[ ASM Light Curves | One-Day Averages | Analysis & Instrument Status | Source Activity | Source List | Main Page ]
The mission carries two pointed instruments, the Proportional Counter Array (PCA) developed by GSFC to cover the lower part of the energy range, and the High Energy X-ray Timing Experiment (HEXTE) developed by UCSD covering the the upper energy range. These instruments are equipped with collimators yielding a FWHM of one degree.
MIT is providing an All-Sky Monitor (ASM) that will scan about 80% of the sky every orbit, allowing monitoring at time scales of 90 minutes or longer, and an on board Experiment Data System (EDS) which processes the data from PCA and ASM. (see below for technical information and the current status of these instruments) The ASM will observe the brightest known X-ray sources for variability and also alert the community when new sources appear.
The Science Operations Center at the NASA's Goddard Space Flight Center will manage the mission science operations. More information about the spacecraft and the instruments can be had from NASA HEASARC. The Guest Obeserver Facility contains useful information about doing science with XTE.
Back to the CSR Home Page
This page is maintained by firstname.lastname@example.org