SOPHIA 2048B

2y ago
45 Views
2 Downloads
6.78 MB
16 Pages
Last View : 2m ago
Last Download : 2m ago
Upload by : Maxine Vice
Transcription

SOPHIA 2048B DatasheetSOPHIA 2048BULTRA-LOW-LIGHT, LOW-NOISESCIENTIFIC CAMERAS 95% peak QE, UV to NIR sensitivity 2 e- read noise Fast, multiport readout ArcTec deep coolingpi.info@teledyne.com PHONE 1.609.587.9797

SOPHIA 4096B DatasheetConnected Teledyne – Helping Drive Your ResultsTeledyne PortfolioTeledyne Imaging provides a collective of expertise acrossthe spectrum. Individually, each division offers best-in-classsolutions. Together, they leverage their combined strengths toprovide the deepest technology portfolio in the world. Fromnano scales in the world of electron microscopy to spacebased astronomical imaging, Teledyne Imaging brings scaleto the world’s most difficult and demanding applications.Working For YouTeledyne is committed to operational excellence at eachstep with involvement at every level of the supply chain –from pixel and sensor design to fabrication, systems andanalysis, reducing our customer’s exposure. By leveraginga continuous link to a network of engineers, we grant ourcustomers full access to our proprietary technologies anddevelopments, providing an optimal solution that surpassesany multi-component integration.PartnershipsTeledyne Imaging has supported customer innovation needsfor decades. Our partners are matched to a dedicated teamof experts that ensure quick integration with software,optical, electrical, and mechanical elements. Additionally,the Teledyne team is in full consultation with their partners,supporting projects from start to end, with supply guarantees.

SOPHIA 2048B DatasheetHighlightsBreakthrough High-Performance CCD CamerasSOPHIA 2048B cameras are designed from the ground up for the most demanding lowlight applications, such as astronomy, in vivo imaging, and semiconductor failure analysis: Back-illuminated CCD sensors with 95%peak QE2048 x 2048 resolution with 13.5 and 15micron pixels, up to 39 mm diagonalHigh frame rates with up to 4-portreadoutCooling down to -90ºC , liquid and aircooling in the same chassisApplications include:Semiconductor Failure Analysis Astronomy Photometry Laser Beam ProfilingLuminescence and Fluorescence Imaging In vivo ImagingDesigned for low-lightapplicationsSOPHIA 2048B cameras offer optimum performance: Air or liquid cooling for low dark current High QE (peak 95%) Wide dynamic range (16-bit readout)When speed is paramountSOPHIA 2048B cameras have the newest readout electronics: Single-, dual-, and quad-port simultaneous readout Multiple ADC speeds (up to 16 MHz) Binning and ROI readout Custom readout modes for microsecond exposures

SOPHIA 2048B DatasheetImaging Software FlexibilityMost imaging experiments need flexibility - and the SOPHIA 2048B is a perfect fit: Microsoft Windows 10 or Linux 64-bit operating system support Seamless integration of controls and data acquisition into MATLAB (MathWorks), LabVIEW (National Instruments), ASCOM, Maxim DL (Cyanogen Imaging), and Python SDK / API compatible with Microsoft Windows and Linux

SOPHIA 2048B DatasheetKey Camera FeaturesSOPHIA 2048B cameras are designed from the ground up for the most demanding lowlight applications, such as astronomy, in vivo imaging, and semiconductor failure analysis:SOPHIA 2048B - 15230.7 mm27.6 mmSOPHIA 2048B - 13227.6 mme2v CCD42-40: 2048 x 2048 resolutionsensor with 13.5 micron pixels and up to8 MHz readout (2 x 4 MHz)30.7 mme2v CCD230-42: 2048 x 2048 resolutionsensor with 15 micron pixels and up to 16MHz readout (4 x 4 MHz)Proprietary 2-portand 4-port readoutfor low noise andhigh frame ratesUltra-high-vacuum,all-metal seal designfor deep cooling(ArcTecTM) down to-90ºCFlexibility to use air,air liquid, or liquidcoolingThe latest UHVtechnology withall-metal constructionand industry-standardCF vacuum interfacefor lifetime vacuumguaranteeReliable PerformancePrinceton Instruments has been designing high-performance scientific cameras for morethan three decades: Hundreds of cameras being used at leading laboratories around the worldYears of trouble-free operation a result of uncompromised engineering design andproductionComplete software ecosystem simplifies image acquisition and processingContinuous innovation to meet evolving requirements and applicationsVacuum chamber limited lifetime warranty

