) at 200 kV (Fig . 2). However, the dataset did not reach
higher resolution, and at this stage i t is not clear what limited the practical performance. One
possible reason is the relatively large pixel size and the need to rely on super -resolution
processing. More advanced algorithm s, such as post-acquisition super resolution (PASR)
(Burton-Smith & Murata, 2023), may help to improve the result.
4. Discussion
The EMDB deposition statistics (Fig. 1) indicate that despite their proven excellent performance
200 kV cryo -microscopes remain heavily underutilized. At cryo-EM facilities that also have 300
kV instruments, 200 kV microscopes are used primarily for sample screening and exploratory
data collection. Understandably, having the option to use a top -of-the-line 300 kV instrument,
researchers will choose to collect their data on it instead of the potentially lower-performing 200
kV machine. Such a choice was indeed justifiable with last generation 200 kV microscopes
equipped with SFEG emitters which limited their performance in the sub-3 Å range, as illustrated
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by the lower number of 200 kV EMDB depositions in this range (Fig. 1) and the temporal envelope
(Fig. 2, Glacios).
The introduction and wider adoption of CFEG emitters in recent years dramatically reshaped the
cryo-EM performance landscape (Fig. 2, solid vs dashed/dotted lines). In particular, it
significantly improved 200 kV performance in the 2 –3 Å range (Fig. 2, Glacios vs CRYO ARM
200/Glacios 2). In addition to their optical performance advantages, CFEGs are also less costly
to maintain because they do not require periodic emitter exchange s. In use, they do exhibit a
gradual decline of emission current over time, necessitating tip flashes every ~8 hours, but this is
handled automatically and can be performed during cryogen filling cycles to avoid extra
acquisition interruptions.
The CRYO ARM 200 II microscope tested here introduces yet another performance-enhancing
feature in the form of a narrow gap objective lens polepiece, which reduces chromatic aberration
and further expands the resolution envelope (Fig. 2, pink line). Its single-particle performance is
comparable to top-of-the-line 300 kV instruments, both in theory and practice, as demonstrated
by the results presented here (Figs. 3, 5, 6). The only practical limitation of the narrow -gap
polepiece is the lack of sample tilti ng capability. This precludes applications such as cryo -
tomography (Nogales & Mahamid, 2024) , MicroED (Clabbers et al. , 2025) , or single particle
samples with severe preferred orientation requiring tilted acquisition (Aiyer et al. , 2024) .
Observations involving thicker samples (≥100 nm), such as cryo -tomography and 2D template
matching of cellular samples, single particle analysis of viruses, liposomes, etc., will continue to
benefit from higher accelerating voltages (Peet et al., 2019) . However, for the vast majority of
single-particle projects, the CRYO ARM 200 II offers uncompromising practical performance.
New technological developments, such as narrow -gap lenses and CFEGs will bring 100 kV
microscopes closer to becoming the most cost- effective option for sample screening and
exploratory data collection. Here, as well as in other recent works (Chan et al., 2024), the first
sub-2 Å cryo -EM test structures from 100 kV instruments were presented. In practice, factors
such as sample thickness, higher sensitivity to optical aberrations, electromagnetic
disturbances, sample charging, and detector performance, must also be considered and tested
before declaring success. Overall, the proof will be in the real -world sample results that will be
coming out of upgraded 100 kV microscopes.
In conclusion, with the technological advances discussed here, cryo-EM instrumentation could
be entering a period of experimental role hand -down, where tasks that were exclusive to 300 kV
instruments will become more common on 200 kV , and those from 200 kV will be shifted to 100
kV . The goal of this process is to make cryo-EM more accessible, affordable, and prolific.
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Figure 1. Resolution statistics of cryo -EM maps with resolution below 6 Å from 300 kV
and 200 kV microscopes deposited in the Electron Microscopy Data Bank (EMDB) in the
last six years (2020 –2025). The resolution histograms (pink and light blue bars) were
normalized by the number of depositions. Log -normal fits of the histograms are shown
with red and blue lines. The number of depositions and median resolution from the log -
normal fits are listed in the text boxes.
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Figure 2. Theoretical temporal coherence envelope of various microscope configurations.
Solid lines represent Cold Field Emission Gun (CFEG) instruments (ΔE = 0.3 eV). Dashed
and dot-dashed lines correspond to Schottky (thermionic) FEG machines (ΔE = 0.7 eV) .
The CRYO ARM 200 II (pink line) evaluated here is second in optical performance after the
top-of-the-line CRYO ARM 300 II and Krios 5.
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Figure 3. 2D Fourier transform amplitudes of an oriented single crystal (100) gold sample
image from the CRYO ARM 200 II. The visibility of lattice plane (046) spots corresponding
to 0.566 Å spacing in the direction of the sample stage tilt axis and lattice plane (044)
spots corresponding to 0.721 Å spacing in the perpendicular direction attest to the
excellent optical performance of the microscope, going beyond 1 Å in all directions.
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Figure 4. Acquisition patterns and exemplary images for the ( a, b) 200 kV and ( c, d) 100
kV apoferritin test datasets. (a, c) Acquisition pattern schematics with support film holes
in light blue, detector size and shape in blue, and beam size and position in pale yellow.
Numbers indicate the acquisition order. ( b, d ) Exemplary images from the datasets
collected at ( b) 200 kV on a Gatan K3 camera, and ( d) 100 kV on a DECTRIS SINGLA
hybrid-pixel detector. The interpolated inter-module gap of the SINGLA detector is visible
as a blurred horizontal stripe through the middle of the image.
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Figure 5. Atomic resolution cryo-EM reconstruction of the 200 kV apoferritin dataset. (a)
Overview of the 3D density map of a monomer. (b) Plot of the gold-standard FSC (GS FSC)
indicating 1.24 Å resolution at 0.143 level and the map -model FSC indicating 1.2 5 Å
resolution at 0.5 level. (c) Sidechain map features. The gray surface is at a lower threshold
level typically used to depict the map. The blue surface is at a high threshold level ,
showcasing the atomic resolution of the map with blobs for individual atoms. T he green
surface represents an Fo - Fc difference density map (3σ level, normalized within a mask)
calculated from a hydrogen -omit model. Positive density peaks are clearly visible at
positions corresponding to hydrogen atoms in the molecular model.
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Figure 6. Rosenthal-Henderson B -factor plots comparing the overall cryo -EM
performance of the CRYO ARM 200 II (red symbols and line) and the Krios G4 (blue
symbols and line) microscopes with apoferritin samples. The slopes of the linear fits (red
and blue lines) correspond to B-factors of 39.0 Å
2 and 38.7 Å2, respectively.
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Figure 7. Effect of radiation damage on resolution. ( a) Plot of the resolution of
reconstructions from the first 1,000 movies containing 58k particles versus the sample
pre-exposure (red symbols) by omitting a varying number of initial frames from the movies.
The experimental distribution was fit well (R2 = 0.997) by a parabola (red line, coefficients
in the legend). The plot also contains numerical estimates of the radiation damage effect
using the measured (black symbols) and 82 % of the measured (blue symbols)
experimental total exposure. (b ) Panels illustrating map feature deterioration with
increasing pre-exposure. Pre-exposure value and map resolution are shown at the top of
each panel.
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Figure 8. Result from the reconstruction of the 100 kV apoferritin dataset collected on
the CRYO ARM 200 II with the DECTRIS SINGLA hybrid-pixel detector. The 3D
reconstruction reached 1.91 Å resolution. (a) 3D density map showing holes in aromatic
sidechains. (b) Gold-standard FSC plot.
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