Showing 1–20 of 122 results
/ Date/ Name
Jun 28, 2023The NANOGrav 15-Year Data Set: Detector Characterization and Noise BudgetJun 28, 2023The NANOGrav 15-year Data Set: Constraints on Supermassive Black Hole Binaries from the Gravitational Wave BackgroundJul 18, 2022A Scintillation Arc Survey of 22 Pulsars with Low to Moderate Dispersion MeasuresJan 10, 2011A 350-MHz GBT Survey of 50 Faint Fermi Gamma-ray Sources for Radio Millisecond PulsarsAug 29, 2011A Chandra X-ray Observation of the Binary Millisecond Pulsar PSR J1023+0038Jul 2, 2018The NANOGrav 11-Year Data Set: Arecibo Observatory Polarimetry And Pulse MicrocomponentsSep 17, 2020Evaluating Low-Frequency Pulsar Observations to Monitor Dispersion with the Giant Metrewave Radio TelescopeOct 22, 2020Astrophysics Milestones For Pulsar Timing Array Gravitational Wave DetectionSep 9, 2020The NANOGrav 12.5-year Data Set: Search For An Isotropic Stochastic Gravitational-Wave BackgroundMay 13, 2020The NANOGrav 12.5-year Data Set: Wideband Timing of 47 Millisecond PulsarsNov 17, 2021Bayesian Solar Wind Modeling with Pulsar Timing ArraysMar 2, 2016The NANOGrav Nine-year Data Set: Mass and Geometric Measurements of Binary Millisecond PulsarsMay 10, 2008No detectable radio emission from the magnetar-like pulsar in Kes 75Jul 16, 2008Relativistic Spin Precession in the Double PulsarMar 31, 2020The GBT 350-MHz Drift Scan Pulsar Survey. III. Detection of a magnetic field in the eclipsing material of PSR J2256-1024Feb 21, 2025Multifrequency Radio Observations of the Magnetar Swift J1818.0--1607Oct 18, 2023The NANOGrav 15-year data set: Search for Transverse Polarization Modes in the Gravitational-Wave BackgroundJul 30, 2024The NANOGrav 15 yr data set: Posterior predictive checks for gravitational-wave detection with pulsar timing arraysJun 19, 2024Exploring pulsar timing precision: A comparative study of polarization calibration methods for NANOGrav data from the Green Bank TelescopeJun 4, 2025The NANOGrav 15-Year Data Set: A Case Study for Simplified Dispersion Measure Modeling for PSR J1455-3330 and the Impact on Gravitational Wave Sensitivity