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THE NEXT-GENERATION INFRARED SPACE MISSION SPICA: PROJECT UPDATES
TAKAO NAKAGAWA,Hiroshi Shibai,HIDEHIRO KANEDA,Kotaro Kohno,Hideo Matsuhara,Hiroyuki Ogawa,TAKASHI ONAKA,Peter Roelfsema,Toru Yamada 한국천문학회 2017 天文學論叢 Vol.32 No.1
We present project updates of the next-generationinfrared space mission SPICA (Space Infrared Telescope for Cosmology and Astrophysics)as of November 2015. SPICA isoptimized for mid- and far-infrared astronomy with unprecedented sensitivity, which will be achievedwith a cryogenically cooled (below 8 K), large (2.5~m) telescope. SPICA is expected to address a number ofkey questions in various fields of astrophysics, ranging from studies of the star-formation history in theuniverse to the formation and evolution of planetary systems. The international collaboration framework of SPICA has been revisited. SPICA under the new framework passed the Mission Definition Review by JAXA in 2015. A proposal under the new framework to ESA is being prepared. The target launch year in the new framework is 2027/28.
THE NEXT-GENERATION INFRARED ASTRONOMY MISSION SPICA UNDER THE NEW FRAMEWORK
NAKAGAWA, TAKAO,SHIBAI, HIROSHI,ONAKA, TAKASHI,MATSUHARA, HIDEO,KANEDA, HIDEHIRO,KAWAKATSU, YASUHIRO The Korean Astronomical Society 2015 天文學論叢 Vol.30 No.2
We present the current status (as of August 2014) of SPICA (Space Infrared Telescope for Cosmology and Astrophysics), which is a mission optimized for mid- and far-infrared astronomy with a cryogenically cooled 3m-class telescope. SPICA is expected to achieve high spatial resolution and unprecedented sensitivity in the mid- and far-infrared, which will enable us to address a number of key problems in present-day astronomy, ranging from the star-formation history of the universe to the formation of planets. We have carried out the "Risk Mitigation Phase" activity, in which key technologies essential to the realization of the mission have been extensively developed. Consequently, technical risks for the success of the mission have been significantly mitigated. Along with these technical activities, the international collaboration framework of SPICA has been revisited, which resulted in la arger contribution from ESA than that in the original plan. To enable the ESA participation under the new framework, a SPICA proposal to ESA is under consideration as a medium-class mission under the framework of the ESA Cosmic Vision. The target launch year of SPICA under the new framework is the mid-2020s.
Observing Simulations of Far-Infrared Surveyor on-board ASTRO-F: Extragalactic Point Sources
Woong-Seob Jeong,Soojong Pak,Hyung Mok Lee,Sam Kim,Jungjoo Sohn,Mikako Matsuura,Takao Nakagawa,Issei Yamamura,Shujl Matsuura,Mitsunobu Kawada,Hidehiro Kaneda,Hiroshi Murakami,Hiroshi Shibai 한국천문학회 2000 天文學會報 Vol.25 No.2
Observing Simulations of Far-Infrared Surveyor on-board ASTRO-F : Extragalactic Point Sources
Woong-Seob Jeong,Soojong Pak,Hyung-Mok Lee,Sam Kim,Jungjoo Sohn,Mikako Matsuura,Takao Nakagawa,Issei Yamamura,Shuji Matsuura,Mitsunoby Kawada,Hidehiro Kaneda,Hiroshi Murakami,Hiroshi Shibai 한국우주과학회 2000 한국우주과학회보 Vol.9 No.2