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astro-ph.SR2025
The Gothard Observatory Synthetic Stellar Photometry Database
József Kovács, Szabolcs Mészáros, Beáta Harmati +6
Context. In order to determine stellar luminosities and radii, it is necessary to know the total bolometric fluxes emitted by the stars, or equivalently the bolometric corrections…
astro-ph.SR2025
Infrared spectral signatures of light r-process elements in kilonovae
Anders Jerkstrand, Quentin Pognan, Smaranika Banerjee +8
A central question regarding neutron star mergers is whether they are able to produce all the r-process elements, from first to third peak. The high abundances of first-peak elemen…