Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2015, Volume 453, Issue 3, pp. 2576 - 2598

We present new limits on an isotropic stochastic gravitational-wave background (GWB) using a six pulsar data set spanning 18 yr of observations from the 2015...

Pulsars: general | Gravitational waves | Methods: data analysis | methods: data analysis | pulsars: general | HIERARCHICAL-MODELS | DISPERSION | RADIATION | PRECISION | TEMPO2 | BLACK-HOLE BINARIES | EVOLUTION | PACKAGE | ASTRONOMY & ASTROPHYSICS | SYSTEMS | gravitational waves | EFFICIENT | Solar and Stellar Astrophysics | Sciences of the Universe | Astrophysics

Pulsars: general | Gravitational waves | Methods: data analysis | methods: data analysis | pulsars: general | HIERARCHICAL-MODELS | DISPERSION | RADIATION | PRECISION | TEMPO2 | BLACK-HOLE BINARIES | EVOLUTION | PACKAGE | ASTRONOMY & ASTROPHYSICS | SYSTEMS | gravitational waves | EFFICIENT | Solar and Stellar Astrophysics | Sciences of the Universe | Astrophysics

Journal Article

Astrophysical Journal, ISSN 0004-637X, 04/2016, Volume 821, Issue 1, pp. 13 - 13

We compute upper limits on the nanohertz-frequency isotropic stochastic gravitational wave background (GWB) using the 9 year data set from the North American...

pulsars: general | gravitational waves | methods: data analysis | methods data analysis | RADIATION | MERGER | GALAXY | EVOLUTION | pulsars general | PULSAR TIMING ARRAY | ASTRONOMY & ASTROPHYSICS | BINARIES | ACCRETION | MASSIVE BLACK-HOLE | GALACTIC NUCLEI | COSMIC STRINGS | Amplitudes | Gravitational waves | Binary stars | Mathematical models | Nanostructure | Strings | Bayesian analysis | Power law

pulsars: general | gravitational waves | methods: data analysis | methods data analysis | RADIATION | MERGER | GALAXY | EVOLUTION | pulsars general | PULSAR TIMING ARRAY | ASTRONOMY & ASTROPHYSICS | BINARIES | ACCRETION | MASSIVE BLACK-HOLE | GALACTIC NUCLEI | COSMIC STRINGS | Amplitudes | Gravitational waves | Binary stars | Mathematical models | Nanostructure | Strings | Bayesian analysis | Power law

Journal Article

Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2016, Volume 458, Issue 2, pp. 1267 - 1288

The highly stable spin of neutron stars can be exploited for a variety of (astro-)physical investigations. In particular arrays of pulsars with rotational...

Methods: Data analysis | Pulsars: General | Physics - Instrumentation and Methods for Astrophysics | Solar and Stellar Astrophysics | Sciences of the Universe | Astrophysics

Methods: Data analysis | Pulsars: General | Physics - Instrumentation and Methods for Astrophysics | Solar and Stellar Astrophysics | Sciences of the Universe | Astrophysics

Journal Article

Physical Review Letters, ISSN 0031-9007, 2015, Volume 115, Issue 4, p. 041101

The paucity of observed supermassive black hole binaries (SMBHBs) may imply that the gravitational wave background (GWB) from this population is anisotropic,...

TEMPO2 | PULSAR TIMING ARRAYS | BLACK-HOLE BINARIES | PHYSICS, MULTIDISCIPLINARY | PACKAGE | COALESCENCE RATE | SYSTEMS | COSMIC STRINGS | RADIATION | COVARIANCE MATRICES | Isotropy | Anisotropy | Rendering | Gravitational waves | Angular distribution | Nanostructure | Stochasticity | Arrays | General Relativity and Quantum Cosmology | Sciences of the Universe | Astrophysics | Physics

TEMPO2 | PULSAR TIMING ARRAYS | BLACK-HOLE BINARIES | PHYSICS, MULTIDISCIPLINARY | PACKAGE | COALESCENCE RATE | SYSTEMS | COSMIC STRINGS | RADIATION | COVARIANCE MATRICES | Isotropy | Anisotropy | Rendering | Gravitational waves | Angular distribution | Nanostructure | Stochasticity | Arrays | General Relativity and Quantum Cosmology | Sciences of the Universe | Astrophysics | Physics

Journal Article

Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2018

We have studied 4265 giant pulses (GPs) from the millisecond pulsar B1937+21; the largest-ever sample gathered for this pulsar, in observations made with the...

Physics - High Energy Astrophysical Phenomena

Physics - High Energy Astrophysical Phenomena

Journal Article

Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 07/2018, Volume 478, Issue 1, pp. 218 - 227

We search for continuous gravitational waves (CGWs) produced by individual supermassive black hole binaries in circular orbits using high-cadence timing...

