works on

From the 1 of 6 linked papers with an AI index.

collaborators

6 papers

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

Sustainability as a design parameter in the early development of the Wide-field Spectroscopic Telescope

L. Fréour, E. Burtin, R. Bacon +13

The paper describes how sustainability is being incorporated into the early design of the Wide-field Spectroscopic Telescope by using life‑cycle assessments to evaluate the carbon…

astro-ph.IM2026

WST -- Wide-field Spectroscopic Telescope: The Next Leap in Wide-field Spectroscopy

Roland Bacon, Olga Bellido, Philippe Dierickx +53

The Wide-field Spectroscopic Telescope (WST) is a concept for a dedicated 12-m spectroscopic survey facility designed to address some of the most important questions in astrophysic…

astro-ph.IM2026

WST, the wide-field spectroscopic telescope: progress on the design of the instruments

David Lee, Joel Vernet, Elizabeth George +47

WST, the Wide-field Spectroscopic Telescope is a proposed new facility that will provide a transformational gain in spectroscopic survey capability over existing facilities. The WS…

astro-ph.IM2026

Embedding Equity, Diversity, and Inclusion in the WST Collaboration

Laurane Fréour, Anna Puglisi, Maria Cristina Fortuna +11

The proposed Wide-field Spectroscopic Telescope (WST) is a next-generation telescope facility with a 12-meter primary mirror that may be operational in the 2040s. The project has a…

astro-ph.GA2025

The differences in the Narrow Line Region of nearby QSOs 1 and 2 -- I: higher excitation and contribution of shocks in type 1's

Gabriel R. Hauschild-Roier, Thaisa Storchi-Bergmann, Rogério Riffel +1

We compare the excitation of the Narrow-Line Region (NLR) of type 1 and type 2 QSOs for redshifts via the analysis of their emission line properties in Sloan Di…