ASI585MC Pro is a new ZWO deep sky camera based on the 4k SONY CMOS sensor with a 1/1.2″ format and 2.9μm pixels. It has a super high sensitivity and a large resolution of 3840*2160 (8.29MP in total). It also features high transmission speeds – In high-speed mode, the fast frame rate can reach 47fps at full resolution! Being an entry-level DSO camera, it offers great advantages of high cost-effectiveness.

Note:

External power supplies are needed for all ASl-cooled cameras. We recommend you use a 12V@3A~5A DC adapter (D5.5×2.1mm, center pole positive) or a lithium battery with 11-14V to power the camera. You can also use ASIAlR to power the cameras. Be aware that using a power supply out of this voltage range will probably lead to irreparable damage to the camera.

One Camera for All

The STARVIS 2 technology brings ASI585MC Pro more advanced imaging performance compared to other cooled cameras. Its high frame rate makes it not only suitable for DSO photography but also solar/lunar/planetary photography.

Jupiter -Jim Rivera

Moon -Christopher Schementi

NGC3372 ( eta Carina) -Simon Lewis

M42, NGC 1976 (Great Orion Nebula) -Simon Lewis

STARVIS 2

STARVIS 2 was developed by SONY and evolved from STARVIS. It is the latest technology with a wider dynamic range and super-high sensitivity beyond the human eye. Benefiting from it, ASI585MC Pro’s sensitivity and signal-to-noise ratio is greatly improved.

Large Full Well Capacity

The back-illuminated structure improves the camera’s full well capacity. Even with unbinned 2.9μm pixels, ASI585MC Pro has a full well capacity of 40ke-, nearly 3 times that of the last-generation sensor IMX485. A larger full well capacity gets the camera higher efficiency in collecting light, can effectively restrain the highlight area from being overexposed, and also can improve the signal-to-noise ratio.

Zero Amp Glow

ASI585MC Pro exhibits extremely clean dark frames with zero amp glow! No matter how long the exposure and how high the gain value is, you can easily get clean and smooth astro images!

Note: This feature is implemented directly at the hardware level, it does not require software control.

512MB DDR3

ASI585MC Pro uses a USB 3.0 interface, along with the built-in 512MB DDR3 cache, ensuring high-speed, smooth, and stable data transmission.

USB 3.0 Port & USB 2.0 HUB

USB 3.0 Port: Provides 5Gb bandwidth to allow ASI585MC Pro to run at 47fps at 8.29MP full resolution (10bit, high-speed mode).
USB 2.0 HUB: Can be used to connect various kinds of USB devices such as EFW, guide camera, and EAF.

Two-stage TEC Cooling

Thanks to the two-stage TEC cooling, ASI585MC Pro can lower the CMOS sensor temperature to more than 35 degrees Celsius below ambient temperature, which can greatly reduce dark current generation and sensor noise even during extended exposure times.

*The Delta T 35℃ is tested at 30℃ ambient temperature. It might get down when the cooling system is working for a long time. Also, as the ambient temperature falls, the Delta T would decrease.

Below is the dark current curve of ASI585MC Pro at the temperature from -20℃ to 30℃.

Camera Performance

Low read noise, High dynamic range

The camera has a built-in HCG mode, which can effectively reduce read noise at high gain and allow the camera to maintain the same high dynamic range as it does at low gain.

When the gain reaches 252, the HCG mode will be automatically turned on and the dynamic range reaches a level close to 11bit. The read noise in this case can be as low as 0.9e.

QE (Quantum efficiency)

Based on our testing results, the QE peak value of ASI585MC Pro is 91%.

Connection Methods (Back Focus Distance: 55mm)

Connection to External Devices

Structural Dimension Diagram

In the Box

ZWO ASI585MC Pro is a perfect match for either of these APO telescopes

How to Use
To use this T-Ring, place the E-Mount T-Ring on your Sony mirrorless camera. Just like changing a lens, line up the T-Ring to your camera’s lens mount. Push it in and turn until you hear a click. The T-Ring has a sturdy bayonet flange that locks for a secure fit. Once you attach the T-Ring to your camera, you’re ready to connect your telescope. The telescope side of the T-Ring has threads that accept a variety of camera adapters, including the Celestron T-Adapter. The adapter you choose depends on the type of photography you wish to do.

