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Results 1 - 3 of 3
EMPRESS. II. Highly Fe-Enriched Metal-poor Galaxies with ?1.0 (Fe/O)? and 0.02 (O/H)? : Possible Traces of Super Massive (>300M?) Stars in Early Galaxies
Volume 15, Issue 24 - article #7
Takashi Kojima
(1,2),
Masami Ouchi
(3,1,4),
Michael Rauch
(5),
Yoshiaki Ono
(1),
Kimihiko Nakajima
(3),
Yuki Isobe
(1,2),
Seiji Fujimoto
(6,7),
Yuichi Harikane
(3,8,1),
Takuya Hashimoto
(9),
Masao Hayashi
(3),
Yutaka Komiyama
(3),
Haruka Kusakabe
(10),
Ji Hoon Kim
(11,12),
Chien-Hsiu Lee
(13),
Shiro Mukae
(1,2),
Tohru Nagao
(14),
Masato Onodera
(11,15),
Takatoshi Shibuya
(16),
Yuma Sugahara
(17),
Masayuki Umemura
(18),
Kiyoto Yabe
(4)
((1) ICRR,
(2) Univ. of Tokyo,
(3) NAOJ,
(4) Kavli IPMU,
(5) Carnegie Observatory,
(6) DAWN fellow,
(7) Univ. of Copenhagen,
(8) UCL,
(9) TCHoU,
(10) Observatoire de Geneve,
(11) Subaru Telescope,
(12) Metaspace,
(13) NOAO,
(14) Ehime Univ.,
(15) SOKENDAI,
(16) Kitami Institute of Tech.,
(17) Waseda Univ.,
(18) Univ. of Tsukuba)
http://arxiv.org/abs/2006.03831
A Lyα Emitter with an Extremely Large Rest-frame Equivalent Width of ~900 Å at
z
= 6.5: A Candidate Population III-dominated Galaxy?
Volume 7, Issue 49 - article #22
Nobunari Kashikawa
,
Tohru Nagao
,
Jun Toshikawa
,
Yoshifumi Ishizaki
,
Eiichi Egami
,
Masao Hayashi
,
Chun Ly
,
Matthew A. Malkan
,
Yuichi Matsuda
,
Kazuhiro Shimasaku
,
Masanori Iye
,
Kazuaki Ota
,
Takatoshi Shibuya
,
Linhua Jiang
,
Yoshiaki Taniguchi
,
and
Yasuhiro Shioya
The Astrophysical Journal - Volume: 761, Issue: 2
Abstract
References
Full text PDF (866 KB)
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A Ly-alpha Emitter with an Extremely Large Rest-frame Equivalent Width of ~900A at z=6.5: A Candidate of Population III-dominated Galaxy?
Volume 7, Issue 42 - article #1
Nobunari Kashikawa
,
Tohru Nagao
,
Jun Toshikawa
,
Yoshifumi Ishizaki
,
Eiichi Egami
,
Masao Hayashi
,
Chun Ly
,
Matthew A. Malkan
,
Yuichi Matsuda
,
Kazuhiro Shimasaku
,
Masanori Iye
,
Kazuaki Ota
,
Takatoshi Shibuya
,
Linhua Jiang
,
Yoshiaki Taniguchi
,
Yasuhiro Shioya
arXiv.org - Astrophysics - Volume: 2012, Issue: 19 Oct
arXiv:1210.4933
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