Polarized optical afterglow reveals magnetic field structure in GRB jets and the gamma-rays linked to scattered radiation by reverse shock heated electrons

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ARCO TEAM

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Jet Angular Structure Revealed by the Brightest Gamma-Ray Burst of All Time

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The TESS-Keck Survey. XVIII. A Sub-Neptune and Spurious Long-period Signal in the TOI-1751 System

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An equation of state of CO for use in planetary modeling

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Prompt gamma-ray burst emission from internal shocks – new insights

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How planets form by pebble accretion V. Silicate rainout delays contraction of sub-Neptunes

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The metal-poor atmosphere of a Neptune/Sub-Neptune planet progenitor / Barat, Desert, Vazan et al. 2024 Nature astronomy

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Internal shocks hydrodynamics: the collision of two cold shells in detail

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How to teach general relativity

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Exploring the environments of FRBs with polarization and Rotation Measure studies

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GRB spectrum from gradual dissipation in a magnetized outflow

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The Foregrounds of the 21 cm Experiments:

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GRB Polarization: A Unique Probe of GRB Physics

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Interiors of ice-rich planets: mixed ice and rock

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Gamma ray burst afterglows from neutron star merger jets

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Bouncing Cosmological Isotropic Solutions in Scalar – Tensor Gravity

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High-energy emission from a magnetar giant flare in the Sculptor galaxy

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Constraining the magnetic field structure in collisionless relativistic shocks with a radio afterglow polarization upper limit in GW 170817

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ARCO Postdoctoral positions and fellowships

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Upper limits from The LOFAR EoR KSP

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Scalarized electric and magnetic black holes in the vector-tensor Horndeski gravity

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The Epoch of Reionization and Cosmic Dawn

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R-process Nucleosynthesis

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The rate of r-process production in the Universe

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Probing Cosmology and Fundamental Physics

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Gamma Ray Bursts

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Gravitational Wave Sources

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Exploring the epoch of hydrogen reionization using FRBs

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Constraining Cosmological models with The LOFAR EoR Upper

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GALAXY FORMATION AND EVOLUTION

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SOLAR AND STELLAR ATMOSPHERE

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Explaining the low luminosity of Uranus – interior evolution model

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On the aspect ratio of ‘Omuamua – surface properties matter

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Planet formation by pebble accretion – emergence of composition gradient in the interior

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Fast Radio Bursts

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Magnetars

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Probing Cosmology and Fundamental Physics

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Nunc sit amet magna

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Maecenas interdum

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Millisecond Pu

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