Body
The Sony E-Mount 42mm T-ring is machined aluminum black anodized. The internal surfaces are blackened and glare-threaded to provide the highest contrast. The T-Ring has a ribbed surface for a secure grip while threading/unthreading. The Sony E-Mount 42mm T-Ring is compatible with M42 x 0.75 (T-Thread) camera adapters.

A T-Ring is one of the first accessories you will need to take pictures through a telescope or spotting scope. If you have a Sony E-mount mirrorless camera body, the Celestron E-Mount T-Ring is the one for you.This T-Ring fits Sony E-mount mirrorless cameras only. It will not work with other Sony A-mount camera bodies without adding a Sony adapter to convert those cameras to E-mount.

Enhance your Canon EOS R series mirrorless cameras with our Saxon T-Mount adapter, meticulously designed to marry your camera with the universe of telescopic imaging. This adapter is the linchpin for attaching your Canon mirrorless camera to a T2 (M42) thread, ensuring a flawless connection for your astronomical adventures.

The adapter comes with an ingenious removable internal M42 thread, easily detached with the included hex key, paving the way for a variety of additional connections (available separately). Upgrade to an M48 x 0.75 thread with our specialized adapter, ideal for those using full-frame sensors where a standard T2 connection may lead to vignetting.

This adapter maintains the critical 25mm distance from the sensor to the female thread, safeguarding the integrity of your imaging pathway. Whether capturing the majesty of a nebula or the intricate craters of the moon, our adapter ensures a comprehensive, unrestricted field of view for the most demanding astrophotographers.

Enjoy the most dazzling views of nebulae with your Celestron Origin when you add this H-alpha H-beta OIII (Hα-Hβ-OIII) imaging filter. This specialized filter allows high throughput of light wavelengths in emission nebulae while blocking other wavelengths that could diminish image quality and detail. The result is bright, colorful nebulae images that “pop” with detail against the black sky background.

How does the Nebula Filter for Origin work? Emission nebulae primarily emit at discrete wavelengths of light—Hα at 656nm, Hβ at 486nm, and OIII at 496/501nm. By strategically transmitting only these wavelengths of light and blocking the rest of the spectrum, the filter dramatically reduces the effect of light pollution. The “bad” light is blocked while the “good” light associated with emission nebulae passes through to Origin’s sensor.

You’ll immediately notice much higher contrast in your images, especially from your light-polluted backyard! And since the transmission at the critical wavelengths is so high, the nebula will not be dimmed—only the background will be blacker. You’ll also notice some contrast improvement in images of nebulae from darker skies, as the filter serves well in blocking natural skyglow.

Nebula Hunting

The Nebula Filter is perfect for imaging emission nebulae like the North America Nebula (NGC 7000), Lagoon Nebula (M8), Orion Nebula (M42), the Carina Nebula (NGC 3372), and dozens more. The imaging filter offers maximum light transmission in the key Hα-Hβ-OIII wavelengths, producing high contrast for emission nebulae like these.

The transmission spectrum for the Nebula Filter is 85% or greater at key wavelengths (486nm, 496nm/501nm, 656nm) and less than 0.5% transmission elsewhere. As a narrowband filter, it blocks much of the visible spectrum and only lets these specific wavelengths through. Because of this, you should not use this filter while observing or imaging broadband emission objects, such as galaxies and star clusters. For those objects, you’ll achieve the best results by removing the nebula filter and reinstalling Origin’s clear optical window.

Other similar imaging filters on the market have much narrower bandpasses at the critical Hα-Hβ-OIII wavelengths. Unfortunately, these filters block much of the incoming Hα-Hβ-OIII light for an f/2.2 optical system like Origin’s 6” RASA. This is because a RASA brings light into the filter at a steeper angle, which causes a spectral shift. If you use filters not explicitly designed for use at f/2.2, some of the light from the nebula will be blocked, resulting in a dimmer image. The Nebula Filter for Origin was custom-engineered to work at f/2.2, so none of the “good” light from the nebula is inadvertently blocked by the filter.

Body and Storage

The filter features a machined aluminum black anodized cell with a knurled rim for easy grip during installation. We’ve added anti-reflection coatings to help suppress reflections on the glass. The filter fits directly into the filter drawer in the Celestron Origin’s front lens cell, where the optical window sits. Simply remove the clear window and replace it with the filter. Origin maintains its optical performance across the entire system with the filter installed. No other adapter is needed.

Each filter comes with a foam-lined plastic storage case to safely store the filter or the optical window glass that came with your Celestron Origin when not in use.

Celestron tests every Nebula Filter for Origin individually to verify its performance. Along with your filter, you will receive a spectral transmission graph (like the one pictured above) showing the results of your filter’s test and verifying it performs as expected throughout the spectrum.

Please note this is for the Celestron Origin Intelligent Home Observatory

Specifications:

Dive into astrophotography with our Saxon T-Mount, precision-engineered for your Nikon Z mirrorless camera. Constructed from high-grade CNC-machined anodized aluminum, this adapter promises both longevity and a flawless fit. It's been thoughtfully designed to maintain the correct backfocus, thereby eliminating the need for additional spacers and streamlining your setup.

With this adapter, you're equipped to attach your camera directly to a telescope and capture the night sky's awe-inspiring beauty with clarity and precision. The robust material ensures a secure connection to your imaging equipment, while the precise backfocus distance guarantees that you'll achieve sharp, focused images across the board.

Perfect for both novice astronomers and seasoned stargazers, our adapter is the bridge between your Nikon Z camera and the wonders of the universe. Simplify your astrophotography experience with this essential, no-fuss tool that stands up to the rigors of night sky exploration.

Main Sensor

The main sensor IMX571 features an APS-C format and 26MP total pixels. The size is 23.5mm in width x 15.7mm in height, and the diagonal is 28.3mm. The 3.76um x 3.76um small pixel size accommodates an impressive full depth of 50ke. With the new hardware technology, it is even extended to 73ke.

Guide Sensor

The SC2210 sensor taken from the ASI220MM Mini camera features very high sensitivity. The QE peak value reaches 92% at 500nm. The read noise is as low as 0.6e. As the new generation of guide sensor, it has achieved great results in guiding, proved by hundreds of astrophotographers.

Start Your Astrophotography Journey with Great Convenience

The ASI2600MC Air combines guiding, imaging, and smart control into one compact, lightweight device. Say goodbye to complex setups and enjoy a seamless, hassle-free astrophotography experience.

Effortlessly Connect Multiple Devices

4x USB2.0, 3x DC12V 10A, 1x USB Type-C
USB 2.0 ports for your focuser, filter wheel, and mount; DC 12V 10A input/output ports for reliable power; and USB Type-C port for fast file transfers—you can focus on capturing stunning images without worrying about connectivity issues.

Shoot with Confidence: Ample Storage and Stability

With a massive 256GB eMMC storage, the ASI2600MC Air allows you to capture multiple targets with ease. Rigorously tested with over 300 benchmarks, it ensures system stability. Plus, the USB 2.0 ports support up to 1TB external storage, giving you plenty of room for all your astrophotography needs.

Cross-Platform Device Control

Except from ASIAIR App, ASI2600MC Air can also wirelessly connect to ZWO’s proprietary PC control software, ASIStudio, and also other 3rd-party PC software. 3rd-party software can be controlled through ASCOM extended protocol Alpaca (requires ASCOM Platform version V6.6 or higher).

Bluetooth Connection Supported

Nice and Neat Wiring with AM3/AM5

Frame Rate

Camera Specifications

The best solution of 55mm back focus length

Mechanical Diagram

Camera Details

What is in the box?

Turn your mobile phone into a telescope for observing and photographing the night sky plus safe viewing of the Sun.

Go beyond the power of your phone's camera.

Both Apple iPhone and Android favourites such a Samsung Galaxy and Google Pixel phones have amazing cameras. Even the best of them are limited for distant views however.

