4.6 Article

The NANOGrav 12.5 yr Data Set: Bayesian Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries

相关参考文献

注意:仅列出部分参考文献,下载原文获取全部文献信息。
Article Astronomy & Astrophysics

Searching for continuous Gravitational Waves in the second data release of the International Pulsar Timing Array

M. Falxa et al.

Summary: The International Pulsar Timing Array 2nd data release is a combination of worldwide collaboration data sets. The study focuses on searching for continuous waves: gravitational wave signals generated by individual supermassive black hole binaries in the local universe. No evidence of such signals was found, and 95% upper limits on their amplitude, h(95), were set. The most sensitive frequency was found to be 10 nHz with h(95) = 9.1 x10(-15), achieving the best upper limit to date at low and high frequencies in the PTA band due to improved observation cadence.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2023)

Article Astronomy & Astrophysics

Noise analysis in the European Pulsar Timing Array data release 2 and its implications on the gravitational-wave background search

A. Chalumeau et al.

Summary: This study analyzes the noise of six pulsars using data from the European Pulsar Timing Array (EPTA) and confirms the existence of a previously reported red noise signal. The results emphasize the importance of noise modeling for the reliable detection of gravitational waves.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2022)

Article Astronomy & Astrophysics

Multimessenger time-domain signatures of supermassive black hole binaries

Maria Charisi et al.

Summary: Supermassive black hole binaries are formed through galaxy mergers and can be identified through electromagnetic and gravitational wave signals. We study the orbital dynamics of these binaries and find that periodic electromagnetic signals are the most promising for connecting with gravitational waves. Currently, multimessenger observations are limited to the most massive and nearby galaxies, but with more data collection, the observation range is expected to expand.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2022)

Article Astronomy & Astrophysics

The International Pulsar Timing Array second data release: Search for an isotropic gravitational wave background

J. Antoniadis et al.

Summary: In this study, we searched for an isotropic stochastic gravitational wave background using the second data release of the International Pulsar Timing Array. We found evidence for a spectrally similar low-frequency stochastic process and demonstrated that the combined international data set is more sensitive. Although no significant evidence of a gravitational-wave origin was found, future international data releases are expected to increase sensitivity and detection probability.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2022)

Article Astronomy & Astrophysics

Consistency of the Parkes Pulsar Timing Array Signal with a Nanohertz Gravitational-wave Background

Boris Goncharov et al.

Summary: Pulsar timing array experiments provide strong evidence for a common-spectrum stochastic process consistent with a nanohertz-frequency gravitational-wave background, but further research is needed to detect spatial correlations. A methodology to distinguish pulsar power spectra from noise power spectra is introduced and tested on simulated data sets, finding that the reported common process in pulsars is consistent with the spectral feature of a pulsar term. This methodology is recommended as a validity test for astrophysical and cosmological backgrounds.

ASTROPHYSICAL JOURNAL LETTERS (2022)

Article Astronomy & Astrophysics

Evaluating the prevalence of spurious correlations in pulsar timing array data sets

Andrew Zic et al.

Summary: Pulsar timing array collaborations have reported evidence for a common-noise process among millisecond pulsars in arrays, which is consistent with expectations for a gravitational-wave background. However, recent simulation analyses suggest that such a detection may be spurious. This paper uses simulated data sets to further test the inference methods for spectral and spatial correlations. The results highlight issues with current methods and suggest that the detection of a common process is not a reliable precursor to the detection of the gravitational-wave background. Future searches should focus on detecting spatial correlations and use more tailored specifications for a common-noise process.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2022)

Article Astronomy & Astrophysics

Quasars with Periodic Variability: Capabilities and Limitations of Bayesian Searches for Supermassive Black Hole Binaries in Time-domain Surveys

Caitlin A. Witt et al.

Summary: This paper utilizes Bayesian methods to distinguish periodic signals from supermassive black hole binaries and random variability in active galactic nuclei. Through careful parameter estimation and model selection analysis, it identifies conditions under which periodic signals are more easily detectable and how to avoid misclassifying DRW signals as binary candidates.

