STScI

Cosmic Origins Spectrograph Instrument Handbook for Cycle 17

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Table of Contents


Table of Contents

Acknowledgments

Chapter 1: Introduction

1.1 Purpose
1.1.1 Document conventions
1.1.2 FEFU: Femto-erg Flux Unit
1.2 Preparing Proposals and Observing with COS
1.2.1 The STScI Spectrographs Branch and COS Team
1.2.2 The STScI Help Desk
1.2.3 COS web pages and supporting information
1.2.4 Non-proprietary COS data

Chapter 2: Special Considerations for Cycle 17

2.1 SM4 and the Installation of COS
2.2 Knowledge of Instrument Performance
2.3 SMOV
2.4 The Availability of COS During Cycle 17
2.5 Limitations on Proposing to Use COS
2.5.1 The COS GTO program
2.5.2 SNAPshots with COS
2.5.3 Non-point sources uses of COS
2.6 Should I Use STIS instead of COS?

Chapter 3: A Tour through COS

3.1 COS' Location in the HST Focal Plane
3.2 COS' Capabilities
3.2.1 Signal-to-noise considerations
3.2.2 Photometric (flux) precision
3.2.3 Wavelength accuracy
3.2.4 Sensitivity
3.2.5 Non-linear photon counting effects (dead-time correction)
3.3 The Design of COS
3.3.1 Optical Configuration
3.3.2 Apertures
3.3.3 The FUV and NUV Channels
3.3.4 Detectors
3.3.5 On-board Calibration Lamps
3.3.6 Mechanisms
3.4 Basic Instrument Operations
3.4.1 Target acquisitions
3.4.2 TIME-TAG and ACCUM
3.4.3 Wavelength calibration
3.4.4 Typical observing sequences
3.4.5 Data storage and transfer
3.5 COS Quick Reference Guide

Chapter 4: Detector Performance

4.1 The FUV XDL
4.1.1 XDL properties
4.1.2 XDL spectrum response
4.1.3 XDL read-out format
4.1.4 Analog-to-digital conversion
4.1.5 Stim pulses (e-stims)
4.1.6 Pulse-height distributions
4.1.7 FUV detector lifetime adjustments
4.2 The NUV MAMA
4.2.1 MAMA properties
4.2.2 MAMA spectral response
4.2.3 MAMA non-linearity
4.2.4 Detector format
4.2.5 Read-out format, A-to-D conversion, etc.

Chapter 5: Spectroscopy with COS

5.1 Configurations and Optical Elements
5.2 Exposure Time Considerations
5.3 Apertures
5.4 TIME-TAG or ACCUM?
5.4.1 TIME-TAG mode
5.4.2 ACCUM mode
5.5 FUV gap coverage and single segment usage
5.6 Internal Wavelength Calibration Exposures
5.6.1 What "TAGFLASH" does during TIME-TAG observations
5.6.2 AUTO wavecals (when "Tagflash" is not used)
5.6.3 User-specified wavelength calibration exposures (GO wavecals)
5.7 Achieving Higher Signal-to-noise
5.8 EXTENDED
5.9 Calibrations
5.9.1 Internal calibrations
5.10 FUV Wavelength Settings And Ranges

Chapter 6: NUV Imaging

6.1 Summary
6.2 Configurations and Optical Elements
6.3 Exposure Time Considerations
6.4 TIME-TAG or ACCUM?
6.5 Attenuation Considerations
6.6 Extended Objects
6.7 Image Characteristics