The Vaonis Hestia extends your phone's camera with a portable, easy to use package.

Witness the sky's beauty day and night with the Hestia Solar Pack. This advanced kit includes the Hestia device, a hard case, and essential accessories for day observation.

(You will need a standard photographic tripod. If you don't have, the team at BINTEL can assist with various options.)

Make your smartphone a door to the Stars.

The iOptron iMate is a single-board computer that features a powerful 64-bit ARM processor with Wi-Fi, preloaded KStars planetarium software, Ekos control and automation tool, and INDI drivers. This hardware-software combination will support the use of most current and future devices (cameras, focusers, filter wheels, etc.) allowing the user to choose a brand and model.

With 32Gb eMMC storage along with a slot for up to 64Gb TF (micro SD) memory, iMate has the ability to control and capture an entire automated imaging session. The iMate is cross-platform; use it with Windows, IOS, Linux, Android, etc.

Features:

• Orange Pi 3 LTS with 64-bit ARM processor, 2GB LPDDR3 SDRAM and 32GB EMMC flash memory
• 1X USB3.0 and 2X USB2.0 ports
• 3X 12VDC outputs (2 programmable)
• Up to 64Gb high speed MicroSD card (class 10 or higher)
• Open Source Architecture
• Preloaded KStarts/Ekos/INDI driver for mount, camera, focuser and other device control
• iPolarServ for iOS and Android polar alignment
• Windows, MacOS, iOS, Linux, Android remote connection to iMate via WIFI network
• Mounting method: 31mm dovetail saddle for finder scope shoe mounting, 1/4"-20 threaded hole, or 2X M3 threaded holes

Combination CCD imaging kit including:

• TRIUS PRO-694 Blue Edition Camera
• Lodestar PRO Guider
• Midi Filter Wheel with built-in OAG (with 7 x 1.25″ filter wheel carousel)

Camera Details

• Medium format, high resolution ‘Exview’ CCD chip, with 6,050,000 x 4.54uM square pixels in a 15.98mm diagonal array.
• Exceptionally low dark signal – No dark frames necessary for most deep sky objects.
• Excellent QE of 77% peak in yellow light, 65% at Hydrogen alpha (656 nm).
• Three port powered USB hub built-in. Can drive a Lodestar PRO or Ultrastar PRO + SX filter wheel.
• High performance two stage cooling for better than -40C delta T
• Dry Argon CCD chamber fill for improved cooling performance.
• Exceptionally effective anti-blooming with minimal effect on linearity and no lost active area.
• Back focal length 16mm +/-1mm.

• High speed USB 2.0 interface for approx. 2.5 second downloads.
• Built-in triple powered USB hub for guider and filter wheel control.
• Single USB cable control for all features – get rid of that dangerous cable tangle!
• Very low power consumption. Less than 1.5 amps at 12v DC.
• Compact and lightweight – only 75mm in diameter x 70mm long – less than 500 grams load on the telescope.

Specification

• CCD type: ICX694AL Exview CCD with ultra low dark current and vertical anti-blooming.
• CCD Full resolution pixel data: Pixel size: 4.54uM x 4.54uM, Image format: 2750 x 2200 pixels
• CCD Image area: 12.49mm (Horizontal) x 9.99mm (Vertical).
• CCD quality: Grade 1 or better – No bad columns, no dead pixels, no more than 50 ‘hot’ pixels (saturated in <10 seconds).
• Spectral Response: QE max at 580nM (~77%), 50% roll-off at 360nM and 770nM.
• Readout Noise: Typically only 3.5 electrons RMS.
• Full-well capacity: Greater than 17,000 e- (unbinned)
• Anti-blooming: Overload margin greater than 800x.
• Dark current: Less than 0.002 electrons/second @ – 10C CCD temperature.
• Data format: 16 bits.
• System gain: 0.27 electrons per ADU
• Computer Interface: Built-in USB 2.0 compatible interface.
• Image download time: Typically 2.5 seconds at full resolution.
• Power requirements: 115VAC / 240VAC @ 12VA, or 12VDC @ 900mA max.
• Cooling system: Regulated set-point cooling supply with thermoelectric cooler to give a minimum CCD temperature of approximately -40C below ambient.
• Size: 75 x 70mm black anodised aluminium barrel with 42mm ‘T2’ thread at the CCD window end & input/output plugs at rear. CCD alignment screws are provided for setting the chip parallel to the focal plane.
• Weight: approx. 450g.

