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BlueMUSE will be an optical medium spectral resolution integral-field-spectrograph to be installed on one of the telescopes of the VLT on Cerro Paranal (Chile). It will complement the MUSE instrument by offering blue-optimised performance, to be able to record data down to the atmospheric cutoff over a similar area on the sky.


Centre de Recherche Astrophysique de Lyon (CRAL); Australian Astronomical Optics; Astrophysique, Instrumentation & Modélisation (AIM), Saclay; Observatoire astronomique de l’Université de Genève; Laboratory of Astrophysics, Ecole Polytechnique Fédérale de Lausanne (EPFL); Laboratoire d’Astrophysique de Marseille (LAM); Centre for Advanced Instrumentation, Physics Department, Durham University; Department of Astronomy, Stockholm University; Institute of Astrophysics and Space Sciences

Involved AIP sections and groups:

3D and Multi Object Spectroscopy
Last update: 9. February 2021