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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
Research Grade Cameras
Discover our range of professional imaging systems from SBIG, FLI, ATIK, QSI, QHY, and ZWO. Designed for precision, sensitivity, and unmatched image quality, these cameras meet the exacting demands of scientific research, astrophotography, and observatory installations. From capturing faint galaxies to recording high-resolution planetary details, they deliver the performance required for serious data collection and produce images that both captivate and educate.
Not sure which camera is right for your needs? Our team has extensive experience with research and educational imaging projects, and we’re here to help you choose the ideal system for your observatory, school, or program.
18 products
18 products
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$6,499.00
In two decades, much has changed beyond recognition. Sensors are now back-illuminated CMOS with native 16-bit digitisation. QE is an amazing 90% and readout is a speedy 120 million pixels per second over USB3, a performance that once was unimaginable. What is maintained by QSI’s newest cameras is the integrated design, attention to detail, and bulletproof reliability.
In the design of the 700 series we have taken our best technology. Filterwheels are mechanically indexed to ensure the most precise location for perfect flat fields. The fused silica window is dew resistant and is coated on both sides with high transmission anti-reflective coating to minimise halos. The cameras use a highly efficient 2-stage Peltier cooler that draws less current and delivers more cooling than some other cameras.
The QSI 726 is the optimum camera for most amateur telescopes. The
28mm diagonal IMX571 maximises the sharpest parts of a telescope’s
image and is less affected by coma and vignetting than larger sensors.
As with its bigger brother the 760, cable clutter is reduced thanks to
the integrated filter wheel (36mm), 2 USB2 in sockets and power out.
Power sockets have threaded connections for maximum reliability.
| Image Sensor | Sony IMX455 mono CMOS sensor | Sony IMX571 mono CMOS sensor |
| Resolution | 9576 × 6380 | 6244 × 4168 |
| Pixel Pitch | 3.76 um | 3.76 um |
| Sensor Size | 43.3mm diagonal (36mm x 24mm) | 28.3mm diagonal |
| Full Well | 51,000 e- | 51,000 e- |
| Read Noise | 1.2 e- | 1.7 e- (typical) |
| Set Point Cooling at ambient of 20 C | -25 °C | -25°C |
| Frame Rate | 2 FPS (Full Frame image) | 4FPS (Full Frame image) |
| Mount Type | M54 × 0.75 | M54 × 0.75 |
| ADC | 16 bit | 16 bit |
| Backfocus Distance | 31 mm | 31 mm |
| Reading Mode | Rolling shutter | Rolling shutter |
| Exposure Range | 1 ms - 24 hours | 1 ms - 24 hours |
| Dark Current | 0.005 e-/p/s | 0.0008 e-/p/s |
| Filter Wheel Mechanical indexing for reproducible flats | Filterwheel for 2" or unmounted filters, 5 or 7 position | 50mm/ 36mm filters |
| Accessories | Off-Axis guide unit | Off-Axis guide unit |
| Computer System | Windows 10+ Linux USB 3.0 8GB | Windows 10+ Linux USB 3.0 8GB |
| Requirements | Ram 64 bit Operating System. | Ram 64 bit Operating System |
ZWO ASI461MM-Pro采用索尼中画幅IMX461传感器,原生16位65536级ADC,背照式结构,量子效率高,深空成像性能优异,银河系成像、科学研究。
