Abstract

We measure the topology (genus curve) of the galaxy distribution in a mock\nredshift catalog designed to resemble the upcoming Sloan Digital Sky Survey\n(SDSS). The catalog, drawn from a large N-body simulation of a Lambda-CDM cos-\nmological model, mimics the anticipated spectroscopic selection procedures of\nthe SDSS in some detail. Sky maps, redshift slices, and 3-D contour maps of the\nmock survey reveal a rich and complex structure, including networks of voids\nand superclusters that resemble the patterns seen in the CfA redshift survey\nand the Las Campanas Redshift Survey (LCRS). The 3-D genus curve can be\nmeasured from the simulated catalog with superb precision; this curve has the\ngeneral shape predicted for Gaussian, random phase initial conditions, but the\nerror bars are small enough to demonstrate with high significance the subtle\ndepartures from this shape caused by non-linear gravitational evolution. These\ndistortions have the form predicted by Matsubara's (1994) perturbative anal-\nysis, but they are much smaller in amplitude. We also measure the 3-D genus\ncurve of the radial peculiar velocity field measured by applying distance-\nindicator relations (with realistic errors) to the mock catalog. This genus\ncurve is consistent with the Gaussian random phase prediction, though it is of\nrelatively low precision because of the large smoothing length required to\novercome noise in the measured velocity field. Finally, we measure the 2-D\ntopology in redshift slices, similar to early slices from the SDSS and to\nslices already observed in the LCRS. The genus curves of these slices are\nconsistent with the observed genus curves of the LCRS, providing further\nevidence in favor of the inflationary CDM model with Omega_M~0.4. The catalog\nis publicly available at http://www.astronomy.ohio-state.edu/~dhw/sdss.html.\n

Keywords

PhysicsRedshiftSkyCold dark matterGalaxySmoothingAstrophysicsDark matterMeasure (data warehouse)Redshift surveyTopology (electrical circuits)GaussianComputer scienceData miningComputer vision

Affiliated Institutions

Related Publications

Publication Info

Year
2000
Type
article
Volume
529
Issue
2
Pages
795-810
Citations
23
Access
Closed

External Links

Social Impact

Social media, news, blog, policy document mentions

Citation Metrics

23
OpenAlex

Cite This

Wesley N. Colley, J. Richard Gott, David H. Weinberg et al. (2000). Topology from the Simulated Sloan Digital Sky Survey. The Astrophysical Journal , 529 (2) , 795-810. https://doi.org/10.1086/308289

Identifiers

DOI
10.1086/308289