Studies of evolution and formation of galaxies and search for high-redshift quasars with southern CCD survey

这项研究的最高目标是通过测量Fell/MgII发射线的高移位类星体的最高目标来确定宇宙的几何参数，并通过识别远红外来源的可靠银河系统演变。我们打算进行一次南部CCD调查，以寻找高移位类（测量Fell/MgII），并收集CCD图像数据（识别远红外源）。在目前的研究中，我们开发了南部CCD调查的仪器和类星体发射模型，已识别的ISO远红外来源，并研究了世界上最佳观测站点的特点。以下是以下的结果：CCD摄像机的控制电路被更换，第一盏工程灯在2001年12月成功发射。该软件于2002年2月更新，第一次科学运行于2002年4月晚些时候排定。当CCD摄像机被延迟时，我们在KPNO、Subarii和Keck的远红外ISO CCD成像和光谱分析中使用VLA进行了良好的深度无线电成像。到日期为止，100个特别的来源已经找到了。作为写作，减少了30个来源的数据。有三个人被鉴定为ULIRGs （超发光红外星系），其中大多数人是相互作用的星系。在QSOBLR中建模线路转移对从观察到的Fell/MgII中产生Fe/Mg丰度非常重要。为了改进这些模型，我们邀请了E博士。来自CUA/NASA的Verner。用于在KPNO进行建模的高质量QSO规格·在与NOAO连接的情况下，我们分析了智利北部过去10年的天气卫星数据，并已查明为阿塔卡马地区最佳网站提供许可证。我们已经建立了一个天气监测器，并在阿塔卡马网站上安装了一个天气监测器。

The ultimate goal of this research is to determine the geometric parameters of the Universe by measuring the Fell/MgII emission line ratios of high-redshift quasars, and to understand galaxy evolution by identifying far-infrared sources. We thus intend to execute a southern CCD survey for searching for high-redshift quasars (measuring Fell/MgII) and for accumulating CCD image data (identifying far-infrared sources). In the present research, we have developed the instrument of the southern CCD survey and the model of quasar emission, identified ISO far-infrared sources, and studied the characteristics of the world best observing site in north Chile. The results are given below:・ The control circuit of the CCD camera was replaced, and the first engineering light was successfully taken in 2001 December. The software was updated in February 2002, and the first scientific run is scheduled in late-April, 2002.・ While the said CCD camera was delayed, we have carried out CCD imaging and spectroscopy of ISO far-infrared at KPNO, Subarii, and Keck as well as deep radio imaging with VLA. Up to date, spectra of 100 sources were taken. As of writing, data reduction has completed for 30 sources. One third of them have been identified with ULIRGs (Ultra-Luminous IR Galaxies), and most of them are interacting galaxies.・ Modeling of line transfer in a QSO BLR is vitally important to derive the Fe/Mg abundance from the observed Fell/MgII. To improve such models, we have invited Dr. E. Verner from CUA/NASA. The high quality QSO spectra for modeling were taken at KPNO・ In conjunction with NOAO, we have analyzed weather satellite data for the last 10 years in north Chile, and has identified with candidates for the best sites in the Atacama area. We have built a weather monitor and installed at the site in the Atacama for monitoring weather.