REVIEW 2 major objections 5 minor 171 references
The High-Energy Light Isotope eXperiment (HELIX) Instrument
T0 review · 2 major / 5 minor · reviewed 2026-08-01 · deepseek-v4-flash
Pith's one-line read A balloon-borne instrument claims to identify cosmic-ray isotopes event by event by combining charge, rigidity, and velocity measurements.
desk verdict HELIX instrument paper is detailed, honest, and worth refereeing; the high-energy isotope separation at >1 GeV/n is still a design target, not a demonstrated result. read the letter →
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
The reading
What carries the argument
The mass relation m = RZe/(γβc²) is the identity that carries the argument: it converts three separately measured quantities—charge, rigidity, and velocity—into a per-particle mass. The drift-chamber tracker in the 1-T magnet supplies R, the ToF scintillators supply Z and low-energy β, and the RICH supplies high-energy β; the fiber hodoscope sharpens the RICH ring center by improving the non-bending-plane track extrapolation.
What would settle it
A flight measurement of the reconstructed mass spectrum for beryllium that shows no separation between the 9Be and 10Be peaks at 3 GeV/n—meaning a mass resolution worse than the design target of 2.5%—would refute the central claim. This could be checked directly in existing 2024 flight data by examining Cherenkov-angle residuals for beryllium candidates.
Extended reading notes
Core claim
The central claim is that event-by-event isotope identification of light cosmic-ray nuclei is achievable with the HELIX configuration. By measuring charge with the ToF detectors and combining rigidity from the tracker with velocity from ToF (low energy) or RICH (high energy), the mass follows from m = RZe/(γβc²). The paper presents the hardware designed to realize this, including a jet-chamber drift tracker with roughly 70-micron spatial resolution, ToF timing on track for 50 ps for beryllium, and an aerogel RICH whose refractive index is calibrated to Δn/n ≈ 7×10⁻⁴. Preliminary flight data show the subsystems performing near their design targets, with the RICH dark rate controlled by timing
Load-bearing premise
The high-energy RICH velocity measurement must be precise enough to separate 9Be from 10Be; that requires knowing the aerogel refractive index to about 7 parts in 10,000 and keeping the focal plane dark rate low, and the 2024 flight showed the cooling system could not yet maintain the required temperature.
Editorial extensions
If this is right
- If the design performance holds, HELIX will deliver the first 10Be/9Be measurement spanning roughly 0.2 to 3+ GeV/n, a regime that discriminates among cosmic-ray propagation models.
- Event-by-event mass reconstruction means isotopic ratios can be measured without relying on unfolding of broad spectra.
- The open magnet geometry, with only about 2 g/cm² of upstream material, minimizes fragmentation of incident nuclei before rigidity measurement, preserving the isotopic signal.
- The engineering flight validated the magnet hold time (about 5.2 days), trigger logic, and DAQ; planned upgrades for the Antarctic flight address RICH cooling and other lessons.
- The NaF corner tiles provide an in-flight cross-calibration between RICH and ToF, tying the two velocity scales together.
Reading between the lines
- The same measurement chain could be pushed to higher energies if the RICH radiator index uniformity and focal-plane dark rate improve; the limiting factor is velocity resolution, not rigidity.
- A precise 10Be/9Be ratio at the high end of the range would test the assumption that cosmic-ray transport is energy-independent, since 10Be decay acts as a clock that depends on propagation time.
- The timing-cut method demonstrated to suppress RICH dark count could be refined or combined with a second Cherenkov radiator to extend separation to heavier isotopes such as 26Al/27Al.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper describes the High-Energy Light Isotope eXperiment (HELIX), a balloon-borne instrument designed to measure light cosmic-ray isotopes (Z < 11). It provides detailed engineering descriptions of the superconducting magnet, drift-chamber tracker, time-of-flight system, ring-imaging Cherenkov detector, hodoscope, and the trigger/data-acquisition/power systems, together with preliminary results from a six-day 2024 engineering flight. The stated goal is event-by-event reconstruction of mass, charge, and rigidity for isotopes from ~0.2 GeV/n to beyond 3 GeV/n, with the primary science objective of measuring the 10Be/9Be flux ratio.
Significance. If the instrument meets its design goals, HELIX will provide a valuable high-energy measurement of 10Be/9Be, a key observable for cosmic-ray propagation models. The paper's strengths are its thorough engineering documentation, clear articulation of design targets, and transparent discussion of unresolved challenges, particularly the RICH cooling insufficiency and the resulting dark-rate problem. It also presents falsifiable predictions, such as the 50 ps ToF resolution for Be and the 2.5% mass resolution at 3 GeV/n, which future flights can test. The preliminary flight data validate several subsystems, including tracker hit resolution, SiPM gain stability, and trigger performance. However, the end-to-end mass resolution, especially the RICH high-energy velocity resolution, is not yet demonstrated; this is an acknowledged risk rather than an internal inconsistency. As an instrument description, the paper is a useful and appropriate contribution.
major comments (2)
- [Sec. 6.3 / Abstract] The abstract states that HELIX allows 'event-by-event reconstruction of primary particle mass, charge, and magnetic rigidity.' This is a load-bearing claim, but it is not yet supported by demonstrated performance. The RICH, which provides velocity above ~1 GeV/n, requires refractive-index knowledge to Δn/n ≈ 7×10^-4 and a focal plane with manageable dark rate (Sec. 6.3). The paper reports that tile surfaces and refractive indices were measured, but it does not report the achieved absolute index uncertainty or any measured Cherenkov-angle/mass resolution from the 2024 flight. The cooling insufficiency (Sec. 6.2) caused elevated dark rates; the timing cut in Fig. 15 reveals candidate rings but no quantitative efficiency or resolution is given. I recommend either reporting the achieved index uncertainty and any beam-test-derived angular resolution (from Ref. [10]), or explicitly limiting th
- [Sec. 5.2 / Sec. 4.6] Similar to the RICH point, the ToF timing for Be is quoted as 'expected to reach a level better than the design target of 50 ps,' while the current muon transit timing is ~200 ps. The DCT section reports an expected diffusion-limited resolution but no measured rigidity resolution. Because the mass resolution at all energies depends on the product of rigidity and velocity resolutions, the paper should make clear in a summary paragraph or table which quantities are measured (e.g., charge resolution, single-hit resolution) and which are design expectations. This would prevent the reader from inferring that the full isotope-identification capability has already been demonstrated.
minor comments (5)
- [Sec. 1] The symbol γ in the mass formula is not defined; please define γ = 1/sqrt(1-β²) for clarity.
- [Sec. 8.2] The trigger terms 'ZHi' and 'ZLo' are used without definition; it would be helpful to state that they refer to high- and low-charge-threshold triggers.
- [Fig. 15] The color scales differ across the four panels; a common scale or explicit color-bar labels would aid comparison of the timing-cut effect.
- [Sec. 6.2] The sentence about the insufficient cooling system could be strengthened by giving the focal-plane temperature range encountered in flight, if available, to quantify the dark-rate impact.
- [Sec. 8.4] The description of downlinked randomly selected events could mention whether these events are used for real-time monitoring or for post-flight science analysis.
Circularity Check
No circularity: HELIX is an instrument description whose physics relations are standard and whose cited prior work supplies external calibration data, not fitted predictions.
full rationale
The paper is a detector description, not a derivation of physical results. The central identification formula m = RZe/(gamma beta c^2) is standard kinematics, and the Cherenkov relation is likewise textbook physics; neither is derived from fitted data. The only quantitative performance claims (e.g., 2.5% mass resolution at 3 GeV/n requiring Delta n/n ~ 7e-4) are stated as design requirements, not as demonstrated predictions. The aerogel refractive-index measurements are reported as performed with an electron beam, with details cited to a separate calibration paper [10] by overlapping authors; that citation supplies external measurement data rather than importing the paper's own conclusions. The 2024 flight results shown (timing ramps, SiPM gain, RICH ring candidates) are illustrative performance checks, not predictions claimed to be validated. The acknowledged cooling insufficiency and higher dark rate are openly stated performance limitations, and the paper does not claim to have achieved the high-energy mass resolution. Self-citations to prior HELIX design/calibration work are load-bearing only in the sense of referencing hardware development and calibration procedures, which are independent of any claimed derivation. No step in the manuscript reduces by construction to its inputs, and no fitted parameter is renamed as a prediction. Hence the circularity score is 0.
Assumptions & free parameters
assumptions (2)
- standard math Lorentz force and relativistic mass formula m = RZe/(γβc²) relate measured rigidity, velocity, and charge to particle mass.
- standard math Cherenkov radiation relation cos θ_c = 1/(nβ) and the known ring geometry convert measured ring radii into particle velocity.
Cite this review
Pith. "Pith review of The High-Energy Light Isotope eXperiment (HELIX) Instrument." pith.science (2026). https://pith.science/paper/BRRBAKNL
@misc{pith2026260720774,
author = {Pith},
title = {Pith review of: The High-Energy Light Isotope eXperiment (HELIX) Instrument},
year = {2026},
howpublished = {\url{https://pith.science/paper/BRRBAKNL}},
note = {Machine review of arXiv:2607.20774}
}
read the original abstract
The HELIX detector is a balloon-borne instrument designed to measure the flux of light (Z < 11) cosmic-ray isotopes. In this paper we describe the initial configuration of HELIX, optimized for measurements in the energy range from approximately 0.2 GeV per nucleon to beyond 3 GeV per nucleon. In addition to a spectrometer, which is based on a one-tesla superconducting magnet and a drift-chamber tracker, HELIX employs scintillator-based time-of-flight counters and a ring-imaging Cherenkov detector, allowing event-by-event reconstruction of primary particle mass, charge, and magnetic rigidity.
Figures
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Reference graph
Works this paper leans on
-
[10]
Billauer, Eli , title =
-
[1]
and others , series =
Ambrosi, G. and others , series =. In-flight operations and efficiency of the AMS-02 silicon tracker , year =
-
[2]
and others , series =
Oliva, A. and others , series =. The AMS-02 Silicon Tracker: Status and Performance Results , year =
-
[3]
36th International Cosmic Ray Conference (ICRC2019) , year = 2019, series =
Cosmic-ray Isotope Measurements with HELIX. 36th International Cosmic Ray Conference (ICRC2019) , year = 2019, series =. doi:10.22323/1.358.0121 , adsurl =
-
[4]
Nuclear Instruments and Methods in Physics Research , year = 1982, month = may, volume =
The jet-chamber of the JADE experiment. Nuclear Instruments and Methods in Physics Research , year = 1982, month = may, volume =. doi:10.1016/0029-554X(82)90658-9 , adsurl =
-
[5]
R.D. Heuer and A. Wagner , title =. Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment , volume =. 1988 , issn =. doi:https://doi.org/10.1016/0168-9002(88)91050-9 , url =
-
[6]
Nuclear Instruments and Methods in Physics Research A , keywords =
Developing a silica aerogel radiator for the HELIX ring-imaging Cherenkov system. Nuclear Instruments and Methods in Physics Research A , keywords =. doi:10.1016/j.nima.2019.02.006 , archivePrefix =. 1901.06663 , primaryClass =
arXiv 2019
-
[7]
Journal of Supercritical Fluids , keywords =
Large area silica aerogel for use as Cherenkov radiators with high refractive index, developed by supercritical carbon dioxide drying. Journal of Supercritical Fluids , keywords =. doi:10.1016/j.supflu.2015.11.022 , archivePrefix =. 1701.00143 , primaryClass =
arXiv 2015
Show all 171 references
-
[8]
Nuclear Instruments and Methods in Physics Research A , keywords =
Electron-beam calibration of aerogel tiles for the HELIX RICH detector. Nuclear Instruments and Methods in Physics Research A , keywords =. doi:10.1016/j.nima.2023.168549 , archivePrefix =. 2307.09689 , primaryClass =
2023
-
[9]
and others , title =
Fleury, J. and others , title =. Journal of Instrumentation , volume =. 2014 , doi =
2014
-
[11]
