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20062026
most citedThe Updated BaSTI Stellar Evolution Models and Isochrones: I. Solar Scaled Calculations

352 citations · 6.6k across the 189 of their papers we have counts for

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6 papers · 1 filter

astro-ph.IM2026

WST instrument Exposure Time Calculator: full simulation of multi-mode spectrograph performance from source to detector

Matteo Ferro, Matteo Genoni, Henri M. J. Boffin +13

We present a comprehensive Exposure Time Calculator (ETC) developed for the Wide-field Spectroscopic Telescope (WST) concept. The WST, currently in its conceptual phase, is designe…

astro-ph.IM2026

HRMOS: A High-Resolution Multi-Object Spectrograph for the VLT

Laura Magrini, Thomas Bensby, Sofia Randich +174

This White Paper presents the scientific rationale and instrument concept for HRMOS (High-Resolution Multi-Object Spectrograph), a next-generation instrument proposed for the ESO V…

astro-ph.IM2024★ 2 cited

ANDES, the high resolution spectrograph for the ELT: science goals, project overview and future developments

A. Marconi, M. Abreu, V. Adibekyan +286

The first generation of ELT instruments includes an optical-infrared high-resolution spectrograph, indicated as ELT-HIRES and recently christened ANDES (ArmazoNes high Dispersion E…

astro-ph.IM2023★ 1 cited

The discovery space of ELT-ANDES. Stars and stellar populations

Ian U. Roederer, Julián D. Alvarado-Gómez, Carlos Allende Prieto +31

The ArmazoNes high Dispersion Echelle Spectrograph (ANDES) is the optical and near-infrared high-resolution echelle spectrograph envisioned for the European Extremely Large Telesco…

astro-ph.IM2015★ 51 cited

Lines and continuum sky emission in the near infrared: observational constraints from deep high spectral resolution spectra with GIANO-TNG

E. Oliva, L. Origlia, S. Scuderi +19

Aims Determining the intensity of lines and continuum airglow emission in the H-band is important for the design of faint-object infrared spectrographs. Existing spectra at low/med…

astro-ph.IM2013★ 95 cited

GALA: an automatic tool for the abundance analysis of stellar spectra

A. Mucciarelli, E. Pancino, L. Lovisi +2

GALA is a freely distributed Fortran code to derive automatically the atmospheric parameters (temperature, gravity, microturbulent velocity and overall metallicity) and abundances…