The Mastcam-Z Radiometric Calibration Targets on NASA’s
Perseverance Rover: Derived Irradiance Time-Series, Dust Deposition, and
Performance over the First 350 Sols on Mars.
M. Merusi1, K. B. Kinch1, M. B.
Madsen1, J. F. Bell III2, J. N.
Maki3, A. G. Hayes4, J.
Joseph4, J. R. Johnson5, M.
Rice6, E. A. Cloutis7, D.
Applin7, M. T. Lemmon8, A. F.
Vaughan9, J. I. Núñez5, E.
Jensen10, J. Z. Kristensen1, K.
Paris2, E. Cisneros2, M. R.
Kennedy10, O. Gasnault11.
1Niels Bohr Institute, University of Copenhagen,
Copenhagen, Denmark
2School of Earth and Space Exploration, Arizona State
University, Tempe, AZ, USA
3Jet Propulsion Laboratory, California Institute of
Technology, Pasadena, CA, USA.
4Department of Astronomy, Cornell University, Ithaca,
NY, USA
5Johns Hopkins University Applied Physics Laboratory,
Laurel, MD, USA
6Geology Department, Western Washington University,
Bellingham, WA, USA
7Department of Geography, University of Winnipeg,
Winnipeg, Manitoba, Canada
8Space Science Institute, Boulder, CO, USA
9USGS Astrogeology Science Center, Flagstaff, AZ
10Malin Space Science Systems, San Diego, CA, USA
11Institut de Recherche en Astrophysique et
Planétologie (IRAP), Université de Toulouse, CNRS, CNES, Toulouse –
France
Corresponding author: Marco Merusi
(marco.merusi@nbi.ku.dk)