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5.1.2.1 fits

FITS is a very well-established format for storage of astronomical table or image data (see https://fits.gsfc.nasa.gov/). This writer stores tables in BINTABLE extensions of a FITS file.

There are a number of variations in exactly how the table data is written to FITS. These can be configured with name=value options in brackets as described below, but for most purposes this isn't required; you can just choose fits or one of the standard aliases for commonly-used combinations like colfits or fits-basic.

In all cases the output from this handler is legal FITS, but some non-standard conventions are used:

fits-plus
In "fits-plus" format, the primary HDU contains an array of bytes which stores the full table metadata as the text of a VOTable document, along with headers that indicate this has been done. Most FITS table readers will ignore this altogether and treat the file just as if it contained only the table. When it is re-read by this or compatible applications however, they can read out the metadata and make it available for use. In this way you can store your data in the efficient and widely portable FITS format without losing the additional metadata such as table parameters, column UCDs, lengthy column descriptions etc that may be attached to the table. This variant, which is the default, can be explicitly selected with the primary=votable option or fits-plus alias (if you don't want it, use primary=basic or fits-basic). This convention is described in more detail in Section 5.1.3.1.
colfits
In Column-Oriented FITS output, the HDU containing the table data, instead of containing a multi-row table, contains a single-row table in which each cell is an (nrow-element) array containing the data for an entire column. The point of this is to keep all the data for a single row localised on the disk rather than scattered through the whole file. This can be more efficient for certain applications, especially when the table is larger than physical memory, and has many columns of which only a few are needed for a particular task, for instance plotting two columns against each other. The overhead for writing this format is somewhat higher than for normal (row-oriented) FITS however, and other FITS table applications may not be able to work with it, so in most cases normal FITS is a better choice. This variant can be selected with the col=true option or the colfits-plus/colfits-basic aliases. If you write to a file with the ".colfits" extension it is used by default.
wide
A private convention is used where required to support encoding of tables with more than 999 columns, which is not possible in standard FITS. If software unaware of this convention (e.g. CFITSIO) is used to read such tables, it will only see the first 998 columns written as intended, plus a column 999 containing an undescribed byte buffer where the rest of the column data is stored. This convention is described in more detail in Section 5.1.3.2.

For convenience, and compatibility with earlier versions, these standard aliases are provided:

fits-plus
Alias for fits or fits(primary=votable).
fits-basic
Alias for fits(primary=basic).
fits-var
Alias for fits(primary=basic,var=true).
colfits-plus
Alias for fits(col=true).
colfits-basic
Alias for fits(col=true,primary=basic).
fits-healpix
This is a special case. It is used for storing HEALPix pixel data in a way that conforms to the HEALPix-FITS serialization convention. In most ways it behaves the same as fits-basic, but it will rearrange and rename columns as required to follow the convention, and it will fail if the table does not contain the required HEALPix metadata (STIL_HPX_* parameters).

The handler behaviour may be modified by specifying one or more comma-separated name=value configuration options in parentheses after the handler name, e.g. "fits(primary=basic,col=false)". The following options are available:

primary = basic|votable[n.n]|none
Determines what is written into the Primary HDU. The Primary HDU (PHDU) of a FITS file cannot contain a table; the following options are available.
basic
A minimal PHDU is written with no interesting content
votable[n.n]
The PHDU contains the full table metadata as the text of a VOTable document, along with headers to indicate that this has been done. This corresponds to the "fits-plus" format. The "[n.n]" part is optional, but if included (e.g. "votable1.5") indicates the version of the VOTable format to use.
none
No PHDU is written. The output is therefore not a legal FITS file, but it can be appended to an existing FITS file that already has a PHDU and perhaps other extension HDUs.
(Default: votable)
col = true|false
If true, writes data in column-oriented format. In this case, the output is a single-row table in which each cell is an array value holding the data for an entire column. All the arrays in the row have the same length, which is the row count of the table being represented. This corresponds to the "colfits" format. (Default: false)
var = FALSE|TRUE|P|Q
Determines how variable-length array-valued columns will be stored. True stores variable-length array values after the main part of the table in the heap, while false stores all arrays as fixed-length (with a length equal to that of the longest array in the column) in the body of the table.The options P or Q can be used to force 32-bit or 64-bit pointers for indexing into the heap, but it's not usually necessary since a suitable choice is otherwise made from the data. (Default: FALSE)
date = true|false
If true, the DATE-HDU header is filled in with the current date; otherwise it is not included. (Default: true)

Multiple tables may be written to a single output file using this format.

If no output format is explicitly chosen, writing to a filename with the extension ".fits", ".fit" or ".fts" (case insensitive) will select fits format for output.


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STILTS - Starlink Tables Infrastructure Library Tool Set
Starlink User Note256
STILTS web page: http://www.starlink.ac.uk/stilts/
Author email: m.b.taylor@bristol.ac.uk
Mailing list: topcat-user@jiscmail.ac.uk