| Item type |
会議発表論文 / Conference Paper(1) |
| 公開日 |
2018-05-01 |
| タイトル |
|
|
タイトル |
From AKARI to SPICA: a New Window to Understand Links between Cosmology and Galaxy Evolution |
|
言語 |
en |
| 言語 |
|
|
言語 |
eng |
| 資源タイプ |
|
|
資源タイプ識別子 |
http://purl.org/coar/resource_type/c_5794 |
|
資源タイプ |
conference paper |
| 著者 |
Pollo, Agnieszka
竹内, 努
Malek, Katarzyna
Solarz, Aleksandra
Pepiak, Agata
松原, 英雄
AKARI team
Pollo, Agnieszka
Takeuchi, Tsutomu T.
Malek, Katarzyna
Solarz, Aleksandra
Pepiak, Agata
Matsuhara, Hideo
AKARI team
|
| 著者所属 |
|
|
|
Jagiellonian University : National Centre for Nuclear Research, Poland |
| 著者所属 |
|
|
|
名古屋大学 |
| 著者所属 |
|
|
|
名古屋大学 |
| 著者所属 |
|
|
|
名古屋大学 |
| 著者所属 |
|
|
|
Jagiellonian University |
| 著者所属 |
|
|
|
宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS) |
| 著者所属（英） |
|
|
|
en |
|
|
Jagiellonian University : National Centre for Nuclear Research, Poland |
| 著者所属（英） |
|
|
|
en |
|
|
Nagoya University |
| 著者所属（英） |
|
|
|
en |
|
|
Nagoya University |
| 著者所属（英） |
|
|
|
en |
|
|
Nagoya University |
| 著者所属（英） |
|
|
|
en |
|
|
Jagiellonian University |
| 著者所属（英） |
|
|
|
en |
|
|
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) |
| 出版者 |
|
|
出版者 |
宇宙航空研究開発機構(JAXA) |
| 出版者（英） |
|
|
出版者 |
Japan Aerospace Exploration Agency (JAXA) |
| 書誌情報 |
宇宙航空研究開発機構特別資料
en : JAXA Special Publication: Proceedings of the SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe
巻 JAXA-SP-17-010E,
p. 71-74,
発行日 2018-03-09
|
| 会議概要（会議名, 開催地, 会期, 主催者等）（英） |
|
|
内容記述タイプ |
Other |
|
内容記述 |
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 |
| 抄録（英） |
|
|
内容記述タイプ |
Other |
|
内容記述 |
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. |
| 内容記述 |
|
|
内容記述タイプ |
Other |
|
内容記述 |
形態: カラー図版あり |
| 内容記述（英） |
|
|
内容記述タイプ |
Other |
|
内容記述 |
Physical characteristics: Original contains color illustrations |
| ISSNONLINE |
|
|
収録物識別子タイプ |
ISSN |
|
収録物識別子 |
2433-2232 |
| 資料番号 |
|
|
内容記述タイプ |
Other |
|
内容記述 |
資料番号: AA1730027014 |
| レポート番号 |
|
|
内容記述タイプ |
Other |
|
内容記述 |
レポート番号: JAXA-SP-17-010E |
AA1730027014.pdf (305.4 kB)
