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Acronyms
|
ADC |
Atmospheric Dispersion Corrector or Analog to Digital Converter (Depends on context) |
|
ADI |
Angular Differential Imaging |
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AEOS |
Advanced Electro-Optical System (USAF Telescope on Maui) |
|
AGB |
Asymptotic Giant Branch |
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ALMA |
Atacama Large Millimeter Array
|
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ATEUI |
Acceptance Test and Engineering User Interface |
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ALTAIR |
ALTitude-conjugate Adaptive optics for the InfraRed |
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AMNH |
American Museum of Natural History |
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AO |
Adaptive Optics |
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AOC |
Adaptive Optics Computer
|
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API |
Application Programming Interface |
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APLC |
Apodized Pupil Lyot Coronagraph |
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AR |
Anti Reflection (coating for tranmissive elements) |
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AU |
Astronomical Unit (1.495 X 1011 m) |
|
ATP |
Acceptance and Test Plan
|
|
AURA |
Association of Universities for Research in Astronomy |
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CAL |
Calibration Subsystem |
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CANOPUS |
The optical bench and associated electronics. Everything that is within the box attached to the ISS. Other subsystems of GeMS include the BTO (Beam Transfer Optics), the laser and LSE (Laser Service Enclosure) and the LLT (Laser Launch Telescope). |
|
CCB |
Change Control Board |
|
CCIT |
Coherent Communications, Imaging and Targeting
|
|
CCC |
Closed Cycle Coolor (CCR) |
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CCR |
Closed Cycle Refrigerator (CCC) |
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CDR |
Critical Design Review |
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CEH |
Command Event Handler (GPI interface to GIAPI) |
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CfAO |
Center for Adaptive Optics
|
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CFHT |
Canada France Hawaii Telescope |
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CGS |
Centimeter gram second system of units |
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CoDR |
Conceptual Design Review |
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CoPI |
Co-Principal Investigator |
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CoPM |
Co-Project Manager
|
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COR |
Coronagraph |
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CP |
Cerro Pachon |
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CVNDF |
Continuously Variable Neutral Density Filter |
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CWS |
Cold Working Surface |
|
d |
Subaperture size projected on the primary mirror (18 cm for GPI)
|
|
D |
Telescope primary mirror diameter (8.0 m for Gemini) |
|
DAC |
Digital to Analog Convertor |
|
DAR |
Differential Atmospheric Refraction |
|
DARPA |
Defense Advanced Research Projects Agency |
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DD |
Double (image) difference
|
|
DHS |
Data Handling System |
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DM |
Deformable Mirror |
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DMS |
Document Management system |
|
DRP |
Data Reduction Pipeline |
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EFS |
External Frame Structure
|
|
EPICS |
Experimental Physics and Industrial Control System |
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ESO |
European Southern Observatory |
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ESO VLT |
European Southern Observatory Very Large Telescope |
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EXAOC |
Extreme Adaptive Optics Coronagraph (original name for GPI) |
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FDRP |
Final Data Reduction Pipeline
|
|
FEA |
Finite Element Analysis |
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FITS |
Flexible Image Transport System |
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FOV |
Field Of View |
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FPRD |
Functional and Performance Requirements Document |
|
FPM |
Focal Plane Mask
|
|
FSM |
Fine Steering Mirror |
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FSS |
Flexure Sensitive Structure |
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FTR |
Fourier Transform wavefront Reconstructor |
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FWHM |
Full Width at Half Maximum |
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GCAL |
Gemini Facility Calibration Unit
|
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GDSN |
Gemini Data Storage network |
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GeMS |
Gemini MCAO System |
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GLAO |
Ground Layer Adaptive Optics |
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GMOS |
Gemini Multi Object Spectrograph |
|
GMP |
Gemini Master Process
|
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GPI |
Gemini Planet Imager |
|
GPOL |
Gemini Polarization module (obsolete) |
|
GSAOI |
Gemini South Adaptive Optics Imager |
|
HCIT |
High Contrast Imaging Test bed |
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HEBS |
High Energy Beam Sensitive
|
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HIA |
Herzberg Institute of Astrophysics |
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HL |
High Level |
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ICD |
Interface Control Document |
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ICS |
Instrument Control System |
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IDL |
Image Display Language (RSI Inc.)
