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About BlueMUSE

BlueMUSE is an optical seeing-limited, blue-optimised, medium spectral resolution, panoramic integral-field-spectrograph, to be installed on one of the telescopes of the VLT on Cerro Paranal (Chile). The project is an evolution of the technology used on the very successful VLT / MUSE instrument, with a similar architecture and technology inovation, but with new and distinct science case enabled by its main characteristics:

  • a wavelength coverage 350 – 580 nm
  • an average spectral resolution R=4000
  • a  field-of-view higher than 1arcmin²

BlueMUSE will offer new and unique science opportunities in many fields of astrophysics, beyond those possible with MUSE. Among the science goals available with this new instrument, it will survey large sample of massive stars in our galaxy and the Local Group, study ionized nebulae, starburst and low surface-brightness galaxies. At high redshift, it would allow us for the first time to detect the IGM unambiguously in emission, as well as study the evolution of the CGM properties near the peak of the Cosmic Star formation history.


Project News

  • BlueMUSE Gate B1 meeting

    The BlueMUSE Gate B1 meeting was held from 22nd to 24th of September at the IFactory, LyonTech La Doua campus. Scientists and engineers from the entire consortium and ESO were present, enabling numerous and fruitful discussions on a broad range of topics related to the project. BlueMUSE continues to move towards the Preliminary Design Review,…

  • The BM Project Office at SPIE Conference – Copenhaguen, July 2026

                  The BlueMUSE Project Office spent last week at the SPIE Conference in Copenhagen. It was an opportunity to present the instrument’s overall architecture, as well as its technical and scientific progress. The presentations and posters from the consortium members were very well received. The event also provided a…

  • Phase B Kick-off meeting in Lyon

    We were very happy to host the BlueMUSE Phase B Kick-off meeting, which happened on February 13th, both at CRAL / Lyon Observatory and online. We shared the current progress / status since Phase A review and discussed the organisation for the next phases. The teams involved in prototyping activities also shared their progress. We…