52 datasets found

TLUSTY OSTAR2002 Grid: O-type stars, Teff = 27500K - 55000 K (Lanz, T., & Hubeny, I. 2003, ApJS, 146, 417)

Black Body flux. Teff from 10 to 200000 K

TLUSTY BSTAR2006 Grid: Early B-type stars, Teff = 15000K - 30000 K (Lanz, T., Hubeny, I. 2007, ApJS, 169, 83)

Husfeld et al models for non-LTE Helium-rich stars

TLUSTY OSTAR2002+BSTAR2006 Grid, The merged files use the BSTAR2006 models for effective temperatures up to 30,000 K and the OSTAR2002 models for higher temperatures.

The BT-COND Model grid of theoretical spectra. Brown dwarfs/extrasolar planets atmosphere models without irradiation and no dust opacity (no dust settling) but updated...

The BT-DUSTY Model grid of theoretical spectra. Brown dwarfs/extrasolar planets atmosphere models without irradiation but including dust opacity (fully efficient dust settling)...

The NextGen Model grid of theoretical spectra; Gas phase only, valid for Teff > 2700 K. Updated opacities. Wavelengths have been converted to air wavelengths.

The NextGen Model grid of theoretical spectra; Gas phase only, valid for Teff > 2700 K. Updated opacities. Wavelengths have been converted to air wavelengths.

The BT-Settl Model grid of theoretical spectra; With a cloud model, valid across the entire parameter range. Using AGSS2009 abundances. Wavelengths have been converted to air...

High resolution theoretical stellar spectra covering 250 to 900nm, fully described in Coelho (2014).

The BT-Settl Model grid of theoretical spectra; With a cloud model, valid across the entire parameter range. Wavelengths have been converted to air wavelengths.

The NextGen Model grid of theoretical spectra (only for solar metallicity)

Low resolution theoretical fluxes covering 130nm to 100micron, fully described in Coelho (2014).

The BT-Settl Model grid of theoretical spectra. With a cloud model, valid across the entire parameter range and using the Caffau et al. (2011) solar abundances. Wavelengths have...

GRAMS (Grid of Red supergiant and Asymptotic giant ModelS) is a grid of radiative transfer (RT) models for dust shells around red supergiant (RSG) and asymptotic giant branch...

GRAMS (Grid of Red supergiant and Asymptotic giant ModelS) is a grid of radiative transfer (RT) models for dust shells around red supergiant (RSG) and asymptotic giant branch...

A grid of LTE and non-LTE synthetic spectra of hot DA white dwarfs. It covers Teff from 17,000 K to 100,000 K and log(g) from 7.0 to 9.5. The stellar models are built for pure...

Morley et al. 2012 T/Y dwarf models

Morley et al. 2014 Y dwarf and exoplanet models