CHONDRITES: MAGNETIC SUSCEPTIBILITY AND TYPE II CHONDRULE OLIVINE Cr2O3 CONTENTS AND THEIR IMPLICATIONS FOR PAIRING. K. Righter, H. Busemann, L. M. Eckart, C. Alexander, J. Schutt, R. Harvey, and J. Karner, Mailcode XI2, NASA Johnson Space Center, 2101 NASA Pkwy, Houston, TX, 77058, USA, ETH Zürich, Inst. Geochem. Petrol, Clausiusstrasse 25, 8092 Zürich, Switzerland; Earth and Planets Laboratory, Carnegie Institution for Science, 5241 Broad Branch Road, NW, Washington, DC 20015-1305; 4 EEPS, Case Western Reserve University, Cleveland, OH 44106; Geology & Geophysics, University of Utah, Salt Lake City UT 84112.

SURVEY OF DOMINION RANGE (DOM) AND MILLER RANGE (MIL) CO3 CARBONACEOUS CHONDRITES: MAGNETIC SUSCEPTIBILITY AND TYPE II CHONDRULE OLIVINE Cr2O3 CONTENTS AND THEIR IMPLICATIONS FOR PAIRING

Benjamin Schrunk*, Yevhen Kushnirenko*, 2 Brinda Kuthanazhi, 2 Junyeong Ahn, Lin-Lin Wang, Evan O’Leary, 2 Kyungchan Lee, 2 Andrew Eaton, 2 Alexander Fedorov, 5 Rui Lou, 4 Vladimir Voroshnin, Oliver J. Clark, Jaime Sánchez-Barriga, Sergey L. Bud’ko, 2 Robert-Jan Slager, 7, ∗ Paul C. Canfield, 2, † and Adam Kaminski 2, ‡ Ames Laboratory, Ames, Iowa 50011, USA Department of Physics and Astronomy, Iowa State University, Ames, Iowa 50011, USA Department of Physics, Harvard University, Cambridge MA 02138, USA Leibniz Institute for Solid State and Materials Research, 01069 Dresden, Germany Helmholtz-Zentrum Berlin für Materialien und Energie, Berlin, Germany School of Physical Science and Technology, Lanzhou University, Lanzhou 730000, China TCM Group, Cavendish Laboratory, University of Cambridge, Cambridge CB3 0HE, United Kingdom

Emergence of Fermi arcs and novel magnetic splitting in an antiferromagnet

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SURVEY OF DOMINION RANGE (DOM) AND MILLER RANGE (MIL) CO3 CARBONACEOUS CHONDRITES: MAGNETIC SUSCEPTIBILITY AND TYPE II CHONDRULE OLIVINE Cr2O3 CONTENTS AND THEIR IMPLICATIONS FOR PAIRING

Emergence of Fermi arcs and novel magnetic splitting in an antiferromagnet