output
20142025
most citedNew Fe I level energies and line identifications from stellar spectra

30 citations

7 papers

astro-ph.HE2025

Stellar flare detection in XMM-Newton with gradient boosted trees

Mario Pasquato, Martino Marelli, Andrea De Luca +5

The EXTraS project, based on data collected with the XMM-Newton observatory, provided us with a vast amount of light curves for X-ray sources. For each light curve, EXTraS also pro…

astro-ph.CO2025★ 3 cited

Euclid: Early Release Observations. A combined strong and weak lensing solution for Abell 2390 beyond its virial radius

J. M. Diego, G. Congedo, R. Gavazzi +183

Euclid is presently mapping the distribution of matter in the Universe in detail via the weak lensing (WL) signature of billions of distant galaxies. The WL signal is most prominen…

astro-ph.CO2025★ 2 cited

Redshift-space galaxy bispectrum in presence of massive neutrinos: A multipole expansion approach for Euclid

Sourav Pal, Debanjan Sarkar, Rickmoy Samanta +1

Massive neutrinos imprint distinctive signatures on the evolution of cosmic structures, notably suppressing small-scale clustering. We investigate the impact of massive neutrinos o…

astro-ph.GA2025★ 12 cited

Euclid: Early Release Observations -- Interplay between dwarf galaxies and their globular clusters in the Perseus galaxy cluster

T. Saifollahi, A. Lançon, Michele Cantiello +183

We present an analysis of globular clusters (GCs) of dwarf galaxies in the Perseus galaxy cluster to explore the relationship between dwarf galaxy properties and their GCs. Our foc…

astro-ph.GA2016★ 9 cited

Universe opacity and EBL

Vaclav Vavrycuk

The observed extragalactic background light (EBL) is affected by light attenuation due to absorption of light by galactic and intergalactic dust in the Universe. Even galactic opac…

astro-ph.SR2014★ 30 cited

New Fe I level energies and line identifications from stellar spectra

Ruth C. Peterson, Robert L. Kurucz

The spectrum of the Fe I atom is critical to many areas of astrophysics and beyond. Measurements of the energies of its high-lying levels remain woefully incomplete, however, despi…