Publications

Introductory papers:

• Probing the Physics of the Solar Atmosphere with the MUlti-slit Solar Explorer (MUSE). I. Coronal Heating, De Pontieu B. et al., ApJ, 926, 52 (2022)
• Probing the Physics of the Solar Atmosphere with the MUlti-slit Solar Explorer (MUSE). II. Flares and Eruptions, Cheung M. et al., ApJ, 926, 53 (2022)
• The Multi-slit Approach to Coronal Spectroscopy with the MUlti-slit Solar Explorer (MUSE), De Pontieu et al., ApJ, 888, 3 (2020)
• Multi-component Decomposition of Astronomical Spectra by Compressed Sensing, Cheung, M. et al., ApJ, 882, 13 (2019)

List of MUSE-related papers: https://ui.adsabs.harvard.edu/public-libraries/UJdBqdzhT6OK4_uOqONu1A

ADS Link to track a broader MUSE relevant references (papers mentioning MUSE): https://ui.adsabs.harvard.edu/search/q=(full%3A%22Multi-slit.Solar.Explorer%22)&sort=date%20desc%2C%20bibcode%20desc&p_=0

When writing a paper about MUSE, please include the following statement in the acknowledgements:

MUSE is led by the Lockheed Martin Solar and Astrophysics Laboratory of Palo Alto, California. MUSE is managed by the Explorer’s Program Office of NASA’s Goddard Space Flight Center in Greenbelt, Maryland, for the Heliophysics Division of NASA’s Science Mission Directorate. Lockheed Martin Advanced Technology Center, along with partner institutions, builds the MUSE instrument and spacecraft and University of California, Berkeley provides the mission operations center. MUSE benefits from international contributions supported by the Norwegian Space Agency (NOSA), the Italian Space Agency (ASI), the German Space Agency at DLR, and from the Max Planck Institute for Solar System Research (MPS).