Astrophysical: Methods

  • Publication
    Milne-Eddington inversion of the Fe I line pair at 630 nm
    Context. The iron lines at 630.15 and 630.25 nm are often used to determine the physical conditions of the solar photosphere. A common approach is to invert...
  • Publication
    Mineralogical analysis of 14 PHAs from ViNOS data
    Potentially hazardous asteroids (PHAs) are objects that can have close encounters with Earth and are significantly large to cause significant regional damage in...
  • Publication
    Mini-moons from horseshoes: A physical characterization of 2022 NX<SUB>1</SUB> with OSIRIS at the 10.4 m Gran Telescopio Canarias
    Context. The near-Earth orbital space is shared by natural objects and space debris that can be temporarily captured in geocentric orbits. Short-term natural...
  • Publication
    Mining the ESO WFI and INT WFC archives for known Near Earth Asteroids. Mega-Precovery software
    The ESO/MPG WFI and the INT WFC wide field archives comprising 330 000 images were mined to search for serendipitous encounters of known Near Earth Asteroids...
  • Publication
    Minor axis kinematics of 19 S0-Sbc bulges
    We present minor axis kinematic profiles for a well-studied sample of 19 early- to intermediate-type disk galaxies. We introduce, for the first time, the use of...
  • Publication
    Misleading variations in estimated rotational frequency splittings of solar p modes: consequences for helioseismology and asteroseismology
    The aim of this paper is to investigate whether there are any 11-yr or quasi-biennial solar-cycle-related variations in solar rotational splitting frequencies...
  • Publication
    Mode visibilities in radial velocity and photometric Sun-as-a-star helioseismic observations
    We analyze more than 5000 days of high-quality Sun-as-a-star, radial velocity GOLF and photometric VIRGO/SPM helioseismic observations to extract precise...
  • Publication
    Model Comparison for the Density Structure across Solar Coronal Waveguides
    The spatial variation of physical quantities, such as the mass density, across solar atmospheric waveguides governs the timescales and spatial scales for wave...
  • Publication
    Model comparison for the density structure along solar prominence threads
    Context. Quiescent solar prominence fine structures are typically modelled as density enhancements, called threads, which occupy a fraction of a longer magnetic...