pco-edge-42-bi-1

pco-edge-42-bi-2

pco-edge-42-bi-3

pco-edge-42-bi-4

pco-edge-42-bi-5

pco-edge-42-bi-6

pco.edge 4.2 bi XU USB sCMOS Camera The pco.edge 4.2 bi XU features a back-illuminated sCMOS sensor with extremely specific coating ideally suited for use in applications in the visible light down to extreme UV (EUV) and soft X-ray radiation. Featuring 2048 x 2048 pixel resolution and 6.5 μm pixel size, the pco.edge 4.2 bi XU allows full frame acquisitions at 40 fps with a dynamic range of 88 dB at a noise level of 1.9 e-.

pco.edge 4.2 bi XU camera for soft X-ray imaging

pco.edge 4.2 bi XU USB sCMOS Camera with CF100-flange. This camera is ideal for imaging extreme UV (EUV) and soft X-ray radiation. Spectral range: 1 to 1100 (1.2 keV to 1.1 eV)

TE-cooled Back-illuminated 4MPix sCMOS Camera

Name: TE-cooled Back-illuminated 4MPix sCMOS Camera
SKU: 101

Spectral Range

Clear

Key Features:

2048 x 2048 Pixel Array
Back-Illuminated sCMOS Sensor
Up to 95% Quantum Efficiency
Spectral Options:
- Monochrome (standard): 370 – 1100nm
- UV-enhanced: 190 – 1100nm
- Extreme UV (EUV) and soft X-ray: 1 nm to 1100 nm (1.2 keV to 1.1 eV)
Adjustable Cooling, Down to -25°C
Low-light mode uses Correlated Multi Sampling to achieve 1.0e^– Median Read Noise
40fps Maximum Frame Rate
USB 3.1 Gen1

Suggested Applications:

brightfield microscopy microscopy
fluorescence microscopy
digital pathology
single molecule localization microscopy
lightsheet fluorescence microscopy (LSFM)
calcium imaging
FRET & FRAP
structured illumination microscopy (SIM)
highspeed bright field ratio imaging
high throughput screening
high content screening
biochip reading
TIRF microscopy
spinning disk confocal microscopy
3D metrology
ophthalmology
photovoltaic inspection
industrial quality inspection
astronomy
bio luminescence
chemiluminescence
Special “XU” version: 1 to 1100 (1.2 keV to 1.1 eV), with CF-100 flange for ultra-high vacuum operation
- EUV (extreme UV) imaging
- soft X-ray radiation

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Product Description

The pco.edge 4.2bi series is based on a back illuminated (bi) sCMOS sensor. This offers a 95% QE performance within the pco.edge line of sCMOS cameras, making the pco.edge 4.2 bi a superb choice for many challenging imaging conditions. The pco.edge 4.2 bi is offered with an USB 3.1 interface, complementing its performance.

The adjustable cooling system in the pco.edge 4.2 bi allows the use of air or water to cool the sensor down to -25 °C. At this temperature, the dark current is reduced to 0.2 e-/pixel/s. TE-cooling is therefore very useful in low-light imaging applications in which long exposures are typically used. For shorter exposures, TE-cooling does not provide a significant benefit. For applications in which exposures are typically shorter than 1s, it is worth considering the pco.panda 4.2 bi which uses the same back-illuminated sensor as this camera, but in a non-cooled configuration.

Depending on the spectral needs of the application, scientists may select a pco.edge 4.2 bi camera with an input window that is optimized for either for the UV or VIS range. In the UV version, a specialized input window is installed internal to the camera. With a factory-installed UV window, the pco.edge 4.2 bi UV camera enables imaging with the back illuminated imager in the ultraviolet wavelength range with responsivity down to 190nm.

A special pco.edge 4.2 bi XU version is offered for EUV and soft X-ray imaging applications. The “XU” version features an extremely specific coating ideally suited for use in applications in the visible light down to extreme UV (EUV) and soft X-ray radiation. Based on the same sCMOS image sensor with 2048 x 2048 pixel resolution and 6.5 μm pixel size, the pco.edge 4.2 bi XU allows full frame acquisitions at 40 fps with a dynamic range of 88 dB at a noise level of 1.9 e^–. The XU version is offered with a CF-100 flange, allowing the camera to be used in vacuum environments down to 1 x 10(-7) mbar.

This camera series supports an HDR mode for wide dynamic range imaging as well as a low light mode which reduces the temporal read-noise by a process of correlated multi sampling (CMS).

The sCMOS image sensor used in this camera has two readout and Analog-to-Digital (A/D) conversion datapaths, shown below as “Top” and “Bottom” readout chains. These pixel values in the two datapaths result from the same exposure.

In the High Dynamic Range (HDR) mode, different analog gains are applied to the Top and Bottom readout chains: the low gain image is optimized for high full well capacity, and the high gain image is optimized for low read noise. The animation below shows the typical HDR mode of operation in which the low-gain and high-gain datapaths are combined. Data from the dimmest content as well as the brightest content are blended in a way to achieve an image with a high intra-scene dynamic Range.

In the low light mode, the top and bottom datapaths are both set to high gain, which means that both A/D converters on the image sensor digitize low intensity pixel values, optimized for low read noise. The signal within each pixel is simultaneously digitized by the two A/D converters and added – a technique that is referred to as correlated multi sampling (CMS). This causes a reduction of the read noise, the trade-off being that the usable intra-scene dynamic range of the sensor is reduced in comparison with that achievable in the HDR mode. This is usually not a concern under low light conditions. Note: sampling theory estimates a noise reduction by a Sqrt(2) factor, see datasheet (see page 2).

This camera series also supports a lightsheet scanning mode which leverages the rolling shutter readout of the sCMOS imager, in which the readout direction of the sensor is from top to bottom. The standard line time value is 12 μs and it can be set from this camera specific line time up to 2 ms. Compared to the standard operation mode, the lightsheet scanning mode enables the selection of the parameters “Line Time” and “Exposure Lines”. This guarantees an optimized synchronization to an existing lightsheet microscope setup which has no selectable speed or timing. It is possible to set a delay prior to the exposure start.

Host Interface: USB 3.1

Spectral Options:

Monochrome (standard): 370 – 1100nm
UV-enhanced: 190 – 1100nm
Extreme UV (EUV) and soft X-ray: 1 nm to 1100 nm (1.2 keV to 1.1 eV)

Image Sensor	sCMOS monochrome (Back Illuminated)
Pixels (H x V)	2048 x 2048
Max. Frame Rate (fps) at full resolution	40
Pixel Size (µm)	6.5 x 6.5
Image Sensor dimensions (mm)	13.3 x 13.3 (diagonal: 18.83)
Peak QE (monochrome)	93% \| 88% (UV version)
Spectral Range (nm)	370 - 1100 \| 190 - 1100 (UV version)
Full Well Capacity (e-)	48,000
Readnoise (e-)	1.8(med) / 1.9(rms) \| Low Light Mode (CMS): 1.0(med) / 1.1(rms)
Dark Current (e-/p/s) @ -25°C sensor temperature	0.2
A/D conversion factor (e-/DN)	0.8
Dynamic Range	26,667:1
Dynamic Range (dB)	up to 88.5
Bit depth	16
Shutter Type	Rolling Shutter (RS)
Exposure range	10μs - 20s
Time Stamp	In image (1μs resolution)
TE-Cooling	adjustable from -25°C to +20°C with air (fan) \| water cooling calibration setpoint: -10°C
Camera Interface	USB3.1 Gen1
Binning horizontal	x1, x2, x4
Binning vertical	x1, x2, x4
ROI horizontal	steps of 32 pixels
ROI vertical	steps of 8 pixels
Trigger input signals	frame trigger, acquire (SMA connectors)
Trigger output signals	exposure, busy (SMA connectors)
Software	pco.camware
SDK	pco.sdk Included
3rd Party Software support	LabVIEW, MATLAB, Micro-Manager and others
Optical Interface	F-mount, C-mount
Dimensions (mm)	80 x 85 x 109
Weight (grams)	920

Use your mouse to read QE data at wavelengths of interest.
Right-click and drag to zoom-in along the X-axis to expand the view for a desired range of wavelength.
To pan left or right within a zoomed-in view, hold down the Shift key and use your mouse.
To revert from a zoomed-in view to a normal view, click on the “Reset zoom” button that is displayed at the top-RHS of the graph.

Transmittance Curves of Windows installed in the pco.edge 4.2bi (VIS) and pco.edge 4.2bi uv (UV) versions

All QE values on this website are the best estimates available from various sources, and not necessarily from the manufacturer of the specific image sensor or from the manufacturer of the cameras in our Product Showcase. They represent the best estimates for the imagers by themselves, with the caveat that glass and other optics in the imaging path can significantly impact the spectral sensitivity of an imaging system.

As described on our Knowledge Base article on this subject, these values exist in a range. Therefore no absolute precision is implied, even when QE values are shown to two decimal places! These values and graphs are intended to be used for reference can be use for making useful comparisons between cameras. They are not intended to be a specification or a performance guarantee.

Using the method described in our Knowledge Base Article titled “How Diffraction Limits the Optical Resolution of a Microscope” one can estimate the performance of this camera when used in a microscope with commercially available microscope objectives. In the table below, it is assumed that the microscope is comprised of the objective and a tube lens with the correct focal length for the objective such that the nominal optical magnification of the microscope is the value that is specified for the objective.

