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Chemodynamically Characterizing the Jhelum Stellar Stream with APOGEE-2 |
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Baryon acoustic oscillations from Integrated Neutral Gas Observations: Broadband corrugated horn construction and testing |
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The variable radio counterpart of Swift J1858.6-0814 |
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Low optical polarization at the core of the optically thin jet of M87 |
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The K2 Galactic Caps Project - going beyond the Kepler field and ageing the Galactic disc |
iacweb |
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Fundamentals of horn antennas with low cross-polarization levels for radioastronomy and satellite communications |
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The diagnostic potential of the weak field approximation for investigating the quiet Sun magnetism: the Si I 10 827 Å line |
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Compositional characterization of V-type candidate asteroids identified using the MOVIS catalogue |
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Physical and dynamical properties of the unusual V-type asteroid (2579) Spartacus |
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AGILE, Fermi, Swift, and GASP/WEBT multi-wavelength observations of the high-redshift blazar 4C +71.07 in outburst |
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Aerosols and Water Ice in Jupiter’s Stratosphere from UV-NIR Ground-based Observations |
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Signatures of the Galactic bar on stellar kinematics unveiled by APOGEE |
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Abundance ratios in dwarf elliptical galaxies |
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Exploring cosmic origins with CORE: Cluster science |
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Exploring cosmic origins with CORE: Extragalactic sources in cosmic microwave background maps |
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Multi-Wavelength Monitoring of the Changing-Look AGN NGC 2617 during State Changes |
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Three Small Planets Transiting a Hyades Star |
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Hungaria asteroid region telescopic spectral survey (HARTSS) I: Stony asteroids abundant in the Hungaria background population |
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Bayesian coronal seismology |
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Comparison of Solar Fine Structure Observed Simultaneously in Lyα and Mg ii h |
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The Strong Gravitationally Lensed Herschel Galaxy HLock01: Optical Spectroscopy Reveals a Close Galaxy Merger with Evidence of Inflowing Gas |
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A Si I atomic model for NLTE spectropolarimetric diagnostics of the 10 827 Å line |
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The puzzling case of the accreting millisecond X-ray pulsar IGR J00291+5934: flaring optical emission during quiescence |
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The optical counterpart to the Be/X-ray binary SAX J2239.3+6116 |
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Discovery of a Very Bright and Intrinsically Very Luminous, Strongly Lensed Lyα Emitting Galaxy at z = 2.82 in the BOSS Emission-Line Lens Survey |
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