@article{https://resolver.caltech.edu/CaltechAUTHORS:20220908-184327219,
    title = "The Isotopic Abundances of Galactic Cosmic Rays with Atomic Number 29 ≤ Z ≤ 38",
    journal = "Astrophysical Journal",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20220908-184327219",
    id = "record",
    issn = "0004-637X",
    doi = "10.3847/1538-4357/ac82e7",
    volume = "936"
}


@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"
}


@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"
}


@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"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20180921-095050945,
    title = "Elemental Composition at the Cosmic-Ray Source Derived from the ACE-CRIS Instrument. I. \_6C to \_(28)Ni",
    journal = "Astrophysical Journal",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20180921-095050945",
    id = "record",
    issn = "1538-4357",
    doi = "10.3847/1538-4357/aad867",
    volume = "865"
}


@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"
}


@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"
}


@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"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20161104-083553694,
    title = "Galactic Cosmic Ray Origins and OB Associations: Evidence from SuperTIGER Observations of Elements \_(26)Fe through \_(40)Zr",
    journal = "Astrophysical Journal",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20161104-083553694",
    id = "record",
    issn = "0004-637X",
    doi = "10.3847/0004-637X/831/2/148",
    volume = "831"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20160422-072602817,
    title = "Observation of the ^(60)Fe nucleosynthesis-clock isotope in galactic cosmic rays",
    journal = "Science",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20160422-072602817",
    id = "record",
    issn = "0036-8075",
    doi = "10.1126/science.aad6004",
    volume = "352"
}


@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"
}


@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"
}


@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"
}


@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"
}


@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"
}


@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"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20130725-072008737,
    title = "Galactic Cosmic-Ray Energy Spectra and Composition during the 2009-2010 Solar Minimum Period",
    journal = "Astrophysical Journal",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20130725-072008737",
    id = "record",
    issn = "0004-637X",
    doi = "10.1088/0004-637X/770/2/117",
    volume = "770"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20101209-103120218,
    title = "Record-setting Cosmic-ray Intensities in 2009 and 2010",
    journal = "Astrophysical Journal Letters",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20101209-103120218",
    id = "record",
    issn = "2041-8205",
    doi = "10.1088/2041-8205/723/1/L1",
    volume = "723"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20091009-094741170,
    title = "Elemental Composition and Energy Spectra of Galactic Cosmic Rays During Solar Cycle 23",
    journal = "Astrophysical Journal",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20091009-094741170",
    id = "record",
    issn = "0004-637X",
    doi = "10.1088/0004-637X/698/2/1666",
    volume = "689"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20090826-142040089,
    title = "Cosmic Ray origin in OB Associations and Preferential Acceleration of Refractory Elements: Evidence from Abundances of Elements \_(26)Fe through \_(34)Se",
    journal = "Astrophysical Journal",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20090826-142040089",
    id = "record",
    issn = "0004-637X",
    doi = "10.1088/0004-637X/697/2/2083",
    volume = "697"
}


@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"
}


@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"
}


@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"
}


@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"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:BINnar08,
    title = "The OB association origin of galactic cosmic rays",
    journal = "New Astronomy Reviews",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:BINnar08",
    id = "record",
    issn = "1387-6473",
    doi = "10.1016/j.newar.2008.05.008",
    volume = "52"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20140827-105038224,
    title = "OB Associations, Wolf-Rayet Stars, and the Origin of Galactic Cosmic Rays",
    journal = "Space Science Reviews",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20140827-105038224",
    id = "record",
    issn = "0038-6308",
    doi = "10.1007/s11214-007-9195-1",
    volume = "130"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20100909-133903373,
    title = "An Overview of the Origin of Galactic Cosmic Rays as Inferred from Observations of Heavy Ion Composition and Spectra",
    journal = "Space Science Reviews",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20100909-133903373",
    id = "record",
    issn = "0038-6308",
    doi = "10.1007/s11214-007-9198-y",
    volume = "130"
}


