论文标题
在普朗克定时数据中测量的紧凑源的极化和变异性
Polarization and variability of compact sources measured in Planck time-ordered data
论文作者
论文摘要
本文介绍了一个新的Planck目录,该目录是偏振和可变的紧凑型源(PCCS-PV),其中包括153个来源,其中大多数是外层次的。数据包括由普朗克测得的总磁通密度和线性极化,频率覆盖率为30至353 GHz,以及时间间距在几天到几年之间。我们将大多数来源分类为横向的,外层次的无线电来源。该目录还包括几个射电星系,Seyfert星系以及银河系和麦哲伦云来源,包括H III区域和行星星云。开发了一种高级提取方法,直接应用于多频Planck时序数据而不是任务天空图,以允许评估极化源的可变性。我们对来自普朗克任务Tod2flux的时级数据的分析使我们能够在Planck使用的全部极化频率(30至353 GHz)中对这些来源的时变发射和极化性能进行分类。 PCCS-PV为所有153个来源提供了时间和频率依赖性的偏振密度。为了说明PCCS-PV的某些潜在应用,我们对所选源的测量进行了初步比较,并与其他天文工具的公开数据进行了比较。总而言之,我们发现普朗克与放射捕集学院(IRAM)极化测量值以及在非常相似的时期的Metsähovi37 GHz值之间的一般一致性。这些合并的测量值还显示了PCCS-PV结果的值和PCCS2目录,用于填充缺失的光谱(或时间)覆盖范围,并有助于定义外层源源的光谱分布。反过来,这些结果为来源的物理特性提供了有用的线索。
This paper introduces a new Planck Catalog of Polarized and Variable Compact Sources (PCCS-PV) comprising 153 sources, the majority of which are extragalactic. The data include both the total flux density and linear polarization measured by Planck with frequency coverage from 30 to 353 GHz, and temporal spacing ranging from days to years. We classify most sources as beamed, extragalactic radio sources; the catalog also includes several radio galaxies, Seyfert galaxies, and Galactic and Magellanic Cloud sources, including H IIi regions and planetary nebulae. An advanced extraction method applied directly to the multifrequency Planck time-ordered data, rather than the mission sky maps, was developed to allow an assessment of the variability of polarized sources. Our analysis of the time-ordered data from the Planck mission, tod2flux, allowed us to catalog the time-varying emission and polarization properties for these sources at the full range of polarized frequencies employed by Planck, 30 to 353 GHz. PCCS-PV provides the time- and frequency-dependent, polarized flux densities for all 153 sources. To illustrate some potential applications of the PCCS- PV, we conducted preliminary comparisons of our measurements of selected sources with published data from other astronomical instruments. In summary, we find general agreement between the Planck and the Institut de Radioastronomie Millimétrique (IRAM) polarization measurements as well as with the Metsähovi 37 GHz values at closely similar epochs. These combined measurements also show the value of PCCS-PV results and the PCCS2 catalog for filling in missing spectral (or temporal) coverage and helping to define the spectral energy distributions of extragalactic sources. In turn, these results provide useful clues as to the physical properties of the sources.