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ID:
ivo://svo.cab/models/grams_ogrid
Title:
GRAMS, O-rich original grid
Short Name:
GRAMS-Orich
Date:
04 Sep 2019 08:31:00
Publisher:
SVO CAB
Description:
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 (AGB) stars. This is the model grid for Oxygen-rich stars
ID:
ivo://svo.cab/models/husfeld
Title:
Husfeld et al models for non-LTE Helium-rich stars
Short Name:
Husfeld
Date:
04 Sep 2019 08:28:51
Publisher:
SVO CAB
Description:
Husfeld et al models for non-LTE Helium-rich stars
ID:
ivo://svo.cab/models/kurucz2003all
Title:
Kurucz ODFNEW /NOVER (2003)
Short Name:
Kurucz2003all
Date:
27 Sep 2022 13:40:47
Publisher:
SVO CAB
Description:
ATLAS9 Kurucz ODFNEW /NOVER models. Newly computed ODFs with better opacities and better abundances have been used.
ID:
ivo://svo.cab/models/kurucz2003alp
Title:
Kurucz ODFNEW /NOVER (2003) alpha:0.4
Short Name:
Kurucz2003a04
Date:
27 Sep 2022 13:46:53
Publisher:
SVO CAB
Description:
ATLAS9 Kurucz ODFNEW /NOVER models. Newly computed ODFs with better opacities and better abundances have been used.
ID:
ivo://svo.cab/models/kurucz2003
Title:
Kurucz ODFNEW /NOVER (2003) alpha:0.0
Short Name:
Kurucz2003
Date:
27 Sep 2022 13:46:24
Publisher:
SVO CAB
Description:
ATLAS9 Kurucz ODFNEW /NOVER models. Newly computed ODFs with better opacities and better abundances have been used.
ID:
ivo://svo.cab/models/kurucz
Title:
Kurucz ODFNEW /NOVER models
Short Name:
Kurucz
Date:
04 Sep 2019 08:29:03
Publisher:
SVO CAB
Description:
Kurucz ODFNEW /NOVER models. Newly computed ODFs with better opacities and better abundances have been used. (The convective treatment is described in Castelli et al. 1997, AA 318, 841.)
ID:
ivo://svo.cab/models/levenhagen
Title:
Levenhagen 2017
Short Name:
Levenhagen
Date:
04 Sep 2019 08:31:00
Publisher:
SVO CAB
Description:
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 hydrogen and the spectra cover a wavelength range from 90 nm to 2.5 micron.
ID:
ivo://svo.cab/models/morley12
Title:
Morley 2012
Short Name:
Morley 2012
Date:
04 Sep 2019 08:31:00
Publisher:
SVO CAB
Description:
Morley et al. 2012 T/Y dwarf models
ID:
ivo://svo.cab/models/morley14
Title:
Morley 2014
Short Name:
Morley 2014
Date:
04 Sep 2019 08:31:00
Publisher:
SVO CAB
Description:
Morley et al. 2014 Y dwarf and exoplanet models
ID:
ivo://svo.cab/models/morley15/cfree/emi
Title:
Morley2015 Cloud free
Short Name:
Morley15Cfree_em
Date:
27 Sep 2022 14:33:18
Publisher:
SVO CAB
Description:
Cloud free models of GJ 1214b “analogs” from Morley et al. 2015. Emission spectra.