{\Large \bf Acronyms}

{\footnotesize
\begin{tabular}{|p{50pt}|p{400pt}|} \hline 
CAN  & Controller Area Network \\ \hline
CCD  & Charge Coupled Device \\ \hline
CFHT & Canada-France-Hawaii Telescope \\ \hline
DC   & Data Collection - Database or other data storage container. \\ \hline
DML  & Device Meta-Language \\ \hline
DMT  & Dark Matter Telescope \\ \hline
FOM  & Figure of Merit \\ \hline
FOV  & Field of View \\ \hline
FWHM & Full-Width at Half-Maximum \\ \hline
GPC  & Giga-Pixel Camera \\ \hline
GS   & Guide Star \\ \hline
GUI  & Graphical User Interface  \\ \hline
IAU  & International Astronomical Union \\ \hline
IOD  & Initial Orbit Determination \\ \hline
IPP  & Image Processing Pipeline \\ \hline
KBO  & Kuiper Belt Object \\ \hline
LAN  & Local Area Network \\ \hline
LSN  & Local Solar Neighborhood \\ \hline
LSS  & Large-Scale Structure \\ \hline
LSST & Large Synoptic Survey Telescope \\ \hline
MBA  & Main Belt Asteroid \\ \hline
MDS  & Medium-Deep Survey  \\ \hline
MOID & Minimum Orbital Intersection Distance - The minimum distance between two orbits. \\ \hline
MOPS & Moving Object Processing System \\ \hline
MPC  & Minor Planet Center (of the IAU) \\ \hline
NEO  & Near Earth Object - An asteroid or comet with perihelion < 1.3AU. \\ \hline
OBS  & Observation Seqencer \\ \hline
ODA  & OTIS Data Archive \\ \hline
OOF  & OTIS Observe File \\ \hline
OOT  & OTIS Observation Tool \\ \hline
OTA  & Orthogonal Transfer Array \\ \hline
OTF  & Optical Transfer Function \\ \hline
OTIS & Observatory and Telescope System \\ \hline
OWS  & OTIS Weather Server \\ \hline
PHO  & Potentially Hazardous Object \\ \hline
PSDC & Pan-STARRS Document Control \\ \hline
PSF  & Point Spread Function \\ \hline
PSPS & Published Science Products System \\ \hline
PTS  & Pan-STARRS Telescope Scheduler \\ \hline
Pan-STARRS & Panoramic Survey Telescope and Rapid Response System  \\ \hline
RFI  & Radio Frequency Interference \\ \hline
SCD  & System Concept Definition \\ \hline
SDSS & Sloan Digital Sky Survey  \\ \hline
SGS  & Science Goals Statement \\ \hline
SNe  & Supernovae \\ \hline
SRS  & Software Requirements Specification \\ \hline
SSS  & Solar System Survey \\ \hline
TAC  & Time Allocation Committee \\ \hline
TBD  & To Be Determined  \\ \hline
TBR  & To Be Reviewed \\ \hline
TCS  &  Telescope Control System \\ \hline
TLA  & Three Letter Acronym \\ \hline
\end{tabular}}

\newpage
{\Large \bf Acronyms (con't)}

{\footnotesize
\begin{tabular}{|p{50pt}|p{400pt}|} \hline 
TLR  & Top Level Requirements \\ \hline
TNO  & Trans-Neptunian Object \\ \hline
TTI  & Transient Time Interval \\ \hline
UDS  & Ultra-Deep Survey  \\ \hline
UDS  & Ultra-Deep Survey  \\ \hline
UET  & Unit Exposure Time \\ \hline
WFS  & Wavefront Sensor   \\ \hline
WFSS & Wavefront Sensor Star  \\ \hline
WL   & Weak Lensing \\ \hline
- & - \\ \hline
RA   & right ascension \\ \hline
DEC  & Declination \\ \hline
GLAT & Galactic Latitude \\ \hline
GLON & Galactic Longitude \\ \hline
ELAT & Ecliptic Latitude \\ \hline
ELON & Ecliptic Longitude \\ \hline
\end{tabular}}

{\Large \bf Glossary}

{\footnotesize
\begin{tabular}{|p{50pt}|p{400pt}|} \hline 
Subaru  & National Astronomical Observatory of Japan's 8.3m telescope \\ \hline
cadence & \\ \hline
Phase 1 & IPP image processing preparation stage \\ \hline
Phase 2 & IPP image reduction stage \\ \hline
Phase 3 & IPP exposure analysis stage \\ \hline
Phase 4 & IPP image combination stage \\ \hline
Detection   & Identification of a source (real or not) in an image \\ \hline
Observation & In MOPS, a detection that corresponds to a real Solar System object \\ \hline
Designation & The identifying label assigned to newly identified Solar System objects \\ \hline
Orbit Identification & The identification of two separately determined orbits as representing the same object. \\ \hline
Attribution & The identification of a detection with a known orbit. \\ \hline
Linkage    & The identification of sets of detections that allow an orbit determination for a Solar System object \\ \hline
Autonomous & operates at night without human intervention 
             for a minimum of three nights out of seven.  
             Daytime summit calibration and maintainance carried out
             four consecutive days a week (Monday-Thursday).   \\ \hline
Robotic & operates at night without human intervention 
         for a minimum of three nights out of seven.  
         Only four days summit maintainence per week necessary,
         human intervention in calibration not required.  \\ \hline
Remote & operates without human intervention at the summit at night. \\ \hline
Transient Time Interval & Time interval between two successive images of the same footprint in order to distinguish between stationary and non-stationary transient detections. \\ \hline
Trans-Neptunian Object & An asteroid or comet that spends most of its time outside Neptune's orbit.  Include classical  \\ \hline
Sweet Spots &  \\ \hline
Potentially Hazardous Object & An asteroid or comet with MOID<0.05AU with Earth's orbit  \\ \hline
Observing Efficiency & ratio of shutter open time to total time in a night excluding weather loss \\ \hline
\end{tabular}
}
