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Spinning neutron stars asymmetric with respect to their rotation axis are potential sources of continuous gravitational waves for ground-based interferometric detectors.
J. H. Taylor & J. M. Cordes, “ Pulsar distances and the galactic distribution of free electrons ”, ApJ, 411, 674, 1993
1993
Earlier work this paper cites.
J. P. Halpern et al, “ PSR J2229+6114: Discovery of an Energetic Young Pulsar in the Error Box of the EGRET Source 3EG J2227+6112 ”, ApJ, 552, L125 2001
2001
Earlier work this paper cites.
R. Dodson et al. ,“ The Vela Pulsar’s Proper Motion and Parallax Derived from VLBI Observations ”, ApJ 596 1137, 2003
2003
Earlier work this paper cites.
R. N. Manchester et al, “ The Australia Telescope National Facility Pulsar Catalogue ”, AJ, 129 1993, 2005
2005
Earlier work this paper cites.
P. Astone et al, “ The short FFT database and the peak map for the hierarchical search of periodic sources ”, Class. Quantum Grav. 22 S1197, 2005
2005
Earlier work this paper cites.
F. Camilo et al, “ PSR J1833–1034: Discovery of the central young pulsar in the supernova remnant G21.5-0.9 ”, ApJ 637 456, 2006
2006
Earlier work this paper cites.
The LIGO Scientific Collaboration and the Virgo Collaboration, “ Beating the spin-down limit on gravitational wave smission from the Crab pulsar ”, The Astrophysical Journal, 683: L45–L49, 2008
2008
Earlier work this paper cites.
D.L. Kaplan et al, “ A Precise Proper Motion for the Crab Pulsar, and the Difficulty of Testing Spin-Kick Alignment for Young Neutron Stars ”, ApJ, 677 1201, 2008
2008
Earlier work this paper cites.
M. Messineo et al, “ Discovery of a Young Massive Stellar Cluster near HESS J1813–178 ”, ApJ 683 L155 2008
2008
Earlier work this paper cites.
P. Astone et al., “ A method for the detection of known sources of continuous gravitational wave signals in non-stationary data ”, Classical Quantum Gravity 27, 194016, 2010
2010
Earlier work this paper cites.
M. Renaud et al, “ Discovery of a highly energetic pulsar associated with IGR J14003-6326 in a young uncatalogated galactic supernova remnant G310.6-1.6. ”, ApJ, 716 663–670, 2010
2010
Earlier work this paper cites.
P. Jaranowski & A. Królak, “ Searching for gravitational waves from known pulsars using the ℱ \mathcal{F} and 𝒢 \mathcal{G} statistics ”, CQG, 27, 194015 , 2010
2010
Earlier work this paper cites.
Z. Arzoumanian et al,“ Discovery of an energetic pulsar associated with SNR G76.9 + 1.0 ”, ApJ 739 39, 2011
2011
Cited alongside, same era.
Leahy D. A. et al ,“ Radio observations of CTB80: detection of the snowplough in an old supernova remnant ”, MNRAS, Volume 423, 2012
2012
Cited alongside, same era.
J. P. Halpern et al, “ Spin-down measure of PSR J1813-1749: The energetic pulsar powering HESS J1813-178 ”, ApJ, 753 L14, 2012
2012
Cited alongside, same era.
M. Pitkin et al, “ A new code for parameter estimation in searches for gravitational waves from known pulsars ”, J. Phys. Conf. Ser. 363, 012041, 2012
2012
Cited alongside, same era.
Kothes R.,“ Distance and age of the pulsar wind nebula 3C 58 ”, A & A 560, 2013
2013
Cited alongside, same era.
The LIGO Scientific Collaboration and the Virgo Collaboration, ” Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO and Advanced Virgo ”, Living Rev Relativ, 19: 1. https://doi.org/10.1007/lrr-2016-1, 2016
2016
Later among the works it cites.
The LIGO and Virgo Collaboration “ GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2 , Phys. Rev. Lett. 118, 221101 , 2017
2017
Closest in time.
2017
Closest in time.
The LIGO Scientific Collaboration and the Virgo Collaboration, “ First search for gravitational waves from known pulsars with advanced LIGO ”, B. P. Abbott et al, ApJ 839 12, 2017
2017
Closest in time.
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M. Marelli et al, “ On the puzzling high-energy pulsations of the energetic radio-quiet γ \gamma -ray pulsar J1813-1246 ”, ApJ, 795 168, 2014
2014
Cited alongside, same era.
P. Arumugasamy et al,“ XMM-NEWTON of young and energetic pulsar J2022+3842 ”, ApJ, 79 103, 2014
2014
Cited alongside, same era.
P. Astone et al., “ A method for narrow-band searches of continuous gravitational wave signals ”, Phys. Rev. D 89, 062008, 2014
2014
Cited alongside, same era.
The LIGO Scientific Collaboration, “ Advanced LIGO ”, Class. Quantum Grav. 32 074001, 2015
2015
Cited alongside, same era.
The LIGO Scientific Collaboration and the Virgo Collaboration,“ Observation of Gravitational Waves from a Binary Black Hole Merger ”, Phys. Rev. Lett. 116, 061102, 2016
2016
Cited alongside, same era.
The LIGO Scientific Collaboration and the Virgo Collaboration, “ GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence ”, Phys. Rev. Lett. 116, 241103, 2016
2016
Cited alongside, same era.
The LIGO Scientific Collaboration and the Virgo Collaboration, “ First search for nontensorial gravitational waves from known pulsars ”, LIGO-P1700009
Cited in the paper.
The LIGO Scientific Collaboration, “ Calibration of the Advanced LIGO detectors for the discovery of the binary black-hole merger GW150914 ”, Phys. Rev. D 95, 062003, 2017
2017
Closest in time.
The LIGO Scientific Collaboration and the Virgo Collaboration, “ Narrow-band search of continuous gravitational-wave signals from Crab and Vela pulsars in Virgo VSR4 data ”, Phys. Rev. D 91, 022004, 2017
2017
Closest in time.
J. M. Yao et al, “ A new electron-density model for estimation of pulsar and FRB distances ”, ApJ, 835, 29, 2017
2017
Closest in time.
S. Mastrogiovanni et al, “ An improved algorithm for narrow-band searches of gravitational waves ”, Class. Quantum Grav. 34 135007, 2017
2017
Closest in time.
2017
Closest in time.
S. M. Sarkissian et al, ” One Year of Monitoring the Vela Pulsar Using a Phased Array Feed ”, Publications of the Astronomical Society of Australia, 34. doi:10.1017/pasa.2017.19 , 2017
2017
Closest in time.