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2005 Annual Report
Index:
Personnel |
Research |
Programmatic |
Publications
III. Programmatic
David Band
supported the preparation for NASA's GLAST mission as a member of the
GLAST Science Support Center (GSSC). He continues to edit the documents
describing the science data products that will be exchanged among the components of the
GLAST ground system (including the GSSC); the file formats have been reviewed by
various groups internal and external to the GLAST mission. He also produced the
first draft of the GLAST Technical Handbook that will assist scientists prepare
guest investigator (GI) proposals. Band continues to edit the
GLAST Project Data Management Plan. He drafted the text announcing the first
GI proposal cycle, both as part of the NASA Research Opportunities in Space and Earth Sciences
(ROSES) and on the GSSC website. Band participated in the second GLAST
Data Challenge that tested the analysis software; he was also part of the team that
prepared for, and ran, the beta test of this analysis software by the
GLAST Users' Committee (GUC). In preparation for this beta test
Band wrote, edited and revised major portions of the user documentation for this software.
Band is the GUC's executive secretary, and thus drafts the minutes of the
GUC's meetings, and maintains the GUC website. He also supervised the
implementation of various tools to support the GLAST user community.
Beckmann is a member of the US INTEGRAL Guest
Observer Facility (GOF) and became
its head in 2006 July. In this position he became responsible for collecting and
organising the INTEGRAL AO-4 budget proposals and support for the AO-5 key
program proposals. In addition, Dr Beckmann continued the work on the
high-level results archive, which has been used intensively by the astronomical
community. To support INTEGRAL operations he attended the INTEGRAL/SPI
team meeting at the MPE in March and gave three presentations.
John Cannizzo's duties consisted of providing support for
Swift and LIGO. The
Swift work consisted of several ``on-call'' shifts of 48 hrs as ``Burst Advocate''.
When a GRB occurs, the BA is notified and must participate in a telecon that begins
within a few minutes of the GRB. The BA must then also be in the daily Swift
planning telecon for several weeks afterward to provide advice for follow-up observations. The
LIGO technical support consists of 8 hr shifts at the LIGO site in Livingston, LA.
Dr Cannizzo also assisted in the preparation of a variety of proposals for new and
upcoming missions. In terms of community work, there was also refereeing for
journals (ApJ, A&A, Nature, etc.).
James Chiang
designed and implemented Automated Science Processing (quicklook) analyses of the GLAST
LAT data that will be used by the LAT Instrument Science Operations Center as part of its
Level 2 processing. These analyses will include GRB detection, spectral and spatial analysis, and
flaring source detection and monitoring, especially for blazar studies. Dr. Chiang
chaired a group to evaluate and implement the LAT instrument response functions that are
used by all
of the LAT high level analysis software. He also continued maintaining and developing several
key software analysis packages for the LAT: Likelihood analysis, observation simulator, data
subselector, instrument response function interfaces, and software for event and spacecraft
FITS file generation. In addition, Dr. Chiang operates as the overall LAT Science Tools
code librarian, and organizes and tags code releases and helps coordinate package development
among the various developers. He also implemented source models for simulation and analyses for the
Blazar and Solar System GLAST Science Working groups.
David Davis
continued as the head of the Data Archives & Software support section at the
GLAST SSC and development for the GLAST mission is progressing smoothly.
The sections particiation in the Ground System tests has gone smoothly. A
beta version science tools was tested by the GLAST
Users Committee and had generally good reviews.
Masaharu Hirayama
continued making contributions to the development of the analysis tools of
GLAST LAT (Large Area Telescope) data. Specifically, the pulsar analysis tools were
improved in its user interface for clarity and ease of use, and added new features for
users' convenience such as
automated time conversions between different time systems. The tools were extensively
tested and reviewed in Data Challenge 2, where a large set of data were generated for a
simulated, all-sky survey by the entire GLAST instruments for 55 days and
participants analyzed the data for their scientific goals, and several useful
feedbacks were collected.
Index:
Personnel |
Research |
Programmatic |
Publications
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