0000000001197782
AUTHOR
D Wilken
Properties of the Binary Neutron Star Merger GW170817
On August 17, 2017, the Advanced LIGO and Advanced Virgo gravitational-wave detectors observed a low-mass compact binary inspiral. The initial sky localization of the source of the gravitational-wave signal, GW170817, allowed electromagnetic observatories to identify NGC 4993 as the host galaxy. In this work, we improve initial estimates of the binary's properties, including component masses, spins, and tidal parameters, using the known source location, improved modeling, and recalibrated Virgo data. We extend the range of gravitational-wave frequencies considered down to 23 Hz, compared to 30 Hz in the initial analysis. We also compare results inferred using several signal models, which ar…
Selinunt, Sizilien. Forschungen in Selinunt, Teil 1. Ein neues Modell für die Stadt Selinunt. Die Feldarbeiten des Jahres 2021
Since 2021, the German Research Foundation has been funding a new interdisciplinary field project to investigate the urban fabric of the Greek colony of Selinous in a spatially comprehensive and diachronic perspective. The project aims at extending the existing model of the ideal Greek city by considering also the historically conditioned fractures in the urban development and the multiple transformations of the living space between the 7th and 3rd century BCE. This is to be pursued by large scale archaeological, geophysical and geoarchaeological prospections, small excavations in selected areas and the thorough study of the finds and archaeobiological remains. This is a report about the fi…
Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
On 2017 August 17, the gravitational-wave event GW170817 was observed by the Advanced LIGO and Virgo detectors, and the gamma-ray burst (GRB) GRB 170817A was observed independently by the Fermi Gamma-ray Burst Monitor, and the Anticoincidence Shield for the Spectrometer for the International Gamma-Ray Astrophysics Laboratory. The probability of the near-simultaneous temporal and spatial observation of GRB 170817A and GW170817 occurring by chance is $5.0\times 10^{-8}$. We therefore confirm binary neutron star mergers as a progenitor of short GRBs. The association of GW170817 and GRB 170817A provides new insight into fundamental physics and the origin of short gamma-ray bursts. We use the ob…