The DOI matches its Crossref record; 59 of the 59 references it cites were found in a registry or an index.
A halo-based galaxy group finder: calibration and application to the 2dFGRS
Open accessAbstract
We use the halo occupation model to calibrate galaxy group finders in magnitude-limited redshift surveys. Since, according to the current scenario of structure formation, galaxy groups are associated with cold dark matter halos, we make use of the properties of the halo population in the design of our group finder. The method starts with an assumed mass-to-light ratio to assign a tentative mass to each group. This mass is used to estimate the size and velocity dispersion of the underlying halo that hosts the group, which in turn is used to determine group membership (in redshift space). This procedure is repeated until no further changes occur in group memberships. We find that the final groups selected this way are insensitive to the mass-to-light ratio assumed. We use mock catalogues, constructed using the conditional luminosity function (CLF), to test the performance of our group finder in terms of completeness of true members and contamination by interlopers. Our group finder is more successful than the conventional Friends-of-Friends group finder in assigning galaxies in common dark matter halos to a single group. We apply our group finder to the 2-degree Field Galaxy Redshift Survey and compare the resulting group properties with model predictions based on the CLF. For the $Λ$CDM `concordance' cosmology we find a clear discrepancy between the model and data in the sense that the model predicts too many rich groups. In order to match the observational results we have to either increase the mass-to-light ratios of rich clusters to a level significantly higher than current observational estimates, or to assume $σ_8 \simeq 0.7$, compared to the `concordance' value of 0.9.
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Spergel, D. N., Verde, L., Peiris, H. V., Komatsu, E., Nolta, M. R., Bennett, C. L., Halpern, M., Hinshaw, G., Jarosik, N., Kogut, A., et al. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/377226 · Cited by 10,976
A Universal Density Profile from Hierarchical Clustering
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1997) · The Astrophysical Journal · doi:10.1086/304888 · Cited by 9,917
A Universal Density Profile from Hierarchical ClusteringPreprint
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1996) · Cited by 6,275
Large-scale bias and the peak background split
Sheth, R. K., & Tormen, G. (1999) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.1999.02692.x · Cited by 2,783
The 2dF Galaxy Redshift Survey: spectra and redshifts
Colless, M., Dalton, G., Maddox, S., Sutherland, W., Norberg, P., Cole, S., Bland-Hawthorn, J., Bridges, T., Cannon, R., Collins, C., et al. (2001) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2001.04902.x · Cited by 2,367
Profiles of dark haloes: evolution, scatter and environment
Bullock, J. S., Kolatt, T. S., Sigad, Y., Somerville, R. S., Kravtsov, A. V., Klypin, A. A., Primack, J. R., & Dekel, A. (2001) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2001.04068.x · Cited by 2,319
Statistical Properties of X‐Ray Clusters: Analytic and Numerical Comparisons
Bryan, G. L., & Norman, M. L. (1998) · The Astrophysical Journal · doi:10.1086/305262 · Cited by 2,295
Cole, S., Lacey, C. G., Baugh, C. M., & Frenk, C. S. (2002) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2000.03879.x · Cited by 1,952
Sheth, R. K., Mo, H. J., & Tormen, G. (2001) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2001.04006.x · Cited by 1,807
Self-citationMeasures of location and scale for velocities in clusters of galaxies - A robust approach
Beers, T. C., Flynn, K., & Gebhardt, K. (1990) · The Astronomical Journal · doi:10.1086/115487 · Cited by 1,395
Cited by
Galaxy and Mass Assembly (GAMA): the GAMA galaxy group catalogue (G3Cv1)
Robotham, A. S. G., Norberg, P., Driver, S. P., Baldry, I. K., Bamford, S. P., Hopkins, A. M., Liske, J., Loveday, J., Merson, A., Peacock, J. A., et al. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.19217.x · Cited by 379
Galaxy Bulges and their Black Holes: a Requirement for the Quenching of Star Formation
Bell, E. F. (2008) · The Astrophysical Journal · doi:10.1086/589551 · Cited by 100
Prediction of galaxy halo masses in SDSS DR7 via a machine learning approach
Calderon, V. F., & Berlind, A. A. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz2775 · Cited by 48
Metadata
- Authors
- Yang, X., Mo, H. J., van den Bosch, F. C., & Jing, Y. P.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2005-02
- Volume
- 356
- Issue
- 4
- Pages
- 1293-1307
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2103612329
- Cited by
- 444
- References
- 59
- FWCI
- 12.88
- Type
- journal article
- Language
- en
- Open access
- green
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- Yang, X., Mo, H. J., van den Bosch, F. C., & Jing, Y. P. (2005). A halo-based galaxy group finder: calibration and application to the 2dFGRS. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1111/j.1365-2966.2005.08560.x
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