其特点是读出噪声非常低,并且可见的固定模式噪声几乎为零。
100 万像素,分辨率为 11656 x 8750。3.76 微米像素可容纳令人印象深刻的 50.3ke 满阱容量。而在 Bin2 模式下,您可以获得更大的 198e 满阱容量和 7.5um x 7.5um 的大像素尺寸。
ASI461MM-Pro 是一款 100MP 相机,具有 44mm x 33mm 的大传感器尺寸和高分辨率
注意:所有 ASI 冷却相机都需要外部电源。我们建议您使用 12v@3amp DC 适配器(5.5 x 21. 中心极正极)
无放大器辉光
传统 CMOS 传感器在工作时会产生微弱的红外光源,这在未校准图像的角落中经常可见。这是“安培辉光”的明显迹象。由于 ASI 4612MM-Pro 使用零安培辉光电路,因此即使在使用高增益、长曝光成像时也不必担心安培辉光。
防露
ASI461MM-Pro 配有聚酰亚胺加热元件,位于保护窗顶部。它将加热保护窗以避免结露问题。
加热器的功耗约为 5W。如果您想节省电量,可以在成像软件中关闭此功能。
相机性能
HCG模式
ASI461MM-Pro集成了HCG模式,当您使用较高增益时,可以帮助您大大降低读出噪声并保持动态范围处于高水平。
设置增益100,则自动开启HCG模式,读出噪声可以很低,而动态范围基本不变。
量子效率
QE 曲线和读出噪声是衡量相机性能的两个最重要的因素。根据我们的计算,ASI461MM-P 的 QE 峰值在 460nm 处为 91%
绝对量子效率
相对量子效率
两级 TEC 冷却
ASI461MM-Pro 的 TEC 冷却系统可以精确控制传感器的温度,并将其降低到低于环境温度 30 – 35 摄氏度
商品详情
与外部设备的连接
结构尺寸
型号:ASI461MM-Pro
$7,499.00
Atik 16200 单色相机是围绕 KAF-16200 传感器全新设计的。这款相机的对角线长度为 35 毫米(APS-H 格式),像素为 6 微米,是高分辨率和传感器空间的完美结合。
它与一系列望远镜完美匹配,而且价格比基于 KAF-11002 和 KAF-16803 的相机更实惠。
该设计将 CCD 置于密封的氩气吹扫室中,并辅以强大的双级珀耳帖和散热器以实现最佳冷却效果。这款相机的温差是 Atik 相机中最低的,典型温度为 -45°C,最高温度为 -50°C。
Atik 16200 单色技术规格
- 传感器类型:CCD - KAF-16200
- 水平分辨率:4499像素
- 垂直分辨率:3599像素
- 像素尺寸:6 µm x 6 µm
- ADC:16位
- 读出噪声:9e-典型值
- 增益系数:0.6e-/ ADU
- 满井:~40,000e-
- 暗电流:0°C 时 >0.25 电子/秒
- 接口:USB 2.0 高速
- 电源:12V DC 2.5A
- 最大曝光长度:无限制
- 最短曝光长度:200 毫秒
- 冷却:热电设定点最大ΔT=>-50°C(典型值-45°C)
- 重量:约1.3公斤
- 后焦距:±19.5 毫米
- 有单色和彩色两种版本可供选择,彩色版本将于 2017 年初推出
多种读数模式
多种读出模式是QHY 16位相机(QHY600/268/461/411)独有的,不同的读出模式驱动时序等不同,导致性能不同,详见“多种读出模式及曲线”部分。
随机变化热噪声抑制功能
在一些背照式CMOS相机中,你可能会发现某些类型的热噪声会随时间而变化。这种热噪声具有典型热噪声固定位置的特点,但其大小与曝光时间无关,而是每一帧都呈现出自己的特点。QHY600/268/461/411采用了创新的抑制技术,可以显著降低此类噪声的表观水平。
UVLO 保护
UVLO(欠压锁定)是为了保护电子设备免受异常低电压造成的损坏。
日常生活经验告诉我们,电器的实际工作电压不能明显超过额定电压,否则会损坏。对于相机这种精密设备,长期在过低的输入电压下工作也会对相机的工作寿命不利,甚至会使电源管理器等器件因长期过载而烧毁。在2021.10.23稳定版之后的一体机驱动和SDK中,当相机输入电压低于11V时,相机会发出警告。
优化 USB 流量以最大程度减少水平条带
CMOS 传感器包含一些水平条带是常见现象。通常,随机水平条带可以通过多帧堆叠去除,因此不会影响最终图像。但是,周期性水平条带无法通过堆叠去除,因此可能会出现在最终图像中。通过在单帧模式或实时帧模式下调整 USB 流量,您可以调整 CMOS 传感器驱动程序的频率,并且可以优化图像上出现的水平条带。这种优化对于在某些情况下去除周期性条带非常有效。
特定 USB_TRAFFIC 值下的典型周期性水平噪声。
调整 USB 流量以避免周期性的水平噪声。
关闭并重新打开电源,重新启动相机
相机设计为使用 +12V 重新启动相机,而无需断开和重新连接 USB 接口。这意味着您只需关闭 +12V 然后重新打开电源即可重新启动相机。此功能对于在天文台远程控制相机非常方便。您可以使用远程控制电源重新启动相机。在远程控制的情况下,无需考虑如何重新连接 USB。
规格
| 模型 | QHY461PH |
| 图像传感器 | SONY IMX461 BSI CMOS 传感器 |
| 像素大小 | 3.76微米×3.76微米 |
| 彩色 / 单色版本 | 仅限单声道 |
| 图像分辨率 | 11760 × 8896 |
| 有效像素 | 102 万像素 |
| 有效图像区域 | 44 毫米 x 33 毫米 |
| 传感器表面玻璃 | AR+AR 多层镀膜透明玻璃 |
| 全井容量(1×1、2×2、3×3) | 标准模式下 50ke- / 200ke- / 450ke- 扩展满阱模式下 80ke- / 320ke- / 720ke- |
| 广告 | 1X1Binning 为 16 位(0-65535 灰度),2X2 为 18 位,3X3 为 19 位,4*4 软件 Binning 为 20 位 |
| 传感器尺寸 | 典型 3.4 英寸 |
| 读出噪音 | 1e 至 3.7e(HGC 模式下) |
| 暗电流 | 约 0.003e/像素/秒 @ -20C |
| 曝光时间范围 | 50微秒 – 3600秒 |
| 帧速率 | USB3.0上2.7FPS@8BIT 1.3FPS@16BIT 10Gb 光纤上 2.7FPS @ 16BIT 6FPS @ 14BIT |
| 快门类型 | 电动卷帘门 |
| 计算机接口 | USB3.0 |
| 滤光轮接口 | 4PIN QHYCCD CFW 接口 |
| 内置图像缓冲区 | 1GByte DDR3 缓冲器 |
| 冷却系统 | 双级 TEC 冷却器(采用空气冷却,温度低于环境温度-35C)。 |
| 防露加热器 | 是的 |
| 望远镜接口 | – |
| 光学窗口类型 | AR+AR 高品质多层防反射涂层 |
| 后焦距 | 32.5 毫米 |
相机曲线
$26,424.00
Our high performance Aluma® CCD Series cameras offer capabilities and features not available in any other scientific-grade imaging camera. This lightweight (2.2 lbs) and compact (4.5″ x 4.5″ x 4″ with handles) camera includes two-stage cooling, USB 2.0 interface, ultra-reliable even-illumination shutter, and fast low-noise readout.
