11.5.3 COS Apertures

This article describes the apertures available for COS observations.

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Format definitions

Boldface type indicates the name of an APT parameter or a value for a parameter.

(red star) Black text indicates an important note.

Magenta text indicates available but unsupported parameters (requires prior approval from STScI).

Red text indicates restricted parameters (for STScI use only).

Brown text indicates text file parameters.

Items in brackets - <value> - are required values.

Items in square brackets - [<value>] - are optional.

Science observations should use the PSA or BOA apertures. The BOA aperture is the same size as the PSA but contains a neutral-density filter that attenuates the source by a factor of ~200. The WCA is intended for wavelength calibrations using the WAVE target. 

Table 11.8: COS Apertures

Aperture

Definition

Size

Usage

PSA

Primary Science Aperture

2.5 arc seconds

Default science aperture

BOA

Bright Object Aperture

2.5 arc seconds

Contains neutral density filter (ND2) for bright objects

WCA

Wavelength Calibration Aperture

20 microns (dispersion) ×

100 microns
(cross-dispersion)

Wavelength Calibrations

Restricted FCA

The FCA is to be used with the DEUTERIUM target for flat-field exposures.

Aperture

Definition

Size

Usage

FCA

Flat-Field Calibration Aperture

0.75 mm × 1.75 mm

Flat-field Calibrations with the deuterium lamp

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11.5.1 COS Internal Calibration Targets
11.5.2 COS Spectral Elements and Central Wavelengths
11.5.4 COS WAVECAL Exposure Parameters
11.5.5 COS Coordinate System



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Change Log

Version Cycle 34 May 2026 

       Editorial changes by the COS team

Version Cycle 33 May 2025

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