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Detection of young (≤20 Myr) stellar populations in apparently quenched low-mass galaxies using red spectral line indices |
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Extended Point-spread Functions for Deep Astronomical Imaging Surveys |
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Broad-band spectral energy distribution of the X-ray transient Swift J1745-26 from outburst to quiescence |
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Constraining the nature of the accreting binary in CXOGBS J174623.5-310550 |
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Recent advancements in the EST project |
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Radio emission in ultracool dwarfs: The nearby substellar triple system VHS 1256-1257 |
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A photometric study of globular clusters observed by the APOGEE survey |
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Rayleigh-Taylor instabilities with sheared magnetic fields in partially ionised plasmas |
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Membership, lithium and chromospheric activity of the young open clusters IC 2391, IC 2602 and IC 4665 from GES (Gaia-ESO Survey) observations |
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Colors of barlenses: evidence for connecting them to boxy/peanut bulges |
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Time-series Analysis of Broadband Photometry of Neptune from K2 |
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The young open cluster NGC 7067 using Strömgren photometry |
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Comparing submillimeter polarized emission with near-infrared polarization of background stars for the Vela C molecular cloud |
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The Absolute Age of the Globular Cluster M15 Using Near-infrared Adaptive Optics Images from PISCES/LBT. |
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Beyond MHD: modeling and observation of partially ionized solar plasma processes |
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Period, epoch, and prediction errors of ephemerides from continuous sets of timing measurements |
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The High AV Quasar Survey: Reddened Quasi-Stellar Objects Selected from Optical/Near-Infrared Photometry—II |
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Mass accretion rates from multiband photometry in the Carina Nebula: the case of Trumpler 14 |
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Polarimetric and spectroscopic optical observations of the ultra-compact X-ray binary 4U 0614+091 |
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The GAPS programme with HARPS-N at TNG. IV. A planetary system around XO-2S |
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Probing the z > 6 Universe with the First Hubble Frontier Fields Cluster A2744 |
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Stellar Observations Network Group: The prototype is nearly ready |
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The deep spectrophotometric mosaic of the Orion Nebula. Preliminary results |
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On the Density Profile of the Globular Cluster M92 |
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Holographic imaging of crowded fields: high angular resolution imaging with excellent quality at very low cost |
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