Nuclear Instruments and Methods in Physics Research A , keywords =
The DAMPE silicon-tungsten tracker. Nuclear Instruments and Methods in Physics Research A , keywords =. doi:10.1016/j.nima.2016.02.077 , adsurl =
2016 doi
-
[12]
, series =
Wakely, S.P. , series =. Galactic Cosmic Rays: Measurements, Models and Methods (Rapporteur Talk) , year =
-
[13]
2021 , author =
Cosmic-Ray Lithium and Beryllium Isotopes with AMS02. 2021 , author =
2021
-
[14]
, keywords =
Measurement of the Abundance of Radioactive ^ 10 Be and Other Light Isotopes in Cosmic Radiation up to 2 GeV Nucleon ^ -1 with the Balloon-borne Instrument ISOMAX. , keywords =. doi:10.1086/422384 , adsurl =
-
[15]
Nuclear Instruments and Methods in Physics Research A , year = 2000, month = nov, volume = 454, pages =
ISOMAX: a balloon-borne instrument to measure cosmic ray isotopes. Nuclear Instruments and Methods in Physics Research A , year = 2000, month = nov, volume = 454, pages =. doi:10.1016/S0168-9002(00)00823-8 , adsurl =
-
[16]
, keywords =
Measurement of the Isotopic Composition of Cosmic-Ray Helium, Lithium, Beryllium, and Boron up to 1700 MEV per Atomic Mass Unit. , keywords =. doi:10.1086/308762 , adsurl =
-
[17]
, keywords =
A measurement of cosmic-ray beryllium isotopes from 200 to 1500 MeV per nucleon. , keywords =. doi:10.1086/156616 , adsurl =
-
[18]
, keywords =
Galactic Cosmic-Ray Confinement Time: ULYSSES High Energy Telescope Measurements of the Secondary Radionuclide 10Be. , keywords =. doi:10.1086/311437 , adsurl =
-
[19]
, keywords =
Charge composition and energy spectra of cosmic-ray nuclei for elements from Be to NI - Results from HEAO-3-C2. , keywords =
-
[20]
, archivePrefix = "arXiv", eprint =
Recovering the Observed B/C Ratio in a Dynamic Spiral-armed Cosmic Ray Model. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/782/1/34 , adsurl =
-
[21]
Physical Review Letters , archivePrefix = "arXiv", eprint =
AMS-02 Results Support the Secondary Origin of Cosmic Ray Positrons. Physical Review Letters , archivePrefix = "arXiv", eprint =. doi:10.1103/PhysRevLett.111.211101 , adsurl =
-
[22]
ArXiv e-prints , archivePrefix = "arXiv", eprint =
Cosmic Frontier Indirect Dark Matter Detection Working Group Summary. ArXiv e-prints , archivePrefix = "arXiv", eprint =
-
[23]
, archivePrefix = "arXiv", eprint =
Galactic electrons and positrons at the Earth: new estimate of the primary and secondary fluxes. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201014225 , adsurl =
-
[24]
, archivePrefix = "arXiv", eprint =
Dark matter and pulsar origins of the rising cosmic ray positron fraction in light of new data from AMS. , archivePrefix = "arXiv", eprint =. doi:10.1103/PhysRevD.88.023013 , adsurl =
-
[25]
, archivePrefix = "arXiv", eprint =
Circum-galactic Gas and the Isotropic Gamma-Ray Background. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/763/1/21 , adsurl =
-
[26]
, archivePrefix = "arXiv", eprint =
Antiproton limits on decaying gravitino dark matter. , archivePrefix = "arXiv", eprint =. doi:10.1088/1475-7516/2013/12/045 , adsurl =
2013 doi
-
[27]
, keywords =
The isotopic composition of cosmic-ray beryllium and its implication for the cosmic ray's age. , keywords =. doi:10.1086/173818 , adsurl =
-
[28]
, keywords =
Fermi-LAT Observations of the Diffuse -Ray Emission: Implications for Cosmic Rays and the Interstellar Medium. , keywords =. doi:10.1088/0004-637X/750/1/3 , adsurl =
-
[29]
, keywords =
Be-10 abundance and the age of cosmic rays - A balloon measurement. , keywords =. doi:10.1086/155045 , adsurl =
-
[30]
, keywords =
Measurement of the Secondary Radionuclides ^ 10 Be, ^ 26 Al, ^ 36 Cl, ^ 54 Mn, and ^ 14 C and Implications for the Galactic Cosmic-Ray Age. , keywords =. doi:10.1086/323842 , adsurl =
-
[31]
, year = 2001, month = oct, volume = 99, pages =
Radioactive Clocks and Cosmic-ray Transport in the Galaxy. , year = 2001, month = oct, volume = 99, pages =
2001
-
[32]
Advances in Space Research , year = 2001, volume = 27, pages =
Cosmic-ray time scales using radioactive clocks. Advances in Space Research , year = 2001, volume = 27, pages =. doi:10.1016/S0273-1177(01)00114-4 , adsurl =
2001 doi
-
[33]
, keywords =
A cosmic-ray age based on the abundance of Be-10. , keywords =. doi:10.1086/183310 , adsurl =
-
[34]
International Cosmic Ray Conference , eprint =
Evaluation of Production Cross Sections of Li, Be, B in CR. International Cosmic Ray Conference , eprint =
-
[35]
, archivePrefix = "arXiv", eprint =
Cosmic ray propagation time scales: lessons from radioactive nuclei and positron data. , archivePrefix = "arXiv", eprint =. doi:10.1088/1475-7516/2011/11/037 , adsurl =
2011 doi
-
[36]
, keywords =
The (C-13)/(C-12) ratio in cosmic ray sources. , keywords =
-
[37]
, archivePrefix = "arXiv", eprint =
Constraining Galactic cosmic-ray parameters with Z 2 nuclei. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201117927 , adsurl =
-
[38]
Physical Review Letters , archivePrefix = "arXiv", eprint =
Cosmic-Ray Positron Energy Spectrum Measured by PAMELA. Physical Review Letters , archivePrefix = "arXiv", eprint =. doi:10.1103/PhysRevLett.111.081102 , adsurl =
-
[39]
, archivePrefix = "arXiv", eprint =
An anomalous positron abundance in cosmic rays with energies 1.5-100GeV. , archivePrefix = "arXiv", eprint =. doi:10.1038/nature07942 , adsurl =
-
[40]
Physical Review Letters , eprint =
New Measurement of the Cosmic-Ray Positron Fraction from 5 to 15GeV. Physical Review Letters , eprint =. doi:10.1103/PhysRevLett.93.241102 , adsurl =
-
[41]
Physical Review Letters , keywords =
First Result from the Alpha Magnetic Spectrometer on the International Space Station: Precision Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5-350 GeV. Physical Review Letters , keywords =. doi:10.1103/PhysRevLett.110.141102 , adsurl =
-
[42]
, archivePrefix = "arXiv", eprint =