The Aluma CCD series supports a wide range of accessories, including the 8-position AFW-8-36R filter wheel.
The Aluma CCD77-00 has an extremely high sensitivity, 260,000 pixel back-illuminated CCD sensor with 24 micron pixels. These are research-grade cameras designed for longer focal length instruments typically with apertures greater than 40 cm.
Aluma CCD is a new generation of research cameras tuned for even better performance. Over two years of collaboration with university researchers helped us bring you an enhanced new Aluma CCD series that represent the ultimate in a high-performance mid-sized 16-bit CCD detector. Using E2V’s best-in-class research grade back-illuminated sensors, the Aluma CCD77-00 gives you the high sensitivity, low noise, and high well depth needed for the most demanding research applications.
Aluma CCD Features include:
- High-performance CCD imaging sensors currently manufactured by SONY and Teledyne E2V
- Light weight, compact design
- Centered optical axis for optimum instrument balance
- Ultra reliable even-illumination (photometric) mechanical shutter
- USB 2.0 interface
- Full frame image buffering eliminates readout artifacts
- 2-Stage TE cooling with typical -50C from ambient
- Twin variable speed fans with SmartCoolingTM technology
- High accuracy temperature regulation
- Built-in RBI Pre-flash (full frame front-illuminated sensors only)
- External TTL trigger inputs and output
- Included 110V / 220V power supply and optional 12VDC operation
- User-rechargeable desiccant plug
- Built-in 1/4-20 tripod mount
- Support for high precision 8-position filter wheels
- Bulletproof firmware update capability – virtually impossible to “brick”
Software Included
All Aluma CCD models ship with MaxIm LT for Windows – a special version of MaxIm DL specific to our cameras. Aluma CCD also supports third-party applications through ASCOM and native drivers.
Compact and Lightweight Design
Aluma CCD cameras measure just 4.25″ x 4.25″ x 4.0″ with handles (3.5″ without handles) and weigh just 2.2 lbs (1 kg).
Even-Illumination Shutter
All Aluma CCD cameras include a mechanical shutter, which is used for both dark/bias calibration frames and for shuttering exposures on full frame sensors. Rather than using a complex iris shutter, which are prone to failure, the Aluma CCD uses a twin vane shutter and direct drive motor for high repeatability, reliability, and extremely long life. The shutter is designed to be “even illumination” for the best accuracy in photometric measurements.
Extreme Sensitivity CCD 77-00 Image Sensor
The Aluma CCD77-00 uses the 0.26 megapixel E2V CCD 77-00 sensor, featuring peak quantum efficiency (QE) of 93% with midband coatings. This full frame, back-illuminated sensor is designed for the ultimate in sensitivity. We offer Midband coating for the highest quantum efficiency. Other coatings are available on special order.
CCD 77-00 Quantum Efficiency Curves The CCD 77-00 has 512 x 512 pixels at 24 microns square, for a 12.3 mm square chip size. This back-illuminated full-frame CCD sensor has extremely low noise and extremely high sensitivity. Combining this high-performance sensor with Aluma CCD’s high cooling performance and low readout noise results in exceptionally clean images. SmartCoolingTM
All Aluma CCD cameras include our powerful new SmartCooling technology. The two-stage cooler, powerful fans, and advanced heat sink designed using thermal flow simulation combine to produce typical cooling delta from ambient of -50C. This is quite a feat considering the Aluma CCD’s very compact and lightweight package. SmartCooling automatically adjusts the fan speed to optimize cooler performance and power consumption. The camera’s firmware is constantly monitoring the sensor and heat sink temperatures, as well as controlling the cooler power. When full cooling power is needed – when ramping down or running near full power – the fans ramp up to their maximum speed, resulting in the strongest possible cooling. When less cooling power is needed the fans automatically slow to reduce noise levels and power consumption. SmartCooling also prevents any possibility of overheating by backing off power if the heat sink gets too hot – so you don’t need to worry if your camera is baking in a hot observatory during the day. Advanced Software Included
All Aluma CCD cameras come with our MaxIm LT software – a $249 value! MaxIm LT is a special version of our venerable MaxIm DL software that provides complete control of your camera, filter wheel, and autoguider, plus advanced image processing capabilities. If you wish you can upgrade to MaxIm DL Pro to get complete observatory integration and even more processing and analysis capabilities. Included Accessories Each Aluma CCD camera package includes: Optional Filter Wheel
The optional AFW-8-36R 8-position filter wheel provides a fast, quiet, and low-cost option. It holds standard 36 mm filters, and inserts are available for 1-1/4″ filters, which are suitable for smaller format CCD sensors. The optional AFW-16-36R filter wheel, attached via AFW to Small Format Camera Adapter, provides for a full sixteen 36 mm filters. Please note that the AFW wheels work with large format accessories, and do not accommodate screw-in 1-1/4″ filters due to their height.
