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Galaxy transformation across the cosmic web: The influence zone of filaments |
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1 month 3 weeks ago |
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Spatially resolved star formation relations in local luminous infrared galaxies along the complete merger sequence |
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Flexible simulation-based inference for galaxy photometric fitting with synthesizer |
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Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra-I cluster: V. Integrated stellar population properties |
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Optical spectral characterization of OP 313: Constraining the contribution of thermal and non-thermal optical emission |
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Binarity at LOw Metallicity (BLOeM): Projected rotational velocities |
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Appraising the Necklace: A post-common-envelope carbon dwarf inside an apparently carbon-poor planetary nebula |
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First detection of VHE gamma-ray signal from the FSRQ TON 0599 |
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TOI-3862 b: A dense super-Neptune deep in the hot Neptune desert |
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Constraints on CMBR Flux due to High-z Dust Emission |
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Cloudy Extrasolar Skies in the JWST Era and their Dependence on Atmospheric Properties |
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The Photometric Analysis of the Environment Around Two Dusty Star-Forming Galaxies at z ~ 2 |
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Preliminary Physical Parameters for the Close Binary in the Planetary Nebula Pa 164 |
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The Spin-Down Stalling Signature Persists in Chromospheric Magnetic Activity |
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JWST Spectra are Consistent with the Edge-on Star-forming Galaxy Scenario for the "Runaway Supermassive Black Hole" |
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Polarization properties of changing-look active galactic nuclei: NGC 1365 and NGC 2992 |
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Gaia20dsk: A new MNor discovered by the GLORIOUS collaboration |
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Properties of Polarized Radio Sources in the Wide Chandra Deep Field South from 2 to 4 GHz |
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A redshift-independent theoretical halo mass function validated with UCHUU simulations |
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