serval
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mzechmeister
calculate radial velocities from stellar spectra
Remove indexing `ind` of valid pixels in counting of pixels per template knot. The valid pixels are selected by the `bmod==0` condition already. For the counting of all possible pixels...
A new astropy warning (only python2) ``` WARNING: ErfaWarning: ERFA function "dtf2d" yielded 1 of "dubious year (Note 6)" [astropy._erfa.core] ``` https://github.com/nu-radio/NuRadioReco/issues/99 https://github.com/astropy/astropy/issues/5809 https://github.com/astropy/astropy/issues/9603 Arising in https://github.com/mzechmeister/serval/blob/f26706f77b2505a94029c8bad3f994b9aed03392/src/brv_we14py.py#L75 Minimal script to...
This can occur with MaroonX hdf spectra: ``` IOError: Unable to create file (unable to open file: name = '...', errno = 17, error message = 'File exists', flags =...
The option should accept an RV file. Currently, there are already the `-vtfix` and `-skippre` options. Actually, it is also related to the `-targrv` option. With is option one could,...
This can happen, if only few data points are available. Low SNR data should not be normalised with a cubic polynomial.
There should be a [rank warning](https://docs.scipy.org/doc/numpy/reference/generated/numpy.RankWarning.html#numpy.RankWarning) if the number of data points is smaller than the number of parameters or if the matrix is poorly conditioned, similar as in [numpy.polyfit](https://docs.scipy.org/doc/numpy/reference/generated/numpy.polyfit.html).
Instead of a binary mask, a telluric absoption spectrum can be used to for mild a priori correction and better weightening. Model spectra for CARM VIS are now available.
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calculate radial velocities from stellar spectra