Antiblooming
n
Binning Modes
Horizontal 1, 2, 3, 4; Vertical 1-255
Computer Interface
USB 2.0
Cooling Delta
50 °C
Exposure
0.12-3600 sec
Filter Size
36mm / 1.25"
Filter Wheel Option
y
Full Well Capacity
300,000 e-
Imaging / Pixel Array
512 x 512
OAG Option
StarChaser
Peak QE
93%
Pixel Digitization Rate
1 MPix/sec
Pixel Size
24 μm
Power
12 VDC, 5A max
Shutter
Mechanical, Even-illumination
Temperature Regulation
y
Total Pixels
262,000 pixels
Weight
0.997kg (2.2 lbs)
$8,899.00
我们全新的高性能 SBIG Aluma CCD 814 相机提供其他任何科学级成像相机所不具备的功能和特性。这款轻巧(1 公斤)且紧凑(带手柄时尺寸为 114 毫米 x 114 毫米 x 102 毫米)的相机包括两级冷却、USB 2.0 接口、超可靠的均匀照明快门和快速低噪声读出。
SBIG Aluma CCD 814 支持多种配件,包括具有微米级滤光片定位的 8 位 FW8S-Aluma 滤光轮、StarChaser SC-2 离轴导星相机和 AO-8A 自适应光学配件。
SBIG Aluma CCD 814 具有高灵敏度、低噪声的 9 百万像素 CCD 传感器,像素为 3.69 微米。它非常适合拍摄高空间分辨率、长时间曝光且安培辉光、暗电流和噪声最小的照片。它还具有执行高比率模拟合并的能力,这对于光谱学等应用非常重要。
SBIG Aluma CCD 814 是新一代研究相机,性能更佳。经过两年多与大学研究人员的合作,我们为您带来了增强型全新 Aluma CCD 系列,该系列代表了高性能中型 16 位 CCD 探测器的最佳价值。我们精心改进了相机电子设备,以提高性能、降低安培辉光和降低噪音。使用索尼一流的 CCD,您将获得具有 CMOS 技术灵敏度的 CCD 的精确和超清晰图像。
Aluma CCD814 – 令人难以置信的灵敏度
ICX-814 CCD 是迄今为止最好的光学传感器之一,峰值量子效率超过 75%,光谱灵敏度非常宽,蓝色灵敏度极高。它还具有非常低的读取噪声、大动态范围和极低的暗电流。高灵敏度和极低噪声的结合意味着您可以更快地获得更清晰、更深的图像。
- 目前由 SONY 和 Teledyne E2V 生产的高性能 CCD 图像传感器
- 轻巧、紧凑的设计
- 居中光轴,实现最佳仪器平衡
- 超可靠的均匀照明(光度测定)机械快门
- USB 2.0 接口
- 全帧图像缓冲消除了读出伪影
- 2 级 TE 冷却,典型温度比环境温度低 50°C
- 采用 SmartCooling TM技术的双变速风扇
- 高精度温度调节
- 内置 RBI 预闪光(仅限全画幅前照式传感器)
- 外部 TTL 触发输入和输出
- 包含 110V / 220V 电源和可选 12VDC 操作
- 用户可充电干燥剂插头
- 内置 1/4-20 三脚架接口
- 支持高精度8位滤光轮
- 与 StarChaser SC-2 离轴导星相机和 AO-8A 自适应光学系统配合使用
- 坚固的固件更新能力——几乎不可能“变砖”
包含高级软件
所有 Aluma CCD 型号均配备适用于 Windows 的 MaxIm LT - 这是我们相机专用的MaxIm DL特殊版本。Aluma CCD 还通过 ASCOM 和原生驱动程序支持第三方应用程序。
紧凑轻巧的设计
Aluma CCD 相机尺寸仅为 114mm x 114mm x 102mm(带手柄)(不带手柄为 89mm),重量仅为 1 千克(2.2 磅)。
机械快门
SBIG Aluma CCD 814 具有电子快门功能,最小曝光时间仅为 0.001 秒。此外,它还具有高可靠性机械快门,有助于实现准确的暗/偏置校准帧。
高性能 ICX-814 图像传感器
SBIG Aluma CCD 814 采用广受欢迎的 900 万像素 SONY ICX-814ALG 传感器。该传感器像素为 3388 x 2712,面积为 3.69 微米见方,芯片尺寸为 12.48 毫米 x 9.98 毫米。
这是一款高灵敏度的隔行 CCD 传感器,具有极低的暗电流和极低的读取噪声。这款高性能传感器与 Aluma CCD 的高冷却性能和低读取噪声相结合,可产生异常清晰的图像。
该传感器采用微透镜技术,可将光线集中在每个像素的敏感区域上。CCD 的灵敏度在可见光谱中心 550 nm 处达到峰值,并在整个可见光谱范围内保持高灵敏度。与市场上的其他传感器相比,ICX-814 在蓝色方面表现尤为出色。
智能冷却技术
所有 Aluma CCD 相机均采用我们强大的全新 SmartCooling 技术。两级冷却器、强大的风扇和使用热流模拟设计的先进散热器相结合,可在环境温度为 -50C 时产生典型的冷却增量。考虑到 Aluma CCD 非常紧凑和轻巧的封装,这真是一项了不起的成就。
SmartCooling 可自动调节风扇速度,以优化冷却器性能和功耗。相机固件会持续监控传感器和散热器温度并控制冷却器功率。当需要全功率冷却时(当功率降低或接近全功率运行时),风扇会加速至最大速度,从而实现最强的冷却效果。当需要的冷却功率较低时,风扇会自动减速以降低噪音水平和功耗。如果散热器过热,SmartCooling 还会通过切断电源来防止过热的可能性,因此您无需担心相机在白天是否被置于炎热的天文台中。
包含高级软件