Pinpointing cosmic ray propagation with the AMS-02 experiment. , archivePrefix = "arXiv", eprint =. doi:10.1088/1475-7516/2010/06/022 , adsurl =
2010 doi
-
[43]
, archivePrefix = "arXiv", eprint =
Astrophysical uncertainties in the cosmic ray electron and positron spectrum from annihilating dark matter. , archivePrefix = "arXiv", eprint =. doi:10.1088/1475-7516/2009/08/003 , adsurl =
2009 doi
-
[44]
, archivePrefix = "arXiv", eprint =
Cosmic ray electrons, positrons and the synchrotron emission of the Galaxy: consistent analysis and implications. , archivePrefix = "arXiv", eprint =. doi:10.1088/1475-7516/2013/03/036 , adsurl =
2013 doi
-
[45]
, keywords =
Cosmic-ray lifetime in the Galaxy - Experimental results and models. , keywords =. doi:10.1007/BF00212240 , adsurl =
-
[46]
Progress of Theoretical Physics Supplement , year = 1958, volume = 6, pages =
Origin of Cosmic Rays. Progress of Theoretical Physics Supplement , year = 1958, volume = 6, pages =. doi:10.1143/PTPS.6.1 , adsurl =
1958 doi
-
[47]
International Cosmic Ray Conference , year = 1999, month = aug, volume = 4, pages =
Radioactive isotopes at relativistic energies: model predictions. International Cosmic Ray Conference , year = 1999, month = aug, volume = 4, pages =
1999
-
[48]
, keywords =
Decaying cosmic ray nuclei in the local interstellar medium. , keywords =
-
[49]
, year = 1998, month = jul, volume = 86, pages =
Cosmic-ray Clocks. , year = 1998, month = jul, volume = 86, pages =. doi:10.1023/A:1005071612125 , adsurl =
1998 doi
-
[50]
, keywords =
A Study of the Surviving Fraction of the Cosmic-Ray Radioactive Decay Isotopes \^ 10Be, \^ 26Al, \^ 36Cl and \^ 54Mn as a Function of Energy Using the Charge Ratios Be/B, Al/Mg, Cl/Ar, and Mn/Fe Measured on HEAO3. , keywords =. doi:10.1086/306224 , adsurl =
-
[51]
Geological Society of America Bulletin , year = 2013, month = sep, volume = 125, pages =
A cosmic trip: 25 years of cosmogenic nuclides in geology. Geological Society of America Bulletin , year = 2013, month = sep, volume = 125, pages =. doi:10.1130/B30774.1 , adsurl =
2013 doi
-
[52]
Nuclear Instruments and Methods in Physics Research B , year = 2010, month = jan, volume = 268, pages =
A new value for the half-life of ^ 10 Be by Heavy-Ion Elastic Recoil Detection and liquid scintillation counting. Nuclear Instruments and Methods in Physics Research B , year = 2010, month = jan, volume = 268, pages =. doi:10.1016/j.nimb.2009.09.020 , adsurl =
2010 doi
-
[53]
Nuclear Instruments and Methods in Physics Research B , year = 2010, month = jan, volume = 268, pages =
Determination of the ^ 10 Be half-life by multicollector ICP-MS and liquid scintillation counting. Nuclear Instruments and Methods in Physics Research B , year = 2010, month = jan, volume = 268, pages =. doi:10.1016/j.nimb.2009.09.012 , adsurl =
2010 doi
-
[54]
Nuclear Physics A , year = 1988, month = dec, volume = 490, pages =
Energy levels of light nuclei A = 5-10. Nuclear Physics A , year = 1988, month = dec, volume = 490, pages =. doi:10.1016/0375-9474(88)90124-8 , adsurl =
1988 doi
-
[55]
, eprint =
beta -radioactive cosmic rays in a diffusion model: Test for a local bubble?. , eprint =. doi:10.1051/0004-6361:20011447 , adsurl =
-
[56]
, archivePrefix = "arXiv", eprint =
Origin of the Cosmic-Ray Spectral Hardening. , archivePrefix = "arXiv", eprint =. doi:10.1088/2041-8205/752/1/L13 , adsurl =
-
[57]
, archivePrefix = "arXiv", eprint =
Secondary cosmic-ray nuclei from supernova remnants and constraints on the propagation parameters. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201218967 , adsurl =
-
[58]
Annual Review of Nuclear and Particle Science , eprint =
Cosmic-Ray Propagation and Interactions in the Galaxy. Annual Review of Nuclear and Particle Science , eprint =. doi:10.1146/annurev.nucl.57.090506.123011 , adsurl =
-
[59]
A Markov Chain Monte Carlo technique to sample transport and source parameters of Galactic cosmic rays. II. Results for the diffusion model combining B/C and radioactive nuclei. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201014010 , adsurl =
-
[60]
, archivePrefix = "arXiv", eprint =
Constraints on Cosmic-ray Propagation Models from A Global Bayesian Analysis. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/729/2/106 , adsurl =
-
[61]
, archivePrefix = "arXiv", eprint =
Testing the Origin of High-energy Cosmic Rays. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/752/1/68 , adsurl =
-
[62]
ArXiv e-prints , archivePrefix = "arXiv", eprint =
AMS-02 data confronts acceleration of cosmic ray secondaries in nearby sources. ArXiv e-prints , archivePrefix = "arXiv", eprint =
-
[63]
, archivePrefix = "arXiv", eprint =
New positron spectral features from supersymmetric dark matter: A way to explain the PAMELA data?. , archivePrefix = "arXiv", eprint =. doi:10.1103/PhysRevD.78.103520 , adsurl =
-
[64]
, archivePrefix = "arXiv", eprint =
Decaying dark matter can explain the e ^ ± excesses. , archivePrefix = "arXiv", eprint =. doi:10.1088/1475-7516/2009/01/043 , adsurl =
2009 doi
-
[65]
, keywords =
Positron fraction in cosmic rays and models of cosmic-ray propagation. , keywords =. doi:10.1103/PhysRevD.82.023009 , adsurl =
-
[66]
Physical Review Letters , archivePrefix = "arXiv", eprint =
Inhomogeneity in Cosmic Ray Sources as the Origin of the Electron Spectrum and the PAMELA Anomaly. Physical Review Letters , archivePrefix = "arXiv", eprint =. doi:10.1103/PhysRevLett.103.111302 , adsurl =
-
[67]
, archivePrefix = "arXiv", eprint =
Pulsar interpretation for the AMS-02 result. , archivePrefix = "arXiv", eprint =. doi:10.1103/PhysRevD.88.023001 , adsurl =
-
[68]
, archivePrefix = "arXiv", eprint =
Probing the Pulsar Origin of the Anomalous Positron Fraction with AMS-02 and Atmospheric Cherenkov Telescopes. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/772/1/18 , adsurl =
