This application is meant to transform portions of synthetic spectra (100 Å to 500 Å) into simulated observations to compare them with observed spectra.
To achive this, SPECFLOW allows to perform a convolution of the synthetic spectra with a rotation profile, an intrumental profile and a turbulent microturbulence velocity profile, and to doppler shift it according to the radial velocity of the star it is meant to represent.
Through the tab "Observed spectra", you will be able to:
Through the tab "Synthetic spectra", you will be able to:
Please connect to the VO-tool of your choice to further visualize your data
Min/max range of stellar parameters
Synthetic spectrum selected from Pollux Database (FITS file)
Central wavelength : Wavelength width :
votable (TOPCAT, CASSIS)