Publication type: Refereed

  • Publication
    Forecasting the success of the WEAVE Wide-Field Cluster Survey on the extraction of the cosmic web filaments around galaxy clusters
    Next-generation wide-field spectroscopic surveys will observe the infall regions around large numbers of galaxy clusters with high sampling rates for the first...
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    Foreground Contributions to 0.2-2° CMB Anisotropies
    We examine the extent to which galactic and extragalactic foregrounds can hamper the detection of primordial Cosmic Microwave background (CMB) anisotropies. We...
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    FOREVER22: galaxy formation in protocluster regions
    We present results from a new cosmological hydrodynamics simulation campaign of protocluster (PC) regions, FOREVER22: FORmation and EVolution of galaxies in...
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    Foreword
    Not Available
  • Publication
    Formation and Evolution of a Multi-threaded Solar Prominence
    We investigate the process of formation and subsequent evolution of prominence plasma in a filament channel and its overlying arcade. We construct a three...
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    Formation and evolution of carbonaceous asteroid Ryugu: Direct evidence from returned samples
    Samples of the carbonaceous asteroid Ryugu were brought to Earth by the Hayabusa2 spacecraft. We analyzed seventeen Ryugu samples measuring 1-8 mm. CO2-bearing...
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    Formation and evolution of dwarf early-type galaxies in the Virgo cluster. II. Kinematic scaling relations
    We place our sample of 18 Virgo dwarf early-type galaxies (dEs) on the (V - K)e-velocity dispersion, Faber-Jackson, and fundamental plane (FP) scaling relations...
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    Formation and evolution of S0 galaxies: a SAURON case study of NGC 7332
    We present SAURON integral-field observations of the S0 galaxy NGC 7332. Existing broad-band ground-based and Hubble Space Telescope (HST) photometry reveals a...
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    Formation and morphology of anomalous solar circular polarization
    Context. The morphology of spectral line polarization is the most valuable observable to investigate the magnetic and dynamic solar atmosphere. However, in...