SOPHIA 2048B DatasheetSOPHIA 2048B - 132 SpecificationsFeatureCCD image sensorDark current @ -90 C(with ambient air @ 20 C)Quantum efficiencySOPHIA 2048B-132-VS-RSOPHIA 2048B-132-VS-UVe2v CCD42-40; back illuminated; deepdepleted; grade 1; NIMOe2v CCD42-40; back illuminated;UV enhanced; grade 1; NIMO0.0001 e-/p/s (typical)See QE curves on next pageCCD format2048 x 2048 imaging pixels: 13.5 x 13.5 μm pixels: 100% fill factorImaging area27.6 x 27.6 mm (optically centered)Deepest coolingtemperature -90 C (typical) with liquid chiller; -90 C (typical) with airThermostating precisionCooling methodFull wellADC speed/16 bitsSystem read noise per port@ 100 kHz@ 1 MHz@ 4 MHzVertical shift speedNonlinearitySoftware-selectable gainsData interfaceI/O signals 0.05 CThermoelectric air or liquid cooling (liquid chiller required)Single pixel: 100 ke- (typical), 80 ke- (minimum);8 MHz, 2 MHz, and 200 kHz3.5 e- rms (typical)7 e- rms (typical)19 e- rms (typical)24 μsec/row (programmable 2% @ 100 kHz1, 2, 4 e-/ADU (low-noise input, typical)USB 3.0 (5 m interface cable provided);Optional fiberoptic interface available for remote operationTwo MCX connectors for programmable frame readout, shutter, trigger inOperating environment 5 C to 30 C non-condensingBake-out temperature70 C (maximum)CertificationCamera head dimensions(L x W x H)Camera head weightSpecifications are subject to changeCE251.6 mm (9.91”) x 129 mm (5.08”) x 142.8 mm (5.62”)6.5 kg (14.3 lbs)

SOPHIA 2048B DatasheetSOPHIA 2048B - 132 QuantumEfficiency CurvesFrame RatesSOPHIA 2048B - 132Binning8 MHz2 MHz200 84.303.761.82

SOPHIA 2048B DatasheetSOPHIA 2048B - 152 SpecificationsFeatureCCD image sensorDark current @ -90 C(with ambient air @ 20 C)CCD processingQuantum nated eXcelon CCD. Highestsensitivity in the visible region. Highsensitivity in the NIR.Extremely low etaloning. 100x lowerdark charge than deep-depletedsensors.Back-illuminated CCD. Highestsensitivity in the visible region. Basicmidband (MB) AR coating.Princeton Instruments’ proprietaryCCD; grade 1; AIMOe2v CCD230-42;grade 1; AIMO0.00025 e-/p/s (typical)Optional CCD processing for UV and NIRSee QE curves on next pageCCD format2048 x 2048 imaging pixels: 15 x 15 μm pixels: 100% fill factorImaging area30.7 x 30.7 mm (optically centered)Lens mountF-mount with integral 45 mm shutterDeepest coolingtemperatureThermostating precisionCooling method -90 C (typical) with liquid chiller; -90 C (typical) with air 0.05 CThermoelectric air or liquid cooling (liquid chiller required)Full wellSingle pixel: 150 ke- (typical)ADC speed/16 bits16 MHz, 4 MHz, and 400 kHzSystem read noise per port@ 100 kHz@ 1 MHz@ 4 MHzVertical shift speedNonlinearitySoftware-selectable gainsData interfaceI/O signalsOperating environmentCertificationCamera head dimensions(L x W x H)Camera head weightSpecifications are subject to change3.6 e- rms (typical)8.5 e- rms (typical)22 e- rms (typical)24 μsec/row (programmable 2% @ 100 kHz1, 2, 4 e-/ADU (low-noise input, typical)USB 3.0 (5 m interface cable provided);Optional fiberoptic interface available for remote operationTwo MCX connectors for programmable frame readout, shutter, trigger in 5 C to 30 C non-condensingCE251.6 mm (9.91”) x 129 mm (5.08”) x 142.8 mm (5.62”)6.5 kg (14.3 lbs)

SOPHIA 2048B DatasheetSOPHIA 2048B - 152 QuantumEfficiency CurvesFrame RatesSOPHIA 2048B - 152Binning16 MHz4 MHz400 15.42.9

