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| NCSA Astronomy Digital Image Library User's Guide | ||||
The aim of the ADIL is to increase the astronomers' productivity through easy access to data. There are a number of ways in which a vast collection of research--ready images could be a powerful research tool:
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Observers planning a new project can access previous observations to aid with sensitivity calculations or exploring new questions to be addressed. |
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New data can be compared with previous observations as part of a multi-frequency study of particular objects. |
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The availability of electronic versions of images and related figures will help astronomers in preparing figures for talks or papers. |
The Library provides advantages not just to users looking for images but also to authors who contribute their images to the Library's collection:
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The ADIL provides a convenient way for astronomers to archive their final, processed images and related data; getting the data back is a click away without having to mess with tapes. |
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It is also a convenient way to share data with collaborators and colleagues without locking up disk space on one's own Web or FTP site. |
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the Library offers another way to present scientific results complementary to the printed journal. For instance, after spending a paragraph describing a complex feature in the data, one could direct the reader to a URN in the Library to view an animation or VRML visualization. |
There are also obvious benefits to the general public, as demonstrated by our recent ``visitor statistics''. The Library is an easy and fun way for people to learn what is new in astronomy. With wide variety of images in the collection, it is fairly simple to gather together a subset of images for an exhibit for non-astronomers.
Clearly, no library can be effective without "books". We are relying on the astronomical community to help build up the collection. We hope that the benefits of contributing images will be obvious and that authors will make it a routine part of the process of presenting scientific results.
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