The Multimission Archive at STScI (MAST) Newsletter disseminates
information to users of the HST, FUSE, IUE, Copernicus, EUVE, HUT,
UIT, WUPPE, IMAPS, BEFS, TUES and VLA-FIRST data archives supported
by MAST. Inquiries should be sent to archive@stsci.edu.
Over 16,000 combined images, created using algorithms developed at
CADC, are available in this initial release. More details are available
at the above World Wide Web (WWW) sites and in the article by David
Schade et al. in this issue. The library of available co-added data
will be augmented simultaneously at all three sites on a regular basis.
Future releases will also provide the association (ASN) files which
will enable users to use the PyDrizzle algorithm to create their own
co-added images.
An example of the improvement afforded by the WFPC2 associations is
given in the figure shown at the above mentioned WWW sites. The figure
compares a portion of a single WFPC2 F814W image of the Chandra Deep
Field South (CDF-S) to the combined, cleaned association of eight
exposures.
Advanced Camera for Surveys (ACS) observations from the Great
Observatories Origins Deep Survey (GOODS;
See the GOODS Website)
constitute one of the Cycle 11 Treasury Programs. The first HLSP from
the GOODS program were delivered to MAST at the beginning of October and
made available
the archive's anonymous ftp site.
These "best effort" processed data
represent preliminary results from the GOODS survey (Version 0.5), and
will eventually be supplemented by deeper images combining all epochs
of observation. These initial HLSP include pipeline-processed,
cosmic-ray cleaned, drizzled and co-added images of each "tile" of the
CDF-S field in the B, V, i, and z bands. The images have also been
corrected for the geometrical distortions introduced by the ACS and
have been put onto the Guide Star Catalog-2 (GSC-2) astrometrical
reference system. More details on the data reduction process can be
found in the file h_goods_s1v05_rdm.txt in the ftp directory.
As of November 15 2002, almost 75 gigabytes of GOODS HLSP have been
retrieved to more than 170 different hosts. MAST is developing ways to
ensure that these and other HLSP will be easily discovered from all
available search methods, including the regular HST search interface
and the mission cross-correlation tool.
The reprocessing effort will take several months to complete, so in the
interim, the FUSE project will generate a simple quick-look preview
from the existing archive, to use until the data are reprocessed. MAST
expects delivery of these quick-looks in early December, when they will
be made available via the FUSE search interface.
At MAST request, the FUSE project has decided upon an agreed package
of "minimum recommended data files" for users who do not want to receive
unneeded files. Additions are being implemented to the FUSE query options
web page
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