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Bintel Glebe
Usually ready for pickup in 24 hours
Bintel 84 Wentworth park road, Glebe, 2073, NSW
Phone:(02) 9518 7255
Hours:
Monday9:30 am–5:30 pm
Tuesday9:30 am–5:30 pm
Wednesday9:30 am–5:30 pm
Thursday9:30 am–5:30 pm
Friday9:30 am–5:30 pm
Saturday9:30 am–4 pm
SundayClosed
FLI Cameras
Finger Lakes Instrumentation (FLI) have a reputation for making high quality imaging equipment which include the MicroLine and ProLine cameras (available with a plethora of CCD sensors), high speed and high capacity filter wheels, and a range of high precision focusers which includes the all popular Atlas. New to the range of cameras is the Kepler series, sporting the latest in Scientific CMOS (sCMOS) sensors which are now available with large pixels, high absolute quantum efficiency, and vanishingly low read noise, the holy trinity!
9 products
9 products
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From $16,470.00
The Kepler KL400FI provides high sensitivity, ultra-low noise with high frame rates, all at a game-changing price to performance ratio. An ideal camera for those applications requiring a sensor without microlenses.
| Sensor | GSENSE400 FI |
| Diagonal Size (mm) | 31.9mm |
| Resolution | 2048x2048 |
| Pixel Size | 11um |
| Bit depth | 16-bit |
| Full Well | 120ke- |
| Read Noise | 1.5e- |
| Dark current | 0.15 EPS @ -20c |
| Shutter | Rolling |
| Peak QEÂ | 68% |
| Interface | USB 3 QSFP |
| Frame Rate | 24 FPS HDR / 48 FPS LDR |
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Optional Accessories
Quantum Efficiency
Quantum efficiency (QE) measures how effectively a detector converts incoming photons into electrons. In our graphs, QE is expressed as a percentage. A sensor’s QE typically varies based on its architecture, coatings, and materials. High QE remains a crucial consideration for applications such as astronomy, space debris imaging, and life science research.
From $20,530.00
Extreme sensitivity, including excellent QE at 240 nm, coupled with ultra-low noise make this camera ideal for challenging applications requiring high dynamic range despite short exposures at high frame rate.
| Sensor | GSENSE400 BI |
| Diagonal Size (mm) | 31.9mm |
| Resolution | 2048x2048 |
| Pixel Size | 11um |
| Bit depth | 16-bit |
| Full Well | 120ke- |
| Read Noise | 1.6e- |
| Dark current | 0.4 EPS @ -20c |
| Shutter | Rolling |
| Peak QEÂ | 95% |
| Interface | USB 3 QSFP |
| Frame Rate | 24 FPS HDR / 48 FPS LDR |
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Optional Accessories
Quantum Efficiency
Quantum efficiency (QE) measures how effectively a detector converts incoming photons into electrons. In our graphs, QE is expressed as a percentage. A sensor’s QE typically varies based on its architecture, coatings, and materials. High QE remains a crucial consideration for applications such as astronomy, space debris imaging, and life science research.
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From $25,090.00
The KL4040 shares the same large area as the KAF-16803 CCD, but with a giant improvement in throughput, substantially lower noise, and higher quantum efficiency. The KL4040 has become an industry favorite for time-resolved applications such as space domain awareness.
| Sensor | GSENSE4040 FI |
| Diagonal Size (mm) | 52.1mm |
| Resolution | 4096 x 4096 |
| Pixel Size | 9um |
| Bit depth | 16-bit |
| Full Well | 70ke- |
| Read Noise | 3.7e |
| Dark current | 0.15 EPS @ -20c |
| Shutter | Rolling |
| Peak QEÂ | 73% |
| Interface | USB 3 QSFP |
| Frame Rate | 23 FPS (QSFP) |
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Optional Accessories
Quantum Efficiency
Quantum efficiency (QE) measures how effectively a detector converts incoming photons into electrons. In our graphs, QE is expressed as a percentage. A sensor’s QE typically varies based on its architecture, coatings, and materials. High QE remains a crucial consideration for applications such as astronomy, space debris imaging, and life science research.
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From $41,660.00
For years we dreamed of a back-illuminated version of the KAF-16803 CCD – and here it is, except with high throughput and lower noise. The KL4040 BI has the high sensitivity of a CCD42-40, but with twice the area and 20% lower cost.
| Sensor | GSENSE4040 BI |
| Diagonal Size (mm) | 52.1mm |
| Resolution | 4096 x 4096 |
| Pixel Size | 9um |
| Bit depth | 16-bit |
| Full Well | 70ke- |
| Read Noise | 2.3e |
| Dark current | 0.15 EPS @ -20c |
| Shutter | Rolling |
| Peak QEÂ | 94% |
| Interface | USB 3 QSFP |
| Frame Rate | 23 FPS (QSFP) |
Optional Accessories
Quantum Efficiency
Quantum efficiency (QE) measures how effectively a detector converts incoming photons into electrons. In our graphs, QE is expressed as a percentage. A sensor’s QE typically varies based on its architecture, coatings, and materials. High QE remains a crucial consideration for applications such as astronomy, space debris imaging, and life science research.
