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TOI-1846 b: a super-Earth in the radius valley orbiting a nearby M dwarf |
iacweb |
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Application of Deep Learning to the Classification of Stokes Profiles: From the Quiet Sun to Sunspots |
iacweb |
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The TOI-2427 system: Two close-in planets orbiting a late K-dwarf star |
iacweb |
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Quiet Sun Magnetism from ViSP Data Multiline Inversions Around 630.1 nm |
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The Central Engine of Low-luminosity Radio Galaxy 3C 270 (NGC 4261) |
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GOTO065054+593624: An 8.5 mag amplitude dwarf nova identified in real time via Kilonova Seekers |
iacweb |
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A Swarm of WASP Planets: Nine Giant Planets Identified by the WASP Survey |
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TOI-3493 b: A planet with a Neptune-like density transiting a bright G0-type star |
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Size and shape of the trans-Neptunian object (470316) 2007 OC10: Comparison with thermal data |
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Few EURONEAR NEA mini-surveys observed with the INT, KASI and T80S telescopes during the ParaSOL synthetic tracking project |
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Evaluating quenching in cosmological simulations of galaxy formation with spectral covariance in the optical window |
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2020 BX<SUB>12</SUB>—The Last Binary Asteroid Discovered at Arecibo |
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The Dwarf Irregular Galaxy NGC 6822. II. Young, Intermediate and Old Stellar Populations: Comparison between Theory and Observations |
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The OTELO survey: New evidence of downsizing from the specific star formation rates, stellar mass functions, and star formation histories of a sample of low-mass galaxies at 0.38 < z < 1.43 |
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Water in Ryugu as a property of processes in its parent body |
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A Nonstop Aurora? The Intriguing Radio Emission from the Rapidly Rotating Magnetic Massive Star HR 5907 |
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The NCORES programme: precise planetary masses, null results, and insight into the planet mass distribution near the radius gap |
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Irradiation origin and stability of CO on trans-Neptunian objects: Laboratory constraints and observational evidence from JWST/DiSCo-TNOs |
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Multi-wavelength picture of the misaligned BL Lac object 3C 371 |
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Detection of stellar wakes in the Milky Way: A deep learning approach |
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Extragalactic globular cluster near-infrared spectroscopy: II. The stellar population synthesis model zero-point problem extends to the near-infrared |
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OrCAS: Origins, Compositions, and Atmospheres of Sub-Neptunes. I. Survey Definition |
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Near-ultraviolet absorption distribution of primitive asteroids from photometric surveys: II. Collisional families |
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HD 119130 b Is Not an "Ultradense" Sub-Neptune |
iacweb |
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Radii, masses, and transit-timing variations of the three-planet system orbiting the naked-eye star TOI-396 |
iacweb |
3 months ago |
