Showing 1–20 of 31 results
/ Date/ Name
Dec 30, 2025Understanding Solar Flares and Energetic Events: Open questions, observational requirements, and instrumental needs over the coming decadeNov 22, 2024The NANOGrav 15 Yr Data Set: Removing Pulsars One by One from the Pulsar Timing ArrayNov 20, 2024The NANOGrav 15 yr Data Set: Harmonic Analysis of the Pulsar Angular CorrelationsJul 9, 2024The Anomalous Acceleration of PSR J2043+1711: Long-Period Orbital Companion or Stellar Flyby?Oct 18, 2023The NANOGrav 15-year data set: Search for Transverse Polarization Modes in the Gravitational-Wave BackgroundSep 1, 2023Comparing recent PTA results on the nanohertz stochastic gravitational wave backgroundJul 25, 2023The NANOGrav 12.5-year Data Set: Search for Gravitational Wave MemoryJun 28, 2023The NANOGrav 15-year Gravitational-Wave Background MethodsJun 28, 2023The NANOGrav 15-year Data Set: Constraints on Supermassive Black Hole Binaries from the Gravitational Wave BackgroundJun 28, 2023The NANOGrav 15-Year Data Set: Detector Characterization and Noise BudgetJun 28, 2023The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave BackgroundJan 11, 2022The International Pulsar Timing Array second data release: Search for an isotropic Gravitational Wave BackgroundNov 17, 2021Bayesian Solar Wind Modeling with Pulsar Timing ArraysOct 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 14, 2020Multi-Messenger Gravitational Wave Searches with Pulsar Timing Arrays: Application to 3C66B Using the NANOGrav 11-year Data SetMay 13, 2020The NANOGrav 12.5-year Data Set: Wideband Timing of 47 Millisecond PulsarsNov 19, 2019The NANOGrav 11-Year Data Set: Limits on Gravitational Wave MemoryJul 17, 2019NANOGrav Education and Outreach: Growing a Diverse and Inclusive Collaboration for Low-Frequency Gravitational Wave AstronomyDec 30, 2018The NANOGrav 11-Year Data Set: Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries