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...
-
-
PublicaciónOptical Spectroscopy of Candidates in the LIGO/Virgo Binary Merger Error BoxesWe performed optical spectroscopy of the candidates inside the gravitational wave errorboxes (S190408an, S190425z, S190426c, S190510g, S190728q, S190814bv). The...
-
PublicaciónPan-STARRS Follow-up of the Gravitational-wave Event S250818k and the Light Curve of SN2025ulzKilonovae are the scientifically rich—but observationally elusive—optical transient phenomena associated with compact binary mergers. Only a handful of events...
-
PublicaciónPanning for gold, but finding helium: Discovery of the ultra-stripped supernova SN 2019wxt from gravitational-wave follow-up observationsWe present the results from multi-wavelength observations of a transient discovered during an intensive follow-up campaign of S191213g, a gravitational wave (GW...
-
CharlaPast, present and future of cosmic microwave background observations: implications for cosmologySince 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...
-
PublicaciónPrecision Ephemerides for Gravitational Wave Searches. II. Cyg X-2Accreting neutron stars in low-mass X-ray binaries are candidate high-frequency persistent gravitational wave sources. These may be detectable with next...
-
PublicaciónPrecision Ephemerides for Gravitational-wave Searches - III. Revised system parameters of Sco X-1Neutron stars (NSs) in low-mass X-ray binaries are considered promising candidate sources of continuous gravitational waves. These NSs are typically rotating...
-
PublicaciónPrecision Ephemerides for Gravitational-wave Searches - IV. Corrected and refined ephemeris for Scorpius X-1Low-mass X-ray binaries have long been theorized as potential sources of continuous gravitational-wave radiation, yet there is no observational evidence from...
-
PublicaciónPrecision Ephemerides for Gravitational-wave Searches. I. Sco X-1Rapidly rotating neutron stars are the only candidates for persistent high-frequency gravitational wave emission, for which a targeted search can be performed...