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EXPORT: Near-IR observations of Vega-type and pre-main sequence stars |
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OJ 287 and the predicted fade of 1998 |
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An automatic procedure for a determination of the effective temperature and gravity - Application to 100 O-type stars |
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A New Bursting X-Ray Transient: SAX J1750.8-2900 |
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Burst-properties as a function of mass accretion rate in GX 3+1 |
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CCD photometry of stars in the old open cluster NGC 188 |
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Spectropolarimetry in a sunspot penumbra. Spatial dependence of Stokes asymmetries in Fe I 1564.8 nm |
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Stray-light measurements at the Observatorio del Teide |
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Oscillations in the Photosphere of a Sunspot Umbra from the Inversion of Infrared Stokes Profiles |
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Distributions, equivalent widths and metallicities of the H II regions in the spiral galaxies NGC 5457 and NGC 4395 |
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A 6.5-day periodicity in the recurrent nova V404 Cygni implying the presence of a black hole |
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Optical Studies of V:404-CYGNI the X-Ray Transient GS:2023+338 - Part Three - the Secondary Star and Accretion Disc |
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Evidence of a supernova origin for the black hole in the system GRO J1655 - 40 |
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VLT spectroscopy of XTE J2123-058 during quiescence: the masses of the two components |
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Rotational broadening and Doppler tomography of the quiescent X-ray nova Centaurus X-4 |
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The Optical Light Curves of XTE J2123-058. III. The Mass of the Binary Components and the Structure of the Quiescent Accretion Disk |
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Tidal Streams in the Galactic Halo: Evidence for the Sagittarius Northern Stream or Traces of a New Nearby Dwarf Galaxy |
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Time Series of Solar Granulation Images. III. Dynamics of Exploding Granules and Related Phenomena |
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Galactic Populations of Radio and Gamma-Ray Pulsars in the Polar Cap Model |
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A New Chemo-evolutionary Population Synthesis Model for Early-Type Galaxies. II. Observations and Results |
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Gamma ray Astrophysics: the multimessenger and Canarian connection |
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Six microlensing planets detected via sub-day signals during the 2023–2024 season |
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New kinematic map of the Milky Way bulge |
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Superresolution color images of Mars and Deimos acquired by the Hyperscout-H hyperspectral imager aboard the Hera mission |
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