activity
20152025
most citedA kilonova as the electromagnetic counterpart to a gravitational-wave source

888 citations · 1.6k across the 29 of their papers we have counts for

collaborators

30 papers

astro-ph.GA2025★ 5 cited

ALMACAL XIII. Evolution of the CO luminosity function and the molecular gas mass density out to ~ 6

Victoria Bollo, Céline Péroux, Martin Zwaan +7

Cold molecular gas, largely traced by CO emission, is the primary fuel for star formation, making it essential for understanding galaxy evolution. ALMA has made significant progres…

astro-ph.GA2024

ALMACAL XII. Data characterisation and products

Victoria Bollo, Martin Zwaan, Celine Peroux +5

The ALMACAL survey is based on a database of reprocessed ALMA calibration scans suitable for scientific analysis, observed as part of regular PI observations. We present all the da…

astro-ph.HE2024

CSS161010: a luminous, fast blue optical transient with broad blueshifted hydrogen lines

Claudia P. Gutiérrez, Seppo Mattila, Peter Lundqvist +38

We present ultraviolet, optical and near-infrared photometric and optical spectroscopic observations of the luminous, fast blue optical transient (LFBOT), CSS161010:045834-081803 (…

astro-ph.GA2024★ 1 cited

METAL-Z: Measuring dust depletion in low metalicity dwarf galaxies

Aleksandra Hamanowicz, Kirill Tchernyshyov, Julia Roman-Duval +6

The cycling of metals between interstellar gas and dust is a critical aspect of the baryon cycle of galaxies, yet our understanding of this process is limited. This study focuses o…

astro-ph.GA2024

MUSE-ALMA Haloes X: The stellar masses of gas-rich absorbing galaxies

Ramona Augustin, Céline Péroux, Arjun Karki +13

The physical processes by which gas is accreted onto galaxies, transformed into stars and then expelled from galaxies are of paramount importance to galaxy evolution studies. Obser…

astro-ph.GA2023★ 7 cited

MUSE-ALMA Haloes IX: Morphologies and Stellar Properties of Gas-rich Galaxies

Arjun Karki, Varsha P. Kulkarni, Simon Weng +15

Understanding how galaxies interact with the circumgalactic medium (CGM) requires determining how galaxies morphological and stellar properties correlate with their CGM properties.…