The Vimos-VLT Deep Survey: Results from the First-Epoch Observations

机译：Vimos-VLT深度调查：第一个时代观测结果结果

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The Vimos-VLT Deep Survey is a spectroscopic survey aiming at collecting more than 50 000 spectra down to a limiting magnitude /AB = 24, and 100 000 down to JAB = 22.5, on a total of about 16 deg2 without any color or morphology preselection We present the N(z) distribution up to z ~ 5, obtained from a purely magnitude-limited sample down to /AB = 24, which is an important input to weak-lensing studies. We discuss the evolution of the galaxy luminosity function up to 2 ~ 2, which exhibits a very strong increase in the typical galaxy luminosity AM* ~ -2 5 in the U band compared to the local value. Surveys like the VVDS also allow to study the galaxy bias as a function of redshift without assumption about its linearity, an assumption that we find to be violated in some cases, A low bias is found, and the lineal bias is shown to increase with redshift

机译：ViMOS-VLT深度调查是一种光谱测量，其旨在将大于50 000光谱收集到限制幅度/ ab = 24，并且在100 000到jab = 22.5的情况下，总共约16个DEG2，没有任何颜色或形态预先选择我们将N（Z）分布呈现为Z〜5的Z〜5，从纯度限制的样品下降到/ ab = 24，这是对弱镜头研究的重要输入。我们讨论了Galaxy亮度函数高达2〜2的演变，与局部值相比，U频带中典型的星系亮度AM *〜-2 5的典型星系亮度呈非常强烈增加。像VVDS这样的调查也允许在没有假设其线性的情况下作为红移的函数研究Galaxy偏见，发现我们发现在某些情况下被侵犯的假设，发现了低偏差，并且线路偏置显示随着红移增加

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《International Astronomical Union》|2005年||共6页
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S. Paltani; O. Ilbert; O. Le Fevre; C. Marinoni; Bottini; B.Garilli; V. Le Bran; D. Maccagni; J.-P. Picat; R. Scaramella; M. Scodeggio; L. Tresse; G. Vettolani; A. Zanichelli; C. Adami; M.Arnaboldi; S. Arnouts; S. Bardelli; M. Bolzonella; A. Cappi; S. Chariot; T. Contini; S. Foucaud; P. Franzetti; I. Gavignaud; L. Guzzo; A. Iovino; H.J. McCracken; B. Marano; A. Mazure; B. Meneux; R. Merighi; R. Pello; A. Polio; L. Pozzetti; M. Radovich; G. Zamorani; E. Zucca; M. Bondi; A. Bongiorno; G. Busarello; P. Ciliegi; L. Gregorini; G. Mathez; Y. Mellier; P. Merluzzi; V. Ripepi; D. Rizzo;
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1. Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model - II. The colour???density relation up to z ?~? 1.5 [J] . O. Cucciati, G. De Lucia, E. Zucca, Astronomy and astrophysics . 2012,第19期

机译：VIMOS-VLT深度勘测与慕尼黑半分析模型的比较-II。色密度比最高可达z？〜？ 1.5
2. The VIMOS-VLT Deep Survey: Mass and light clustering in the Universe during the last 8 billion years [J] . A. POLLO, U. ABBAS, B. MENEUX, Il Nuovo Cimento della Societa Italiana di Fisica, B. General physics, relativity, astronomy and mathematical physics and methods . 2008,第9a11期

机译：VIMOS-VLT深度调查：过去80亿年中宇宙中的质量和光聚集
3. The VIMOS-VLT Deep Survey: Mass and light clustering in the during the last 8 billion years [J] . A.POLLOCK, U. ABBAS, B.MENEUX, Il Nuovo Cimento della Societa Italiana di Fisica, B. General physics, relativity, astronomy and mathematical physics and methods . 2007,第9a11期

机译：VIMOS-VLT深度调查：过去80亿年中的质量和光聚集
4. The Vimos-VLT Deep Survey: Results from the First-Epoch Observations [C] . S. Paltani, O. Ilbert, O. Le Fevre, International Astronomical Union . 2005

机译：Vimos-VLT深度调查：第一个时代观测结果结果
5. The development of a deep-towed gravity meter, and its use in marine geophysical surveys of offshore southern California and an airborne laser altimeter survey of Long Valley, California. [D] . Ridgway, Jeffrey R. 1997

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6. Survey of Deep-Learning Approaches for Remote Sensing Observation Enhancement [O] . Grigorios Tsagkatakis, Anastasia Aidini, Konstantina Fotiadou, 2019

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7. The Vimos-VLT Deep Survey: Results from the First-Epoch Observations [O] . Le Fèvre, O., Marinoni, C., Garilli, B., 2005

机译：Vimos-VLT深度调查：第一次观测的结果
8. Joint US-Japan Observations with the Infrared Space Observatory (ISO): Deep Surveys and Observations of High-Z Objects [R] . Sanders, D. B. 1997

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The Vimos-VLT Deep Survey: Results from the First-Epoch Observations

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