- PIO
- Safety
- Sciops
- Gemini Home
- Special Instructions
- Telescopes and Sites
- Instruments
- Observing with Gemini
- Schedules
- Data and Results
- Helpdesk
- Future Instrumentation
- Statistics
- Publications
Change page style:
NICI Filters
NICI has one filter wheel in each science channel. The current filter complement is listed below, with the location of each filter indicated by the Gemini ID numbers in the "Channel 1" and "Channel 2" columns. Click on an ID number to see the transmission curve for the actual filter element in that channel, if available.
The 1% 1.6 µm filters are used with the H-band 50/50 beamsplitter for Simultaneous Spectral Differential Imaging (SSDI) in the methane bandhead. These filters were built to high precision specifications for optimal image quality. They are mounted in both filter wheels so they can be interchanged to help cancel non-common-path errors between the two science channels.
The remaining filters are from the same batch as the NIRI filters.
| NICI Filters | ||||
| Filter Name | Central Wavelength | Wavelength range or Width | Channel 1 (Red) Gemini ID |
Channel 2 (Blue) Gemini ID |
| Block | -- | -- | -- | -- |
| CH4 H 1% S |
1.587 | 0.0150 (0.94%) | G0724 | G0722 |
| CH4 H 1% Sp | 1.603 | 0.0162 (1.01%) | G0728 | G0726 |
| CH4 H 1% L | 1.628 | 0.0174 (1.07%) | G0720 | G0732 |
| CH4 H 1% L_2 | 1.628 | 0.0174 (1.07%) | G0735 | |
| CH4 H 4% S | 1.578 | 0.062 (4.00%) | G0742 | G0743 |
| CH4 H 4% L | 1.652 | 0.066 (3.95%) | G0740 | G0737 |
| J |
1.25 | 1.15-1.33 | G0702 | |
| H | 1.65 | 1.49-1.78 | G0703 | |
| K | 2.20 | 2.03-2.36 | G0704 | |
| Ks | 2.15 | 1.99-2.30 | G0705 | |
| Kprime | 2.12 | 1.95-2.30 | G0706 | |
| Lprime | 3.78 | 3.43-4.13 | G0707 | |
| Mprime | 4.68 | 4.55-4.79 | G0708 | |
| [Fe II] | 1.644 | 1.5% | G0712 | |
| H2 1-0 S(1) | 2.1239 | 1.23% | G0709 | |
| Br-gamma | 2.1686 | 1.36% | G0711 | |
| Kcont | 2.2718 | 1.55% | G0710 | |
| CH4 H 6.5% S | 1.596 | 0.1175 (7.3%) | G0713 | |
| CH4 H 6.5% L | 1.701 | 0.0972 (5.7%) | G0714 | |
Created 15 July 2005, B. Rodgers and T. Hayward
Modified 26 October 2007, E. Christensen