The position angles determined from galmag
are in the range 
-
.
They do not go all the way to 
,
since 
the major axis
of a galaxy does not have a positive and a negative direction,
as opposed to for example a coordinate axis.
If a galaxy has an isophote twist, i.e. the position angle changes with
the radius r, the position angle might cross the upper or lower limit of
or  
,
respectively, and thereby appearing
discontinuous. This is in a way a cosmetical problem. Since the
position angle is only determined to within a factor of 
,
we can 
add or subtract 
at certain radii 
to make the profile look continuous.
This was done using the task pa1shift. 
An example of this is shown in Figure 
.
 
Properties of E and S0 Galaxies in the Clusters HydraI and Coma
Master's Thesis, University of Copenhagen, July 1997![]()
Bo Milvang-Jensen (milvang@astro.ku.dk)