標(biāo)題: Titlebook: Looking Deep in the Southern Sky; Proceedings of the E Raffaella Morganti,Warrick J. Couch Conference proceedings 1999 Springer-Verlag Berl [打印本頁(yè)] 作者: Ferret 時(shí)間: 2025-3-21 18:53
書(shū)目名稱Looking Deep in the Southern Sky影響因子(影響力)
書(shū)目名稱Looking Deep in the Southern Sky影響因子(影響力)學(xué)科排名
書(shū)目名稱Looking Deep in the Southern Sky網(wǎng)絡(luò)公開(kāi)度
書(shū)目名稱Looking Deep in the Southern Sky網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書(shū)目名稱Looking Deep in the Southern Sky被引頻次
書(shū)目名稱Looking Deep in the Southern Sky被引頻次學(xué)科排名
書(shū)目名稱Looking Deep in the Southern Sky年度引用
書(shū)目名稱Looking Deep in the Southern Sky年度引用學(xué)科排名
書(shū)目名稱Looking Deep in the Southern Sky讀者反饋
書(shū)目名稱Looking Deep in the Southern Sky讀者反饋學(xué)科排名
作者: Dissonance 時(shí)間: 2025-3-21 23:20
B. J. Boyle,S. M. Croom,R. J. Smith,T. Shanks,L. Miller,N. Loaring作者: 修正案 時(shí)間: 2025-3-22 04:24
M. J. Drinkwater,E. M. Sadler,J. I. Davies,R. J. Dickens,M. D. Gregg,Q. A. Parker,S. Phillipps,R. M.作者: promote 時(shí)間: 2025-3-22 06:38 作者: Distribution 時(shí)間: 2025-3-22 12:31 作者: headway 時(shí)間: 2025-3-22 13:58
Gravitational Lensing in the 2dF Galaxy Redshift Survey The presence of the lensed quasar has allowed unprecedented determinations of the mass distribution of this system (.., Schmidt, Webster & Lewis 1998). This paper is concerned with predicting the number of lensed quasars and galaxies that could be detected using only the 2dF GRS spectra as a primar作者: Acetaminophen 時(shí)間: 2025-3-22 19:47
Conference proceedings 1999ry Synthesis Telescope (MOST) Wide Field continuum survey at radio wavelengths. With all these new facilities, important progress will be made regarding important issues such as the large- scale structure of the universe, the very early universe and the associated first epoch of galaxy formation. Th作者: 顛簸地移動(dòng) 時(shí)間: 2025-3-23 00:21 作者: STEER 時(shí)間: 2025-3-23 02:17
978-3-662-22119-8Springer-Verlag Berlin Heidelberg 1999作者: 廢止 時(shí)間: 2025-3-23 08:25
Looking Deep in the Southern Sky978-3-540-49460-7Series ISSN 1431-2433 Series E-ISSN 1611-6143 作者: indenture 時(shí)間: 2025-3-23 13:17
ESO Astrophysics Symposiahttp://image.papertrans.cn/l/image/588623.jpg作者: 手勢(shì) 時(shí)間: 2025-3-23 14:08 作者: 用手捏 時(shí)間: 2025-3-23 19:24 作者: MANIA 時(shí)間: 2025-3-24 01:49 作者: Amendment 時(shí)間: 2025-3-24 03:50 作者: 邊緣帶來(lái)墨水 時(shí)間: 2025-3-24 09:01 作者: 土產(chǎn) 時(shí)間: 2025-3-24 12:04
Surveys of Peculiar Velocities of GalaxiesSubstantial progress has recently been made in the understanding of the mass distribution in the local Universe through analysis of the all-sky velocity field. The current status of such peculiar velocity surveys is reviewed in this paper. Recent discrepant conclusions for the density of the Universe are discussed.作者: Assault 時(shí)間: 2025-3-24 15:18
The Cosmological Uncertainty PrincipleWe are investigating light propagation through evolving cosmological dark matter distributions, in order to determine the magnification properties of the universe, particularly in the weak lensing limit.作者: lacrimal-gland 時(shí)間: 2025-3-24 21:18 作者: 高興去去 時(shí)間: 2025-3-25 00:14
A Complete 2dF Survey of Fornaxuasars, any previously unrecognised compact galaxies and a large sample of Galactic stars. Here we present initial results from the first 680 objects observed, including the discovery of a number of dwarf galaxies in the cluster more compact than any previously known.作者: 玉米 時(shí)間: 2025-3-25 06:53 作者: 高度贊揚(yáng) 時(shí)間: 2025-3-25 08:20 作者: orient 時(shí)間: 2025-3-25 12:47
Conference proceedings 1999ere arose quite naturally. In the optical and the near-infrared, the Very Large Telescope (VLT) will soon be operational. In the radio, the Australia Telescope Com- pact Array is going to be upgraded to higher frequencies (20 and 100 GHz), together with an improvement in very long baseline interfero作者: Vldl379 時(shí)間: 2025-3-25 17:30 作者: Capitulate 時(shí)間: 2025-3-25 23:57 作者: Servile 時(shí)間: 2025-3-26 00:08 作者: 勉勵(lì) 時(shí)間: 2025-3-26 08:17 作者: ABYSS 時(shí)間: 2025-3-26 10:46 作者: accessory 時(shí)間: 2025-3-26 16:04 作者: ADOPT 時(shí)間: 2025-3-26 17:37
