Astrophysics (Index)About

spectral feature

(feature)
(recognizable feature of a spectrum)

The term spectral feature is a catch-all for any recognizable feature (i.e., detail) of a spectrum. If it provides specific evidence of some characteristic of the source, the term spectral signature applies. It might refer to an emission line or absorption line, or the line shape, or a spectral band. Examples include a Balmer jump, a vegetation red edge or a Compton hump. Some lines are common in galaxies and recognizable even when redshifted, offering a means to estimate distance using the Hubble constant.

The phrase spectral feature extraction is used in discussions of computer techniques aimed at analyzing spectra, allowing and population groupings and examples of specific phenomena to be selected from extensive survey data. Machine learning (ML) methods are of interest.


(spectrography)
Further reading:
http://www.lamost.org/public/node/256?locale=en
https://dictionary.obspm.fr/index.php?showAll=1&formSearchTextfield=spectral+feature
https://ui.adsabs.harvard.edu/abs/2018PASP..130h4203K/abstract

Referenced by pages:
Balmer jump (BJ)
Balmer-break galaxy (BBG)
brightness temperature (TB)
chemically peculiar star (CP star)
Compton reflection
continuum
emission line galaxy (ELG)
extinction
galaxy age determination
Gunn-Peterson trough
H-alpha (Ha)
hypergiant
LB-1
Lick indices
lithium (Li)
Lyman break (LB)
Lyman continuum (LyC)
non-thermal emission
P Cygni profile
photometric redshift (photo-z)
radio galaxy (RG)
reddening
self-absorption
spectral class
spectral signature
spectral temperature
spectral type
starburst galaxy
stellar atmosphere
stellar luminosity determination
stellar temperature determination
stripped star
telluric star
temperature
thermal emission
Thomson optical depth (τT)
vegetation red edge (VRE)
Wien's displacement law
Y-type star (Y)

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