Evidence map›Paper›PMID 33380752›Full record

ReviewSpace science reviews2021

The SuperCam Instrument Suite on the NASA Mars 2020 Rover: Body Unit and Combined System Tests.

Roger C Wiens, Sylvestre Maurice, Scott H Robinson, Anthony E Nelson, Philippe Cais, Pernelle Bernardi, Raymond T Newell, Sam Clegg, Shiv K Sharma, Steven Storms and 122 more

Abstract readReview
In one paragraph

Review in Space science reviews, 2021. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 51 papers.

0numbers the graph read from it
0cells of the map it votes in
51citing papers in PubMed
–field-weighted citation impact
1 · What the graph read from it

What it found

Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.

The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

The trial behind it

Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.

Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.

3 · Its place in the literature

Who cites it

51 citing papers in PubMed.

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  15. Multi-technique characterization of iron reduction by an AntarcticApplied and environmental microbiology · 2025
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4 · The record

Corrections and comments

PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.

5 · Who and what money

Authors and funding

132 authors.

Roger C WiensLos Alamos National Laboratory, Los Alamos, NM USA.ORCID 0000-0002-3409-7344
Sylvestre MauriceInstitut de Recherche en Astrophysique et Planetologie (IRAP), Université de Toulouse, UPS, CNRS, Toulouse, France.
Scott H RobinsonLos Alamos National Laboratory, Los Alamos, NM USA.
Anthony E NelsonLos Alamos National Laboratory, Los Alamos, NM USA.
Philippe CaisLaboratoire d'astrophysique de Bordeaux, Univ. Bordeaux, CNRS, Bordeaux, France.
Pernelle BernardiLaboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris, Meudon, France.
Raymond T NewellLos Alamos National Laboratory, Los Alamos, NM USA.
Sam CleggLos Alamos National Laboratory, Los Alamos, NM USA.
Shiv K SharmaUniversity of Hawaii, Manoa, HI USA.
Steven StormsLos Alamos National Laboratory, Los Alamos, NM USA.
Jonathan DemingLos Alamos National Laboratory, Los Alamos, NM USA.
Darrel BeckmanLos Alamos National Laboratory, Los Alamos, NM USA.
Ann M OllilaLos Alamos National Laboratory, Los Alamos, NM USA.
Olivier GasnaultInstitut de Recherche en Astrophysique et Planetologie (IRAP), Université de Toulouse, UPS, CNRS, Toulouse, France.
Ryan B AndersonU.S. Geological Survey Astrogeology Science Center, Flagstaff, AZ USA.
Yves AndréCentre National d'Etudes Spatiales, Toulouse, France.
S Michael AngelUniversity of South Carolina, Columbia, SC USA.
Gorka AranaUniversity of Basque Country, UPV/EHU, Bilbao, Spain.
Elizabeth AudenLos Alamos National Laboratory, Los Alamos, NM USA.
Pierre BeckInstitut de Planétologie et d'Astrophysique de Grenoble, Université Grenoble Alpes, Grenoble, France.
Joseph BeckerLos Alamos National Laboratory, Los Alamos, NM USA.
Karim BenzeraraInstitut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS, Museum National d'Histoire Naturelle, Sorbonne Université, Paris, France.
Sylvain BernardInstitut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS, Museum National d'Histoire Naturelle, Sorbonne Université, Paris, France.
Olivier BeyssacInstitut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS, Museum National d'Histoire Naturelle, Sorbonne Université, Paris, France.
Louis BorgesLos Alamos National Laboratory, Los Alamos, NM USA.
Bruno BousquetCentre Lasers Intenses et Applications, University of Bordeaux, Bordeaux, France.
Kerry BoydLos Alamos National Laboratory, Los Alamos, NM USA.
Michael CaffreyLos Alamos National Laboratory, Los Alamos, NM USA.
Jeffrey CarlsonJet Propulsion Laboratory/Caltech, Pasadena, CA USA.
Kepa CastroUniversity of Basque Country, UPV/EHU, Bilbao, Spain.
Jorden CelisLos Alamos National Laboratory, Los Alamos, NM USA.