-
[69]
Astroparticle Physics , archivePrefix = "arXiv", eprint =
Measurements of cosmic-ray secondary nuclei at high energies with the first flight of the CREAM balloon-borne experiment. Astroparticle Physics , archivePrefix = "arXiv", eprint =. doi:10.1016/j.astropartphys.2008.07.010 , adsurl =
2008 doi
-
[70]
, keywords =
Relative abundances of secondary and primary cosmic rays at high energies. , keywords =. doi:10.1086/168349 , adsurl =
-
[71]
, archivePrefix = "arXiv", eprint =
Energy Spectra of Primary and Secondary Cosmic-Ray Nuclei Measured with TRACER. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/742/1/14 , adsurl =
-
[72]
, keywords =
Measurement of Boron and Carbon Fluxes in Cosmic Rays with the PAMELA Experiment. , keywords =. doi:10.1088/0004-637X/791/2/93 , archivePrefix =. 1407.1657 , primaryClass =
-
[73]
, year = 2016, month = dec, volume =
Precision Measurement of the Boron to Carbon Flux Ratio in Cosmic Rays from 1.9 GV to 2.6 TV with the Alpha Magnetic Spectrometer on the International Space Station. , year = 2016, month = dec, volume =. doi:10.1103/PhysRevLett.117.231102 , adsurl =
2016 doi
-
[74]
Measurement of the cosmic-ray secondary-to-primary ratios with CALET on the International Space Station
Akaike, Yosui and Maestro, Paolo. Measurement of the cosmic-ray secondary-to-primary ratios with CALET on the International Space Station. Proc. 37th ICRC (Berlin). doi:10.22323/1.395.0112
-
[75]
, eprint =
The Modified Weighted Slab Technique: Models and Results. , eprint =. doi:10.1086/318358 , adsurl =
-
[76]
, eprint =
Challenging Cosmic-Ray Propagation with Antiprotons: Evidence for a ``Fresh'' Nuclei Component?. , eprint =. doi:10.1086/367697 , adsurl =
-
[77]
, keywords =
The Cosmic-Ray 3He/ 4He Ratio from 200 MeV per Nucleon to 3.7 GeV per Nucleon. , keywords =. doi:10.1086/305358 , adsurl =
-
[78]
, keywords =
The Absolute Flux of Protons and Helium at the Top of the Atmosphere Using IMAX. , keywords =. doi:10.1086/308645 , adsurl =
-
[79]
Physical Review Letters , keywords =
Relative abundance of the helium isotopes He-3 and He-4 in the cosmic radiation. Physical Review Letters , keywords =. doi:10.1103/PhysRevLett.53.505 , adsurl =
-
[80]
, archivePrefix = "arXiv", eprint =
Isotopic Composition of Light Nuclei in Cosmic Rays: Results from AMS-01. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/736/2/105 , adsurl =
-
[81]
, archivePrefix = "arXiv", eprint =
Propagation of H and He cosmic ray isotopes in the Galaxy: astrophysical and nuclear uncertainties. , archivePrefix = "arXiv", eprint =. doi:10.1007/s10509-012-1138-y , adsurl =
-
[82]
Advances in Space Research , year = 1997, month = may, volume = 19, pages =
\^ 3He and \^ 2H measurements and what they tell us about cosmic ray propagation in the galaxy. Advances in Space Research , year = 1997, month = may, volume = 19, pages =. doi:10.1016/S0273-1177(96)00141-X , adsurl =
1997 doi
-
[83]
Acceleration and Transport of Energetic Particles Observed in the Heliosphere , year = 2000, series =
Reacceleration in a Monte Carlo diffusion model for the propagation of galactic cosmic rays. Acceleration and Transport of Energetic Particles Observed in the Heliosphere , year = 2000, series =. doi:10.1063/1.1324348 , adsurl =
-
[84]
Acceleration and Transport of Energetic Particles Observed in the Heliosphere , year = 2000, series =
A measurement of cosmic ray deuterium from 0.5-2.9 GeV/nucleon. Acceleration and Transport of Energetic Particles Observed in the Heliosphere , year = 2000, series =. doi:10.1063/1.1324352 , adsurl =
-
[85]
Nuclear Instruments and Methods in Physics Research A , year = 2011, month = oct, volume = 654, pages =
The TRACER instrument: A balloon-borne cosmic-ray detector. Nuclear Instruments and Methods in Physics Research A , year = 2011, month = oct, volume = 654, pages =. doi:10.1016/j.nima.2011.05.050 , adsurl =
2011 doi
-
[86]
Nuclear Instruments and Methods in Physics Research A , year = 2000, month = mar, volume = 443, pages =
A superconducting solenoidal spectrometer for a balloon-borne experiment. Nuclear Instruments and Methods in Physics Research A , year = 2000, month = mar, volume = 443, pages =
2000
-
[87]
, keywords =
Measurement of Cosmic-Ray Hydrogen and Helium and Their Isotopic Composition with the BESS Experiment. , keywords =. doi:10.1086/324140 , adsurl =
-
[88]
International Cosmic Ray Conference , year = 2003, month = jul, volume = 4, pages =
New Measurements of the Li, Be, and bIsotopes as a Test of Cosmic Ray Transport Models. International Cosmic Ray Conference , year = 2003, month = jul, volume = 4, pages =
2003
-
[89]
, keywords =
Isotopic composition of cosmic-ray boron and nitrogen. , keywords =. doi:10.1086/166348 , adsurl =
-
[90]
, keywords =
The low-energy galactic cosmic ray carbon, nitrogen, and oxygen isotopic composition. , keywords =. doi:10.1086/158747 , adsurl =
-
[91]
International Cosmic Ray Conference , keywords =
The energy dependence of the neon-22 excess in the cosmic radiation. International Cosmic Ray Conference , keywords =
-
[92]
Galactic source distribution of heavy cosmic rays and the energy dependent overabundance of ^ 22 Ne. Proc. 26th ICRC (Salt Lake City) , year = 1999, month = aug, volume = 4, pages =
1999
-
[93]
Acceleration and Transport of Energetic Particles Observed in the Heliosphere , year = 2000, series =
^ 22 Ne excess in cosmic rays from the inner galaxy. Acceleration and Transport of Energetic Particles Observed in the Heliosphere , year = 2000, series =. doi:10.1063/1.1324350 , adsurl =
-
[94]
, keywords =
The Superbubble Origin of ^ 22 Ne in Cosmic Rays. , keywords =. doi:10.1086/375192 , adsurl =
-
[95]
Nuclear Physics A , year = 2005, month = jul, volume = 758, pages =
Isotopic Composition of Cosmic Rays: Results from the Cosmic Ray Isotope Spectrometer on the ACE Spacecraft. Nuclear Physics A , year = 2005, month = jul, volume = 758, pages =. doi:10.1016/j.nuclphysa.2005.05.038 , adsurl =
2005 doi
-
[96]
, eprint =
Cosmic-Ray Neon, Wolf-Rayet Stars, and the Superbubble Origin of Galactic Cosmic Rays. , eprint =. doi:10.1086/496959 , adsurl =
-
[97]
, keywords =
Isotopic anomalies in cosmic rays and the metallicity gradient in the Galaxy. , keywords =
-
[98]
Reviews of Modern Physics , year = 1994, month = jan, volume = 66, pages =
On the origin of the light elements (Z < 6). Reviews of Modern Physics , year = 1994, month = jan, volume = 66, pages =. doi:10.1103/RevModPhys.66.193 , adsurl =
1994 doi
-
[99]
, archivePrefix = "arXiv", eprint =
Production and evolution of Li, Be, and B isotopes in the Galaxy. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201219043 , adsurl =
-
[100]
, archivePrefix = "arXiv", eprint =
On the origin and composition of Galactic cosmic rays. , archivePrefix = "arXiv", eprint =. doi:10.1051/0004-6361/201117448 , adsurl =
-
[101]
Joint SOHO/ACE workshop ''Solar and Galactic Composition'' , year = 2001, series =
Measurements of the isotopes of lithium, beryllium, and boron from ACE/CRIS. Joint SOHO/ACE workshop ''Solar and Galactic Composition'' , year = 2001, series =. doi:10.1063/1.1434007 , adsurl =
2001 doi
-
[102]
Joint SOHO/ACE workshop ''Solar and Galactic Composition'' , year = 2001, series =
The cosmic-ray contribution to galactic abundances of the light elements: Interpretation of GCR LiBeB abundance measurements from ACE/CRIS. Joint SOHO/ACE workshop ''Solar and Galactic Composition'' , year = 2001, series =. doi:10.1063/1.1434006 , adsurl =
2001 doi
-
[103]
International Cosmic Ray Conference , year = 1999, month = aug, volume = 4, pages =
Test of the Diffusion Halo and the Leaky Box Model by means of secondary radioactive Cosmic Ray Nuclei with different life times. International Cosmic Ray Conference , year = 1999, month = aug, volume = 4, pages =
1999
-
[104]
, year = 1998, month = jul, volume = 86, pages =
The Advanced Composition Explorer. , year = 1998, month = jul, volume = 86, pages =. doi:10.1023/A:1005082526237 , adsurl =
1998 doi
-
[105]
Advances in Space Research , eprint =
Observations of the Li, Be, and B isotopes and constraints on cosmic-ray propagation. Advances in Space Research , eprint =. doi:10.1016/j.asr.2006.09.008 , adsurl =
2006 doi
-
[106]
Elemental Composition at the Cosmic-Ray Source Derived from the ACE-CRIS Instrument. I. _ 6 C to _ 28 Ni. , keywords =. doi:10.3847/1538-4357/aad867 , adsurl =
-
[107]
Science , keywords =
Observation of the ^ 60 Fe nucleosynthesis-clock isotope in galactic cosmic rays. Science , keywords =. doi:10.1126/science.aad6004 , adsurl =
-
[108]
Joint SOHO/ACE workshop ''Solar and Galactic Composition'' , year = 2001, series =
GCR neon isotopic abundances: Comparison with wolf-rayet star models and meteoritic abundances. Joint SOHO/ACE workshop ''Solar and Galactic Composition'' , year = 2001, series =. doi:10.1063/1.1434008 , adsurl =
2001 doi
-
[109]
, keywords =
Constraints on the Time Delay between Nucleosynthesis and Cosmic-Ray Acceleration from Observations of \^ 59NI and \^ 59CO. , keywords =. doi:10.1086/312242 , adsurl =
-
[110]
, year = 2001, month = oct, volume = 99, pages =
The Origin of Primary Cosmic Rays: Constraints from ACE Elemental and Isotopic Composition Observations. , year = 2001, month = oct, volume = 99, pages =
2001
-
[111]
Journal of Physics Conference Series , year = 2013, month = feb, volume = 409, number = 1, eid =
H, He, Li and Be Isotopes in the PAMELA-Experiment. Journal of Physics Conference Series , year = 2013, month = feb, volume = 409, number = 1, eid =. doi:10.1088/1742-6596/409/1/012030 , adsurl =
2013 doi
-
[112]
, keywords =
Lithium and Beryllium Isotopes with the PAMELA Experiment. , keywords =. doi:10.3847/1538-4357/aacf89 , archivePrefix =. 1806.10948 , primaryClass =
-
[113]
Nuclear Instruments and Methods in Physics Research A , year = 2011, month = oct, volume = 654, pages =
Upgrade of the Alpha Magnetic Spectrometer (AMS-02) for long term operation on the International Space Station (ISS). Nuclear Instruments and Methods in Physics Research A , year = 2011, month = oct, volume = 654, pages =. doi:10.1016/j.nima.2011.06.051 , adsurl =
2011 doi
-
[114]
Nuclear Physics B Proceedings Supplements , year = 2013, month = oct, volume = 243, pages =
The Alpha Magnetic Spectrometer on the International Space Station. Nuclear Physics B Proceedings Supplements , year = 2013, month = oct, volume = 243, pages =. doi:10.1016/j.nuclphysbps.2013.09.028 , adsurl =
2013 doi
-
[115]
39th COSPAR Scientific Assembly , year = 2012, series =
CREAM Balloon Flights and Beyond. 39th COSPAR Scientific Assembly , year = 2012, series =
2012
-
[116]
39th COSPAR Scientific Assembly , year = 2012, series =
The CALET mission for high energy astroparticle physics on the International Space Station. 39th COSPAR Scientific Assembly , year = 2012, series =
2012
-
[117]
Astroparticle Physics , year = 2017, pages =
The DArk Matter Particle Explorer mission. Astroparticle Physics , year = 2017, pages =
2017
-
[118]
a new public cosmic ray propagation code Basic phenomenology, sample results, and a bit of USINE
USINE:. a new public cosmic ray propagation code Basic phenomenology, sample results, and a bit of USINE. Cosmic Rays for Particle and Astroparticle Physics , year = 2011, editor =. doi:10.1142/9789814329033\_0053 , adsurl =
2011 doi
-
[119]
, eprint =
Propagation of Cosmic-Ray Nucleons in the Galaxy. , eprint =. doi:10.1086/306470 , adsurl =
-
[120]
Physical Review Letters , archivePrefix = "arXiv", eprint =
Three-Dimensional Model of Cosmic-Ray Lepton Propagation Reproduces Data from the Alpha Magnetic Spectrometer on the International Space Station. Physical Review Letters , archivePrefix = "arXiv", eprint =. doi:10.1103/PhysRevLett.111.021102 , adsurl =
