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Fermi User’s Group Fermi User’s Group – 1 6 February 2009 6 February 2009 GAMMA-RAY BURST MONITOR Status, Results, Plans Bill Paciesas

GAMMA-RAY BURST MONITOR

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GAMMA-RAY BURST MONITOR. Status, Results, Plans Bill Paciesas. GBM Triggers. 315 triggers in 208 days 144 GRBs 126 SGR (90 from AXP 1E1547.0−5408) 9 terrestrial Gamma Flashes 13 particle events 23 others, including 1 solar flare. GRB Localization Accuracy. Preliminary. GRB 081215A. - PowerPoint PPT Presentation

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Page 1: GAMMA-RAY BURST MONITOR

Fermi User’s GroupFermi User’s Group – – 11 – – 6 February 2009 6 February 2009

GAMMA-RAY BURST MONITOR

Status, Results, Plans

Bill Paciesas

Page 2: GAMMA-RAY BURST MONITOR

Fermi User’s GroupFermi User’s Group – – 22 – – 6 February 2009 6 February 2009

GBM Triggers

315 triggers in 208 days 144 GRBs 126 SGR (90 from AXP 1E1547.0−5408) 9 terrestrial Gamma Flashes 13 particle events 23 others, including 1 solar flare

Page 3: GAMMA-RAY BURST MONITOR

Fermi User’s GroupFermi User’s Group – – 33 – – 6 February 2009 6 February 2009

GRB Localization Accuracy

Type Number of GRBs with accurate

independent locations

Reported Average

Error (degrees)

Actual Average

Error (degrees)

Inferred Systematic

Error (degrees)

FSW 18 bursts with good on-board error estimates

12.0 9.6 Included in FSW error estimate

Automaticon-ground

22 6.9 7.6 3.5

Human-in-loop I 24 4.78 4.35 --

Human-in-loop II

30 3.67 3.98 2.06

Page 4: GAMMA-RAY BURST MONITOR

Fermi User’s GroupFermi User’s Group – – 44 – – 6 February 2009 6 February 2009

GRB 081215A Intense hard event at ~90° to LAT axis Would have been a good repoint

candidate but GBM did not recommend repoint

FSW location was below horizon On-board algorithm makes assumptions

about spectral hardness & atmospheric scattering that were not optimal for this GRB

What is the LAT response to cal-only or tkr-only events?

LAT Cal-only & Tkr-only

GBM > 1 MeV

GBM < 1 MeV

Page 5: GAMMA-RAY BURST MONITOR

Fermi User’s GroupFermi User’s Group – – 55 – – 6 February 2009 6 February 2009

Pulsed Source MonitoringGX 1+4

Page 6: GAMMA-RAY BURST MONITOR

Fermi User’s GroupFermi User’s Group – – 66 – – 6 February 2009 6 February 2009

Near-Term Plans

FSW revision Improve classification of triggers

Simplify inclusion of known active sources (esp. SGRs) Add special algorithms for TGFs

Add more ARR decision info to TRIGDAT Misc operational improvements

Improve & quantify of location accuracy Improve calibration & detector response