Narrow Diffuse Interstellar Bands: A Survey with Precise Wavelengths

By G. Galazutdinov, F. Musaev, J. Krełowski, G. Walker. 2000

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STUDIES OF THE DIFFUSE INTERSTELLAR BANDS. III. HD 183143 (2009, unknown): “A number of atomic and (diatomic) molecular interstellar lines are also present in the spectrum of HD 183143 (Gredel et al. 1993; Galazutdinov et al. 2000a; McCall et al. 2002).”
ON THE SOURCE OF THE DUST EXTINCTION IN TYPE Ia SUPERNOVAE AND THE DISCOVERY OF ANOMALOUSLY STRONG Na i ABSORPTION (2013, background): “The rest wavelength of the 5780 Å DIB is also not very accurately known, with the uncertainty corresponding to 10–15 km s−1 in radial velocity (e.g., Galazutdinov et al. 2000; Tuairisg et al. 2000; Hobbs et al. 2008, 2009).”
A Catalog of Diffuse Interstellar Bands in the Spectrum of HD 204827 (2008, methodology): “…of Table 2 present the central wavelengths, as reported by the previous authors, of those DIBs detected in our spectra that had already been noted in one or more of the DIB atlases compiled by Jenniskens &Desert (1994), Galazutdinov et al. (2000), Tuairisg et al. (2000), orWeselak et al. (2000).”