pith. sign in

Arecibo Observatory

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Papers (5)

  1. Model for a Noise Matched Phased Array Feed astro-ph.IM · 2019 · author #6
  2. Testing GR with the Double Pulsar: Recent Results astro-ph · 2005 · author #14
  3. Understanding the radio emission geometry of multi-component radio pulsars from retardation and aberration effects astro-ph · 2002 · author #2
  4. The characteristics of millisecond pulsar emission: II. Polarimetry astro-ph · 1998 · author #9
  5. The characteristics of millisecond pulsar emission: I. Spectra, pulse shapes and the beaming fraction astro-ph · 1998 · author #12

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