Astronomers Go Infrared to Map Brightest Galaxies in Universe

Astronomers Go Infrared to Map Brightest Galaxies in Universe

Credit: ESA-C. Carreau

A 3D projection of almost 300 galaxies in the census in the same part of the sky. The third dimension shows how many billions of years back in time we are seeing each galaxy, determined by observations from the Keck Observatory. At top are images from the Hubble Space Telescope of five galaxies in the census.

Astronomers Go Infrared to Map Brightest Galaxies in Universe

Images of six of the dusty galaxies as seen by Hubble Space Telescope with distances (in billions of light years) measured by the W. M. Keck Observatory. The background is an image of the sky in far-infrared from Herschel, where dusty galaxies like this are most easily detected. The Keck data (shown in blue below galaxy images), which spreads the light of each galaxy into a spectrum, allowed the astronomers to measure distances to each galaxy using “fingerprints” of atoms and molecules in each galaxy. These galaxies were previously unidentified due to the large amounts of dust absorbing the visible light.

Kamuela, Hawaii – A group of astronomers from the University of Hawaii at Manoa, the U.S. Mainland, Canada, and Europe recently used the twin telescopes of the W. M. Keck Observatory on Mauna Kea, Hawaii, to conduct a census of the brightest, but until now unseen, galaxies in the distant Universe, bringing astronomers one step closer to understanding how galaxies form and evolve.

These galaxies glow so brightly at infrared wavelengths that they would outshine our own Milky Way by hundreds, maybe thousands, of times. They are forming stars so quickly that between 100 and 500 new stars are born in each galaxy every year, and have been coined “starbursts” by astronomers.

While it’s not clear what gives these galaxies their intense luminosity, it could be the result of a collision between two spiral-type galaxies, similar to the Milky Way and Andromeda Galaxies. Or they could be in a particularly gas-rich region of space, where galaxies form stars quickly due to constant bombardment from gas and dust.

Despite their brightness, these galaxies are nearly invisible at the wavelengths our eyes and most telescopes on Earth can see because they contain huge amounts of dust, which absorbs visible starlight.  But they were detectable directly in the infrared from observations at the Herschel Space Observatory, said Dr. Caitlin Casey, a Hubble fellow at the UH Manoa Institute for Astronomy and the lead scientist behind the new results. “Herschel is an infrared space telescope sensitive to wavelengths not observable from within Earth’s atmosphere,” she said.

“Detecting these bright infrared galaxies used to be difficult, and a handful was plenty; now with Herschel we are finding them by the thousands, enabling a census like this,” said Göran Pilbratt, European Space Agency Herschel Project Scientist.

Once found, taking measurements of these galaxies at visible wavelengths required using the 10-meter Keck telescopes, the two largest optical telescopes in the world. Over the course of several nights the group was able to detect and measure distances to nearly 800 of these galaxies.

“For the first time, we have been able to measure distances, star formation rates, and temperatures for a brand new set of 767 previously unidentified galaxies,” said Dr. Scott Chapman, a co-author on the studies. “The previous similar survey of distant infrared starbursts only covered 73 galaxies. This is a huge improvement.”

“While some of the galaxies are nearby, most are very distant; we even found galaxies that are so far that their light has taken 12 billion years to travel here, so we are seeing them when the Universe was only a ninth of its current age,” Casey said. “Now that we have a pretty good idea of how important this type of galaxy is in forming huge numbers of stars in the Universe, the next step is to figure out why and how they formed.”

“It’s hard to figure out how most galaxies formed based on information from only a small part of the Universe, just like it’s hard to guess how big an elephant is if you only get a glimpse of its tail,” Casey said. “Now that we have an accurate census of starbursting galaxies across a huge time period in the Universe’s history, we can start to piece together how these galaxies grew and evolved.”

Two papers detailing these results are published online today in the Astrophysical Journal.

Founded in 1967, the Institute for Astronomy at the University of Hawaii at Manoa conducts research into galaxies, cosmology, stars, planets, and the sun. Its faculty and staff are also involved in astronomy education, deep space missions, and in the development and management of the observatories on Haleakala and Mauna Kea. The Institute operates facilities on the islands of Oahu, Maui, and Hawaii.

Herschel is a European Space Agency space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.

The W. M. Keck Observatory operates two, 10-meter optical/infrared telescopes on the summit of Mauna Kea on the Island of Hawaii. The twin telescopes feature a suite of advanced instruments including imagers, multi-object spectrographs, high-resolution spectrographs, integral-field spectroscopy and a world-leading laser guide star adaptive optics system. The Observatory is a private 501(c) 3 non-profit organization and a scientific partnership of the California Institute of Technology, the University of California and NASA.

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UCLA observers will work with MOSFIRE tonight. And UCI/UCB observers will work with NIRC2-LGS/NIRC2-NGS. Sun set 05:59:00pm rise 06:12:00am
Observers from UCR will use MOSFIRE on Keck 1, while on Keck 2, UCI observers will use DEIMOS. Sun set 06:00:00pm rise 06:12:00am
On Keck 1, we have UCR observers using LRIS-ADC. On Keck 2, we have Swinburne observers using ESI. Sun set 06:00:00pm rise 06:11:00am
CIT observers will use LRISP-ADC on Keck 1, and UCSC observers will use ESI on Keck 2 tonight. Sun set 06:01:00pm rise 06:11:00am
Our guests tonight are observers from UCSC and Swinburne, using LRISP-ADC and DEIMOS respectively. Sun set 06:02:00pm rise 06:10:00am