-
[121]
, keywords =
Cosmic-ray propagation in the Galaxy and in the heliosphere - The path-length distribution at low energy. , keywords =. doi:10.1086/191197 , adsurl =
-
[122]
Reviews of Modern Physics , year = 1976, month = apr, volume = 48, pages =
On the origin of cosmic rays: Some problems in high-energy astrophysics. Reviews of Modern Physics , year = 1976, month = apr, volume = 48, pages =. doi:10.1103/RevModPhys.48.161 , adsurl =
1976 doi
-
[123]
I - Proton nucleon component
Origin of cosmic rays - Galactic models with halo. I - Proton nucleon component. , keywords =. doi:10.1007/BF00639701 , adsurl =
-
[124]
ArXiv e-prints , archivePrefix = "arXiv", eprint =
The Fermi Bubbles Revisited. ArXiv e-prints , archivePrefix = "arXiv", eprint =
-
[125]
Nuclear Instruments and Methods in Physics Research A , year = 1994, month = apr, volume = 343, pages =
Theory of ring imaging Cherenkov counters. Nuclear Instruments and Methods in Physics Research A , year = 1994, month = apr, volume = 343, pages =. doi:10.1016/0168-9002(94)90532-0 , adsurl =
1994 doi
-
[126]
Nuclear Instruments and Methods in Physics Research A , year = 2007, month = mar, volume = 572, pages =
The AMS-02 tracker alignment system for 3D position control with artificial laser generated straight tracks. Nuclear Instruments and Methods in Physics Research A , year = 2007, month = mar, volume = 572, pages =. doi:10.1016/j.nima.2006.10.273 , adsurl =
2007 doi
-
[127]
Nuclear Instruments and Methods in Physics Research A , year = 2011, month = may, volume = 639, pages =
The AMS-02 RICH detector: Performance during ground-based data taking at CERN. Nuclear Instruments and Methods in Physics Research A , year = 2011, month = may, volume = 639, pages =. doi:10.1016/j.nima.2010.09.036 , adsurl =
2011 doi
-
[128]
Journal of Instrumentation , archivePrefix = "arXiv", eprint =
Design and construction of a Cherenkov imager for charge measurement of nuclear cosmic rays. Journal of Instrumentation , archivePrefix = "arXiv", eprint =. doi:10.1088/1748-0221/6/06/P06004 , adsurl =
-
[129]
Nuclear Instruments and Methods in Physics Research A , year = 2005, month = nov, volume = 553, pages =
Focusing aerogel RICH (FARICH). Nuclear Instruments and Methods in Physics Research A , year = 2005, month = nov, volume = 553, pages =. doi:10.1016/j.nima.2005.08.073 , adsurl =
2005 doi
-
[130]
Nuclear Instruments and Methods in Physics Research A , year = 2010, month = mar, volume = 614, pages =
Characterization study of silica aerogel for Cherenkov imaging. Nuclear Instruments and Methods in Physics Research A , year = 2010, month = mar, volume = 614, pages =. doi:10.1016/j.nima.2009.12.029 , adsurl =
2010 doi
-
[131]
status and physics prospects
The RICH detector of the AMS-02 experiment:. status and physics prospects. Astroparticle, Particle and Space Physics, Detectors and Medical Physics Applications , year = 2008, archivePrefix = "arXiv", eprint =. doi:10.1142/9789812819093\_0151 , adsurl =
2008 doi
-
[132]
Nuclear Instruments and Methods in Physics Research A , year = 2011, month = may, volume = 639, pages =
The CLAS12 large area RICH detector. Nuclear Instruments and Methods in Physics Research A , year = 2011, month = may, volume = 639, pages =. doi:10.1016/j.nima.2010.10.047 , adsurl =
2011 doi
-
[133]
Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series , year = 2006, series =
Replicated carbon fiber RICH mirror for AMS-02. Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series , year = 2006, series =. doi:10.1117/12.671864 , adsurl =
2006 doi
-
[134]
Nuclear Instruments and Methods in Physics Research A , year = 2011, month = may, volume = 639, pages =
Study of transparent silica aerogel with high refractive index. Nuclear Instruments and Methods in Physics Research A , year = 2011, month = may, volume = 639, pages =. doi:10.1016/j.nima.2010.08.125 , adsurl =
2011 doi
-
[135]
Advances in Space Research , year = 2001, volume = 27, pages =
The abundance of radioactive nuclei under different physical environments around the solar system. Advances in Space Research , year = 2001, volume = 27, pages =. doi:10.1016/S0273-1177(01)00115-6 , adsurl =
2001 doi
-
[136]
, archivePrefix = "arXiv", eprint =
Measurement of the Isotopic Composition of Hydrogen and Helium Nuclei in Cosmic Rays with the PAMELA Experiment. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/770/1/2 , adsurl =
-
[137]
Nuclear Instruments and Methods in Physics Research A , year = 2008, month = oct, volume = 596, pages =
The AMS silicon tracker: Construction and performance. Nuclear Instruments and Methods in Physics Research A , year = 2008, month = oct, volume = 596, pages =. doi:10.1016/j.nima.2008.07.116 , adsurl =
2008 doi
-
[138]
Nuclear Physics B Proceedings Supplements , year = 1999, month = aug, volume = 78, pages =
Development towards Ultra-thin Superconducting Solenoid Magnets for High Energy Particle Detectors. Nuclear Physics B Proceedings Supplements , year = 1999, month = aug, volume = 78, pages =. doi:10.1016/S0920-5632(99)00604-0 , adsurl =
1999 doi
-
[139]
Applied Superconductivity, IEEE Transactions on , year = 2000, month =
High-strength and high-RRR Al-Ni alloy for aluminum-stabilized superconductor. Applied Superconductivity, IEEE Transactions on , year = 2000, month =
2000
-
[140]
, archivePrefix = "arXiv", eprint =
Interactions of Cosmic Rays in the Atmosphere: Growth Curves Revisited. , archivePrefix = "arXiv", eprint =. doi:10.1088/0004-637X/778/2/87 , adsurl =
-
[141]
and Heintze, J
Bock, P. and Heintze, J. and Kunst, T. and Schmitt, B. and Smolik, L. Drift Chamber Readout With Flash ADCs. 1. Time and Space Resolution. Nucl.Instrum.Meth. 1986. doi:10.1016/0168-9002(86)90215-9
