SPEC: Calibrations
There is no need for observers to take flat fields or arc lamp calibration images for the OSIRIS spectrograph. Wavelength calibration and pixel to pixel variations are accounted for in the Data Reduction Pipeline (DRP) via the Rectification Matrices.
IMAG: Dome Flats
While the dome flat lamp is adjustable, the OSIRIS imager typically
uses it at full power (level = 0). The dome flat lamp power level
can be between 0.0 and 20.0,
0 = brightest, 20 = faintest.
Filter | dcs.FLAMP (power) | OOPGUI Itime (s) | oids.TRUITIME (s) | Approx. DN | Approx. DN/s |
---|---|---|---|---|---|
Hbb | 0.0 | 3 | 2.950 | 15,000 | 5,100 |
FeII | 0.0 | 30 | 29.505 | 8,500 | 290 |
Kp | 0.0 | 3 | 2.950 | 10,400 | 3,500 |
BrGamma | 0.0 | 40 | 39.832 | 14,000 | 350 |
Current as of 2021 June 30 for Keck1
IMAG: Flats for Download
Filter | TRICK Dichroic | Normalized Flat | oids.TRUITIME (s) | oids.COADDS | Median DN | Lamps On | Lamps Off |
---|---|---|---|---|---|---|---|
BrGamma | Open | BrG_open | 8.851 | 1 | 3115 | BrG_open_on | BrG_open_off |
BrGamma | hBand | BrG_hBand | 8.851 | 1 | 3174 | BrG_hBand_on | BrG_hBand_off |
Kn3 | Open | Kn3_open | 4.425 | 1 | 5650 | Kn3_open_on | Kn3_open_off |
Kn3 | hBand | Kn3_hBand | 4.425 | 1 | 5735 | Kn3_hBand_on | Kn3_hBand_off |
Kp | Open | Kp_open | 2.950 | 1 | 10003 | Kp_open_on | Kp_open_off |
Kp | hBand | Kp_hBand | 2.950 | 1 | 10272 | Kp_hBand_on | Kp_hBand_off |
IMAG: Flats Structure
Filter | Open | TRICK Dichroic | TRICK - Open | TRICK / Open |
---|---|---|---|---|
BrGamma | ![]() |
![]() |
![]() |
![]() |
Kn3 | ![]() |
![]() |
![]() |
![]() |
Kp | ![]() |
![]() |
![]() |
![]() |
Stretch for all images: HistEq, Range: -1.0 to +2.0