 or both temperature and 
polarisation coefficients
 or both temperature and 
polarisation coefficients 
 ,
, 
 ,
, 
 ,
, 
 (and
 (and  
 ,
, 
 ,
, 
 ,
, 
 ,
, 
 when applicable). If the 
keyword PDMTYPE is found in the header, fits2cl assumes the table to be in the 
special format used by Planck and will ignore the first data column. 
If the input FITS file contains several
extensions or HDUs, the one to be read can be specified thanks to the CFITSIO 
Extended File Name Syntax, using its number (eg, file.fits[2] or file.fits+2) or its
EXTNAME value (eg. file.fits[beam_100x100]). By default, only the first valid
extension will be read.
 when applicable). If the 
keyword PDMTYPE is found in the header, fits2cl assumes the table to be in the 
special format used by Planck and will ignore the first data column. 
If the input FITS file contains several
extensions or HDUs, the one to be read can be specified thanks to the CFITSIO 
Extended File Name Syntax, using its number (eg, file.fits[2] or file.fits+2) or its
EXTNAME value (eg. file.fits[beam_100x100]). By default, only the first valid
extension will be read.
call fits2cl*( filename, clin, lmax, ncl, header, [units] )
Reads a power spectrum from the FITS file `cl.fits' and stores the result in cl(0:lmax,1:ncl) which are the nclcoefficients up to
lmax. The FITS header is returned in header, the column units in units.
 values
  from an input power spectrum.
 values
  from an input power spectrum.
  
Version 3.83, 2024-11-13