1986 doi
-
[142]
, title =
Haino, S. , title =. 2009 , number =
2009
-
[143]
Nuclear Instruments and Methods in Physics Research A , year = 1997, month = feb, volume = 400, pages =
The High-Energy Antimatter Telescope (HEAT): An instrument for the study of cosmic-ray positrons. Nuclear Instruments and Methods in Physics Research A , year = 1997, month = feb, volume = 400, pages =. doi:10.1016/S0168-9002(97)00945-5 , adsurl =
1997 doi
-
[144]
and Milgrome, O
Garcia-Sciveres, M. and Milgrome, O. and Zimmerman, T. and Volobuev, I. and Ely, R.P. and others. The SVX3D integrated circuit for dead-timeless silicon strip readout. Nucl.Instrum.Meth. 1999. doi:10.1016/S0168-9002(99)00409-X
1999 doi
-
[145]
Nuclear Instruments and Methods in Physics Research A , archivePrefix = "arXiv", eprint =
Operational experience, improvements, and performance of the CDF Run II silicon vertex detector. Nuclear Instruments and Methods in Physics Research A , archivePrefix = "arXiv", eprint =. doi:10.1016/j.nima.2013.07.015 , adsurl =
2013 doi
-
[146]
Yoshimura, and others , series =
K. Yoshimura, and others , series =. The second Antarctic Flight of BESS-Polar Experiment: Flight Summary and Detector Performance , year =
-
[147]
Physical Review Letters , year = 1995, month = jul, volume = 75, pages =
Cosmic Ray Positrons at High Energies: A New Measurement. Physical Review Letters , year = 1995, month = jul, volume = 75, pages =. doi:10.1103/PhysRevLett.75.390 , adsurl =
1995 doi
-
[148]
, keywords =
Cosmic-Ray Electrons and Positrons from 1 to 100 GeV: Measurements with HEAT and Their Interpretation. , keywords =. doi:10.1086/322324 , adsurl =
-
[149]
, keywords =
Measurement of Separate Cosmic-Ray Electron and Positron Spectra with the Fermi Large Area Telescope. , keywords =. doi:10.1103/PhysRevLett.108.011103 , archivePrefix =. 1109.0521 , primaryClass =
-
[150]
Multi-Pixel Photon Counter, https://www.hamamatsu.com/resources/pdf/ssd/s13360-2050ve\_etc\_kapd1053e.pdf , year=
Hamamatsu , booktitle=. Multi-Pixel Photon Counter, https://www.hamamatsu.com/resources/pdf/ssd/s13360-2050ve\_etc\_kapd1053e.pdf , year=
-
[151]
A novel sub-millimeter resolution PET detector with TOF capability , year=
Tianpeng Xu and Jie Wen and Qiang Wang and Qingyang Wei and Tianyu Ma and Yaqiang Liu and Yuan-Chuan Tai , booktitle=. A novel sub-millimeter resolution PET detector with TOF capability , year=
-
[152]
, year = 2018, month = jan, volume =
Observation of New Properties of Secondary Cosmic Rays Lithium, Beryllium, and Boron by the Alpha Magnetic Spectrometer on the International Space Station. , year = 2018, month = jan, volume =. doi:10.1103/PhysRevLett.120.021101 , adsurl =
2018 doi
-
[153]
, year = 2020, month = may, volume =
Properties of Neon, Magnesium, and Silicon Primary Cosmic Rays Results from the Alpha Magnetic Spectrometer. , year = 2020, month = may, volume =. doi:10.1103/PhysRevLett.124.211102 , adsurl =
2020 doi
-
[154]
, keywords =
Measurement of the Cosmic Ray Helium Energy Spectrum from 70 GeV to 80 TeV with the DAMPE Space Mission. , keywords =. doi:10.1103/PhysRevLett.126.201102 , archivePrefix =. 2105.09073 , primaryClass =
-
[155]
doi:10.1088/1748-0221/9/01/c01049 , url =
J Fleury and S Callier and C de La Taille and N Seguin and D Thienpont and F Dulucq and S Ahmad and G Martin , title =. doi:10.1088/1748-0221/9/01/c01049 , url =
-
[156]
arXiv e-prints , keywords =
Rapporteur Talk: Cosmic Ray Direct Measurements, 37th ICRC (Berlin), 2021. arXiv e-prints , keywords =
2021
-
[157]
, keywords =
Galactic halo size in the light of recent AMS-02 data. , keywords =. doi:10.1051/0004-6361/202038064 , archivePrefix =. 2004.00441 , primaryClass =
2004 arXiv
-
[158]
, keywords =
AMS-02 beryllium data and its implication for cosmic ray transport. , keywords =. doi:10.1103/PhysRevD.101.023013 , archivePrefix =. 1910.04113 , primaryClass =
1910 arXiv
-
[159]
Nuclear Instruments and Methods in Physics Research A , keywords =
The RICH detector of AMS-02: 5 years of operation in space. Nuclear Instruments and Methods in Physics Research A , keywords =. doi:10.1016/j.nima.2016.12.011 , adsurl =
2016 doi
-
[160]
, year = 2019, month = nov, volume =
Properties of Cosmic Helium Isotopes Measured by the Alpha Magnetic Spectrometer. , year = 2019, month = nov, volume =. doi:10.1103/PhysRevLett.123.181102 , adsurl =
2019 doi
-
[161]
arXiv e-prints , keywords =
Results from a Pilot Study on the Measurement of Nuclear Fragmentation with NA61/SHINE at the CERN SPS: ^ 11 C Production in C+p Interactions at 13.5 A GeV/c. arXiv e-prints , keywords =
-
[162]
2019 , month=
University of Michigan’s Upgraded Large Vacuum Test Facility,. 2019 , month=
2019
-
[163]
2021 , month=
NASA , title=. 2021 , month=
2021
-
[164]
Ajima and others , keywords =
Y. Ajima and others , keywords =. A superconducting solenoidal spectrometer for a balloon-borne experiment , journal =. 2000 , issn =. doi:https://doi.org/10.1016/S0168-9002(99)01010-4 , url =
-
[165]
Journal of Physics: Conference Series , abstract =
Johannes Rauch and Tobias Schlüter , title =. Journal of Physics: Conference Series , abstract =. doi:10.1088/1742-6596/608/1/012042 , url =
-
[166]
Moleculoy Series-HFM
HPI. Moleculoy Series-HFM
-
[167]
FX11 Series
Hirose Electric. FX11 Series
-
[168]
King , title =
Davis E. King , title =. Journal of Machine Learning Research , year =
-
[169]
Dini Group Wayback Machine
Dini Group. Dini Group Wayback Machine
-
[170]
Garfield, a drift chamber simulation program
Veenhof, Rob. Garfield, a drift chamber simulation program. Nucl. Instrum. Meth. A. 1998. doi:10.1016/S0168-9002(98)00851-1
1998 doi
-
[171]
Garfield++: Simulation of gaseous detectors
Garfield++ Collaboration. Garfield++: Simulation of gaseous detectors
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