@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20190729-091757335,
    chapter = "Elemental Source Composition Measurements and the Origin of Galactic Cosmic Rays",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20190729-091757335",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20190821-081636867,
    chapter = "SuperTIGER Abundances of Galactic Cosmic-Rays for the Charge Interval Z=41-56",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20190821-081636867",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20190821-073116292,
    chapter = "Galactic Cosmic Ray Energy Spectra for Heavy Elements (Ne to Zn) from ∼0.8 to ∼10 GeV/nuc with the SuperTIGER Instrument",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20190821-073116292",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20180828-122925735,
    chapter = "Preliminary SuperTIGER Abundances of Galactic Cosmic-Rays for the Charge Interval Z=41-56 and Prospects for SuperTIGER-2",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20180828-122925735",
    id = "record",
    doi = "10.22323/1.301.0201"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20180828-122926410,
    chapter = "Recent Results from the Cosmic Ray Isotope Spectrometer on NASA's Advanced Composition Explorer",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20180828-122926410",
    id = "record",
    doi = "10.22323/1.301.1089"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20180828-122926511,
    chapter = "Galactic Cosmic Ray Energy Spectrum for Fe from \textasciitilde 0.8 to \textasciitilde 10 GeV/nuc with the SuperTIGER Instrument",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20180828-122926511",
    id = "record",
    doi = "10.22323/1.301.0167"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20180828-122926089,
    chapter = "Abundances of Ultra-Heavy Galactic Cosmic Rays from the SuperTIGER Instrument",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20180828-122926089",
    id = "record",
    doi = "10.22323/1.236.0438"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20180828-122925525,
    chapter = "Analysis of GCR Spectra and Composition Using Penetrating Particle Data from the CRIS Instrument on ACE",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20180828-122925525",
    id = "record",
    doi = "10.22323/1.236.0340"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20180828-122925947,
    chapter = "SuperTIGER and the Origin of Galactic Cosmic-Rays",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20180828-122925947",
    id = "record",
    doi = "10.22323/1.236.0435"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20180828-122925420,
    chapter = "Galactic Cosmic-Ray Composition and Spectra for Ne through Cu from 0.8 to 10 GeV/nuc with the SuperTIGER Instrument",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20180828-122925420",
    id = "record",
    doi = "10.22323/1.236.0341"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20180828-122925311,
    chapter = "Observation of ^(60)Fe in the Galactic Cosmic Rays",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20180828-122925311",
    id = "record",
    doi = "10.22323/1.236.0275"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20180910-131321786,
    chapter = "Elemental Abundances of Ultra-Heavy GCRs measured by SuperTIGER and ACE-CRIS and the Origin of Galactic Cosmic Rays",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20180910-131321786",
    id = "record",
    doi = "10.22323/1.236.0038"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150618-091430431,
    chapter = "The Orbiting Astrophysical Spectrometer In Space (OASIS)",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150618-091430431",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150528-144715835,
    chapter = "A Comparison of ACE Measurements of Galactic Cosmic-Ray Abundances and Energy Spectra for Two Successive Solar Minima",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150528-144715835",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150506-152948443,
    chapter = "A Comparison of ACE/CRIS Measurements of Galactic
 Cosmic-Ray Abundances and Energy Spectra for Two
 Successive Solar Minima",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150506-152948443",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150528-144033949,
    chapter = "Time Dependence of Solar Modulation throughout Solar Cycle 23 as Inferred from ACE Measurements of Cosmic-Ray Energy Spectra",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150528-144033949",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150501-112031636,
    chapter = "Co/Ni Ratio Between 0.8 - 5.0 GeV/nucleon from the TIGER-2001 Flight",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150501-112031636",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150501-111243485,
    chapter = "Can ^(59)Ni Synthesized in OB Associations Decay to ^(59)Co Before Being Accelerated to Cosmic-ray Energies?",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150501-111243485",
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150415-153704362,
    chapter = "Can ^(59)Ni Synthesized in OB Associations Decay to ^(59)Co Before Being Accelerated to Cosmic-ray Energies",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150415-153704362",
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150414-113415014,
    chapter = "Measurement of the Relative Abundances of the Ultra-Heavy Galactic Cosmic Rays (30 ≤ Z ≤ 40) with TIGER",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150414-113415014",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20160722-135442634,
    chapter = "Primary and secondary contributions to arriving abundances of cosmic-ray nuclides",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20160722-135442634",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150501-113522940,
    chapter = "The P, S, Ar, and Ca isotopic composition of the galactic cosmic ray source",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150501-113522940",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150413-154918541,
    chapter = "Cosmic-ray helium intensities over the solar cycle from ACE",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150413-154918541",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150501-112052606,
    chapter = "Primary and secondary contributions to arriving abundances of cosmic x-ray nuclides",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150501-112052606",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140905-105722780,
    chapter = "The Cosmic Ray Radiation Dose in Interplanetary Space - Present Day and Worst-Case Evaluations",
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    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140902-091332874,
    chapter = "Observations of the Ultra-Heavy Galactic Cosmic-Ray Abundances (30 ≤ Z ≤ 40) with TIGER",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20140902-091332874",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150409-092051213,
    chapter = "The Level of Solar Modulation of Galactic Cosmic Rays from 1997 to 2005 as Derived from ACE Measurements of Elemental Energy Spectra",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150409-092051213",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20111004-094736990,
    title = "Physics of the outer heliosphere",
    chapter = "Cosmic-Ray Spectra in Interstellar Space",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20111004-094736990",
    id = "record",
    isbn = "0-7354-0199-3",
    doi = "10.1063/1.1809509"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150403-091555049,
    chapter = "Measurements of the Ultra-Heavy Galactic Cosmic-Ray Abundances between Z=30 and Z=40 with the TIGER Instrument",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150403-091555049",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150406-143812415,
    chapter = "Extended Energy Spectrum Measurement of Elements With the Cosmic Ray Isotope Spectrometer (CRIS)",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150406-143812415",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150406-135715114,
    chapter = "New Measurement of the Li, Be, an B Isotopes as a Test of Cosmic Ray Transport Models",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150406-135715114",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150406-141916278,
    chapter = "Direct Evidence of Energy-Loss in Electron-Capture-Decay Secondary Isotopes in the Heliosphere",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150406-141916278",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150403-093115681,
    chapter = "Possible Detection of Large Solar Particle Event at Balloon Altitudes during the 2001-2002 TIGER Flight",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150403-093115681",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20111116-133416059,
    title = "Solar and Galatic Composition",
    chapter = "GCR Neon Isotopic Abundances: Comparison with Wolf-Rayet Star Models and Meteoritic Abundances",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20111116-133416059",
    id = "record",
    isbn = "0-7354-0042-3",
    doi = "10.1063/1.1434008"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20111118-151333593,
    title = "Solar and Galactic Composition: A Joint SOHO/ACE Worshop",
    chapter = "Constraints on the nucleosynthesis of refractory nuclides in galactic cosmic rays",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20111118-151333593",
    id = "record",
    isbn = "0-7354-0042-3",
    doi = "10.1063/1.1434010"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20111118-100206530,
    title = "Solar and Galactic Composition: A Joint SOHO/ACE Workshop",
    chapter = "Measurements of the isotopes of lithium, beryllium, and boron from ACE/CRIS",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20111118-100206530",
    id = "record",
    isbn = "0-7354-0042-3",
    doi = "10.1063/1.1434007"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20111222-093454569,
    title = "Solar and Galactic Composition",
    chapter = "The cosmic-ray contribution to galactic abundances of the light elements: Interpretation of GCR LiBeB abundance measurements from ACE/CRIS",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20111222-093454569",
    id = "record",
    isbn = "0-7354-0042-3",
    doi = "10.1063/1.1434006"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150303-131355783,
    chapter = "Measurements of the Isotopes of Lithium, Beryllium, and Boron from ACE/CRIS",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150303-131355783",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150303-134629834,
    chapter = "The Isotopic Composition of Cosmic-Ray Calcium",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150303-134629834",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150302-133128195,
    chapter = "ECCO: Th/U/Pu/Cm Dating of Galactic Cosmic Ray Nuclei",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150302-133128195",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150302-133152754,
    chapter = "The Energetic Trans-Iron Composition Experiment (ENTICE) on the Heavy Nuclei Explorer (HNX) Mission",
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    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150303-135509933,
    chapter = "CRIS Measurements of Electron-Capture-Decay Isotopes: ^(37)Ar, ^(44)Ti, ^(49)V, ^(51)Cr, ^(55)Fe, and ^(57)Co",
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150302-135738779,
    chapter = "The Heavy Nuclei eXplorer (HNX) Mission",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150302-135738779",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20200506-160349946,
    title = "The Astrophysics of Galactic Cosmic Rays",
    chapter = "The Origin of Primary Cosmic Rays: Constraints from ACE Elemental and Isotopic Composition Observations",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20200506-160349946",
    id = "record",
    isbn = "9789048158621",
    doi = "10.1007/978-94-017-3239-0\_2"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:SPOaipcp00,
    title = "Acceleration and Transport of Energetic Particles Observed in the Heliosphere: ACE 2000 Symposium, Indian Wells, CA,  5-8 January 2000",
    chapter = "Co/Ni element ratio in the galactic cosmic rays between 0.8 and 4.3 GeV/nucleon",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:SPOaipcp00",
    id = "record",
    isbn = "1-56396-951-3",
    doi = "10.1063/1.1324354"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150219-131410930,
    title = "Acceleration and Transport of Energetic Particles Observed in the Heliosphere",
    chapter = "Secondary Electron-Capture-Decay Isotopes and Implications for the Propagation of Galactic Cosmic rays",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150219-131410930",
    id = "record",
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150217-140314289,
    chapter = "The Trans-Iron Galactic Element Recorder (TIGER): A Balloon-borne Cosmic-Ray Experiment",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150217-140314289",
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150217-142509052,
    chapter = "The Charge (Z) Identification Module (ZIM) for ACCESS: An Instrument Calibration using 10.6 GeV/nucleon 79AU",
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    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150217-141245529,
    chapter = "The Trans-Iron Galactic Element Recorder for the Ultra-Long Duration Balloon Project Demo 2000",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150217-141245529",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140717-162349735,
    chapter = "The Response of Particle Detectors to Gold Nuclei at 11 GeV/nucleon",
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20141022-162035331,
