English

Methods for Averaging Spectral Line Data

Instrumentation and Methods for Astrophysics 2023-10-18 v3

Abstract

The ideal spectral averaging method depends on one's science goals and the available information about one's data. Including low-quality data in the average can decrease the signal-to-noise ratio (SNR), which may necessitate an optimization method or a consideration of different weighting schemes. Here, we explore a variety of spectral averaging methods. We investigate the use of three weighting schemes during averaging: weighting by the signal divided by the variance ("intensity-noise weighting"), weighting by the inverse of the variance ("noise weighting"), and uniform weighting. Whereas for intensity-noise weighting the SNR is maximized when all spectra are averaged, for noise and uniform weighting we find that averaging the 35-45% of spectra with the highest SNR results in the highest SNR average spectrum. With this intensity cutoff, the average spectrum with noise or uniform weighting has ~95% of the intensity of the spectrum created from intensity-noise weighting. We apply our spectral averaging methods to GBT Diffuse Ionized Gas (GDIGS) hydrogen radio recombination line (RRL) data to determine the ionic abundance ratio, y+, and discuss future applications of the methodology.

Keywords

Cite

@article{arxiv.2310.09076,
  title  = {Methods for Averaging Spectral Line Data},
  author = {L. D. Anderson and B. Liu and Dana S. Balser and T. M. Bania and L. M. Haffner and Dylan J. Linville and Matteo Luisi and Trey V. Wenger},
  journal= {arXiv preprint arXiv:2310.09076},
  year   = {2023}
}

Comments

Accepted by PASP

R2 v1 2026-06-28T12:49:49.563Z