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1.1.1 Convert the image to a FITS file
Description
This function converts the image into a FITS file.
If the image has a rest frequency associated with it, it will always write velocity information into the FITS file. By default the frequency information will be primary as it is better defined than velocity information. If you select velocity=T then by default the velocity is written in the optical convention, but if optical=F it will use the radio convention instead.
The FITS definition demands equal increment pixels. Therefore, if you write velocity information as primary and use the optical velocity definition, the increment is computed at the spectral reference pixel. If the bandwidth is large, this may incur non-negligible coordinate calculation errors far from the reference pixel.
By default the image is written as a floating point FITS file (bitpix= -32). Under rare circumstances you might want to save space and write it as scaled 16 bit integers (bitpix = 16). You can have tofits calculate the scaling factors by using the default minpix and maxpix. If you set minpix and maxpix, values outside of that range will be truncated. This can be useful if all of the FITS images dynamic range is being used by a few high or low values and you are not interested in preserving those values exactly. Besides the factor of two space savings you get by using 16 instead of 32 bits, integer images usually also compress well (for example, with the standard GNU software facility gzip).
If the specified region-of-interest extends beyond the image, it is truncated.
The output mask is the combination (logical OR) of the default input pixel mask (if any) and the OTF mask.
Sometimes it is useful to drop axes of length one (degenerate axes) because not all FITS readers can handle them. Use the dropdeg argument if you want to do this.
Arguments
| Inputs |
| ||
| outfile |
| FITS file name. Default is input name + ’.fits’
| |
| allowed: | string |
|
| Default: |
|
|
| velocity |
| prefer velocity (rather than frequency) as primary
spectral axis?
| |
| allowed: | bool |
|
| Default: | false |
|
| optical |
| use the optical (rather than radio) velocity convention?
| |
| allowed: | bool |
|
| Default: | true |
|
| bitpix |
| Bits per pixel, -32 (floating point) or 16 (integer)
| |
| allowed: | int |
|
| Default: | -32 |
|
| minpix |
| Minimum pixel value for BITPIX=16, Default is to
autoscale if minpix ¿ maxpix.
| |
| allowed: | double |
|
| Default: | 1 |
|
| maxpix |
| Maximum pixel value for BITPIX=16, Default is to
autoscale if maxpix ¡ minpix.
| |
| allowed: | double |
|
| Default: | -1 |
|
| region |
| The region of interest. Default is whole image.
| |
| allowed: | any |
|
| Default: | record |
|
| mask |
| OTF mask, Boolean LEL expression or mask region
Default is none.
| |
| allowed: | any |
|
| Default: | variant |
|
| overwrite |
| Overwrite (unprompted) pre-existing output file?
| |
| allowed: | bool |
|
| Default: | false |
|
| dropdeg |
| Drop degenerate axes?
| |
| allowed: | bool |
|
| Default: | false |
|
| deglast |
| Put degenerate axes last in header?
| |
| allowed: | bool |
|
| Default: | false |
|
| async |
| Run asynchronously?
| |
| allowed: | bool |
|
| Default: | false |
|
Example
"""
# print "\t----\t tofits Ex 1 \t----" ia.maketestimage() ok = ia.tofits(’MYFILE.FITS’,overwrite=true) # write FITS image file ok = ia.tofits(’MYFILE2.FITS’, bitpix=16, overwrite=true) # Write as scaled 16 bit integers ia.close() # """ |
Please send any comments or questions about CASA or AIPS++ to aips2-requests@nrao.edu
Copyright © 2007 Associated Universities Inc., Washington, D.C.
This code is available under the terms of the GNU General Public Lincense
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Updated daily during alpha development.