所有 SBIG 相机均配备我们的 MaxIm LT 软件 - 价值 200 美元!MaxIm LT 是我们备受推崇的 MaxIm DL 软件的一个特殊版本,可完全控制您的相机、滤光轮和自动导星器,以及高级图像处理功能。如果您愿意,可以升级到 MaxIm DL Pro,以获得完整的天文台集成以及更多的处理和分析功能。
附带配件
每个 Aluma CCD 相机套件包括:
- MaxIm LT 软件 – 请使用此表单申请您的许可证
- 豪华手提箱
- 通用电源(110V / 220V,50-60 Hz)
- 2英寸鼻托适配器
- 包含软件、驱动程序和文档的 USB 闪存盘
- 15 英尺(4.5 米)USB 线缆
可选的 FW8S-Aluma 8 位滤光轮包含正定心机制,每次都能精确地将每个滤光片置于完全相同的位置。这种单像素精度完全消除了平场后的灰尘点和其他伪影的重影。
正向定位机制提供单像素滤波器位置精度
精密平场定位和超精确索引
左上图显示滤镜上有灰尘点。拍摄平场校准帧,然后滤镜轮旋转几次,然后拍摄第二张经过平场校准的照片(右上图)。没有看到灰尘点的痕迹。这种高精度可产生最高质量的图像和出色的光度测量精度。
Aluma 轮可容纳标准 36 毫米滤镜,并提供 1-1/4 英寸滤镜插件,适用于较小格式的 CCD 传感器。
Aluma 滤光轮取代了相机的前板,从而最大限度地减少了后焦,确保相机/滤光轮组合能够在尽可能广泛的光学系统上达到聚焦。
对于天文成像,Aluma CCD 系列可与StarChaser SC-2离轴导星相机配合使用。这可提供可靠的导星,不受光学系统弯曲的影响。它还支持可选的 AO-8A 自适应光学附件的操作。
所有 Aluma CCD 型号均可与 AO-8A 自适应光学附件配合使用。AO-8A 使用倾斜窗口来快速精确地调整图像位置以响应自动导星器反馈。使用自适应光学系统不会出现间隙、粘滞或滞后,并且移动非常精确和准确。这使得 AO-8A 不仅可以消除周期性误差、漂移和阵风的影响,还可以减少大气视宁度的影响
$8,099.00
Aluma CCD 694 支持多种配件,包括具有微米级滤光片定位的 8 位 FW8S-Aluma 滤光轮、StarChaser SC-2 离轴导星相机和 AO-8A 自适应光学配件。
Aluma CCD 694 具有高灵敏度、低噪声的 6 百万像素 CCD 传感器,像素大小为 4.54 微米。它非常适合拍摄高空间分辨率、长时间曝光且安培辉光、暗电流和噪声最小的照片。它还具有执行高比率模拟合并的能力,这对于光谱学等应用非常重要。
Aluma CCD 是新一代研究相机,性能更佳。经过两年多与大学研究人员的合作,我们为您带来了增强型全新 Aluma CCD 系列,该系列代表了高性能中型 16 位 CCD 探测器的最佳价值。我们精心改进了相机电子设备,以提高性能、最小化安培辉光和降低噪音。使用索尼一流的 CCD,您将获得具有 CMOS 技术灵敏度的 CCD 的精确和超清晰图像。
Aluma CCD 694 – 令人难以置信的灵敏度
ICX-694 CCD 是迄今为止最好的光学传感器之一,峰值量子效率超过 75%,光谱灵敏度非常宽,蓝色灵敏度极高。它还具有非常低的读取噪声、大动态范围和极低的暗电流。高灵敏度和极低噪声的结合意味着您可以更快地获得更清晰、更深的图像。
- 目前由 SONY 和 Teledyne E2V 生产的高性能 CCD 图像传感器
- 轻巧、紧凑的设计
- 居中光轴,实现最佳仪器平衡
- 超可靠的均匀照明(光度测定)机械快门
- USB 2.0 接口
- 全帧图像缓冲消除了读出伪影
- 2 级 TE 冷却,典型温度比环境温度低 50°C
- 采用 SmartCooling TM技术的双变速风扇
- 高精度温度调节
- 内置 RBI 预闪光(仅限全画幅前照式传感器)
- 外部 TTL 触发输入和输出
- 包含 110V / 220V 电源和可选 12VDC 操作
- 用户可充电干燥剂插头
- 内置 1/4-20 三脚架接口
- 支持高精度8位滤光轮
- 与 StarChaser SC-2 离轴导星相机和 AO-8A 自适应光学系统配合使用
- 坚固的固件更新能力——几乎不可能“变砖”
包含高级软件
所有 Aluma CCD 型号均配备适用于 Windows 的 MaxIm LT - 这是我们相机专用的MaxIm DL特殊版本。Aluma CCD 还通过 ASCOM 和原生驱动程序支持第三方应用程序。
紧凑轻巧的设计
Aluma CCD 相机尺寸仅为 114mm x 114mm x 102mm(带手柄)(不带手柄为 89mm),重量仅为 1 千克(2.2 磅)。
机械快门
SBIG Aluma CCD 814 具有电子快门功能,最小曝光时间仅为 0.001 秒。此外,它还具有高可靠性机械快门,有助于实现准确的暗/偏置校准帧。
高性能 ICX-694 图像传感器
Aluma CCD 694 采用广受欢迎的 600 万像素 SONY ICX-694ALG 传感器。该传感器的像素为 2750 x 2200,面积为 4.54 微米见方,芯片尺寸为 14.6 毫米 x 12.8 毫米。
这是一款高灵敏度的隔行 CCD 传感器,具有极低的暗电流和极低的读取噪声。这款高性能传感器与 Aluma CCD 的高冷却性能和低读取噪声相结合,可产生异常清晰的图像。
该传感器采用微透镜技术,可将光线集中在每个像素的敏感区域上。CCD 的灵敏度在可见光谱中心 550 nm 处达到峰值,并在整个可见光谱范围内保持高灵敏度。与市场上的其他传感器相比,ICX-694 在蓝色方面表现尤为出色。
智能冷却技术
所有 Aluma CCD 相机均采用我们强大的全新 SmartCooling 技术。两级冷却器、强大的风扇和使用热流模拟设计的先进散热器相结合,可在环境温度为 -50C 时产生典型的冷却增量。考虑到 Aluma CCD 非常紧凑和轻巧的封装,这真是一项了不起的成就。
