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Atomic data for the Gaia-ESO Survey |
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1 week ago |
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H α fluxes and extinction distances for planetary nebulae in the IPHAS survey of the northern galactic plane |
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Downflowing umbral flashes as evidence of standing waves in sunspot umbrae |
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Shadows in the Dark: Low-surface-brightness Galaxies Discovered in the Dark Energy Survey |
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On the radial abundance gradients of nitrogen and oxygen in the inner Galactic disc |
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Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre |
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MuSCAT3: a 4-color simultaneous camera for the 2m Faulkes Telescope North |
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LiteBIRD satellite: JAXA's new strategic L-class mission for all-sky surveys of cosmic microwave background polarization |
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Spectropolarimetric observations of the CIZA J2242.8+5301 northern radio relic: no evidence of high-frequency steepening |
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The T<SUB>e</SUB>[N II]-T<SUB>e</SUB>[O III] temperature relation in H II regions and the reliability of strong-line methods |
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WD1032 + 011, an inflated brown dwarf in an old eclipsing binary with a white dwarf |
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Very high redshift quasars and the rapid emergence of supermassive black holes |
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A search for optical and near-infrared counterparts of the compact binary merger GW190814 |
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An ultrahot Neptune in the Neptune desert |
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Are extreme asymptotic giant branch stars post-common envelope binaries? |
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Processing GOTO data with the Rubin Observatory LSST Science Pipelines I: Production of coadded frames |
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The miniJPAS survey: star-galaxy classification using machine learning |
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Erratum: A search for optical and near-infrared counterparts of the compact binary merger GW190814 |
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Planet Hunters TESS II: findings from the first two years of TESS |
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A deep learning approach to test the small-scale galaxy morphology and its relationship with star formation activity in hydrodynamical simulations |
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The Second Data Release of the Survey of the MAgellanic Stellar History (SMASH) |
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ESPRESSO at VLT. On-sky performance and first results |
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Collisional history of Ryugu's parent body from bright surface boulders |
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An ALMA/NOEMA survey of the molecular gas properties of high-redshift star-forming galaxies |
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Accurately constraining velocity information from spectral imaging observations using machine learning techniques |
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