Light curve completion and forecasting using fast and scalable Gaussian
processes (MuyGPs)
- URL: http://arxiv.org/abs/2208.14592v1
- Date: Wed, 31 Aug 2022 01:52:00 GMT
- Title: Light curve completion and forecasting using fast and scalable Gaussian
processes (MuyGPs)
- Authors: Im\`ene R. Goumiri, Alec M. Dunton, Amanda L. Muyskens, Benjamin W.
Priest, Robert E. Armstrong
- Abstract summary: Ground-based observations from commercial off the shelf (COTS) cameras remain inexpensive compared to higher precision instruments.
limited sensor availability combined with noisier observations can produce gappy time-series data.
Deep Neural Networks (DNNs) have become the tool of choice due to their empirical success at learning complex nonlinear embeddings.
- Score: 0.0
- License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
- Abstract: Temporal variations of apparent magnitude, called light curves, are
observational statistics of interest captured by telescopes over long periods
of time. Light curves afford the exploration of Space Domain Awareness (SDA)
objectives such as object identification or pose estimation as latent variable
inference problems. Ground-based observations from commercial off the shelf
(COTS) cameras remain inexpensive compared to higher precision instruments,
however, limited sensor availability combined with noisier observations can
produce gappy time-series data that can be difficult to model. These external
factors confound the automated exploitation of light curves, which makes light
curve prediction and extrapolation a crucial problem for applications.
Traditionally, image or time-series completion problems have been approached
with diffusion-based or exemplar-based methods. More recently, Deep Neural
Networks (DNNs) have become the tool of choice due to their empirical success
at learning complex nonlinear embeddings. However, DNNs often require large
training data that are not necessarily available when looking at unique
features of a light curve of a single satellite.
In this paper, we present a novel approach to predicting missing and future
data points of light curves using Gaussian Processes (GPs). GPs are non-linear
probabilistic models that infer posterior distributions over functions and
naturally quantify uncertainty. However, the cubic scaling of GP inference and
training is a major barrier to their adoption in applications. In particular, a
single light curve can feature hundreds of thousands of observations, which is
well beyond the practical realization limits of a conventional GP on a single
machine. Consequently, we employ MuyGPs, a scalable framework for
hyperparameter estimation of GP models that uses nearest neighbors
sparsification and local cross-validation. MuyGPs...
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