A directed search for continuous Gravitational Waves from the Galactic Center
arXiv:1309.6221 · doi:10.1103/PhysRevD.88.102002
Abstract
We present the results of a directed search for continuous gravitational waves from unknown, isolated neutron stars in the Galactic Center region, performed on two years of data from LIGO's fifth science run from two LIGO detectors. The search uses a semi-coherent approach, analyzing coherently 630 segments, each spanning 11.5 hours, and then incoherently combining the results of the single segments. It covers gravitational wave frequencies in a range from 78 to 496 Hz and a frequency-dependent range of first order spindown values down to -7.86 x 10^-8 Hz/s at the highest frequency. No gravitational waves were detected. We place 90% confidence upper limits on the gravitational wave amplitude of sources at the Galactic Center. Placing 90% confidence upper limits on the gravitational wave amplitude of sources at the Galactic Center, we reach ~3.35x10^-25 for frequencies near 150 Hz. These upper limits are the most constraining to date for a large-parameter-space search for continuous gravitational wave signals.
12 pages, 3 figures, 1 table; PDFLaTeX; to be published in Phys.Rev.D; a science summary can be found at http://www.ligo.org/science/Publication-GCSearch/index.php
References in corpus (42)
- The ATNF Pulsar Catalogue
- The Galactic Center Massive Black Hole and Nuclear Star Cluster
- LIGO: The Laser Interferometer Gravitational-Wave Observatory
- Detector configuration of KAGRA - the Japanese cryogenic gravitational-wave detector
- Data analysis of gravitational-wave signals from spinning neutron stars. I. The signal and its detection
- Neutron Star Mass Measurements. I. Radio Pulsars
- The Accelerations of Stars Orbiting the Milky Way's Central Black Hole
- Maximum elastic deformations of compact stars with exotic equations of state
- Searching for periodic sources with LIGO. II: Hierarchical searches
- Beating the spin-down limit on gravitational wave emission from the Crab pulsar
- Setting upper limits on the strength of periodic gravitational waves using the first science data from the GEO600 and LIGO detectors
- Maximum elastic deformations of relativistic stars
- Observational constraints on hyperons in neutron stars
- Coherent searches for periodic gravitational waves from unknown isolated sources and Scorpius X-1: results from the second LIGO science run
- The generalized F-statistic: multiple detectors and multiple GW pulsars
- Beating the spin-down limit on gravitational wave emission from the Vela pulsar
- Searches for gravitational waves from known pulsars with S5 LIGO data
- Probing the Spacetime Around Sgr A* with Radio Pulsars
- First search for gravitational waves from the youngest known neutron star
- All-sky search for periodic gravitational waves in LIGO S4 data
- The Einstein@Home search for periodic gravitational waves in LIGO S4 data
- A strongly magnetized pulsar within grasp of the Milky Way's supermassive black hole
- Spinning down newborn neutron stars: nonlinear development of the r-mode instability
- Multiwavelength Constraints on Pulsar Populations in the Galactic Center
- How to adapt broad-band gravitational-wave searches for r-modes
- Upper limit map of a background of gravitational waves
- Discovery of Three Pulsars from a Galactic Center Pulsar Population
- Einstein@Home all-sky search for periodic gravitational waves in LIGO S5 data
- Directional limits on persistent gravitational waves using LIGO S5 science data
- Einstein@Home search for periodic gravitational waves in early S5 LIGO data
- First all-sky upper limits from LIGO on the strength of periodic gravitational waves using the Hough transform
- All-sky LIGO Search for Periodic Gravitational Waves in the Early S5 Data
- Discovery of two pulsars towards the Galactic Centre
- All-sky Search for Periodic Gravitational Waves in the Full S5 LIGO Data
- Constraints on the dense matter EOS from the measurements of PSR J0737-3039A moment of inertia and PSR J0751+1807 mass
- Exploiting Large-Scale Correlations to Detect Continuous Gravitational Waves
- Are neutron stars with crystalline colour superconducting cores interesting for the LIGO experiment?
- Estimating the sensitivity of wide-parameter-space searches for gravitational-wave pulsars
- A Catalog of Diffuse X-ray-Emitting Features within 20 pc of Sgr A*: Twenty Pulsar Wind Nebulae?
