Glossary
The following terms and acronyms are used in this Handbook.
A-D | Analog to Digital |
ACS | Advanced Camera for Surveys |
ABMAG | –2.5 log (Fν) – 48.60 where Fν is the flux from the source in erg/cm2/s/hz |
APT | Astronomer’s Proposal Tool. Used to construct Phase I and Phase II observing proposals: https://www.stsci.edu/scientific-community/software/astronomers-proposal-tool-apt |
BOP | Bright-Object Protection |
CALSTIS | STIS calibration pipeline software: https://stistools.readthedocs.io/en/latest/calstis.html |
CCD | Charge Coupled Device. Solid-state photon counting device |
CDBS | Calibration Data Base. System for maintaining reference files and tables used to calibrate HST observational datasets. |
CIM | Calibration insert mechanism |
COS | Cosmic Origins Spectrograph |
CP, CfP | Call for Proposals |
CR | Cosmic ray |
CR-SPLIT | Division of a CCD exposure into shorter exposures to be used for cosmic ray rejection |
CTE | Charge Transfer Efficiency |
CTI | Charge Transfer Inefficiency, CTI = 1 – CTE |
CVZ | Continuous Viewing Zone. A range of target declinations for which full-orbit observations may be obtained (without Earth occultation). |
DQ | Data Quality. DQ flags in the data files indicate various potential or actual problems with the data. |
DHB | Data Handbook: https://hst-docs.stsci.edu/stisdhb |
DN | Data Number |
ETC | Exposure Time Calculator. ETCs are Web based tools, which can be accessed at https://etc.stsci.edu. |
ERO | Early Release Observations |
FGS | Fine Guidance Sensors |
FITS | Flexible Image Transport System. A generic IEEE and NASA defined standard file format used for storing image data. |
FOC | Faint Object Camera |
FOS | Faint Object Spectrograph |
FOV | Field of View |
FSW | Flight Software |
FTP | File Transfer Protocol. Basic tool used to retrieve files from a remote system. Ask your system manager for information about using FTP. |
FUV | Far ultraviolet (~912–2000 Å) |
FWHM | Full Width at Half Maximum |
GALEX | Galaxy Evolution Explorer |
GHRS | Goddard High-Resolution Spectrograph |
GO | General Observer |
GSC | Guide Star Catalog |
GTO | Guaranteed Time Observer |
Help Desk | Facility for getting help on HST related topics: http://hsthelp.stsci.edu or help@stsci.edu. |
HITM | Hole in the Mirror. Part of the optical path for some calibration lamps. |
HSP | High-Speed Photometer |
HST | Hubble Space Telescope |
HUT | Hopkins Ultraviolet Telescope |
ICD | Interface control document. Defines data structures used between software or systems to ensure compatibility. |
IDT | Instrument Definition Team |
IHB | Instrument Handbook |
IR | Infrared |
IRAF | Image Reduction and Analysis Facility. The environment in which STSDAS operates (no longer supported). |
IS | Instrument Scientist |
ISR | Instrument Science Report |
IUE | International Ultraviolet Explorer |
K | Degree Kelvin |
LMC | Large Magellanic Cloud |
LSF | Line spread function |
MAMA | Multi-Anode Microchannel Array. STIS uses MAMA detectors for FUV and NUV observations. |
MAST | Barbara A. Mikulski Archive for Space Telescopes. A repository for data from HST, JWST, and other missions: https://mast.stsci.edu/ |
MCP | Microchannel Plate |
MSM | Mode-Selection Mechanism |
ND | Neutral density |
NIR | Near infrared |
NICMOS | Near-Infrared Camera and Multi-Object Spectrograph |
NUV | Near ultraviolet (~2000–4000 Å) |
OSS | Observation Support System |
OTA | Optical Telescope Assembly |
OTFR | On-the-Fly Re-processing. Re-processing of data, using the most recent/appropriate reference files and software, when the data are requested from the archive. |
PC | Program Coordinator |
Peakdown | Movement of a target along a slit to center it under an occulting bar. |
