Jim Sahli Goddard Space Flight Center Greenbelt, Md. XTE Status Report #1 Jan. 17, 1996 10 a.m. NASA's X-Ray Timing Explorer (XTE) has concluded its engineering checkout and the science team is now conducting a calibration of its science instruments before commissioning the spacecraft for full-time science research at the end of this month. "We are checking out the spacecraft instruments and mapping out the particular space environment of our orbit under current conditions. The densities of energetic electrons and protons determine when our instruments can safely operate and obtain good data," said Dr. Jean Swank, XTE project scientist. "We are doing that while observing selected X-ray sources that allow us to calibrate the instrument parameters and determine that the whole system for interpreting the data is working correctly," said Swank. With the pointed instruments, the Proportional Counter Array (PCA) and High Energy X-ray Timing Experiment (HEXTE), "we first looked at a supernova remnant containing a spinning neutron star called PSR 1509-58, with a 150- millisecond period. The PCA obtained about 120 good X-ray counts and clearly detected the neutron star's periodic flashes. Results from this "first light" X-ray observation, an observation of the Crab nebula and pulsar and a short look at a quasiperiodic oscillator, can be found on the internet at the URL http://heasarc.gsfc.nasa.gov/docs/xte/SOF/First_Results.html. “The first of many expected observations of the binary X-ray source Cygnus X-2 (the second X-ray source found in the constellation Cygnus) found oscillations of a few percent at a frequency of 20 Hz (a period of 50 milliseconds). The excellent signal to noise ratio promises us exciting sensitivity to oscillation changes. These give rise to the smearing of the frequency in the not-quite periodic oscillations and will change the frequency greatly in additional observations,” said Swank. After initial observations, the spacecraft’s All Sky Monitor (ASM) experienced problems with internal high-voltage breakdown in 2 of 3 detectors. The instrument has been turned off while the data is analyzed to determine possible recoveries. "In the next couple of weeks, we will do some observations of special targets being observed at the same time with other satellites, while we continue to work on our calibrations. We hope the system will then be ready for the proposed science program. We hope the ASM can be on-line then too," said Swank. "We concluded our engineering checkout Friday (Jan. 5). We have checked all of the spacecraft subsystems and have determined that they are operating as required. The bottom line is that NASA's new X-ray satellite is on orbit and working," said Dale Schulz, XTE project manager. "During that first week on orbit the XTE operations team also turned on the three instruments. At this point we are fine tuning and calibrating the spacecraft," said Schulz. The XTE mission is being managed by the Goddard Space Flight Center in Greenbelt, Md. The satellite was launched Dec. 30 at 8:48 a.m. EST from the Cape Canaveral Air Station in Florida. The satellite was placed into a circular 360 statute mile (580 kilometer) orbit with an inclination of 23 degrees by a Delta II launch vehicle. Among the objects to be studied by NASA'S XTE mission are stellar black holes, neutron stars and quasars. Stellar blackholes and neutron stars represent the end stages of the lives of stars several times heavier than the Sun. Quasars are thought to be super-massive black holes about the size of the solar system, containing the mass of billions of stars. Spacecraft officials have indicated that they are monitoring a loss of solar array power which is stable at this time. Engineers say that science objectives can be met with the existing power generation capability. The XTE Science Operations Facility home page can be found at http:// heasarc.gsfc.nasa.gov/docs/xte/SOF/XTESOF.html. It has links to other information about the schedule and progress of the spacecraft checkout. Subsequent XTE status reports will be issued as further information becomes available. -30-