SmartCooling 可自动调节风扇速度,以优化冷却器性能和功耗。相机固件会持续监控传感器和散热器温度并控制冷却器功率。当需要全功率冷却时(当降低或接近全功率运行时),风扇会加速至最大速度,从而实现最强的冷却效果。当需要较少的冷却功率时,风扇会自动减速以降低噪音水平和功耗。如果散热器过热,SmartCooling 还会通过切断电源来防止过热的可能性,因此您不必担心相机在白天是否被置于炎热的天文台中。
包含高级软件
所有 SBIG 相机均配备我们的 MaxIm LT 软件 - 价值 200 美元!MaxIm LT 是我们备受推崇的 MaxIm DL 软件的一个特殊版本,可完全控制您的相机、滤光轮和自动导星仪,并提供高级图像处理功能。如果您愿意,可以升级到 MaxIm DL Pro,以获得完整的天文台集成以及更多的处理和分析功能。
附带配件
每个 Aluma CCD 相机套件包括:
- MaxIm LT 软件 – 请使用此表单申请您的许可证
- 豪华手提箱
- 通用电源(110V / 220V,50-60 Hz)
- 2英寸鼻托适配器
- 包含软件、驱动程序和文档的 USB 闪存盘
- 15 英尺(4.5 米)USB 线缆
可选的 FW8S-Aluma 8 位滤光轮包含正定心机制,每次都能将每个滤光片精确地置于完全相同的位置。这种单像素精度完全消除了平场拍摄后的灰尘点和其他伪影的重影。
正向定位机制提供单像素滤波器位置精度
精密平场定位和超精确索引
左上图显示滤镜上有灰尘点。拍摄平场校准帧,然后滤镜轮旋转几次,然后拍摄第二张经过平场校准的照片(右上图)。没有看到灰尘点的痕迹。这种高精度可产生最高质量的图像和出色的光度测量精度。
Aluma 轮可容纳标准 36 毫米滤镜,并提供 1-1/4 英寸滤镜插件,适用于较小格式的 CCD 传感器。
Aluma 滤光轮取代了相机的前板,从而最大限度地减少了后焦,确保相机/滤光轮组合能够在尽可能广泛的光学系统上达到聚焦。
对于天文成像,Aluma CCD 系列可与StarChaser SC-2离轴导星相机配合使用。这可提供可靠的导星,不受光学系统弯曲的影响。它还支持可选的 AO-8A 自适应光学附件的操作。
所有 Aluma CCD 型号均可与 AO-8A 自适应光学附件配合使用。AO-8A 使用倾斜窗口来快速精确地调整图像位置以响应自动导星器反馈。使用自适应光学系统不会出现间隙、粘滞或滞后,并且移动非常精确和准确。这使得 AO-8A 不仅可以消除周期性误差、漂移和阵风的影响,还可以减少大气视宁度的影响
From $15,889.00
SBIG Aluma AC2020BSI
超高灵敏度背照式科学级 CMOS 相机。400 万像素传感器,像素大小为 6.5 微米,具有自适应光学功能,兼容 StarChaser Guider。
SBIG Aluma AC2020BSI 采用 1 类传感器。
熔融石英腔体窗口可配备 VIS-NIR 和 UV-VIS 光学涂层选项。
即将推出 – 可预订。
SBIG Aluma AC 系列代表了天文成像系统先进科学 CMOS 相机的最新技术。相机的先进设计允许通过 USB 3.0 连接将数据高速下载到控制计算机。SBIG Aluma AC2020BSI 使用 Gpixel GSENSE2020BSI-H CMOS 传感器,该传感器具有 400 万像素,分辨率为 6.5 微米,阵列尺寸为 2048 x 2048。传感器尺寸略大于 13.3 平方毫米。Aluma AC 系列具有强大的两级冷却功能,并支持可选的水冷。Aluma AC 相机可直接通过 12VDC 8A 电源供电。
设计特点包括:
背照式传感器
令人难以置信的灵敏度!高性能背照式传感器在制造过程中被翻转并变薄,因此入射光在到达敏感像素区域之前不会遇到任何电路。这为整个可见光谱及更远的光谱提供了最佳灵敏度。
GSENSE2020BSI-H 中的传感器峰值量子效率为 91%,可见光谱中峰值较宽。对于近紫外和红外应用,它在 200 nm 至 1000 nm 范围内具有良好的灵敏度。
腔体窗口涂层选项
GSENSE2020BSI-H 传感器是无窗的,可为整个传感器提供最佳灵敏度。对于无窗传感器,我们建议每年给干燥剂塞充电一次,以避免传感器受到湿气污染的风险。
密封传感器室上的熔融石英光学窗口有两种标准涂层可供选择,具体取决于您的应用。VIS-NIR 提供 400 nm 至 1000 nm 范围内的最佳灵敏度。UV-VIS 提供 250 nm 至 700 nm 范围内的最佳透射率。
StackPro™
SBIG Aluma AC2020BSI 科学 CMOS 相机具有StackPro™ ,这是一项在相机内部执行图像堆叠的革命性功能。
CMOS 传感器的阱深和位深度通常比其前身 CCD 传感器更有限。同时,现代 CMOS 传感器的读取噪声比同等 CCD 低得多。这种低读取噪声可以发挥优势,通过堆叠许多较短的曝光来实现相同的最终结果。然而,这会导致大量额外的磁盘使用和后期处理。
StackPro™ 可在相机内部自动执行堆叠。它会自动将您的曝光细分为最多 16 个单独的子曝光,并在下载之前将它们堆叠在相机内部。这可避免硬盘中堆积过多的数据。堆叠还可用作高动态范围 (HDR) 模式的替代方案。
H DR 模式
AC2020BSI 中的传感器能够在 HDR 模式下运行,其中高增益和低增益图像可同时读出。我们附带的 MaxIm LT 软件具有 HDR 合并功能,可大大简化生成清晰、高度线性图像的过程。
出色的冷却效果
与业界领先的 STX 系列相机共享的经过验证的针式散热器设计可散发热量,同时提供低振动。包括SmartCooling™智能热电冷却和风扇操作。
水循环准备就绪
对于高环境温度环境,液体冷却选项可提高热性能并有助于最大限度地减少暗电流。
用户可充电干燥剂
SBIG 率先采用了高科技用户可更换的滤芯,其中装有陶瓷过滤器和分子筛干燥剂。与其他竞争相机不同,当其腔体干燥剂最终饱和时,它们需要工厂维修,而用户可以轻松重新填充干燥剂。这消除了昂贵的维修需求,更不用说相关的停机时间和运输成本了。此功能在高湿度地区尤其重要。
