“Zombie” or active? An alternative explanation to the properties of star-forming galaxies at high redshift
A&A, 617 (2018) A131
Published online: 2018-10-02
Articles citing this article
The Citing articles tool gives a list of articles citing the current article.
The citing articles come from EDP Sciences database, as well as other publishers participating in CrossRef Cited-by Linking Program. You can set up your personal account to receive an email alert each time this article is cited by a new article (see the menu on the right-hand side of the abstract page).
Cited article:
This article has been cited by the following article(s):
GA-NIFS: witnessing the complex assembly of a star-forming system at z = 5.7
Gareth C Jones, Andrew J Bunker, Kseniia Telikova, Santiago Arribas, Stefano Carniani, Stephane Charlot, Francesco D’Eugenio, Roberto Maiolino, Michele Perna, Bruno Rodríguez Del Pino, Hannah Übler, Chris Willott, Manuel Aravena, Torsten Böker, Giovanni Cresci, Mirko Curti, Jorge González-López, Rodrigo Herrera-Camus, Isabella Lamperti, Eleonora Parlanti, Pablo G Pérez-González and Vicente VillanuevaMonthly Notices of the Royal Astronomical Society 540 (4) 3311 (2025)
https://doi.org/10.1093/mnras/staf899
ALMA twenty-six arcmin2 survey of GOODS-S at one millimeter (ASAGAO): Millimeter properties of stellar mass selected galaxies
Yuki Yamaguchi, Kotaro Kohno, Bunyo Hatsukade, Tao Wang, Yuki Yoshimura, Yiping Ao, James S Dunlop, Eiichi Egami, Daniel Espada, Seiji Fujimoto, Natsuki H Hayatsu, Rob J Ivison, Tadayuki Kodama, Haruka Kusakabe, Tohru Nagao, Masami Ouchi, Wiphu Rujopakarn, Ken-ichi Tadaki, Yoichi Tamura, Yoshihiro Ueda, Hideki Umehata and Wei-Hao WangPublications of the Astronomical Society of Japan 72 (4) (2020)
https://doi.org/10.1093/pasj/psaa057
High-redshift star formation in the Atacama large millimetre/submillimetre array era
J. A. Hodge and E. da CunhaRoyal Society Open Science 7 (12) 200556 (2020)
https://doi.org/10.1098/rsos.200556
Large Population of ALMA Galaxies at z > 6 with Very High [O iii] 88 μm to [C ii] 158 μm Flux Ratios: Evidence of Extremely High Ionization Parameter or PDR Deficit?
Yuichi Harikane, Masami Ouchi, Akio K. Inoue, Yoshiki Matsuoka, Yoichi Tamura, Tom Bakx, Seiji Fujimoto, Kana Moriwaki, Yoshiaki Ono, Tohru Nagao, Ken-ichi Tadaki, Takashi Kojima, Takatoshi Shibuya, Eiichi Egami, Andrea Ferrara, Simona Gallerani, Takuya Hashimoto, Kotaro Kohno, Yuichi Matsuda, Hiroshi Matsuo, Andrea Pallottini, Yuma Sugahara and Livia ValliniThe Astrophysical Journal 896 (2) 93 (2020)
https://doi.org/10.3847/1538-4357/ab94bd