Quasars: Supermassive black holes | Binaries: General | Stars: Neutron | Gravitational waves | Pulsars: Individual: PSR J1713+0747 | Stars: Black holes | ARRAY | stars: black holes | pulsars: individual: PSR J1713+0747 | RADIATION | stars: neutron | SPACED DATA | MILLISECOND PULSARS | SYSTEMATIC SEARCH | ASTRONOMY | ASTRONOMY & ASTROPHYSICS | B1937+21 | gravitational waves | binaries: general | quasars: supermassive black holes | DATA RELEASE | PROBE | EFFICIENT

Quasars: Supermassive black holes | Binaries: General | Stars: Neutron | Gravitational waves | Pulsars: Individual: PSR J1713+0747 | Stars: Black holes | ARRAY | stars: black holes | pulsars: individual: PSR J1713+0747 | RADIATION | stars: neutron | SPACED DATA | MILLISECOND PULSARS | SYSTEMATIC SEARCH | ASTRONOMY | ASTRONOMY & ASTROPHYSICS | B1937+21 | gravitational waves | binaries: general | quasars: supermassive black holes | DATA RELEASE | PROBE | EFFICIENT

Journal Article

Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2016, Volume 458, Issue 2, pp. 2161 - 2187

We analyse the stochastic properties of the 49 pulsars that comprise the first International Pulsar Timing Array (IPTA) data release. We use Bayesian...

Methods: Data analysis | Pulsars: General | LIMITS | methods: data analysis | pulsars: general | DISPERSION | FREQUENCY GRAVITATIONAL-RADIATION | PRECISION | VARIABILITY | WAVES | BLACK-HOLE BINARIES | SHAPELETS | MILLISECOND PULSAR | ASTRONOMY & ASTROPHYSICS | SCATTERING | Sciences of the Universe

Methods: Data analysis | Pulsars: General | LIMITS | methods: data analysis | pulsars: general | DISPERSION | FREQUENCY GRAVITATIONAL-RADIATION | PRECISION | VARIABILITY | WAVES | BLACK-HOLE BINARIES | SHAPELETS | MILLISECOND PULSAR | ASTRONOMY & ASTROPHYSICS | SCATTERING | Sciences of the Universe

Journal Article

Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 12/2018, Volume 481, Issue 4, pp. 5501 - 5516

Pulsar-timing analyses are sensitive to errors in the Solar-system ephemerides (SSEs) that timing models utilize to estimate the location of the Solar-system...

Pulsars: general | Ephemerides | Methods: data analysis | Methods: statistical | methods: data analysis | ephemerides | ROTATION PERIOD | SPIN NOISE | pulsars: general | DISPERSION | GRAVITY-FIELD | MODEL | MILLISECOND PULSARS | PRECISION | EPHEMERIS | methods: statistical | ASTRONOMY & ASTROPHYSICS | MASS | DARK-MATTER | Physics - Earth and Planetary Astrophysics

Pulsars: general | Ephemerides | Methods: data analysis | Methods: statistical | methods: data analysis | ephemerides | ROTATION PERIOD | SPIN NOISE | pulsars: general | DISPERSION | GRAVITY-FIELD | MODEL | MILLISECOND PULSARS | PRECISION | EPHEMERIS | methods: statistical | ASTRONOMY & ASTROPHYSICS | MASS | DARK-MATTER | Physics - Earth and Planetary Astrophysics

Journal Article

Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 12/2019, Volume 490, Issue 4, pp. 4666 - 4687

ABSTRACT In this paper, we describe the International Pulsar Timing Array second data release, which includes recent pulsar timing data obtained by three...

Physics - High Energy Astrophysical Phenomena

Physics - High Energy Astrophysical Phenomena

Journal Article

International Journal of Modern Physics C, ISSN 0129-1831, 11/2007, Volume 18, Issue 11, pp. 1735 - 1746

In this paper, three methods for computing non-rotating neutron star models are discussed. The relativistic Oppenheimer–Volkoff (OV) equations of hydrostatic...

Stars: neutron | Equations of state | Methods: numerical | MASSES | GROUND-STATE | methods | PHASE-TRANSITIONS | stars | COMPACT STARS | PHYSICS, MATHEMATICAL | equations of state | 3RD FAMILY | numerical | COMPUTER SCIENCE, INTERDISCIPLINARY APPLICATIONS | MODELS | neutron | NEUTRON-STAR STRUCTURE | DENSE MATTER

Stars: neutron | Equations of state | Methods: numerical | MASSES | GROUND-STATE | methods | PHASE-TRANSITIONS | stars | COMPACT STARS | PHYSICS, MATHEMATICAL | equations of state | 3RD FAMILY | numerical | COMPUTER SCIENCE, INTERDISCIPLINARY APPLICATIONS | MODELS | neutron | NEUTRON-STAR STRUCTURE | DENSE MATTER

Journal Article

04/2018

We search for continuous gravitational waves (CGWs) produced by individual super-massive black-hole binaries (SMBHBs) in circular orbits using high-cadence...

Physics - High Energy Astrophysical Phenomena

Physics - High Energy Astrophysical Phenomena

Journal Article

Annals of Nutrition and Metabolism, ISSN 0250-6807, 10/2009, Volume 54, Issue 4, pp. 325 - 326

Journal Article

European Journal of Cancer, ISSN 0959-8049, 2001, Volume 37, pp. S318 - S318

Journal Article

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