no code implementations • 2 Jul 2018 • Peter A. Gentile, Maura A. McLaughlin, Paul B. Demorest, Ingrid H. Stairs, Zaven Arzoumanian, Kathryn Crowter, Timothy Dolch, Megan E. DeCesar, Justin A. Ellis, Robert D. Ferdman, Elizabeth C. Ferrara, Emmanuel Fonseca, Marjorie E. Gonzalez, Glenn Jones, Megan L. Jones, Michael T. Lam, Lina Levin, Duncan R. Lorimer, Ryan S. Lynch, Cherry Ng, David J. Nice, Timothy T. Pennucci, Scott M. Ransom, Paul S. Ray, Ren'ee Spiewak, Kevin Stovall, Joseph K. Swiggum, Weiwei Zhu
We present the polarization pulse profiles for 28 pulsars observed with the Arecibo Observatory by the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) timing project at 2. 1 GHz, 1. 4 GHz, and 430 MHz.
High Energy Astrophysical Phenomena
1 code implementation • 18 Jan 2016 • Lina Levin, Maura A. McLaughlin, Glenn Jones, James M. Cordes, Daniel R. Stinebring, Shami Chatterjee, Timothy Dolch, Michael T. Lam, T. Joseph W. Lazio, Nipuni Palliyaguru, Zaven Arzoumanian, Kathryn Crowter, Paul B. Demorest, Justin A. Ellis, Robert D. Ferdman, Emmanuel Fonseca, Marjorie E. Gonzalez, Megan L. Jones, David J. Nice, Timothy T. Pennucci, Scott M. Ransom, Ingrid H. Stairs, Kevin Stovall, Joseph K. Swiggum, Weiwei Zhu
For most of the 10 pulsars for which the scaling has been measured, the bandwidths scale with frequency less steeply than expected for a Kolmogorov medium.
High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics