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.

 

Saturday 16 March 2024

Release of Version 2.6.3 of AstroDMx Capture

Nicola has released Version 2.6.3 of AstroDMx Capture

Mutatis mutandis

This is a feature release of AstroDMx Capture that introduces several new functions together with native support for Apple Silicon (ARM64) computers. In addition to this, there are SDK updates, various bug fixes and other improvements.

Apple Silicon

Version 2.6.3 introduces a native build for Apple Silicon computers. At the current time, this build supports cameras that have native Apple Silicon SDKs provided by the manufacturers. The list of supported cameras is as follows:

SVBONY

DSLRs

Altair

Touptek

OGMA

UVC (Web cams)

INDI Cameras

If you are Apple user and your camera is not listed above, then you should download the build for x86-64 and run it using Rosetta.

Significant New Features

A number of new features have been implemented for this release.

SVBONY: Bad Pixel Correction

SVBONY has added a bad pixel correction function into its SDK and this functionality has been implemented in this release.

After connecting to an SVBONY camera, you should notice the new functions under the “Controls: Camera” category located on the right hand side of the main UI. Depending upon the camera used, this will either just show a checkbox to active the functionality or both a checkbox and a slider. The slider can be used to alter the severity of the correction. This function is active by default.

IMPORTANT: This functionality does not exist on the SV105 or the SV205.

Plate Solver Functions

It is now possible to specify a path to the ASTAP star database. This allows for the ASTAP command line program to be in a different directory (folder) than the corresponding star databases. This function can be found in the setup UI for ASTAP.

It is now possible to automatically reduce the size of the image that is uploaded to Astrometry.net. Many high resolution astronomy cameras produce very large files which can take a long time to upload over an Internet connection. This function reduces the size of the image which allows for a faster upload to astrometry.net and faster solves. The image size is controlled by a percentage slider and can be found under the setup UI for Astrometry.net.

Disk Space Information

AstroDMx Capture now informs the user of the amount of disk space available for captures. This information is reported in the status bar (at the very bottom of the main window), in the log window and on the capture dialog box.

In addition to this, warning messages are shown in the log window if disk space is becoming critical.

Stability Features

Previously, if a camera had a glitch, it could cause AstroDMx to lockup on exit or when changing pixel formats/resolutions. If this happened, it would need the user to manually kill the application. The reason for such lockups were caused by threads becoming “stuck” in an SDK function call. Fortunately, this didn’t happen often but could be more common with specific camera types or even faulty USB cables/ports.

This version now has a monitor that detects such anomalies and, if a block is found, AstroDMx force-terminates the offending thread before handing control back to the user. This should completely remote the possibility of AstroDMx locking up due to camera SDK problems.

If such a problem is detected, the user is shown a message indicating that processing is active and asked to wait.

macOS UI

There have been changes to improve the visual appearance of the macOS user interface. This is specifically associated with the borders that group related controls. Most of the user interface has been improved but there are still some dialog boxes that are still to be done.

Version: 2.6.3 summary

Added: MacOS Apple Silicon (ARM64) native support

Added: Bad Pixel Correction for SVBONY cameras

Added: Functionality to specify the path to the star database for the ASTAP plate solver

Added: Functionality to reduce the size of images when uploaded to the Astrometry.net plat solver

Added: Disk space information for the drive where image data are saved

Added: A monitor that automatically kills the video handling threads if there is a lockup in a camera SDK. Occasionally, a camera SDK function can lockup, if this happens it would stop AstroDMx Capture from closing and would require the user to force terminate the application. This function detects such anomalies and force terminates the threads as cleanly as possible which means that AstroDMx will not lockup in such circumstances

Changes: Improvements for the macOS user interface

Changes: Improvements to the system information dialog

Updated: PlayerOne SDK

Updated: QHY SDK (all platforms, including macOS)

Updated: SVBONY SDK

Updated: OGMA Camera SDK

Updated: Atik SDK (not including ARM Linux builds)

Updated: libusb to 1.0.27 (includes changes to stop assertions being thrown in certain circumstances. These assertions could sometimes cause AstroDMx to crash)

Bug fixes and other improvements

Important Note

Initial users have reported that after downloading the Apple Silicon build of AstroDMx Capture, it reports that the app bundle is corrupt. It is not corrupt but is being incorrectly reported so by Apple. After further investigation, it appears that this is because AstroDMx is not notarised by Apple and that this is a requirement for Apple Silicon applications. 

