Princeton Instruments Light Field 4 Brochure Rev A0

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64-bit Data Acquisition Software DRAFT

Transcript of Princeton Instruments Light Field 4 Brochure Rev A0

8/2/2019 Princeton Instruments Light Field 4 Brochure Rev A0

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64-bit Data Acquisition Software

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Download a FREEevaluation version.

The best way toexperience the realadvantage of thissoftware is through thefull-feature evaluationversion available fordownload at: 

www.princetoninstruments.com/lighteld

The Power ofRevolutionary

ThinkingThis software is different.

Princeton Instruments LightField™ is

a new 64-bit image and spectral

acquisition software package

that provides a cutting-edge

user interface and the powerful

functionality needed to set up

and perform complex optical

diagnostic experiments.

This unique and revolutionary tool

lets researchers around the world

realize the true potential of their

advanced Princeton Instruments

low-light-level cameras and

spectrographs.

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Princeton Instruments has pioneered state-of-the-art technology and instrumentationfor more than three decades, including:

eXcelon•™ technology for minimizing

etaloning and improving sensitivity

No-compromise ProEM•™ EMCCD

cameras with single-photon-detectioncapabilities

Faster, smarter PI-MAX•® 3 ICCD cameras

that offer <500 picosecond gating

InGaAs-sensor-based cameras for NIR•

imaging and spectroscopy up to 2.2 μm

Now, with the introduction of LightField, aswell as the amazing IntelliCal™ calibrationoption, Princeton Instruments has successfullyredened the very nature of scienticimaging and spectroscopy software.

From the world leaderin low-light imaging,spectroscopy, and

x-ray detection...

LightField is an

integral part of

the best all-around

hardware/software

solutions on the

market today!

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www.princetoninstruments.com

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Whether analyzing properties of nanomaterials or observing celestial

objects, researchers require the best optical diagnostic tools.

While state-of-the-art hardware can deliver single-photonsensitivity, associated software tools leave much to bedesired. Too often, a researcher’s early enthusiasmfor their new hardware quickly wanes as thepoor design and inherent limitations of theaccompanying software become apparent.

But now there’s LightField. Say farewell

to disappointment and frustration. Theexcitement is here to stay!

Time for a change!

We’ve raised the bar!At the beginning of the LightField design project,Princeton Instruments had a fundamental choice to make.

We could either simply update an existing softwarepackage, like most companies do, or we could createsoftware entirely from the ground up, based on more than

30 years of application experience and feedback fromthe world’s leading laboratories. We chose the latterapproach.

The result is nothing less than remarkable!

It’s all about the data! LightField’s power derives from its simple but surprisingly novelguiding principle: “Provide researchers with reliable data asquickly as possible.”

In seeking to fulll this promise, the Princeton Instruments software

team created a brand new user interface, brand new calibration

methods, and even brand new concepts.

There is no comparable software available for the typical

laboratory environment!

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Two Standout

Capabilities

PI-MAX® 3 ICCD Camera Support 

What you see is truly what you get!

Princeton Instruments PI-MAX 3 ICCD cameras can measure events with ultranetemporal resolution in imaging and spectroscopy experiments via:

• A SuperSynchro™ timing generator• <500 picosecond gate widths (exposure times)

 Whenever a compatible PI-MAX 3 camera is connected, LightField displays a highlyintuitive “virtual” dashboard akin to a laboratory oscilloscope so that you can:

• Adjust the gate delay, width, SyncMaster™, and auxiliary delays on-the-y• Easily synchronize your PI-MAX 3 camera with external lasers• Quickly plot “time vs. intensity” graphs via a single click

LightField offers patent-pending IntelliCal for accurate spectrum calibration in both the

wavelength and intensity spaces! Data using standard spectral calibration (left); same

data utilizing LightField’s IntelliCal wavelength and intensity calibration (right).

Introducing IntelliCal™Automated wavelength and intensity calibration!

Publish with absolute condence. For the rst time, the spectral response of allelements in the detection path, including that of the grating and the camera, has beentaken into account.

LightField’s optional IntelliCal feature lets you rmly and immediately establish theaccuracy of your spectroscopic data on a pixel-by-pixel basis:

• Calibrate the entire spectrum in both the wavelength and intensity scalesagainst the NIST database

• Rely on patent-pending technology that delivers up to 10x better accuracythan standard calibration

To learn more about this revolutionary new feature, download our IntelliCal technicalnotes at www.princetoninstruments.com/lighteld.

LightField provides complete timing control for compatible PI-MAX 3 cameras.

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LightFieldprovideshundreds

of incrediblefeatures!Here are just a fewof our favorites...

Princeton Instruments LightField 64-bit Acqusiition software

Drag and Drop DevicesYes, simply drag and drop to create your experimentconguration. For spectroscopy, control the light pathby directly clicking the mirrors!

The Best BarView the status of hardware andacquisition settings at a glance!

A Virtual OscilloscopeA special dashboard appears whenever a compatiblePI-MAX 3 ICCD camera is connected. Take complete controlof gate delays, widths, and trigger input/output signals!

Gray Is GreatLightField’s muted gray background minimizesinterference with light-sensitive experiments. Ifcomplete darkness is required, LightField cansimply turn off monitors during acquisition.

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See the Stats The Online Statistics window gives you a quickoverview of key measurements.

All Shall Be Revealed Want a better look? Use the Image Histogramfunction to adjust image contrast.

 Images EverywhereGo ahead and work on multiple display monitors! A single imageor an entire data viewer can be relocated to a secondary monitor.

Princeton Instruments LightField 64-bit Acqusiition software

LightFieldallows youto compare

live andpreviouslyacquireddata

quickly!

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TOP 10 Features

LightField is smart. Justconnect the hardware,launch LightField, andyou’re ready to start

capturing data. It’sthat simple!

LightField detectsattached hardwareand sets up intelligentdefaults for you.

We know howimportant your data is!

LightField automatically

saves every acquisitionto your desired folderand keeps track of allexperiment settings inthe le header.

It even saves yourraw data when apost-processingfeature is applied.

2. Peace ofmind...

1.

Get upand go!

3.

It knowsyou...In many labs, PrincetonInstruments camerasand spectrographsare used by multiple

researchers.

LightField providesan easy “experimentsetup” save/loadfunction that quicklyloads your experimentsettings for you.

Need to capture dataover an extendedperiod of time?

Thanks to its native64-bit architecture,LightField is not onlyable to utilize all the

memory (RAM) availableon your computer, it canstream multi-gigabytepixel data directlyinto the hard drive, allwithout missing a beat.

4.

Streamsof data...

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TOP 10 Features

Multi-camera control,multi-spectrographcontrol.

LightField controls

each of the PrincetonInstruments camerasand spectrographsin your lab from asingle computer.

5.

Unite!6.

Simpler spectrographalignment...

7.

What’snew withStep & Glue?

8.

It’s allabouttiming!

LightField’s ROI andPeak Find featureshelp you align yourcamera on yourspectrograph morequickly than everbefore. Go from out-of-the-box to spectralacquisition in minutes!

Traditional approachescan be plagued by ahost of spectral artifacts.Our Intensity Calibrationroutine automaticallycorrects these artifacts,delivering a spectrumfree of instrumental bias.

For the rst time, highresolution and a broadspectral range can beachieved simultaneouslywith no compromises!

Every frame (or sub-framein kinetics readout mode) isautomatically hardware timestamped with 1 µsec accuracyand stored in the le data.

Simply perform a cross-sectionanalysis ona sequence

of framesto quicklygain insightinto thetemporalnature ofyour data.

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Make it your own!

Customize, customize, customize...Fancy your own user interface or post-processing tools? Need to integrate LightField with othersoftware packages? No problem. LightField has powerful add-ins and automation features built-in sothat you can get what you really want. All you need is familiarity with programming languages. Weeven provide more than 20 examples of add-in programs to get you started!

Add-ins: These are user-written utilities or tools that customize the LightField experience. Forexample, you can modify/add toolbars and tabs, add post-processing or real-time functions (e.g.,lters), or c hange display types. 

Automation: You can run LightField from a third-party software program either in the backgroundor the foreground. This is a convenient way to automate routine tasks from familiar programs.

Software SDK: For OEMs and system integrators, a comprehensive PICAM applicationprogramming interface (API) is provided for free. Programmers will love the example programs withsource code that we have included in the software development kit (SDK).

TOP 10 Features

No marketing hyperbolehere. LightField allowscomplete control oversupported PrincetonInstruments cameras and

spectrographs.

All available readoutmodes, such as frametransfer, kinetics, spectra-kinetics (microsecond timeresolution), and customchip (>10 kHz framerates), are supported.

9.

Searchanddecide.

10.

Powerful,yet easy!

Cameras and spectrographs canhave a multitude of settings, butonly a few are used routinely.

LightField’s smart search functionquickly directs you to the controlsyou want, as you type.

