MessageToEagle.com - Astronomers at Arizona State University have found an exceptionally distant galaxy,
ranked among the top 10 most distant objects currently known in space.
Light from the recently detected galaxy left the object about 800 million years after the beginning of the universe,
when the universe was in its infancy.
A team of astronomers, led by James Rhoads, Sangeeta Malhotra, and Pascale Hibon of the School of Earth and Space Exploration
at ASU, identified the remote galaxy after scanning a moon-sized patch of sky with the IMACS instrument on the Magellan
Telescopes at the Carnegie Institution's Las Campanas Observatory in Chile.
The observational data reveal a faint infant galaxy, located 13 billion light-years away.
"This galaxy is being observed at a young age. We are seeing it as it was in the very distant past, when the universe
was a mere 800 million years old," says Rhoads, an associate professor in the school.
"This image is like a baby picture of this galaxy, taken when the universe was only 5 percent of its current age.
Studying these very early galaxies is important because it helps us understand how galaxies form and grow."
The galaxy, designated LAEJ095950.99+021219.1, was first spotted in summer 2011. It is a rare example of a
galaxy from that early epoch. It will help astronomers make progress in understanding the process of galaxy formation.
This galaxy, like the others that Malhotra, Rhoads, and their team seek, is extremely faint and was detected by
the light emitted by ionized hydrogen. The object was first identified as a candidate early-universe galaxy in a paper
led by team member and former ASU postdoctoral researcher Hibon. The search employed a unique technique they pioneered
that uses special narrow-band filters that allow a small wavelength range of light through.
A special filter fitted to the telescope camera was designed to catch light of narrow wavelength ranges, allowing the
astronomers to conduct a very sensitive search in the infrared wavelength range. "We have been using this technique since
1998 and pushing it to ever-greater distances and sensitivities in our search for the first galaxies at the
edge of the universe," says Malhotra, an associate professor in the school.
False color image of the galaxy LAEJ095950.99+021219.1 . In this image, blue corresponds to optical light
(wavelength near 500 nm), red to near-infrared light (wavelength near 920 nm), and green to the narrow range of
wavelengths admitted by the narrow bandpass filter (around 968 nm). LAEJ095950.99+021219.1 appears as the green
source near the center of the image cutout. The image shows about 1/6000 of the area that was surveyed. (Credit:
Photo by James Rhoads)
"Young galaxies must be observed at infrared wavelengths and this is not easy to do using ground-based telescopes,
since the Earth's atmosphere itself glows and large detectors are hard to make."
To be able to detect these very distant objects which were forming near the beginning of the universe, astronomers
look for sources which have very high redshifts. Astronomers refer to an object's distance by a number called its
"redshift," which relates to how much its light has stretched to longer, redder wavelengths due to the expansion of
the universe.
Objects with larger redshifts are farther away and are seen further back in time. LAEJ095950.99+021219.1
has a redshift of 7. Only a handful of galaxies have confirmed redshifts greater than 7, and none of the others is
as faint as LAEJ095950.99+021219.1.
"We have used this search to find hundreds of objects at somewhat smaller distances.
We have found several hundred galaxies at redshift 4.5, several at redshift 6.5, and now at redshift 7 we have
found one," explains Rhoads. "We've pushed the experiment's design to a redshift of 7 -- it's the most distant
we can do with well-established, mature technology, and it's about the most distant where people have been
finding objects successfully up to now."
"With this search, we've not only found one of the furthest galaxies known, but also the faintest
confirmed at that distance. Up to now, the redshift 7 galaxies we know about are literally the top one percent of
galaxies. What we're doing here is to start examining some of the fainter ones -- thing that may better represent
the other 99 percent," Malhotra adds.
Resolving the details of objects that are far away is challenging, which is why images of distant young galaxies
such as this one appear small, faint, and blurry.
"As time goes by, these small blobs which are forming stars, they'll dance around each other, merge with each
other and form bigger and bigger galaxies. Somewhere halfway through the age of the universe they start looking
like the galaxies we see today -- and not before. Why, how, when, where that happens is a fairly active area of
research," explains Malhotra.
The find was enabled by the combination of the Magellan telescopes' tremendous light gathering capability and exquisite
image quality, thanks to the mirrors built in Arizona's Steward Observatory; and by the unique ability of the IMACS
instrument to obtain either images or spectra across a very wide field of view.
The research, published in the June 1 issue of The Astrophysical Journal Letters, was supported by the National Science Foundation (NSF).
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