activity
20142024
most citedThe SAMI Galaxy Survey: instrument specification and target selection

506 citations · 2.9k across the 47 of their papers we have counts for

collaborators

46 papers

astro-ph.GA2024

ALESS-JWST: Joint (sub-)kiloparsec JWST and ALMA imaging of submillimeter galaxies reveals heavily obscured bulge formation events

Jacqueline A. Hodge, Elisabete da Cunha, Sarah Kendrew +25

We present JWST NIRCam imaging targeting 13 infrared-luminous () galaxies from the ALESS survey with uniquely deep, high-resolution…

astro-ph.GA2023★ 18 cited

Radio spectral properties of star-forming galaxies between 150-5000MHz in the ELAIS-N1 field

Fangxia An, M. Vaccari, P. N. Best +9

By combining high-sensitivity LOFAR 150MHz, uGMRT 400MHz and 1,250MHz, GMRT 610MHz, and VLA 5GHz data in the ELAIS-N1 field, we study the radio spectral properties of radio-detecte…

astro-ph.GA2023★ 9 cited

Exploring the Intrinsic Scatter of the Star-Forming Galaxy Main Sequence at redshift 0.5 to 3.0

Rongjun Huang, Andrew J. Battisti, Kathryn Grasha +4

Previous studies have shown that the normalization and scatter of the galaxy 'main sequence' (MS), the relation between star formation rate (SFR) and stellar mass (), evolves…

astro-ph.GA2022★ 16 cited

Morphology & Environment's Role on the Star Formation Rate -- Stellar Mass Relation in COSMOS from 0 < z < 3.5

Kevin C. Cooke, Jeyhan S. Kartaltepe, Caitlin Rose +6

We investigate the relationship between environment, morphology, and the star formation rate -- stellar mass relation derived from a sample of star-forming galaxies (commonly refer…

astro-ph.GA2022★ 34 cited

LoTSS Jellyfish Galaxies IV: Enhanced Star Formation on the Leading Half of Cluster Galaxies and Gas Compression in IC3949

Ian D. Roberts, Maojin Lang, Daria Trotsenko +7

With MaNGA integral field spectroscopy, we present a resolved analysis of star formation for 29 jellyfish galaxies in nearby clusters, identified from radio continuum imaging taken…

astro-ph.GA2022★ 29 cited

COSMOS2020: Manifold Learning to Estimate Physical Parameters in Large Galaxy Surveys

I. Davidzon, K. Jegatheesan, O. Ilbert +16

We present a novel method to estimate galaxy physical properties from spectral energy distributions (SEDs), alternate to template fitting techniques and based on self-organizing ma…