Wednesday 1 May 2024

Solar and Lunar imaging with the SVBONY SC432M fan-cooled CMOS camera

Nicola has implemented the SVBONY SC432M solar camera in AstroDMx Capture. It works fine but we have requested that SVBONY make certain modifications to the SDKs for all platforms to present only cooling data relevant to the camera.

The SC432M Mono Solar Camera IMX432 - Global Shutter, Large Pixels, greyscale  camera for Moon Sun and Planets. It has a silver coloured body that effectively reflects sunlight. The camera is fan cooled with the fan being powered by a USB C port connected to a 5v USB supply. This system helps to maintain the system several degrees cooler than if the cooling fan is not employed.

The 9um pixel size of the IMX432 has a well depth of 100ke with a total of 1.7MP  (the resolution is 1608*1104

The large pixel size means that it works at longer focal ratios, such as Maksutovs, SCTs and Daystar quarks. If one is using a shorter focal length telescope, a Barlow lens can be used to increase the focal length of the system

Skymax 127 modified for motor focus, fitted with a photo grade Baader solar filter (OD 3.7) and an SC432M placed at the focus.


Screenshot of AstroDMx Capture streaming data from the SC432M through a Baader Ca K-line filter and the Skymax 127 + solar filter


Four overlapping 1000-frame SER files were captured, the best 90% of the frames stacked in Autostackert!, stitched in Microsoft ICE, wavelet processed in waveSharp and post processed in the GIMP 2.10.

The Sun in Ca K-line light



Closer view

The Skymax 127 fitted with a dew shield and the SC432M placed at the focus.


Two overlapping 1000-frame SER files were captured in AstroDMx Capture for Windows.


The best 90% of the frames stacked in Autostackert!, stitched in Microsoft ICE, wavelet processed in waveSharp and post processed in the GIMP 2.10.

The Moon April 16th


Two overlapping 1000-frame SER files were captured in AstroDMx Capture for Linux on the next night.


The best 90% of the frames stacked in Autostackert!, stitched in Microsoft ICE, wavelet processed in waveSharp and post processed in the GIMP 2.10.

The Moon April 17th


Closer view


A Meade RB70 f/10 doublet refractor was fitted with a x 2 Barlow and the SC432M camera and mounted on the Celestron AVX mount. 


Four 1000 frame overlapping SER files were captured in AstroDMx Capture. The best 95% of the frames in each SER file were stacked in AutoStakkert! , stitched in Microsoft ICE, wavelet processed in waveSharp and post processed in the GIMP 2.10.

One pane of the mosaic


Final 4 pane mosaic of the Moon


A Coronado Solarmax II, 60, BF15 H-alpha scope was fitted with a x2 Barlow and the SC432M camera and was mounted on the Celestron AVX mount. A 1000 frame SER file was captured in AstroDMx Capture. 


The data were part processed in SER player, stacked in Autostakkert!, wavelet processed in waveSharp and post processed in GIMP 2.10.

The Sun in H-alpha light


Closer view


The SC432M camera was fitted with the lens from a x2 Barlow and placed at the focus of a CaK PST solar scope.


Screenshot of AstroDMx Capture for Linux capturing a 200-frame SER file in Ca K-line light using a region of interest.


The SER file was stacked in Autostakkert! , wavelet processed in waveSharp and post processed in the GIMP 2.10.

The Sun in Ca K-line light


By using a long focal length scope or using Barlow lenses, it was possible to match the camera to the scope fairly well.

The SC432M has a global shutter which means that the information from the sensor is read out instantly instead of gradually across the chip as with a rolling shutter. Zoltan Trenovszki states that a global shutter will prevent the occurrence of Newton's rings.  It is not immediately clear why a global shutter would avoid Newton's rings. However, with charge/voltage conversion in a CCD sensor, a vertical and horizontal charge transport first takes place. The serial charge/voltage conversion of all pixels takes place outside the sensor in the camera’s electronics. In contrast, the charge/voltage conversion in CMOS sensors occurs in every pixel on the sensor. This difference in charge handling could potentially contribute to the appearance of Newton’s rings in CMOS sensors.
Considering the shutter mechanism: Most CCD sensors use a global shutter, which exposes the entire image simultaneously. On the other hand, most CMOS sensors use “rolling shutters,” which expose different parts of the frame at different points in time. This difference in exposure mechanism might also play a role in the formation of Newton’s rings. 
With the SC432M we saw no sign of Newton's rings, even when using a Barlow lens which is the classical situation for causing the phenomenon. If this proves to be general, it will be a great benefit for H-alpha imaging without having to tilt the camera in the optical axis.

