Sarah Kendrew

Continuum fitting using individual points instead of spectral regions

2

Some of our JWST mid-IR spectra with low resolution have dense forests of emission lines (H recombination lines). The automated continuum fit tends to interpret as noise what is actually...

linear to log spectral axis conversion

2

Is there the ability to convert a Spectrum1D object's spectral axis from linear to log space (and reverse), with flux conservation? I have seen other issues (e.g. #255) discussing resampling/rebinning...

would it be possible to add a query option for exposure types? this would help when querying for TA products for example.