C. Cheng

activity

20182021

most citedResolving a dusty, star-forming SHiZELS galaxy at z=2.2 with HST, ALMA and SINFONI on kiloparsec scales

38 citations · 42 across the 2 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2021★ 38 cited

Resolving a dusty, star-forming SHiZELS galaxy at z=2.2 with HST, ALMA and SINFONI on kiloparsec scales

R. K. Cochrane, P. N. Best, I. Smail +5

We present ~0.15'' spatial resolution imaging of SHiZELS-14, a massive (M*~10^11 M_sol), dusty, star-forming galaxy at z=2.24. Our rest-frame ~1kpc-scale, matched-resolution data c…

astro-ph.GA2020★ 4 cited

Cosmic evolution of molecular gas mass density from an empirical relation between $L_{1.4GHz}$ and $L_{CO}^{'}$

G. Orellana-González, E. Ibar, R. Leiton +8

Historically, GHz radio emission has been used extensively to characterize the star-formation activity in galaxies. In this work, we look for empirical relations amongst the radio…

astro-ph.GA2018

VALES V: A kinematic analysis of the molecular gas content in $H$ -ATLAS galaxies at $z \sim 0.03 - 0.35$ using ALMA

J. Molina, Edo Ibar, V. Villanueva +19

We present Atacama Large Millimeter/submillimeter Array (ALMA) resolved observations of molecular gas in galaxies up to $z = 0.35$ to characterise the role of global galactic dynamic…

Resolving a dusty, star-forming SHiZELS galaxy at z=2.2 with HST, ALMA and SINFONI on kiloparsec scales

Cosmic evolution of molecular gas mass density from an empirical relation between L1.4GHz​ and LCO′​

VALES V: A kinematic analysis of the molecular gas content in H-ATLAS galaxies at z∼0.03−0.35 using ALMA

Cosmic evolution of molecular gas mass density from an empirical relation between $L_{1.4GHz}$ and $L_{CO}^{'}$

VALES V: A kinematic analysis of the molecular gas content in $H$ -ATLAS galaxies at $z \sim 0.03 - 0.35$ using ALMA