Found 13 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 -
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 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: 2026-04-20 -
Since it is not possible to predict when a Gamma-Ray Burst (GRB) occurs, the follow-up ground telescopes must be distributed as uniform as possible all over the world in order to collect...
Search relevance: 1.00 | Views last month: 1 | Published on: 2026-04-20 -
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 -
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 -
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 -
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 -
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: 0 | Published on: 2025-10-20 -
LAT data between 100 MeV and 10 GeV filtered for solar counts in 1-minute time bins, no energy binning, using light-bucket method. Contains exposure (cm^2 s) information.
Search relevance: 1.00 | Views last month: 0 | Published on: 2026-04-20 -
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 -
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: 2026-04-20 -
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: 0 | Published on: 2025-08-04