Chapter 7: Target Acquisitions

7.1 Planning a COS Acquisition
7.2 Safety First: Bright Object Protection
7.2.1 FUV bright object protection
7.2.2 NUV bright object protection
7.2.3 Screening limits
7.2.4 Risks from nearby objects
7.3 How Accurate an Acquisition Do I Need?
7.3.1 Centering accuracy and photometric precision
7.3.2 Centering accuracy and the wavelength scale
7.3.3 Centering accuracy and spectroscopic resolution
7.4 COS Acquisitions and Coordinate Accuracy
7.5 Imaging Acquisitions
7.5.1 Exposure times and count rates
7.5.2 Imaging acquisitions with mediocre coordinates
7.6 FUV Dispersed-Light Acquisitions
7.6.1 FUV dispersed-light acquisition summary
7.6.2 Mode=ACQ: The spiral target search
7.6.3 PEAKXD: Peaking up in the cross-dispersion direction
7.6.4 PEAKD: Peaking up in the along-dispersion direction
7.7 NUV Dispersed-Light Acquisitions
7.8 Acquisition Techniques for Crowded Regions

Chapter 8: Observing Strategy and Phase I

8.1 Designing a COS Observing Proposal
8.1.1 Identify the science requirements and COS configuration
8.1.2 Use of Available-but-Unsupported capabilities
8.1.3 Calculate exposure time and assess feasibility
8.1.4 Identify the need for additional exposures
8.1.5 Estimating data volume
8.1.6 Determine total orbit request
8.2 Bright-Object Protection
8.2.1 Limiting magnitudes and bright object limits
8.3 Patterns and Dithering
8.4 A "Road Map" for Optimizing Observations
8.4.1 Get the tools and rules
8.4.2 Choose instrument configurations
8.5 Parallel Observations While Using COS

Chapter 9: Overheads and Orbit Usage Determination

9.1 Summary
9.2 Generic Observatory Overhead
9.3 Spectral Element Movement Overheads
9.4 Acquisition Overheads
9.5 Science Exposure Overheads
9.6 Examples of Orbit Estimates
9.6.1 Example 1: NUV TIME-TAG
9.6.2 Example 2: NUV plus FUV TIME-TAG
9.6.3 Example 3: FUV Acquisition plus FUV TIME-TAG
9.6.4 FUV TIME-TAG with BOA and FLASH=NO

Chapter 10: Exposure-Time Calculator (ETC)

10.1 The COS Exposure Time Calculators
10.2 Count Rate, Sensitivity, and S/N
10.2.1 Centering accuracy and photometric precision
10.3 Detector and Sky Backgrounds
10.3.1 Detector dark background
10.3.2 Earthshine
10.3.3 Zodiacal light
10.3.4 Geocoronal airglow emission
10.4 Extinction Correction
10.5 Tabular Sky Backgrounds
10.6 Examples
10.6.1 A Flat-spectrum source
10.6.2 An early-type star
10.6.3 A solar-type star with an emission line

Chapter 11: COS in Phase II

11.1 Essential Program Information
11.2 A "Roadmap" for Phase II Program Preparation
11.3 Get the Tools and Rules
11.4 Specify Instrument Usage Particulars
11.4.1 Gather essential target information
11.4.2 Assess target acquisition strategies
11.4.3 Determine the science exposure needs
11.5 Recap of COS Optional Parameters

Chapter 12: Data Products and Data Reduction

12.1 COS Data Products
12.1.1 FUV TIME-TAG data
12.1.2 NUV TIME-TAG data
12.1.3 FUV ACCUM data
12.1.4 NUV ACCUM data
12.1.5 NUV ACQ/IMAGE data

Chapter 13: Reference Material

13.1 Apertures
13.1.1 The Aperture Mechanism (ApM)
13.1.2 Primary Science Aperture
13.1.3 Bright Object Aperture
13.1.4 Wavelength Calibration Aperture
13.1.5 Flat-field Calibration Aperture
13.2 COS Mechanisms
13.2.1 Optics Select Mechanism 1 (OSM1)
13.2.2 Optics Select Mechanism 2 (OSM2)
13.2.3 External shutter
13.3 COS Optical Elements
13.3.1 FUV Gratings
13.3.2 NUV Gratings
13.3.3 Mirrors

Glossary


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