Gratings for the Argus Multiple Object Spectrograph
The following gratings can all be used with Argus. Resolutions are shown for
3 pixel images with the Loral 1K x 3K CCD which at the present time is
the only CCD available for use with Argus. The projected size of the fibers
on this chip is approximately 3 pixels. There is no slit, so this is the
limiting resolution.
Gratings
First Order
Grating # Lines/mm Blaze (A) Resolution (A) Coverage (A)
(3 pixels) (3072 pixels)
250 158 4000 11 Complete
400 158 8000 11 Complete
510 300 10000 5.9 6000
181 316 7500 5.6 5600
KPGL2 316 4400 5.6 5600
KPGL3 527 5500 3.4 3300
420 600 8000 3.0 2900
KPGL1 632 4200 2.8 2800
380 1200 8000 1.5 1500
KPGLF 632 8200 2.8 2800
450 632 11000 2.8 2800
KPGLD 790 8500 2.2 2200
KPGLG 860 11000 2.0 2000
There is also an echelle grating with 316 l/mm, with an effective blaze at
56120 Angstroms. See the echelle mode
documentation for information about how to use this grating.
Notes:
- These are FIRST order figures. Obviously, not all these gratings are
designed to be used in first order. When used in second order, coverage
and resolution are half the figure given.
- Blaze is in "Littrow", i.e. normal incidence. The effective blaze is
about 92% of the Littrow wavelength.
- Gratings 400 and 510 are silver coated and thus do not reflect light below
about 4000A.
- Gratings 510, 420 and 380 are not very efficient in second order.
- Grating number 380 produces very bad ghost reflections at some
wavelengths.
- "Complete" spectral coverage means that the chip is larger than the first
order spectrum over the wavelength range to which the chip is sensitive. This
does not imply that the chip can be used efficiently over such a large range.