3.4. Properties of VELMOD Likelihood
The mock catalogs may be used to
illustrate some important features of the VELMOD analysis also. An example
of these is shown in Figure 3. The left-hand
panel
shows forw
versus
I
for one of the 20 catalogs. The right-hand panels show how three other
quantities vary
with
I
in the same VELMOD run: the amplitude of the LG random velocity
wLG (top panel), the velocity noise
v (middle
panel), and the TF
scatter
TF
for each of the two mock TF samples
(A82 and
MAT)
considered (bottom panel). Note
first that the amplitude of the LG velocity vector is minimized near the
true value
of
I.
This generally was seen in the mock catalogs; it reflects the fact that the
fits at the wrong values
of
I
try to compensate for wrong peculiar velocity predictions with Local Group
motion. If wLG
was held fixed at its maximum likelihood value, or set equal to zero,
the
forw
versus
I
curves would have sharper minima, and
the
-uncertainty
would be reduced (cf. Section 4.5).
Unfortunately, we
cannot do this for the real universe because we do not know
wLG a priori. Nevertheless, there we will find similar
behavior; wLG has a minimum near the best-fit value
of
I
for the real universe.
![]() |
Figure 3. Some
of the parameters obtained from running VELMOD on a single mock catalog.
The left-hand panel shows the likelihood statistic along with the cubic fit
used to determine its minimum. The right-hand panels show the amplitude of
the Local Group random velocity vector, the velocity noise
|