Publication type: Refereed

  • Publication
    Concerning colour: The effect of environment on type Ia supernova colour in the dark energy survey
    Recent analyses have found intriguing correlations between the colour (c) of type Ia supernovae (SNe Ia) and the size of their 'mass-step', the relationship...
  • Publication
    Concerning the Existence of a ``Turbulent'' Magnetic Field in the Quiet Sun
    We report on the a5F-y5Fo multiplet of Ti I and its interest for the study of ``turbulent'' magnetic fields in the quiet solar photosphere. In particular, we...
  • Publication
    CONCERTO at APEX On-sky performance in continuum
    Context. CarbON CII line in post-rEionisation and ReionisaTiOn epoch (CONCERTO) instrument is a low-resolution mapping spectrometer based on lumped element...
  • Publication
    Condensation of dust around the Wolf-Rayet star WR 125
    Infrared photometry of the WC7-type Wolf-Rayet star WR 125 (MR 93) in 1981-91 shows a 10-fold rise in the 3-4 micron flux during 1990-91. This, together with...
  • Publication
    Conditions for Reionizing the Universe with a Low Galaxy Ionizing Photon Escape Fraction
    We explore scenarios for reionizing the intergalactic medium with low galaxy ionizing photon escape fractions. We combine simulation-based halo mass–dependent...
  • Publication
    Conducting the SONG: The Robotic Nature and Efficiency of a Fully Automated Telescope
    We present a description of “the Conductor,” an automated software package that handles all observations at the first Stellar Observations Network Group (SONG)...
  • Publication
    Confidence levels of evolutionary synthesis models
    The stochastic nature of the IMF in young stellar clusters implies that clusters of the same mass and age do not present the same unique values of their...
  • Publication
    Confidence levels of evolutionary synthesis models. II. On sampling and Poissonian fluctuations
    In terms of statistical fluctuations, stellar population synthesis models are only asymptotically correct in the limit of a large number of stars, where...
  • Publication
    Confidence Limits of Evolutionary Synthesis Models
    The probabilistic nature of the IMF in stellar systems implies that clusters of the same mass and age do not present the same unique values of their observed...