Y. Fudamoto

activity

20142026

most citedThe KMOS^3D Survey: design, first results, and the evolution of galaxy kinematics from 0.7<z<2.7

597 citations · 5.5k across the 150 of their papers we have counts for

collaborators

Showing 2017Show all

3 papers · 1 filter

astro-ph.GA2017★ 70 cited

The most distant, luminous, dusty star-forming galaxies: redshifts from NOEMA and ALMA spectral scans

Y. Fudamoto, R. J. Ivison, I. Oteo +23

We present 1.3- and/or 3-mm continuum images and 3-mm spectral scans, obtained using NOEMA and ALMA, of 21 distant, dusty, star-forming galaxies (DSFGs). Our sample is a subset of…

astro-ph.GA2017★ 61 cited

The Dust Attenuation of Star-forming Galaxies at $z \sim 3$ and Beyond: New Insights from ALMA Observations

Yoshinobu Fudamoto, Pascal A. Oesch, Eva Schinnerer +10

We present results on the dust attenuation of galaxies at redshift $\sim 3 - 6$ by studying the relationship between the UV spectral slope ( $β_{UV}$ ) and the infrared excess (IRX;…

astro-ph.GA2017★ 80 cited

A New Constraint on Reionization from Evolution of the Ly $α$ Luminosity Function at $z \sim 6 - 7$ Probed by a Deep Census of $z = 7.0$ Ly $α$ Emitter Candidates to 0.3 $L^{*}$

Kazuaki Ota, Masanori Iye, Nobunari Kashikawa +10

We detect 20 $z = 7.0$ Ly $α$ emitter (LAE) candidates to $L (Ly α) \geq 2 \times 1 0^{42}$ erg s $^{- 1}$ or $0.3$ $L_{z = 7}^{*}$ and in $6.1 \times 1 0^{5}$ Mpc $^{3}$ volume in the Subaru D…

The most distant, luminous, dusty star-forming galaxies: redshifts from NOEMA and ALMA spectral scans

The Dust Attenuation of Star-forming Galaxies at z∼3 and Beyond: New Insights from ALMA Observations

A New Constraint on Reionization from Evolution of the Lyα Luminosity Function at z∼6−7 Probed by a Deep Census of z=7.0 Lyα Emitter Candidates to 0.3 L∗

The Dust Attenuation of Star-forming Galaxies at $z \sim 3$ and Beyond: New Insights from ALMA Observations

A New Constraint on Reionization from Evolution of the Ly $α$ Luminosity Function at $z \sim 6 - 7$ Probed by a Deep Census of $z = 7.0$ Ly $α$ Emitter Candidates to 0.3 $L^{*}$