SOPHIA 2048B DatasheetApplicationsAstronomyGround-based optical astronomy covers an expansive rangeof scientific research. Longer exposures are common dueto the faint signal of objects within space. The SOPHIA,with deep cooling down to -90 C, has ultra-low dark noise,making it ideal for longer exposure experiments. With a peakquantum efficiency of 95%, the SOPHIA is optimized for highsensitivity over the visible wavelength range.The SOPHIA has a large format CCD sensor, increasing lightcapture and throughput. This is perfect for capturing largerobjects, for enhancing object calibration by imaging morereference stars per frame, and for ultra-low light capture offaint objects. The quad-port readout architecture allows forfaster readout speeds with similar read noise, for dynamicobject capture. Deep-depletion technology and enhancednear infrared sensitivity, with 95% QE over the 700-850 nmrange, also makes the SOPHIA a great fit for NIR applicationssuch as exoplanet characterization.In vivo imagingSmall animal research is key for translational medical research.Optical imaging detection is a common technique used withinmedical imaging and can provide important information forresearch areas such as disease detection and medicinal drugefficacy.The SOPHIA camera has a large format CCD sensor for highthroughput in vivo imaging over the 300 - 1000 nm range.The large field of view offers high efficiency, allowing forgreater visualization of target tissue while reducing samplephotodamage. As more of the sample area can be imaged,more quantitative analysis can be done on each acquiredframe.With deep cooling down, a high dynamic range and 95%quantum efficiency, the SOPHIA is often chosen for ultra-lowlight imaging, common within in vivo studies. The low noiseof the SOPHIA makes it perfect for long integration times,providing effective acquisition over a large imaging area.

SOPHIA 2048B DatasheetNanotechnology CharacterizationNanotechnology encompasses a variety of researchcharacterizing dimensions that are less than approximately 100nanometers, including the development of faster electronics,the enhancement of biomedical imaging, and the creation ofultra-strong, extremely lightweight materials.With a peak quantum efficiency of greater than 95% and alarge format sensor for high throughput, the SOPHIA provideshigh sensitivity for nanoparticle detection. The large fieldof view offers more quantitative analysis per frame whilstdeep cooling provides ultra-low dark noise, meaning longerexposures can be used for measuring extremely faint signals.Nanotechnology can be characterized via imaging andspectroscopy, each providing complementary information.The SOPHIA can be utilized for both, providing high qualityacquisition regardless of technique used. The addition ofeXcelon technology, with high NIR and UV quantum efficiencyalongside reduced etaloning (fringing), offers better imagingand spectral quality for low-light nanoparticles in this range.

SOPHIA 2048B DatasheeteXcelon 0100010501100Wavelength (nm)1010 1050 1090Etaloning Performance Comparison - eXcelon : B/IWavelength (nm)% QE Increase (eXcelon : BI)NOTES: QE data at 25 C. The PIXIS: 512 eXcelon QE data represents calculated measured values.B eXcelon provides superior QE over the standardback-illuminated (“B/I”) version in the UV-NIR range.B eXcelon provides significantly lower etaloning(unwanted fringes) compared to standard backilluminated (“B/I”) version.eXcelon is available as an option for most Teledyne CCDand CMOS sensors600 nm700 nm800 nm900 nm1000 edCCDData taken with white light source through a monochromator comparing etaloningperformance of eXcelon vs. back-illuminated CCDs.

SOPHIA 2048B DatasheetLightField SoftwareThe Future of Scientific Imaging and SpectroscopySoftwareThe combination of LightField and the SOPHIA 2048B provides researchers with the mostadvanced and reliable toolset for experimental setup, data acquisition, and post processing: Powerful 64-bit software packageincludes Microsoft Windows 10 support CompletecontrolofTeledynePrinceton Instruments cameras andspectrometers Dependable data integrity via automaticsaving to disk, time stamping, andretention of both raw and correcteddata Full experimental details and systemsettings are archived and can bereloaded for future experimentsensuring maximum reproducibility For light-sensitive experiments, the user interface offers “low light” and “no light” modes duringdata acquisition LightField works seamlessly in multi-user facilities, remembering each user’s hardware andsoftware configurations Simple math functions and complex transforms can be applied to live or stored data, with anincluded easy-to-use editor to create your own formulas Integrated LabVIEW , MATLABTM , PythonTM , ASCOM and Maxim DLTM Exports to your favorite file formats, including TIFF, FITS, ASCII, AVI, IGOR, and Origin Demo camera mode allows the user to view all of the settings and parameters associated withany camera without physically connecting the camera Live data processing operations provide real-time evaluation of incoming data to optimizeexperimental parameters

SOPHIA 2048B DatasheetAccessoriesSOPHIA 2048B cameras can be provided in custom configurations to suit your experiment.Please contact your local Teledyne Princeton Instruments representative. The mostcommon configurations are listed below:Quick Start GuideUSB 3.0 cableI/O breakoutcable (BNC)SOPHIA 2048BPower supplyCameraOptional accessories and customization: LightField softwarePICam SDK/API for Linux and Microsoft Windows (provided for free)Customized coatings and filters from UV to NIRCustom optical assemblies