Weak Lensing with MEGACAM and the VLTd projected mass map and projected power spectrum are remarkably similar to the original ones. We thus are confident that the superb images obtained with MEGACAM, combined with the redshift distribution of sources inferred from the VIRMOS survey, will be a unique tool for cosmology.作者: 的事物 時(shí)間: 2025-3-27 00:21 作者: GUILE 時(shí)間: 2025-3-27 03:51 作者: Obloquy 時(shí)間: 2025-3-27 08:04 作者: Neuralgia 時(shí)間: 2025-3-27 13:26 作者: CRUE 時(shí)間: 2025-3-27 15:35
ESO Imaging Survey made to address this problem by carrying out a public imaging survey to produce targets for the first year of operation of the VLT. Here the goals, strategy and preliminary results of this effort are presented. Current plans to greatly expand the imaging facilities of ESO in the short and long-term作者: CAJ 時(shí)間: 2025-3-27 21:11
Cosmological Tests from the New Surveys (i) the importance of understanding selection effects in catalogues and matching Northern and Southern surveys; (ii) the 2dF galaxy redshift survey of 250,000 galaxies (iii) the proposed 6dF redshift and peculiar velocity survey of near-infrared galaxies (iv) radio sources and the X-Ray Background 作者: NAVEN 時(shí)間: 2025-3-27 22:41
Mapping the Dark Matter with Weak Gravitational Lensing dark matter distribution in the Universe. Concentrating on those aspects which require deep wide-field imaging surveys, I will describe the basic principles of weak lensing and discuss its future application (a) to determine the statistical properties of the dark matter halos of individual galaxies作者: 無(wú)孔 時(shí)間: 2025-3-28 05:33
Weak Lensing with MEGACAM and the VLTts will be dedicated to surveys. In this proceeding, we show how we can use MEGACAM+VIRMOS to map the mass distribution on large scales. Simulated projected mass density maps show that mass reconstruction from lensing inversion can recover the input power spectrum using MEGACAM images. The mass reco作者: 有機(jī)體 時(shí)間: 2025-3-28 08:37
Gravitational Lensing in the 2dF Galaxy Redshift Survey Boyle 1997). As such it will provide a great deal of information about the galaxy population (.., luminosity function, clustering properties) in the local (?..? ? 0.1) universe. However, the spectral information obtained will not provide any direct information about the mass of the survey galaxies.作者: impaction 時(shí)間: 2025-3-28 11:37
A Weak Gravitational Lensing Cluster Surveyhe mass of the clusters is determined via weak gravitational lensing, and correlated with the X-ray and optical properties. This direct probe of the cluster mass distribution will constrain the dynamical and thermodynamical state and evolution of the cluster population.作者: 貿(mào)易 時(shí)間: 2025-3-28 17:31 作者: 有角 時(shí)間: 2025-3-28 19:40
Deep Images of Bright Galaxiesng magnitudes, especially for extended objects. This limit can be extended even further by applying special photographic techniques to the plates and combining the enhanced information from several deep plates. This allows us to reach a limiting (B) surface brightness of about 28 B mag aresec., whic作者: llibretto 時(shí)間: 2025-3-29 02:02
A Deep Tech Pan Survey of Dwarf Spheroidal Galaxies in Virgo the U.K. Schmidt Telescope. The objects we detect have the same physical sizes and surface brightnesses as Local Group dwarf spheroidal galaxies. The luminosity function of these extremely low luminosity galaxies (down to .. ? ?11 or about 5 × 10...) is very steep, with a power law slope . ? ?2, su作者: 容易做 時(shí)間: 2025-3-29 05:30
Surveys with a 4m Liquid Mirror Telescope is its very low cost, is particularly well suited for the search and study of gravitational lenses, type Ia supernovae, faint nearby red, brown and white dwarfs, halo stars with high proper motions and, more generally, all variable phenomena like quasars, variable stars, micro-lensing effects, etc.作者: conception 時(shí)間: 2025-3-29 08:29
eder?sterreichischen Wirtschaft vertritt. Den Mittelpunkt der Organisation bilden das Pr?sidium und die Direktion. Die weitere Gliederung unterscheidet in die Kammer im engeren Sinne sowie in die sieben Sparten: Bank und Versicherung, Gewerbe und Handwerk, Handel, Industrie, Information und Consulti作者: Infelicity 時(shí)間: 2025-3-29 15:18
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