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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 | Catalog Last Checked: August 04, 2025 at 09:13 AM -
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 | Catalog Last Checked: October 06, 2025 at 04:18 AM -
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: 2 | Catalog Last Checked: May 06, 2026 at 07:45 PM -
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 | Catalog Last Checked: April 20, 2026 at 04:12 PM -
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 | Catalog Last Checked: May 06, 2026 at 07:44 PM -
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 | Catalog Last Checked: August 04, 2025 at 10:51 AM -
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: 1 | Catalog Last Checked: May 26, 2026 at 07:15 PM -
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 | Catalog Last Checked: August 04, 2025 at 09:04 AM -
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 | Catalog Last Checked: August 04, 2025 at 08:37 AM -
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 | Catalog Last Checked: October 20, 2025 at 04:21 AM -
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 | Catalog Last Checked: April 20, 2026 at 04:12 PM -
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 | Catalog Last Checked: August 04, 2025 at 09:12 AM -
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 | Catalog Last Checked: August 04, 2025 at 09:14 AM
