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DESI Emission-line Galaxies: Unveiling the Diversity of [O II] Profiles and Its Links to Star Formation and Morphology |
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Non-local thermodynamic equilibrium inversions of the Si I 10827 Å spectral line |
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A Fourth Planet in the Kepler-51 System Revealed by Transit Timing Variations |
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Lens Mass Estimate in the Galactic Disk Extreme Parallax Microlensing Event Gaia19dke |
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A new method of reconstructing images of gamma-ray telescopes applied to the LST-1 of CTAO |
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Coronal and chromospheric activity of Teegarden's star |
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An ultra-short-period super-Earth with an extremely high density and an outer companion |
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Constraining the overcontact phase in massive binary evolution: III. Period stability of known B+B and O+B overcontact systems |
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Environmental Quenching of Low-surface-brightness Galaxies Near Hosts from Large Magellanic Cloud to Milky Way Mass Scales |
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Physical properties of trans-Neptunian object (143707) 2003 UY<SUB>117</SUB> derived from stellar occultation and photometric observations |
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Magnetic diffusion in solar atmosphere produces measurable electric fields |
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The abundance of clustered primordial black holes from quasar microlensing |
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The PAU survey: photometric redshift estimation in deep wide fields |
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A study of interacting galaxies from the Arp-Madore catalog: Triggering of star formation and nuclear activity |
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Dynamical system analysis and observational constraints of cosmological models in mimetic gravity |
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Results of the follow-up of ANTARES neutrino alerts |
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Good data in good and bad times: operations of the CARMENES radial-velocity survey at Calar Alto |
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LeMMINGs. Multiwavelength constraints on the co-existence of nuclear star clusters and AGN in nucleated galaxies |
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The hierarchical cosmic web and assembly bias |
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Constraints on Lorentz invariance violation from the extraordinary Mrk 421 flare of 2014 using a novel analysis method |
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First light simultaneous triple-channel optical observations of the OPTICAM system at the OAN-SPM |
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Gaia22dkvLb: A Microlensing Planet Potentially Accessible to Radial-velocity Characterization |
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Precise characterisation of HD 15337 with CHEOPS: A laboratory for planet formation and evolution |
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Scrutinizing evidence for the triggering of active galactic nuclei in the outskirts of massive galaxy clusters at z ≈ 1 |
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Bayesian inference methodology to characterize the dust emissivity at far-infrared and submillimeter frequencies |
iacweb |
3 months ago |
