Trend Filtering -- I. A Modern Statistical Tool for Time-Domain
  Astronomy and Astronomical Spectroscopy
  The problem of denoising a one-dimensional signal possessing varying degrees
of smoothness is ubiquitous in time-domain astronomy and astronomical
spectroscopy. For example, in the time domain, an astronomical object may
exhibit a smoothly varying intensity that is occasionally interrupted by abrupt
dips or spikes. Likewise, in the spectroscopic setting, a noiseless spectrum
typically contains intervals of relative smoothness mixed with localized higher
frequency components such as emission peaks and absorption lines. In this work,
we present trend filtering, a modern nonparametric statistical tool that yields
significant improvements in this broad problem space of denoising $spatially$
$heterogeneous$ signals. When the underlying signal is spatially heterogeneous,
trend filtering is superior to any statistical estimator that is a linear
combination of the observed data---including kernel smoothers, LOESS, smoothing
splines, Gaussian process regression, and many other popular methods.
Furthermore, the trend filtering estimate can be computed with practical and
scalable efficiency via a specialized convex optimization algorithm, e.g.
handling sample sizes of $n\gtrsim10^7$ within a few minutes. In a companion
paper, we explicitly demonstrate the broad utility of trend filtering to
observational astronomy by carrying out a diverse set of spectroscopic and
time-domain analyses.
