61 citations
- Eötvös Loránd UniversityHU5 papers
- University of BirminghamGB5 papers
- University of TorontoCA5 papers
- California Institute of TechnologyUS4 papers
- Curtin UniversityAU4 papers
- Eureka ScientificUS4 papers
- George Mason UniversityUS4 papers
- Goddard Space Flight CenterUS4 papers
- Hillsdale CollegeUS4 papers
- Lafayette CollegeUS4 papers
- National Radio Astronomy ObservatoryUS4 papers
- Newcastle UniversityGB4 papers
4 papers · 1 filter
The NANOGrav 15 yr Data Set: Customized Chromatic Noise Models
Bjorn Larsen, Jeremy G. Baier, Daniel J. Oliver +53
Pulsar timing arrays conduct low-frequency gravitational wave searches, which require comprehensive accounting of various noise sources to achieve robust results. Interstellar prop…
Gravitational Wave Measurement of the - Intrinsic Scatter at High Redshift
Cayenne Matt, Kayhan Gültekin, Gabriella Agazie +109
The observed GWB spectrum is higher in amplitude than model predictions by a factor of 2-3. Using a semi-analytic model, we evaluate the effect of a high-scatter supermassive black…
Searching for Exotrojans in Pulsar Systems
Jackson D. Taylor, Emmanuel Fonseca, Lankeswar Dey +50
Trojan asteroids are found in the equilateral triangle Lagrange points of the Sun-Jupiter system in great number, though they also exist less prolifically in other parts of the Sol…
Inference on inner galaxy structure via gravitational waves from supermassive binaries
Yifan Chen, Matthias Daniel, Daniel J. D'Orazio +107
The detection of a stochastic gravitational wave background by pulsar-timing arrays indicates the presence of a population of supermassive black hole binaries. Although the observe…