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The FY 2002 Budget Request for the Astronomical
Sciences (AST) Subactivity is $156.26 million, an increase of $7.62
million, or 5.1 percent, over the FY 2001 Current Plan of $148.64
million.
(Millions of Dollars)
|
FY
2000 Actual |
FY 2001
Current Plan |
FY 2002
Request |
Change |
Amount |
Percent |
Astronomical Sciences |
42.96
|
53.94
|
54.71
|
0.77
|
1.4%
|
Facilities |
79.57
|
94.70
|
101.55
|
6.85
|
7.2%
|
Total, AST |
$122.53
|
$148.64
|
$156.26
|
$7.62
|
5.1%
|
NSF is the lead federal agency for ground-based astronomy,
providing about two-thirds of the federal support for this area
of science, including almost all of the federal support for radio
astronomy.
Astronomy Research and Instrumentation includes support
for astronomical and astrophysical studies of the origins and characteristics
of planets, the Sun, other stars, our galaxy, extragalactic objects
such as clusters of galaxies and quasars, and the structure and
origin of the Universe. The development of advanced technologies
and instrumentation and university radio observatories are also
supported. Support often includes funding for graduate students
and postdoctoral fellows as well as for instrumentation and other
research needs. Also supported within this program element is NSF's
Electromagnetic Spectrum Management (ESM) program, which participates
with other federal agencies in coordinating the use of the electromagnetic
spectrum for research and other activities.
The FY 2002 budget request includes $54.71 million
for research and instrumentation support in the Astronomical Sciences
that will advance the scientific priorities of studies in cosmology
and the origin of the universe and the formation of stars and planets.
Other priorities include continued support for the development of
adaptive optics systems for telescopes, the search for extra-solar
planets, research on the origin, evolution, and structure of the
Universe, including significant activities in the area of particle
astrophysics. A number of these activities involve intra- and interagency
partnerships. Grant size will be increased to allow researchers
to capitalize on the investments made by the federal, state, and
private sectors in major new observational facilities. Support will
also be provided for research and development that may lead to important
facility upgrades or new installations in the future. Through the
ITR priority area, support will be provided for research and applications
in databases, data mining, and high speed computation. The Science
and Technology Center (STC) for Adaptive Optics will be funded within
AST in FY 2002.
An exciting example of the research supported in
the Astronomical Sciences is related to "cosmic shear",
defined as slight distortions in the images of distant galaxies
caused by large intervening structures of primarily dark matter.
A group of astronomers led by J. A. Tyson from Lucent Technologies,
G. Bernstein of the University of Michigan, and Ian Dell' Antonio
of the National Optical Astronomy Observatories detected a statistical
signal of cosmic shear for the first time using wide-field images
with the NSF Cerro Tololo Inter-American Observatory 4-meter telescope,
part of NOAO. This initial detection was based upon measurements
of the images of about 50,000 galaxies and demonstrates the principles
to be used in a much larger cosmic shear survey currently underway.
These measurements will provide a powerful tool to determine fundamental
cosmological parameters related to the distribution of mass in the
universe, and will test the foundations of cosmology.
The Facilities budget line item includes support
for three national facilities: the National Astronomy and Ionosphere
Center (NAIC), the National Optical Astronomy Observatories (NOAO),
and the National Radio Astronomy Observatory (NRAO). Also included
is the U.S. share of operations for the International Gemini Observatories,
twin 8-meter telescopes located in the northern and southern hemispheres.
These facilities together provide world-class observing capabilities
throughout the electromagnetic spectrum, from radio to infrared
and optical regimes of the electromagnetic spectrum. Also included
in the facilities budget line is continued maintenance of the established
infrastructure for the Atacama Large Millimeter Array (ALMA), an
international project being undertaken in partnership with the European,
Chilean and Canadian communities. ALMA will be the world's most
sensitive, high resolution millimeter wavelength telescope.
FY 2002 support for Facilities totals $101.55 million,
and includes:
Support for Gemini Observatories at a level of
$11.0 million. The northern Gemini telescope is now in regular
science operations, and the southern telescope expects to begin
science observations in mid-2001. The Gemini Observatory remains
the highest priority among our optical and infrared facilities.
Activities for Gemini in FY 2002 will include development of advanced
instrumentation and expansion of the public information and outreach
effort to better serve the citizens of all of the partner countries.
Following a one-time increment in FY 2001 that
enabled major improvements in facilities infrastructure, NAIC
will be supported at $9.40 million, the level specified in the
National Science Board-approved cooperative agreement. This level
of support will enable continued operation and maintenance of
the renovated Arecibo telescope and the development of instrumentation
to take advantage of its greater sensitivity.
Support for NOAO is at the level of $32.02 million.
NOAO provides observational facilities to the U.S. astronomical
community in both the Northern and Southern hemispheres. Support
is provided for operations and maintenance of a suite of optical/infrared
and solar telescopes, and for the operations of the U.S. Gemini
Project Office. Activities in FY 2002 include continued design
and planning for the Advanced Technology Solar Telescope (ATST),
an instrument that will be of significant value to studies in
atmospheric sciences and space weather in addition to astronomical
research.
Following a one-time increment in FY 2001 that
enabled major improvements in facilities infrastructure and attention
to deferred maintenance, NRAO support will be decreased to the
level of $40.13 million. This reduction of funds has been redirected
in part to support ALMA. NRAO support will provide for operations,
maintenance, and instrumentation for their unique telescopes,
including the Robert C. Byrd Green Bank Telescope, the Very Large
Array (VLA), and the Very Long Baseline Array (VLBA). Activities
in FY 2002 include making remaining enhancements in operations
at the VLA and the Byrd Telescope.
Included are funds for maintenance of the established
infrastructure for the Atacama Large Millimeter Array (ALMA),
an international project being undertaken in Chile in partnership
with the European and Canadian community. Additional activities
in FY 2002 will include testing of antenna prototypes and the
design and development of advanced, ultra-sensitive millimeter-wavelength
receivers. The project leadership is also pursuing other significant
international partnerships. ALMA will be the world's most sensitive,
high resolution millimeter wavelength telescope. Funding within
the Major Research Equipment Account for Phase I of this project
was completed in FY 2001.
The proposal to fund ALMA within the Research and
Related Activities account is tentative pending the review of facilities
management issues and the development of a plan to enhance the Foundation's
management of large facilities. It may be determined that it is
more appropriate to fund ALMA from within the Major Research Equipment
account.
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