output
20172026
most citedA Radio Counterpart to a Neutron Star Merger

543 citations

Showing 2022 · astro-ph.GAShow all

73 papers · 2 filters

astro-ph.GA202221 cited

MUSE-ALMA Haloes VII: Survey Science Goals & Design, Data Processing and Final Catalogues

Céline Péroux, Simon Weng, Arjun Karki +16

The gas cycling in the circumgalactic regions of galaxies is known to be multi-phase. The MUSE-ALMA Haloes survey gathers a large multi-wavelength observational sample of absorptio…

astro-ph.GA20229 cited

WALLABY Pilot Survey: HI gas kinematics of galaxy pairs in cluster environment

Shin-Jeong Kim, Se-Heon Oh, Jing Wang +22

We examine the HI gas kinematics of galaxy pairs in two clusters and a group using Australian Square Kilometre Array Pathfinder (ASKAP) WALLABY pilot survey observations. We compar…

astro-ph.GA202220 cited

ALMACAL IX: multi-band ALMA survey for dusty star-forming galaxies and the resolved fractions of the cosmic infrared background

Jianhang Chen, R. J. Ivison, Martin A. Zwaan +8

Wide, deep, blind continuum surveys at submillimetre/millimetre (submm/mm) wavelengths are required to provide a full inventory of the dusty, distant Universe. However, conducting…

astro-ph.GA202226 cited

Galaxy and Mass Assembly (GAMA): Extended Intra-Group Light in a group at from deep Hyper-Suprime Cam images

Cristina Martinez-Lombilla, Sarah Brough, Mireia Montes +7

We present a pilot study to assess the potential of Hyper Suprime-Cam Public Data Release 2 (HSC-PDR2) images for the analysis of extended faint structures within groups of galaxie…

astro-ph.GA202222 cited

WALLABY Pilot Survey: Public release of HI kinematic models for more than 100 galaxies from phase 1 of ASKAP pilot observations

N. Deg, K. Spekkens, T. Westmeier +29

We present the Widefield ASKAP L-band Legacy All-sky Blind surveY (WALLABY) Pilot Phase I HI kinematic models. This first data release consists of HI observations of three fields i…

astro-ph.GA202213 cited

The impact of carbon and oxygen abundances on the metal-poor initial mass function

Piyush Sharda, Anish M. Amarsi, Kathryn Grasha +5

Star formation models predict that the metal-poor initial mass function (IMF) can be substantially different from that observed in the metal-rich Milky Way. This changeover occurs…