amitkundupabra
commented
5 years ago Dear Sir, I also have an another issue, I am running code SYNAPPS on a set of online available spectra of type Ic SNe, the problem is that, most of available spectra are in form of wavelength and flux. Flux_err is not given. So how can I apply SYNAPPS on these spectra ? And is it necessary that our flux and Flux_err should be in normalised form?
After successfully running the code SYNAPPS, where do I get the best fit values of opacity, temperature and other parameters? What does 'f' and 'x' in cache file mean as shown below? """"""""""""""""""""""""""""""""""" New Min: f=5.14e+02 x=[ 6.92e-01 2.61e-01 4.64e-01 1.42e+01 3.00e+01 1.29e+01 -1.47e+00 1.81e+00 1.21e-01 -1.16e+00 2.00e+00 2.00e+00 1.02e+00 0.00e+00 2.00e+00 1.31e+00 1.44e+00 1.88e+00 -8.18e-01 3.75e-02 -9.94e-02 1.88e+00 2.00e+00 4.75e-01 2.00e+00 1.42e+01 1.42e+01 1.42e+01 1.42e+01 1.42e+01 1.42e+01 1.42e+01 1.42e+01 1.42e+01 1.42e+01 1.42e+01 1.42e+01 1.42e+01 1.42e+01 1.42e+01 1.42e+01 1.42e+01 1.42e+01 1.42e+01 2.50e+01 2.50e+01 2.50e+01 2.50e+01 2.50e+01 2.50e+01 2.50e+01 2.50e+01 2.50e+01 2.50e+01 2.50e+01 2.50e+01 2.50e+01 2.50e+01 2.50e+01 2.50e+01 2.50e+01 2.50e+01 2.50e+01 6.25e-01 9.50e-01 5.00e+00 2.10e+00 7.00e-01 8.00e-01 1.00e-01 1.00e-01 1.00e+00 1.00e+00 9.87e-01 1.10e+00 1.10e+00 5.00e+00 5.00e+00 1.23e+00 1.10e+00 2.23e+00 1.16e+00 1.20e+01 1.76e+01 5.00e+00 1.51e+01 9.69e+00 2.50e+01 1.00e+01 1.00e+01 9.38e+00 5.44e+00 1.40e+01 1.26e+01 2.50e+01 2.50e+01 5.00e+00 1.12e+01 5.00e+00 2.50e+01 2.50e+01 ] step=6.25e-02 tag=100288 state=Evaluated Success: 15034 """"""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""