Theoretical spectra web server

TLUSTY OSTAR2002 (?)

T_eff:	-	(?)
Log(g):	-	(?)
Z/Z0:	-	(?)

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Grids do not always have a uniform coverage of all the parameter space.
You can get a hint about grid coverage seeing what combinations of Tegg,Logg are available.

References:

TLUSTY OSTAR2002
- TLusty web page
- Hubeny, I., Lanz, T. 1995, ApJ, 439, 875H
  NLTE line blanketed model atmospheres of hot stars. I. Hybrid Complete Linearization/Accelerated Lambda Iteration Method
- Lanz, T., Hubeny, I. 2003, ApJS, 146, 417
  A Grid of Non-LTE Line-blanketed Model Atmospheres of O-Type Stars

AMES-Cond 2000
AMES-Dusty 2000
Bayo et al, M types from Collinder 69
Black Body
BT-COND
BT-DUSTY
BT-NextGen (AGSS2009)
BT-NextGen (GNS93)
BT-Settl
BT-Settl 2014
BT-Settl-CIFIST
Coelho Synthetic stellar library (High Resolution)
Coelho Synthetic stellar library (SEDs)
DRIFT-PHOENIX
GRAMS, C-rich grid
GRAMS, O-rich original grid
HRES
Husfeld et al models for non-LTE Helium-rich stars
Keck LRIS spectra of late-M, L and T dwarfs
Kesseli et al.
Koester
Kurucz ODFNEW /NOVER models
L and T dwarf data archive
Levenhagen 2017
MILES
Morley 2012
Morley 2014
NextGen
NextGen (solar)
POPSTAR with Chabrier IMF
POPSTAR with Ferrini IMF
POPSTAR with Kroupa IMF
POPSTAR with Salpeter IMF (1)
POPSTAR with Salpeter IMF (2)
Saumon 2012
SD Grid
The NIRSPEC Brown Dwarf Spectroscopic Survey
The SpeX Prism Spectral Libraries
TLUSTY BSTAR2006
TLUSTY OSTAR2002
TLUSTY OSTAR2002+BSTAR2006
TMAP
TMAP (Grid 1)
TMAP (Grid 2)
TMAP (Grid 3)
TMAP - Tubingen
UVES/VLT