|
|
IFS |
Integral Field Spectrograph |
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IMF |
Initial Mass Function |
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INO |
Institut Nationale d'Optique |
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IR |
Infrared-Red |
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IRAS |
Infra-Red Astronomy Satellite
|
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ISS |
Instrument Support Structure |
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IWD |
Inner Working Distance |
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JPL |
Jet Propulsion Laboratory |
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JWST |
James Webb Space Telescope |
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LAN |
Local Area Network
|
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LAO |
Laboratory for Adaptive Optics |
|
LLNL |
Lawrence Livermore National Lab |
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mas |
milli-arcsec (4.848 nanoradian) |
|
M1 |
Gemini primary mirror |
|
M2 |
Gemini secondary mirror
|
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M3 |
Gemini Tertiary (or science fold mirror) |
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MCD |
Motion Control Daemon |
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MEMS |
Micro Electro-Mechanical System |
|
MJ |
Mass of Jupiter (1.8988 X 1027 kg) |
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MK |
Mauna Kea
|
|
MWBS |
Multi-Wavelength Beam Splitter |
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MWI |
Multi-Wavelength Imager |
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N |
Number of subapertures across the primary mirror (44 for GPI) |
|
NCP |
Non-Common Path |
|
NDR |
Non-Destructive Read
|
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NIRC2 |
Near Infrared Camera 2 for adaptive optics at Keck |
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NIRSPEC |
Near Infrared Spectrometer instrument at Keck |
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NRC |
National Research Council (careful, there is an American and a Canadian one, separate entities) |
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NSF |
National Science Foundation |
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NTP |
Network Time Protocol
|
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OAP |
Off Axis Parabola |
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OCDD |
Operational Concept Definition Document |
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OCS |
Observatory Control System |
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ODRP |
On-Line Data Reduction Pipeline |
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OFC |
Optimized-gain Fourier Control
|
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OIWFS |
On-Instrument Wavefront Sensor |
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OIWGS |
On Instrument Wave Front Sensor |
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OMSS |
Opto-Mechanical Superstructure |
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OSIRIS |
OH-Suppressing Infrared Imaging Spectrograph at Keck |
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OT |
Observing Tool
|
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OWD |
Outer Working Distance |
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PA |
Position Angle |
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pc |
Parsec (3.085 X 1016 m) |
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PCS |
Primary Control System |
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PDR |
Preliminary Design Review
|
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PE |
Project Engineer |
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PI |
Principal Investigator |
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Piezo |
Piezo effect actuator |
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PN |
Planetary Nebula |
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pnCCD |
pnSensor based CCD.
|
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PM |
Project Manager |
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PPM |
Pupil Plane Mask |
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PS |
Project Scientist |
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PSDI |
Phase-Shifting Diffraction Interferometer |
|
PSF |
Point Spread Function
|
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PZT |
Lead Zirconium Titanate (Piezo effect actuator) |
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QE |
Quantum Efficiency |
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QPT |
Queue Planning Tool |
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RFP |
Request for Proposal |
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RMS |
Root Mean Square
|
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ROC |
Radius Of Curvature |
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ROI |
Region of Interest |
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RPC |
Remote Procedure Call |
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RSS |
Root Sum Square |
|
SC |
Science Camera
|
|
SCC |
Supervisory and Component-Control Computer (Obsolete, see TLC) |
|
SCS |
Gemini Telescope Secondary Control System |
|
SD |
Simple (image) difference |
|
SE |
Systems Engineer |
|
Seqexec |
Sequence Executor
|
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SFWFS |
Spatially Filtered Wave Front Sensor |
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SNR |
Signal to Noise Ratio |
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SOW |
Statement of Work |
|
SPIE |
Society of Photoelectric Instrumentation Engineers |
|
SRD |
Software Requirements Document
|
|
SSDI |
Simultaneous Spectral Differential Imaging |
|
SSD |
Speckle Suppressing Device |
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SSICD |
Subsystem Interface Control Document |
|
SSRD |
Subsystem Requirements Document |
|
STScI |
Space Telescope Science Institute
|
|
TBC |
To Be Confirmed |
|
TBD |
To Be Determined |
|
TCS |
Telescope Control System |
|
TLC |
Top Level Computer (for GPI was SCC) |
|
TMA |
Three Mirror Anastigmat
|
|
TPF |
Terrestrial Planet Finder |
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TRIDENT |
Three Channel Differential Imager for CHF Telescope |
|
T/T |
Tip/Tilt |
|
T/T/F |
Tip/Tilt/Focus |
|
UCB |
University of California, Berkeley
|
|
UCLA |
University of California, Los Angeles |
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UCO |
UCO/Lick Observatory |
|
UCSC |
University of California, Santa Cruz |
|
UdeM |
Université de Montréal |
|
USAF |
United States Air Force
|
|
VLT |
Very Large Telescope |
|
WBS |
Work Breakdown Structure |
|
WD |
White Dwarf |
|
WFE |
WaveFront Error |
|
WFS |
WaveFront Sensor
|
|
WIRCAM |
Wide-Field Infrared Camera |