activity
20242026
collaborators

7 papers

astro-ph.CO2026

CORN -- Chronometers of Relic Nature I: The first estimate of the expansion rate of the Universe using compact relic galaxies

Krzysztof Lisiecki, Nicola Principi Cavaterra, Agnieszka Pollo +10

Measuring the expansion rate of the Universe is a central challenge in cosmology. Independent and robust methods are essential to validate existing measurements and assess potentia…

astro-ph.GA2026

From DES to KiDS: Domain adaptation for cross-survey detection of low-surface-brightness galaxies

Hareesh Thuruthipilly, Krzysztof Lisiecki, Junais +19

Low-surface-brightness galaxies (LSBGs) are vital for understanding galaxy formation, but their diffuse nature makes them challenging to detect. Upcoming large-scale surveys are ex…

astro-ph.GA2026

Impact of stochastic star-formation histories and dust on selecting quiescent galaxies with JWST photometry

K. Lisiecki, D. Donevski, A. W. S. Man +16

While the James Webb Space Telescope (JWST) now allows identifying quiescent galaxies (QGs) out to early epochs, the photometric selection of quiescent galaxy candidates (QGCs) and…

astro-ph.GA2026

Evolution of the infrared luminosity function and its corresponding dust-obscured star formation rate density out to z~6

M. P. Koprowski, J. V. Wijesekera, J. S. Dunlop +5

We present a new determination of the evolving far-infrared galaxy luminosity function (FIR LF) and the resulting inferred evolution of dust-obscured star-formation rate density (S…

astro-ph.GA2026

Evolution of dust attenuation in star-forming galaxies with UV slope, stellar mass, and redshift out to

J. V. Wijesekera, M. P. Koprowski, J. S. Dunlop +5

Aims. We derive a dependence of the IRX on UV slope , stellar mass , and redshift out to , and establish consistent functional relations that can be used fo…

astro-ph.GA2025

ALMA reveals diverse dust-to-gas mass ratios and quenching modes in old quiescent galaxies

Giuliano Lorenzon, Darko Donevski, Allison W. S. Man +18

Recent discoveries of dust and molecular gas in quiescent galaxies (QGs) up to challenge the long-standing view that the interstellar medium depletes rapidly once star for…