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Glossary

The following terms and acronyms are used in this handbook.

A-D: Analog to digital.

CCD: Charge-coupled device. Solid-state, light detecting device.

CDBS: Calibration Data Base. System for maintaining reference files and tables used to calibrate HST observational datasets.

CIT: California Institute of Technology.

COBE: Cosmic Background Explorer.

COSTAR: Corrective Optics Space Telescope Axial Replacement.

CP: Call for Proposals.

CR: Cosmic ray.

CVZ: Continuous viewing zone.

DQ: Data quality.

DQE: Detector quantum efficiency.

DN: Data number.

ETC: Exposure Time Calculator.

FAQ: Frequently asked questions.

FGS: Fine Guidance Sensors.

FITS: Flexible Image Transport System. A generic IEEE- and NASA-defined standard used for storing image data.

FOC: Faint Object Camera.

FOM: Field Offset Mirror (or mechanism)

FOS: Faint Object Spectrograph.

FOV: Field of view.

FPA: Focal plane array.

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.

FWHM: Full width at half maximum.

GASP: Guide Star Astrometric Support Program.

GEIS: Generic Edited Information Set. The multigroup format used by STSDAS for storing some HST image data.

GHRS: Goddard High-Resolution Spectrograph.

GO: General Observer.

GTO: Guaranteed Time Observer.

HSP: High-Speed Photometer.

HST: Hubble Space Telescope.

ICD: Interface control document. Defines data structures used between software or systems to ensure compatibility.

IDT: Instrument Development Team.

IR: Infrared.

IRAF: Image Reduction and Analysis System. The system on which -STSDAS is built.

IUE: International Ultraviolet Explorer.

K: Degree Kelvin.

LSF: Line spread function.

MOS: Multi-object spectroscopy.

ND: Neutral density.

NICMOS: Near-Infrared Camera and Multi-Object Spectrograph.

NUV: Near ultraviolet.

OPUS: OSS and PODPS Unified Systems.

OSS: Observation Support System.

OTA: Optical Telescope Assembly.

PAM: Pupil Alignment Mirror (or mechanism).

PI: Principal investigator.

PODPS: Post-Observation Data Processing System.

PSF: Point spread function.

QE: Quantum efficiency.

RA: Right ascension.

rms: Root mean square.

SAM: Small angle motion.

SLTV: System level thermal vacuum (testing phase).

SMOV: Servicing Mission Orbital Verification.

S/N: Signal-to-noise ratio.

SSR: Solid state recorder.

ST-ECF: Space Telescope European Coordinating Facility.

STEIS: Space Telescope Electronic Information System. The World Wide Web host from which information, software, documentation, and other resources pertaining to the HST can be obtained.

STIS: Space Telescope Imaging Spectrograph.

STScI: Space Telescope Science Institute.

STSDAS: Space Telescope Science Data Analysis System. The complete suite of data analysis and calibration routines used to process HST data.

SV: Science verification. Process of taking observations that can be used for HST instrument calibration.

TAC: Telescope Allocation Committee.

TEC: Thermal electrically cooled.

URL: Uniform resource locator. Address for WWW.

UV: Ultraviolet.

VCS: Vapor cooled shield.

WF/PC: Wide Field/Planetary Camera.

WFPC2: Wide Field Planetary Camera-2. Replacement for WF/PC installed during first servicing mission of December 1993.

WWW: World Wide Web. Hypertext-oriented method for finding and retrieving information over the Internet.

YSO: Young stellar object.



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Copyright © 1997, Association of Universities for Research in Astronomy. All rights reserved. Last updated: 07/24/97 15:36:55