Purpose
This page aims to pull together definitions for the jargon and technical terms that get used by the Fermi collaboration. A glossary exists in the SLAC Workbook, but as far as we can tell it hasn't been updated in a while. A short glossary also exists in the FSSC Cicerone.
The purpose of this glossary in particular is to provide new Fermi members (especially junior members) with a resource to tackle all the jargon that gets tossed around. Therefore, please avoid using more jargon to explain jargon. The definitions should stand alone as much as possible, and can link to papers / Confluence pages / etc. for more detailed information. The explanations should only provide what is necessary for a basic understanding; details can go in the links.
This glossary focuses on terms that are difficult to just google ("GlastRelease", "theta"). It also includes googleable terms that have specific applications to Fermi (e.g., AGN observations in gamma rays rather than AGN in general).
0-9
| term | definition | links |
|---|---|---|
| #FGL | A catalog of LAT point sources, which are objects in the sky that are bright in gamma rays over a long period of time. These are often active galaxies, supernova remnants, pulsars, and pulsar wind nebulae. So far, the LAT team has published the 1FGL (which used 11 months of LAT data) and 2FGL (2 years of LAT data). There is also a 0FGL (3 months of LAT data), also known as the Bright LAT source list. The Catalog group is currently working on 3FGL. (see also Catalog) | 0FGL page |
| #FHL | ||
| #LAC | ||
A
| term | definition | links |
|---|---|---|
| ACD | (Anti-Coincidence Detector) The ACD is the collection of scintillating tiles that detect charged particles, and is crucial to background rejection. The ACD covers the tracker (the part of the LAT that converts gamma rays into electron-positron pairs and then tracks these pairs' trajectories). Charged particles will also register as signals in the tracker, so the ACD is used to determine if a signal is actually a charged particle and not a gamma ray. If an ACD tile has a "hit" (detects a charged particle) that lines up with a signal, then that fact is used to "veto" the signal (i.e., declare that it's not a gamma ray). | |
| AGN (group) | (Active Galactic Nuclei) | AGN group page |
| ARR | (Autonomous Repoint Request) | |
| ATel | (Astronomer's Telegram) | |
| ATS | ||
B
| term | definition | links |
|---|---|---|
| BA | (burst advocate) | |
| back | ||
| back-converting | ||
| BGO | (bismuth germanate detector) | |
| blazar | ||
| BL Lac | ||
| boresight | ||
C
| term | definition | links |
|---|---|---|
| C&A (group) | (Calibration and Analysis) | C&A group page |
| CAL | (Calorimeter) | |
| Calorimeter | (CAL) | |
| cat. / Cat. | (category) | |
| catalog | LAT catalogs | |
| Catalog (group) | Catalog group page | |
| category | ||
| clean (event class) | ||
| CR | (cosmic ray) | |
| CTB | ||
D
| term | definition | link |
|---|---|---|
| dec | (declination) | |
| diffuse (group) | Diffuse group page | |
| diffuse (event class) | ||
| DM (group) | (Dark Matter) | DM group link |
| DQM | (Data Quality Monitor) | |
| ds9 | (Deep Space 9 (seriously)) ds9 is a piece of software that is used for data visualization and imaging. For instance, someone analyzing Fermi data might use ds9 to look at a counts map (a map of where the photons that Fermi observed came from). | http://ds9.si.edu/site/Home.html |
| dSph | (dwarf spheroidal galaxy) |
E
| term | definition | link |
|---|---|---|
| Earth limb / Earth's limb | ||
| EBL | (Extragalactic Background Light) | |
| effective area | ||
| EPO | (Education and Public Outreach) | |
| event | ||
| event class | ||
| Evo | see also "SeeVogh" | |
| exposure | ||
F
| term | definition | link |
|---|---|---|
| FA | (flare advocate) | |
| fits / .fits (file type) | ||
| FltOps | (Flight Operations) | |
| FOT | (Flight Operations Team) | |
| FOV / FoV | (field of view) | |
| front | ||
| front-converting | ||
| FSW | (Flight Software) | |
| FT1 (file) | ||
| FT2 (file) | ||
| FTOOLS | ||
