otic-capsule
发表于 2025-3-23 12:48:55
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admission
发表于 2025-3-23 15:07:50
The Matter Spectral Density from Lensed Cosmic Microwave Background Observationsu and Okamoto (ApJ 557:L79–L83, 2001; ApJ 574:566–574, 2002; Phys Rev D 67:083002, 2003). We finish the paper with a discussion regarding the potential scientific applications and the challenges associated with estimating the noise spectrum from simulations.
捕鲸鱼叉
发表于 2025-3-23 18:44:44
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Ingredient
发表于 2025-3-24 01:48:03
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spondylosis
发表于 2025-3-24 02:43:45
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tolerance
发表于 2025-3-24 07:40:20
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Gourmet
发表于 2025-3-24 11:33:38
Robust, Data-Driven Inference in Non-linear Cosmostatisticsedshifts and their number density distribution from approximate, photometric redshift data. The second focuses on cosmic voids and uses them to construct . which allow reconstructing the expansion history of the Universe using the Alcock-Paczynski test. In both cases we find that non-linearities . t
Fraudulent
发表于 2025-3-24 16:08:15
Simulation-Aided Inference in Cosmologynces about cosmological parameters. The first method is a Bayesian calibration approach adapted from Kennedy and O’Hagan (J R Stat Soc B 68:425–464, 2001) and Higdon et al. (J Am Stat Assoc 103:570–583, 2008). It makes use of a response surface model that approximates the simulation output at untrie
collateral
发表于 2025-3-24 20:25:21
Commentary: Simulation-Aided Inference in Cosmologyudy of a set of techniques that are likely to become a standard part of the astrostatistics toolbox. The problems addressed by these techniques models based on expensive computer simulations that run on high-performance computing (HPC) platforms, which can only sparsely sample a large-dimensional in
壕沟
发表于 2025-3-25 01:41:43
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