We expect the
x- and
y-locations,
X N,A (
t) and
Y N,A (
t), of the observer's centroid estimates to deviate from
N,A (
t) and
N,A (
t) for two reasons; first, the responses will be degraded by noise. Additionally, we expect that observers may not combine information about disparate dots precisely according to
Equation A1. We anticipate that the weight given a particular dot
z may deviate from
Equation A1 depending on the distance of
z from the true centroid. Specifically, we assume that the
x- and
y-locations of the observer's response on trial
t in condition (
N,
A) are given by
Equation 2 where the weight
w(
z) assigned to a given dot
z on trial
t is
for
R N,A as a function intended to capture biases in the weighting of central versus peripheral points in the dot cloud. Specifically, we estimate a parameter
α N,A to determine the distance correction factor
R N,A as follows:
R N,A is defined for −1 <
α N,A < 1. For
α N,A < 0,
R N,A is a decreasing function of the distance of a dot from (
N,A (
t),
N,A (
t)); thus, in this case, the bias introduced by
R N,A yields a “robust” estimator of the centroid—i.e., an estimator that gives most weight to dots near the middle of the cloud and is relatively immune to dots located in the periphery. The reverse is true if
α N,A > 0; in this case,
R N,A is an increasing function of distance, yielding an “anti-robust” estimator of the centroid that gives more weight to peripheral than to central dots in the cloud. In actuality, for
α N,A in a large neighborhood around 0,
R N,A is essentially constant across all dot distances in any of our displays; specifically, for
α N,A greater than around 0.025 and less than around 0.975, dots contribute to the centroid computation with weights that are roughly independent of their distance (in pixels) from (
N,A (
t),
N,A (
t)); that is, the computation is approximately a standard centroid (as given by
Equation A1).