ING Banner
Home > Astronomy > ISIS > Red Arm


ISIS Red Arm

The default chip for the ISIS red arm is RED+. It is a red-sensitive array of 4096×2048 (15.0 micron) pixels with almost no fringing.

  1. General information on the RED+ CCD
  2. Wavelength coverage and spectral resolution
  3. Spatial scale
  4. Fringing and cosmetic defects
  5. Linearity measurements
  6. Shutter effect
  7. Bad pixel masks
  8. Atlas of arc lines in the red arm

Wavelength coverage and spectral resolution

The table below gives the dispersion provided by each grating when mounted blaze to collimator (see the ISIS manual for more in depth details on gratings and their properties), and the spectral range covered by the REDPLUS CCD. The REDPLUS detector is mounted on the red arm with its 4096 pixels axis along the dispersion direction, giving maximum utility of the beam width leaving the camera. However, the camera optics vignette the outer regions of the dispersed light beam such that approximately 800 pixels at either end of the CCD are vignetted. A plot of the CCD vignetting function across the chip is shown below to illustrate this effect. This function was measured in May 2011 from a flat-field exposure corrected by CCD quantum efficiency, grating efficiency and tungsten lamp spectral emissivity functions. The unvignetted region is from (spectral) pixel 800 to 3200 (calculated so that the flux differences are within 5%), which is essentially the central 2400 pixels. The unvignetted and 50% vignetted spectral ranges in Å are given in the table below.

The dispersions of the red-arm gratings in Å/mm are 121 (R158R), 62 (R316R), 33 (R600R) and 17 (R1200R). The pixel size of the REDPLUS detector is 15 microns, and the corresponding grating dispersions in Å/pixel are listed in the table, as are the slit widths that project to four pixels (60 microns) with the gratings set at blaze. The spectral resolution elements, Δλ, in Å for a 1-arcsec slit are also listed. The corresponding nominal spectral resolutions, λ/Δλ, at 7000Å with a 1-arcec slit are approximately 909 (R158R), 1842 (R316R), 3867 (R600R) and 9333 (R1200R). Resolutions for others slit widths and wavelengths can be computed with the SLITTOOLS calculator.

Note in the table that the slit width projecting to four pixels increases with grating resolution. This is due to grating anamorphic de-magnification, which is parameterised by cos(θ+φ/2)/cos(θ-φ/2), where θ is the grating tilt with respect to zero order and φ is the camera-collimator angle. This relation demonstrates why the slit size projecting to four pixels is larger for the higher resolution gratings; they are set to larger tilt angles for a given central wavelength, and so their de-magnification is greater. See here for a discussion of this effect.

ISIS wavelength coverage and resolution with REDPLUS
Grating
Blaze
Total Spectral range (Å)
Unvignetted range 2400 pixels (Å)
50% unvignetted range 3285 pixels (Å)
Dispersion (Å/pixel)
Slit-width for 60µ at the detector (in arcsecs)
Resol. element with a 1" slit (Å)
R158R
6500
7530
4412
6038
1.81
0.94
7.70
R316R
6500
3858
2260
3094
0.93
0.98
3.80
R600R
7000
2054
1202
1646
0.49
1.08
1.81
R1200R
7200
1055
618
846
0.26
1.38
0.75

According to sampling theory a line as recorded on the detector is fully sampled if it has at least two dispersion elements across its FWHM, and so the detector oversamples the resolution element when the slit width is set to 1-arcsec (e.g. to approximately match seeing). In this configuration the detector can be binned ×2 spectrally to increase the signal-to-noise in each wavelength bin, without loss of spectral resolution. This can also be done at the reduction stage, but binning on-chip reduces the readout noise contribution to the resolution element.

It is also possible of course to improve spectral resolution by reducing the slit width. This increases slit losses especially in moderate seeing, and in any case the slit should project to at least two pixels so that the resolution element remains fully sampled by the detector.

Spatial scale

The red (and blue) camera is a folded Schmidt design of focal length 500 mm and gives a scale of 14.9 arcsec/mm along the slit. Hence a spatial scale of 0.22 arcsec/pixel is achieved with the REDPLUS. It is possible to bin in the spatial direction if one is not concerned with high spatial resolution observations, indeed the seeing conditions need to be excellent to allow full advantage to be taken of using an unbinned chip with this pixel scale. The maximum unvignetted slit-length usable with ISIS is 3.7 arcmin (corresponding to 1000 spatial detector pixels, spanning ~[600:1600, 1:4200]).

Fringing and cosmetic defects

REDPLUS  is a very low-fringing high-QE CCD. Fringing begins at about 8000Å, and the ripples are visible at about the 1% level at 9000Å. Here you will find more information.

Shutter effect

The Prontor shutter opens the aperture radially symmetrically. The same shutter effect as for the blue arm was measured for the red arm.

Bad pixel masks

Bad pixel masks for RED+ with different binning were created using noao.imred.ccdred task in IRAF. All masks are created for the default CCD window [585:1550,1:4200].

bad pixel mask bin 1 1           bad pixel mask bin 1 2           bad pixel mask bin 2 1

bad pixel mask bin 2 2           bad pixel mask bin 3 1           bad pixel mask bin 3 2

bad pixel mask bin 4 2

Atlas of arc lines in the red arm

An atlas of arc lines for a range of central wavelengths of the red arm gratings is available here.


Top | Back

Contact:  (ISIS Instrument Specialist)
Last modified: 23 April 2016