Baptiste ChideInstitut Supérieur de l'Aéronautique et de l'Espace (ISAE), Toulouse, France.
Kevin ClarkJet Propulsion Laboratory/Caltech, Pasadena, CA USA.
Edward CloutisUniversity of Winnipeg, Winnipeg, Canada.
Elizabeth C CordobaJet Propulsion Laboratory/Caltech, Pasadena, CA USA.
Agnes CousinInstitut de Recherche en Astrophysique et Planetologie (IRAP), Université de Toulouse, UPS, CNRS, Toulouse, France.
Magdalena DaleLos Alamos National Laboratory, Los Alamos, NM USA.
Lauren DefloresJet Propulsion Laboratory/Caltech, Pasadena, CA USA.
Dorothea DelappLos Alamos National Laboratory, Los Alamos, NM USA.
Muriel DeleuzeCentre National d'Etudes Spatiales, Toulouse, France.
Matthew DirmyerLos Alamos National Laboratory, Los Alamos, NM USA.
Christophe DonnyCentre National d'Etudes Spatiales, Toulouse, France.
Gilles DromartUniv Lyon, ENSL, Univ Lyon 1, CNRS, LGL-TPE, 69364 Lyon, France.
M George DuranLos Alamos National Laboratory, Los Alamos, NM USA.
Miles EganUniversity of Hawaii, Manoa, HI USA.
Joan ErvinJet Propulsion Laboratory/Caltech, Pasadena, CA USA.
Cecile FabreGeoRessources, Université de Lorraine, Nancy, France.
Amaury FauInstitut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS, Museum National d'Histoire Naturelle, Sorbonne Université, Paris, France.
Woodward FischerCalifornia Institute of Technology, Pasadena, CA USA.
Olivier ForniInstitut de Recherche en Astrophysique et Planetologie (IRAP), Université de Toulouse, UPS, CNRS, Toulouse, France.
Thierry FouchetLaboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris, Meudon, France.
Reuben FresquezLos Alamos National Laboratory, Los Alamos, NM USA.
Jens FrydenvangUniversity of Copenhagen, Copenhagen, Denmark.
Denine GaswayLos Alamos National Laboratory, Los Alamos, NM USA.
Ivair GontijoJet Propulsion Laboratory/Caltech, Pasadena, CA USA.
John GrotzingerCalifornia Institute of Technology, Pasadena, CA USA.
Xavier JacobInstitut de mécanique des fluides de Toulouse (CNRS, INP, Univ. Toulouse), Toulouse, France.
Sophie JacquinodLaboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris, Meudon, France.
Jeffrey R JohnsonJohns Hopkins University Applied Physics Laboratory, Laurel, MD USA.
Roberta A KlisiewiczLos Alamos National Laboratory, Los Alamos, NM USA.
James LakeLos Alamos National Laboratory, Los Alamos, NM USA.
Nina LanzaLos Alamos National Laboratory, Los Alamos, NM USA.
Javier LasernaUniversidad de Malaga, Malaga, Spain.
Jeremie LasueInstitut de Recherche en Astrophysique et Planetologie (IRAP), Université de Toulouse, UPS, CNRS, Toulouse, France.
Stéphane Le MouélicLaboratoire de Planétologie et Géodynamique, Université de Nantes, Université d'Angers, CNRS UMR 6112, Nantes, France.
Carey LegettLos Alamos National Laboratory, Los Alamos, NM USA.
Richard LeveilleMcGill University, Montreal, Canada.
Eric LewinInstitut de Planétologie et d'Astrophysique de Grenoble, Université Grenoble Alpes, Grenoble, France.
Guillermo Lopez-ReyesUniversity of Valladolid, UVA, Valladolid, Spain.
Ralph LorenzJohns Hopkins University Applied Physics Laboratory, Laurel, MD USA.
Eric LorignyCentre National d'Etudes Spatiales, Toulouse, France.
Steven P LoveLos Alamos National Laboratory, Los Alamos, NM USA.
Briana LuceroLos Alamos National Laboratory, Los Alamos, NM USA.
Juan Manuel MadariagaUniversity of Basque Country, UPV/EHU, Bilbao, Spain.
Morten MadsenUniversity of Copenhagen, Copenhagen, Denmark.
Soren MadsenJet Propulsion Laboratory/Caltech, Pasadena, CA USA.
Nicolas MangoldLaboratoire de Planétologie et Géodynamique, Université de Nantes, Université d'Angers, CNRS UMR 6112, Nantes, France.
Jose Antonio ManriqueUniversity of Valladolid, UVA, Valladolid, Spain.
J P MartinezLos Alamos National Laboratory, Los Alamos, NM USA.
Jesus Martinez-FriasAgencia Estatal Consejo Superior de Investigaciones Cientificas, Madrid, Spain.
Kevin P McCabeLos Alamos National Laboratory, Los Alamos, NM USA.
Timothy H McConnochieUniversity of Maryland, College Park, MD USA.