Camera Parameters
Optical Format	#Megapixels	#H pixels	#V pixels	Pixel size (μm)	H size (mm)	V size (mm)	Diagonal (mm)
18.8mm < 4/3"	4.2	2048	2048	6.5	13.31	13.31	18.83
Commercially Available Objectives
Objective: Mag/NA	1X\0.03NA	2X\0.1NA	4X\0.13NA	10X\0.26NA	20X\0.5NA	40X\0.75NA	60X\0.85NA	100X\1.4NA
Min. feature size (um)	11.18	3.36	2.58	1.29	0.67	0.45	0.39	0.24
Max pix size (um)	5.59	3.36	5.16	6.45	6.70	9.00	11.70	12.00
FN (mm)	22	22	22	22	22	22	22	22
WD (mm)	8	56.3	17.2	16	2.1	16	0.66	0.31-0.4
NA	0.03	0.1	0.13	0.26	0.5	0.75	0.85	1.4
Magnification	1	2	4	10	20	40	60	100
Estimated Performance of Camera and Objective Combinations
(*) Limiting Resolution (µm)	13	6.5	3.25	1.3	0.67	0.45	0.39	0.24
Vignetting?	No	No	No	No	No	No	No	No
FOV (H x V) mm	13.31 x 13.31	6.66 x 6.66	3.33 x 3.33	1.33 x 1.33	0.67 x 0.67	0.33 x 0.33	0.22 x 0.22	0.13 x 0.13
FOV (diagonal) mm	18.83	9.42	4.71	1.88	0.94	0.47	0.31	0.19
Please contact our imaging experts for assistance in selecting a camera & objective combination that fulfils your FOV & resolution requirements at application-specific wavelengths.
1) The minimum feature size is estimated using the Rayleigh Criteria at λ = 550nm; it can be re-calculated for other wavelengths. R = 1.22*λ/(2NA)
2) The maximum pixel size is estimated by applying the Nyquist criteria to the minimum feature size as it appears on the imager plane. Maximum pixel size = R*magnification/2
3) Camera and Objective combinations which meet the Nyquist criteria and are therefore diffraction limited are indicated by showing the Limiting Resolution in green font. (*)
4) Values for Working Distance (WD) and Field Number (FN) are shown for reference only. Actual values may vary.
5) Vignetting, a darkening of the image at the corners, may be observed if the Imager Diagonal is larger than the Field Number of the Objective.

Optical Format	#Megapixels	#H pixels	#V pixels	Pixel size (μm)	H size (mm)	V size (mm)	Diagonal (mm)
18.8mm < 4/3"	4.2	2048	2048	6.5	13.31	13.31	18.83
In applications that require the best achievable optical resolution, it is desirable to use a lens with an optical resolution ≥ 76.9 lp/mm for an image sensor with a pixel size of 6.5μm. This will ensure that the optical resolution of the camera & lens combination is Nyquist-limited by the pixel-size of the camera, and not by the quality of the lens.

The imager in this camera has a diagonal of 18.83mm, which is smaller than the ~21.6mm diameter image projected by lenses designed to be compatible with the 4/3″ optical format. These lenses can be used with this camera without vignetting, since their projected image will slightly overfill the image sensor.

The optical resolution of the lenses shown exceed the limiting optical resolution of 76.9 lp/mm imposed by the 6.5μm pixels and therefore all these lenses meet the Nyquist criteria. The limiting resolution for the camera and lens system (shown in the table below as the minimum resolvable feature) is therefore set by the camera, and not the lens.


Add to My List	Lens P/N	Resolution @ Center \| Edge	(*)Meets Nyquist criteria?	Focal Length	AFOV	Min. WD	Optical Magnification	Diag FOV at Min. WD	H FOV at Min. WD	V FOV at Min. WD	(**) Min resolvable feature	1mm feature =
Request Quote Already in Quote View My Quote List	1-24719	160 \| 100	yes	8.0	99.3	100	0.08	235	166	166	0.16	12
Request Quote Already in Quote View My Quote List	1-19910	160 \| 100	yes	12.0	76.2	100	0.12	157	111	111	0.11	18
Request Quote Already in Quote View My Quote List	1-19911	160 \| 100	yes	16.0	60.9	100	0.16	118	83	83	0.08	25
Request Quote Already in Quote View My Quote List	1-19912	160 \| 100	yes	25.0	41.3	150	0.17	113	80	80	0.08	26
Request Quote Already in Quote View My Quote List	1-19913	160 \| 100	yes	35.0	30.1	200	0.18	108	76	76	0.07	27
Request Quote Already in Quote View My Quote List	1-19914	160 \| 100	yes	50.0	21.3	300	0.17	113	80	80	0.08	26

Notes:
The working distance (WD) is defined as the distance from the object plane to the front of the lens.
The above are theoretical estimates provided for reference, and are not a guarantee of performance. Actual FOVs and optical resolution are best determined by experiment.
FOV dimensions and min. resolvable feature sizes are estimated with the object plane placed at the minimum WD of the lens. A similar calculation may be performed for longer WDs. Please contact us for assistance: our specialists can help you identify a lens that meets your FOV requirements at a Working Distance that is convenient for your workflow.
Increasing the WD will result in larger FOVs, and lower optical resolution (an increase in the smallest resolvable feature size).
(*) The system meets Nyquist criteria if the optical resolution at the center of the lens (in lp/mm) is ≥ the pixel-size limited resolution (see above).
(**) The minimum resolvable feature size is estimated based on whether the lens meets the Nyquist criterion. If the Nyquist limit is met, then the resolution of the system is the estimated to be the distance on the sample plane that corresponds to two pixels in the image plane. If not, it is estimated based on the limiting resolution of the lens.
The method used in the above table is detailed in the linked knowledge base article titled "Choosing a Lens to meet FOV and WD requirements"