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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
Monochrome Deep Sky Cameras
44 products
44 products
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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
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.
$5,699.00
- 传感器类型:CCD - Sony ICX814
- 水平分辨率:3380像素
- 垂直分辨率:2704像素
- 像素大小:3.69 µM x 3.69 µM
- ADC:16位
- 读出噪声:5e-典型值
- 接口:USB 2.0 高速,带嵌入式集线器
- 电源:12V DC 2A
- 最大曝光长度:无限制
- 最小曝光长度:1/1000 秒
- 冷却:热电设定点,最大 ΔT=-38°C
- 重量:约 900 克
- 后焦距:~27mm
- 仅作为单声道
方便使用是设计的关键。Atik One 还配有内置 USB 集线器和配件电源端口,这样您就可以控制电缆杂乱。您的成像设备只需 2 根电缆!除此之外,还有两个 1/4 英寸三脚架安装孔,为您提供更多安装相机、其他配件或管理电缆的选择。
5 位置集成式 1.25 英寸滤光轮配有一个用于放置滤光片的机械滚轮,可确保连续拍摄的图像具有最高水平的可重复性。滤光轮由我们的软件原生控制,或具有用于第三方程序的 Ascom 驱动程序。为了减少更换滤光片的麻烦,相机配备了一个工具,允许在不打开相机的情况下装入滤光片。
Atiks 自己的捕获软件(Artemis)用于相机控制和数据采集,并且包含插件以便与 Astroart 和 Maxim DL 一起使用。
还包括Dawn图像处理软件。
系统要求:
- 配有 512MB RAM 的 Pentium IV PC
- Windows XP/Vista/Win7/Win8/Win8(非 RT)
- CD-ROM 驱动器
- USB 2.0 端口
通用(110-230V)电源适配器是可选的。
$2,299.00
Atik Infinity Mono
技术规格
- 传感器类型:CCD - Sony ICX825
- 水平分辨率:1392像素
- 垂直分辨率:1040像素
- 像素大小:6.45 µm x 6.45 µm
- ADC:16位
- 读出噪声:6e-典型值
- 增益系数:0.37e-/ADU
- 满井:~24,000e-
- 速度:每秒2-3帧
- 接口:USB 2.0高速和ST4兼容导向端口
- 电源:12V DC 1A
- 最大曝光长度:120 秒
- 最小曝光长度:1/1000 秒
- 冷却:被动
- 重量:约 340 克
- 后焦距:13mm
以下是 Atik You tube 频道的视频链接:
$5,599.00
规格
| 传感器类型: | CCD-索尼 ICX814 |
| 水平分辨率: | 3380 像素 |
| 垂直分辨率: | 2704 像素 |
| 像素大小: | 3.69 微米 x 3.69 微米 |
| ADC: | 16 位 |
| 读出噪声: | 5e-典型值 |
| 界面: | Mini-USB 2.0 高速 |
| 力量: | 12伏直流1安 |
| 最大曝光长度: | 无限 |
| 最短曝光长度: | 1/1000 秒 |
| 冷却: | 热电设定点最大 ΔT=-25°C |
| 重量: | 约 400克 |
| 后焦距: | 13 毫米 |
Atik 490EX 完全支持低至 f/2 的 1.25 英寸滤镜,因此您无需更换任何轮子或滤镜的现有投资。当您打算投资可通过多台望远镜的 CCD 相机时,这是一个额外的优势。
Atik-4 系列相机是著名 3 系列相机的升级版,具有更好的冷却效果和更窄的机身。它们得益于设定点冷却,可轻松拍摄匹配的暗帧,并且只需 12V 电源即可方便进行现场操作。令人印象深刻的灵敏度、出色的冷却效果和窄外形使 Atik 4 系列成为适用于现代望远镜(包括 Hyperstar/Fastar 系统)的出色 CCD 相机。
$5,199.00
规格
| 传感器类型: | CCD-索尼 ICX694 |
| 水平分辨率: | 2750 像素 |
| 垂直分辨率: | 2200 像素 |
| 像素大小: | 4.54 微米 x 4.54 微米 |
| ADC: | 16 位 |
| 读出噪声: | 5e-典型值 |
| 界面: | Mini-USB 2.0 高速 |
| 力量: | 12伏直流1安 |
| 最大曝光长度: | 无限 |
| 最短曝光长度: | 1/1000 秒 |
| 冷却: | 热电设定点最大 ΔT=-25°C |
| 重量: | 约400克 |
| 后焦距: | 13 毫米 |
Atik 460EX 完全支持低至 f/2 的 1.25 英寸滤镜,因此您无需更换任何轮子或滤镜的现有投资。当您打算投资可通过多台望远镜的 CCD 相机时,这是一个额外的优势。
Atik-4 系列相机是著名 3 系列相机的升级版,具有更好的冷却效果和更窄的机身。它们得益于设定点冷却,可轻松拍摄匹配的暗帧,并且只需 12V 电源即可方便进行现场操作。令人印象深刻的灵敏度、出色的冷却效果和窄外形使 Atik 4 系列成为适用于现代望远镜(包括 Hyperstar/Fastar 系统)的出色 CCD 相机。
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