- Parameter-space correlations of the optimal statistic for continuous gravitational-wave detection
- Search for Periodic Gravitational Wave Sources with the Explorer Detector
- Constraining crystalline color superconducting quark matter with gravitational-wave data
Cited by in corpus (61)
- Gravitational waves from known pulsars: results from the initial detector era
- 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
- Searches for Continuous-Wave Gravitational Radiation
- The Milky Way's Supermassive Black Hole: How good a case is it? A Challenge for Astrophysics & Philosophy of Science
- Search for anisotropic gravitational-wave backgrounds using data from Advanced LIGO and Advanced Virgo's first three observing runs
- Astromaterial Science and Nuclear Pasta
- First low-frequency Einstein@Home all-sky search for continuous gravitational waves in Advanced LIGO data
- Continuous gravitational waves from neutron stars: current status and prospects
- Postprocessing methods used in the search for continuous gravitational-wave signals from the Galactic Center
- Searches for Continuous Gravitational Waves from Fifteen Supernova Remnants and Fomalhaut b with Advanced LIGO
- Fast and Accurate Sensitivity Estimation for Continuous-Gravitational-Wave Searches
- Search for continuous gravitational waves: Improving robustness versus instrumental artifacts
- Searches for continuous gravitational waves from nine young supernova remnants
- Searches for continuous gravitational waves from neutron stars: A twenty-year retrospective
- Directional limits on persistent gravitational waves using data from Advanced LIGO's first two observing runs
- Directed searches for continuous gravitational waves from binary systems: parameter-space metrics and optimal Scorpius X-1 sensitivity
- Mis-Modelling in Gravitational Wave Astronomy: The Trouble With Templates
- A new data analysis framework for the search of continuous gravitational wave signals
- Hidden Markov model tracking of continuous gravitational waves from a binary neutron star with wandering spin. II. Binary orbital phase tracking
- Einstein@Home all-sky search for continuous gravitational waves in LIGO O2 public data
- Gravitational Waves from Compact Dark Objects in Neutron Stars
- Robust semicoherent searches for continuous gravitational waves with noise and signal models including hours to days long transients
- Directed search for continuous gravitational-wave signals from the Galactic Center in the Advanced LIGO second observing run
- First search for long-duration transient gravitational waves after glitches in the Vela and Crab pulsars
- Second Einstein Telescope Mock Data and Science Challenge: Low Frequency Binary Neutron Star Data Analysis
- Flat parameter-space metric for all-sky searches for gravitational-wave pulsars
- Hierarchical follow-up of sub-threshold candidates of an all-sky Einstein@Home search for continuous gravitational waves on LIGO sixth science run data
- Results of the deepest all-sky survey for continuous gravitational waves on LIGO S6 data running on the Einstein@Home volunteer distributed computing project
- All-sky search for long-duration gravitational wave transients with LIGO
- Optimal directed searches for continuous gravitational waves
- Directed searches for continuous gravitational waves from twelve supernova remnants in data from Advanced LIGO's second observing run
- Search for gravitational waves from twelve young supernova remnants with a hidden Markov model in Advanced LIGO's second observing run
- Adaptive clustering procedure for continuous gravitational wave searches
- Application of a hierarchical MCMC follow-up to Advanced LIGO continuous gravitational-wave candidates
- Bayesian parameter estimation of core collapse supernovae using gravitational wave simulations
- Search for continuous gravitational waves from neutron stars in globular cluster NGC 6544
- Empirically estimating the distribution of the loudest candidate from a gravitational-wave search
- Cross-correlation method for intermediate-duration gravitational wave searches associated with gamma-ray bursts
- Empirically extending the range of validity of parameter-space metrics for all-sky searches for gravitational-wave pulsars
- Search for transient gravitational waves in coincidence with short duration radio transients during 2007-2013
- Optimally setting up directed searches for continuous gravitational waves in Advanced LIGO O1 data
- Banks of templates for all-sky narrow-band searches of gravitational waves from spinning neutron stars
- Stochastic gravitational-wave background searches and constraints on neutron-star ellipticity
- Prospects for Multimessenger Observations of Thorne-Żytkow Objects
- First Constraining Upper Limits on Gravitational Wave Emission from NS 1987A in SNR 1987A
- Novel directed search strategy to detect continuous gravitational waves from neutron stars in low- and high-eccentricity binary systems
- Optimizing the third generation of gravitational-wave observatories for Galactic astrophysics
- Fully coherent follow-up of continuous gravitational-wave candidates: an application to Einstein@Home results
- Probing the Fermi-LAT GeV excess with gravitational waves
- Results of an all-sky high-frequency Einstein@Home search for continuous gravitational waves in LIGO's fifth science run
- Line-robust statistics for continuous gravitational waves: safety in the case of unequal detector sensitivities
- Density-clustering of continuous gravitational wave candidates from large surveys
- Optimizing StackSlide setup and data selection for continuous-gravitational-wave searches in realistic detector data
- Prospects for the observation of continuous gravitational waves from spinning neutron stars lensed by the galactic supermassive black hole
- Gravitational Wave Searches for Post-Merger Remnants of GW170817 and GW190425
- Gravitational-wave searches in the era of Advanced LIGO and Virgo
- Searches for continuous gravitational waves from young supernova remnants in the early third observing run of Advanced LIGO and Virgo
- Target-based Optimization of Advanced Gravitational-Wave Detector Network Operations
- Gravitational waves from spinning neutron stars as not-quite-standard sirens
- Efficient Search for Detection Candidates Using a Peak Finder Strategy for All-Sky-All-Frequency Gravitational Wave Radiometer