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All-sky monitoring with the fermi gamma ray burst monitor
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Wilson-Hodge, Colleen A. |
| Copyright Year | 2010 |
| Description | We are currently monitoring the transient hard X-ray/soft gamma ray sky using the Gamma Ray Burst Monitor (GBM) on-board Fermi. The twelve GBM NaI detectors span 8 keV to 1MeV, while the two GBM BGO detectors span about 150 keV to 40 MeV. With GBM, we detect transient events on multiple timescales. Brief events, such as Gamma Ray Bursts, Solar flares, and magnetar bursts are detected with on-board triggers. On longer timescales, we use the Earth occultation technique to monitor a number of sources, including X-ray binaries, AGN, and solar flaring activity. To date we have detected 7 sources above 100 keV. Transient activity from accretion-powered pulsars is monitored using epoch-folding techniques. With GBM we track the pulsed flux and frequency for a number of pulsars. We will present highlights of GBM observations on various timescales. |
| File Size | 1507494 |
| Page Count | 13 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_20100035086 |
| Archival Resource Key | ark:/13960/t0gv0km77 |
| Language | English |
| Publisher Date | 2010-07-18 |
| Access Restriction | Open |
| Subject Keyword | Astronomy Solar Flares X Ray Binaries Pulsars Magnetars Detection Gamma Ray Bursts Fermi Gamma-ray Space Telescope Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Presentation |