WST -- Widefield Spectroscopic Telescope: addressing the instrumentation challenges of a new 12m class telescope dedicated to widefield Multi-object and Integral Field Spectroscopy

Fuente: arXiv
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Autori principali: Lee, David, Vernet, Joel D. R., Bacon, Roland, Jeanneau, Alexandre, Oliva, Ernesto, Brucalassi, Anna, Tozzi, Andrea, Araiza-Durán, José A., Bianco, Andrea, Kragt, Jan, Navarro, Ramon, Garilli, Bianca, Dohlen, Kjetil, Kneib, Jean-Paul, Araujo, Ricardo, Rombach, Maxime, Hernandez, Eloy, de Jong, Roelof S., Kelz, Andreas, Watson, Stephen, Louth, Tom, Bryson, Ian, George, Elizabeth, Hubin, Norbert, Bryant, Julia, Lawrence, Jon
Natura: Preprint
Pubblicazione: 2024
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author Lee, David
Vernet, Joel D. R.
Bacon, Roland
Jeanneau, Alexandre
Oliva, Ernesto
Brucalassi, Anna
Tozzi, Andrea
Araiza-Durán, José A.
Bianco, Andrea
Kragt, Jan
Navarro, Ramon
Garilli, Bianca
Dohlen, Kjetil
Kneib, Jean-Paul
Araujo, Ricardo
Rombach, Maxime
Hernandez, Eloy
de Jong, Roelof S.
Kelz, Andreas
Watson, Stephen
Louth, Tom
Bryson, Ian
George, Elizabeth
Hubin, Norbert
Bryant, Julia
Lawrence, Jon
author_facet Lee, David
Vernet, Joel D. R.
Bacon, Roland
Jeanneau, Alexandre
Oliva, Ernesto
Brucalassi, Anna
Tozzi, Andrea
Araiza-Durán, José A.
Bianco, Andrea
Kragt, Jan
Navarro, Ramon
Garilli, Bianca
Dohlen, Kjetil
Kneib, Jean-Paul
Araujo, Ricardo
Rombach, Maxime
Hernandez, Eloy
de Jong, Roelof S.
Kelz, Andreas
Watson, Stephen
Louth, Tom
Bryson, Ian
George, Elizabeth
Hubin, Norbert
Bryant, Julia
Lawrence, Jon
contents WST - Widefield Spectroscopic Telescope: We summarise the design challenges of instrumentation for a proposed 12m class Telescope that aims to provide a large (>2.5 square degree) field of view and enable simultaneous Multi-object (> 20,000 objects) and Integral Field spectroscopy (inner 3x3 arcminutes field of view), initially at visible wavelengths. For the MOS mode, instrumentation includes the fiber positioning units, fiber runs and the high (R~40,000) and low (R~3,000 - 4,000) resolution spectrographs. For the MUSE like Integral Field Spectrograph, this includes the relay from the Telescope Focal Plane, the multi-stage splitting and slicing and almost 150 identical spectrographs. We highlight the challenge of mass production at a credible cost and the issues of maintenance and sustainable operation.
format Preprint
id arxiv_https___arxiv_org_abs_2405_19198
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle WST -- Widefield Spectroscopic Telescope: addressing the instrumentation challenges of a new 12m class telescope dedicated to widefield Multi-object and Integral Field Spectroscopy
Lee, David
Vernet, Joel D. R.
Bacon, Roland
Jeanneau, Alexandre
Oliva, Ernesto
Brucalassi, Anna
Tozzi, Andrea
Araiza-Durán, José A.
Bianco, Andrea
Kragt, Jan
Navarro, Ramon
Garilli, Bianca
Dohlen, Kjetil
Kneib, Jean-Paul
Araujo, Ricardo
Rombach, Maxime
Hernandez, Eloy
de Jong, Roelof S.
Kelz, Andreas
Watson, Stephen
Louth, Tom
Bryson, Ian
George, Elizabeth
Hubin, Norbert
Bryant, Julia
Lawrence, Jon
Instrumentation and Methods for Astrophysics
WST - Widefield Spectroscopic Telescope: We summarise the design challenges of instrumentation for a proposed 12m class Telescope that aims to provide a large (>2.5 square degree) field of view and enable simultaneous Multi-object (> 20,000 objects) and Integral Field spectroscopy (inner 3x3 arcminutes field of view), initially at visible wavelengths. For the MOS mode, instrumentation includes the fiber positioning units, fiber runs and the high (R~40,000) and low (R~3,000 - 4,000) resolution spectrographs. For the MUSE like Integral Field Spectrograph, this includes the relay from the Telescope Focal Plane, the multi-stage splitting and slicing and almost 150 identical spectrographs. We highlight the challenge of mass production at a credible cost and the issues of maintenance and sustainable operation.
title WST -- Widefield Spectroscopic Telescope: addressing the instrumentation challenges of a new 12m class telescope dedicated to widefield Multi-object and Integral Field Spectroscopy
topic Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2405.19198