Following the discovery of the gravitational-wave source GW170817 by three Laser Interferometer Gravitational-wave Observatory (LIGO)/Virgo antennae (Abbott et...
-
PublicationMASTER Optical Detection of the First LIGO/Virgo Neutron Star Binary Merger GW170817
-
PublicationMASTER 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...
-
PublicationMulti-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...
-
PublicationObservational 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...
-
PublicationObservatory 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...
-
PublicationOptical 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...
-
PublicationPanning 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...
-
TalkPast, 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...
-
PublicationPrecision 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...