Unfortunately, Apple Notarisation requires a significant yearly financial payment to Apple and, as AstroDMx Capture is made available free of charge, this cost cannot be justified. 

Fortunately, there is a simple solution to this problem. The procedure is as follows:

  1. Double click on the downloaded AstroDMx Capture DMG file

  2. Drag AstroDMx Capture.app into /Applications

  3. Launch a terminal and type the following:

  4. xattr -cr /Applications/AstroDMx*

  5. Press enter

Once the above procedure is complete, AstroDMx Capture should run correctly.


I am pleased to say that Nicola has resumed work on INDIGO support in AstroDMx Capture

Monday 11 March 2024

 Seestar S50 - Wi-Fi range extension

Introduction to the Seestar S50

The ZWO Seestar S50 is a smart altazimuth telescope. It is a 50mm apochromatic triplet with a built in UV/IR cut filter and a dualband 20nm H-alpha and 30nm (OIII, H-beta) light-pollution filter (atumatically or 'manual' placed in the light path. It has a built in camera which uses the Sony IMX462 CMOS sensor which has a resolution of 1920 x 1080 pixels (2 MP). The Seestar S50 has a focal length of 250mm, and a focal ratio of f/5. For solar observing/imaging, a solar filter is provided. It has a built in dew heater and the Seestar software, which runs on Android or iOS can control the scope and autofocusing. The Seestar S50 can be set to capture 10s 20s or 30s exposures or video (which can be RAW or MP4). Being an altazimuth mount, if long exposures are being used, it will depend on which part of the sky and elevation one is imaging, which exposure it will be reasonable to use. Our initial deep sky imaging was done with 10s exposures.

The scope plate solves to centre the object once located. The built in compass aids the telescope in finding it's targets. Once located and centred (which is a quick process) the scope can be set to start capturing. It captures exposures and does a live stack so you can see the image building up on the screen. (We used a 10.4 " Android tablet to get a really good view of the developing image.) 


Before the scope starts capturing images, it prepares by capturing darks which are then applied in real time to the captured images. It is possible to save just the stacked image, or, as we did, to save each of the individual exposures so that they can be stacked and processed in other software.

Equipment Required to extend the Seestar S50s Wi-Fi range

1. Two high frequency ethernet over mains adapters.



2. Wi-Fi Repeater/Access point configured as a Wireless Access Point.



3. A Seestar S50 operating in Station Mode The Seestar S50 broadcasts its own network.



Ethernet over mains Adapters

Ethernet over mains adaptors are devices that are capable of routing data via electrical power lines. In order to set up a powerline network, two ethernet over mains adapters are needed. Each device consists of a standard mains plug (containing the appropriate circuitry) with an RJ45 ethernet port.

The first device is connected directly to the local local area network in the house via ethernet and is plugged into a standard mains AC socket. The second device is plugged into the AC outlet of the long mains extension lead out by the Seestar S50, and its ethernet port carries the same data signal as the first. Once the devices are connected, they automatically negotiate the fastest stable speed.

Wireless access point

A wireless access point (AP) is a device that takes a direct ethernet connection and transmits the signal wirelessly. The device essentially creates an independent wireless network which can have its own SSID and wireless password, however, the parameters can be the same as the primary network if required.

Procedure

A power extension lead is plugged into a standard mains outlet and the other end is taken to the desired remote location close to the Seestar S50. At the remote location, a wireless access point is plugged into the extension together with an ethernet over mains adapter and the two are connected via a short ethernet cable. The local side of the network (in the house) consists of an ethernet over mains adapter connected directly to the local area network via an ethernet cable.

Everything connected to the Seestar S50 at a distance from the house


The Seestar S50 telescope is taken to an imaging location and the the wireless access point plus ethernet over mains is placed close by. A tablet computer is then connected to the Seestar S50 in the usual way, once the connection is established, the Seestar’s Station Mode is activated and is connected to the remote wireless access point.

