activity
20242026
collaborators

5 papers

astro-ph.GA2026

The ALMA carbon monoxide supernova (ACOS) survey II. Turbulent giant molecular clouds at the positions of core-collapse supernovae

M. Solar, M. J. Michałowski, J. Nadolny +11

Context. Study of cold molecular hydrogen gas (hereafter molecular gas) provides crucial insights into its interplay with star-forming regions. However, the connection between mole…

astro-ph.GA2026

Atomic gas properties at the positions of supernovae Type Ia, II, and Ib/c

Bruno Šlaus, Natalia Gotkiewicz, Michał J. Michałowski +6

Understanding which stars explode as which type of supernovae (SNe) is crucial to measure their contribution to the metal production and feedback halting star formation. Most of th…

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.HE2025

Early Light Curve Excess in Type IIb Supernovae Observed by the ATLAS Survey: Qualitative Constraints on Progenitor Systems

Bastian Ayala, Joseph P. Anderson, G. Pignata +8

Type IIb supernovae (SNe IIb) often exhibit an early light curve excess (EE) preceding the main peak powered by radioactive nickel decay. The physical origin of this early emission…

astro-ph.GA2024

Evolution of the star formation rate surface density main sequence. Insights from a semi-analytic simulation since

Jakub Nadolny, Michał J. Michałowski, Massimiliano Parente +4

Recent high-redshift () spatially resolved observations with the James Webb Space Telesescope have shown the evolution of the star formation rate (SFR) surface density ($Σ_{\…