Table of Contents Advanced Camera for Surveys Instrument Handbook for Cycle 19 Acknowledgments Chapter 1: Introduction Chapter 2: Changes After SM4 and Considerations for Cycle 19 2.1 SM4 Repair of ACS 2.2 Comparison of ACS/WFC and WFC3/UVIS 2.3 Comparison of ACS/HRC and WFC3/UVIS 2.4 Dithering in Cycle 19 Chapter 3: Introduction to ACS 3.1 ACS Location in the HST Focal Plane 3.2 Instrument Capabilities 3.3 Instrument Design 3.3.1 Detectors 3.3.2 ACS Optical Design 3.4 Basic Instrument Operations 3.4.1 Target Acquisitions 3.4.2 Typical ACS Observing Sequence 3.4.3 Data Storage and Transfer 3.5 ACS Quick Reference Guide Chapter 4: Detector Performance 4.1 Overview 4.2 The CCDs 4.2.1 Detector Properties 4.2.2 CCD Spectral Response 4.2.3 Quantum Efficiency Hysteresis 4.2.4 CCD Long-Wavelength Fringing 4.2.5 Readout Format 4.2.6 Analog-To-Digital Conversion 4.2.7 Flat Fields 4.3 CCD Operations and Limitations 4.3.1 CCD Saturation: The CCD Full Well 4.3.2 CCD Shutter Effects on Exposure Times 4.3.3 Read Noise 4.3.4 Dark Current 4.3.5 Warm and hot pixels 4.3.6 Cosmic Rays 4.3.7 Charge Transfer Efficiency 4.3.8 UV Light and the HRC CCD 4.4 The SBC MAMA 4.4.1 MAMA Properties 4.4.2 SBC Spectral Response 4.4.3 Optical Performance 4.5 SBC Operations and Limitations 4.5.1 SBC Scheduling Policies 4.5.2 MAMA Overflow of the 16 Bit Buffer 4.5.3 MAMA Darks 4.5.4 SBC Signal-To-Noise Ratio Limitations 4.5.5 SBC Flatfield 4.5.6 SBC Nonlinearity 4.6 SBC Bright-Object Limits 4.6.1 Overview 4.6.2 Observational Limits Chapter 5: Imaging 5.1 Imaging Overview 5.2 Important Considerations for ACS Imaging 5.2.1 Optical Performance 5.2.2 CCD Throughput Comparison 5.2.3 Limiting Magnitudes 5.2.4 Signal-To-Noise Ratios 5.2.5 Saturation 5.2.6 Faint Horizontal Striping in WFC CCDs 5.3 Wide Field Optical CCD Imaging 5.3.1 Filter Set 5.4 High-Resolution Optical and UV Imaging 5.4.1 Filter Set 5.4.2 Multiple Electron Events 5.4.3 Red Leaks 5.5 Ultraviolet Imaging with the SBC 5.5.1 Filter Set 5.5.2 Red Leaks 5.5.3 SBC Imaging Filter Shifts 5.6 ACS Point Spread Functions 5.6.1 CCD Pixel Response Function 5.6.2 Model PSFs 5.6.3 Encircled Energy 5.6.4 Geometric Distortions 5.6.5 PSFs at Red Wavelengths and the UV 5.6.6 Residual Aberrations Chapter 6: Polarimetry, Coronagraphy and Prism/Grism Spectroscopy 6.1 Polarimetry 6.1.1 Introduction 6.1.2 Performance of ACS Polarizers 6.1.3 Implementation of ACS Polarizers 6.1.4 Challenges and Limitations of ACS Polarimetry 6.2 Coronagraphy 6.2.1 Coronagraph Design 6.2.2 Acquisition Procedure and Pointing Accuracy 6.2.3 Vignetting and Flat Fields 6.2.4 Coronagraphic Performance 6.2.5 Subtraction of the coronagraphic PSF 6.2.6 The Off-Spot PSF 6.2.7 Occulting Spot Motions 6.3 Grism/Prism Spectroscopy 6.3.1 WFC G800L 6.3.2 HRC G800L 6.3.3 HRC PR200L 6.3.4 SBC PR110L 6.3.5 SBC PR130L 6.3.6 Observation Strategy 6.3.7 Extraction and Calibration of Spectra Chapter 7: Observing Techniques 7.1 Designing an ACS