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Our goal is to detect low-frequency gravitational waves and use our measurements to characterize the low-frequency gravitational wave universe. Our pulsar timing observations also allow a wealth of other astrophysical experiments and applications.
Pulsars Observed
79
Times of Arrival Observed
543k
Papers Published
270
Citations
14.8k
Clockwise from top-left: one of the VLA telescopes; the CHIME telescope; collaboration members at a Busy Week; the Green Bank Telescope at sunset; and a collaboration meeting at Arecibo Observatory. Images: VLA adapted from Jeremy Zilar, CHIME from Andre Renard/CHIME Collaboration, Green Bank Telescope from Jee Seymour