@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"
}


@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"
}


@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",
    id = "record"
}


@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"
}


@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"
}


@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"
}


@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",
    id = "record"
}


@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"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:BINjpcs06,
    title = "Superbubbles, Wolf-Rayet stars, and the origin of galactic cosmic rays",
    journal = "Journal of Physics: Conference Series",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:BINjpcs06",
    id = "record",
    issn = "1742-6596",
    doi = "10.1088/1742-6596/47/1/008",
    volume = "47"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20110120-162201593,
    title = "Wolf-Rayet stars, OB associations, and the origin
 of galactic cosmic rays",
    journal = "New Astronomy Reviews",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20110120-162201593",
    id = "record",
    issn = "1387-6473",
    doi = "10.1016/j.newar.2006.06.058",
    volume = "50"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20110601-134548173,
    title = "A search for the signature of microquasars in the cosmic ray iron spectrum measured by TIGER",
    journal = "Advances in Space Research",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20110601-134548173",
    id = "record",
    issn = "0273-1177",
    doi = "10.1016/j.asr.2005.10.037",
    volume = "37"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20140827-093644016,
    title = "Cosmic-Ray Neon, Wolf-Rayet Stars, and the Superbubble Origin of Galactic Cosmic Rays",
    journal = "Astrophysical Journal",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20140827-093644016",
    id = "record",
    issn = "0004-637X",
    doi = "10.1086/496959",
    volume = "634"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20140826-114144077,
    title = "Isotopic Composition of Cosmic Rays: Results from the Cosmic Ray Isotope Spectrometer on the ACE Spacecraft",
    journal = "Nuclear Physics A",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20140826-114144077",
    id = "record",
    issn = "0375-9474",
    doi = "10.1016/j.nuclphysa.2005.05.038",
    volume = "758"
}


@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"
}


@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140905-105722780,
    chapter = "The Cosmic Ray Radiation Dose in Interplanetary Space - Present Day and Worst-Case Evaluations",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20140905-105722780",
    id = "record"
}


@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"
}


@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"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20140826-164919486,
    title = "Cosmic ray energy loss in the heliosphere: Direct evidence from electron-capture-decay secondary isotopes",
    journal = "Journal of Geophysical Research A",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20140826-164919486",
    id = "record",
    issn = "0148-0227",
    doi = "10.1029/2003JA009876",
    volume = "108"
}


@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"
}


@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"
}


@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"
}


@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"
}


@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"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20140827-082013151,
    title = "Measurement of the Secondary Radionuclides ^(10)Be, ^(26)Al, ^(36)Cl, ^(54)Mn, and ^(14)C and Implications for the Galactic Cosmic-Ray Age",
    journal = "Astrophysical Journal",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20140827-082013151",
    id = "record",
    issn = "0004-637X",
    doi = "10.1086/323842",
    volume = "563"
}


@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"
}


@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"
}


@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"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20140827-090214937,
    title = "The Origin of Primary Cosmic Rays: Constraints from ACE Elemental and Isotopic Composition Observations",
    journal = "Space Science Reviews",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20140827-090214937",
    id = "record",
    issn = "0038-6308",
    doi = "10.1023/A:1013816209004",
    volume = "99"
}


@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"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20140826-115932195,
    title = "Cosmic-ray time scales using radioactive clocks",
    journal = "Advances in Space Research",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20140826-115932195",
    id = "record",
    issn = "0273-1177",
    doi = "10.1016/S0273-1177(01)00114-4",
    volume = "27"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20140826-133307053,
    title = "Galactic cosmic ray neon isotopic abundances measured by the cosmic ray isotope spectrometer (CRIS) on ACE",
    journal = "Advances in Space Research",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20140826-133307053",
    id = "record",
    issn = "0273-1177",
    doi = "10.1016/S0273-1177(01)00119-3",
    volume = "27"
}


@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20150302-133152754,
    chapter = "The Energetic Trans-Iron Composition Experiment (ENTICE) on the Heavy Nuclei Explorer (HNX) Mission",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150302-133152754",
    id = "record"
}


@article{https://resolver.caltech.edu/CaltechAUTHORS:20140826-112434005,
    title = "The isotopic source composition of cosmic-ray iron, cobalt, and nickel",
    journal = "Advances in Space Research",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20140826-112434005",
    id = "record",
    issn = "0273-1177",
    doi = "10.1016/S0273-1177(01)00120-X",
    volume = "27"
}


