Astrofísicas: Ondas gravitacionales

  • Publicación
    MASTER Optical Observation of LIGO/VIRGO S200302c Event
    The results of LIGO/Virgo S200302c (O3) error-box optical inspection by MASTER are presented. We observed 4242 square degrees square degrees inside 3σ error box...
  • Publicación
    Multi-messenger Observations of a Binary Neutron Star Merger
    On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves...
  • Publicación
    Observational constraints on the optical and near-infrared emission from the neutron star-black hole binary merger candidate S190814bv
    Context. Gravitational wave (GW) astronomy has rapidly reached maturity, becoming a fundamental observing window for modern astrophysics. The coalescences of a...
  • Publicación
    Observatory science with eXTP
    In this White Paper we present the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies related to Observatory Science targets...
  • Publicación
    Optical Spectroscopy of Candidates in the LIGO/Virgo Binary Merger Error Boxes
    We performed optical spectroscopy of the candidates inside the gravitational wave errorboxes (S190408an, S190425z, S190426c, S190510g, S190728q, S190814bv). The...
  • Publicación
    Panning for gold, but finding helium: Discovery of the ultra-stripped supernova SN 2019wxt from gravitational-wave follow-up observations
    We present the results from multi-wavelength observations of a transient discovered during an intensive follow-up campaign of S191213g, a gravitational wave (GW...
  • Charla
    Past, present and future of cosmic microwave background observations: implications for cosmology
    Since its discovery in 1964, the cosmic microwave background (CMB) has been one of the basic pillars of the cosmological model. However, it is only very...
  • Publicación
    Precision Ephemerides for Gravitational Wave Searches. II. Cyg X-2
    Accreting neutron stars in low-mass X-ray binaries are candidate high-frequency persistent gravitational wave sources. These may be detectable with next...
  • Publicación
    Precision Ephemerides for Gravitational-wave Searches - III. Revised system parameters of Sco X-1
    Neutron stars (NSs) in low-mass X-ray binaries are considered promising candidate sources of continuous gravitational waves. These NSs are typically rotating...