This process projects the Seestar S50 onto the primary network which allows a tablet computer (or smartphone) to be used anywhere that is within range of the primary wireless network. In addition to extending the Wi-Fi of the Seestar S50, this has the added benefit of providing power to the Seestar S5 telescope/mount if required, by means of a Mains/USB charger via the USB C  port on the Seestar S50 so that it is not reliant on its internal battery if it is going to be in operation for a long time and maybe using its internal dew heater.

Mains-USB charger


The complete Seestar Wi-Fi extender kit


This procedure will allow the user to control the Seestar S50 from the comfort of indoors whilst the Seestar S50 is placed at a distance from the house in a place where it has optimal access to the night sky for imaging.

We tested the system with the Seestar S50 in Scenery mode. We were able to slew the scope and autofocus on objects at a distance whilst being in the house, well ouside the normal Wi-Fi range of the SeestaS50 which would have been exacerbated by the thick stone walls. The ethernet over mains brought the signal into the house network and it worked perfectly.

A tree across the valley


A wind turbine at the head of the valley


Some images captured with our Seestar S50

The Orion nebula as presented by the Seestar S50


Processed image


The Pacman nebula as presented by the Seestar S50


Processed image


The Tadpoles nebula as presented by the Seestar S50


Processed image



The Rosette nebula as Presented by the Seestar S50



Processed Image


Steve Wainwright and Nicola Mackin

Sunday 25 February 2024

Using AstroCrop to crop and register Bridge camera images taken on a static tripod.

The camera used is a Panasonic Lumix DMC-FZ72, 60x optical zoom bridge camera mounted on a sturdy Manfrotto static tripod. Images are captured at ISO 100 in burst mode (3 images per burst). If the sky stays clear during the capturing session, the aim is to capture 150 images. Allowing for the images to be saved to a fast SD card, it takes about 2.5 minutes to capture all of the images. During this time interval, there is virtually no image rotation, so stacking does not require derotation.

The first example was to image the 99.6% Moon.

At ISO 100 and 1/1000s exposure at 60 x optical zoom at f/5.9 and F=215mm. With the sensor used in the camera, this is the equivalent of 1200mm with a 35mm sensor. The 150 images are captured as the highest quality jpgs and a captured image has dimensions of 4608 x 3456 pixels

Precisely cropping and registering the images in AstroCrop.

In order to get very precise and well registered crops it is necessary to set the crop search perimeter (the distance searched away from the crop box) to a large number. We used 35 pixels . The larger the search perimeter value, the longer the cropping/registering will take. With a modern computer, the time taken is acceptable.


A single frame from the camera


The reference frame is selected and the crop box is sized and positioned


Cropping and registering in progress



Single cropped image



The cropped/registered images sum-stacked in Siril



Wavelet sharpened in waveSharp



Levels adjusted in waveSharp and saved


The image was post processed in Gimp 2.10

99.6% Moon



The second example was to image the Sun

Lumix DMC-FZ72 fitted with an ICE ND 100000 filter


A Panasonic Lumix DMCFZ72, 60x optical zoom bridge camera fitted with an ICE ND100000 solar filter and mounted on a static tripod was used to capture 69 images of the Sun at ISO 100 and 1/2000s. The images were precisely cropped/registered in Nicola Mackin's AstroCrop before being sum stacked in Siril, wavelet processed in waveSharp and post processed in the Gimp 2.10.

Reference frame set and crop-box sized and positioned



Cropping/registering in progress



Sum-stacking the cropped/registered images



Wavelet sharpening in waveSharp


The image was post processed in Gimp 2.10

The Sun showing the huge sunspot group AR3590


These two examples demonstrate that when images are captured in a sufficiently short period of time that image rotation is negligible by a camera on a static tripod, AstroCrop can crop and register the images so that a simple sum-stacking is all that is required to produce a 16 bit stacked image ready for processing. We find that capturing 150 images is sufficient to give a worthwhile image with an increase in signal to noise ratio of  12.25 compared with a single image. The camera we use is quite old and it is possible that more modern versions may capture faster and more images in burst mode. There is, however, a law of diminishing returns for the increase in Signal to Noise ratio as a function of the number of images stacked. However, the more images that are stacked, the higher the signal to noise ratio in the final image.

The 150 images does give a respectable S/N which allows for wavelet enhancing of the fine details without enhancing the noise.