The UVKLIB spectral library (A.J. Pickles, PASP 110, 863, 1998) provides spectra for different spectral types in the domain 115nm - 2500nm with a step size of 0.5 nm.
Kurucz model spectra cover the range 100nm - 1100nm with a step size of 0.1 nm.
The planetary nebula spectrum corresponds to NGC 7009, Emiss. lines from Hyung & Aller, 1995; Barker, 1983. Produced by J. R. Walsh (Space Telescope European Coordinating Facility), May 1996. This spectrum cover the range 100nm - 1100nm
Orion nebula is a composite spectrum. UV lines, optical lines, nebular continuum plus hot star model atmospheres. Produced by J. R. Walsh (Space Telescope European Coordinating Facility), May 1996. This spectrum covers the range 100nm - 1100nm.
The Kinney-Calzetti atlas contains spectral templates of galaxies covering the ultraviolet to near-infrared spectral range, i.e. from 120nm up to around 993nm. The following list of templates have been selected from the atlas.
File Name Spectral coverage Comments
(angstroms)
elliptical 1235 - 9935 -
s0 1235 - 9940 -
sa 1235 - 9940 -
sb 1235 - 9940 -
starb1 1235 - 9945 starburst with E(B-V) < 0.1
starb2 1235 - 9945 starburst with 0.11 < E(B-V) < 0.21
starb3 1235 - 9945 starburst with 0.25 < E(B-V) < 0.35
starb4 1235 - 9945 starburst with 0.39 < E(B-V) < 0.50
starb5 1235 - 9945 starburst with 0.51 < E(B-V) < 0.60
starb6 1235 - 9945 starburst with 0.61 < E(B-V) < 0.70
Calzetti, D., Kinney, A.L. & Storchi-Bergmann, T. 1994, ApJ 429, 582
Kinney, A.L., Calzetti, D., Bohlin, R.C., McQuade, K., Storchi-Bergmann, T. & Schmitt, H.R. 1996, ApJ August issue
The MARCS set of spectra was made using the one-dimensional, hydrostatic, plane-parallel LTE model atmospheres (https://marcs.astro.uu.se) for stars in the temperature range 3,000 to 8,000 K and log g = 3 to 5. Only models with solar metallicity and microturbulence = 2 km/s were considered.
They were used as input to the Spectrum stellar spectral synthesis program to compute flux calibrated spectra, in the wavelength range from 3,00 to 20,000 nm, with a resolution of 0.001 nm.
These spectra were then rebinned logarithmically to a final resolution of 200,000 using SpectRes. It is a pleasure to thank Dr. Richard O. Gray from the Appalachian State University for adapting his code and providing the necessary line lists.
Please refer to the PHOENIX web page. The wavelength range supported is from 50nm to 5.5μm.
Please refer to the SWIRE web page