| fv |
G
| term | definition | link |
|---|---|---|
| GALPROP | ||
| GBM | (Gamma-ray Burst Monitor) The GBM is the second | |
| GCN | (Gamma-ray Coordinates Network) | |
| GEANT | ||
| GLAST | (Gamma-ray Large Area Space Telescope) GLAST is the name that Fermi was referred to before it was launched. It is tradition to give NASA missions a different name after launch, as a good-luck superstition. | |
| GlastRelease | ||
| GLEAM | ||
| GRB (group) | (Gamma-Ray Burst) | GRB group page |
| gt_____ | The standard set of software used to analyze LAT data are called the Science Tools. Each individual tool has a specific function. The names all start with "gt", for "GLAST", which was the original pre-launch name of Fermi. | Science Tools references |
H
| term | definition | link |
|---|---|---|
| HEASARC | ||
I
| term | definition | link |
|---|---|---|
| IRF | (Instrument Response Function) | |
| ISOC | ||
J
| term | definition | link |
|---|---|---|
| JIRA | ||
K
L
| term | definition | link |
|---|---|---|
| L1Proc | Level 1 Processing | |
| LAT | (Large Area Telescope) | |
| LAT Low Energy | ||
| light curve | ||
| likelihood | ||
| livetime | ||
| LLE | (LAT Low Energy) | |
| LMC | (Large Magellanic Cloud) | |
| LPA |
M
| term | definition | link |
|---|---|---|
| MC | (Monte Carlo) | |
| merit / merit file | ||
| MET | (Mission Elapsed Time) | |
| MIP | (minimum ionizing particle) | |
| MOC | ||
| MSP | (millisecond pulsar) | |
| MW | (multiwavelength) |
N
| term | definition | link |
|---|---|---|
| nadir | ||
| nadir observations | ||
| NaI | (sodium iodide) | |
O
P
| term | definition | link |
|---|---|---|
| Pass #, version # | ||
| phi | ||
| pipeline | ||
| pointed observations | ||
| pole pointing | ||
| PSF | (point-spread function) | |
| PSR | (pulsar) | Pulsar group page |
| PWN | (pulsar wind nebula) | |
Q
R
| term | definition | link |
|---|---|---|
| RA | (right ascension) | |
| ROI | (region of interest) The ROI is the region of space that is being analyzed. A typical ROI for an individual source (such as a pulsar or a gamma-ray burst) is 10 or 12 degrees, although the exact size can differ and depends on the many factors. | |
| ROOT, .root file |
S
| term | definition | link |
|---|---|---|
| SAA | (South Atlantic Anomaly) | |
| Science Tools | ||
| SeeVogh | ||
| senior review | ||
| SMC | (Small Magellanic Cloud) | |
| SNR | (supernova remnant) | SNR group page |
| source (event class) | ||
| star trackers |
T
| term | definition | link |
|---|---|---|
| TDRSS | (Tracking and Data Relay Satellite System) | |
| TGFs | (terrestrial gamma-ray flashes) | |
| theta | ||
| ToO | (Target of Opportunity) | |
| transient | ||
| transient (event class) | ||
| TRK | (Tracker) The Tracker is a part of the LAT whose purpose is twofold: 1) To convert gamma rays into electron-positron pairs, and 2) To track these pairs of charged particles through the instrument in order to figure out where the original gamma ray came from. The Tracker is made of alternating layers of tungsten foils (to convert the gamma rays) and silicon strip detectors (to track the pairs), arranged in 64 columns (8 by 8). | |
| Trunc64 | ||
| TS | (test statistic) |
U
| term | definition | link |
|---|---|---|
| ultraclean (event class) | ||
V
W
| term | definition | link |
|---|---|---|
| walkthrough | ||
| WAM | (Weekly Analysis Meeting) An online collaboration-wide meeting held every Friday at 8 am PST / 11 am EST / 5 pm CST. The WAMs are held over SeeVogh, which can be downloaded at this website. Topics discussed during WAMs include collaboration-wide items of interest (such as newly released Fermi data), detections of GRBs (gamma-ray bursts) and flaring AGN (active galactic nuclei), and walkthroughs (short summaries) of upcoming papers within the LAT collaboration. | WAM agenda page |
| white paper | ||
X
Y
Z
| term | definition | link |
|---|---|---|
| zenith | The point on the sky that is opposite to the Earth for the Fermi spacecraft. |  (diagram from Wikipedia) (imagine the person is Fermi) |
| zenith angle cut | ||