SOPHIA 2048B DatasheetSOPHIA 2048B - 132SOPHIA 2048B - 152

SOPHIA 2048B ULTRA-LOW-LIGHT, LOW-NOISE SCIENTIFIC CAMERASContact your local Teledyne PrincetonInstruments representative for additionalinformation.Teledyne Princeton Instruments – USATel: 1 609.587.9797pi.info@teledyne.comChinaTel: 86 157 2153 5343pi.info.china@teledyne.comFranceTel: 33.1.70.38.19.00EVR@teledyne.comGermanyTel: 49 (0) 89-660 779 3pi.germany@teledyne.comJapanTel: 81.3.5639.2741PI.Nippon@teledyne.comImage CreditsUnited KingdomTel: 44 (0) 7810 835 719pi.info@teledyne.comPage 2:Yu et al., “Coherent X-ray scattering beamline at port 9C of Pohang Light Source II,” J.Synchrotron Rad. 21, 264-267 (2014). doi: 10.1107/S1600577513025629Copyright 2021 Princeton Instruments, Inc. All rights reserved. ArcTec and KURO are trademarks and SOPHIA, eXcelon, and LightField areregistered trademarks of Princeton Instruments, Inc. Microsoft and Windows are registered trademarks of Microsoft Corporation in the UnitedStates and other countries. Linux is the registered trademark of Linus Torvalds in the U.S. and other countries. Python is a registered trademark ofthe Python Software Foundation. All other brand and product names are the trademarks or registered trademarks of their respective owners andmanufacturers.Use and Disclosure of Data Information contained herein is classified as EAR99 under the U.S. Export Administration Regulations. Export, re-exportor diversion contrary to U.S. law is prohibited.GET IN TOUCH to find out morewww.princetoninstruments.comRev A0-03022021

sensor with 13.5 micron pixels and up to 8 MHz readout (2 x 4 MHz) e2v CCD230-42: 2048 x 2048 resolution sensor with 15 micron pixels and up to 16 MHz readout (4 x 4 MHz) SOPHIA 2048B - 132 27.6 mm 30.7 mm 27.6 mm 30.7 mm SOPHIA 2048B - 152 Reliable Performance Princeton Instruments has been designing high-performance scientific cameras for more

Related Documents:

4 INAUGURATION Le village du WE des Sciences de Sophia Antipolis 2014 sera inauguré le Samedi 11 Octobre, à 17h00, en présence du Maire de Valbonne Sophia Antipolis, de représentants de PERSAN, de la CASA, du Conseil général des Alpes-Maritimes, du Conseil régional PACA, et de la DRRT.

With SOPHIA’s auto-tuning capability, Redis is able to oper-ate through the entire range of workload sizes and read/write intensities, while the vanilla Redis fails with large work-loads. The main contributions of SOPHIA are: 1. We show that state-of-the-art static tuners when applied

Yes, sharing is the key to elf wealth,” said Sophia. 19. After lunch, they took us to their garden. “Liam is a bio-hacker, constantly experimenting with new plants like these grapes that keep us from getting sun burned,” explained Sophia. Liam continued, “When I develop a particularly

Sophia Mergiali-Sahas Page 2 Bibliography and Index. 2. Writing history with the Saints: from the society of the saints to the society of the Palaeologan era (1261-1453) (in Greek), Editions Herodotos, Athens 2014. ARTICLES 1. «Paul Lemerle (22 aνril 1908 - 17 juillet 1989)», Modern Greek Studies Yearbook 6 (1990) 427-42. 2.

The dark-eyed girl became unusually lively and pretty, and her presence cheered them. Of the two old maidens, the younger one--Sophia Ivanovna--was the kindlier, while the older one--Maria Ivanovna--was of austere disposition. Sophia Ivanovna kept the girl in decent clothes, taught her to read and intended to give her an education.

dark-eyed girl became unusually lively and pretty, and her presence cheered them. Of the two old maidens, the younger one--Sophia Ivanovna--was the kindlier, while the older one--Maria Ivanovna--was of austere disposition. Sophia Ivanovna kept the girl in decent clothes, taught her to read and intended to give her an education.

installing or operating your new air conditioning unit. Make sure to save this manual for future reference. This manual only describes the installation of the outdoor unit. When installing the indoor unit, refer to the installation manual of the indoor unit. MULTI-ZONE INVERTER SOPHIA SPLIT AIR CONDITIONER WITH HEAT PUMP OUTDOOR UNIT

technologies and computation methods for the automotive traction motors. Various cooling methods, including the natural, forced air, forced liquid and phase change types, are discussed with the pros and cons of each method being compared. The key factors for optimizing the heat transfer efficiency of each cooling system are highlighted here. Furthermore, the real life examples of these methods .