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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 Workbook, but as far as we can tell it hasn't been updated in a while.

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

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#FGLA 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
1FGL catalog
(with paper link)
2FGL catalog
(with paper link)
3FGL paper

#FHL  
#LAC  
   
   

 

A

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ACD(Anti-Coincidence Detector) 
AGN(Active Galactic Nuclei) 
ARR(Autonomous Repoint Request) 
ATel(Astronomer's Telegram) 
ATS  
   
   
   
   
   
   

B

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BA(burst advocate) 
back  
back-converting  
BGO(bismuth germanate detector) 
blazar  
BL Lac  
boresight  
   

C

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C&ACalibration and Analysis (group);  
CAL(Calorimeter) 
Calorimeter(CAL) 
cat. / Cat.(category) 
catalog LAT catalogs
Catalog (group)  
category  
clean (event class)  
CR(cosmic ray) 
CTB  
   
   
   

D

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dec(declination) 
diffuse  
DMDark Matter (group);  
DQM(Data Quality Monitor) 
ds9  
dSph(dwarf spheroidal galaxy) 

E

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Earth limb / Earth's limb  
EBL(Extragalactic Background Light) 
EPO(Education and Public Outreach) 
event  
event class  
Evosee also "SeeVogh" 
exposure  
   

F

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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

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GALPROP  
GBM(Gamma-ray Burst Monitor) 
GCN(Gamma-ray Coordinates Network) 
GEANT  
GLAST  
GlastRelease  
GLEAM  
GRB(gamma-ray burst) 
gt_____  
   
   

H

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HEASARC  
   
   
   
   
   

I

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IRF(Instrument Response Function) 
ISOC  
   
   
   
   
   
   
   
   
   
   

J

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JIRA  
   
   
   
   

K

L

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L1Proc  
LAT(Large Area Telescope) 
LAT Low Energy  
light curve  
likelihood  
livetime  
LLE(LAT Low Energy) 
LMC(Large Magellanic Cloud) 
LPA  

M

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MC(Monte Carlo) 
merit / merit file  
MIP(minimum ionizing particle) 
MOC  
MSP(millisecond pulsar) 
MW(multiwavelength) 

N

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nadir  
nadir observations  
NaI(sodium iodide) 
   

O

P

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Pass #, version #  
phi  
pipeline  
pointed observations  
pole pointing  
PSF(point-spread function) 
PSR(pulsar) 
PWN(pulsar wind nebula) 
   

Q

R

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RA(right ascension) 
ROI(region of interest) 
ROOT, .root file  

S

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SAA(South Atlantic Anomaly) 
Science Tools  
SeeVogh  
senior review  
SMC(Small Magellanic Cloud) 
SNR(supernova remnant) 
source (event class)  
star trackers  

T

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TDRSS(Tracking and Data Relay Satellite System) 
TGFs(terrestrial gamma-ray flashes) 
theta  
ToO(Target of Opportunity) 
transient  
transient (event class)  
TRK(Tracker) 
Trunc64  
TS(test statistic) 

U

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ultraclean (event class)  
   
   

V

W

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white paper  
   
   

X

Y

Z

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zenith  
zenith angle cut  
   
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