StarTools comprises several modules with deep, state-of-the-art functionality that rival (and often improve on) other software packages.
Thanks to StarTools' Tracking feature the Color module provides you with unparalleled flexibility and color fidelity when it comes to colour presentation in your image.
The Compose module is easy-to-use, but extremely flexible compositing and channel extraction tool. As opposed to all other software, the Compose module allows you to effortless process, LRGB, LLRGB, or narrowband composites like SHO, LSHO, Duo/Tri/Quadband and more composites, as if they were simple RGB datasets.
The crop module is an easy-to-use image cropping tool with quick aspect ratio presets and switchable luminance and chroma preview modes.
StarTools' Deconvolution module allows for recovering detail in seeing-limited and diffraction-limited datasets. StarTools' deconvolution is unique amongst astrophotography software in several ways;
The Unified De-Noise module offers detail-aware, astro-specific noise reduction. Paired with StarTools' Tracking feature, it yields pin-point accurate results that have no equal.
The Entropy module is a novel module that enhances detail in your image, using latent detail cues in the color information of your dataset.
The FilmDev module was created from the ground up as a robust equivalent to the classic Digital Development algorithm that attempts to emulate classic film response when first developing a raw stacked image.
The HDR (High Dynamic Range) module optimises local dynamic range, in order to bring out the maximum amount of detail that is hidden in your data.
The Lens module was created to digitally correct for lens distortions and some types of chromatic aberration in the more affordable lens systems, mirror systems and eyepieces.
New as of StarTools 1.6 beta, is the Stereo 3D module. The Stereo 3D module can be used to synthesise depth information based on astronomical image feature characteristics.
The Super Structure allows you to manipulate the super structures in your image separately from the rest of the image. It is useful to push back busy star fields, or emphasise nebulosity by colour, luminance, or both.
The Wipe module detects, models and removes source of unwanted light bias, whether introduced in the optical train, camera or by light pollution.
High-resolution data sets, such as those from a DSLR typically require at least 4Gb of RAM.
For its unique engine to function, StarTools needs to be able to make mathematical sense of your signal flow.
You can convert everything you see to a format you find convenient. Give it a try!