Tuesday 30 April 2024

Lunar imaging with the SV205C camera

The SC205C camera also goes under the same name as its predecessor, the SV205.

The original SV205 was a challenging camera suffering badly from pixel vignetting that was largely due to the fact that its sensor was intended for tablets or phones and not telescopes. That having been said, we were able to obtain some very good lunar images with the original SV205 by doing real time flatfield correction and conversion to grey-scale in AstroDMx Capture.

The SV205C (the new SV205) is a much better camera that does not suffer from the pixel vignetting shown by the original version. It is still basically an 8MP camera and has a Sony STARVIS IMX415 backlit sensor with 1.45 micron square pixels.

There have been some issues with this camera not working in macOS and Nicola is currently working on this.

We tested the camera using AstroDMx Capture for Linux.

The SV205C was mounted at the focus of a Skymax 127 Maksutov which was mounted on a Celestron AVX GOTO mount.

1000-frame SER files were captured of selected regions of the Moon with AstroDMx Capture.

Screenshots of AstroDMx Capture streaming and capturing data from an SV205C through a Skymax 127 Maksutov



The best 90% of frames in the SER files were stacked in Autostakkert! , wavelet processed in waveSharp and post processed in the GIMP 2.10.

Tycho region


Closer view


Plato region

Closer view

The SV205C is a much easier camera to use for lunar imaging than the original version. It is also now at a better price point for a potential purchaser. 

Nicola has implemented the SV205C in AstroDMx Capture for Apple Silicon. At the moment it is proving intractable in macOS x86-64 but Nicola is working on it.

Thursday 4 April 2024

The Appeal of the Seestar S50 Smart Telescope

The Seestar S50 smart telescope is a remarkable, low cost device of high quality.

It is a 50mm, apochromatic triplet with a focal length of 250mm, an integral Sony IMX462 sensor with a resolution of 1920x1080 pixels camera is built in, and the whole unit weighs 3 kg. It comes with a solar filter and a built in dualband, broadband (light pollution) filter that can be switched in an out. It also has an anti-dew heater that can be turned on to help avoid dew formation on the objective.

The Seestar S50 is controlled by Seestar software that runs on Android or iOS devices such as smart phone or tablets. It is much more satisfying to use a large tablet screen than a small phone screen, although both work.

Screenshot of the tablet screen running the Seestar software

I will say right now that I wish that there was an SDK that would allow the Seestar S50 to be controlled by other capture software such as our own AstroDMx Capture. However, that being said, at the moment no such SDK exists.

The Seestar S50 can be set to capture 10s, 20s or 30s exposures. The device then live-stacks the images as they are captured. It rejects images and doesn’t stack an image if it has star trails or if the are insufficient stars (usually due to passing clouds). It can be set to save each individual image captured and live-stacked so that they can be independently stacked in other software. Before live stacking begins, dark frames are automatically captured and they are applied in real time to the stacking frames. When a frame is successfully added to the stack, the time is incremented so that it is always possible to see the total accumulated exposure time.

Screenshot of the live-stack of M51 after 10 minutes of 10s exposures have been captured


When the imager decides to terminate the captures, the Seestar S50 saves the integrated image to the tablet device that has been controlling it.

Integrated image of M51 saved to the controlling tablet


It can be set to watermark the image with relevant information. This is a very useful feature.

This is part of the appeal of the Seestar S50. The stacked image is presented in quite an acceptable form suitably labelled. For a casual user or outreach this may be all that is required.

Here are some other examples of integrated images with very modest total exposure times:






If all of the individual images are saved, they will be saved in a folder on the Seestar S50 with a name such as  M51 –sub. The interesting and useful fact is that if, say on the next night, M51 is imaged again, the individual files will be saved into the same folder ready to be re-stacked and having more information added to the subject image.

