Spring School of Spectroscopic Data Analyses
Determination of Atmospheric Parameters of B, A, F and G type stars
8–12 April 2013, Wrocław, Poland
IRAF
Image Reduction and Analysis Facility (IRAF) is a software for the reduction and analysis of astronomical data. All necessary information about IRAF and how to install it can be found here:
http://iraf.noao.edu/
The pdf file with the atlas of ThAr lines useful for calibration can be downloaded from here .
ATLAS9
ATLAS9 package for the determination of stellar atmospheres is available on at R. L. Kurucz web page, together with a database of model grids, opacity grids and line lists:
http://kurucz.harvard.edu/
Another important source of information about ATLAS9 and how to install and compile it is Atmos webbage:
http://atmos.obspm.fr/index.php/
And Fiorella Castelli's web page:
http://wwwuser.oat.ts.astro.it/castelli/
ATLAS9 code and compilation instructions from Tatiana Ryabchikova can be taken from here:
Download
SME
Spectroscopy Made Easy (SME) is IDL software and a compiled external library that fits an observed high-resolution stellar spectrum with a synthetic spectrum to determine stellar parameters and abundances. All necessary codes, tutorials and manuals can be foud here:
http://www.astro.uu.se/~piskunov/RESEARCH/RT_3D/
And the instruction for installation (from Nikolai Piskunov):
Download
SME: tutorial
Download
SME: lines
Download
Lecture3
sm_info_additional.tar.gz
SIU
Spectrum Investigation Utility (SIU) is IDL software (Johannes Reetz, Munich) for the determination of stellar atmospheric parameters and chemical composition. All necessary codes and installation information can be downloaded here:
Download
siu_info.txt-download
ARES
ARES is a C code developed for the measurement of Equivalent Width of absorption lines in stellar spectra.
All necessary codes and manuals can be downloaded from here:
http://www.astro.up.pt/~sousasag/ares/
New materials from Sergio Sousa:
TestD.fits
lines_FeIandFeII.dat
ultimate_list.dat
Final_Harps_linelist.rdb
MOOG
MOOG performs an LTE line analysis and spectrum synthesis. All necessary codes and manuals can be taken from here:
Download
Atomic data
There are several sources of atmomic data. Please register in VALD database before the beginning of the School.
http://kurucz.harvard.edu/linelists.html
http://wwwuser.oat.ts.astro.it/castelli/linelists.html
http://www.astro.uu.se/~vald/php/vald.php
Stellar spectra
Spectra for the reduction and calibration are available here:
Download
Spectra of the stars we will analyse are available here:
Download
A Digital Spectral Classification Atlas
A Digital Spectral Classification Atlas prepared by Richard Gray is available here:
Download