ASTROPHYSICAL JOURNAL (2022)

Article Astronomy & Astrophysics

Exploring Realistic Nanohertz Gravitational-wave Backgrounds

Bence Becsy et al.

Summary: Hundreds of millions of supermassive black hole binaries are expected to contribute to the gravitational-wave signal. A method is proposed to create realistic pulsar timing array data sets using synthetic catalogs of binaries. Several properties of these realistic backgrounds are explored to distinguish them from backgrounds formed in the early universe. The impact of confusion noise from a stochastic background on the detection of individual binaries is also investigated.

ASTROPHYSICAL JOURNAL (2022)

Article Astronomy & Astrophysics

Fast Bayesian analysis of individual binaries in pulsar timing array data

Bence Becsy et al.

Summary: Searching for gravitational waves in pulsar timing array data is a computationally intensive task. This study introduces a new formulation of the likelihood function that significantly speeds up the Bayesian analysis. By dividing the parameters into projection and shape parameters and precomputing the expensive inner products, the exploration of the projection parameters is accelerated by more than four orders of magnitude. The method also efficiently marginalizes nuisance parameters, making it important for handling large pulsar timing datasets and sophisticated analyses.

PHYSICAL REVIEW D (2022)

Article Astronomy & Astrophysics

Primordial gravitational waves from NANOGrav: A broken power-law approach

Micol Benetti et al.

Summary: This study revisits the possibility that the stochastic common-spectrum process detected by the NANOGrav pulsar timing array experiment could be due to primordial gravitational waves. By considering a broken power-law parametrization for the stochastic gravitational wave background (SGWB) spectrum, the authors find that this phenomenological model is able to explain the NANOGrav signal while remaining consistent with a variety of cosmological and gravitational wave observations. Further exploration of connections to specific well-motivated early-Universe models is warranted.

PHYSICAL REVIEW D (2022)

Article Astronomy & Astrophysics

Multi-messenger Approaches to Supermassive Black Hole Binary Detection and Parameter Estimation: Implications for Nanohertz Gravitational Wave Searches with Pulsar Timing Arrays

Tingting Liu et al.

Summary: This study investigates the effects of applying electromagnetic information to aid in the search for gravitational wave signals in pulsar timing array data. It finds that using electromagnetic priors can significantly improve the accuracy of binary detection and increase the likelihood of detecting signals in cases where none are found. Additionally, combining electromagnetic and gravitational wave data can lead to overall improvements in parameter estimation, regardless of the source's location or frequency.

ASTROPHYSICAL JOURNAL (2021)

Article Astronomy & Astrophysics

Common-red-signal analysis with 24-yr high-precision timing of the European Pulsar Timing Array: inferences in the stochastic gravitational-wave background search

S. Chen et al.

Summary: This study searched for a stochastic gravitational-wave background (GWB) using data from six radio millisecond pulsars, finding spectral properties consistent with theoretical predictions but lacking the required HD correlation for GWB detection. The most favored model was found to be common uncorrelated red noise, with the results being marginally influenced by Solar system ephemeris effects.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Article Physics, Multidisciplinary

Constraining Cosmological Phase Transitions with the Parkes Pulsar Timing Array

Xiao Xue et al.

Summary: Researchers search for a stochastic gravitational wave background using the Parkes Pulsar Timing Array data set, but find no evidence of the expected Hellings-Downs spatial correlation, leading to constraints on first-order phase transition model parameters. The analysis indicates that pulsar timing is particularly sensitive to low-temperature phase transitions, making it a useful tool for studying dark and QCD phase transitions.

PHYSICAL REVIEW LETTERS (2021)

Article Physics, Multidisciplinary

Searching for Gravitational Waves from Cosmological Phase Transitions with the NANOGrav 12.5-Year Dataset

Zaven Arzoumanian et al.

Summary: The study explores a potential first-order phase transition gravitational wave signal, possibly occurring at temperatures below the electroweak scale, in 45 pulsars from the NANOGrav dataset. However, there is no strong preference for this phase-transition interpretation over the standard astrophysical explanation of supermassive black hole mergers. Future datasets are expected to improve discriminating power, enhance signal-to-noise ratio, and extend sensitivity to lower frequencies, offering a chance to better distinguish such signals.

