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A world map of GROWTH institutions including our new partners - the University of Washington, Seattle and University of Sydney, Australia.

GROWTH welcomes two new partners

The Department of Astronomy at the University of Washington (UW) and the University of Sydney, Australia officially joined the GROWTH collaboration last week. The new GROWTH partners bring wealth of expertise in large transient surveys and radio follow up observations, respectively.

Four members from the University of Washington will join the GROWTH team. Eric Bellm is currently a Research Assistant Professor and the Alert Production Science Lead for the Large Synoptic Survey Telescope (LSST). Eric is an expert in the development of large astronomical surveys who continues to be heavily involved in the recently launched Zwicky Transient Facility survey – GROWTH’s primary discovery engine. Dr. Melissa Graham and Dr. Zach Golkhou will each be involved in the follow up observations of supernovae at late times and follow up of transients potentially associated with gravitational wave events. Andy Connolly, is the director of the Data Intensive Research in Astrophysics and Cosmology (DIRAC) Institute at UW brings extensive knowledge in developing algorithms and software for large datasets. He will also share educational resources with the GROWTH community of educators and students.

The University of Washington is already a partner in the ZTF project and one of the founders of the LSST Corporation. Its partnership with GROWTH is a strategic step towards strengthening the link between the survey facilities and the community of observers who conduct coordinated follow up. The GROWTH community will also have access to observations taken with the 3.5m telescope at Apache Point Observatory, New Mexico for follow up observations as part of the observing time allocated to the UW researchers. Last but not least, the GROWTH SURF program is now open to the large pool of undergraduate students at UW.

With LSST on the horizon, now is the time to be perfecting tools and strategies for time-domain follow-up. Joining the GROWTH network will help UW connect sophisticated data analysis with rapid follow-up observations—and train the next generation of scientists along the way," - says Bellm.

Another set of students located almost diametrically opposite in the world on the campus of the University of Sydney will also have the opportunity to experience global research via our GROWTH SURF. The university is now GROWTH’s first partner located in the southern hemisphere after Tara Murphy, an associate professor in the Sydney Institute for Astronomy joined the GROWTH collaboration. Tara worked closely with the GROWTH team of radio astronomers during the radio follow up of the GW170817 event securing valuable data of the neutron star merger on the ATCA (Australia Telescope Compact Array) telescope. The GROWTH education community is particularly excited to welcome Tara who has extensive teaching experience having developed online courses and outreach activities. She is also the founder of Grok Learning – an online platform to teach coding to high school and university students.

"We are very excited to join GROWTH and share our interest and expertise in time variable astronomy, both from a research and teaching perspective. We look forward to working together, particularly when LIGO enters its next observing run in 2019" - says Tara Murphy.

"Multi-messenger astronomy is by nature an extremely collaborative endeavor bringing together a diverse set of astronomers and facilities around the globe. GROWTH is a true reflection of this new mode of conducting astronomical research and we are thrilled to see our team expand both in size and collective expertise" – says Mansi Kasliwal, GROWH Principal Investigator and an assistant professor of astronomy at Caltech.


Iva Kostadinova
GROWTH Communications and Media Contact
+1 626 395 2952

GROWTH is funded by the National Science Foundation under Grant No 1545949. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation.