论文标题
2500平方学SPT-SZ调查的毫米波点源:目录和人口统计数据
Millimeter-wave Point Sources from the 2500-square-degree SPT-SZ Survey: Catalog and Population Statistics
论文作者
论文摘要
我们提出了SPT-SZ调查中检测到的发射点源的目录,SPT-SZ调查是一个连续的2530平方学区域,该区域与2008年至2011年的South Pole望远镜(SPT)进行了调查,其中三个频段为95、150和220 GHz。该目录包含4845个源,在至少一个频段中以4.5 sigma的显着性测量,对应于95、150和220 GHz的大约9.8、5.8和20.4 mjy的检测。 SPT带中的光谱行为用于基于紧凑的,发射源的物理机制,将源分类为两个种群,这些机制在毫米波长处明亮:来自活性银河核和尘埃的热发射的同步辐射。后一个人口包括通常称为亚毫米星系(SMG)的高红移来源的组成部分。在调查探测的相对明亮的通量范围内,预计这些来源将通过强烈的重力镜头放大。该调查还包含与原始群体相一致的来源,高红移处的一组尘土飞扬的星系经历了崩溃。我们在无线电,红外和X射线波长的外部目录中将SPT-SZ目录交叉匹配,并确定可用的红移信息。该目录将以同步加速器为主导的3980和865个以尘埃为主导的来源分成,我们确定了506个SMG的列表。目录中的十个来源被确定为恒星。我们使用bootstrap方法计算完整目录的数量计数,以及同步子和尘土飞扬的组件,并将我们的测量计数与模型进行比较。本文代表了SPT-SZ调查中点源的第三个也是最后一个目录。
We present a catalog of emissive point sources detected in the SPT-SZ survey, a contiguous 2530-square-degree area surveyed with the South Pole Telescope (SPT) from 2008 - 2011 in three bands centered at 95, 150, and 220 GHz. The catalog contains 4845 sources measured at a significance of 4.5 sigma or greater in at least one band, corresponding to detections above approximately 9.8, 5.8, and 20.4 mJy in 95, 150, and 220 GHz, respectively. Spectral behavior in the SPT bands is used for source classification into two populations based on the underlying physical mechanisms of compact, emissive sources that are bright at millimeter wavelengths: synchrotron radiation from active galactic nuclei and thermal emission from dust. The latter population includes a component of high-redshift sources often referred to as submillimeter galaxies (SMGs). In the relatively bright flux ranges probed by the survey, these sources are expected to be magnified by strong gravitational lensing. The survey also contains sources consistent with protoclusters, groups of dusty galaxies at high redshift undergoing collapse. We cross-match the SPT-SZ catalog with external catalogs at radio, infrared, and X-ray wavelengths and identify available redshift information. The catalog splits into 3980 synchrotron-dominated and 865 dust-dominated sources and we determine a list of 506 SMGs. Ten sources in the catalog are identified as stars. We calculate number counts for the full catalog, and synchrotron and dusty components, using a bootstrap method and compare our measured counts with models. This paper represents the third and final catalog of point sources in the SPT-SZ survey.