PHYSICAL REVIEW LETTERS (2021)

Article Astronomy & Astrophysics

Astrophysics Milestones for Pulsar Timing Array Gravitational-wave Detection

Nihan S. Pol et al.

Summary: The NANOGrav Collaboration has found strong Bayesian evidence for a common-spectrum stochastic process in their 12.5 yr pulsar timing array data set, with median characteristic strain amplitude at periods of a year. Even though evidence for the quadrupolar Hellings & Downs interpulsar correlations, which are characteristic of gravitational-wave signals, was not yet significant. By injecting a wide range of stochastic gravitational-wave background (GWB) signals into the data set, three key milestones were quantified, including the expectation of robust evidence for an interpulsar-correlated GWB signal after 15-17 yr of data accumulation.

ASTROPHYSICAL JOURNAL LETTERS (2021)

Article Astronomy & Astrophysics

Multimessenger Pulsar Timing Array Constraints on Supermassive Black Hole Binaries Traced by Periodic Light Curves

Chengcheng Xin et al.

Summary: Researchers compiled a catalog of 149 periodic light curves from supermassive black hole binary systems, predicting their gravitational-wave strain and detectability based on various parameters. The International Pulsar Timing Array (IPTA) is expected to significantly increase detection sensitivities for SMBHBs by 2025 with nearly uniform sky coverage.

ASTROPHYSICAL JOURNAL (2021)

Article Astronomy & Astrophysics

The NANOGrav 11 yr Data Set: Limits on Supermassive Black Hole Binaries in Galaxies within 500 Mpc

Zaven Arzoumanian et al.

Summary: This study used NANOGrav data to constrain SMBHBs in nearby massive galaxies, identifying 216 galaxies with possible binaries within NANOGrav's sensitive volume. The research ranked the detectability of potential SMBHBs and placed constraints on the chirp mass and mass ratio of 216 hypothetical binaries.

ASTROPHYSICAL JOURNAL (2021)

Article Astronomy & Astrophysics

On the Evidence for a Common-spectrum Process in the Search for the Nanohertz Gravitational-wave Background with the Parkes Pulsar Timing Array

Boris Goncharov et al.

Summary: A nanohertz-frequency stochastic gravitational-wave background can be potentially detected through the precise timing of millisecond pulsars, revealing a common-spectrum component. Recent data supports the presence of a common-spectrum process, but analysis may suffer from model misspecification. Extensions and combinations of datasets will improve the prospects of identifying spatial correlations necessary for claiming a detection of the gravitational-wave background.

ASTROPHYSICAL JOURNAL LETTERS (2021)

Article Astronomy & Astrophysics

Implications of the NANOGrav results for inflation

Sunny Vagnozzi

Summary: The NANOGrav pulsar timing array experiment provides evidence for a potential detection of a stochastic gravitational wave background, with implications for matching the upper limits set by BICEP2/Keck Array and Planck. Results suggest the existence of a parameter space related to big bang nucleosynthesis constraints.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Article Astronomy & Astrophysics

Massive black hole binary systems and the NANOGrav 12.5 yr results

H. Middleton et al.

Summary: NANOGrav has detected a common stochastic signal across a series of pulsars, potentially linked to a stochastic gravitational-wave background caused by unresolved massive black hole binaries. Using astronomical models and additional constraints, the merger rate and timescale of black hole binaries can be inferred, suggesting that a sufficiently large population of black holes will form and merge within a Hubble time.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Article Astronomy & Astrophysics

The NANOGrav 12.5 yr Data Set: Observations and Narrowband Timing of 47 Millisecond Pulsars

Md F. Alam et al.

Summary: This study presents TOA measurements and timing models of 47 millisecond pulsars observed between 2004 and 2017. The data was collected at the Arecibo Observatory and the Green Bank Telescope by NANOGrav. The research includes narrowband analysis for calculating multiple TOAs within narrow radio-frequency bands.

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES (2021)

Article Astronomy & Astrophysics

The NANOGrav 12.5 yr Data Set: Wideband Timing of 47 Millisecond Pulsars

Md F. Alam et al.

Summary: A new analysis of profile data from 47 millisecond pulsars using wideband timing methods shows remarkable agreement with results from NG12.5, with certain cases benefiting from 10%-15% more precise timing model parameters. This wideband timing data set serves as a stepping stone for gravitational wave analyses, reducing TOA volume and potentially speeding up complex pulsar timing array computations.

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES (2021)

Article Astronomy & Astrophysics

Joint search for isolated sources and an unresolved confusion background in pulsar timing array data

Bence Becsy et al.

CLASSICAL AND QUANTUM GRAVITY (2020)

Article Astronomy & Astrophysics

Spikey: self-lensing flares from eccentric SMBH binaries

Betty X. Hu et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2020)

Article Astronomy & Astrophysics

The NANOGrav 12.5 yr Data Set: Search for an Isotropic Stochastic Gravitational-wave Background

Zaven Arzoumanian et al.

ASTROPHYSICAL JOURNAL LETTERS (2020)

Article Astronomy & Astrophysics

The NANOGrav 11 yr Data Set: Limits on Gravitational Wave Memory

K. Aggarwal et al.

ASTROPHYSICAL JOURNAL (2020)

Article Astronomy & Astrophysics

The NANOGrav 11 yr Data Set: Evolution of Gravitational-wave Background Statistics

J. S. Hazboun et al.

ASTROPHYSICAL JOURNAL (2020)

Article Astronomy & Astrophysics

The Parkes Pulsar Timing Array project: second data release

Matthew Kerr et al.

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA (2020)

Review Astronomy & Astrophysics

The astrophysics of nanohertz gravitational waves

Sarah Burke-Spolaor et al.

ASTRONOMY AND ASTROPHYSICS REVIEW (2019)

Article Astronomy & Astrophysics

Constraining astrophysical observables of galaxy and supermassive black hole binary mergers using pulsar timing arrays

Siyuan Chen et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2019)

Article Astronomy & Astrophysics

The International Pulsar Timing Array: second data release

B. B. P. Perera et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2019)

Article Astronomy & Astrophysics

Microarcsecond VLBI Pulsar Astrometry with PSRπ II. Parallax Distances for 57 Pulsars

A. T. Deller et al.

ASTROPHYSICAL JOURNAL (2019)

Article Astronomy & Astrophysics

Supermassive Black Hole Binary Candidates from the Pan-STARRS1 Medium Deep Survey

T. Liu et al.

ASTROPHYSICAL JOURNAL (2019)

Article Astronomy & Astrophysics

Realistic sensitivity curves for pulsar timing arrays

Jeffrey S. Hazboun et al.

PHYSICAL REVIEW D (2019)

Article Astronomy & Astrophysics

Single sources in the low-frequency gravitational wave sky: properties and time to detection by pulsar timing arrays

Luke Zoltan Kelley et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2018)

Article Astronomy & Astrophysics

The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package

A. M. Price-Whelan et al.

ASTRONOMICAL JOURNAL (2018)

Article Astronomy & Astrophysics

Binary Pulsar Distances and Velocities from Gaia Data Release 2

Ross J. Jennings et al.

ASTROPHYSICAL JOURNAL (2018)

Article Astronomy & Astrophysics

The NANOGrav 11 Year Data Set: Pulsar-timing Constraints on the Stochastic Gravitational-wave Background

Z. Arzoumanian et al.

ASTROPHYSICAL JOURNAL (2018)

Article Astronomy & Astrophysics

A consistent measure of the merger histories of massive galaxies using close-pair statistics - I. Major mergers at z < 3.5

Carl J. Mundy et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2017)

Article Astronomy & Astrophysics

The local nanohertz gravitational-wave landscape from supermassive black hole binaries

Chiara M. F. Mingarelli et al.

NATURE ASTRONOMY (2017)

Article Astronomy & Astrophysics

THE NANOGRAV NINE-YEAR DATA SET: EXCESS NOISE IN MILLISECOND PULSAR ARRIVAL TIMES

M. T. Lam et al.

ASTROPHYSICAL JOURNAL (2017)

Article Astronomy & Astrophysics

The NANOGrav Nine-year Data Set: Measurement and Analysis of Variations in Dispersion Measures

M. L. Jones et al.

ASTROPHYSICAL JOURNAL (2017)

Article Astronomy & Astrophysics

A NEW ELECTRON-DENSITY MODEL FOR ESTIMATION OF PULSAR AND FRB DISTANCES

J. M. Yao et al.

ASTROPHYSICAL JOURNAL (2017)

Article Astronomy & Astrophysics

European Pulsar Timing Array limits on continuous gravitational waves from individual supermassive black hole binaries

S. Babak et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2016)

Article Astronomy & Astrophysics

The gamma-ray millisecond pulsar deathline, revisited New velocity and distance measurements

L. Guillemot et al.

ASTRONOMY & ASTROPHYSICS (2016)

Article Astronomy & Astrophysics

Constraints on individual supermassive black hole binaries from pulsar timing array limits on continuous gravitational waves

Katelin Schutz et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2016)

Article Astronomy & Astrophysics

The International Pulsar Timing Array: First data release

J. P. W. Verbiest et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2016)

Article Astronomy & Astrophysics

High-precision timing of 42 millisecond pulsars with the European Pulsar Timing Array

G. Desvignes et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2016)

Article Astronomy & Astrophysics

A population of short-period variable quasars from PTF as supermassive black hole binary candidates

M. Charisi et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2016)

Article Astronomy & Astrophysics

The gamma-ray millisecond pulsar deathline, revisited New velocity and distance measurements

L. Guillemot et al.

ASTRONOMY & ASTROPHYSICS (2016)

Article Astronomy & Astrophysics

THE NANOGRAV NINE-YEAR DATA SET: LIMITS ON THE ISOTROPIC STOCHASTIC GRAVITATIONAL WAVE BACKGROUND

Z. Arzoumanian et al.

ASTROPHYSICAL JOURNAL (2016)

Article Astronomy & Astrophysics

SYSTEMATIC AND STOCHASTIC VARIATIONS IN PULSAR DISPERSION MEASURES

M. T. Lam et al.

ASTROPHYSICAL JOURNAL (2016)

Article Astronomy & Astrophysics

Expected properties of the first gravitational wave signal detected with pulsar timing arrays

Pablo A. Rosado et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2015)

Article Astronomy & Astrophysics

European Pulsar Timing Array limits on an isotropic stochastic gravitational-wave background

L. Lentati et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2015)

Article Astronomy & Astrophysics

A systematic search for close supermassive black hole binaries in the Catalina Real-time Transient Survey

Matthew J. Graham et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2015)

Article Multidisciplinary Sciences

Gravitational waves from binary supermassive black holes missing in pulsar observations

R. M. Shannon et al.

SCIENCE (2015)

Article Astronomy & Astrophysics

GRAVITATIONAL WAVE HOTSPOTS: RANKING POTENTIAL LOCATIONS OF SINGLE-SOURCE GRAVITATIONAL WAVE EMISSION

Joseph Simon et al.

ASTROPHYSICAL JOURNAL (2014)

Article Computer Science, Interdisciplinary Applications

XSEDE: Accelerating Scientific Discovery

John Towns et al.

COMPUTING IN SCIENCE & ENGINEERING (2014)

Article Astronomy & Astrophysics

Targeting supermassive black hole binaries and gravitational wave sources for the pulsar timing array

Pablo A. Rosado et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2014)

Article Astronomy & Astrophysics

An all-sky search for continuous gravitational waves in the Parkes Pulsar Timing Array data set

X-J Zhu et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2014)

Article Astronomy & Astrophysics

Bayesian inference for pulsar-timing models

Sarah J. Vigeland et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2014)

Article Astronomy & Astrophysics

Astropy: A community Python package for astronomy

Thomas P. Robitaille et al.

ASTRONOMY & ASTROPHYSICS (2013)

Article Astronomy & Astrophysics

THE SECOND FERMI LARGE AREA TELESCOPE CATALOG OF GAMMA-RAY PULSARS

A. A. Abdo et al.

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES (2013)

Article Astronomy & Astrophysics

The Parkes Pulsar Timing Array

G. Hobbs

CLASSICAL AND QUANTUM GRAVITY (2013)

Article Astronomy & Astrophysics

The North American Nanohertz Observatory for Gravitational Waves

M. A. McLaughlin

CLASSICAL AND QUANTUM GRAVITY (2013)

Article Multidisciplinary Sciences

Gravitational-Wave Limits from Pulsar Timing Constrain Supermassive Black Hole Evolution

R. M. Shannon et al.

SCIENCE (2013)

Article Astronomy & Astrophysics

Systematic investigation of the expected gravitational wave signal from supermassive black hole binaries in the pulsar timing band

A. Sesana

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2013)

Article Astronomy & Astrophysics

ON PULSAR DISTANCE MEASUREMENTS AND THEIR UNCERTAINTIES

J. P. W. Verbiest et al.

ASTROPHYSICAL JOURNAL (2012)

Article Astronomy & Astrophysics

The relativistic pulsar-white dwarf binary PSR J1738+0333-II. The most stringent test of scalar-tensor gravity

Paulo C. C. Freire et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2012)

Article Astronomy & Astrophysics

Placing limits on the stochastic gravitational-wave background using European Pulsar Timing Array data

R. van Haasteren et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2011)

Article Astronomy & Astrophysics

ASSESSING THE ROLE OF SPIN NOISE IN THE PRECISION TIMING OF MILLISECOND PULSARS

Ryan M. Shannon et al.

ASTROPHYSICAL JOURNAL (2010)

Article Astronomy & Astrophysics

A VERY CLOSE BINARY BLACK HOLE IN A GIANT ELLIPTICAL GALAXY 3C 66B AND ITS BLACK HOLE MERGER

Satoru Iguchi et al.

ASTROPHYSICAL JOURNAL LETTERS (2010)

Article Astronomy & Astrophysics

The sensitivity of the Parkes Pulsar Timing Array to individual sources of gravitational waves

D. R. B. Yardley et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2010)

Article Astronomy & Astrophysics

PRECISION ASTROMETRY WITH THE VERY LONG BASELINE ARRAY: PARALLAXES AND PROPER MOTIONS FOR 14 PULSARS

S. Chatterjee et al.

ASTROPHYSICAL JOURNAL (2009)

Article Astronomy & Astrophysics

Timing stability of millisecond pulsars and prospects for gravitational-wave detection

J. P. W. Verbiest et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2009)

Article Astronomy & Astrophysics

Generic tests of the existence of the gravitational dipole radiation and the variation of the gravitational constant

K. Lazaridis et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2009)

Article Astronomy & Astrophysics

The stochastic gravitational-wave background from massive black hole binary systems: implications for observations with Pulsar Timing Arrays

A. Sesana et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2008)

Article Astronomy & Astrophysics

High-precision baseband timing of 15 millisecond pulsars

A. W. Hotan et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2006)

Article Astronomy & Astrophysics

TEMPO2, a new pulsar-timing package - I. An overview

GB Hobbs et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2006)

Article Astronomy & Astrophysics

The parallax and proper motion of PSR J0030+0451

AN Lommen et al.

ASTROPHYSICAL JOURNAL (2006)

Article Astronomy & Astrophysics

The mass of a millisecond pulsar

BA Jacoby et al.

ASTROPHYSICAL JOURNAL (2005)

Article Astronomy & Astrophysics

Masses, parallax, and relativistic timing of the PSR J1713+0747 binary system

EM Splaver et al.

ASTROPHYSICAL JOURNAL (2005)

Article Astronomy & Astrophysics

The parallax, mass and age of the PSR J2145-0750 binary system

O Löhmer et al.

ASTRONOMY & ASTROPHYSICS (2004)