电子和机械快门
GSENSE CMOS 传感器具有电子滚动快门。此外,Aluma AC 系列相机还配备机械快门,可方便地进行暗帧减法,以实现最佳性能和灵敏度。这对于远程/机器人操作至关重要。
可选 12 位滤光轮
SBIG Aluma AC2020BSI 与新型 12 位置 SBIG AFW-12-50R滤光轮兼容,使用 50 毫米圆形滤光片。
它还兼容 7 位置FW7-STX滤光轮,使用 50 毫米方形滤光片。
提供自导和自适应光学选项
可用的 SBIG StarChaser SC-3是在滤镜前集成自动导航的绝佳低成本选择,并且它支持我们的 SBIG AO-X自适应光学配件。
AO-X 使用倾斜窗口来快速精确地调整图像位置,以响应自动导航器的反馈。使用自适应光学系统,不会出现间隙、静摩擦或滞后,移动精确准确。这使得 AO-X 不仅可以消除周期性误差、漂移和阵风的影响,还可以减少大气视宁度的影响。与 Aluma AC 相机一起使用时,AO-X 需要 StarChaser SC-3。
更多信息请参阅AO-X 。
USB 3.0 接口
Aluma AC 包含一个 USB 3.0 接口端口,用于高速下载。对于需要较长电缆长度的安装,该端口还兼容 USB 2.0。
I2C AUX 端口
STX 相机有一个方便的辅助控制端口(也称为 I2C AUX 端口),用于控制滤光轮并提供可选的外部触发接口。与旧款 SBIG 型号不同,AUX 端口不用于 AO-X 控制,因为此功能现在由可选的 SBIG StarChaser SC-3 离轴引导相机处理。
MaxIm LT 软件
所有 SBIG 相机均配备我们的 MaxIm LT 软件 - 价值 200 美元!MaxIm LT 是我们备受推崇的 MaxIm DL 软件的一个特殊版本,可完全控制您的相机、滤光轮和自动导星器,以及高级图像处理功能。如果您愿意,可以升级到 MaxIm DL Pro,以获得完整的天文台集成以及更多的处理和分析功能。
附带配件
所有 Aluma AC 相机都配有豪华手提箱、通用电源、Aluma AC 电源延长线、USB 3.0 线和 MaxIm LT 软件。
规格
| 接触 |
0.001 至 3600 秒 |
|---|---|
| 操作系统兼容性 | Windows 7、8、10 x86/x64、MacOS 10.14 “Mojave” x86 二进制文件、Ubuntu 18.04 LTS x64、Raspbian Buster armhf、Ubuntu MATE arm64 |
| 全画幅下载 | 0.1 秒 |
| 重量 | 3.5 磅 / 1.6 千克 |
| 过滤器尺寸 | 50毫米方形 |
| 读取噪声(典型值) | 2-CMS 读出模式下为 1.2 e-,常规模式下为 1.6 e- |
| 温度调节 | 是的 |
| 计算机接口 | USB 3.0 |
| 力量 | 12 伏直流 8 安 |
| 冷却三角洲 | 典型值 ~ 40 °C,包括水冷选项 |
| 自适应光学选项 | AO-X 和 StarChaser SC-3 |
| A/D转换器 | 双 12 位,具有 HDR 功能 |
| 暗电流 e-/p/s | 0.16 e-/p/秒 @ -20C |
| 全井容量 | 55,000 电子 |
| 传感器尺寸 | 13.3 毫米 x 13.3 毫米 |
| 成像/像素阵列 | 2048 x 2048 |
| 快门 | 卷帘电子、机械暗快门 |
| 过滤器前的自我引导 | 是的,使用 StarChaser |
| 像素大小 | 6.5 微米 |
| 总像素 | 400 万 |
| 滤光轮选项 | FW7-STX |
| OAG 选项 | 追星者 |
| 影像传感器 | 长光辰芯 GSENSE2020BSI |
| 室内窗户 | 可见光-近红外光、紫外-可见光 |
From $9,565.00
In two decades, much has changed beyond recognition. Sensors are now back-illuminated CMOS with native 16-bit digitisation. QE is an amazing 90% and readout is a speedy 120 million pixels per second over USB3, a performance that once was unimaginable. What is maintained by QSI’s newest cameras is the integrated design, attention to detail, and bulletproof reliability.
In the design of the 700 series we have taken our best technology. Filterwheels are mechanically indexed to ensure the most precise location for perfect flat fields. The fused silica window is dew resistant and is coated on both sides with high transmission anti-reflective coating to minimise halos. The cameras use a highly efficient 2-stage Peltier cooler that draws less current and delivers more cooling than some other cameras.
