First author Work
-
The most distant, luminous, dusty star-forming galaxies: redshifts from NOEMA and ALMA spectral scans
Y. Fudamoto, R. J. Ivison, I. Oteo, et al. 2017, MNRAS 472, 2028 -
The Dust Attenuation of Star-forming Galaxies at z∼3 and Beyond: New Insights from ALMA Observations
Y. Fudamoto, P. A. Oesch, E. Schinnerer, et al. 2017, MNRAS, 472, 483
Collaborating Work
-
Probing star formation and ISM properties using galaxy disk inclination I: Evolution in disk opacity since z~0.7
S. K. Leslie, M. T. Sargent, E. Schinnerer; ...& Y. Fudamoto, et al. 2018, A&A accepted
-
A New Constraint on Reionization by a Census of z = 7.0 Lyα Emitters with a Deep and Large Sample to 0.3 L*: Evolution of Lyα Luminosity Function and Equivalent Width at z ~ 6 - 7
K. Ota; M. Iye; N. Kashikawa; A. Konno; ... & Y. Fudamoto, et al., 2017 (arXiv: 1703.02501)
-
The ALMA spectroscopic survey in the Hubble Ultra Deep Field: Search For [CII]
Line and Dust Emission in 6 < z < 7 Galaxies
Aravena, M.; Decarli, R.; Walter, F.; ... & Y. Fudamoto, et al., 2016, ApJ, 833, 71
-
The KMOS3D Survey: Design, First Results, and the Evolution of Galaxy Kinematics from 0.7 <= z <= 2.7
Wisnioski, E.; Förster Schreiber, N. M.; Wuyts, S.; ... & Y. Fudamoto, et al., 2015, 799, 209