A Uniform Database of 2.4-45.4 Micron Spectra from the Infrared Space Observatory Short Wavelength Spectrometer

By G. Sloan, K. Kraemer, S. Price, R. Shipman. 2003

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A NEW CLASS OF LUMINOUS TRANSIENTS AND A FIRST CENSUS OF THEIR MASSIVE STELLAR PROGENITORS (2008, methodology): “The MIR magnitudes and colors forη-Carina, VY CMa, and NML Cyg were synthesized from ISO spectra (Sloan et al. 2003).”
The Dust Cloud around the White Dwarf G29-38 (2005, background): “—Continuum-subtracted spectrum of the silicate feature from G2939, compared to similarly subtracted silicate features of the diffuse ISM, the O-rich star Mira, comet Hale-Bopp, and the zodiacal light.”
Fundamental parameters and infrared excesses of Hipparcos stars (2012, methodology): “…Satellite Low-Resolution Spectrometer (IRAS LRS) and Infrared Space Observatory Short Wavelength Spectrometer (ISO SWS) spectra of these sources are also given (Sloan & Price 1998; Sloan, Little-Marenin & Price 1998; Sloan et al. 2003; based on the classification method of Kraemer et al. 2002).”