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Titlebook: ISO Surveys of a Dusty Universe; Proceedings of a Rin D. Lemke,M. Stickel,K. Wilke Conference proceedings 2000 Springer-Verlag Berlin Heide

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书目名称ISO Surveys of a Dusty Universe
副标题Proceedings of a Rin
编辑D. Lemke,M. Stickel,K. Wilke
视频video
概述The ISO data have been released into the public domain only recently.This is the first thorough survey what science can do with them.Includes supplementary material:
丛书名称Lecture Notes in Physics
图书封面Titlebook: ISO Surveys of a Dusty Universe; Proceedings of a Rin D. Lemke,M. Stickel,K. Wilke Conference proceedings 2000 Springer-Verlag Berlin Heide
描述Many of the ISO observers who assembled for this workshop at Ringberg c- tle met for the third time in the Bavarian Alps. At two previous meetings in 1989 and 1990 surveys were only a minor topic. At that time we were excited by the discoveries of the IRAS survey mission and wanted to follow it up with pointed observations using an observatory telescope equipped with versatile instruments. With the rapid development of detector arrays and stimulated by ISO’s Observing Time Allocation Committee, however, surveys eventually became an issue for the upcoming mission. In a review paper on “Infrared S- veys - the Golden Age of Exploration” given at an IAU meeting in 1996, Chas Beichman already mentioned that there are ISO surveys. They were at the bottom of his hit list, while the winners were future space missions (Planck, SIRTF, etc. ) and ground-based surveys in preparation (Sloan, 2MASS, DE- NIS, etc. ). He organized his table according to the relative explorable volume, calculated from the solid angle covered on the sky and the maximum distance derived from the detection sensitivity. Clearly, with this ?gure of merit, ISO, as a pointed observatory, is rated low. Applying the classic
出版日期Conference proceedings 2000
关键词Galaxy; LED; MOKE; Quasar; Redshift; Star; astronomy; cluster; collision; spectra; stellar
版次1
doihttps://doi.org/10.1007/3-540-45553-1
isbn_ebook978-3-540-45553-0Series ISSN 0075-8450 Series E-ISSN 1616-6361
issn_series 0075-8450
copyrightSpringer-Verlag Berlin Heidelberg 2000
The information of publication is updating

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发表于 2025-3-21 20:38:58 | 显示全部楼层
Conference proceedings 20001989 and 1990 surveys were only a minor topic. At that time we were excited by the discoveries of the IRAS survey mission and wanted to follow it up with pointed observations using an observatory telescope equipped with versatile instruments. With the rapid development of detector arrays and stimula
发表于 2025-3-22 03:18:53 | 显示全部楼层
ISO Deep Far-Infrared Survey in the Lockman Hole al. by a factor of 10–50. The slopes of the number densities are similar at the both wavelengths, implying far-infrared sources are at low redshift. Comparisons with radio and X-ray sources indicate most of far-infared sources are star-forming galaxies.
发表于 2025-3-22 06:38:14 | 显示全部楼层
FIRBACK Source Counts and Cosmological Implications at other wavelengths, we have developped a phenomenological model, which constrains in a simple way the luminosity function evolution with the redshift, and fits all the existing deep source counts from the mid-infrared to the submillimetre range.
发表于 2025-3-22 08:50:01 | 显示全部楼层
The Extragalactic Background and Its Fluctuations in the Far-Infrared Wavelengthsations, we have used the FIRBACK observations. FIRBACK is a deep cosmological survey conducted at 170μm with ISOPHOT [.]. We show that the emission of unresolved extra-galactic sources clearly dominates, at arc-minute scales, the background fluctuations in the lowest galactic emission regions. This is the first detection of the CFIRB fluctuations.
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Near Infrared Extragalactic Backgroundn foreground emission components. 2- point correlation analysis indicates that the fluctuation has a characteristic spatial frequencyat 1 ∼ 2 × 10. arcmin. These results indicate that the detected isotropic emission is cosmological in origin, and is new observational evidence for the study of the formation and evolution of galaxies.
发表于 2025-3-23 01:00:45 | 显示全部楼层
The European Large Area ISO Survey (ELAIS): Latest Results A comprehensive identification programme is underway and a number of extremely luminous objects have already been discovered. This survey provides an exciting legacy from the ISO mission and (amongst many goals) will allow us to provide important constraints on the obscured star-formation history of the Universe.
发表于 2025-3-23 04:26:00 | 显示全部楼层
A Local Infrared Perspective to Deeper ISO Surveyssing longer wavelength IRAS colour criteria and produce complete 12 μm samples of galaxies and stars. This new technique allows us to estimate the contribution of non-dusty galaxies to the IRAS 12 μm counts and produce a true local mid-infrared extragalactic sample compatible with ISO surveys. We present our initial analysis and results.
发表于 2025-3-23 07:32:23 | 显示全部楼层
The Star Formation History of the Universeound in an Ω. = 1 universe, but this model fails to account for even the lowest estimates of the 140–350 μm background by a factor of 2. Either the observed values are overestimated or we need a new population of submm sources. The problem is eased in a . = 0, Ωo = 0.3 or . = 0.7, Ωo = 0.3 universe.
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