INAF              

A library of high-resolution synthetic stellar spectra in the optical interval


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Important notice:

We provide the library for three different spectral resolution:

  • at FWHM=1 Angstrom constant throughout the wavelength range;
  • at the R=10,000;
  • at the original resolving power of R=500,000.
In addition, we also join here two IDL routines, to ease a straighforward reading of the data and further change the Resolving Power (and/or the FWHM resolution) of the full library, according to the user's requirements.
If you are interested in the FULL-RESOLUTION (R = λ/Δλ = 500,000) version of the library please post an e-mail request HERE.



Parameter codes for file names:

 
Metallicity:

m20 log Z/Zsun = −2.00p00 log Z/Zsun = +0.00
m15 log Z/Zsun = −1.50p03 log Z/Zsun = +0.30
m10 log Z/Zsun = −1.00p05 log Z/Zsun = +0.50
m05 log Z/Zsun = −0.50 
Surface gravity:

g00 log g = 0.00g30 log g = 3.00
g05 log g = 0.50g35 log g = 3.50
g10 log g = 1.00g40 log g = 4.00
g15 log g = 1.50g45 log g = 4.50
g20 log g = 2.00g50 log g = 5.00
g25 log g = 2.50 

Effective Temperature: txxxxxx Teff = xxxxxx K (a number between 3000 and 50,000 K)
Microturbulent Velocity: k2 ξ = 2 km/s (fixed)



FWHM = 1 Angstrom

Download single "all-in-one" tar packages of the gz-ipped spectra for the entire library (~70 Mb) or for fixed metallicity (~12 Mb each):


bluered_fwhm1a.tar
 

bluered_fwhm1a_m30.tar

bluered_fwhm1a_m03.tar
bluered_fwhm1a_m20.tarbluered_fwhm1a_p00.tar
bluered_fwhm1a_m10.tarbluered_fwhm1a_p03.tar

BLUERED_wavelengths.dat.gz

 

R = 10,000

Download single "all-in-one" tar packages of the gz-ipped spectra for the entire library (~140 Mb) or for fixed metallicity (~24 Mb each):


bluered_r10.tar
 

bluered_r10_m30.tar

bluered_r10_m03.tar
bluered_r10_m20.tar bluered_r10_p00.tar
bluered_r10_m10.tarbluered_r10_p03.tar

BLUERED_wavelengths.dat.gz

 

R = 500,000

Pick up the individual spectra (~3 Mb each).


 

 


Download the routine to read BLUERED spectra:

[IDL]

Download the routine to degrade the resolving power
of BLUERED spectra:

[IDL]



To BLUERED Homepage

To Alberto Buzzoni's Homepage

To Emanuele Bertone's Homepage



 
 EB/Jan 2009