Justin M McGlownLos Alamos National Laboratory, Los Alamos, NM USA.
Scott M McLennanState University of New York, Stony Brook, NY USA.
Noureddine MelikechiUniversity of Massachusetts, Lowell, MA USA.
Pierre-Yves MeslinInstitut de Recherche en Astrophysique et Planetologie (IRAP), Université de Toulouse, UPS, CNRS, Toulouse, France.
John M MichelLos Alamos National Laboratory, Los Alamos, NM USA.
David MimounInstitut Supérieur de l'Aéronautique et de l'Espace (ISAE), Toulouse, France.
Anupam MisraUniversity of Hawaii, Manoa, HI USA.
Gilles MontagnacUniv Lyon, ENSL, Univ Lyon 1, CNRS, LGL-TPE, 69364 Lyon, France.
Franck MontmessinLaboratoire Atmosphères, Milieux, Observations Spatiales, Paris, France.
Valerie MoussetCentre National d'Etudes Spatiales, Toulouse, France.
Naomi MurdochInstitut Supérieur de l'Aéronautique et de l'Espace (ISAE), Toulouse, France.
Horton NewsomUniversity of New Mexico, Albuquerque, NM USA.
Logan A OttLos Alamos National Laboratory, Los Alamos, NM USA.
Zachary R OusnamerJet Propulsion Laboratory/Caltech, Pasadena, CA USA.
Laurent ParesInstitut de Recherche en Astrophysique et Planetologie (IRAP), Université de Toulouse, UPS, CNRS, Toulouse, France.
Yann ParotInstitut de Recherche en Astrophysique et Planetologie (IRAP), Université de Toulouse, UPS, CNRS, Toulouse, France.
Rafal PawluczykFiberTech Optica, Kitchener, ON Canada.
C Glen PetersonLos Alamos National Laboratory, Los Alamos, NM USA.
Paolo PilleriInstitut de Recherche en Astrophysique et Planetologie (IRAP), Université de Toulouse, UPS, CNRS, Toulouse, France.
Patrick PinetInstitut de Recherche en Astrophysique et Planetologie (IRAP), Université de Toulouse, UPS, CNRS, Toulouse, France.
Gabriel PontCentre National d'Etudes Spatiales, Toulouse, France.
Francois PouletInstitut d'Astrophysique Spatiale (IAS), Orsay, France.
Cheryl ProvostFiberTech Optica, Kitchener, ON Canada.
Benjamin QuertierLaboratoire d'astrophysique de Bordeaux, Univ. Bordeaux, CNRS, Bordeaux, France.
Heather QuinnLos Alamos National Laboratory, Los Alamos, NM USA.
William RapinInstitut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS, Museum National d'Histoire Naturelle, Sorbonne Université, Paris, France.
Jean-Michel ReessLaboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris, Meudon, France.
Amy H ReganLos Alamos National Laboratory, Los Alamos, NM USA.
Adriana L Reyes-NewellLos Alamos National Laboratory, Los Alamos, NM USA.
Philip J RomanoJet Propulsion Laboratory/Caltech, Pasadena, CA USA.
Clement RoyerInstitut d'Astrophysique Spatiale (IAS), Orsay, France.
Fernando RullUniversity of Valladolid, UVA, Valladolid, Spain.
Benigno SandovalLos Alamos National Laboratory, Los Alamos, NM USA.
Joseph H SarraoLos Alamos National Laboratory, Los Alamos, NM USA.
Violaine SautterInstitut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS, Museum National d'Histoire Naturelle, Sorbonne Université, Paris, France.
Marcel J SchoppersJet Propulsion Laboratory/Caltech, Pasadena, CA USA.
Susanne SchröderDeutsches Zentrum für Luft- und Raumfahrt (DLR), Institute of Optical Sensor Systems, Berlin, Germany.
Daniel SeitzLos Alamos National Laboratory, Los Alamos, NM USA.
Terra ShepherdLos Alamos National Laboratory, Los Alamos, NM USA.
Pablo SobronSETI Institute, Mountain View, CA USA.
Bruno DuboisUniversité de Toulouse; UPS-OMP, Toulouse, France.
Vishnu SridharJet Propulsion Laboratory/Caltech, Pasadena, CA USA.
Michael J ToplisInstitut de Recherche en Astrophysique et Planetologie (IRAP), Université de Toulouse, UPS, CNRS, Toulouse, France.
Imanol Torre-FdezUniversity of Basque Country, UPV/EHU, Bilbao, Spain.
Ian A TrettelJet Propulsion Laboratory/Caltech, Pasadena, CA USA.
Mark UnderwoodJet Propulsion Laboratory/Caltech, Pasadena, CA USA.
Andres ValdezLos Alamos National Laboratory, Los Alamos, NM USA.
Jacob ValdezLos Alamos National Laboratory, Los Alamos, NM USA.
Dawn VenhausLos Alamos National Laboratory, Los Alamos, NM USA.
Peter WillisJet Propulsion Laboratory/Caltech, Pasadena, CA USA.

