Bootstrap in some Non-standard
Problems
The talk will
consider some issues with the consistency of different bootstrap methods for
constructing confidence intervals in two non-standard problems characterized by
shape restricted estimation. The study of consistency of bootstrap methods in
these problems is motivated by the problem of estimation of dark matter in
dwarf spheroidal galaxies in Astronomy.
The Grenander estimator, the nonparametric maximum likelihood
estimator of an unknown non-increasing density function f on [0, ∞), is a
prototypical example of a class of shape constrained estimators that converge
at rate cube-root n. We focus on this example and illustrate different
approaches of constructing confidence intervals for f(t0), for 0 <
t0 < ∞. It is
claimed that the bootstrap estimate of the sampling distribution of the Grenander estimator, when generating bootstrap samples from
the empirical distribution function (e.d.f.) or its
least concave majorant (the maximum likelihood
estimate), does not have any weak limit, conditional on the data, in
probability.
The other problem
arises in Astronomy and is similar to the Wicksell’s
Corpuscle problem (1925, Biometrika). We observe (X1,X2), the first two co-ordinates of a three
dimensional spherically symmetric random vector (X1,X2,X3). Interest focuses on estimating F, the distribution
function of
X
+ X
+ X
. This
gives rise to an inverse problem with missing data. We propose two estimators
of F and
derive their limit distributions.
Although the normalized estimators of F converge to a normal distribution, the non-standard
asymptotics involved with the non-standard rate of convergence
, cast doubt on the consistency of bootstrap methods. We
focus on bootstrapping from the e.d.f. of data, and
show that both the estimates can be bootstrapped consistently. A comparison of
the two examples sheds light on some of the reasons for the (in)-consistency of
bootstrap methods.
_________________
*This is joint work with Moulinath Banerjee and Michael Woodroofe