Microline 16200

16 Megapixel Sensor. 6 Micron Pixels. Sensor Diagonal 34.5mm. Peak QE ~ 60 Percent. Full Well Capacity 39000 Two Readout Speeds. 6 Electrons Readoutnoise at 8 Sec. Downloadspeed. 11.5 Electrons Readoutnoise at 1.5 Sec. Downloadspeed. Cooling 55 Degrees Below Ambient.

Microline 16200

Compact Form Factor. Works with 50mm Diameter Filters. Low Dark Shot Noise Trough Deep Cooling. RBI Flood. Almost Twice The Dynamic Range Compared To The Usual 10 Electron Readout Noise Cameras.

Microline 16200

7 Minutes Red Exposure, No Calibration

Microline 16200

7 Minutes Luminance Exposure, No Calibration

Microline 16200

Bias Frame -35°

Dark Frame 7 Min. -35°

Microline 16200

RGB 60 60 60

Microline 16200

SII Ha OIII 60 60 60 Bin 2x2

Microline 50100

50 Megapixel Sensor. 6 Micron Pixels. Sensor Diagonal 61.2mm. Peak QE ~ 63 Percent. Full Well Capacity 40300 Two Channel Readout. 10 Electrons Readoutnoise at 3.2 Sec. Downloadspeed. RBI Flood. Cooling 45 Degrees Below Ambient.

Microline 50100

Calibrated

7 Min Luminance Uncalibrated

Microline 50100

Dark Frame 15 Min. -30° RBI Flood

Bias Frame -30°

Microline 50100

LRGB 120 40 40 40

LRGB 120 40 40 40

Microline 50100

SII Ha OII 90 120 90

Thank You

FIGURE OF MERITFINGER LAKES INSTRUMENTATION

A COMPREHENSIVE MEASUREMENT OF SENSITIVITY (QE)

BASED ON QUANTUM EFFICIENCY, 360 NM - 1000 NM

Finger Lakes Instrumentation Figure of Merit

360-1000 nm

Blue 360-520 nm

Green 480-600 nm

Red 600-700 nm

NIR 700-1000

nme2v DD 2753 765 624 551 1264e2v BB 2509 671 586 472 742

e2v MB 2210 607 638 541 842

Kepler KL400 2196 673 654 538 784

KAF-3200 1784 496 506 482 644

e2v UV 1771 541 458 391 704KAF-1001 1510 368 406 380 625

KAF-4320 1504 360 400 383 622

KAF-09000 1464 417 446 363 537

Kepler KL2020 1369 357 406 440 452

KAF-16801 1263 315 358 380 466KAF-50100 1243 419 411 305 381

KAF-6303 1237 323 382 374 459

KAF-16803 1212 406 401 292 379

KAF-16200 1161 291 386 387 353

KAF-8300 1133 382 371 285 343KAI-04070 892 400 339 211 166

KAI-16070 860 394 328 188 164

KAI-11002 829 399 314 182 142

KAI-08670 828 389 315 181 150

KAI-16050 700 328 287 153 123

KAI-29050 698 328 287 152 122

FIGURE OF MERITFINGER LAKES INSTRUMENTATION

A COMPREHENSIVE MEASUREMENT OF SENSITIVITY (QE)

NEW CAMERASFINGER LAKES INSTRUMENTATION

PRODUCT OVERVIEW

COBALT LARGE FORMAT CAMERA LINE NEW!

Cobalt Cameras:

• Large format CCDs • Advanced high-powered cooling system • 4-point Optical Correction System

• 1 degree tip/tilt • Shipped: +/- 0.1mm

• 90mm shutter standard • Optional 110mm high-speed shutter

COBALT LARGE FORMAT CAMERA SHIPPING!

