@inproceedings{oai:jaxa.repo.nii.ac.jp:00002991,
 author = {Pollo, Agnieszka and 竹内, 努 and Malek, Katarzyna and Solarz, Aleksandra and Pepiak, Agata and 松原, 英雄 and AKARI team and Pollo, Agnieszka and Takeuchi, Tsutomu T. and Malek, Katarzyna and Solarz, Aleksandra and Pepiak, Agata and Matsuhara, Hideo and AKARI team},
 book = {宇宙航空研究開発機構特別資料, JAXA Special Publication: Proceedings of the SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe},
 month = {Mar},
 note = {SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe (June 18-21, 2013. Ito Hall, the University of Tokyo), Bunkyou-ku, Tokyo, Japan, Understanding the complex relation between the evolution of large scale structure of the Universe and of galaxies themselves is one of the key problems of modern cosmology. It is well known that galaxy clustering depends on galaxy types and properties, and that this relation evolved with cosmic time in a way which is not yet well understood. In the same time, optical surveys cannot be sufficient to solve the emerging questions: one of the key problems is the evolving dust extinction in galaxies. Hence the necessity of deep multiwavelength infrared observations to understand the link between galaxies and the underlying large scale structure woven from dark matter. However, the present-day infrared observations usually suffer from relatively low resolution which makes it impossible for example to trace the relation between the evolution of galaxies and the history of intergalactic interactions. Also, the spectroscopic data in the infrared are limited. In this paper, we summarize some of the results of our measurements of clustering of dusty galaxies from on the AKARI data, both deep surveys and all-sky survey. We mention the key problems which could not be successfully solved yet: the relation between galaxy clustering and interactions inside one dark matter halo; the evolution of the position in the large scale structure of the extreme types of infrared galaxies, like (U)LIRGs. We discuss the perspectives to answer these questions thanks to SPICA unique sensitivity, resolution, and spectroscopic capabilities., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730027014, レポート番号: JAXA-SP-17-010E},
 pages = {71--74},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {From AKARI to SPICA: a New Window to Understand Links between Cosmology and Galaxy Evolution},
 volume = {JAXA-SP-17-010E},
 year = {2018}
}