AGILE archival data reveal gamma-ray flares from a source matching IGR J17354-3255, with orbital phase correlation supporting physical association and high-energy emission from SFXTs.
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The Compton Spectrometer and Imager
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Revised supernova opacity modeling reopens the Turner window for hadronically coupled axions, enabling resonant absorption searches in NaI detectors for couplings |g_app| between 10^{-6.5} and 10^{-2}.
A neural network outputs HEALPix probability distributions from COSI BGO shield counts to localize short GRBs and compute possibly multi-modal 90% confidence regions.
Six s-wave proton resonances in 19Ne were identified via angular distributions in the 19F(3He,t)19Ne reaction, with asymptotic normalizations computed in the symmetry-adapted no-core shell model, showing that prior studies underestimated uncertainties in the 18F(p,α)15O rate.
A balloon mission concept with 8192 TES detectors projects 200 eV FWHM resolution at 511 keV and 35-sigma detection of the galactic center 511 keV line to study its shape and substructure.
Gamma-ray observations impose an upper bound of order 1 GeV on the mass of a photon-coupled scalar dark matter candidate produced via thermal misalignment.
In the minimal Majoron model the particle can explain all dark matter with mass below about 10 MeV from misalignment or freeze-in, and remains compatible with thermal leptogenesis when misalignment dominates or with mild tuning.
COSI is projected to detect MeV polarization from up to about 6 blazar flares over its two-year mission, mostly flat-spectrum radio quasars, assuming GeV-like flare rates and baseline backgrounds.
Solar axion-like particles up to 5.5 MeV produce off-axis MeV photons via two-body decay, enabling new space and terrestrial searches that could probe g_aγ down to 10^{-12} GeV^{-1}.
Reviews mechanisms generating polarized X-rays in high-energy astrophysics and the detectors for measuring polarization fraction and angle.
citing papers explorer
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AGILE detection of transient {\gamma}-ray emission from the region of the supergiant fast X-ray transient source IGR J17354-3255
AGILE archival data reveal gamma-ray flares from a source matching IGR J17354-3255, with orbital phase correlation supporting physical association and high-energy emission from SFXTs.
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Revisiting Turner Window Axions: The Untapped Potential of NaI Dark Matter Detectors
Revised supernova opacity modeling reopens the Turner window for hadronically coupled axions, enabling resonant absorption searches in NaI detectors for couplings |g_app| between 10^{-6.5} and 10^{-2}.
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Localization and Confidence Region Estimation of Short GRBs with the COSI BGO Shield Using a HEALPix-Based Deep Learning Approach
A neural network outputs HEALPix probability distributions from COSI BGO shield counts to localize short GRBs and compute possibly multi-modal 90% confidence regions.
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Properties of states in \textsuperscript{19}Ne important for the \textsuperscript{18}F$(p,\alpha)$\textsuperscript{15}O reaction rate
Six s-wave proton resonances in 19Ne were identified via angular distributions in the 19F(3He,t)19Ne reaction, with asymptotic normalizations computed in the symmetry-adapted no-core shell model, showing that prior studies underestimated uncertainties in the 18F(p,α)15O rate.
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Design of a mission to measure the shape and substructure of the 511 keV gamma-ray line from the center of the Milky Way
A balloon mission concept with 8192 TES detectors projects 200 eV FWHM resolution at 511 keV and 35-sigma detection of the galactic center 511 keV line to study its shape and substructure.
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Gamma-Ray Signatures of Thermal Misalignment Dark Matter
Gamma-ray observations impose an upper bound of order 1 GeV on the mass of a photon-coupled scalar dark matter candidate produced via thermal misalignment.
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Minimal Majoron Dark Matter
In the minimal Majoron model the particle can explain all dark matter with mass below about 10 MeV from misalignment or freeze-in, and remains compatible with thermal leptogenesis when misalignment dominates or with mild tuning.
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Detectability of Polarized Gamma-ray Emission from Blazar Flares with COSI
COSI is projected to detect MeV polarization from up to about 6 blazar flares over its two-year mission, mostly flat-spectrum radio quasars, assuming GeV-like flare rates and baseline backgrounds.
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Looking for Lights from the Darkness: Signals from MeV-scale Solar Axion-like Particles
Solar axion-like particles up to 5.5 MeV produce off-axis MeV photons via two-body decay, enabling new space and terrestrial searches that could probe g_aγ down to 10^{-12} GeV^{-1}.
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Astrophysical X-Ray Polarization
Reviews mechanisms generating polarized X-rays in high-energy astrophysics and the detectors for measuring polarization fraction and angle.