There is a paradigm shift in the way that we think of long exposure times when working with the Seestar S50. Instead of thinking of long individual exposures as we are used to with normal equatorial astro-imaging, we think of accumulated shorter exposures. This harks back to earlier days of amateur electronic imaging at about the turn of the century, with off-chip integration, when software was developed to sum individual 1/50s half frames from very low-lux surveillance cameras into 32bit FITS files using software such as AstroVideo developed by Bev Ewen-Smith of the COAA observatory in the Algarve, or Vega developed by Colin Bowness in the UK. Then frame accumulating video cameras such as Mintrons or the Samsung SDC-435 (SCB-2000), extended this idea to summing the frames into a buffer on the camera for periods of up to 5s or even 10s whilst continually releasing copies of the accumulated image into the video stream at 25fps. In these cases, long exposure times were synthesised by the summing (stacking) of captured shorter exposures. They say that there is nothing new under the Sun and these days this type of work is called EAA (Electronically Assisted Astronomy), we didn’t have a name for it back in the day. The reason for this type of thinking in relation to the Seestar S50 is that it works with an AZ mount. Longer exposures than the 10s, 20s or 30s exposures would allow star trailing to occur within an individual exposure. Although some users of the Seestar S50 leave their scope to stack images of a given object over several hours, others accumulate data by capturing for a shorter period of time at a similar time over several nights (if they are fortunate enough to get several relatively consecutive clear nights.) A combination of these approaches can be used.

Various software can be used to stack the saved (already calibrated) Seestar S50 images: Deep Sky Stacker, PixInsight and Siril and others can be used. Also ZWO’s own ASIDeepStack software works well and can be readily downloaded from the ZWO website. However, it stacks into a 16 bit file rather than a 32 bit file. ZWO’s ASIVideoStack software also works very well for stacking RAW AVI files of the Moon, Sun or planets. It must be said that the Seestar S50 is not really suitable for planetary imaging. Whilst it can be done, the images scale is too small for detailed images of the planets. However, For lunar and solar imaging, the Seestar S50 is ideal.

Image of the Moon as saved to the controlling tablet


Processed image of the 98.2% Moon


Snapshot of the Sun setting over the mountain across the valley


A processed image of the Sun showing lots of sunspots, March 22, 2024


Examples of processed Seestar S50 deep sky images

The Orion nebula


The Pacman nebula


The tadpoles nebula


Central part of the Rosette nebula and the Satellite cluster


M13


M37


The results shown here represent an initial exploration into the capabilities of the Seestar S50 with relatively short total exposures. It is intended to explore the results obtainable from longer individual exposures and longer total exposure times.

Part of the allure of the Seestar S50 is that it is a very portable and easy to use GOTO telescope and mount. It really is a grab and go device that can be taken to alternative sites and be set up and imaging in minutes. Also, the package contains everything you need from a robust carry case, small, stable tripod and even a solar filter.

That having been said, there is a small ecosystem of low cost, 3D printed accessories that enterprising enthusiasts have made available in markets such as eBay and Etsy. These accessories include dust lens caps, dew shields, filter holders and Bahtinov masks. Probably the most essential accessory is a dew shield because the Seestar’s objective lens is not very far inside the tube case. The Bahtinov masks can be useful to achieve perfect focus. Whilst the autofocus facilty is very good, there is a focus facilty that can be invoked, and with the use of a Bahtinov mask, achieve perfect focus on a bright star. Filter holders can be useful if one wishes to switch out the built-in dualband broadband light pollution filter, leaving only the built-in UV/IR cut filter over the sensor, and then use for example, a narrowband dualband filter such as a Ha/OIII filter or a SII/OIII filter. There are even 1.25” to 2” filter converters that can be used to hold smaller filters. We have yet to test any of these accessories other than a Dewshield that we made from a 2” sandwiched filter holder and a short piece of black pipe of the correct diameter that we flocked on the inside with black felt. The device can still hold a 2” filter if required.

Seestar S50 accessories



The accessory which speeds up the setting up of the Seestar S50 is a low cost leveling device that allows the scope/mount to be leveled in moments without having to extend and retract the tripod legs. The Seestar S50 has a built-in leveling system that involves getting two green circles to overlap on the controlling tablet screen. This can be quite awkward, but with the aid of the leveling device, it is both quick and easy. The leveling device fits between the Seestar S50 and the tripod and is installed by simply screwing it onto the tripod and the scope.

Leveling device

The versatility of the Seestar S50 is increased by the fact that it has a Scenery mode for taking images of objects and animals in the landscape. It also has a very useful time-lapse capture mode.

Snapshot of a sheep on the mountainside across the valley


In conclusion, we can say that the Seestar S50 is a serious, low cost, versatile apochromatic telescope system that is quick and easy to set up and use.