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Titlebook: Highlights of Spanish Astrophysics III; Proceedings of the f Jesús Gallego (SEA President),Jaime Zamorano (SEA Conference proceedings 2003

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41#
發(fā)表于 2025-3-28 18:03:56 | 只看該作者
42#
發(fā)表于 2025-3-28 20:29:11 | 只看該作者
Clusters of Galaxies in X-Rays: Dark Matterters. The new X-ray satellites Chandra and XMM yield exciting new results for galaxy cluster physics and cosmology. We show the interesting X-ray observations of two intermediate redshift clusters, RBS797 (. = 0.35) and CL 0939+4713 (. = 0.41) taken with Chandra and XMM respectively.
43#
發(fā)表于 2025-3-29 00:35:23 | 只看該作者
44#
發(fā)表于 2025-3-29 05:02:54 | 只看該作者
45#
發(fā)表于 2025-3-29 07:29:45 | 只看該作者
SNe-Ia and the Formation History of Early-Type Galaxiesnd with galaxy mass suggests different dynamical formation scenarios between high- and low-mass ellipticals, favouring inside-out formation in low-mass systems versus an outside-in process in massive elliptical galaxies.
46#
發(fā)表于 2025-3-29 11:59:41 | 只看該作者
Major Improvements to Estimate Luminosity Functions Using Maximum Likelihood Methodsithin the ML method; (4) combination of heterogeneous samples made out with different selection criteria; and (5) implementation for objective-prism images..These new improvements are mandatory for a good determination of the LF, and its reliability has been checked by means of simulations.
47#
發(fā)表于 2025-3-29 16:44:52 | 只看該作者
Structure Formation in the Universe, at a higher significance, previous measurements by several groups. The observations can be reconciled with flat A universe with σ. ? 1 provided the linear spectrum is steeper (. ? 1) than in the ACDM model on small (cluster) scales. The galaxy distribution are anti-bias with . 0.1 on small scales, increasing with scale to . 1 at 10 Mpc/..
48#
發(fā)表于 2025-3-29 20:32:19 | 只看該作者
roach relying on a swarm of subordinate agents executed in a virtual environment to determine optimal strategies. The problem is treated as a “Narrow AGI” problem with the scope of goals and environments bound to financial markets, specifically crypto-markets. Such an agent is called an “adaptive mu
49#
發(fā)表于 2025-3-30 01:43:18 | 只看該作者
50#
發(fā)表于 2025-3-30 07:00:05 | 只看該作者
J. Miralda-Escudéf uniform definitions of what constitutes intelligence and what is information, the capabilities such models provide differ according to their interpretations of intelligence and implicit assumptions about what is information. The variety of interpretations of intelligence and information also indic
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