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

The SuperCam instrument suite provides the Mars 2020 rover, Perseverance, with a number of versatile remote-sensing techniques that can be used at long distance as well as within the robotic-arm workspace. These include laser-induced breakdown spectroscopy (LIBS), remote time-resolved Raman and luminescence spectroscopies, and visible and infrared (VISIR; separately referred to as VIS and IR) reflectance spectroscopy. A remote micro-imager (RMI) provides high-resolution color context imaging, and a microphone can be used as a stand-alone tool for environmental studies or to determine physical properties of rocks and soils from shock waves of laser-produced plasmas. SuperCam is built in three parts: The mast unit (MU), consisting of the laser, telescope, RMI, IR spectrometer, and associated electronics, is described in a companion paper. The on-board calibration targets are described in another companion paper. Here we describe SuperCam's body unit (BU) and testing of the integrated instrument. The BU, mounted inside the rover body, receives light from the MU via a 5.8 m optical fiber. The light is split into three wavelength bands by a demultiplexer, and is routed via fiber bundles to three optical spectrometers, two of which (UV and violet; 245-340 and 385-465 nm) are crossed Czerny-Turner reflection spectrometers, nearly identical to their counterparts on ChemCam. The third is a high-efficiency transmission spectrometer containing an optical intensifier capable of gating exposures to 100 ns or longer, with variable delay times relative to the laser pulse. This spectrometer covers 535-853 nm (

Indexed as

Infrared spectroscopyJezero craterLIBSMarsMicrophone on MarsPerseverance roverRaman spectroscopySuperCam

Identifiers

PMID33380752
PMCPMC7752893

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