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東京大学大学院情報理工学系研究科創造情報学専攻修士論文フォーマット（2021年／日本語版）を、学生有志がOverleafに対応させたものです。This is the master's thesis format (2021/Japanese version) of the Department of Creative Informatics, Graduate School of Information Science and Technology, the University of Tokyo, adapted to Overleaf by student volunteers.

東京大学理学部情報科学科の学位論文を組版するためのドキュメントクラス iscs-thesis (v1.3) を Overleaf で使えるようにしたものです。

社会文化環境学専攻修士論文要旨のフォーマット, Overleaf対応させた非公式テンプレートです It is made by students and not official.

東京大学大学院情報理工学系研究科コンピュータ科学専攻 修士論文を組版するためのドキュメントクラス iscs-thesis (v1.3) を Overleaf に対応させたものです。

東京大学大学院情報理工学系研究科コンピュータ科学専攻 博士論文をを組版するためのドキュメントクラス iscs-thesis (v1.3) を Overleaf に対応させたものです。

東京大学大学院新領域創成科学研究科社会文化環境学専攻の修士/博士論文のWordテンプレートを学生有志がOverleaf対応させた非公式テンプレートです。

A template for thesis of Department of Mechano-Informatics, Graduate School of Information Science and Technology, The University of Tokyo.

計数工学科システムコースの卒論のテンプレートです。 https://qiita.com/yokotech/items/4e98f75caf7b52282b19 に従って作業を行ったものをここにおいています。

AKARI and Spinning Dust: A look at microwave dust emission via the Infrared Aaron C. Bell's Master's Course Thesis ABSTRACT: Rapidly spinning dust particles having a permanent electric dipole moment have been shown to be a likely carrier of the anomalous microwave emission (AME), a continuous excess of microwave flux in the 10 to 90 GHz range. Small grains, possibly polycyclic aromatic hydrocarbons (PAHs), are a leading suspect. In the absence of a definitive answer on the presence of PAHs or their role as an AME carrier, some predictions have been made as to the implications of spinning PAH emission. Due to the overlap between the CMB and the galactic foreground, this topic is requiring cosmologists to consider the ISM with more care. ISM astronomers are also needing to consider the contribution of cosmological radiation to large-scale dust investigations. We present data from AKARI/Infrared Camera (IRC) due to the effective PAH band coverage of its 9 micron survey to investigate their role within the 98 AME candidate regions identified by Planck Collaboration et al. (2014). We supplement AKARI data with the four Infrared Astronomical Satellite (IRAS) all-sky maps and complement with the Planck High Frequency Instrument (HFI) bands at 857 and 545 GHz to constrain the full dust thermal spectral energy distribution (SED). We sample the average spectral energy distributions (SEDs) all 98 regions. We utilize all 7 AKARI photometric bands, as well as the 4 IRAS bands and 2 HFI. We carry out a modified blackbody fitting, and estimate the optical depth of thermal dust at 250 micron, and compare this to AME parameters. We also show plots of each band's average intensity for all 98 regions vs. AME parameters. We find a positive trend between the optical depth and AME. In the band-by-band comparison the AKARI 9 micron intensity shows a weaker trend with AME. In general, the MIR correlates less strongly with AME than the FIR. The optical depth vs. AME trend improves slightly when looking only at significant AME regions. Scaling the IR intensities by the ISRF strength G0 does not improve the correlations. A slightly positive trend found previously among 10 AME regions vs. AME significance is revisited, using the larger sample of 98. However the trend does not hold up to the full data set. We cannot offer strong support of a spinning dust model. The results highlight the need for full dust SED modelling, and for a better understanding of the role that magnetic dipole emission from dust grains could play in producing the AME.