Article in Science advances, 2025. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 5 papers.
0numbers the graph read from it
0cells of the map it votes in
5citing 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.
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
33 authors.
Mariek E SchmidtDepartment of Earth Sciences, Brock University, St. Catharines, ON L2S 3A1, Canada.ORCID 0000-0003-4793-7899
Tanya V KizovskiDepartment of Earth Sciences, Brock University, St. Catharines, ON L2S 3A1, Canada.ORCID 0000-0001-8188-9769
Yang LiuJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.ORCID 0000-0003-0308-0942
Juan D Hernandez-MontenegroDivision of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA.ORCID 0000-0001-7505-4650
Michael M TiceDepartment of Geology and Geophysics, Texas A&M University, College Station, TX 77843, USA.ORCID 0000-0003-2560-1702
Allan H TreimanLunar and Planetary Institute (USRA), Houston, TX 77058, USA.ORCID 0000-0002-8073-2839
Joel A HurowitzDepartment of Geosciences, Stony Brook University, Stony Brook, NY 11794, USA.ORCID 0000-0002-5857-8652
David A KlevangTechnical University of Denmark, DTU Space, Department of Measurement and Instrumentation, Kongens Lyngby, 2800, Denmark.ORCID 0000-0001-7182-8567
Abigail L KnightMcDonnell Center for the Space Sciences, Department of Earth and Planetary Sciences, Washington University in St. Louis, St. Louis, MO 63130, USA.ORCID 0000-0001-6832-8190
Joshua LabrieDepartment of Earth Sciences, Brock University, St. Catharines, ON L2S 3A1, Canada.ORCID 0009-0005-4355-2942
Nicholas J ToscaDepartment of Earth Sciences, University of Cambridge, Cambridge CB2 3EQ, UK.ORCID 0000-0003-4415-4231
Scott J VanBommelMcDonnell Center for the Space Sciences, Department of Earth and Planetary Sciences, Washington University in St. Louis, St. Louis, MO 63130, USA.ORCID 0000-0002-6565-0827
Sophie BenaroyaDepartment of Earth and Atmospheric Sciences, University of Alberta, Edmonton, AB T6G 2E3, Canada.
Larry S CrumplerNew Mexico Museum of Natural History and Science, Albuquerque, NM 87104, USA.ORCID 0000-0002-5941-6372
Briony H N HorganEarth, Atmospheric, and Planetary Sciences, Purdue University, West Lafayette, IN 47907, USA.ORCID 0000-0001-6314-9724
Arya UdryDepartment of Geosciences, University of Nevada Las Vegas, Las Vegas, NV 89154, USA.ORCID 0000-0002-0074-8110
Anastasia YanchilinaDivision of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA.ORCID 0000-0003-3782-6343
Abigail C AllwoodJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.ORCID 0009-0002-9779-7855
Morgan L CableJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.ORCID 0000-0002-3680-302X
John R ChristianMcDonnell Center for the Space Sciences, Department of Earth and Planetary Sciences, Washington University in St. Louis, St. Louis, MO 63130, USA.ORCID 0000-0003-4646-2852
David T FlannerySchool of Earth and Atmospheric Sciences, Queensland University of Technology, Brisbane, QLD 4000, Australia.ORCID 0000-0001-8982-496X
Christopher M HeirweghJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.ORCID 0009-0002-8234-7288
Thomas L J HenleyDepartment of Earth Sciences, Brock University, St. Catharines, ON L2S 3A1, Canada.ORCID 0000-0001-9889-5313
Jesper HennekeTechnical University of Denmark, DTU Space, Department of Measurement and Instrumentation, Kongens Lyngby, 2800, Denmark.ORCID 0000-0002-3195-7417
Michael W M JonesSchool of Chemistry and Physics and Central Analytical Research Facility, Queensland University of Technology, Brisbane, QLD 4000, Australia.ORCID 0000-0002-0720-8715
Brendan J OrensteinSchool of Earth and Atmospheric Sciences, Queensland University of Technology, Brisbane, QLD 4000, Australia.ORCID 0000-0002-6586-4227
Christopher D K HerdDepartment of Earth and Atmospheric Sciences, University of Alberta, Edmonton, AB T6G 2E3, Canada.ORCID 0000-0001-5210-4002
Nicholas RandazzoDepartment of Earth and Atmospheric Sciences, University of Alberta, Edmonton, AB T6G 2E3, Canada.
David ShusterDepartment of Earth and Planetary Science, University of California, Berkeley, CA 94720-4767, USA.ORCID 0000-0003-2507-9977
Meenakshi WadhwaSchool of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA.ORCID 0000-0001-9187-1255
Funding
No grant is acknowledged in the PubMed record.
6 · The paper itself
Abstract
The Jezero crater floor features a suite of related, iron-rich lavas that were examined and sampled by the Mars 2020 rover Perseverance, and whose textures, minerals, and compositions were characterized by the Planetary Instrument for X-ray Lithochemistry (PIXL). This suite, known as the Máaz formation (fm), includes dark-toned basaltic/trachy-basaltic rocks with intergrown pyroxene, plagioclase feldspar, and altered olivine and overlying trachy-andesitic lava with reversely zoned plagioclase phenocrysts in a K-rich groundmass. Feldspar thermal disequilibrium textures indicate that they were carried from their crustal staging area. Bulk and mafic minerals have very high FeO and low MgO to FeO
Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the OpenQuestion graph.
Diverse and highly differentiated lava suite in Jezero crater, Mars: Constraints on intracrustal magmatism revealed by Mars 2020 PIXL. · full record | OpenQuestion