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- TRENDS 202227 Jul, 2022
- Advancing IDEA in Planetary Science 27 Jul, 2022
- The Arecibo Observatory: An Engine for Science and Scientists in Puerto Rico and Beyond27 Jul, 2022
- Cryogenic Frontend work for the 12m telescope entering phase II21 Jul, 2022
- A Parkes “Murriyang” Search for Pulsars and Fast Transients in the Large Magellanic Cloud 11 Jul, 2022
- A Comparison of Multiphase Magnetic Field Tracers in a High Galactic Latitude Region of the Filamentary Interstellar Medium 11 Jul, 2022
- The First Observation of Additional Ionospheric Layers Over Arecibo Using an Incoherent Scatter Radar11 Jul, 2022
- Decoding the star forming properties of gas-rich galaxy pairs11 Jul, 2022
- Crater Ejecta Across Maxwell Montes, Venus, and Possible Effects on Future Rock Type Measurements 11 Jul, 2022
- On Single-pulse Energies of Some Bright Pulsars Observed at 1.7 GHz11 Jul, 2022
- Probing the Local Interstellar Medium with Scintillometry of the Bright Pulsar B1133 + 16 11 Jul, 2022
- Arecibo Celebrates National Engineers Week 06 Apr, 2022
- The Arecibo Observatory at the Upcoming 240th American Astronomical Society Meeting06 Apr, 2022
- The Arecibo Observatory Survey Salvage Committee Report06 Apr, 2022
- Facilities and Operations Update06 Apr, 2022
Students from across North America participate in the NANOGrav Student Training Workshop prior to the science meeting.
|Astronomy||NANOGrav Meeting Hosted at UCF|
The University of Central Florida (UCF) hosted the semi-annual NANOGrav science meeting and student training workshop from March 2 - 6th. The meeting gave scientists the opportunity to assess their ongoing projects and discuss future work, including their next big release of 15 years worth of data. NANOGrav, or the North American Nanohertz Observatory for Gravitational Waves, is a collaboration of scientists from across the U.S. and Canada who search for gravitational waves by measuring their effects on the light-travel times of signals coming from pulsars.
Dr. Maura McLaughlin, Eberly distinguished professor of physics and astronomy at West Virginia University and co-Director of the NANOGrav Physics Frontiers Center, said that the “science meeting went very well,” adding that the project is “placing strong constraints on the upper limits for the gravitational wave background”.
The NANOGrav project uses the world’s most sensitive radio telescopes for its project: Arecibo Observatory (AO) in Puerto Rico and the Green Bank Telescope in West Virginia, both of which are facilities of the National Science Foundation. The project uses over 800 hours of telescope time per year at AO, which contributes to about half of the overall NANOGrav sensitivity to the gravitational waves, thanks to the massive size of the telescope.
The University of Central Florida currently leads the consortium that manages the Arecibo Observatory. Dr. McLaughlin expressed that “hosting the meeting at UCF gave students and faculty at the university an opportunity to learn more about the project, and it would be great to have even more involvement from UCF.”
The meeting included a two-day workshop for undergraduate students - an “onboarding” opportunity that prepares them for the high level scientific discussions during the meeting. Dr. Benetge Perera, a scientist at AO, explained that during the workshop “students had the opportunity to learn pulsar searches, timing, and gravitational wave detection techniques with expert assistance, and then do practical assignments with actual data”.
Highlights of the meeting also included a discussion on Diversity & Equity by Barbara Thompson, the Associate Director of UCF’s Office of Diversity & Inclusion, and a public talk by Dr. Sarah Vigeland, assistant professor at the University of Wisconsin Milwaukee, titled “Pulsar Timing Arrays: Opening a New Gravitational-Wave Window on the Universe”.
Article written by Dr. Tracy Becker - AO Collaborator / SwRI Research Scientist
Head of the Astronomy Dept.
Keywords: arecibo, observatory, Vigeland, McLaughlin, UCF, NANOGrav, workshop, Green, Bank, Wisconsin,