diff --git a/docs/co_lines.rst b/docs/co_lines.rst index caf7ed57..5dc07e16 100644 --- a/docs/co_lines.rst +++ b/docs/co_lines.rst @@ -3,7 +3,7 @@ COLines ======= -This class implements simulations for Galactic CO emission involving the first 3 CO rotational lines, i.e. :math:`J=1-0,2-1,3-2` whose center frequency is respectively at :math:`\nu_0 = 115.3, 230.5,345.8` GHz. The CO emission map templates are the CO Planck maps obtained with ``MILCA`` component separation algorithm (See `Planck paper `). The CO maps have been released at the nominal resolution (10 and 5 arcminutes). However, to reduce noise contamination from template maps (especially at intermediate and high Galactic latitudes), we convolved them with a 1 deg gaussian beam. +This class implements simulations for Galactic CO emission involving the first 3 CO rotational lines, i.e. :math:`J=1-0,2-1,3-2` whose center frequency is respectively at :math:`\nu_0 = 115.3, 230.5,345.8` GHz. The CO emission map templates are the CO Planck maps obtained with ``MILCA`` component separation algorithm (See `Planck paper `_). The CO maps have been released at the nominal resolution (10 and 5 arcminutes). However, to reduce noise contamination from template maps (especially at intermediate and high Galactic latitudes), we convolved them with a 1 deg gaussian beam. The Stokes I map is computed from the template one as it follows: