A.B.Giles
NASA / GSFC USRA
The Rossi X-ray Timing Explorer (RXTE) spacecraft was launched on 30th December 
1995 and contains a large Proportional Counter Array (PCA) experiment developed 
at GSFC. Telemetry from RXTE is returned via the NASA Tracking and Data Relay 
Satellite System (TDRSS) which, apart from specific gaps in coverage, provides 
a steady stream of nearly continuous real time data packets. The PCA has an 
area of 7000  and produces high count rates for many x-ray sources.  
This provides the opportunity for some serious interpretation and decision 
making in real time. The display programs developed by the PCA team fall into 4 
classes: Housekeeping, General performance (Instrumental and calibration bias), 
Spectral (Science bias) and Temporal (Science bias). These displays are used 
by the duty scientist and experiment controllers to monitor the observation 
in progress to try and ensure that the observation is proceeding as planned 
and that modifications to the observing modes are not required. Guest Observers 
(GO's) can be present in the Science Operations Facility (SOF) for their 
observations. The PCA team can also monitor their experiment using these 
programs. The SOF are making some of these tools available to GO's for 
remote display at their home institutions for the specific duration of 
their observations. It is also planned to provide semi real time displays of 
public data via WWW. This paper briefly describes the available display 
options.
 and produces high count rates for many x-ray sources.  
This provides the opportunity for some serious interpretation and decision 
making in real time. The display programs developed by the PCA team fall into 4 
classes: Housekeeping, General performance (Instrumental and calibration bias), 
Spectral (Science bias) and Temporal (Science bias). These displays are used 
by the duty scientist and experiment controllers to monitor the observation 
in progress to try and ensure that the observation is proceeding as planned 
and that modifications to the observing modes are not required. Guest Observers 
(GO's) can be present in the Science Operations Facility (SOF) for their 
observations. The PCA team can also monitor their experiment using these 
programs. The SOF are making some of these tools available to GO's for 
remote display at their home institutions for the specific duration of 
their observations. It is also planned to provide semi real time displays of 
public data via WWW. This paper briefly describes the available display 
options.