| Publicación |
Coincidence between morphology and star formation activity through cosmic time: the impact of the bulge growth |
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Hace 2 months 1 week |
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Carbon Abundances in Compact Galactic Planetary Nebulae: An Ultraviolet Spectroscopic Study with the Space Telescope Imaging Spectrograph (STIS) |
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Hace 2 months 1 week |
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Photometric Signature of Ultraharmonic Resonances in Barred Galaxies |
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Hace 2 months 1 week |
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Polarization angle requirements for CMB B-mode experiments. Application to the LiteBIRD satellite |
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Detection of Gravitational Redshift in Open Cluster Nondegenerate Stars |
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Properties of the Be-type stars in 30 Doradus |
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The early afterglow of GRB 190829A |
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Measuring the mass of the black widow PSR J1555-2908 |
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Hace 2 months 1 week |
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Inferring the helium abundance of extragalactic globular clusters using integrated spectra |
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Hace 2 months 1 week |
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Velocity dispersion and dynamical masses for 388 galaxy clusters and groups. Calibrating the M<SUB>SZ</SUB> − M<SUB>dyn</SUB> scaling relation for the PSZ2 sample |
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The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: cosmological implications from multitracer BAO analysis with galaxies and voids |
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CHEOPS geometric albedo of the hot Jupiter HD 209458 b |
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The nature of the Cygnus extreme B supergiant 2MASS J20395358+4222505 |
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HD 207897 b: A dense sub-Neptune transiting a nearby and bright K-type star |
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Parameters of the eclipsing binary α Draconis observed by TESS and SONG |
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Hace 2 months 1 week |
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HATS-74Ab, HATS-75b, HATS-76b, and HATS-77b: Four Transiting Giant Planets Around K and M Dwarfs |
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Hace 2 months 1 week |
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Estimating fundamental parameters of nearby M dwarfs from SPIRou spectra |
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Fundamental physics with ESPRESSO: Precise limit on variations in the fine-structure constant towards the bright quasar HE 0515−4414 |
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K2-99 revisited: a non-inflated warm Jupiter, and a temperate giant planet on a 522-d orbit around a subgiant |
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Observational evidence for two-component distributions describing solar magnetic bright points |
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Euclid preparation. XVI. Exploring the ultra-low surface brightness Universe with Euclid/VIS |
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Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertainty |
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Dark Energy Survey Year 3 Results: Measuring the Survey Transfer Function with Balrog |
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The building up of observed stellar scaling relations of massive galaxies and the connection to black hole growth in the TNG50 simulation |
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On the most luminous planetary nebulae of M 31 |
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