    chapter = "An Experiment to Measure the Elemental Abundances of Ultra-Heavy Cosmic Rays",
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140703-222609991,
    chapter = "ENergetic Trans-Iron Composition Explorer (ENTICE): A mission concept",
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    id = "record",
    doi = "10.1117/12.253969"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140505-092241472,
    chapter = "Large Isotope Spectrometer for Astromag",
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    doi = "10.1063/1.39145"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140507-141130693,
    chapter = "Cosmic Ray Elemental Abundances for 26<Z<40 Measured on HEAO-3",
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140501-111300538,
    chapter = "Energy Spectra Between 10 and Several Hundred GeV/Nucleon for Elements from \_(18)Ar to \_(23)V: Results from HEAO-3",
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140507-142235633,
    chapter = "Global Representation of the Cross Sections for the Production of Fragments of UH Nuclei",
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140507-142954825,
    chapter = "Response of Ionization Chambers and Cherenkov Counters to Relativistic Ultraheavy Nuclei",
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140501-104547780,
    chapter = "The Abundances of the Heavier Elements in the Cosmic Radiation",
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    id = "record",
    doi = "10.1063/1.38010"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140429-140516645,
    chapter = "Measurements of Ultraheavy Cosmic Rays with HEAO-3",
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140512-134901454,
    chapter = "Release of Nuclei from Relativistic Nucleus-Nucleus Interactions",
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140512-140457870,
    chapter = "Response of Ionization Chambers and Cherenkov Counters to Relativistic Ultraheavy Nuclei",
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    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140512-132135742,
    chapter = "Anisotropy of Galactic Iron of Energy 30 to 500 GeV/amu Studied by HEAO-3",
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    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140512-133126620,
    chapter = "The Abundances of Ultraheavy Elements in the Cosmic Radiation",
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    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140512-120447856,
    chapter = "Cosmic-Ray Energy Spectra Between Ten and Several Hundred GeV/amu for Elements from \_(18)Ar to \_(25)Ni--Results from HEAO-3",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20140512-120447856",
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140512-135723222,
    chapter = "The Energy Dependence of Fragmentation Cross-Sections of Relativistic Heavy Nuclei",
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    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140501-122628758,
    chapter = "Lead, Platinum, and Other Heavy Elements in the Primary Cosmic Radiation--HEAO-3 Results",
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    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140430-092247563,
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140501-131651042,
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140501-121609969,
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140430-142415830,
    chapter = "Abundances of 'secondary' elements among the ultraheavy cosmic rays: Results from HEAO-3",
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    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20190605-090230780,
    title = "Unstable Current Systems and Plasma Instabilities in Astrophysics",
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    id = "record",
    isbn = "9789027718877",
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140501-134843543,
    chapter = "Energy Spectra of Elements with 18 ≤ Z ≤ 28 Between 10 and 300 GeV/amu",
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    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140501-144334411,
    chapter = "Elemental Abundances of Cosmic Rays with Z > 33 as Measured on HEAO-3",
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140423-144626311,
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140423-143013765,
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140423-142851255,
    chapter = "The Cosmic-Ray Abundances of the Platinum-Lead Elements as Measured on HEAO-3",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20140423-142851255",
    id = "record"
}


@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140423-143205864,
    chapter = "Interactions of 200 GeV Gold Nuclei in Light Elements",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20140423-143205864",
    id = "record"
}


@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140423-144319881,
    chapter = "Correlation of Source Abundances of Ultraheavy Cosmic Rays with First Ionization Potential - Results from HEAO-3",
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    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140423-143400546,
    chapter = "Abundances of 'Secondary' Elements Among the Ultraheavy Cosmic Rays - Results from HEAO-3",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20140423-143400546",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140423-141835138,
    chapter = "Cosmic-Ray Abundances of the Even Charge Elements from \_(50)Sn to \_(58)Ce Measured on HEAO-3",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20140423-141835138",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140423-140020677,
    chapter = "Cosmic Ray Elemental Abundances for 26 ≤ Z ≤ 42 Measured on HEAO-3",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20140423-140020677",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20181115-131341372,
    title = "Origin of Cosmic Rays",
    chapter = "Heavy Nuclei Experiment on HEAO-3",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20181115-131341372",
    id = "record",
    isbn = "9789400984752",
    doi = "10.1017/s0074180900074453"
}


@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140417-151754488,
    chapter = "Abundances of Cosmic Ray Nuclei for 26 ≤ Z ≤ 40 From HEAO-3 Heavy Nuclei Experiment",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20140417-151754488",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140417-154647949,
    chapter = "Abundances of Cosmic Ray Nuclei Heavier than \_(50)Sn",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20140417-154647949",
    id = "record"
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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140417-151643116,
    chapter = "Implications of Ultraheavy Cosmic-Ray Source Composition Derived from Observations by the HEAO-3 Heavy Nuclei Experiment",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20140417-151643116",
    id = "record"
}