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Discovery of optical and infrared accretion disc wind signatures in the black hole candidate MAXI J1348-630 |
iacweb |
Hace 1 month |
| Publicación |
Evolution of thermal and non-thermal radio continuum emission on kpc scales - predictions for SKA |
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Dark energy survey year 3 results: cosmological constraints from the analysis of cosmic shear in harmonic space |
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Pegasus V/Andromeda XXXIV-a newly discovered ultrafaint dwarf galaxy on the outskirts of Andromeda |
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The luminosity of cluster galaxies in the Cluster-EAGLE simulations |
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Doubling of minute-long quasi-periodic pulsations from super-flares on a low-mass star |
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Stellar migration in the Auriga simulations |
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The black hole population in low-mass galaxies in large-scale cosmological simulations |
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Searching for technosignatures in exoplanetary systems with current and future missions |
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ASTRI Mini-Array core science at the Observatorio del Teide |
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The Pristine survey - XVII. The C-19 stream is dynamically hot and more extended than previously thought |
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The young HD 73583 (TOI-560) planetary system: two 10-M<SUB>⊕</SUB> mini-Neptunes transiting a 500-Myr-old, bright, and active K dwarf |
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Hace 1 month |
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Atmospheric characterization of terrestrial exoplanets in the mid-infrared: biosignatures, habitability, and diversity |
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Occulter to earth: prospects for studying earth-like planets with the E-ELT and a space-based occulter |
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LUMINARIES IN THE SKY: THE TESS LEGACY SAMPLE OF BRIGHT STARS. II. In depth seismic characterisation of the 34 luminaries found in the PLATO LOP fields |
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Tales of stellar and binary co-evolutionand stellar cannibalism |
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Towards space-qualification of astrophotonic devices in the optical/IR |
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Unlocking Kepler's Full Potential with Gaia DR3: Color-Magnitude Diagram, Binary Systems, and Galactic Kinematics |
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From the Main Sequence to the Red Giant Branch: Asteroseismology of Solar-like Oscillators |
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Measuring Rotation Periods from TESS in PLATO LOPS2 Fields |
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Is turbulent convection the only exciting mechanism of acoustic modes in solar-like oscillators? |
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Ensemble Boutique Modeling of Kepler Giants |
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When stars speak too fast: probing the first dredge up beyond the Nyquist frequency |
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Finding the sweet spot: Modelling of oscillating red giant binaries |
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Characterising six solar analogues observed by Kepler, K2, and Hermes |
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