ROSAT Guest Observer Facility

ROSAT Status Report #97:

July 5, 1994


Note: This status report comes from the The Max-Planck Institut für Extraterrestriche Physik (MPE).

Contents


SATELLITE STATUS

No major problems were encountered during the last month.

MISSION PLANNING

Mid June the ROSAT IUC (International User Committee) made the final selection on the AO-5 proposals. The list of accepted proposals can be found in the ROSAT Service Area in directory 'timeline' (file ao5.accepted).

(In the USA the accepted AO-5 targets list is now available on legacy under /rosat/timelines/ao5.targets).

Official end of the PSPC observing program and future PSPC observations

As part of the current timeline, which foresees a PSPC observing period once per month, the PSPC will be moved into focus for a last seven-day period lasting from June 30 to July 6, 1994. After this period, the regular ROSAT PSPC guest observer program will be officially ended. During 4 years of operation the two PSPCs onboard ROSAT have performed not only the most comprehensive X-ray all-sky survey ever, but also 80 percent of ROSAT's pointed observations amounting to some 3600 PSPC fields in total.

At this point, the PSPC gas tanks are almost empty. The residual gas pressure is approximately ten bars, which can be compared with 600 bars at launch in June 1990. The remaining gas will be saved for observations of very special importance. Such observations can be proposed on a TOO basis ("Super-TOO"). Corresponding proposals should be sent to:

J. Trümper, MPE Garching
Fax: 0049-89-3299 3569,
e-mail: jtrumper@mpe-garching.mpg.de.

(For USA proposers, GSFC request that a CC: of any TOO request also be sent to Rob Petre at LHEAVX::PETRE, for our information).

If a Super-TOO observation is approved, the PSPC will need to be activated for several contiguous days in order to make the most efficient use of the gas supply (each activation requires flushing the detector). This implies that in addition to the TOO program a limited amount of PSPC observing time will become available again. This observing time will be used to complete priority A and B observations of AO's 1-4. In order to be selected, a priority A or B target previously must have gained less than 70 percent of the requested observing time, and it must be accessible at the chosen observing time. While some guest observers will benefit from this philosophy and obtain additional data, we emphasize that the target selection will be totally dependent on the chosen TOO and only a small fraction of the uncompleted A and B observations will be rescheduled.


PROPERTY RIGHTS for REPROCESSED DATASETS

All principal investigators (PI) of ROSAT observations, that have originally been processed before January 1993, already have or will receive their data once more: reprocessed (REV 2 processing) and in the new FITS format (RDF). These reprocessed data belong, for a period of half a year (starting from delivery), exclusively to the PI. Thereafter, they will enter the ROSAT Data Archive (RDA) and replace the data processed by REV 0 software. In addition, results from these observations will be entered (after screening at the Data Centers) into the ROSAT Result Archive (RRA). The RRA will open towards the end of the year.

Data processed after January 1993 are not affected by the main problem in REV 0 processing - occasional jumps of about 1 sec in the event time - and therefore reprocessed sets of these data will not be sent out but directly go to the archives.


ROSAT WORKSHOP III at MPE on OCTOBER 26 and 27

The success of the previous two ROSAT Workshops has convinced us to organize also a 1994 meeting. Please mark the date, October 26 and 27 (Wed./Thu.), in your planning for the autumn. Details will be announced in the next ROSAT NEWS.

NEW EXSAS/MIDAS RELEASE

Around mid-July all EXSAS sites will receive new EXSAS software, fully compatible with the MAY94 version of MIDAS. This MIDAS version now supports also the OSF operating system on DEC Alpha machines, in addition to many UNIX flavors and VMS.

Beginning with that release, the most recent EXSAS software also will be placed in the ROSAT Service Area, from where it can be retrieved. It is planned that future releases of the software will be distributed on tape only on special request.


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Curator: Michael Arida (ADNET); arida@milkyway.gsfc.nasa.gov
HEASARC Guest Observer Facility


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This file was last modified on Monday, 25-Jun-2012 15:16:21 EDT

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