24.01.2013 Views

STScI Annual Report 2002: A Living Mission

STScI Annual Report 2002: A Living Mission

STScI Annual Report 2002: A Living Mission

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

36 improvements<br />

Better Management of Anomaly <strong>Report</strong>ing<br />

Anomalies sometimes affect the quality of science data from Hubble. When this<br />

occurs, the responsible Institute staff members and astronomers using the<br />

data must be informed. In the past, anomaly reporting involved unrelated tools,<br />

manual effort, and various locations for storing information, which, for example,<br />

made data collection for trending evaluations difficult to accomplish. An Institute<br />

initiative called PROMPT— PRoblem Observation Management ProjecT—has<br />

improved anomaly reporting by automating processes to ensure completeness<br />

and consistency and consolidating information in one database. PROMPT has<br />

three components: AlertObs collects anomoly information through a graphical<br />

user interface, places it in a database, and distributes an alert message to<br />

Institute staff; AlertPI generates the Observation Exception <strong>Report</strong>, which is sent<br />

to the proposal contact and placed in a database; and AlertAQ processes new or<br />

updated AlertObs anomaly entries and documents them in the archive catalogue.<br />

PHASTGMS Improves Hubble Proposing<br />

The Institute organized the PHASTGMS (PHASe I to Grants Management System)<br />

project to resolve problems encountered in Cycle 10 when the Phase I proposals<br />

were processed. Four groups joined in this effort— the Science Policies Division,<br />

the Grants Administration Branch, the Engineering and Software Services<br />

Division, and the Program Coordinators. The PHASTGMS project established new<br />

procedures for proposal processing, set requirements for tools to maintain the<br />

Principal Investigator and Co-Investigator addresses, created an interface control<br />

document to rationalize transitions between systems and responsible groups,<br />

and supported the use of the Astronomers Proposal Tool (APT) for Phase I<br />

submission, which was in place for Cycle 12. The PHASTGMS improvements will<br />

ensure rapid and efficient processing of proposals as well as the creation of<br />

an accurate database for proposal management and tracking.<br />

Improvements in the Hubble Program Selection Process<br />

The Institute began the Hubble Treasury Program, which the HST Second Decade<br />

committee recommended, to increase the number of large programs and to<br />

pursue strategic science objectives, such as synergism with other missions and<br />

acquiring important data sets that otherwise would not be available for many<br />

years after the end of the Hubble mission. The Director appointed the Hubble<br />

Treasury Program Advisory Committee to provide advice on ways and means,<br />

strategic directions, and opportunities to promote community participation in<br />

the Hubble Treasury Program. After considering the various ways to facilitate<br />

large collaborations, we conducted a well-attended Hubble Treasury workshop in<br />

fall <strong>2002</strong>, in which numerous possible Treasury projects were enunciated. We<br />

then formed interest groups, which began the work of formulating proposals for<br />

large observing programs based on these ideas. We plan to repeat this activity<br />

every year in connection with the summer meeting of the American Astronomical<br />

Society. Data sets from Hubble Treasury programs are non-proprietary and<br />

immediately available to the community. After processing, observing teams will<br />

provide 'science-ready' data sets to the archive plus ancillary data products,<br />

such as catalogues. Because supporting observations at other wavelengths add<br />

value to these programs, we will continue to work with other important national<br />

facilities—such as Chandra, SIRTF, NOAO, and Gemini—to coordinate observing<br />

projects on multiple telescopes.

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!