Directed searches for continuous gravitational waves from twelve supernova remnants in data from Advanced LIGO's second observing run

Abstract

We describe directed searches for continuous gravitational waves from twelve well localized non-pulsing candidate neutron stars in young supernova remnants using data from Advanced LIGO's second observing run. We assumed that each neutron star is isolated and searched a band of frequencies from 15 to 150\,Hz, consistent with frequencies expected from known young pulsars. After coherently integrating spans of data ranging from 12.0 to 55.9 days using the F-statistic and applying data-based vetoes, we found no evidence of astrophysical signals. We set upper limits on intrinsic gravitational wave amplitude in some cases stronger than 10^{-25}, generally about a factor of two better than upper limits on the same objects from Advanced LIGO's first observing run.

v2 updated to version accepted for publication in Physical Review D

References in corpus (18)

• The ATNF Pulsar Catalogue
• The LIGO Open Science Center
• The Youngest Galactic Supernova Remnant: G1.9+0.3
• All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO O2 data
• Directional limits on persistent gravitational waves from Advanced LIGO's first observing run
• Searching for gravitational waves from Cassiopeia A with LIGO
• Spinning down newborn neutron stars: nonlinear development of the r-mode instability
• How to adapt broad-band gravitational-wave searches for r-modes
• Discovery of the radio and X-ray counterpart of TeV Gamma-ray source HESS J1731-347
• DA495 - an aging pulsar wind nebula
• The (Re-)Discovery of G350.1-0.3: A Young, Luminous Supernova Remnant and Its Neutron Star
• A New Young Galactic Supernova Remnant Containing a Compact Object: G15.9+0.2
• Candidate radio supernova remnants observed by the GLEAM survey over $345^{\circ }<l<60^{\circ }$ and $180^{\circ }<l<240^{\circ }$
• An Einstein@home search for continuous gravitational waves from Cassiopeia A
• Cross-correlation search for continuous gravitational waves from a compact object in SNR 1987A in LIGO Science Run 5
• Discovery of a Candidate Central Compact Object in the Galactic Nonthermal SNR G330.2+1.0
• Chandra View of DA 530: A Sub-Energetic Supernova Remnant with a Pulsar Wind Nebula?
• Chandra Confirmation of a Pulsar Wind Nebula in DA 495

Cited by in corpus (22)

• Searches for Continuous-Wave Gravitational Radiation
• Searches for continuous gravitational waves from neutron stars: A twenty-year retrospective
• Narrowband searches for continuous and long-duration transient gravitational waves from known pulsars in the LIGO-Virgo third observing run
• Search methods for continuous gravitational-wave signals from unknown sources in the advanced-detector era
• Status and perspectives of Continuous Gravitational Wave searches
• Search for Continuous Gravitational Waves from the Central Compact Objects in Supernova Remnants Cassiopeia A, Vela Jr. and G347.3-0.5
• Search for gravitational waves from twelve young supernova remnants with a hidden Markov model in Advanced LIGO's second observing run
• New searches for continuous gravitational waves from seven fast pulsars
• First searches for gravitational waves from r-modes of the Crab pulsar
• Deep exploration for continuous gravitational waves at 171--172 Hz in LIGO second observing run data
• Search for continuous gravitational waves from Fomalhaut b in the second Advanced LIGO observing run with a hidden Markov model
• Results from an Einstein@Home search for continuous gravitational waves from G347.3 at low frequencies in LIGO O2 data
• First Constraining Upper Limits on Gravitational Wave Emission from NS 1987A in SNR 1987A
• Anisotropic neutron star crust, solar system mountains, and gravitational waves
• Geometric Approach to Analytic Marginalisation of the Likelihood Ratio for Continuous Gravitational Wave Searches
• Search for continuous gravitational waves from HESS~J1427-608 with a hidden Markov model
• Population synthesis and parameter estimation of neutron stars with continuous gravitational waves and third-generation detectors
• Searches for continuous gravitational waves from young supernova remnants in the early third observing run of Advanced LIGO and Virgo
• Harnessing the potential of PyStoch: detecting continuous gravitational waves from interesting supernova remnant targets
• Results from an Einstein@Home search for continuous gravitational waves from Cassiopeia A and Vela Jr. using LIGO O2 data
• Searches for Continuous Gravitational Waves from Supernova Remnants in the first part of the LIGO-Virgo-KAGRA Fourth Observing run
• Gravitational waves from spinning neutron stars as not-quite-standard sirens