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Lite (Light) satellite for the studies of
B-mode polarization and Inflation from cosmic background Radiation Detection


‰F’ˆq‹óŒ¤‹†ŠJ”­‹@\(JAXA)E‰F’ˆ‰ÈŠwŒ¤‹†Š(ISAS)
’|ˆä —m TAKEI Yoh
•Ÿ‰Æ ‰p”V FUKE Hideyuki
¼Œ´ ‰p—Y MATSUHARA Hideo
–ž“c ˜a‹v MITSUDA Kazuhisa
ŽRè “TŽq YAMASAKI Noriko
‹g“c “N–ç YOSHIDA Tetsuya


‰F’ˆq‹óŒ¤‹†ŠJ”­‹@\(JAXA)EŒ¤‹†ŠJ”­–{•”(ARD)
²“¡ —mˆê SATO Yoichi
ŽÂè Œc—º SHINOZAKI Keisuke
™“c Š°”V SUGITA Hiroyuki


‰ªŽR‘åŠw (Okayama University)
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Ζì G˜a ISHINO Hirokazu
Ž÷—Ñ “ÖŽq KIBAYASHI Atsuko
•ž•” —¢ HATTORI Kaori
ŽOàV ®“T MISAWA Naonori
”ü”n Šo MIMA Satoru


UC Berkeley
Adnan Ghribi  
William Holzapfel  
Bradley Johnson  
Adrian Lee  
Paul Richards  
Aritoki Suzuki  —é–Ø—Lt
Huan Tran  


Lawrence Berkeley National Laboratory (LBNL)
Julian Borrill  


‹ß‹E‘åŠw (Kinki University)
‘å“c ò OHTA Izumi


‚ƒGƒlƒ‹ƒM[‰Á‘¬ŠíŒ¤‹†‹@\(KEK)E‰Á‘¬ŠíŒ¤‹†Ž{Ý(ACCL)
‹g“c ŒõG YOSHIDA Mitsuhiro


‚ƒGƒlƒ‹ƒM[‰Á‘¬ŠíŒ¤‹†‹@\(KEK)E‘f—±ŽqŒ´ŽqŠjŒ¤‹†Š(IPNS)
ΓO”’ WŽ¡ ISHIDOSHIRO Koji
•ÐŽR L•F KATAYAMA Nobuhiko
²“¡ L–¾ SATO Nobuaki
ZàV ˆê‚ SUMISAWA Kazutaka
“c“‡ Ž¡ TAJIMA Osamu
‰iˆä ½ NAGAI Makoto
‰i“c —³ NAGATA Ryo
¼–ì Œº‹L NISHINO Haruki
‰HŸ ¹Žj HAZUMI Masashi
’·’Jì ‰ë–ç HASEGAWA Masaya
”óŒû Šx—Y HIGUCHI Takeo
¼‘º ’mŠx MATSUMURA Tomotake


‚ƒGƒlƒ‹ƒM[‰Á‘¬ŠíŒ¤‹†‹@\(KEK)E’´“`“±’ቷHŠwƒZƒ“ƒ^[(CSC)
–Ø‘º ½G KIMURA Nobuhiro
—é–Ø •qˆê SUZUKI Toshikazu
“sŠÛ —²s TOMARU Takayuki


‘‡Œ¤‹†‘åŠw‰@‘åŠw (SOKENDAI)
–öÀ ‚¦‚è YAGINUMA Eri


University of Texas, Austin
Eiichiro Komatsu ¬¼ ‰pˆê˜Y


‘—§“V•¶‘ä(NAOJ)Eæ’[‹ZpƒZƒ“ƒ^[(ATC)
‰LàV ‰À“¿ UZAWA Yoshinori
ŠÖ–{ —T‘¾˜Y SEKIMOTO Yutaro
ГΞ ԓ NOGUCHI Takashi


“Œ–k‘åŠwiTohoku University)
Šª —TŽi CHINONE Yuji
•ž•” ½ HATTORI Makoto


’}”g‘åŠw(Tsukuba University)
‚“c ‘ì TAKADA Suguru


—‰»ŠwŒ¤‹†Š(RIKEN)Eƒeƒ‰ƒwƒ‹ƒcƒCƒ[ƒWƒ“ƒOŒ¤‹†ƒ`[ƒ€(THz Sensing and Imaging Team)
‘å’J ’ms OTANI Chiko


‰¡•l‘—§‘åŠw (Yokohama National University)
‚–Ø —Y‘¾ TAKAGI Yuta
’†‘º ³Œá NAKAMURA Shogo
‘ºŽR Œd MURAYAMA Satoshi



LiteBIRD