Constraining the evolution of dark energy with a combination of galaxy cluster observables
S Wang, J Khoury, Z Haiman, M May - Physical Review D—Particles, Fields …, 2004 - APS
We show that the abundance and redshift distribution (d N/dz) of galaxy clusters in future
high-yield cluster surveys, combined with the spatial power spectrum [P c (k)] of the same …
high-yield cluster surveys, combined with the spatial power spectrum [P c (k)] of the same …
Constraining the evolution of dark energy with a combination of galaxy cluster observables
S Wang, J Khoury, Z Haiman, M May - Physical Review. D, Particles …, 2004 - inis.iaea.org
[en] We show that the abundance and redshift distribution (dN/dz) of galaxy clusters in future
high-yield cluster surveys, combined with the spatial power spectrum [P c (k)] of the same …
high-yield cluster surveys, combined with the spatial power spectrum [P c (k)] of the same …
[PDF][PDF] Constraining the Evolution of Dark Energy with a Combination of Galaxy Cluster Observables
S Wang, J Khoury, Z Haiman, M May - arXiv preprint astro-ph/0406331 - scholar.archive.org
We show that the abundance and redshift distribution (dN/dz) of galaxy clusters in future
high–yield cluster surveys, combined with the spatial power spectrum (Pc (k)) of the same …
high–yield cluster surveys, combined with the spatial power spectrum (Pc (k)) of the same …
Constraining the evolution of dark energy with a combination of galaxy cluster observables
W Sheng, J Khoury, Z Haiman, M May - Physical Review. D, Particles Fields, 2004 - osti.gov
We show that the abundance and redshift distribution (dN/dz) of galaxy clusters in future
high-yield cluster surveys, combined with the spatial power spectrum [P {sub c}(k)] of the …
high-yield cluster surveys, combined with the spatial power spectrum [P {sub c}(k)] of the …
Constraining the evolution of dark energy with a combination of galaxy cluster observables
S Wang, J Khoury, Z Haiman, M May - Phys. Rev. D, 2004 - inspirehep.net
We show that the abundance and redshift distribution ($ dN/dz $) of galaxy clusters in future
high--yield cluster surveys, combined with the spatial power spectrum ($ P_c (k) $) of the …
high--yield cluster surveys, combined with the spatial power spectrum ($ P_c (k) $) of the …
[引用][C] Constraining the evolution of dark energy with a combination of galaxy cluster observables
S Wang, J Khoury, Z Haiman, M May - Physical Review D, 2004 - cir.nii.ac.jp
Constraining the evolution of dark energy with a combination of galaxy cluster observables |
CiNii Research CiNii 国立情報学研究所 学術情報ナビゲータ[サイニィ] 詳細へ移動 検索フォームへ …
CiNii Research CiNii 国立情報学研究所 学術情報ナビゲータ[サイニィ] 詳細へ移動 検索フォームへ …
Constraining the Evolution of Dark Energy with a Combination of Galaxy Cluster Observables
S Wang, J Khoury, Z Haiman, M May - arXiv preprint astro-ph/0406331, 2004 - arxiv.org
We show that the abundance and redshift distribution ($ dN/dz $) of galaxy clusters in future
high--yield cluster surveys, combined with the spatial power spectrum ($ P_c (k) $) of the …
high--yield cluster surveys, combined with the spatial power spectrum ($ P_c (k) $) of the …
Constraining the evolution of dark energy with a combination of galaxy cluster observables
S Wang, J Khoury, Z Haiman, M May - Physical Review D, 2004 - ui.adsabs.harvard.edu
We show that the abundance and redshift distribution (dN/dz) of galaxy clusters in future
high-yield cluster surveys, combined with the spatial power spectrum [P c (k)] of the same …
high-yield cluster surveys, combined with the spatial power spectrum [P c (k)] of the same …