_version_ 1866912004324720640
author Richard, Johan
Giroud, Rémi
Laurent, Florence
Krajnović, Davor
Jeanneau, Alexandre
Bacon, Roland
Abreu, Manuel
Adamo, Angela
Araujo, Ricardo
Bouché, Nicolas
Brinchmann, Jarle
Cai, Zhemin
Castro, Norberto
Calcines, Ariadna
Chapuis, Diane
Claeyssens, Adélaïde
Cortese, Luca
Daddi, Emanuele
Davison, Christopher
Goodwin, Michael
Harris, Robert
Hayes, Matthew
Jauzac, Mathilde
Kelz, Andreas
Kneib, Jean-Paul
Lanotte, Audrey A.
Lawrence, Jon
Bouteiller, Vianney Le
Breton, Rémy Le
Lehnert, Matthew
Sanchez, Angel Lopez
McGregor, Helen
McLeod, Anna F.
Monteiro, Manuel
Morris, Simon
Opitom, Cyrielle
Pécontal, Arlette
Robertson, David
Roth, Martin M.
van de Sande, Jesse
Smith, Russell
Steinmetz, Matthias
Swinbank, Mark
Urrutia, Tanya
Verhamme, Anne
Weilbacher, Peter M.
Wendt, Martin
Wildi, François
Zheng, Jessica
consortium, The BlueMUSE
author_facet Richard, Johan
Giroud, Rémi
Laurent, Florence
Krajnović, Davor
Jeanneau, Alexandre
Bacon, Roland
Abreu, Manuel
Adamo, Angela
Araujo, Ricardo
Bouché, Nicolas
Brinchmann, Jarle
Cai, Zhemin
Castro, Norberto
Calcines, Ariadna
Chapuis, Diane
Claeyssens, Adélaïde
Cortese, Luca
Daddi, Emanuele
Davison, Christopher
Goodwin, Michael
Harris, Robert
Hayes, Matthew
Jauzac, Mathilde
Kelz, Andreas
Kneib, Jean-Paul
Lanotte, Audrey A.
Lawrence, Jon
Bouteiller, Vianney Le
Breton, Rémy Le
Lehnert, Matthew
Sanchez, Angel Lopez
McGregor, Helen
McLeod, Anna F.
Monteiro, Manuel
Morris, Simon
Opitom, Cyrielle
Pécontal, Arlette
Robertson, David
Roth, Martin M.
van de Sande, Jesse
Smith, Russell
Steinmetz, Matthias
Swinbank, Mark
Urrutia, Tanya
Verhamme, Anne
Weilbacher, Peter M.
Wendt, Martin
Wildi, François
Zheng, Jessica
consortium, The BlueMUSE
contents BlueMUSE is a blue-optimised, medium spectral resolution, panoramic integral field spectrograph under development for the Very Large Telescope (VLT). With an optimised transmission down to 350 nm, spectral resolution of R$\sim$3500 on average across the wavelength range, and a large FoV (1 arcmin$^2$), BlueMUSE will open up a new range of galactic and extragalactic science cases facilitated by its specific capabilities. The BlueMUSE consortium includes 9 institutes located in 7 countries and is led by the Centre de Recherche Astrophysique de Lyon (CRAL). The BlueMUSE project development is currently in Phase A, with an expected first light at the VLT in 2031. We introduce here the Top Level Requirements (TLRs) derived from the main science cases, and then present an overview of the BlueMUSE system and its subsystems fulfilling these TLRs. We specifically emphasize the tradeoffs that are made and the key distinctions compared to the MUSE instrument, upon which the system architecture is built.
format Preprint
id arxiv_https___arxiv_org_abs_2406_13914
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle The Blue Multi Unit Spectroscopic Explorer (BlueMUSE) on the VLT: science drivers and overview of instrument design
Richard, Johan
Giroud, Rémi
Laurent, Florence
Krajnović, Davor
Jeanneau, Alexandre
Bacon, Roland
Abreu, Manuel
Adamo, Angela
Araujo, Ricardo
Bouché, Nicolas
Brinchmann, Jarle
Cai, Zhemin
Castro, Norberto
Calcines, Ariadna
Chapuis, Diane
Claeyssens, Adélaïde
Cortese, Luca
Daddi, Emanuele
Davison, Christopher
Goodwin, Michael
Harris, Robert
Hayes, Matthew
Jauzac, Mathilde
Kelz, Andreas
Kneib, Jean-Paul
Lanotte, Audrey A.
Lawrence, Jon
Bouteiller, Vianney Le
Breton, Rémy Le
Lehnert, Matthew
Sanchez, Angel Lopez
McGregor, Helen
McLeod, Anna F.
Monteiro, Manuel
Morris, Simon
Opitom, Cyrielle
Pécontal, Arlette
Robertson, David
Roth, Martin M.
van de Sande, Jesse
Smith, Russell
Steinmetz, Matthias
Swinbank, Mark
Urrutia, Tanya
Verhamme, Anne
Weilbacher, Peter M.
Wendt, Martin
Wildi, François
Zheng, Jessica
consortium, The BlueMUSE
Instrumentation and Methods for Astrophysics
Astrophysics of Galaxies
BlueMUSE is a blue-optimised, medium spectral resolution, panoramic integral field spectrograph under development for the Very Large Telescope (VLT). With an optimised transmission down to 350 nm, spectral resolution of R$\sim$3500 on average across the wavelength range, and a large FoV (1 arcmin$^2$), BlueMUSE will open up a new range of galactic and extragalactic science cases facilitated by its specific capabilities. The BlueMUSE consortium includes 9 institutes located in 7 countries and is led by the Centre de Recherche Astrophysique de Lyon (CRAL). The BlueMUSE project development is currently in Phase A, with an expected first light at the VLT in 2031. We introduce here the Top Level Requirements (TLRs) derived from the main science cases, and then present an overview of the BlueMUSE system and its subsystems fulfilling these TLRs. We specifically emphasize the tradeoffs that are made and the key distinctions compared to the MUSE instrument, upon which the system architecture is built.
title The Blue Multi Unit Spectroscopic Explorer (BlueMUSE) on the VLT: science drivers and overview of instrument design
topic Instrumentation and Methods for Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2406.13914