The DOI matches its Crossref record; 44 of the 44 references it cites were found in a registry or an index.
Constraints on Cosmological Parameters from Future Galaxy Cluster Surveys
Open accessAbstract
We study the expected redshift evolution of galaxy cluster abundance between 0 ≲ z ≲ 3 in different cosmologies, including the effects of the cosmic equation of state parameter w ≡ p /ρ. Using the halo mass function obtained in recent large-scale numerical simulations, we model the expected cluster yields in a 12 deg 2 Sunyaev-Zeldovich effect (SZE) survey and a deep 10 4 deg 2 X-ray survey over a wide range of cosmological parameters. We quantify the statistical differences among cosmologies using both the total number and redshift distribution of clusters. Provided that the local cluster abundance is known to a few percent accuracy, we find only mild degeneracies between w and either Ω m or h . As a result, both surveys will provide improved constraints on Ω m and w . The Ω m - w degeneracy from both surveys is complementary to those found either in studies of cosmic microwave background (CMB) anisotropies or of high-redshift supernovae (SNe). As a result, combining these surveys together with either CMB or SNe studies can reduce the statistical uncertainty on both w and Ω m to levels below what could be obtained by combining only the latter two data sets. Our results indicate a formal statistical uncertainty of ≈3% (68% confidence) on both Ω m and w when the SZE survey is combined with either the CMB or SN data; the large number of clusters in the X-ray survey further suppresses the degeneracy between w and both Ω m and h . Systematics and internal evolution of cluster structure at the present pose uncertainties above these levels. We briefly discuss and quantify the relevant systematic errors. By focusing on clusters with measured temperatures in the X-ray survey, we reduce our sensitivity to systematics such as nonstandard evolution of internal cluster structure.
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Citations
Cites
Measurements of Ω and Λ from 42 High‐Redshift Supernovae
Perlmutter, S., Aldering, G., Goldhaber, G., Knop, R. A., Nugent, P., Castro, P. G., Deustua, S., Fabbro, S., Goobar, A., Groom, D. E., et al. (1999) · The Astrophysical Journal · doi:10.1086/307221 · Cited by 18,062
Numerical recipes in C: the art of scientific computing
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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
Cosmological consequences of a rolling homogeneous scalar field
Ratra, B., & Peebles, P. J. E. (1988) · Physical Review D · doi:10.1103/physrevd.37.3406 · Cited by 4,310 · cited 1×
“From a particle physics point of view, such w > −1 can arise in a number of theories (see Freese, Adams & Frieman 1987, Ratra & Peebles 1988, Turner & White 1997, Caldwell, Dave & Steinhardt 1998 and references therein).”
BackgroundThe Large-Scale Structure of the Universe
Peebles, P. J. E. (1981) · Princeton University Press eBooks · doi:10.1515/9780691206714 · Cited by 2,851
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
The mass function of dark matter haloes
Jenkins, A., Frenk, C. S., White, S. D. M., Colberg, J. M., Cole, S., Evrard, A. E., Couchman, H. M. P., & Yoshida, N. (2001) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2001.04029.x · Cited by 1,659
Carroll, S. M., Press, W. H., & Turner, E. L. (1992) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.aa.30.090192.002435 · Cited by 1,542
Schmidt, B. P., Suntzeff, N. B., Phillips, M. M., Schommer, R. A., Clocchiatti, A., Kirshner, R. P., Garnavich, P., Challis, P., Leibundgut, B., Spyromilio, J., et al. (1998) · The Astrophysical Journal · doi:10.1086/306308 · Cited by 1,505
Cited by
SEVEN-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE(WMAP) OBSERVATIONS: COSMOLOGICAL INTERPRETATION
Komatsu, E., Smith, K. M., Dunkley, J., Bennett, C. L., Gold, B., Hinshaw, G., Jarosik, N., Larson, D., Nolta, M. R., Page, L., et al. (2011) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/192/2/18 · Cited by 8,802
Dalal, N., Doré, O., Huterer, D., & Shirokov, A. (2008) · Physical Review D · doi:10.1103/physrevd.77.123514 · Cited by 830
The large-scale structure of the Universe
Springel, V., Frenk, C. S., & White, S. D. M. (2006) · Nature · doi:10.1038/nature04805 · Cited by 780
GALAXY CLUSTERS DISCOVERED WITH A SUNYAEV-ZEL'DOVICH EFFECT SURVEY
Staniszewski, Z., Ade, P. A. R., Aird, K. A., Benson, B. A., Bleem, L. E., Carlstrom, J. E., Chang, C. L., Cho, H.-M., Crawford, T. M., Crites, A. T., et al. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/701/1/32 · Cited by 322
“A catalog of clusters with masses and redshifts can be used to constrain the matter density, the density fluctuation amplitude, and the dark energy equation of state (Wang & Steinhardt 1998; Haiman et al. 2001; Holder et al. 2001; Molnar et al. 2004; Wang et al. 2004; Lima & Hu 2007).”
MethodSelf-citationLoCuSS: Subaru Weak Lensing Study of 30 Galaxy Clusters
Okabe, N., Takada, M., Umetsu, K., Futamase, T., & Smith, G. P. (2010) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/62.3.811 · Cited by 266
Metadata
- Authors
- Haiman, Z., Mohr, J. J., & Holder, G. P.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2001-06
- Volume
- 553
- Issue
- 2
- Pages
- 545-561
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2000953049
- Cited by
- 462
- References
- 44
- FWCI
- 20.97
- Type
- journal article
- Language
- en
- Open access
- bronze
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