Compton Observatory Science Report #141 Thursday, October 28, 1993 Eric Chipman, Compton Observatory Science Support Center Questions or comments can be sent to the Compton SSC. Phone 301/286-7764, e-mail SPAN GROSSC::CHIPMAN, Internet chipman@grossc.gsfc.nasa.gov. Normal operations continue. There was a maneuver on Monday, October 25, to the attitude of Viewing Period 305. The times for this maneuver were 1431Z to 1439Z. The maneuver angle was 5.81 degrees, and the HGA boom angle from the equator is now 17.6 degrees. ARCHIVES -------- Archive contents- BATSE - Bursts and flares to trigger 1463, Four months of daily HER and SHER data (some problems with this data are being looked at) Additional HER and SHER data up to April 1992 has been received at the SSC and is being installed in the archive. Some high-level pulsar light curves have been received at the SSC COMPTEL - Periods 1,4,6,7,8,12 and 13 are in the archive. The remainder of periods 1-13 have been received at the SSC and are being processed. EGRET - Periods 0.2-32 are available (Maps and photon lists) OSSE - Periods 1.0 - 15 and 17 are now in the archive (SDB data). Period 16 has been received at the SSC and is being processed. Some pulsar data is also available off-line. BATSE ----- Dr. Oleg Terekhov of IKI has been visiting in Huntsville this week. He is discussing with the BATSE team the possiblities for joint Phebus/Granat-BATSE gamma-ray burst studies. The x-ray transient GRO J1719-24 shown only a slight decrease in flux since its peak near October 1st. The current 20-100 keV flux is approximately 1.2 Crab. A fit to the flux history gives a lower limit to the decay time of 130 days. During viewing period 305 the BATSE pulsar hardware is being used to collect 31 ms single sweep data in an effort to detect weak bursts from the soft gamma repeater SGR 1806-20. Searches are also being conducted in the lowest energy channel of the DISCLA data. Normal BATSE folded-on-board pulsar data is only being collected for the Crab Pulsar. COMPTEL ------- The COMPTEL instrument continues routine observations. At the Gamma-Ray Burst Workshop last week in Hunstville the following results were presented by the collaboration: a report on the new detection of a number of low-intensity, hard-spectra gamma-ray bursts, previously unanalysed due to their low flux in hard x-rays, in the COMPTEL database (Ryan et al.); a summary report on observations of gamma-ray bursts by COMPTEL during the first year of the GRO mission, including GRB 910814, which shows evidence for a spectral break at MeV energies (Hanlon et al.), and a status report on the BATSE/COMPTEL/NMSU rapid burst response campaign (Kippen et al.) (Note: with the recent acquisition of new hardware for the rapid processing of burst data, the goal of the team is to determine an accurate location for favorable bursts occurring within the field of view of COMPTEL, within two hours of the receipt of the burst trigger message from BATSE). In addition, a comparison of data obtained by the GRO instruments, including COMPTEL, for the burst of 1 June 1991 was presented by Share et al. EGRET ----- EGRET operations were normal this week. This was the first full week of the deep survey. Because of the nature of the study the analysis will be long, but it is hoped that the rewards will be high. A large group of abstracts on the all-sky survey have been submitted for papers to be presented as posters at the January, 1994 AAS meeting. Several other abstracts on EGRET work have been submitted. OSSE ---- OSSE operations are normal. In viewing period 305, the Z-axis target is the Virgo sky survey region (Key project) centered at (l,b) = (278,+63), and the X-axis target is the galactic center region, including GRS 1716-249 (PI team). Members of the OSSE team from NRL, Northwestern University, and Clemson University were together this week here at NRL to review the instrument status and progress on recent data analysis, and to begin the organization for Phase 4 proposal writing. Data from viewing period 16 was delivered to the Compton GRO Science Support Center Archive today. The targets during that time were the Galactic Center region, NGC 7582, and NGC 253.