-
If absorption is requested when there are no blocks, `lmitt.formula()` is currently set to stop ([lmitt.R lines 245-53](https://github.com/benbhansen-stats/propertee/blob/7d8fb2f9dbabdbe397ac53c17a983…
-
Hi Corentin,
I am using this package to find out the corrected redshift using the metal absorption lines. Can you give some idea how the code measures the redshift. Because when I plot the measure…
-
Hi Corentin,
Is it reasonable to add a feature that force some of the lines to be absorption and some others to be emission? I'm fitting optical spectra to find z~2.3 galaxies and have to discr…
-
The `estfun_DA` vignette has been revised to include plans for an alternate design-based variance estimator along lines I've discussed with Xinhe and Julian; see the version on the design branch, sect…
-
Put in an A0 star and see if the Paschen line depths are recovered at the correct wavelengths.
Also see that an injected emission line and correct width is recovered. Should be narrower in order 2 …
-
Here's a video showing what's wrong: https://mega.nz/file/9BQSlLgK#gM5e3I3g31r7Izsw3LFPSAuCaimqngeQZUEDuTJCAlc
Basically it looks like there is some kind of invisible line blocking cells absorbing …
-
fantastic gh file, elegant but easy to use. I am wondering, how to calculate the water depth like those data in gif
-
Spectroscopy has these child concepts:
Atomic spectroscopy
Electronic spectroscopy
Galaxy spectroscopy
Lyman alpha forest
Molecular spectroscopy
Radio spectroscopy
Rotational spectroscopy
Tran…
-
Determine extinction based on HI lines, H2 lines to help with the degeneracy of the silicate absorption band and the surrounding PAH bands.
-
reported by: @CloudyLex
we have redone most of the figures in the quick start guide using Jeremy Sander's veusz program
http://home.gna.org/veusz/
The BLR spectrum on page 14 Figure 3 which were no…