Peakup | Movement of a target in one or both directions to center it in a slit. |
Phase | A proposal for observing time on HST |
Phase | An approved HST proposal; includes detailed instructions for how a program is to be executed |
PI | Principal investigator |
PSF | Point-spread function |
QE | Quantum efficiency |
QEH | Quantum efficiency hysteresis |
QSO | Quasi-stellar object |
RA | Right ascension |
reference file | Data file containing STIS parameters or calibration information which is used by the pipeline |
rms | Root mean square |
SAA | South Atlantic anomaly. A region of enhanced background radiation. STIS is not used when the orbital path of HST passes through the SAA. |
SIM | Space Interferometry Mission |
SITe | Scientific Image Technologies; company that designed the STIS CCD |
SM4 | Servicing mission 4. Servicing mission in which STIS operations were restored |
SMOV | Servicing Mission Observatory Verification |
S/N, SNR | Signal-to-noise ratio |
ST-ECF | Space Telescope European Coordinating Facility |
STAN | Space Telescope Analysis Newsletter |
stenv | Environment for HST and JWST pipelines and (most) packages formerly available through astroconda: https://stenv.readthedocs.io/en/latest/ |
STIS | Space Telescope Imaging Spectrograph |
stistools | A suite of software tools for STIS data calibration and analysis: https://stistools.readthedocs.io/en/latest/ |
stis_cti | Pixel-based CTI correction software for the STIS CCD: https://www.stsci.edu/hst/instrumentation/stis/data-analysis-and-software-tools/pixel-based-cti |
STMAG | STScI magnitude system; –2.5 log (Fλ) –21.10 where Fλ is the flux from the source in erg/cm2/s/Å |
STScI | Space Telescope Science Institute |
STSDAS | Space Telescope Science Data Analysis System. The complete suite of IRAF data analysis and calibration routines used to process HST data (no longer supported). |
SV | Science verification. Process of taking observations that can be used for HST instrument calibration. |
synphot | Synthetic Photometry software package: https://synphot.readthedocs.io/en/latest/ |
TAC | Telescope Allocation Committee |
TAS | Target Acquisitions Simulator: https://stistarg.readthedocs.io/en/latest/ |
TDS | Time-dependent Sensitivity |
TIR | Technical Instrument Report |
URL | Uniform resource locator. Address for websites. |
UV | Ultraviolet |
WF/PC | Wide Field/Planetary Camera |
WFPC2 | Wide Field Planetary Camera-2. Replacement for WF/PC installed during first servicing mission of December 1993. |
WFC3 | Wide Field Camera 3 |
-
STIS Instrument Handbook
- • Acknowledgments
- Chapter 1: Introduction
-
Chapter 2: Special Considerations for Cycle 33
- • 2.1 Impacts of Reduced Gyro Mode on Planning Observations
- • 2.2 STIS Performance Changes Pre- and Post-SM4
- • 2.3 New Capabilities for Cycle 33
- • 2.4 Use of Available-but-Unsupported Capabilities
- • 2.5 Choosing Between COS and STIS
- • 2.6 Scheduling Efficiency and Visit Orbit Limits
- • 2.7 MAMA Scheduling Policies
- • 2.8 Prime and Parallel Observing: MAMA Bright-Object Constraints
- • 2.9 STIS Snapshot Program Policies
- Chapter 3: STIS Capabilities, Design, Operations, and Observations
- Chapter 4: Spectroscopy
- Chapter 5: Imaging
- Chapter 6: Exposure Time Calculations
- Chapter 7: Feasibility and Detector Performance
-
Chapter 8: Target Acquisition
- • 8.1 Introduction
- • 8.2 STIS Onboard CCD Target Acquisitions - ACQ
- • 8.3 Onboard Target Acquisition Peakups - ACQ PEAK
- • 8.4 Determining Coordinates in the International Celestial Reference System (ICRS) Reference Frame
- • 8.5 Acquisition Examples
- • 8.6 STIS Post-Observation Target Acquisition Analysis
- Chapter 9: Overheads and Orbit-Time Determination
- Chapter 10: Summary and Checklist
- Chapter 11: Data Taking
-
Chapter 12: Special Uses of STIS
