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University of Hawai‘i Astronomers to Help Map the First Galaxies of the Universe

April 24, 2021, 6:12 PM HST
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JWST will map and model the core of galaxies nearby. Credit: NASA

Astronomers from the University of Hawaiʻi Institute for Astronomy (IfA) will play a key role in helping unveil the universe’s very first galaxies, more than 13 billion light years away.

This week, NASA announced the first suite of science programs for its groundbreaking James Webb Space Telescope, set to launch in October 2021. The IfA researchers are part of the “COSMOS-Webb” project, which will be the largest guest observer program in JWST’s first year of operation.

The IfA astronomers will conduct detailed follow-up observations of galaxies seen in the JWST images, using the telescopes on Maunakea. The JWST is the largest and most powerful space telescope ever built and will succeed NASA’s Hubble Space Telescope. It is equipped to observe some of the most distant objects in the universe, using upgraded infrared sensitivity and resolution.

”Ground-based observations from Maunakea will be critical for turning the JWST images into a three-dimensional map of the universe,” said David Sanders, lead IfA investigator. 

Sanders and his IfA team are part of the newly selected COSMOS-Webb program, comprised of nearly 50 researchers from 30 institutions worldwide, including IfA, the Rochester Institute of Technology (RIT), and University of Texas at Austin (UT Austin). The COSMOS-Webb program will help NASA map the first galaxies formed at “Cosmic Dawn”, when the universe was less than 1/20th of its current age.

JWST will explore the cores of merging galaxies. Credit: NASA
James Webb Space Telescope (JWST) Credit: NASA
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Surveying on Maunakea

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Researchers will conduct spectroscopic follow-up of interesting galaxies at the W.M. Keck Observatory and a brand new instrument at Subaru Telescope, called the Prime Focus Spectrograph. According to UH, Subaru’s new instrument will be crucial for determining distances to all galaxies in the JWST survey.

The program will log more than 200 hours of observation time on Maunakea to conduct an ambitious survey of half a million galaxies. An unprecedented 32,000 galaxies will be observed using mid-infrared imaging. Researchers will rapidly release data to the public so it can lead to other studies.

“The sheer scope of our program is so exciting,” said IfA alumna Jeyhan Kartaltepe, a professor at RIT’s School of Physics and Astronomy. “The first year of Webb observations will result in a lot of new discoveries that people will want to explore more in-depth in future cycles.”

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Essential earlier research

Much of the earlier research in this specific part of the sky has been centered at the IfA, including the S-COSMOS survey, a deep infrared imaging survey using NASA’s Spitzer Space Telescope. Led by Sanders, the project was an essential precursor to this JWST program. 

“COSMOS-Webb has the potential to be ground-breaking in ways we haven’t even dreamt yet,” said former IfA Hubble Fellow Caitlin Casey, now an assistant professor and Cosmos-Webb principal investigator at UT Austin. “You don’t know what treasures are there to find until you use an incredible telescope like Webb to stare at the sky for a long time.”

COSMOS-Webb is one of just 286 general scientific observer programs  NASA selected out of more than 1,000 proposals for the telescope’s first year of science. These specific programs will provide the worldwide astronomical community with one of the first extensive opportunities to investigate scientific targets. JWST is slated to be operational in 2022. 

More information is available at the Space Telescope Science Institute website.

Aerial view of telescopes on Maunakea. Keck and Subaru will be used to conduct research.
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