HST Call for Proposals and HST Primer for Cycle 24
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Table of Contents
Chapter 1: Introduction
1.1 About this Document
1.2 What’s New This Cycle
1.3 Resources, Documentation and Tools
1.3.1 Phase I “Roadmap”
1.3.2 Cycle 24 Announcement Webpage
1.3.3 Cycle 24 Call for Proposals
1.3.4 Instrument Handbooks
1.3.5 The Astronomer’s Proposal Tool (APT)
and the Aladin Sky Atlas
1.3.6 Exposure Time Calculators (ETCs)
1.3.7 HST Data Archive
1.3.8 Data Reduction and Calibration
1.4 STScI Help Desk
Chapter 2: System Overview
2.1 Telescope Design and Field of View
2.2 Orbital Constraints
2.2.1 Continuous Viewing Zone (CVZ)
2.2.2 South Atlantic Anomaly (SAA)
2.2.3 Predicted HST Position
2.3 Pointing Constraints
2.4 Orientation and Roll Constraints
2.5 Data Storage and Transmission
2.5.1 Onboard Data Storage
Chapter 3: Telescope Performance
3.1 Optical Performance
3.2 HST Guiding Performance
3.3 HST Observing Efficiency
Chapter 4: Cycle 24 Scientific Instruments
4.1 Advanced Camera for Surveys (ACS)
4.2 Wide Field Camera 3 (WFC3)
4.3 Fine Guidance Sensor (FGS)
4.4 Cosmic Origins Spectrograph (COS)
4.4.1 Far-Ultraviolet Channel (COS/FUV)
4.4.2 Near-Ultraviolet Channel (NUV)
4.4.3 COS FUV XDL Gain Sag
4.4.4 Optimizing the Science Return of COS
4.5 Space Telescope Imaging Spectrograph (STIS)
4.6 Additional Observing Modes
4.6.1 Imaging Polarimetry
4.6.2 Slitless Imaging Spectroscopy
4.6.3 Ramp and Quad Filters
4.6.4 Coronagraphy
4.6.5 Observations with Two Instruments - Parallel Observing
4.7 Instrument Comparisons
4.7.1 HST Imaging
4.7.2 Spectrographs
Chapter 5: Observing Considerations
5.1 Bright-Object Constraints
5.1.1 ACS, COS & STIS
5.1.2 FGS
5.1.3 WFC3
5.2 Target Acquisitions
5.2.1 Target Acquisition without the Ground System
5.2.2 Target Acquisition with Ground System Support
5.3 Solar System Targets
5.4 Offsets, Patterns, and Dithering
5.5 Spatial Scans
Chapter 6: Orbit Calculation
for a Phase I Proposal
6.1 Overview of an Observing Program
6.1.1 General Observer (GO) Programs
6.1.2 Snapshot Programs
6.2 HST Visits
6.2.1 Defining New Visits and Optimizing Scheduling
Efficiency and Flexibility
6.2.2 Instrument Specific Limitations on Visits
6.3 The Orbital Visibility Period
6.4 Acquisition Times and Instrument Overheads
6.4.1 Guide Star Acquisition Times
6.4.2 Target Acquisition Times
6.4.3 Instrument Overhead Times
6.4.4 Telescope Repositioning Overhead Times
6.5 Constructing the Program
Chapter 7: Data Processing
and the
HST Data Archive
7.1 Routine Science Data Processing
7.1.1 Space Telescope Science Data Analysis System
7.2 The HST Data Archive
7.2.1 Web Access to the HST Data Archive
7.3 Hubble Legacy Archive (HLA)
7.4 Hubble Source Catalogs (HSC)
Appendix A: Orbit Calculation Examples
A.1 ACS Example
A.2 COS Examples
A.2.1 Example 1: COS NUV Imaging and Spectroscopy
in One Orbit
A.2.2 Example 2: COS NUV Imaging and FUV Spectroscopy
in Two Orbits
A.3 FGS Example
A.4 STIS Example
A.5 WFC3 Examples
A.5.1 Example 1: IR, 1 orbit, 2 filters
A.5.2 Example 2: UVIS, Dithering, 2 Orbits, 1 Filter
Appendix B: HST Mission
B.1 Servicing Missions and Instrument Complements
B.1.1 Servicing Mission 1 (SM1)
B.1.2 Servicing Mission 2 (SM2)
B.1.3 Loss and Recovery of NICMOS
B.1.4 Servicing Missions 3A (SM3A) and 3B (SM3B)
B.1.5 Loss of STIS
B.1.6 Loss of ACS Wide Field Camera and High Resolution
B.1.7 SM4
Appendix C: Legacy Instruments
C.1 Faint Object Camera (FOC)
C.2 Faint Object Spectrograph (FOS)
C.3 Goddard High Resolution Spectrograph (GHRS)
C.4 High Speed Photometer (HSP)
C.5 Wide Field and Planetary Camera 1 (WF/PC)
C.6 Wide Field and Planetary Camera 2 (WFPC2)
C.7 The Advanced Camera for Surveys High
Resolution Channel (ACS/HRC)
C.8 Near Infrared Camera and Multi-Object
Spectrometer (NICMOS)
Appendix D: Internet Links
Appendix E: Glossary of Acronyms
and Abbreviations

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