The Fermi Science Support Center (FSSC) runs the guest investigator program, creates and maintains the mission time line, provides analysis tools for the scientific community, and archives and serves the Fermi data. This web site is the portal to Fermi for all guest investigators.
Look into the "Resources" section for finding schedules, publications, useful links etc. The "Proposals" section is where you will be able to find the relevant information and tools to prepare and submit proposals for guest investigator projects. At "Data" you will be able to access the Fermi databases and find the software to analyse them. Address all questions and requests to the helpdesk in "Help".
The Fermi Science Support Center and the GBM Team are pleased to announce the availability of the second GBM catalog of Gamma-Ray Bursts (GRBs) in the HEASARC browse interface. The catalog will soon appear in the Astrophysical Journal (Supplement Series). This catalog is in two parts: a general description (A. von Kienlin et al., http://arxiv.org/abs/1401.5080) and a spectral analysis (D. Gruber et al., http://arxiv.org/abs/1401.5069). The general catalog includes 953 GRBs that triggered GBM between 2008-07-12 and 2012-07-11. The spectral catalog reports spectral analyses of 943 GRBs, including revised analyses of the GRBs in the first catalog, from 2008-07-12 to 2010-07-11. Data from these catalogs are now available at the HEASARC in searchable tables via the Browse interface.
Black widow spiders and their Australian cousins, known as redbacks, are notorious for their tainted love, expressed as an unsettling tendency to kill and devour their male partners. Astronomers have noted similar behavior among two rare breeds of binary system that contain rapidly spinning neutron stars, also known as pulsars.
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An exceptionally close stellar explosion discovered on Jan. 21 has become the focus of observatories around and above the globe, including several NASA spacecraft. The blast, designated SN 2014J, occurred in the galaxy M82 and lies only about 12 million light-years away. This makes it the nearest optical supernova in two decades and potentially the closest type Ia supernova to occur during the life of currently operating space missions.
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