| Publicación |
Disentangling the Galactic Halo with APOGEE. II. Chemical and Star Formation Histories for the Two Distinct Populations |
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Metallicity gradient of the thick disc progenitor at high redshift |
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The origin of the LMC stellar bar: clues from the SFH of the bar and inner disc |
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Elemental Abundances of Kepler Objects of Interest in APOGEE. I. Two Distinct Orbital Period Regimes Inferred from Host Star Iron Abundances |
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NIHAO - XIV. Reproducing the observed diversity of dwarf galaxy rotation curve shapes in ΛCDM |
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C/O ratios in planetary nebulae with dual-dust chemistry from faint optical recombination lines |
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An application of an optimal statistic for characterizing relative orientations |
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A dearth of small particles in the transiting material around the white dwarf WD 1145+017 |
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Overdensity of galaxies in the environment of quasar pairs |
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Magneto-optical Effects in the Scattering Polarization Wings of the Ca I 4227 Å Resonance Line |
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A search for optical bursts from the repeating fast radio burst FRB 121102 |
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A cut-off in the TeV gamma-ray spectrum of the SNR Cassiopeia A |
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Search for very high-energy gamma-ray emission from the microquasar Cygnus X-1 with the MAGIC telescopes |
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Observations of the galaxy cluster CIZA J2242.8+5301 with the Sardinia Radio Telescope |
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The First Post-Kepler Brightness Dips of KIC 8462852 |
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K2-106, a system containing a metal-rich planet and a planet of lower density |
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Surges and Si IV Bursts in the Solar Atmosphere: Understanding IRIS and SST Observations through RMHD Experiments |
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Intermittent Reconnection and Plasmoids in UV Bursts in the Low Solar Atmosphere |
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Planck intermediate results. LI. Features in the cosmic microwave background temperature power spectrum and shifts in cosmological parameters |
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Search for light bosons in decays of the 125 GeV Higgs boson in proton-proton collisions at √{s}=8 TeV |
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Rise of the Titans: A Dusty, Hyper-luminous “870 μm Riser” Galaxy at z ∼ 6 |
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SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES): Faint-end Counts at 450 μm |
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Low-metallicity (sub-SMC) massive stars |
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Charge-transfer interaction between C60 fullerene and alkylnaphthalenes |
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Alone on a wide wide sea. The origin of SECCO 1, an isolated star-forming gas cloud in the Virgo cluster*†‡ |
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