防锈
发表于 2025-3-30 10:52:55
http://reply.papertrans.cn/103/10220/1021959/1021959_51.png
WAX
发表于 2025-3-30 14:15:22
http://reply.papertrans.cn/103/10220/1021959/1021959_52.png
hedonic
发表于 2025-3-30 18:22:34
http://reply.papertrans.cn/103/10220/1021959/1021959_53.png
Granular
发表于 2025-3-31 00:05:39
Early 2017 Limits on Neutrino Masses and Mass Ordering,collaboration, Dawson KS et al, The Baryon oscillation spectroscopic Survey of SDSS-III. Astron J 145:10, 2013, ) had released cosmological products from their final data release, DR12, containing over a million galaxies.
冷峻
发表于 2025-3-31 04:23:11
http://reply.papertrans.cn/103/10220/1021959/1021959_55.png
商店街
发表于 2025-3-31 08:11:13
http://reply.papertrans.cn/103/10220/1021959/1021959_56.png
DAMN
发表于 2025-3-31 12:30:13
Scale-Dependent Galaxy Bias and CMB Lensing-Galaxy Cross-Correlations,, ), galaxy clustering (i.e. power spectrum) data represents a powerful probe of massive neutrinos (and more generally of free-streaming species). However, naïvely comparing the constraining power of .(.) versus BAO measurements revealed that improvements are needed in order to fully harness the
Surgeon
发表于 2025-3-31 14:31:50
http://reply.papertrans.cn/103/10220/1021959/1021959_58.png
Feature
发表于 2025-3-31 21:15:45
Massive Neutrinos Meet (Non-Phantom) Dark Energy,siderably when relaxing assumptions on the underlying cosmological model and allowing for an extended parameter space. An example is discussed in Sect. IVC of [.] (not discussed in Chap. .), where we treated the dark energy equation of state as a free parameter (this quantity is fixed to . in .CDM):
有组织
发表于 2025-3-31 23:37:32
http://reply.papertrans.cn/103/10220/1021959/1021959_60.png