The QSI 760 is our flagship product. The full frame IMX455 is widely regarded as the premium sensor for astronomers. The integrated 2”/50mm filter wheel minimises back focus, essential for the widest compatibility with focal reducers. Cable clutter is reduced thanks to the integrated filter wheel, 2 USB2 in sockets and power out. Power sockets have threaded connections for maximum reliability.
| Image Sensor | Sony IMX455 mono CMOS sensor | Sony IMX571 mono CMOS sensor |
| Resolution | 9576 × 6380 | 6244 × 4168 |
| Pixel Pitch | 3.76 um | 3.76 um |
| Sensor Size | 43.3mm diagonal (36mm x 24mm) | 28.3mm diagonal |
| Full Well | 51,000 e- | 51,000 e- |
| Read Noise | 1.2 e- | 1.7 e- (typical) |
| Set Point Cooling at ambient of 20 C | -25 °C | -25°C |
| Frame Rate | 2 FPS (Full Frame image) | 4FPS (Full Frame image) |
| Mount Type | M54 × 0.75 | M54 × 0.75 |
| ADC | 16 bit | 16 bit |
| Backfocus Distance | 31 mm | 31 mm |
| Reading Mode | Rolling shutter | Rolling shutter |
| Exposure Range | 1 ms - 24 hours | 1 ms - 24 hours |
| Dark Current | 0.005 e-/p/s | 0.0008 e-/p/s |
| Filter Wheel Mechanical indexing for reproducible flats | Filterwheel for 2" or unmounted filters, 5 or 7 position | 50mm/ 36mm filters |
| Accessories | Off-Axis guide unit | Off-Axis guide unit |
| Computer System | Windows 10+ Linux USB 3.0 8GB | Windows 10+ Linux USB 3.0 8GB |
| Requirements | Ram 64 bit Operating System. | Ram 64 bit Operating System |
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 QE | 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 QE | 95% |
| Interface | USB 3 QSFP |
| Frame Rate | 11 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 $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 QE | 73% |
| 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 $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 QE | 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 $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 QE | 68% |
| Interface | USB 3 QSFP |
| Frame Rate | 24 FPS HDR / 48 FPS LDR |
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 QE | 95% |
| Interface | USB 3 QSFP |
| Frame Rate | 24 FPS HDR / 48 FPS LDR |
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 QE | 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.
$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 QE | 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.
$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 QE | 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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