Adding INTEGRAL to the third interplanetary network

Details Adding INTEGRAL to the third interplanetary network Adding INTEGRAL to the third interplanetary network

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003head....7.0503h&link_type=abstract

American Astronomical Society, HEAD meeting #7, #05.03; Bulletin of the American Astronomical Society, Vol. 35, p.863

Other

Scientific paper

The BGO anticoincidence system of the INTEGRAL spectrometer (SPI-ACS) presents a cross-sectional area of up to 5200 square centimeters for gamma-rays of energy 80 keV and above. It has been equipped with a trigger to take high time resolution (50 ms) data when a gamma-ray burst occurs. We have been utilizing these data as part of the third interplanetary network of GRB detectors, which also includes the Ulysses, Mars Odyssey, RHESSI, and Wind spacecraft. We have detected and localized numerous bursts, including some which also localized by IBIS, and others which have IPN-only localizations. We will review some of the data obtained to date and discuss the unique properties which INTEGRAL brings to the IPN.

Affiliated with

Also associated with

No associations

Rating

Adding INTEGRAL to the third interplanetary network does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Adding INTEGRAL to the third interplanetary network, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Adding INTEGRAL to the third interplanetary network will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1524643