Science Watch® - Tracking Trends and Performance in Basic Research
March/April 2004


Sloan Digital Sky Survey’s Stellar Successes
by Simon Mitton
WHAT'S HOT IN PHYSICS
Rank      Paper Citations This Period (Sep -
Oct 03)
Rank Last Period (Jul - Aug 03)
1 K. Eguchi, et al., "First results from KamLAND: Evidence for reactor antineutrino disappearance," Phys. Rev. Lett., 90(2): 1802, 17 January 2003. [12 institutions worldwide] *636FP 50 4
2 Q.R. Ahmad, et al., "Direct evidence for neutrino flavor transformation from neutral-current interactions in the Sudbury Neutrino Observatory," Phys. Rev. Lett., 89(1): 1301, 1 July 2002. [17 institutions worldwide] *563YN 46 3
3 A. Bachtold, et al., "Logic circuits with carbon nanotube transistors," Science, 294(5545): 1317-20, 9 November 2001. [Delft U., Netherlands; Ecole Norm. Super., Paris, France] *491VF 37
4 M. Greiner, et al., "Quantum phase transition from a superfluid to a Mott insulator in a gas of ultracold atoms," Nature, 415(6867): 39-44, 3 January 2002. [U. Munich, Germany; Max Planck Inst. Quantum Optics, Garching, Germany; ETH Zurich, Switzerland] *507KZ 36 1
5 C. Stoughton, et al., "Sloan Digital Sky Survey: Early release data," Astronom. J., 123(1753): 485-548, January 2002. [56 institutions worldwide] *520EJ 34
6 R.R. Metsaev, "Type IIB Green-Schwartz superstring in plane wave Ramond-Ramond background," Nucl. Phys. B, 625: 70-96, 18 March 2002. [Lebedev Phys. Inst., Moscow, Russia] *531CY 33 6
7 Q.R. Ahmad, et al., "Measurement of day and night neutrino energy spectra at SNO and constraints on neutrino mixing parameters," Phys. Rev. Lett., 89(1): 1302, 1 July 2002. [17 institutions worldwide] *563YN 30 7
8 C.B. Netterfield, et al., "A measurement by BOOMERANG of multiple peaks in the angular power spectrum of the cosmic microwave background," Astrophys. J., 571(2): 604-14, 1 June 2002. [14 institutions worldwide] *556CB 29 8
9 D.N. Spergel, et al., "First-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Determination of cosmological parameters," Astrophys. J. Suppl. Ser., 148(1): 175-94, September 2003. [6 U.S. and Canadian institutions] *715BR 28
10 R.R. Metsaev, A.A. Tseytlin, "Exactly solvable model of superstring in plane wave Ramond-Ramond background," Phys. Rev. D, 65(12): 6004, 15 June 2002. [Lebedev Phys. Inst., Moscow, Russia; Imperial Coll., London, U.K.; Ohio St. U., Columbus] *572JW 26
 SOURCE: ISI's Hot Papers DatabaseRead  the full legend.

Mapmaking and surveying have a long tradition in astronomy, going back to at least the second century BCE, when Hipparchus compiled a catalog (long since lost) of 850 stars. Three centuries later, Claudius Ptolemy listed 1,028 star positions, published in his Almagest, the basic text from antiquity on astronomical theory. Copernicus used Ptolemy’s catalog, which was superseded by the last of the great pre-telescopic astronomers, Tycho Brahe. A further 200 years elapsed until William Herschel produced the first real sky survey: a compilation not just of individual stars, but also binaries, clusters, gas and dust nebulae, and galaxies. In the course of this immense undertaking he discovered the planet Uranus, for which King George III gave him a generous pension for life.

The Sloan Digital Sky Survey (SDSS), the subject of newcomer #5, is the most ambitious astronomical survey project ever undertaken. Its origin goes back to 1988 when a team of observers designed a "next-generation" redshift survey, targeting galaxies and quasars. They planned a 100-fold increase in the number of extragalactic objects with good spectroscopy, a survey of the distances of the nearest million galaxies, plus 100,000 quasars. Adding in the stars of the Milky Way, the sky survey called for the positions and brightnesses of 108 celestial objects.

Sunspot, New Mexico is the home base of SDSS: the Apache Point Observatory provides a good site at 2,800 meters, where the atmosphere contains little water vapor. APO is one of darkest sites in the United States, thanks to clean air and distance from large cities. The 2.5-m telescope has the most complex camera ever built, with 30 CCD chips, each of 4 megapixels, cooled by liquid N; the field of view is 3º. A good night of observing produces 200 Gb of data on magnetic tape. Fermilab is the lead center for the data pipelines, automated computer programs that turn the digitized data into useful information on real stars, galaxies, and quasars. The turnaround time needs to be not much more than a week, so that follow-up spectroscopic observations can be planned for the next lunar dark phase. On a good night of spectroscopy anything from 3,000 – 5,500 redshifts is secured, in batches of 640 at a pass using fiber optic feeds.

SDSS will survey 104 square degrees, about 1/4 of the whole sky, and yield a 3D picture of the universe through a volume 100 times that explored to date. Hot Paper #5 is termed "Early data release." The spirit of SDSS is that data are made freely available as quickly as possible. The June 2001 release is for 462 deg2, with data on 1.4 x 107 objects, and 54,000 follow-up spectra.

The high citation rate is entirely down to the thrilling science in this first release. SDSS is great at finding very high redshift quasars, with record breakers at z=6.0 and 6.2 in this release, and further objects at 6.1, 6.28, and 6.4 announced since publication of #5. These quasars are less than 109 years old, and they host the first generation of supermassive black holes. Their distances are so great that their light has passed through dozens of intervening galaxies, whose properties are imprinted on the quasar absorption-line spectrum.

SDSS can probe the distribution of both hot and dark matter. These early results reinforce the current model of a low-density universe with accelerating expansion. SDSS researchers have also looked at the dynamical behavior of thousands of satellite galaxies orbiting around giant parents. They’ve concluded that the gravitational pull of abundant dark matter is speeding up the velocities of the satellites. Although the survey does not tell us what dark matter actually is, it confirms its presence inside galaxies.

In a neat twist, SDSS has also unmasked a secret of the solar system. Asteroids show up as tiny streaks in the field of view. There are fewer asteroids with diameters below 4 km than researchers were expecting, which is good news because it suggests future collisions of an asteroid with Earth may be less likely. The colors of asteroids, revealed by SDSS, show that the population between Mars and Jupiter is spatially separated into two types: an inner belt of rocky asteroids, and an outer zone of carbonaceous bodies.end

Dr. Simon Mitton is Senior Fellow of
St Edmund’s College, University of Cambridge, U
.K.

Science Watch®, March/April 2004, Vol. 15, No. 2
Citing URL: http://www.sciencewatch.com/march-april2004/sw_march-april2004_page6.htm

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