贪婪地吃 发表于 2025-3-26 21:09:50
http://reply.papertrans.cn/43/4271/427026/427026_31.pngLoathe 发表于 2025-3-27 02:44:47
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.高谈阔论 发表于 2025-3-27 07:11:14
http://reply.papertrans.cn/43/4271/427026/427026_33.png培养 发表于 2025-3-27 09:36:54
http://reply.papertrans.cn/43/4271/427026/427026_34.png震惊 发表于 2025-3-27 15:19:31
http://image.papertrans.cn/h/image/427026.jpg调色板 发表于 2025-3-27 21:10:21
http://reply.papertrans.cn/43/4271/427026/427026_36.pngobviate 发表于 2025-3-27 22:52:17
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.spinal-stenosis 发表于 2025-3-28 05:20:36
http://reply.papertrans.cn/43/4271/427026/427026_38.png哑剧 发表于 2025-3-28 09:28:09
http://reply.papertrans.cn/43/4271/427026/427026_39.pngIncorporate 发表于 2025-3-28 10:42:54
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.