Why do the sky backgrounds of my pictures vary so much between the types of objects?
Our proprietary image processing algorithm applies different parameters for each object (colorimetry, saturation, histogram …). That’s why you can see rendering differences between your photos of clusters, nebulae or galaxies. The quality of the photos also depend on the observation conditions (temperature, light pollution, transparency of the sky, turbulence …) and the level of difficulty of the star (magnitude…).
Our software is constantly evolving and updates are regularly made to improve the image processing and to refine the quality of the photos. You will quickly see tremendous progress in this area!
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[Vespera range] What are the image formats offered by Vespera?
All our instruments can provide the same image formats: - JPEG (as shown on your screen) - TIFF (the final stacked picture that will need to be processed) - FITS (the unitary pictures that will need to be sorted and processed) Here is an article ...
How much acquisition time should you aim for to improve image quality?
It all comes down to noise reduction Your smart telescope’s sensor captures light from celestial objects, which we refer to as the signal. However, it also generates noise, which is an undesirable byproduct. This noise comes from factors like light ...
How to save my pictures on my PC/Laptop (Windows users)?
We have created a fast and simple way to transfer your pictures from your Vespera's internal storage to your PC or laptop: 1. Connect your laptop to Vespera’s Wi-Fi signal. 2. Open your File Explorer to access the navigation bar. Make sure to disable ...
Why don't we see all the objects in the sky on the interactive map?
The sky map contains a part of the sky objects present in the field: The objects present in our catalog Other objects deemed large or interesting enough to be represented. To avoid overloading, we only display the names of the 20 most interesting ...
Can I observe the same objects over multiple nights?
Yes! Stellina’s Multi-Night mode, introduced in 2024, allows users to extend their observations over several nights. This feature enhances the signal-to-noise ratio, improving image quality and revealing finer details in deep-sky objects.