- 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:
Zero Points
A zero point is defined as the magnitude of an object that would yield 1 ADU/sec at an airmass of 1. They depend on instrument and telescope transmittances as well as detector electronics. Zero points tend to be stable at the 3% level over many months. Measured values need to be corrected for variation of atmospheric extinction with airmass. The following table contains zero points for NIRI with its f/6 camera and broad band filters. Extinction values are taken from Tokunaga, Simons & Vacca (2002 PASP 114, 180) for 2mm of precipitable water vapor. See their Table 2 for extinction values for other amounts of precipitable water.
For more detailed information on the NIRI zero points please see the Instrument Performance Monitoring project web page.
| Filter | Central wavelength (µm) |
Zero point magnitude (for 1 ADU/s) |
Sky background (mag/arcsec) |
Typical extinction (mag/airmass) |
| Y | 1.02 | 22.98 | ||
| J | 1.25 | 23.97 | 15 to 16 | 0.015 |
| H | 1.64 | 24.04 | 14 to 14.5 | 0.015 |
| Kprime | 2.12 | 23.68 | 13.7 to 14.2 | 0.059 |
| Kshort | 2.15 | 23.40 | 13.6 to 14.1 | 0.043 |
| K | 2.20 | 23.43 | 13.5 to 14.0 | 0.033 |
| L' | 3.77 | 22.21 | 3.5 | 0.104 |
| M' | 4.68 | 20.1 | 0.3 | 0.223 |