From $56,360.00
The Kepler KL6060 FI camera delivers an expansive field of view (FOV), exceptional low-noise performance, high frame rates, and outstanding dark current specifications. As our most cost-effective large-format camera, it is perfectly suited for space domain awareness and other high-precision imaging applications that demand both reliability and performance.
| Sensor | GSENSE6060 FI |
| Diagonal Size (mm) | 83.9mm |
| Resolution | 6144 x 6144 |
| Pixel Size | 10um |
| Bit depth | 16-bit |
| Full Well | 95ke- |
| Read Noise | 4.2 e- |
| Dark current | 0.07 EPS @ -20c |
| Shutter | Rolling |
| Peak QEÂ | 73%% |
| Interface | USB 3 QSFP |
| Frame Rate | 19 FPS (QSFP) |
Optional Accessories
Quantum Efficiency
Quantum efficiency (QE) measures how effectively a detector converts incoming photons into electrons. In our graphs, QE is expressed as a percentage. A sensor’s QE typically varies based on its architecture, coatings, and materials. High QE remains a crucial consideration for applications such as astronomy, space debris imaging, and life science research.
From $143,850.00
The Kepler KL6060 BI camera features a back-illuminated sensor, offering unparalleled sensitivity for even the most challenging low-light environments. With its large field of view (FOV), low-noise performance, and high frame rates, the KL6060 BI is ideal for Space Domain Awareness and other critical low-light imaging applications, where both reliability and performance are paramount.
| Sensor | GSENSE6060 BI |
| Diagonal Size (mm) | 83.9mm |
| Resolution | 6144 x 6144 |
| Pixel Size | 10um |
| Bit depth | 16-bit |
| Full Well | 95ke- |
| Read Noise | 3.0 e- |
| Dark current | 0.1 EPS @ -20c |
| Shutter | Rolling |
| Peak QEÂ | 95% |
| Interface | USB 3 QSFP |
| Frame Rate | 11 FPS (QSFP) |
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Optional Accessories
Quantum Efficiency
Quantum efficiency (QE) measures how effectively a detector converts incoming photons into electrons. In our graphs, QE is expressed as a percentage. A sensor’s QE typically varies based on its architecture, coatings, and materials. High QE remains a crucial consideration for applications such as astronomy, space debris imaging, and life science research.
$8,439.00
Designed and manufactured in the USA with same extreme reliability as the thousands of FLI OEM cameras. Install in remote observatories around the world with complete confidence in a long, trouble-free life. High sensitivity CMOS camera with 90% quantum efficiency and 15.9 mm diagonal field of view is an ideal replacement for 1" format CCDs.
| Sensor | IMX533 |
| Diagonal Size (mm) | 16mm |
| Resolution | 3003 x 3003 |
| Pixel Size | 3.76um |
| Bit depth | 14-bit |
| Full Well | 50ke- |
| Read Noise | 1e- |
| Dark current | 0.002 EPS @ -20c |
| Shutter | Rolling |
| Peak QEÂ | 91%% |
| Interface | USB 3 QSFP |
| Frame Rate | 20FPS |
Optional Accessories
Quantum Efficiency
Quantum efficiency (QE) measures how effectively a detector converts incoming photons into electrons. In our graphs, QE is expressed as a percentage. A sensor’s QE typically varies based on its architecture, coatings, and materials. High QE remains a crucial consideration for applications such as astronomy, space debris imaging, and life science research.
$9,749.00
Designed and manufactured in the USA with same extreme reliability as the thousands of FLI OEM cameras. Install in remote observatories around the world with complete confidence in a long, trouble-free life. High sensitivity with exceptionally low noise and dark current. Great combination of resolution and frame rate.
| Sensor | IMX571 |
| Diagonal Size (mm) | 28.2 |
| Resolution | 6244 x 4168 |
| Pixel Size | 3.76um |
| Bit depth | 15-bit |
| Full Well | 50ke- |
| Read Noise | 1e- |
| Dark current | 0.002 EPS @ -20c |
| Shutter | Rolling |
| Peak QEÂ | 91%% |
| Interface | USB 3 QSFP |
| Frame Rate | 7FPS |
Optional Accessories
Quantum Efficiency
Quantum efficiency (QE) measures how effectively a detector converts incoming photons into electrons. In our graphs, QE is expressed as a percentage. A sensor’s QE typically varies based on its architecture, coatings, and materials. High QE remains a crucial consideration for applications such as astronomy, space debris imaging, and life science research.
$14,699.00
Designed and manufactured in the USA with same extreme reliability as the thousands of FLI OEM cameras. Install in remote observatories around the world with complete confidence in a long, trouble-free life. Full frame sensor with 90% quantum efficiency and massive 43.1mm diagonal field of view to increase throughput.
| Sensor | IMX455 |
| Diagonal Size (mm) | 43.2 |
| Resolution | 9568 x 6300 |
| Pixel Size | 3.76um |
| Bit depth | 16-BIT |
| Full Well | 50ke- |
| Read Noise | 1e- |
| Dark current | 0.002 EPS @ -20C |
| Shutter | Rolling |
| Peak QEÂ | 91% |
| Interface | USB 3 QSFP |
| Frame Rate | 4FPS |
Optional Accessories
Quantum Efficiency
Quantum efficiency (QE) measures how effectively a detector converts incoming photons into electrons. In our graphs, QE is expressed as a percentage. A sensor’s QE typically varies based on its architecture, coatings, and materials. High QE remains a crucial consideration for applications such as astronomy, space debris imaging, and life science research.
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