Difference between revisions of "Main Page"
(Encourage use of the Google forms and the Nabble archive) |
|||
Line 8: | Line 8: | ||
Although AIJ maintains the general purpose image processing capabilities of ImageJ, AIJ is streamlined for time-series differential photometry, light curve detrending and fitting, and light curve plotting, especially for applications requiring ultra-precise light curves (e.g., exoplanet transits). Its interactive image display is designed for astronomical applications. It reads and writes standard Flexible Image Transport System (FITS) files, as well as other common image formats, provides FITS header viewing and editing, and is World Coordinate System aware, including an automated interface to the astrometry.net web portal for plate solving images. AIJ provides research-grade image calibration and analysis tools with a GUI driven approach, and is easily installed with cross-platform compatibility. It enables new users, even at the level of undergraduate student, high school student, or amateur astronomer, to quickly start processing, modeling, and plotting astronomical image data with one tightly integrated software package that works on laptops and servers alike. | Although AIJ maintains the general purpose image processing capabilities of ImageJ, AIJ is streamlined for time-series differential photometry, light curve detrending and fitting, and light curve plotting, especially for applications requiring ultra-precise light curves (e.g., exoplanet transits). Its interactive image display is designed for astronomical applications. It reads and writes standard Flexible Image Transport System (FITS) files, as well as other common image formats, provides FITS header viewing and editing, and is World Coordinate System aware, including an automated interface to the astrometry.net web portal for plate solving images. AIJ provides research-grade image calibration and analysis tools with a GUI driven approach, and is easily installed with cross-platform compatibility. It enables new users, even at the level of undergraduate student, high school student, or amateur astronomer, to quickly start processing, modeling, and plotting astronomical image data with one tightly integrated software package that works on laptops and servers alike. | ||
This wiki offers open access to curated documentation, an archive of frequently asked questions and answers, and an active site to which registered AIJ users may contribute. The | This wiki offers open access to curated documentation, an archive of frequently asked questions and answers, and an active site to which registered AIJ users may contribute. The [http://astroimagej.170.s1.nabble.com/ discussion forum] remains available at this time, an archive of its contents is here too, while this site is a source for up to date guidance and advice on the use of AIJ at all levels. | ||
* [https://www.astro.louisville.edu/software/astroimagej/mediawiki-1.37.2/index.php/Special:WikiForum New AIJ Wiki forum] | * [https://www.astro.louisville.edu/software/astroimagej/mediawiki-1.37.2/index.php/Special:WikiForum New AIJ Wiki forum] | ||
* [https://www.astro.louisville.edu/software/astroimagej/aijnabble | * [https://www.astro.louisville.edu/software/astroimagej/aijnabble Local archive of the Nabble forum] | ||
* [https://www.astro.louisville.edu/software/astroimagej/mediawiki-1.37.0/index.php/Special:AllPages Index to pages on the AIJ Wiki] | * [https://www.astro.louisville.edu/software/astroimagej/mediawiki-1.37.0/index.php/Special:AllPages Index to pages on the AIJ Wiki] | ||
* [https://www.astro.louisville.edu/software/astroimagej/mediawiki-1.37.0/index.php/Special:Search Search this Wiki] | * [https://www.astro.louisville.edu/software/astroimagej/mediawiki-1.37.0/index.php/Special:Search Search this Wiki] | ||
Line 17: | Line 17: | ||
Select the "Request account" option at the upper right if you want to join here, or use these forms. | Select the "Request account" option at the upper right if you want to join here, or use these forms. | ||
* [https://docs.google.com/forms/d/13f4rpjcwjyNbOFsNxsTZcqtJD1TAGUnpizruAepwtoc/edit Request a user account | * [https://docs.google.com/forms/d/13f4rpjcwjyNbOFsNxsTZcqtJD1TAGUnpizruAepwtoc/edit Request a user account to contribute to the forum and content] | ||
* [https://docs.google.com/forms/d/1hZ_zf8Ul9KKygUsJXzZ-2OLJnhXnpXha8a_Hj7fl9ds/edit Submit a question or comment | * [https://docs.google.com/forms/d/1hZ_zf8Ul9KKygUsJXzZ-2OLJnhXnpXha8a_Hj7fl9ds/edit Submit a question or comment] | ||
Our main website provides access to the software. | Our main website provides access to the software. | ||
* [https://www.astro.louisville.edu/software/astroimagej/ Download and install the most recent version for Windows, Mac, and Linux] | * [https://www.astro.louisville.edu/software/astroimagej/ Download and install the most recent version for Windows, Mac, and Linux] |
Revision as of 03:44, 16 June 2022
AstroImageJ
AstroImageJ (AIJ) provides an astronomy-specific friendly graphical environment and tools for accurate precision image calibration and analysis. It is focused on processing for spectrophotometric data from ground-based and space-based resources providing Flexible Image Transport (FITS) files of raw and previously calibrated images. AIJ includes tools for accurate time-based measurements and will generate light curves from aperture photometry as well as fitted profiles for exoplanet transits. Its users include
- Astronomers of all kinds, professional, academic and amateur, who prefer a modern, well-documented and validated processing tool also compatible with command-line and Python scripting for interactive processing and analysis of their data
- Students and anyone interested in astronomy who want a tool to visualize and explore "real" images and data from public archives for HST, JWST, and their own telescopes
- Developers who may use the flexibility of an open source ImageJ core with the option to add modules of their own devising
Although AIJ maintains the general purpose image processing capabilities of ImageJ, AIJ is streamlined for time-series differential photometry, light curve detrending and fitting, and light curve plotting, especially for applications requiring ultra-precise light curves (e.g., exoplanet transits). Its interactive image display is designed for astronomical applications. It reads and writes standard Flexible Image Transport System (FITS) files, as well as other common image formats, provides FITS header viewing and editing, and is World Coordinate System aware, including an automated interface to the astrometry.net web portal for plate solving images. AIJ provides research-grade image calibration and analysis tools with a GUI driven approach, and is easily installed with cross-platform compatibility. It enables new users, even at the level of undergraduate student, high school student, or amateur astronomer, to quickly start processing, modeling, and plotting astronomical image data with one tightly integrated software package that works on laptops and servers alike.
This wiki offers open access to curated documentation, an archive of frequently asked questions and answers, and an active site to which registered AIJ users may contribute. The discussion forum remains available at this time, an archive of its contents is here too, while this site is a source for up to date guidance and advice on the use of AIJ at all levels.
- New AIJ Wiki forum
- Local archive of the Nabble forum
- Index to pages on the AIJ Wiki
- Search this Wiki
Select the "Request account" option at the upper right if you want to join here, or use these forms.
Our main website provides access to the software.