- PIO
- Sciops
- Gemini Home
- Telescopes and Sites
- Science Visitors at Gemini
- Observing With Gemini
- Instruments
- NORTH
- ALTAIR
- GMOS
- GNIRS
- NIFS
- NIRI
- SOUTH
- FLAMINGOS-2
- GeMS
- GMOS
- GPI
- GSAOI
- NICI
- VISITING
- Visiting Instrument Policy
- DSSI Speckle Camera (North)
- TEXES (North)
- RESOURCES
- Integration Time Calculators
- Adaptive Optics
- GCAL
- Magnitudes and Fluxes
- Near-IR Resources
- Mid-IR Resources
- Observing Condition Constraints
- Performance Monitoring
- SV/Demo Science
- Future Instrumentation
- Queue and Schedules
- Data and Results
- Helpdesk
- Statistics
Change page style:
Grisms
FLAMINGOS-2 currently contains three grisms (located in the grism wheel; see the FLAMINGOS-2 optomechanical diagrams). When used with a 2-pixel slit (0.36"), the two moderate-resolution grisms, JH and HK, have resolving power R = λ/dλ ~1250. These cover "octave" wavelength ranges: the JH grism wavelength range is 0.9-1.8 microns, and the HK grism wavelength range is 1.2-2.4 microns (see the filters page for details on the matching JH and HK bandpass filters). With these grisms spectra in two near-IR bands are obtained simultaneously. The HK grism may be used with the HK filter to obtain H- and K-band spectra in first order, or it may be used with the JH filter to obtain H-band spectra in the first order and J-band spectra in second order; the JH grism covers both the J- and H-bands in first order. The peak transmission for both grisms is 80%.
The third grism has resolving power R~3000, and is called the "R3K" grism. The R3K grism can be used with any of the single-band broadband filters -- Y, J-low, J, H, Ks -- to obtain spectra in near-IR one band at a time.
Predicted dispersions and resolving powers for the three grisms, when used with a 2-pixel wide slit (or slitlet), are presented below. The plots of resolving power as a function of wavelength use the laboratory-measured wavelength solutions for the grisms.
| Grism | Filter | Wavelength [µm] |
Order | 2-pix Slit Dispersion [Angstrom/pixel] |
R = λ/dλ (2-pix slit) |
Resolving Power as Function of λ |
| JH | JH |
1.25 | 1 | 6.667 | 938 | Plot |
| 1.65 | 1 | 6.667 | 1238 | |||
| HK | JH |
1.10 | 2 | 4.000 | 1375 | |
| HK | 1.65 | 1 | 7.826 | 1054 | Plot | |
| 2.20 | 1 | 7.826 | 1406 | |||
| R3K | J-low |
1.10 | 6 | 1.667 | 3300 | Plot |
| J | 1.25 | 5 | 2.022 | 3090 | Plot | |
| H | 1.65 | 4 | 2.609 | 3162 | Plot | |
| Ks | 2.20 | 3 | 3.462 | 3178 | Plot |
Plots of the net system throughput with the grisms are linked from the table below. These plots use the grism efficiency data produced by the grism manufacturer and scales them by the throughput curves for the FLAMINGOS-2 optical train. (Laboratory measurements made of the net system transmission made in Florida are consistent with these throughput curves.) These transmission curves do not include the effects of the atmosphere, the telescope, or the detector. Values for the mean transmission over the full data range (Tmean), the mean over the wavelength range where the transmission is greater than or equal to 80% of the maximum transmission (T80%), and the maximum transmission (Tmax) are given.
| Grism | Filter | Tmean | T80% | Tmax | Plot |
| JH | JH | 43% | 54% | 59% | Plot |
| HK | HK | 47% | 55% | 63% | Plot |
| R3K (order 6) | J-low | 8% | 18% | 20% | Plot |
| R3K (order 5) | J | TBD | TBD | TBD | |
| R3K (order 4) | H | 20% | 36% | 38% | |
| R3K (order 3) | Ks | 13% | 34% | 35% |
Throughput curves for the grisms only, based on lab measurements, are also available.