activity
20092026
most citedGaia Data Release 3: Processing and validation of BP/RP low-resolution spectral data

219 citations · 2.1k across the 50 of their papers we have counts for

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Showing 2024Show all

5 papers · 1 filter

astro-ph.IM2024★ 2 cited

The Survey of Surveys: machine learning for stellar parametrization

A. Turchi, E. Pancino, F. Rossi +6

We present a machine learning method to assign stellar parameters (temperature, surface gravity, metallicity) to the photometric data of large photometric surveys such as SDSS and…

astro-ph.IM2024

End-to-End simulation framework for astronomical spectrographs: SOXS, CUBES and ANDES

A. Scaudo, M. Genoni, G. Li Causi +73

We present our numerical simulation approach for the End-to-End (E2E) model applied to various astronomical spectrographs, such as SOXS (ESO-NTT), CUBES (ESO-VLT), and ANDES (ESO-E…

astro-ph.GA2024★ 6 cited

Exploring fluorine chemical evolution in the Galactic disk: the open cluster perspective

Shilpa Bijavara Seshashayana, Henrik Jönsson, Valentina D'Orazi +6

Open clusters are ideal tools for tracing the abundances of different elements because their stars are expected to have the same age, distance, and metallicity. Therefore, they ser…

astro-ph.SR2024★ 5 cited

Stellar population astrophysics (SPA) with the TNG: Measurement of the He I 10830Å line in the open cluster Stock 2

Mingjie Jian, Xiaoting Fu, Noriyuki Matsunaga +10

The precise measurement of stellar abundances plays a pivotal role in providing constraints on the chemical evolution of the Galaxy. However, before spectral lines can be employed…

astro-ph.SR2024

Stellar population astrophysics (SPA) with the TNG. Abundance analysis of nearby red giants and red clump stars: combining high resolution spectroscopy and asteroseismology

Nagaraj Vernekar, Sara Lucatello, Angela Bragaglia +4

Context: Asteroseismology, a powerful approach for obtaining internal structure and stellar properties, requires surface temperature and chemical composition information to determi…