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

Forestall

書目名稱ISO Surveys of a Dusty Universe影響因子(影響力)




書目名稱ISO Surveys of a Dusty Universe影響因子(影響力)學(xué)科排名




書目名稱ISO Surveys of a Dusty Universe網(wǎng)絡(luò)公開度




書目名稱ISO Surveys of a Dusty Universe網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱ISO Surveys of a Dusty Universe被引頻次




書目名稱ISO Surveys of a Dusty Universe被引頻次學(xué)科排名




書目名稱ISO Surveys of a Dusty Universe年度引用




書目名稱ISO Surveys of a Dusty Universe年度引用學(xué)科排名




書目名稱ISO Surveys of a Dusty Universe讀者反饋




書目名稱ISO Surveys of a Dusty Universe讀者反饋學(xué)科排名

DAFT

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

Anecdote

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.

表臉

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.

induct

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.

懸掛

大方一點(diǎn)

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.

翅膀拍動(dòng)

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.

–LOUS

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.

ELUC

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.