stilts tcube in=2QZ_6QZ_pubcat.fits out=ccm.fits \ cols='Bj_R U_Bj Bj' binsizes='0.05 0.05 0.5' bounds='-2:1 -3:2 :'
stilts tcube in=iras_psc.vot out=flux60_map.fits \ icmd='addskycoords fk5 galactic ra dec glat glon' \ cols='glat glon' nbins='400 200' \ scale=Fnu_60 combine=sum
Fnu_60
fluxes
from objects in that rectangle of (glat,glon>
space.
Bounds are determined automatically from the data, and the number of
pixels in each dimension (400 in latitude and 200 in longitude) are
specified, which means that the pixel sizes don't have to be.
Since the input table contains sky positions in equatorial
coordinates rather than galactic ones, the addskycoords
filter is used to preprocess the data before the cube generation
step (see Section 6.1).