The DOI matches its Crossref record; 77 of the 77 references it cites were found in a registry or an index.
CHANDRA CLUSTER COSMOLOGY PROJECT. II. SAMPLES AND X-RAY DATA REDUCTION
Open accessAbstract
We discuss the measurements of the galaxy cluster mass functions at z ≈ 0.05 and z ≈ 0.5 using high-quality Chandra observations of samples derived from the ROSAT PSPC All-Sky and 400 deg 2 surveys. We provide a full reference for the data analysis procedures, present updated calibration of relations between the total cluster mass and its X-ray indicators ( T X , M gas , and Y X ) based on a subsample of low- z relaxed clusters, and present a first measurement of the evolving L X – M tot relation (with M tot estimated from Y X ) obtained from a well defined statistically complete cluster sample and with appropriate corrections for the Malmquist bias applied. Finally, we present the derived cluster mass functions, estimate the systematic uncertainties in this measurement, and discuss the calculation of the likelihood function. We confidently measure the evolution in the cluster comoving number density at a fixed mass threshold, e.g., by a factor of 5.0 ± 1.2 at M 500 = 2.5 × 10 14 h −1 M ☉ between z = 0 and 0.5. This evolution reflects the growth of density perturbations, and can be used for the cosmological constraints complementing those from the distance–redshift relation.
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Cites
Savitzky-Golay Smoothing Filters
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FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: COSMOLOGICAL INTERPRETATION
Komatsu, E., Dunkley, J., Nolta, M. R., Bennett, C. L., Gold, B., Hinshaw, G., Jarosik, N., Larson, D., Limon, M., Page, L., et al. (2009) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/180/2/330 · Cited by 5,786
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Parameter estimation in astronomy through application of the likelihood ratio
Cash, W. (1979) · The Astrophysical Journal · doi:10.1086/156922 · Cited by 3,083
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
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
Baryonic Features in the Matter Transfer Function
Eisenstein, D. J., & Hu, W. (1998) · The Astrophysical Journal · doi:10.1086/305424 · Cited by 2,239
Merger rates in hierarchical models of galaxy formation
Lacey, C., & Cole, S. (1993) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/262.3.627 · Cited by 2,190
Toward a Halo Mass Function for Precision Cosmology: The Limits of Universality
Tinker, J., Kravtsov, A. V., Klypin, A., Abazajian, K., Warren, M., Yepes, G., Gottlöber, S., & Holz, D. E. (2008) · The Astrophysical Journal · doi:10.1086/591439 · Cited by 1,819
Self-citationThe 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
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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
NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: COSMOLOGICAL PARAMETER RESULTS
Hinshaw, G., Larson, D., Komatsu, E., Spergel, D. N., Bennett, C. L., Dunkley, J., Nolta, M. R., Halpern, M., Hill, R. S., Odegard, N., et al. (2013) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/208/2/19 · Cited by 5,121
Bocquet, S., Dietrich, J. P., Schrabback, T., Bleem, L. E., Klein, M., Allen, S. W., Applegate, D. E., Ashby, M. L. N., Bautz, M., Bayliss, M., et al. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab1f10 · Cited by 365
Self-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
von der Linden, A., Allen, M. T., Applegate, D. E., Kelly, P. L., Allen, S. W., Ebeling, H., Burchat, P. R., Burke, D. L., Donovan, D., Morris, R. G., et al. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt1945 · Cited by 259
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Metadata
- Authors
- Vikhlinin, A., Burenin, R. A., Ebeling, H., Forman, W. R., Hornstrup, A., Jones, C., Kravtsov, A. V., Murray, S. S., Nagai, D., Quintana, H., & Voevodkin, A.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2009-02-20
- Volume
- 692
- Issue
- 2
- Pages
- 1033-1059
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2085061516
- Cited by
- 722
- References
- 77
- FWCI
- 33.93
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Vikhlinin, A., Burenin, R. A., Ebeling, H., Forman, W. R., Hornstrup, A., Jones, C., Kravtsov, A. V., Murray, S. S., Nagai, D., Quintana, H., & Voevodkin, A. (2009). CHANDRA CLUSTER COSMOLOGY PROJECT. II. SAMPLES AND X-RAY DATA REDUCTION. The Astrophysical Journal. https://doi.org/10.1088/0004-637x/692/2/1033
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