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GNIRS Calibration Exposure Times
The following tables provide proper GCAL configurations and exposure times for GCAL flats and arcs for GNIRS.
The values given cover a range of configurations, slit widths and wavelengths. If your particular configuration is not here, you may be able to extrapolate from similar settings. If not, please submit a query via the HelpDesk.
UPDATE May 2006: New GNIRS CAL sensitivities are now listed below
following the installation of a new NIR color balance GCAL filter.
Sufficient illumination of XD orders 3 - 9 (2.55 - 0.77 microns)
is now achieved with 2 GCAL flat settings without saturating the lower orders.
If your science needs to utilize XD order 10, then please specify this
in a NOTE within your phase II, and let your contact scientist know. They
will add a third flat field field step to the template sequence below.
UPDATE March 2005: New xenon (Xe) lamp REPLACES krypton (Kr) lamp to provide better
wavelength calibration for R=18,000 observations.
Jump to instrument config:
- Cross-dispersed, 32 l/mm grating (XD-32)
- Cross-dispersed, 111 l/mm grating (XD-111)
- IFU, 32 l/mm grating (IFU-32)
- IFU, 111 l/mm grating (IFU-111)
- Long slit, short camera, 32 l/mm grating (LS-S32)
- Long slit, short camera, 111 l/mm grating (LS-S111)
- Long slit, long camera, 111 l/mm grating (LS-L111)
| ;a name="XD111">Cross-Dispersed 111 l/mm, Short Camera (Long Camera not yet available with XD-111) |
|||||
| GNIRS Configuration | GCAL Configuration | ||||
| Filter | Slit Width (arcsec) | Lamp | Filter | Exposure Time (s) | Coadds |
| XD | 0.3, 0.45, 0.675 | IR* | NIR balance | 4.0 | 4 |
| XD | 1.0, 3.0 | IR* | NIR balance | 0.6 | 8 |
| XD | 0.3, 0.45, 0.675 | QH** | NIR balance | 1.5 | 6 |
| XD | 1.0, 3.0 | QH** | NIR balance | 0.2 | 8 |
| XD | 0.3, 0.45, 0.675, 1.0, 3.0 | Ar | none | 0.2 | 20 |
* The IR lamp is a better flat field source for XD Order 3 (the first continuous order viewed from the left in the image display).
** The QH lamp now illuminates ALL the XD orders without saturating the array! There is an absorption feature due to the QH source present in the first order on the left as seen in the display (XD order 3). Use the IR lamp flat for this order only instead of the QH flat.
*Both Ar and Xe lamp exposures may be needed for sufficient calibration in some wavelength regions at this resolution. Check for availability of Ar and Xe emission lines here.
Last update July 28, 2006; Greg Doppmann