Welcome and thank you for visiting! Here, you will find source code, news, and updates on the AIDA package developed mainly by Erik Hom in John Sedat's lab at UCSF, as described in J. Opt. Soc. Am. A 24:1580-1600.
AIDA is a de novo implementation and extension of the MISTRAL myopic deconvolution method developed by Mugnier et al.
(2004) [J. Opt. Soc. Am. A 21:1841-1854]. The MISTRAL approach, used
thus far to process astronomical images, has been shown to yield object
reconstructions with excellent edge preservation and photometric
precision. AIDA improves upon the original MISTRAL implementation in
the following ways:
AIDA runs on Mac OS 10.4 (including PowerPCs and IntelMacs), Windows 2000 and XP, and Linux (32- or 64-bit machines; AIDA was actually built and tested on Debian).
Importantly, you will need Python 2.4 installed on your system along with "Priithon" -- a free numerical Python platform developed and assembled by Sebastian Haase (Sedat Lab, UCSF). You may choose to download Priithon for your operating system here, or directly from the links below. (N.B. These are either .zip or .tbz archives and should be uncompressed using "gunzip [filename.zip]" or "tar -xjvf [filename.tbz]", respectively.)The AIDA package continues to be a work in progress (for better or worse, this code has undergone multiple re-writes/streamlining efforts). We provide this software as is and cannot guarantee support or assistance. However, feel free to email bug notices and constructive feedback; we will try to address concerns/requests as we are able (email: aida-feedback/at/freshboom/period/com).
For announcements about updates or additions to the software available here, please subscribe to the AIDA mailing list by sending mail to: aida-subscribe/at/freshboom/period/com.
last modified November 6, 2007
AIDA Development Team (aida-feedback/at/freshboom/period/com)