- • 12.1 Slitless First-Order Spectroscopy
- • 12.2 Long-Slit Echelle Spectroscopy
- • 12.3 Time-Resolved Observations
- • 12.4 Observing Too-Bright Objects with STIS
- • 12.5 High Signal-to-Noise Ratio Observations
- • 12.6 Improving the Sampling of the Line Spread Function
- • 12.7 Considerations for Observing Planetary Targets
- • 12.8 Special Considerations for Extended Targets
- • 12.9 Parallel Observing with STIS
- • 12.10 Coronagraphic Spectroscopy
- • 12.11 Coronagraphic Imaging - 50CORON
- • 12.12 Spatial Scans with the STIS CCD
-
Chapter 13: Spectroscopic Reference Material
- • 13.1 Introduction
- • 13.2 Using the Information in this Chapter
-
13.3 Gratings
- • First-Order Grating G750L
- • First-Order Grating G750M
- • First-Order Grating G430L
- • First-Order Grating G430M
- • First-Order Grating G230LB
- • Comparison of G230LB and G230L
- • First-Order Grating G230MB
- • Comparison of G230MB and G230M
- • First-Order Grating G230L
- • First-Order Grating G230M
- • First-Order Grating G140L
- • First-Order Grating G140M
- • Echelle Grating E230M
- • Echelle Grating E230H
- • Echelle Grating E140M
- • Echelle Grating E140H
- • PRISM
- • PRISM Wavelength Relationship
-
13.4 Apertures
- • 52X0.05 Aperture
- • 52X0.05E1 and 52X0.05D1 Pseudo-Apertures
- • 52X0.1 Aperture
- • 52X0.1E1 and 52X0.1D1 Pseudo-Apertures
- • 52X0.2 Aperture
- • 52X0.2E1, 52X0.2E2, and 52X0.2D1 Pseudo-Apertures
- • 52X0.5 Aperture
- • 52X0.5E1, 52X0.5E2, and 52X0.5D1 Pseudo-Apertures
- • 52X2 Aperture
- • 52X2E1, 52X2E2, and 52X2D1 Pseudo-Apertures
- • 52X0.2F1 Aperture
- • 0.2X0.06 Aperture
- • 0.2X0.2 Aperture
- • 0.2X0.09 Aperture
- • 6X0.2 Aperture
- • 0.1X0.03 Aperture
- • FP-SPLIT Slits 0.2X0.06FP(A-E) Apertures
- • FP-SPLIT Slits 0.2X0.2FP(A-E) Apertures
- • 31X0.05ND(A-C) Apertures
- • 0.2X0.05ND Aperture
- • 0.3X0.05ND Aperture
- • F25NDQ Aperture
- 13.5 Spatial Profiles
- 13.6 Line Spread Functions
- • 13.7 Spectral Purity, Order Confusion, and Peculiarities
- • 13.8 MAMA Spectroscopic Bright Object Limits
-
Chapter 14: Imaging Reference Material
- • 14.1 Introduction
- • 14.2 Using the Information in this Chapter
- 14.3 CCD
- 14.4 NUV-MAMA
-
14.5 FUV-MAMA
- • 25MAMA - FUV-MAMA, Clear
- • 25MAMAD1 - FUV-MAMA Pseudo-Aperture
- • F25ND3 - FUV-MAMA
- • F25ND5 - FUV-MAMA
- • F25NDQ - FUV-MAMA
- • F25QTZ - FUV-MAMA, Longpass
- • F25QTZD1 - FUV-MAMA, Longpass Pseudo-Aperture
- • F25SRF2 - FUV-MAMA, Longpass
- • F25SRF2D1 - FUV-MAMA, Longpass Pseudo-Aperture
- • F25LYA - FUV-MAMA, Lyman-alpha
- • 14.6 Image Mode Geometric Distortion
- • 14.7 Spatial Dependence of the STIS PSF
- • 14.8 MAMA Imaging Bright Object Limits
- Chapter 15: Overview of Pipeline Calibration
- Chapter 16: Accuracies
-
Chapter 17: Calibration Status and Plans
- • 17.1 Introduction
- • 17.2 Ground Testing and Calibration
- • 17.3 STIS Installation and Verification (SMOV2)
- • 17.4 Cycle 7 Calibration
- • 17.5 Cycle 8 Calibration
- • 17.6 Cycle 9 Calibration
- • 17.7 Cycle 10 Calibration
- • 17.8 Cycle 11 Calibration
- • 17.9 Cycle 12 Calibration
- • 17.10 SM4 and SMOV4 Calibration
- • 17.11 Cycle 17 Calibration Plan
- • 17.12 Cycle 18 Calibration Plan
- • 17.13 Cycle 19 Calibration Plan
- • 17.14 Cycle 20 Calibration Plan
- • 17.15 Cycle 21 Calibration Plan
- • 17.16 Cycle 22 Calibration Plan
- • 17.17 Cycle 23 Calibration Plan
- • 17.18 Cycle 24 Calibration Plan
- • 17.19 Cycle 25 Calibration Plan
- • 17.20 Cycle 26 Calibration Plan
- • 17.21 Cycle 27 Calibration Plan
- • 17.22 Cycle 28 Calibration Plan
- • 17.23 Cycle 29 Calibration Plan
- • 17.24 Cycle 30 Calibration Plan
- • 17.25 Cycle 31 Calibration Plan
- • 17.26 Cycle 32 Calibration Plan
- Appendix A: Available-But-Unsupported Spectroscopic Capabilities
- • Glossary