Implementing and testing the SVBONY SC715C prototype planetary camera with AstroDMx Capture.
Nicola has been implementing the prototype camera in AstroDMx Capture.
The SC715C camera
The SC715C camera is built around the IMX715 sensor which shows no amp glow and has small pixels of 1.45 μm x 1.45 μm size, and a sensor size of 5.6mm x 3.2mm; 8.4M pixels.
It is a 12 bit camera and offers:
24 bit RGB (8 bit)
48 bit RGB (16 bit)
8 bit RAW
16 bit RAW
In this case the RAW is true RAW straight from the sensor and not changed by any processes such as white balance, gamma etc. Which are destructive processes. We believe that this is the best approach to RAW data and that as a principle, all changes should be made in processing, not by the camera.
Comparing the SC715C with the SV705C
The SC715C camera is well suited to capturing high resolution lunar, solar or planetary images, more so than the SC705C which has 2.9μm x 2.9μm pixels and a sensor size of 11.2mm x 6.3mm which, whilst it can capture quite high resolution images, is much more suited to EAA and Deep Sky imaging than the SC715C because the SV705C’s pixels are 4 times the area of those of the SC715C and have a much greater full well depth.
The SV705C and the SC715C are cameras with different purposes and therefore complement each other.
The SC715C was tested with AstroDMx Capture and an Ekinox 80mm ED, F=440mm refractor with a Skywatcher Autofocuser and an IR/UV cut filter for lunar imaging and Deep Sky imaging only with the bright DSO, the Orion nebula.
Ekinox 80mm ED f/5.5 refractor
To achieve optimum focus AstroDMx Capture sent the scope with plate solving, to the star Deneb which was brought to focus using a Bahtinov mask and using a 4tronix Focus RF Autofocuser controller to remotely control the autofocuser.
4tronix Focus RF Autofocuser controller
Screenshot of AstroDMx Capture focusing on the star Deneb using a Bahtinov mask
Capturing Lunar data
AstroDMx Capture was used to capture two overlapping 1500 frame 16bit RAW SER files of the 59% waxing Moon
Area 1
The advantage of capturing RAW files is that they are only 1/3 the size of RGB files, so they are captured quicker and use only 1/3 of the storage space of RGB files.
Area 2
The best 60% of the frames in each of the two SER files were debayered and stacked in Autostakkert!4. The two resulting images were stitched together in Microsoft ICE, wavelet sharpened in waveSharp and post processed in Gimp 2.10 and ACDSee.
Final image of the 59% waxing Moon
Full size (scroll to explore the image)
This is a very good result from a small, F=440mm refractor. We shall soon be testing with a much longer focal length Maksutov telescope to further explore the high resolution capabilities of the SC715C.
In order to illustrate the high resolution results, 5 equal areas were cropped out of the image and independently optimised for levels in each area.
Mare Imbrium, Mare Serenitatis, Montes Apenninus, Archimedes, Aristillus, Autolycus region
Palus Somni, Mare Tranquillitatis, Mare Crisium region
Herschel, Ptolomaeus, Alphonsus, Arzachel, Albategnius region
Fernelius, Stofler, Faraday region
Mare Nectaris, Theophilus, Cyrillus, Catharina, Rupes Altai, Piccolomini region
Capturing data on the bright (mag 4.0) DSO, the Orion nebula
100 x 10s exposures of the Orion nebula were captured along with Flats and Darks.
AstroDMx Capture capturing 10s RAW Fits files of the Orion nebula
The data were debayered, calibrated and stacked in PixInsight processed with SPCC and StarXterminator and further processed in Siril, Gimp 2.10, GraXpert and Seti Astro Suite Cosmic Clarity.
The final Orion nebula image oriented in a more familiar way
The small pixel size of the SC715C enabled the resolution of the trapezium stars.
The SC715C is so far shaping up to be a very capable high resolution camera with TRUE RAW imaging capabilities, that will complement other cameras in the imager’s collection.