Spectral atlas

In astronomy, a spectral atlas is a collection of spectra of one or more objects, intended as a reference work for comparison with spectra of other objects. Several different types of collections are titled spectral atlases: those intended spectral classification, for key reference or as a collection of spectras of a general type of object.

In any spectral atlas, generally all the spectra have been taken with the same equipment, or with very similar instruments at different locations, to provide data as uniform as possible in its spectral resolution, wavelength coverage, noise characteristics, etc.

Types

For spectral classification

When assigning a spectral classification, a spectral atlas is a collection of standard spectra of stars with known spectral types, against which a spectrum of an unknown star is compared. It is analogous to an identification key in biology. Originally, such atlases included reproductions of the monochrome spectra as recorded on photographic plates, as in the original Morgan-Keenan-Kellman atlas[1] and other atlases.[2] These atlases include identifications and notations for use of those spectral features to be used as discriminators between close spectral types. With very large surveys of the sky which include automated assignment of spectral classification from the digital spectra data, graphical atlases have been supplanted by libraries of spectra of standard stars which often can be downloaded from VizieR and other sources.

For key reference

A spectral atlas can be a very high-quality spectrum of a key reference object, often made with very high spectral resolution, generally presented in large-format graphical form as a line chart (but normally strictly without markers at specific data points) of intensity or relative intensity (which for a star whose spectrum is dominated by absorption lines runs from zero to a normalized continuum) as a function of wavelength. Such spectral atlases have been made several times for the Sun (e.g.,[3][4][5]), Arcturus, other bright stars, planets, quasars, etc. Unlike classification atlases, such atlases made from data taken with photographic media were digitized with a densitometer and the digitized result is presented. Sometimes these atlases include identifications of spectral features, but often such identifications are presented in tabular form in separate publications (e.g.,[6]).

For objects of a general type

A spectral atlas can be a collection of spectra of different individual objects of a general type, showing the variety of spectra inherent to the type, or a collection of spectra from a single object that varies over time, showing the variations in the spectra.

Notes

  1. ↑ Morgan, W. W.; Keenan, P. C.; Kellman, Edith (1943). An atlas of stellar spectra, with an outline of spectral classification. Chicago: The University of Chicago Pres. Bibcode:1943assw.book.....M.
  2. ↑ Yamashita, Yasumasa; Nariai, Kyoji (1977). An Atlas of representative stellar spectra. Tokyo: University of Tokyo Press. Bibcode:1977aars.book.....Y.
  3. ↑ Delbouille, L.; Roland, G.; Neven, L. (1973). Atlas photometrique DU spectre solaire de λ3000 a λ10000. Liège: Universite de Liège, Institut d'Astrophysique. Bibcode:1973apds.book.....D.
  4. ↑ Kurucz, Robert L.; Furenlid, Ingemar; Brault, James; Testerman, Larry (1984). Solar flux atlas from 296 to 1300 nm. Sunspot, New Mexico: National Solar Observatory. Bibcode:1984sfat.book.....K.
  5. ↑ Delbouille, L.; Roland, G.; Neven, L. (1990). Atlas photometrique DU spectre solaire de λ3000 a λ10000, vol. 2. Liège: Universite de Liège, Institut d'Astrophysique. Bibcode:1990apds.book.....D.
  6. ↑ Moore, C. E.; Minnaert, M. G. J.; Houtgast, J. (1966). The solar spectrum 2935Å to 8770Å. Washington: US Government Printing Office. Bibcode:1966sst..book.....M.
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