Both the long- and short-wavelength IUE spectrographs have two
entrance apertures: a small aperture (nominal 3 arcsec diameter circle)
and a large aperture (nominal 10 arcsec by 20 arcsec slot). Although the
various methods available for determining the fundamental dimensions do
not always yield results which agree to within the limits set by the
internal consistency of each (see Panek 1982), the IUE Three Agency
Committee adopted recommended values for certain dimensions, which are
presented in Table 2.1. These values do not reflect the true
physical dimensions of the apertures but rather the size as projected on
the camera faceplate. As a result, each spectrograph has its own
distinct measurement of aperture sizes.
The camera plate scales have been redetermined (Garhart 1996; LWP
1.5644, LWR 1.5526, and SWP 1.5300 arcseconds per pixel) using the most
recent measurements for the small-to-large aperture offsets in pixels
(Table 2.2) and FES aperture center locations in arcseconds
(Pitts 1988). These latest incarnations replace the oft-quoted plate
scale figure of 1.525 arcseconds per pixel (Bohlin et al. 1980), a value
that had been used for all three cameras. The aperture separations in
the directions along and perpendicular to the dispersion are given in
Table 2.2 for low dispersion. The corresponding values for
the high-dispersion offsets are obtained by transposing the entries for
the low-dispersion offsets along and perpendicular to the dispersion in
Table 2.2. Refer to Figures 2.16 through 2.18 to
determine the correct sign for the high-dispersion offsets.
The geometry of the two entrance apertures in relation to the image scan lines and the high and low resolution dispersion directions are shown in Figures 2.16 through 2.18 for the LWP, LWR, and SWP cameras. Note particularly the fact that the displacement between the short-wavelength large aperture (SWLA) and the short-wavelength small aperture (SWSA) is very nearly along the echelle dispersion direction. Therefore, short-wavelength high-dispersion images in which both apertures are exposed will result in nearly complete superposition of the large- and small-aperture spectra (with a wavelength offset). The displacement of the long-wavelength large aperture (LWLA) and the long-wavelength small aperture (LWSA) is less coincident with the echelle dispersion direction in this spectrograph, so that superposition of large- and small-aperture high-dispersion spectra is not as serious in the long-wavelength spectrograph.
For the purposes of judging the extent and separation of the apertures in the spectral domain, the scales given in Table 2.3 may be used in conjunction with the quantities in Tables 2.1 and 2.2. Note that in high dispersion a given shift along the dispersion corresponds closely to a constant Doppler velocity shift, whereas in low dispersion a given shift corresponds to a constant wavelength shift.
Camera | Low (Å/px) | High (km/s/px) |
LWP | 2.66 | 7.21 |
LWR | 2.66 | 7.27 |
SWP | 1.68 | 7.72 |