collaborators

13 papers

astro-ph.CO2026

Cosmography with DESI-DR1 Cosmic Chronometers: Direct H(z) measurements from Luminous Red Galaxy ages

Carlos A. Álvarez, Marcos M. Cueli, Balakrishna S. Haridasu +6

Providing robust redshift estimates for almost 3 million luminous red galaxies (LRGs), the Dark Energy Spectroscopic Instrument (DESI) offers a unique opportunity to test the expan…

astro-ph.HE2026

The impact of stellar binaries and star cluster dynamics on pair-instability supernovae

Francesco Gabrielli, Cristiano Ugolini, Lavinia Paiella +12

Pair-instability supernovae (PISNe) are among the most luminous transients in the Universe. However, they have never been confidently observed. Solving this puzzle would have key i…

astro-ph.SR2026

Bolometric correction for cosmologically redshifted stars with dust: an update to the YBC database

Yang Chen, Xiaoting Fu, Léo Girardi +2

Observations from HST & JWST continue to reveal gravitationally magnified high-redshift star candidates, resulting in increasing demand for accurate stellar bolometric corrections…

astro-ph.GA2026

Ages of the resolved stellar populations inside the JWST/MIRI bubbles in NGC 628

Avinash Ck, Divakara Mayya, Alessandro Bressan +3

JWST images in the MIRI filters are characterized by prominent interstellar bubbles, most of which are expected to be created by mechanical energy injected into the interstellar me…

astro-ph.SR2026

The impact of envelope binding energies on the merger rate density of binary compact objects

Cecilia Sgalletta, Guglielmo Costa, Giuliano Iorio +8

The common envelope (CE) phase plays a key role in the formation of binary compact object systems. Its final outcome strongly depends on the envelope binding energy, but this quant…

astro-ph.GA2026

Impact of initial mass function on the chemical evolution of high-redshift galaxies

Boyuan Liu, Michela Mapelli, Volker Bromm +10

Recent observations by the James Webb Space Telescope (JWST) have found evidence for an invariant relation between stellar mass, metallicity, and star formation rate up to $z\sim 8…