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1 Gamma-Ray Astronomy with GLAST May 24, 2008 Toby Burnett WALTA meeting.

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Presentation on theme: "1 Gamma-Ray Astronomy with GLAST May 24, 2008 Toby Burnett WALTA meeting."— Presentation transcript:

1 1 Gamma-Ray Astronomy with GLAST May 24, 2008 Toby Burnett WALTA meeting

2 2 GLAST meets its spacecraft, last December GLAST meets its launch vehicle (last week)

3 3 Launch: from Cape Canaveral – June 3, 2008 We are #332 WALTA meeting

4 4

5 GLAST already on MySpace! 5WALTA meeting

6 But what is gamma-ray astronomy? WALTA meeting6 relevant names: mass charge particle cosmic ray proton muon photon x-ray gamma ray radio wave visible light ultraviolet infrared wave wave length frequency fluxspectrum telescope magnetic field energyJoule (J) electron volt (eV) AAA battery kilowatt hour gallon of gas

7 The cosmic ray spectrum WALTA meeting7 Flux  Energy  Questions: 1.Which astronomical objects are the origin of cosmic rays? 2.Above the “Knee”, can we locate the origins? astronomy possible here?

8 Astronomy with photons WALTA meeting8 Green: E =2.5 eV =500 nm  wave-likeparticle-like 

9 The atmosphere matters! WALTA meeting9

10 Telescopes & particle detectors WALTA meeting10  e+e+ e–e– calorimeter (energy measurement) particle tracking detectors conversion foil anticoincidence shield Pair-Conversion Telescope WALTA meeting Optical telescope (SDSS): A fancy camera with a CCD photon detector Schematic for a gamma- ray detector

11 11 GAP! GLAST ( Mike Turner 1989 ) WALTA meeting

12 12 log 10 (E/1 MeV) E*flux, (m -2 s -1 ) galactic protons He, CNO Galactic electrons Albedo gamma secondary protons secondary e ± WALTA meeting

13 LAT: 20 MeV – >300 GeV GBM: 10 keV – 25 MeV 13 Large Area Telescope (LAT) GLAST Burst Monitor (GBM) An International Science Mission Large Area Telescope (LAT) GLAST Burst Monitor (GBM) Spacecraft (General Dynamics WALTA meeting

14 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 X 0 ) 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. WALTA meeting14 Calorimeter e+e+ e–e–  ACD Tracker 1.7 m

15 15 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 WALTA meeting

16 16WALTA meeting

17 GLAST’s view of the sky 17WALTA meeting

18 GLAST sources found (simulation) WALTA meeting18


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