Comparison of spectral properties of microwave background inhomogeneities on Planck maps with spectral properties of sources of RCR, NVSS and Planck catalogues

E. Majorova, O. Zhelenkova
{"title":"Comparison of spectral properties of microwave background inhomogeneities on Planck maps with spectral properties of sources of RCR, NVSS and Planck catalogues","authors":"E. Majorova, O. Zhelenkova","doi":"10.22323/1.425.0019","DOIUrl":null,"url":null,"abstract":"A study of the spectral properties of positive spots on multifrequency Planck maps near RCR sources showed their identity with the spectral properties of NVSS sources and closest objects of the Planck catalogue associated with them. In both cases, a linear correlation was found between spectral indices of radio sources in the range of 0.15 - 3.94 GHz and spectral indices of closest spots (of Planck objects) in the frequency range 30 - 217 GHz. The compare of the combined spectra of RCR sources and closest positive spots with the combined spectra of NVSS sources and associated with them objects from the Planck catalogue suggests that the spots found near RCR sources may be manifestations of them in the sub-millimeter range, and most of the spots are extragalactic in nature. Part of the combined spectra of RCR objects and nearby positive spots can be explained by the variability of radio sources. The spectrum of averaged temperatures of hot spots detected near RCR sources was constructed, which showed a quantitative excess over those obtained earlier by modeling, which can be explained by the influence of synchrotron background or the contribution of radio source to radiation in the submillimeter range. The contribution of these unaccounted for radio sources to the foreground background can affect the resulting map of the cosmological microwave background.","PeriodicalId":355234,"journal":{"name":"Proceedings of The Multifaceted Universe: Theory and Observations - 2022 — PoS(MUTO2022)","volume":"15 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2022-09-26","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Proceedings of The Multifaceted Universe: Theory and Observations - 2022 — PoS(MUTO2022)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.22323/1.425.0019","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0

Abstract

A study of the spectral properties of positive spots on multifrequency Planck maps near RCR sources showed their identity with the spectral properties of NVSS sources and closest objects of the Planck catalogue associated with them. In both cases, a linear correlation was found between spectral indices of radio sources in the range of 0.15 - 3.94 GHz and spectral indices of closest spots (of Planck objects) in the frequency range 30 - 217 GHz. The compare of the combined spectra of RCR sources and closest positive spots with the combined spectra of NVSS sources and associated with them objects from the Planck catalogue suggests that the spots found near RCR sources may be manifestations of them in the sub-millimeter range, and most of the spots are extragalactic in nature. Part of the combined spectra of RCR objects and nearby positive spots can be explained by the variability of radio sources. The spectrum of averaged temperatures of hot spots detected near RCR sources was constructed, which showed a quantitative excess over those obtained earlier by modeling, which can be explained by the influence of synchrotron background or the contribution of radio source to radiation in the submillimeter range. The contribution of these unaccounted for radio sources to the foreground background can affect the resulting map of the cosmological microwave background.
普朗克图上微波背景不均匀性与RCR、NVSS和普朗克星表源光谱特性的比较
对RCR源附近多频普朗克图上正点的光谱特性的研究表明,它们与NVSS源和与之相关的普朗克星表中最近天体的光谱特性一致。在这两种情况下,射电源在0.15 - 3.94 GHz范围内的频谱指数与最近点(普朗克天体)在30 - 217 GHz频率范围内的频谱指数之间存在线性相关。将RCR源和最近正点的组合光谱与NVSS源的组合光谱以及与它们相关的普朗克星表天体的组合光谱进行比较,表明在RCR源附近发现的斑点可能是它们在亚毫米范围内的表现,并且大多数斑点的性质是河外的。部分RCR天体和附近正点的组合光谱可以用射电源的变异性来解释。构建了RCR源附近探测到的热点平均温度谱,该谱比之前的建模结果显示出数量上的过剩,这可以通过同步加速器背景的影响或射电源对亚毫米范围辐射的贡献来解释。这些未知的射电源对前景背景的贡献可能会影响宇宙微波背景的结果图。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 求助全文
来源期刊
自引率
0.00%
发文量
0
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信