Observing Proposal 7.1.1 Identify Science Requirements and Define ACS Configuration 7.1.2 Available but Unsupported Modes 7.1.3 Determine Exposure Time and Check Feasibility 7.1.4 Identify Need for Additional Exposures 7.1.5 Data Volume Constraints 7.1.6 Determine Total Orbit Request 7.1.7 Charge Transfer Efficiency 7.1.8 Image Anomalies 7.2 SBC Bright Object Protection 7.2.1 How Do You Determine if You Violate a Bright Object Limit for SBC Exposures? 7.2.2 Policy and Observers’ Responsibility in Phase I and Phase II 7.2.3 Bright-Object Protection for Solar System Observations 7.2.4 Prime and Parallel Observing with the SBC 7.3 Operating Modes 7.3.1 WFC ACCUM Mode 7.3.2 SBC ACCUM Mode 7.4 Patterns and Dithering 7.5 A Road Map for Optimizing Observations 7.6 CCD Gain Selection 7.7 ACS Apertures 7.7.1 WFC Apertures 7.7.2 Ramp Filter Apertures 7.7.3 The Small Filter Apertures 7.7.4 Polarizer Apertures 7.7.5 HRC Apertures 7.7.6 SBC Apertures 7.8 Specifying Orientation on the Sky 7.8.1 Determining Orientation for Phase II 7.9 Parallel Observations 7.9.1 Parallel Observing 7.10 Pointing Stability for Moving Targets Chapter 8: Overheads and Orbit-Time Determination 8.1 Overview 8.2 ACS Exposure Overheads 8.2.1 Subarrays 8.3 Orbit Use Determination Examples 8.3.1 Sample Orbit Calculation 1: 8.3.2 Sample Orbit Calculation 2: 8.3.3 Sample Orbit Calculation 3: 8.3.4 Sample Orbit Calculation 4: 8.3.5 Sample Orbit Calculation 5: Chapter 9: Exposure-Time Calculations 9.1 Overview 9.1.1 The ACS Exposure Time Calculator 9.2 Determining Count Rates from Sensitivities 9.2.1 Imaging 9.2.2 Spectroscopy 9.3 Computing Exposure Times 9.3.1 Calculating Exposure Times for a Given signal-to-noise 9.3.2 Exposure Time Estimates for Red Targets in F850LP 9.4 Detector and Sky Backgrounds 9.4.1 Detector Backgrounds 9.4.2 Sky Background 9.5 Extinction Correction 9.6 Exposure-Time Examples 9.6.1 Example 1: WFC Imaging a Faint Point Source 9.6.2 Example 2: SBC Objective Prism Spectrum of a UV Spectrophotometric Standard Star 9.6.3 Example 3: WFC VIS Polarimetry of the Jet of M87 9.6.4 Example 4: SBC imaging of Jupiter’s Aurora at Lyman-alpha 9.6.5 Example 5: Coronagraphic imaging of the Beta-Pictoris Disk (This HRC mode is longer available) 9.7 Tabular Sky Backgrounds Chapter 10: Imaging Reference Material 10.1 Introduction 10.2 Using the Information in this Chapter 10.2.1 Sensitivity Units and Conversions 10.2.2 Signal-to-Noise 10.2.3 Point Spread Functions WFC/F435W WFC/F475W WFC/F502N WFC/F550M WFC/F555W WFC/F606W WFC/F625W WFC/F658N WFC/F660N WFC/F775W WFC/F814W WFC/F850LP WFC/G800L WFC/CLEAR HRC/F220W HRC/F250W HRC/F330W HRC/F344N HRC/F435W HRC/F475W HRC/F502N HRC/F550M HRC/F555W HRC/F606W HRC/F625W HRC/F658N HRC/F660N HRC/F775W HRC/F814W HRC/F850LP HRC/F892N HRC/G800L HRC/PR200L HRC/CLEAR SBC/F115LP SBC/F122M SBC/F125LP SBC/F140LP SBC/F150LP SBC/F165LP SBC/PR110L SBC/PR130L 10.3 Distortion in the ACS 10.3.1 WFC 10.3.2 HRC 10.3.3 SBC Glossary
