Astrophysical: Galaxies

  • Publication
    Control sample for galaxy pairs: Simulations and Observations
    Several attempts have been made in order to isolate the effect of galaxy interactions by comparing galaxy in pairs with isolated galaxies. However, different...
  • Publication
    Converting Hα Luminosities into Star Formation Rates
    Star formation rates (SFRs) of galaxies are commonly calculated by converting the measured Hα luminosities (LHα) into current SFRs. This conversion is based on...
  • Publication
    Convolutional neural network-reconstructed velocity for kinetic SZ detection
    We report the detection of the kinetic Sunyaev-Zel'dovich (kSZ) effect in galaxy clusters with a 4.9σ significance using the latest 217 GHz Planck map from data...
  • Publication
    Cool Gas and Massive Stars: The Nuclear Ring in M100
    The SAURON integral-field spectrograph was used to observe the central area of the barred spiral galaxy M100 (NGC 4321). M100 contains a nuclear ring of star...
  • Publication
    Coordinated Multiwavelength Observation of 3C 66A during the WEBT Campaign of 2003-2004
    The BL Lac object 3C 66A was the target of an extensive multiwavelength monitoring campaign from 2003 July through 2004 April (with a core campaign from 2003...
  • Publication
    Coronal line forest AGN - II. Analysis of the spectral energy distribution
    Coronal-Line Forest Active Galactic Nuclei (CLiF AGN) are characterized by strong, high-ionization lines, which are in contrast to what is found in typical AGNs...
  • Publication
    Coronal-line forest active galactic nuclei - I. Physical properties of the emission-line regions
    Coronal-line forest (CLiF) active galactic nuclei (AGNs) are characterized by strong high-ionization lines, which contrasts with what is found in most AGNs...
  • Publication
    Coronal-line forest active galactic nuclei - I. Physical properties of the emission-line regions
    Coronal-line forest (CLiF) active galactic nuclei (AGNs) are characterized by strong high-ionization lines, which contrasts with what is found in most AGNs...
  • Publication
    Correction to: Strong CO absorption features in massive ETGs