Loadstar Pro details

The Lodestar PRO is an upgraded version of the very popular Lodestar X2 autoguider with quicker download times and lower read noise electronics. The original Lodestar used the ICX429 Exview chip from Sony and offered excellent sensitivity. However, the Lodestar X2 and the Lodestar PRO utilise Sony’s upgraded version of the CCD, the ICX829, with considerably improved QE and read noise. This new ‘Exview 2’ chip approximately doubles the Lodestar sensitivity and adds nearly a full star magnitude to the minimum guide star brightness. We have also redesigned the boards so that a standard RJ12 guide socket can be used. This will please many users who have found the small ‘ZH’ cable socket to be too delicate.

Specification

• CCD – Sony ICX829AL ExView2 monochrome CCD
• Pixel count – 752(H) x 580(V)
• Pixel size – 8.6 x 8.3uM
• Optical size – 6.47 x 4.81 mm
• Read noise – Typically 5.5 electrons
• Gain – 0.4 e/ADU
• Barrel size – 31.75mm dia. x 85mm long (1.25 inch eyepiece push fit size)
• Barrel thread – 25.4mm x 0.75mm ‘CS’ mount lens thread
• Computer connection – ‘Mini B’ USB socket for USB2.0
• Output connection – Standard RJ12 autoguider socket
• Output type – Opto-isolated 4 lines (N,S,E & W) pull down with common return line
• Download rate – Approx. 10 frames per second in binned 2×2 mode (recommended)

Antlia SII 3nm Pro narrowband filter optimizes the FWHM (full-width half maximum) to 3nm bandpass. As the bandwidth becomes narrower, the 3nm Pro narrowband filters enhance the contrast of emission targets by lowering the unwanted background signal. Antlia SII 3nm Pro filter is designed to deliver 88% transmission at the 671.6nm line which provides you with the maximum signal and well-defined nebulae structures.

Conventional broader narrowband filters cause a heavy loss in transmission due to the strong (Center Wavelength (CWL)-shift. We guarantee T>88% within 1nm range of the center bandwidth, which means that the 3nm Pro narrowband filter can guarantee high transmittance for working with both long focal ratios and fast optical systems. Blue-shift data show that Antlia SII 3nm Pro filters can be used with nearly all systems as fast as f/3 with minimal loss in emission signal and meet the requirements of fast optics like Hyperstar and RASA.

The out-of-band blocking specification is rated OD5 (0.001%) which delivers an excellent SNR(signal-to-noise ratio) and effective cut-off rate to minimize interference from other wavelengths. Improved sharp cut-off astrophotography 3nm Pro filters are designed to minimize halos around bright stars.

Application and Performance:

High transmittance and smallest bandwidth to maximize contrast

A steep spectral profile minimizes halos around bright stars

A single substrate to eliminate internal reflections

Narrowband Objects: SII Emission Nebulae, Planetary, Wolf-Rayet Nebulae and Supernova Remnants

Use in light-polluted areas and dark sites

Extend imaging time when the moon is up

All Antlia narrowband Pro filters can be used down to F/3 with a slight loss of signal

All Antlia Narrowband filters are edge-blackened to eliminate internal reflections from stray light

Superior optical reliability reduces post-image processing

This filter is not suited to deep-sky objects that do not contain SII emissions.

Technical Specifications:

Basic Substrate: Schott optical substrate

Filter Thickness：2mm+/-0.05mm for 2'' mounted

FWHM (Full width at half maximum): 3nm

CWL (Central Wavelength): 671.6nm

Peak Transmission: ＞88%

Blocking: > 5 OD(0.001% out of band blocking) @ 300-1000nm

Surface Quality: S/D (scratch/dig)= 60/40 (Refer to MIL-O-13830)

Transmitted Wavefront: Lambda/4 or better.