You can evenbuild your owncustom settingsdock to accessfrequently usedsettings!

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Key Features List

Princeton Instruments LightField 64-bit Acqusiition software

Acquisition

& Control

Supported cameras: PIXIS, PI-MAX 3•*, ProEM, PyLoN™, Quad-RO

Supported spectrographs: Acton Series spectrographs, including LS785•

Multiple-camera & multiple-spectrograph control (with separate instances)•

Single-frame & sequence acquisition•

Direct stream to disk: multi-gigabyte data•

Multiple regions of interest (ROI)•

Live-frame accumulation/averaging•

Kinetics, spectra-kinetics, custom sensor modes (if applicable)•

Auto-dim monitor & auto-orientation for spectra and images•

Time stamping: track exposure start/end time & frame number•

SuperSynchro timing control•

Gate tracking: track/store gate delay & width with each frame•

Live statistics: min, max, standard deviation, center of mass•

Trigger & camera/spectrograph shutter controls•

Demo mode: simulate the performance of any supported Princeton•

Instruments camera

Spectral

Calibration

IntelliCal•**: automated point-by-point intensity & wavelength calibration

(up to 10x more accurate than standard calibration)Standard calibration: wavelength space calibration•

X-axis calibration in wavelength (nm) & wavenumbers (cm•-1)

USB-powered, NIST-traceable calibration sources•

Spectrograph alignment helper•

Step & Glue: broad wavelength range•

Peak Find•

Auto-expose•

View One-click quick view after acquisition•

Compare live & previously acquired data•

Spectral overlay•

Live auto-scale•

Zoom & pan controls•

Live X & Y cross-sections•

Full-screen mode•

Multiple-monitor support•

Option to turn off display during long acquisitions•

Separate desk copy for ofine viewing/processing of data•

Playback/review with time stamp & gate tracking information•

User

Interface

Visual status indicators: experiment progress, background/ateld•

correction on, image orientation, intensier on/off, experiment errorCustom settings dock: drag most often used settings into a separate dock•

Settings search: highlights relevant settings as you type•

Save & load multiple-user experiment settings•

Keyboard shortcuts•

Timing dashboard: visual intensier gate timing control for•

PI-MAX 3 ICCD cameras

Post-

Processing

Background, ateld correction•

Change image/spectral orientation•

Software binning•

Frame combining•

Cross-sections: X, Y & frame cross-sections (automatic “time vs. intensity”•

plot generation)

Extract data: select ROI & frame range•

Help &

Updates

Online help (F1) & PDF manual included•

Online software updates•

Field rmware updates for cameras (when available)•

Extensions

& Custom

Programming

Add-ins: customize LightField interface/operation with custom buttons, tabs,•

etc. from within LightFieldAutomation: control LightField from third-party programs (e.g., Microsoft•

Visual Basic®, National Instruments® LabVIEW®, MathWorks® MATLAB®)PICAM API: create custom acquisition programs from the ground up•

* A factory upgrade may be necessary to enable LightField compatibility for certain PI-MAX 3 cameras.** IntelliCal is an optional LightField feature.

File Formats Acquisition in Princeton Instruments SPE 3.0 format•

SPE le header contains complete experiment information (can be viewed•

in XML format)Export data to TIF (16 bits), SPC, FITS, CSV (ASCII) formats•

Automatically save raw & corrected le data•

Copy/paste image & spectral data directly into supported Microsoft•® 

Windows® programs (e.g., Notepad, Word®, Excel®)

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www.princetoninstruments.com | [email protected] +1.877.474.2286 | USA +1.609.587.9797

Copyright © 2011 Princeton Instruments, Inc. All rights reserved. 

Excel, Microsoft, Visual Basic, Windows, and Word are registeredtrademarks of Microsoft Corporation in the United States and othercountries. All other brand and product names are the trademarks orregistered trademarks of their respective owners and manufacturers.

Computer System Requirements

Supported Operating Systems:

Microsoft Windows 7 Professional& Ultimate – 64 bits

Minimum Requirements:

• 2 GHz dual-core processor• 4 GB of RAM• 2 GB of available hard-disk space required

for installation; additional hard-drive spacerequired for data acquisition/storage

• DVD drive• One or more of the following interface

ports:- USB 2.0 (for PIXIS, spectrographs,

IntelliCal light sources)- IEEE-1394a (for Quad-RO)- GigE (for ProEM, PI-MAX 3, PyLoN)

Specifcations are subject to change. Please

contact Princeton Instruments or your localPrinceton Instruments representative for thelatest information pertaining to LightField.

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