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2023PASP..135k4504A - Publ. Astron. Soc. Pac., 135, part no 11, 4504 (2023/November-0)

Methods for Averaging Spectral Line Data.

ANDERSON L.D., LIU B., BALSER D.S., BANIA T.M., HAFFNER L.M., LINVILLE D.J., LUISI M. and WENGER T.V.

Abstract (from CDS):

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 (S/N), 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 S/N is maximized when all spectra are averaged, for noise and uniform weighting we find that averaging the 35%-45% of spectra with the highest S/N results in the highest S/N 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 hydrogen radio recombination line data to determine the ionic abundance ratio, y+, and discuss future applications of the methodology.

Abstract Copyright: © 2023. The Author(s). Published by IOP Publishing Ltd on behalf of the Astronomical Society of the Pacific (ASP). All rights reserved

Journal keyword(s): Computational methods - Warm ionized medium

Simbad objects: 1

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