You signed in with another tab or window. Reload to refresh your session.You signed out in another tab or window. Reload to refresh your session.You switched accounts on another tab or window. Reload to refresh your session.Dismiss alert
PS: Concerning the orders - it would be useful for echelle spectra as well and there are in fact two order numbers. One is the relative order counting from 1 (in IRAF it is called aperture number) and then there is an ABSOLUTE echelle order number - it is the real n where the echelle optics is working (number of wavelengths whic will fit the distance between two grooves on echelle grating. This absolute is important for checking the wavelength calibration etc ...
It sounds like those might even need distinct UCDs.
BM: Very interested to see echelle spectra supported too. We have a lot of archival echelle spectra taken with the AAT (e.g. UCLES). Petr's note about the
orders for a check on wavelength calibration are spot on. Reduction pipelines can sometimes misidentify orders, resulting in order-scale wavelength shifts
that are quite bad, so it's useful to be able to pick up on those.
PS: Order is more complex for Eschelle spectra - absolute order and relative order - useful for discovery and plotting so would like to see two utypes added.
Presentations by Vandana Desai
DM group meeting:
The text was updated successfully, but these errors were encountered: