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Absence of nuclear polycyclic aromatic hydrocarbon emission from a compact starburst: The case of the type-2 quasar Mrk 477 |
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Backscattering and Line Broadening in Orion |
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Mass Production of 2021 KMTNet Microlensing Planets. III. Analysis of Three Giant Planets |
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Site selection for the Hayabusa2 artificial cratering and subsurface material sampling on Ryugu |
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Dark Energy Survey Year 3 results: Measurement of the baryon acoustic oscillations with three-dimensional clustering |
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Lower-than-expected flare temperatures for TRAPPIST-1 |
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CO in the ALMA Radio-source Catalogue (ARC): The molecular gas content of radio galaxies as a function of redshift |
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Fossil group origins. XII. The large-scale environment around fossil systems |
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Large Ion-neutral Drift Velocities and Plasma Heating in Partially Ionized Coronal Rain Blobs |
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On the Characterization of GJ 504: A Magnetically Active Planet-host Star Observed by the Transiting Exoplanet Survey Satellite (TESS) |
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The new multi-frequency instrument (MFI2) for the QUIJOTE facility in Tenerife |
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The Gravitational-wave Optical Transient Observer (GOTO) |
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GRANCAIN: the first light infrared camera for the adaptive optics of GTC: optical and mechanical design status |
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Constraining the overcontact phase in massive binary evolution. II. Period stability of known O+O overcontact systems |
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StraKLIP: A Novel Pipeline for Detection and Characterization of Close-in Faint Companions through the Karhunen-Loéve Image Processing Algorithm |
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A Mass Model for the Lensing Cluster SDSS J1004+4112: Constraints from the Third Time Delay |
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Development of Fast and Precise Scan Mirror Mechanism for an Airborne Solar Telescope |
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KMT-2021-BLG-0171Lb and KMT-2021-BLG-1689Lb: two microlensing planets in the KMTNet high-cadence fields with followup observations |
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Euclid preparation. XX. The Complete Calibration of the Color-Redshift Relation survey: LBT observations and data release |
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A Multi-epoch, Multiwavelength Study of the Classical FUor V1515 Cyg Approaching Quiescence |
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J-PLUS: Detecting and studying extragalactic globular clusters. The case of NGC 1023 |
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The BINGO Project. III. Optical design and optimization of the focal plane |
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The BINGO project. II. Instrument description |
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Lessons from the massive relic NGC 1277: Remaining in situstar formation in the cores of massive galaxies |
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