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

AMES-Cond 2000
AMES-Dusty 2000
ATMO 2020, CEQ
ATMO 2020, NEQ strong
ATMO 2020, NEQ weak
Bayo et al, M types from Collinder 69
Black Body
BT-COND
BT-DUSTY
BT-NextGen (AGSS2009)
BT-NextGen (GNS93)
BT-Settl
BT-Settl (AGSS2009)
BT-Settl (CIFIST)
BT-Settl (GNS93)
BT-Settl 2014
Coelho Synthetic stellar library (High Resolution)
Coelho Synthetic stellar library (SEDs)
DRIFT-PHOENIX
Exogan
Goyal local
Goyal rainout
GRAMS, C-rich grid
GRAMS, O-rich original grid
Granada HRES Library
Husfeld et al models for non-LTE Helium-rich stars
Keck LRIS spectra of late-M, L and T dwarfs
Kesseli et al.
Koester WD models
Kurucz ODFNEW /NOVER (2003)
Kurucz ODFNEW /NOVER models
Kurucz ODFNEW /NOVER, alpha: 0.0 (2003)
Kurucz ODFNEW /NOVER, alpha: 0.4 (2003)
L and T dwarf data archive
Levenhagen 2017
MILES
Morley 2012
Morley 2014
Morley2015 Cloud free
Morley2015 Cloud free
Morley2015 Cloudy
Morley2015 Cloudy (Transm.)
Morley2015 Haze (Soot)
Morley2015 Haze (Soot) (Transm.)
Morley2015 Haze (Tholin)
Morley2015 Haze (Tholin) (Transm.)
MUSE 1d Spectral Library
NextGen
NextGen (solar)
Pacheco et al 2021
POPSTAR with Chabrier IMF
POPSTAR with Ferrini IMF
POPSTAR with Kroupa IMF
POPSTAR with Salpeter IMF (1)
POPSTAR with Salpeter IMF (2)
Saumon 2012
SED@
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 (Grid 4)
TMAP - Tubingen
UVES/VLT


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