P T H Pang
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Explore the profile of P T H Pang including associated specialties, affiliations and a list of published articles.
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Articles
17
Citations
178
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Recent Articles
1.
Acernese F, Agathos M, Ain A, Albanesi S, Allene C, Allocca A, et al.
Phys Rev Lett
. 2023 Aug;
131(4):041403.
PMID: 37566847
In this Letter, we present the design and performance of the frequency-dependent squeezed vacuum source that will be used for the broadband quantum noise reduction of the Advanced Virgo Plus...
2.
Abbott R, Abbott T, Acernese F, Ackley K, Adams C, Adhikari N, et al.
Phys Rev Lett
. 2022 Aug;
129(6):061104.
PMID: 36018635
We report on a search for compact binary coalescences where at least one binary component has a mass between 0.2 M_{⊙} and 1.0 M_{⊙} in Advanced LIGO and Advanced Virgo...
3.
Abbott R, Abbott T, Abraham S, Acernese F, Ackley K, Adams A, et al.
Phys Rev Lett
. 2021 Jul;
126(24):241102.
PMID: 34213926
We search for gravitational-wave signals produced by cosmic strings in the Advanced LIGO and Virgo full O3 dataset. Search results are presented for gravitational waves produced by cosmic string loop...
4.
Abbott B, Abbott R, Abbott T, Abraham S, Acernese F, Ackley K, et al.
Living Rev Relativ
. 2020 Oct;
23(1):3.
PMID: 33015351
We present our current best estimate of the plausible observing scenarios for the Advanced LIGO, Advanced Virgo and KAGRA gravitational-wave detectors over the next several years, with the intention of...
5.
Abbott R, Abbott T, Abraham S, Acernese F, Ackley K, Adams C, et al.
Phys Rev Lett
. 2020 Sep;
125(10):101102.
PMID: 32955328
On May 21, 2019 at 03:02:29 UTC Advanced LIGO and Advanced Virgo observed a short duration gravitational-wave signal, GW190521, with a three-detector network signal-to-noise ratio of 14.7, and an estimated...
6.
Acernese F, Agathos M, Aiello L, Allocca A, Amato A, Ansoldi S, et al.
Phys Rev Lett
. 2019 Dec;
123(23):231108.
PMID: 31868444
Current interferometric gravitational-wave detectors are limited by quantum noise over a wide range of their measurement bandwidth. One method to overcome the quantum limit is the injection of squeezed vacuum...
7.
Abbott B, Abbott R, Abbott T, Abraham S, Acernese F, Ackley K, et al.
Phys Rev Lett
. 2019 Nov;
123(16):161102.
PMID: 31702344
We present a search for subsolar mass ultracompact objects in data obtained during Advanced LIGO's second observing run. In contrast to a previous search of Advanced LIGO data from the...
8.
Abbott B, Abbott R, Abbott T, Acernese F, Ackley K, Adams C, et al.
Phys Rev Lett
. 2019 Aug;
123(1):011102.
PMID: 31386391
The recent discovery by Advanced LIGO and Advanced Virgo of a gravitational wave signal from a binary neutron star inspiral has enabled tests of general relativity (GR) with this new...
9.
Abbott B, Abbott R, Abbott T, Acernese F, Ackley K, Adams C, et al.
Phys Rev Lett
. 2019 Mar;
122(6):061104.
PMID: 30822067
We analyze the impact of a proposed tidal instability coupling p modes and g modes within neutron stars on GW170817. This nonresonant instability transfers energy from the orbit of the...
10.
Abbott B, Abbott R, Abbott T, Acernese F, Ackley K, Adams C, et al.
Phys Rev Lett
. 2018 Dec;
121(23):231103.
PMID: 30576173
We present the first Advanced LIGO and Advanced Virgo search for ultracompact binary systems with component masses between 0.2 M_{⊙}-1.0 M_{⊙} using data taken between September 12, 2015 and January...