activity
20002021
most cited3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since

1.4k citations · 9.9k across the 73 of their papers we have counts for

collaborators

73 papers

astro-ph.GA2021★ 95 cited

Extending the evolution of the stellar mass-size relation at to low stellar mass galaxies from HFF and CANDELS

Kalina V. Nedkova, Boris Häußler, Danilo Marchesini +23

We reliably extend the stellar mass-size relation over to low stellar mass galaxies by combining the depth of Hubble Frontier Fields (HFF) with the large volume c…

astro-ph.GA2021★ 66 cited

Significant Dust-Obscured Star Formation in Luminous Lyman-break Galaxies at

Sander Schouws, Mauro Stefanon, Rychard J. Bouwens +13

We make use of ALMA continuum observations of luminous Lyman-break galaxies at to probe their dust-obscured star-formation. These observations are sensitive…

astro-ph.GA2021★ 163 cited

Galaxy Stellar Mass Functions from z~10 to z~6 using the Deepest Spitzer/IRAC Data: No Significant Evolution in the Stellar-to-Halo Mass Ratio of Galaxies in the First Gyr of Cosmic Time

Mauro Stefanon, Rychard J. Bouwens, Ivo Labbé +3

We present new stellar mass functions at , , , and, for the first time, , constructed from Lyman-Break galaxies previously ident…

astro-ph.GA2021★ 35 cited

Blue Rest-Frame UV-Optical Colors in z~8 Galaxies from GREATS: Very Young Stellar Populations at ~650 Myr of Cosmic Time

Mauro Stefanon, Rychard J. Bouwens, Ivo Labbé +4

Deep rest-optical observations are required to accurately constrain the stellar populations of galaxies. Due to significant limitations in the availability of such data fo…

astro-ph.GA2020★ 10 cited

MOSEL Survey: Tracking the Growth of Massive Galaxies at 2<z<4 using Kinematics and the IllustrisTNG Simulation

Anshu Gupta, Kim-Vy Tran, Jonathan Cohn +13

We use K-band spectroscopic data from the Multi-Object Spectroscopic Emission Line (MOSEL) survey to analyze the kinematic properties of galaxies at z>3. Our sample consists of 34…

astro-ph.GA2020★ 16 cited

ZFIRE: Measuring Electron Density with [OII] as a function of environment at z = 1.62

Anishya Harshan, Anshu Gupta, Kim-Vy Tran +8

The global star formation rates (SFR) of galaxies at fixed stellar masses increase with redshift and are known to vary with environment unto z~2. We explore here whether the change…