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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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31#
發(fā)表于 2025-3-26 21:09:50 | 只看該作者
32#
發(fā)表于 2025-3-27 02:44:47 | 只看該作者
The UV Opacity of High-Redshift Galaxies galaxies we show that . no more than 4% of the continuum UV flux can escape (3. limit) from each galaxy. This result is compatible with observations of low-z galaxies, but is in contradiction with some recent results based on spectroscopy of . ≈ 3 galaxies.
33#
發(fā)表于 2025-3-27 07:11:14 | 只看該作者
34#
發(fā)表于 2025-3-27 09:36:54 | 只看該作者
35#
發(fā)表于 2025-3-27 15:19:31 | 只看該作者
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36#
發(fā)表于 2025-3-27 21:10:21 | 只看該作者
37#
發(fā)表于 2025-3-27 22:52:17 | 只看該作者
AXIS: An XMM-Newton International Surveypril 2000 to April 2002, after which a large number of XMM-Newton target fields have been imaged and ~ 400 X-ray sources have been identified. In this paper we present a few highlights of the AXIS science results (whose full exploitation is still on-going) both at high galactic latitudes and in the Galactic plane.
38#
發(fā)表于 2025-3-28 05:20:36 | 只看該作者
39#
發(fā)表于 2025-3-28 09:28:09 | 只看該作者
40#
發(fā)表于 2025-3-28 10:42:54 | 只看該作者
Cosmology with Galaxy Clusters through the Sunyaev-Zel’dovich Effect small subsample of the cluster catalogue. We also show how it is possible to get an accurate estimate of the cluster flux using a non-parametric component separation algorithm, and how using morphological redshifts it is possible to make a high-z preselection of the small subsample to be observed in the optical.
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