Parallelism: less than 30 arcsec

Single / Non-glued substrate

Warranty: 3 years against delamination

SKU: ANTLIASii3nm2

Introducing the Fusion series, Sky-Watcher’s latest innovation in astronomy, designed to revolutionize your stargazing experience. The Fusion series combines advanced features with user-friendly design, offering unparalleled performance and ease of use.

Fusion 120i Key Features:

• Lightweight and Durable: The Fusion 120i mount weighs only 8kg, making it portable yet sturdy, with a payload capacity of 12kg.
• Compact Dimensions: Measuring 335mm x 214mm x 467mm, this mount is ideal for both home observatories and field astronomy.
• Precision Engineering: Equipped with a worm wheel and worm gear transmission mechanism, the Fusion 120i ensures precise movement. The Altitude and Azimuth axes each have 180 teeth, providing smooth and accurate tracking.
• GOTO Functionality: Revolutionize your navigation of the stars with the GOTO function, making it easier than ever to locate celestial objects.
• Wi-Fi Enabled: Control your telescope wirelessly via the SynScan Pro APP and SynScan APP, available on both smartphones and tablets.
• Dual Axis Clutch Locking: Features clutch locking for both Altitude and Azimuth axes, offering greater control and stability during observation sessions.
• Versatile Power Supply: Choose between the built-in rechargeable lithium battery (9.6V 4.5Ah) and an external DC12V-15V 3A power supply for extended use.
• Compatibility: Compatible with OTAs featuring Losmandy style dovetails and Vixen style dovetails, ensuring a wide range of usability.

Seamless Integration and Control:

The Fusion 120i’s Wi-Fi functionality allows for seamless control via the SynScan Pro APP and SynScan APP, making it a breeze to adjust settings and track objects from your smartphone or tablet. The mount’s intuitive interface, combined with advanced GOTO capabilities, transforms your stargazing experience into an effortless adventure.

Whether you’re a seasoned astronomer or a passionate beginner, the Fusion series provides the perfect balance of technology and convenience to revolutionize your astronomical pursuit

EQ Wedge

There's also the Sky-Watcher Fusion Wedge to convert your Fusion mount into an EQ (Equatorial) platform. 

New Planetary Camera from ZWO

ZWO ASI664MC is a remarkable new planetary CMOS camera. The 1/1.8" Sony IMX664 sensor features a small pixel size of 2.4µm pixel and a high resolution of 2704 x 1536 (4.15Mp). In high-speed mode the frame rate reaches 95 fps, while the read-out noise remains at a low level, as low as 0.46e!

Starvis 2 Technology

If you're not familiar with SONY STARVIS technology it offers the ZWO ASI664MC outstanding image quality and image performance.

High Transmission Speed

This camera has a USB 3.0 Interface, along with the built-in 256MB DDR# cache, ensuring high-speed, smooth, and stable data transmission.

ZWO ASI664MC vs ZWO ASI662MC

ZWO ASI664MC can be considered as an iteration of the ASI662MC. With the great improvement in sensor size and resolution, it provides a larger FOV and results in high-quality images containing more details.

Zero Amp Glow

ZWO ASI664MC adopts no-glow circuitry to avoid annoying amp glow being produced and ensure the image quality no matter how long the exposure and how high the gain value is.

(NOTE: This feature is implemented directly at the hardware level, it does not require software control.)

Camera Curve

Low readout noise, high dynamic range

The camera has a built-in HCG mode, which can effectively reduce readout noise at high gain and keep the dynamic range at the same level as it does at low gain. At 252 and above the HCG is automatically turned on; the dynamic range is close to 11bit; the readout noise can be lower than 1.0e.

Quantum Efficiency

QE noise and readout are very important parameters to measure the camera's performance. Higher QE and lower readout noise are necessary to improve the image signal-to-noise ratio. according to our estimation, the QE peak value of the ZWO ASI664MC is about 91%

Protective Window

The ASI664MC adopts an AR-coated filter as a protective window (Diameter: 21mm, Thickness: 1,1mm). It improved the camera's performance in UV and NIR wavelengths.