X-ray spectral modelling of the AGN obscuring region in the CDFS: Bayesian model selection and catalogue
A&A, 564 (2014) A125
Published online: 2014-04-17
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A Multiwavelength Machine-learning Approach to Classifying X-Ray Sources in the Fields of Unidentified 4FGL-DR4 Sources
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X-Ray Diagnostics of Cassiopeia A’s “Green Monster”: Evidence for Dense Shocked Circumstellar Plasma
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A Comparison of the X-Ray Polarimetric Properties of Stellar and Supermassive Black Holes
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Non-standard neutrino interactions mediated by a light scalar at DUNE
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Multiple Clues for Dayside Aerosols and Temperature Gradients in WASP-69 b from a Panchromatic JWST Emission Spectrum
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GRB 231115A: A Nearby Magnetar Giant Flare or a Cosmic Short Gamma-Ray Burst?
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Sulfur Dioxide and Other Molecular Species in the Atmosphere of the Sub-Neptune GJ 3470 b
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Analysis of BOSS galaxy data with weighted skew-spectra
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Inferring Small Neutron Star Spins with Neutron Star–Black Hole Mergers
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A detailed chemical study of the extreme velocity stars in the galaxy
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The Importance of Optical Wavelength Data on Atmospheric Retrievals of Exoplanet Transmission Spectra
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The more the merrier: SRG/eROSITA discovers two further galaxies showing X-ray quasi-periodic eruptions
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A Comprehensive Analysis of Textbook-version Afterglow Light Curves of Gamma-Ray Bursts and Implication for Universal Radiation Physics of Baryonic Jets
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Parameterizing pressure–temperature profiles of exoplanet atmospheres with neural networks
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TOI-663: A newly discovered multi-planet system with three transiting mini-Neptunes orbiting an early M star
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Stripe 82-XL: The ∼54.8 deg2 and ∼18.8 Ms Chandra and XMM-Newton Point-source Catalog and Number of Counts
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The MOPYS project: A survey of 70 planets in search of extended He I and H atmospheres
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The JWST EXCELS survey: too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5
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Determining the Extents, Geometries, and Kinematics of Narrow-line Region Outflows in Nearby Seyfert Galaxies
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Detecting galaxy groups populating the local Universe in the eROSITA era
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