The Third Interplanetary Network

Details The Third Interplanetary Network The Third Interplanetary Network

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aipc.1358..385h&link_type=abstract

GAMMA RAY BURSTS 2010. AIP Conference Proceedings, Volume 1358, pp. 385-388 (2011).

Other

Gamma-Ray Sources (Astronomical), Spacecraft, Gravitational Lenses, Gravitational Waves, Gamma-Ray Sources, Gamma-Ray Bursts, Spacecraft/Atmosphere Interactions, Relativity And Gravitation, Gravitational Radiation, Magnetic Fields, And Other Observations

Scientific paper

The 3rd interplanetary network (IPN), which has been in operation since 1990, presently consists of 9 spacecraft: AGILE, Fermi, RHESSI, Suzaku, and Swift, in low Earth orbit; INTEGRAL, in eccentric Earth orbit with apogee 0.5 light-seconds Wind, up to ~7 light-seconds from Earth; MESSENGER, en route to Mercury; and Mars Odyssey, in orbit around Mars. The IPN operates as a full-time, all-sky monitor for transients down to a threshold of about 6×10-7 erg cm-2 or 1 photon cm-2 s-1. It detects ~335 cosmic gamma-ray bursts per year. These events are generally not the same ones detected by narrower field of view instruments such as Swift, INTEGRAL IBIS, SuperAGILE, and MAXI; the localization accuracy is in the several arcminute and above range. The data are publicly available and can be utilized for a wide variety of studies.

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