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Last modified: March 15, 2001
FITSML for Flexible Image Transport System

[March 15, 2001] The FITSML is an XML/XDF language rendition of the Flexible Image Transport System that is used primarily in astronomy. A pre-draft FITSML DTD is available, along with sample documents.

"The Flexible Image Transport System, or FITS, is the format adopted by the astronomical community for data interchange and archival storage. The FITS Support Office is responsible for documenting the FITS standard, participating in its evolution, and advising NASA astrophysics missions on how to present their data in FITS format.

"FITS (Flexible Image Transport System) is a data format designed to provide a means for convenient exchange of astronomical data between installations whose standard internal formats and hardware differ. A FITS data file is composed of a sequence of Header Data Units (HDUs). The header consists of keyword=value statements, which describe the organization of the data in the HDU and the format of the contents. It may provide additional information, for example, about instrument status or the history of the data. The data follow, structured as the header specifies. The data section of the HDU may contain a digital image, but, except for the first HDU, it doesn't have to. Other possible formats include tables and multidimensional matrices that are not images. An HDU need not contain data. If the first HDU contains data, they must be organized as an array of one or more dimensions; in subsequent HDUs, called extensions, other organizations are possible, consistent with certain rules. The 'Image' in FITS comes from the original use of the format to transport digital images, but it's not just for images any more."

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