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Cosmic Origins SpectrographInstrument Handbookfor Cycle 22 > Chapter 8: Target Acquisitions > 8.8 Centering Accuracy and Data Quality

8.8
A centering accuracy of 0.3 arcsec in the cross-dispersion (XD) direction is required to achieve optimum photometric accuracy and spectral resolution. In the along-dispersion (AD) direction, the minimum accuracy is set by velocity requirements: 15 km/s for the medium-resolution modes, 150 km/s for G140L, and 175 km/s for G230L. Since the AD requirements are in units of km/s, they are detector and wavelength dependent. Assuming that the wavelength error budget is split evenly between the COS TA and wavelength scale accuracy, the strictest pointing requirements are 0.041 arcsec for the NUV channel and 0.106 arcsec for the FUV channel.
8.8.1 Centering Accuracy and Wavelength Accuracy
To achieve a wavelength accuracy of 15 km/s, the target should be centered to within about 0.040.07 arcsec for NUV observations and 0.10.2 arcsec for FUV observations. The throughput of COS is not affected by centering errors of less than 0.4 arcsec, so high centering precision is not strictly necessary if science goals do not require that the wavelength zero point be well constrained. For example, the spectra of some objects may include foreground interstellar or inter-galactic absorption lines that can be used to establish the zero point of the wavelength scale.
8.8.2 Centering Accuracy and Photometric Precision
Figure 8.5 shows the relative transmission of the PSA as a function of the displacement of a point source from the aperture center, as measured using each of the four NUV gratings. These and the corresponding FUV curves are nearly identical and show that the transmission of the COS apertures is essentially flat within the central 0.4 arcsec, then tails off in a non-linear but approximately symmetrical profile (COS ISR 2010-09).
Figure 8.5: Relative Transmission of the COS PSA at NUV Wavelengths
Transmitted flux as a function of displacement from aperture center for all four NUV gratings. The dotted lines mark the edge of the aperture (1.25”). The two curves labeled D and XD refer to offsets along the dispersion and cross-dispersion axes, respectively. The other curves trace offsets in the cross-dispersion direction. For all gratings, the absolute transmission through the PSA for a centered point source is at least 95%.
8.8.3 Centering Accuracy and Spectroscopic Resolution
Targets placed within 0.4 arcsec of the aperture center will achieve maximum spectral resolution. Centering errors larger than 0.4 arcsec will lead to progressively poorer resolution. Targets at the edge of the aperture have approximately half the spectral resolution of well-centered targets.

Cosmic Origins SpectrographInstrument Handbookfor Cycle 22 > Chapter 8: Target Acquisitions > 8.8 Centering Accuracy and Data Quality

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