Found 27 datasets matching filters.
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Autonomous flare finder identifies all flares ≥ GOES C-Class detected by GBM above 10 keV. (FITS file)
Search relevance: 1.00 | Views last month: 18 | Published on: 2025-08-04 -
This table lists all of the triggers observed by a subset of the 14 GBM detectors (12 NaI and 2 BGO) which have been classified as gamma-ray bursts (GRBs). Note that there are two Browse catalogs...
Search relevance: 1.00 | Views last month: 7 | Published on: 2025-11-01 -
Fermi is a powerful space observatory that will open a wide window on the universe. Gamma rays are the highest-energy form of light, and the gamma-ray sky is spectacularly different from the one...
Search relevance: 1.00 | Views last month: 5 | Published on: 2025-08-04 -
Fermi is a powerful space observatory that will open a wide window on the universe. Gamma rays are the highest-energy form of light, and the gamma-ray sky is spectacularly different from the one...
Search relevance: 1.00 | Views last month: 2 | Published on: 2026-03-07 -
Fermi is a powerful space observatory that will open a wide window on the universe. Gamma rays are the highest-energy form of light, and the gamma-ray sky is spectacularly different from the one...
Search relevance: 1.00 | Views last month: 2 | Published on: 2025-09-06 -
Time-dependent detector response matrices for each GBM detector covering the duration of every GBM flare. Needed in the spectral analysis software to relate observed count-rate spectra to model...
Search relevance: 1.00 | Views last month: 2 | Published on: 2025-10-06 -
The Fermi Gamma-Ray Burst Monitor (GBM) is not a pointed or imaging instrument. To determine fluxes for known sources, we measure the change in the count rate observed in the NaI (or BGO)...
Search relevance: 1.00 | Views last month: 2 | Published on: 2025-08-04 -
The Fermi Gamma-ray Space Telescope was launched in June 2008 to explore high-energy phenomena in the Universe. This GI program is targeted specifically at Fermi observations of high-energy solar...
Search relevance: 1.00 | Views last month: 2 | Published on: 2026-04-13 -
For GBM, input is daily or trigger CSPEC or CTIME file from Fermi archive and corresponding response file from our archive. For LAT, input is daily spectrum file and corresponding response file,...
Search relevance: 1.00 | Views last month: 1 | Published on: 2025-08-04 -
This table lists all of the triggers observed by one or more of the 14 GBM detectors (12 NaI and 2 BGO). Note that there are two Browse catalogs resulting from GBM triggers. All GBM triggers are...
Search relevance: 1.00 | Views last month: 1 | Published on: 2025-08-04 -
This List is based on GCN Circulars issued by the GBM collaboration.
Search relevance: 1.00 | Views last month: 1 | Published on: 2025-08-03 -
Time histories of NaI, GBO, and GOES data, with flare and day/night markers. Orbital plots are on RHESSI orbit times.
Search relevance: 1.00 | Views last month: 1 | Published on: 2025-08-04 -
Fermi is a powerful space observatory that will open a wide window on the universe. Gamma rays are the highest-energy form of light, and the gamma-ray sky is spectacularly different from the one...
Search relevance: 1.00 | Views last month: 0 | Published on: 2025-08-04 -
Fermi is a powerful space observatory that will open a wide window on the universe. Gamma rays are the highest-energy form of light, and the gamma-ray sky is spectacularly different from the one...
Search relevance: 1.00 | Views last month: 0 | Published on: 2025-08-04 -
LAT solar gamma-ray flux > 100 MeV, one point per solar exposure (i.e. average of the 20-40 minutes of solar observation every ~1.5 hours) calculated by two different methods.
Search relevance: 1.00 | Views last month: 0 | Published on: 2025-08-04 -
For each source we plot the history of pulse frequency and pulsed flux measured using the Fermi Gamma-Ray Burst Monitor (GBM) NaI detectors. For these measurements we use the CTIME data which...
Search relevance: 1.00 | Views last month: 0 | Published on: 2025-08-04 -
Time periods when the >100 MeV fluxes computed via the light-bucket method deviate significantly from the mean level during a 4-day period.
Search relevance: 1.00 | Views last month: 0 | Published on: 2025-08-04 -
Fermi is a powerful space observatory that will open a wide window on the universe. Gamma rays are the highest-energy form of light, and the gamma-ray sky is spectacularly different from the one...
Search relevance: 1.00 | Views last month: 0 | Published on: 2026-04-04 -
The Fermi GBM Daily Data database table contains entries for each day for which GBM data has been processed.
Search relevance: 1.00 | Views last month: 0 | Published on: 2025-08-04
