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T. Sadecki

Researcher at National Science Foundation

Publications -  166
Citations -  55022

T. Sadecki is an academic researcher from National Science Foundation. The author has contributed to research in topics: LIGO & Gravitational wave. The author has an hindex of 71, co-authored 156 publications receiving 43516 citations.

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Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory

Arnauld Albert, +1932 more
TL;DR: In this article, the authors search for high-energy neutrinos from the binary neutron star merger in the GeV-EeV energy range using the ANTARES, IceCube, and Pierre Auger Observatories.
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Effects of waveform model systematics on the interpretation of GW150914

B. P. Abbott, +1033 more
TL;DR: In this paper, the effects of possible systematic errors in the waveform models on estimates of its source parameters were investigated and no evidence for a systematic bias relative to the statistical error of the original parameter recovery of GW150914 due to modeling approximations or modeling inaccuracies was found.
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Identification and mitigation of narrow spectral artifacts that degrade searches for persistent gravitational waves in the first two observing runs of Advanced LIGO

P. B. Covas, +262 more
- 22 Jan 2018 - 
TL;DR: In this paper, a variety of methods used for finding, identifying and mitigating these artifacts, illustrated with particular examples, are described in the form of lists of line artifacts that can safely be treated as non-astrophysical.
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Search for Subsolar-Mass Ultracompact Binaries in Advanced LIGO’s First Observing Run

B. P. Abbott, +1260 more
TL;DR: The null result constrains the coalescence rate of monochromatic (delta function) distributions of nonspinning in primordial black hole binary formation scenario and strengthens the presently placed bounds from microlensing surveys of massive compact halo objects (MACHOs) provided by the MACHO and EROS Collaborations.
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Directional Limits on Persistent Gravitational Waves from Advanced LIGO’s First Observing Run

B. P. Abbott, +1018 more
TL;DR: Directed searches for narrowband gravitational waves from astrophysically interesting objects yield median frequency-dependent limits on strain amplitude at the most sensitive detector frequencies between 130-175 Hz, which represents a mean improvement of a factor of 2 across the band compared to previous searches of this kind.