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
Some new modes have been added and there is no way to find the wavelength calibration because the necessary reference lamps have been added, here we will track those missing lamps.
Note: All reference lamps must be obtained using binning 1x1 and the narrowest possible lamp.
2100_3900 1x2 slit 0.45
2100_5000A 2x2, slit 1.0 arcseconds
2100_6507A Filter GG455 binning 1x2 slit 0.45"
1200_CaNIR Filter OG570 binning 1x2 slit 0.8
600UV 2x2 slit 1.0 CuHeAr
600UV 2x2 slit 1.5 (same as above)
Data was obtained after February 13th, 2024
2024/02/16
2024/02/17
2024/02/21
The text was updated successfully, but these errors were encountered:
The 1200_CaNIR is spectroscopically the same as 1200M7, using this workaround will not affect your wavelength solution.
Clone the goodman pipeline package git clone https://github.com/soar-telescope/goodman_pipeline.git
Move into the folder and navigate to goodman_pipeline/goodman_pipeline/data/ref_comp
Copy the 1200M7 HgArNe lamp cp goodman_comp_1200M7_OG570_HgArNe.fits goodman_comp_1200_CaNIR_OG570_HgArNe.fits
Using any proper tool for editing headers change the header of goodman_comp_1200CaNIR_OG570_HgArNe.fits to the following values WAVMODE = 1200_CaNIR
If you have other lamps might want to repeat the same (steps 3 and 4) of all the 1200M7 lamps
Now you need to tell the pipeline where to find it. You must place it in a different folder, there must be only reference lamps there, if you can locate where the package is installed you can also copy it there, where all the other lamps are. Then use the --reference-files option to tell the pipeline where to search for lamps.
Some new modes have been added and there is no way to find the wavelength calibration because the necessary reference lamps have been added, here we will track those missing lamps.
Note: All reference lamps must be obtained using binning 1x1 and the narrowest possible lamp.
Data was obtained after February 13th, 2024
The text was updated successfully, but these errors were encountered: