1 gamma-ray astronomy with glast may 24, 2008 toby burnett walta meeting
Post on 21-Dec-2015
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But what is gamma-ray astronomy?
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relevant names:
masscharge particle
cosmic rayprotonmuonphoton x-ray gamma ray radio wave visible light ultraviolet infrared
wavewave lengthfrequency
flux spectrum
telescope
magnetic fieldenergy Joule (J)
electron volt (eV)
AAA batterykilowatt hourgallon of gas
The cosmic ray spectrum
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Flu
x
Energy
Questions:1.Which astronomical objects are the origin of cosmic rays?2.Above the “Knee”, can we locate the origins?
astronomy possible here?
The atmosphere matters!
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Telescopes & particle detectors
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e+ e– calorimeter (energy measurement)
particle tracking detectors
conversion foil
anticoincidenceshield
Pair-Conversion Telescope
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Optical telescope (SDSS):A fancy camera with a CCD photon detector
Schematic for a gamma-ray detector
12log10(E/1 MeV)
E*f
lux,
(m
-2 s-1
)
galactic protons
He, CNO
Galactic electrons
Albedo gamma secondary protons
secondary e±
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LAT: 20 MeV – >300 GeV
GBM: 10 keV – 25 MeV
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Large Area Telescope (LAT)
GLAST Burst Monitor (GBM)
An International Science Mission
Large Area Telescope (LAT)
GLAST Burst Monitor (GBM)
Spacecraft (General Dynamics
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• Precision Si-strip Tracker 18 XY tracking planes. Single-sided silicon strip detectors (228 m pitch) Measure the photon direction; gamma ID.
• Hodoscopic CsI Calorimeter Array of 1536 CsI(Tl) crystals in 8 layers. (8 X0) Measure the photon energy; image the shower.
• Segmented Anticoincidence Detector (ACD) 89 plastic scintillator tiles. Reject background of charged cosmic rays; segmentation removes self-veto effects at high energy.
• Electronics System Includes flexible, robust hardware trigger and software filters.
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Calorimeter
e+ e–
ACD
Tracker1.7 m
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Galactic center
3C279 (blazar)
Vela ( radio pulsar)
Crab (radio pulsar)
Geminga (radio-quiet pulsar)
PKS 0202-512 (blazar)
Isolated neutron star?
SN remnant?
Point things: near and far Diffuse things: CR
interactions in matter
Orion Cloud
LMC
EGRET all-sky survey (E>100 MeV)
Extragalactic diffuse
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