Searching for gravitational waves from Cassiopeia A with LIGO
暂无分享,去创建一个
B. Krishnan | M. Landry | B. Machenschalk | D. McClelland | G. Mendell | C. Messenger | B. Owen | M. Papa | M. Pitkin | K. Riles | S. Scott | A. Sintes | J. Betzwieser | N. Christensen | T. Creighton | E. Goetz | R. Gustafson | D. Jones | K. Wette | J. Whelan | G. Woan | B. Allen | V. Dergachev | R. Prix | D. Hammer | H. Pletsch | M. Ashley | David Jones | I. Gholami | P. Patel | L. D. L. Jordana | M. Trias | L. S. de la Jordana | M. Landry
[1] Piotr Jaranowski,et al. Data analysis of gravitational-wave signals from spinning neutron stars. V. A narrow-band all-sky search , 2010, 1003.0844.
[2] et al,et al. Einstein@Home search for periodic gravitational waves in LIGO S4 data , 2008, 0804.1747.
[3] E. al.,et al. Erratum: All-sky search for periodic gravitational waves in LIGO S4 data [Phys. Rev. D 77, 022001 (2008)] , 2007, 0708.3818.
[4] C. Broeck,et al. BEATING THE SPIN-DOWN LIMIT ON GRAVITATIONAL WAVE EMISSION FROM THE VELA PULSAR , 2008, 0805.4758.
[5] M. M. Casey,et al. All-sky search for periodic gravitational waves in LIGO S4 data [Phys. Rev. D 77, 022001 (2008)][Publisher's note] , 2008 .
[6] D. Jones,et al. Are neutron stars with crystalline color-superconducting cores relevant for the LIGO experiment? , 2007, Physical review letters.
[7] L. Lin. Constraining crystalline color superconducting quark matter with gravitational-wave data , 2007, 0708.2965.
[8] Reinhard Prix,et al. Template-based searches for gravitational waves: efficient lattice covering of flat parameter spaces , 2007, 0707.0428.
[9] I. Wasserman,et al. Toroidal magnetic fields in type II superconducting neutron stars , 2007, 0705.2195.
[10] K. Glampedakis,et al. Modelling magnetically deformed neutron stars , 2007, 0705.1780.
[11] et al,et al. Upper limit map of a background of gravitational waves (Physical Review D - Particles, Fields, Gravitation and Cosmology (2007) 76, (082003)) , 2007, astro-ph/0703234.
[12] M. M. Casey,et al. Upper limits on gravitational wave emission from 78 radio pulsars (Physical Review D - Particles, Fields, Gravitation and Cosmology (2007) 76, (042001)) , 2007, gr-qc/0702039.
[13] D. M. Whitbeck. Observational Consequences of Gravitational Wave Emission From Spinning Compact Sources , 2006 .
[14] T. Hayler,et al. Searches for periodic gravitational waves from unknown isolated sources and Scorpius X-1: Results from the second LIGO science run , 2006 .
[15] B. Owen. Detectability of periodic gravitational waves by initial interferometers , 2006 .
[16] M. Dopita,et al. The Expansion Asymmetry and Age of the Cassiopeia A Supernova Remnant , 2006, astro-ph/0603371.
[17] G. Pavlov,et al. Near-Infrared and Optical Limits for the Central X-Ray Point Source in the Cassiopeia A Supernova Remnant , 2005, astro-ph/0509552.
[18] et al,et al. First all-sky upper limits from LIGO on the strength of periodic gravitational waves using the Hough transform , 2005, gr-qc/0508065.
[19] M. Bejger,et al. Constraints on the dense matter equation of state from the measurements of PSR J0737¿3039A moment of inertia and PSR J0751+1807 mass , 2005, astro-ph/0508105.
[20] B. Schutz,et al. Generalized F-statistic : Multiple detectors and multiple gravitational wave pulsars , 2005, gr-qc/0504011.
[21] R. Manchester,et al. The Australia Telescope National Facility Pulsar Catalogue , 2005 .
[22] B. Owen. Maximum elastic deformations of compact stars with exotic equations of state. , 2005, Physical review letters.
[23] M. M. Casey,et al. Limits on gravitational-wave emission from selected pulsars using LIGO data. , 2004, Physical review letters.
[24] M. M. Casey,et al. Setting upper limits on the strength of periodic gravitational waves from PSR J1939+2134 using the first science data from the GEO 600 and LIGO detectors , 2004 .
[25] G. Pavlov,et al. Central Compact Objects in Supernova Remnants , 2003, astro-ph/0311526.
[26] C. Cutler. Gravitational Waves from Neutron Stars with Large Toroidal B-fields , 2002, gr-qc/0206051.
[27] J. Heyl,et al. The Central X-Ray Point Source in Cassiopeia A , 2000, astro-ph/0001026.
[28] C. Palomba. Pulsars ellipticity revised , 1999, astro-ph/9912356.
[29] Bernard F. Schutz,et al. Gravitational waves from hot young rapidly rotating neutron stars , 1998, gr-qc/9804044.
[30] B. Schutz,et al. Data analysis of gravitational-wave signals from spinning neutron stars. I. The signal and its detection , 1998, gr-qc/9804014.
[31] T. Hales. Sphere packings, I , 1998, Discret. Comput. Geom..
[32] B. Owen,et al. Search templates for gravitational waves from inspiraling binaries: Choice of template spacing. , 1995, Physical review. D, Particles and fields.
[33] A. Fabian,et al. The Three-dimensional Structure of the Cassiopeia A Supernova Remnant. I. The Spherical Shell , 1995 .
[34] N. J. A. Sloane,et al. Sphere Packings, Lattices and Groups , 1987, Grundlehren der mathematischen Wissenschaften.
[35] V. Radhakrishnan. On the nature of pulsars , 1982 .
[36] M. Zimmermann,et al. Gravitational waves from rotating and precessing rigid bodies - Simple models and applications to pulsars , 1979 .
[37] J. Gunn,et al. On the nature of pulsars. I - Theory. , 1969 .
[38] S. Vila. Nature of Pulsars , 1969, Nature.
[39] D. Layzer. The Nature of Pulsars , 1968, Nature.