DC4320 with ON Semi KAF-4320:

• 2k x 2k • 24 micron pixels • 65 Deg C cooling • 4 channel output • 70mm diagonal • 72% peak QE • 500,000 e- full well capacity

• Price Range: $35995 - $52995 (+/- 90mm shutter, Grade 1 or 2)

Ideal for Long Focal Length Telescopes

COBALT LARGE FORMAT CAMERA EXCELLENT QE

DC4320 with ON Semi KAF-4320:

• 2k x 2k, 24 micron pixels • 65 Deg C cooling • 70mm diagonal • 72% Peak QE • 4 channel output • 4-point Optical Correction

• 1 degree tip/tilt • Shipped: +/- 0.1mm

• Price Range: $35995 - $52995 (+/- 90mm shutter, Grade 1 or 2)

KAF-4320: Figure of Merit rating 1504 KAF-16803: Figure of Merit rating 1212

COBALT LARGE FORMAT CAMERA HIGHEST QE

DC23084 with e2v CCD230-84:

• 4k x 4k • 5 micron pixels • 60 Deg C cooling • 4 channel output • 4-point Optical Correction

• 1 degree tip/tilt • Shipped: +/- 0.1mm

Price Range: $ 185,000 2k x 2k available @ $50,000, 70 Deg C cooling

CCD230-84: Figure of Merit rating 2210 KAF-16803: Figure of Merit rating 1212

93% PEAK QE, 87mm Diagonal

KEPLER CAMERA HIGH-SPEED CAMERA LINE NEW!

Kepler Cameras:

• CMOS, Scientific CMOS, and Interline sensors • Air & Liquid Cooled standard • Modular design with user replaceable

• Shutter Assembly

• Cooling Fan

• Camera Power Board

• Lightweight & Compact Design • USB 3.0 Standard • SFP and QSFP Fiber Interfaces (optional)

SFP = Small Form-factor Pluggable

KEPLER SCMOS CAMERA NEW CAMERA

KL400 Cooled sCMOS Camera: • 2k x 2k • 11 micron pixels • 32mm diagonal • Up to 48 fps • 89000 e- full well • USB 3.0 connectivity • Three mode design

• High Gain • Low Gain • High Dynamic Range (96 DB)

• 24 frames per second, HD mode • 48 frames per second, high or low gain mode

95% PEAK QE 1.2 e- read noise

96 dB dynamic range

Kepler KL400: Figure of Merit rating 2196

KEPLER SCMOS CAMERAS

KL400 Cooled sCMOS:

• 2k x 2k • 11 micron pixels • 32mm diagonal • Up to 48 fps • 89000 e- full well • 95% QE • 1.2 e- read noise • 96 dB dynamic range

• Price Range: $19,000

95% PEAK QE, 1.2 e- read noise, 96 dB dynamic range

SFP = Small Form factor Pluggable

KEPLER SCMOS CAMERAS NEW CAMERA

KL2020 Cooled sCMOS Camera:

• 2k x 2k • 6.5 micron pixels • 18.8 mm diagonal • 48000 e- full well • USB 3.0 • SFP and QSFP Fiber Interfaces (optional)

• Price Range: $12,000

2.0 e- read noise 376 frames per sec

COMING SOON:

New FLI web site with:

QE Tool

Back-Focus Calculator

Figure of Merit Comparator

A SPECIAL THANK YOU TO GERALD RHEMANN

(COMET IMAGE)

Congratulations to TRAPPIST South Observatory Seven Earth-Like Planets Discovered!

TRAPPIST used a Back-Illuminated ProLine for the Initial Discovery May 20, 2016

ThankYou!

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Sinai School of Medicine · NASA Ames · NASA Goddard · NASA Johnson · National Astronomical Observatories of China · National Astronomical Research Institute of Thailand/NARIT · National Institute of Aeronautics and Space (Indonesia) · National Institute of Health · National Renewable Energy Laboratory · National Taiwan University · National University of Ireland · Nauchny Observatory (Ukraine) · Naval Ordnance Test Unit · Naval Research Laboratory · New Mexico State University · New Mexico Tech · New York State Dept. of Health · New York University · Nikon · NIST · Northrop Grumman · Northwestern Polytechnical University (China) · Northwestern University · Novosibirsk State University (Russia) · Observatoire de Oukaimeden (Morocco) · Observatorio Astronomico Nacional (Bolivia) · Observatory Hamburg (Germany) · Olympus · Oxford University (UK) · Palomar Observatory · Paul Scherrer Institute (Switzerland) · Pennsylvania State University · Physical Research Lab (India) · Pontifi cia Universidad Catolica de Chile · Princeton University · Pulkova Observatory (Russia) · Purdue University · Purple Mountain Observatory (China) · Qatar Foundation · Raytheon · Reial Academia de Ciencies i Arts de Barcelona (Spain) · Rheinisch-Westfaelische Technische Hochschule (Germany) · Rochester Institute of Technology · Royal Melbourne Institute of Technology (Australia) · Sandia National Laboratories · Sanglok Observatory (Tajikistan) · Scripps Research Institute · Seoul National University (South Korea) · SETI Institute · Shan Dong University (China) · Shanghai Institute of Technical Physics (China) · Shanghai Observatory (China) · Shumen University (Bulgaria) · Siding Spring Observatory (Australia) · Siemens · Simon Fraser University (Canada) · SLAC National Accelerator Laboratory · South African Large Telescope (SALT) · St. Francis Xavier University (Canada) · Stanford University · STFC (UK) · Sydney University (Australia) · Tarleton University · Technical Universities of Darmstadt, Dresden, and Ilmenau (Germany) · Technion University (Israel) · Tel Aviv University (Israel) · Tenagra Observatories · Terskol Observatory (Russia) · Texas A&M University · Texas State University · The Ohio State University · Tiraspol Observatory (Moldova) · Tubitak National Observatory (Turkey) · Turksat University (Turkey) · Tuskegee University · Universidad Nacional Autónoma de México · Universidad Nacional de La Plata (Argentina) · Universita di Roma (Italy) · Universitat de Barcelona (Spain) · Universitat de Valencia (Spain) · Université de Montreal (Canada) · Universiteit Leiden (Netherlands) · Universities of Alabama, Alaska, Arizona, California, Central Florida, Chicago, Hawaii, Illinois, Iowa, Kentucky, Maryland, Massachusetts, Minnesota, Nevada, New Mexico, North Carolina, North Dakota, Notre Dame, Pittsburgh, Rochester, South Carolina, Texas, Virginia, Washington, and Wisconsin · Universities of Bremen, Duisburg, Freiburg, Göttingen, Heidelberg, Kiel, Konstanz, Magdeburg, Potsdam, and Würzburg (Germany) · University College Dublin (Ireland) · University Observatory Munich (Germany) · University of Bern (Switzerland) · University of Bradford (UK) · University of Calgary (Canada) · University of Dresden (Germany) · University of Jena (Germany) · University of Lethbridge (Canada) · University of Munich (Germany) · University of the Pacifi c · University of Quebec at Montreal, UQAM (Canada) · University of Newcastle (UK) · University of Queensland (Australia) · University of Toronto (Canada) · University of the Virgin Islands · University of Warwick (UK) · University of Western Australia · University of Western Ontario (Canada) · Upice Observatory (Czech Republic) · UPJS Institute of Physics (Slovakia) · US National Park Service · Ussurijsk Observatory (Russia) · Utah State University · Uzhgorod Observatory (Ukraine) · VA Hospital San Francisco · Victoria University of Wellington (New Zealand) · Virginia Tech · Washington and Lee University · Washington University in St. Louis · Wayne State University · Western Kentucky University · Wheaton College · Whitehead Institute of Biomedical Research · Whitman College · Williams College · Xi’an Institute of Optics and Precision Mechanics of CAS (XIOPM) · Xi’an University of Technology (China) · Xidian University (China) · Yale University · YBJ Observatory (Tibet) · Yunnan Observatory (China) · Zvenigorod Observatory (Russia)

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