Research Article

A Characterization of the Diffuse Galactic Emissions in the Anticenter of the Galaxy

Figure 2

Temperature maps ( ) for the ARCHEOPS data (left), the thermal dust emission model (center), and residuals (right). From top to bottom, we present the 545, 353, 217, and 143 GHz maps.
746020.fig.002a
(a)
746020.fig.002b
(b)
746020.fig.002c
(c)
746020.fig.002d
(d)
746020.fig.002e
(e)
746020.fig.002f
(f)
746020.fig.002g
(g)
746020.fig.002h
(h)
746020.fig.002i
(i)
746020.fig.002j
(j)
746020.fig.002k
(k)
746020.fig.002l
(l)
746020.fig.002m
(m)
746020.fig.002n
(n)
746020.fig.002o
(o)
746020.fig.002p
(p)
746020.fig.002q
(q)
746020.fig.002r
(r)