output
20172025
most citedA Radio Counterpart to a Neutron Star Merger

543 citations

Showing 2019Show all

72 papers · 1 filter

astro-ph.GA20199 cited

The growth of bulges and discs in relatively HI-rich galaxies: indication from HI scaling relations

Xinkai Chen, Jing Wang, Xu Kong +3

We study the relation between the properties of the bulge/disc components and the HI mass fraction of galaxies. We find that at fixed stellar mass, disc colours are correlated with…

astro-ph.CO201998 cited

First Season MWA Phase II EoR Power Spectrum Results at Redshift 7

W. Li, J. C. Pober, N. Barry +44

The compact configuration of Phase II of the Murchison Widefield Array (MWA) consists of both a redundant subarray and pseudo-random baselines, offering unique opportunities to per…

astro-ph.GA20193 cited

Spatial segregation of massive clusters in dwarf galaxies

Bruce G. Elmegreen, A. Adamo, M. Boquien +14

The relative average minimum projected separations of star clusters in the Legacy ExtraGalactic UV Survey (LEGUS) and in tidal dwarfs around the interacting galaxy NGC 5291 are det…

astro-ph.GA201946 cited

The Strength of the 2175Å Feature in the Attenuation Curves of Galaxies at 0.1<z<3

A. J. Battisti, E. da Cunha, I. Shivaei +1

We update the spectral modeling code MAGPHYS to include a 2175Å absorption feature in its UV-to-near-IR dust attenuation prescription. This allows us to determine the strength of t…

astro-ph.GA201913 cited

The role of environment in galaxy evolution in the SERVS Survey I: density maps and cluster candidates

Nick Krefting, Anna Sajina, Mark Lacy +10

We use photometric redshifts derived from new -band through 4.5m Spitzer IRAC photometry in the 4.8\,deg of the XMM-LSS field to construct surface density maps in the red…

astro-ph.GA201944 cited

X-shooter Spectroscopy and HST Imaging of 15 Ultra Massive Quiescent Galaxies at

Mikkel Stockmann, Sune Toft, Anna Gallazzi +23

We present a detailed analysis of a large sample of spectroscopically confirmed ultra-massive quiescent galaxies () at . This sam…