Search Results for "layer"

Opens/saves TIF, FITS, PNG, XISF, PXM, RAW, JPG, XCF, PSD, WEBP. AsinH, Sqrt, Ln, Exp and Sqr stretching, HSL and RGB adjusting, Levels and Curves adjusting and Background Extraction for Color Balance, Flatness and Gradient Correction. Arithmetic between images. Resizing and croping. Color Balance based on background, selection or stars B-V (after platesolving). Debayering/Bayering. Inversion, mirroring, rotation, barrel/pincushion correction. RGB alignment/shifting. Erode, Dilate, ......

Swiss Ephemeris .Net Gateway Library for AstroLight (Swenglal) is a low-level .Net library meant to provide an easy access to Swiss Ephemeris official library (swedll32.dll) in .Net projects. It also contains some handy .Net methods providing a low level abstraction layer for a convenient use of swedll32. This means that this software CAN NOT BE USED WITHOUT Swiss Ephemeris library (swedll32.dll) nor without Swiss Ephemeris files. Note that Swiss Ephemeris is developped and supported by Astrodienst and distributed under GNU Public Licence (GPL) and SEPL (Swiss Ephemeris Public Licence). ...

ProC 3.0 is a scientific workflow engine to build, manage and execute workflows (pipelines) in heterogeneous environments, supporting GRID and other means of parallel processing. It includes a data management component (DMC) to transparently access databases for storage of results and automatically adds metadata to track the processing of data products, so that at every time a full processing history is available. The software was developed and used within the ESA Planck satellite mission.

SITools2 is a new CNES generic tool performed by a joint effort between CNES and scientific laboratories. The aim of SITools is to provide a self-manageable data access layer deployed on already existing scientific laboratory databases.

This project is no longer under active development. It has been superceded by the alignment subsystem which is now part of the main INDI project. This project provides an "alignment layer" driver to sit above INDI telescope drivers. This layer performs transformation services for telescope coordinates as they pass up and down to the underlying driver. The conversion matrices are computed from alignment datums passed down into the alignment layer. The N point alignment model can be used for both equatorial and alt azimuth mounts. ...

General purpose scientific framework and its astronomy samples

SPIDR (Space Physics Interactive Data Resource) is a distributed database and application server network, built to select, visualize and model historical space weather data. SPIDR is a web-application and a grid of data mining web-services.

The Online Astronomy Project will create a complete, web-enabled, robotic astronomy system that is hardware independent (ASCOM standard abstraction layer) and capable of servicing multiple telescopes and types of observation programs at once.