@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"
}


@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"
}


@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"
}


@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"
}


@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",
    url = "https://resolver.caltech.edu/CaltechAUTHORS:20150303-135509933",
    id = "record"
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    chapter = "The Heavy Nuclei eXplorer (HNX) Mission",
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    title = "Acceleration and Transport of Energetic Particles Observed in the Heliosphere",
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    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",
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    chapter = "The Trans-Iron Galactic Element Recorder for the Ultra-Long Duration Balloon Project Demo 2000",
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    chapter = "The Trans-Iron Galactic Element Recorder (TIGER): A Balloon-borne Cosmic-Ray Experiment",
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    chapter = "The Charge (Z) Identification Module (ZIM) for ACCESS: An Instrument Calibration using 10.6 GeV/nucleon 79AU",
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    chapter = "The Response of Particle Detectors to Gold Nuclei at 11 GeV/nucleon",
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    chapter = "An Experiment to Measure the Elemental Abundances of Ultra-Heavy Cosmic Rays",
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    chapter = "ENergetic Trans-Iron Composition Explorer (ENTICE): A mission concept",
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    title = "Determination of the Cross Sections for the Production of Fragments from Relativistic Nucleus-Nucleus Interactions. Part II: Parametric Fits",
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    doi = "10.1103/PhysRevC.42.2530",
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    title = "Determination of the Cross Sections for the Production of Fragments from Relativistic Nucleus-Nucleus Interactions. Part I: Measurements",
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    issn = "0556-2813",
    doi = "10.1103/PhysRevC.42.2508",
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    chapter = "Large Isotope Spectrometer for Astromag",
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    chapter = "Response of Ionization Chambers and Cherenkov Counters to Relativistic Ultraheavy Nuclei",
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    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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    chapter = "Cosmic Ray Elemental Abundances for 26<Z<40 Measured on HEAO-3",
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    chapter = "Global Representation of the Cross Sections for the Production of Fragments of UH Nuclei",
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    title = "Abundances of ultraheavy elements in the cosmic radiation: results from HEAO 3",
    journal = "Astrophysical Journal",
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    title = "Charge, mass, and energy changes during fragmentation of relativistic nuclei",
    journal = "Physical Review C",
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    issn = "0556-2813",
    doi = "10.1103/PhysRevC.39.1785",
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    chapter = "The Abundances of the Heavier Elements in the Cosmic Radiation",
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    title = "Cosmic-ray energy spectra between 10 and several hundred GeV per atomic mass unit for elements from \_(18)Ar to \_(28)Ni - Results from HEAO 3",
    journal = "Astrophysical Journal",
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    title = "Systematics of the release of residual nuclei from relativistic nucleus-nucleus interactions",
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    id = "record",
    issn = "0556-2813",
    doi = "10.1103/PhysRevC.36.1870",
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    title = "ASTROMAG: A Superconducting Particle Astrophysics Magnet Facility for the Space Station",
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    id = "record",
    issn = "0018-9464",
    doi = "10.1109/TMAG.1987.1064905",
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    chapter = "Cosmic-Ray Energy Spectra Between Ten and Several Hundred GeV/amu for Elements from \_(18)Ar to \_(25)Ni--Results from HEAO-3",
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    chapter = "Release of Nuclei from Relativistic Nucleus-Nucleus Interactions",
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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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@inbook{https://resolver.caltech.edu/CaltechAUTHORS:20140429-140516645,
    chapter = "Measurements of Ultraheavy Cosmic Rays with HEAO-3",
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    chapter = "The Energy Dependence of Fragmentation Cross-Sections of Relativistic Heavy Nuclei",
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    chapter = "The Abundances of Ultraheavy Elements in the Cosmic Radiation",
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    title = "Lead, platinum, and other heavy elements in the primary cosmic radiation - HEAO 3 results",
    journal = "Astrophysical Journal",
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    chapter = "Implications of Source Abundances of Ultraheavy Cosmic Rays",
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    chapter = "Abundances of 'secondary' elements among the ultraheavy cosmic rays: Results from HEAO-3",
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    title = "Unstable Current Systems and Plasma Instabilities in Astrophysics",
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    chapter = "Elemental Abundances of Cosmic Rays with Z > 33 as Measured on HEAO-3",
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    title = "Elemental Abundances of Ultraheavy Cosmic Rays",
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    title = "Cosmic Ray Abundances of Sn, Te, Xe, and Ba Nuclei Measured on HEAO 3",
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    title = "Cosmic-ray abundances of Sn, Te, Xe, and BA nuclei measured on HEAO 3",
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    title = "The abundance of the actinides in the cosmic radiation as measured on HEAO 3",
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    title = "Cosmic-ray abundances of elements with atomic number 26 ≤ Z ≤ 40 measured on HEAO 3",
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    url = "https://resolver.caltech.edu/CaltechAUTHORS:20140212-075813791",
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    title = "Cosmic-Ray Abundances of Elements with Atomic Number 26 ≤ Z ≤ 40 Measured on HEAO-3",
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    url = "https://resolver.caltech.edu/CaltechAUTHORS:20140417-151939075",
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