Astronomers from Japan, Sweden, the United Kingdom and ESO have used the Atacama Large Millimeter/submillimeter Array (ALMA to observe one of the most distant galaxies known. SXDF-NB1006-2 lies at a redshift of 7.2, meaning that we see it only 700 million years after the Big Bang.
The team was hoping to find out about the heavy chemical elements  present in the galaxy, as they can tell us about the level of star formation, and hence provide clues about the period in the history of the Universe known as cosmic reionisation.
"Seeking heavy elements in the early Universe is an essential approach to explore the star formation activity in that period," said Akio Inoue of Osaka Sangyo University, Japan, the lead author of the research paper, which is being published in the journal Science. "Studying heavy elements also gives us a hint to understand how the galaxies were formed and what caused the cosmic reionisation," he added.
In the time before objects formed in the Universe, it was filled with electrically neutral gas. But when the first objects began to shine, a few hundred million years after the Big Bang, they emitted powerful radiation that started to break up those neutral atoms -- to ionise the gas. During this phase -- known as cosmic reionisation -- the whole Universe changed dramatically. But there is much debate about exactly what kind of objects caused the reionisation. Studying the conditions in very distant galaxies can help to answer this question.
Before observing the distant galaxy, the researchers performed computer simulations to predict how easily they could expect to see evidence of ionised oxygen with ALMA. They also considered observations of similar galaxies that are much closer to Earth, and concluded that the oxygen emission should be detectable, even at vast distances .
They then carried out high-sensitivity observations with ALMA  and found light from ionised oxygen in SXDF-NB1006-2, making this the most distant unambiguous detection of oxygen ever obtained . It is firm evidence for the presence of oxygen in the early Universe, only 700 million years after the Big Bang.
Oxygen in SXDF-NB1006-2 was found to be ten times less abundant than it is in the Sun. "The small abundance is expected because the Universe was still young and had a short history of star formation at that time," commented Naoki Yoshida at the University of Tokyo. "Our simulation actually predicted an abundance ten times smaller than the Sun. But we have another, unexpected, result: a very small amount of dust."
The team was unable to detect any emission from carbon in the galaxy, suggesting that this young galaxy contains very little un-ionised hydrogen gas, and also found that it contains only a small amount of dust, which is made up of heavy elements. "Something unusual may be happening in this galaxy," said Inoue. "I suspect that almost all the gas is highly ionised."
The detection of ionised oxygen indicates that many very brilliant stars, several dozen times more massive than the Sun, have formed in the galaxy and are emitting the intense ultraviolet light needed to ionise the oxygen atoms.
The lack of dust in the galaxy allows the intense ultraviolet light to escape and ionise vast amounts of gas outside the galaxy. "SXDF-NB1006-2 would be a prototype of the light sources responsible for the cosmic reionisation," said Inoue.
"This is an important step towards understanding what kind of objects caused cosmic reionisation," explained Yoichi Tamura of the University of Tokyo. "Our next observations with ALMA have already started. Higher resolution observations will allow us to see the distribution and motion of ionised oxygen in the galaxy and provide vital information to help us understand the properties of the galaxy."
 In astronomical terminology, chemical elements heavier than lithium are known as heavy elements.
 The Japanese infrared astronomy satellite AKARI had found that this oxygen emission is very bright in the Large Magellanic Cloud, which has an environment similar to the early Universe.
 The original wavelength of the light from doubly ionised oxygen is 0.088 millimetres. The wavelength of the light from SXDF-NB1006-2 is stretched to 0.725 millimetres by the expansion of the Universe, making the light observable with ALMA.
 Earlier work by Finkelstein et al. suggested the presence of oxygen at a slightly earlier time, but there was no direct detection of an emission line, as is the case in the new work.
This research was presented in the paper entitled: "Detection of an oxygen emission line from a high redshift galaxy in the reionization epoch" by Inoue et al., published in the journal Science.
The team is composed of: Akio Inoue (Osaka Sangyo University, Japan), Yoichi Tamura (The University of Tokyo, Japan), Hiroshi Matsuo (NAOJ/Graduate University for Advanced Studies, Japan), Ken Mawatari (Osaka Sangyo University, Japan), Ikkoh Shimizu (Osaka University, Japan), Takatoshi Shibuya (University of Tokyo, Japan), Kazuaki Ota (University of Cambridge, United Kingdom), Naoki Yoshida (University of Tokyo, Japan), Erik Zackrisson (Uppsala University, Sweden), Nobunari Kashikawa (NAOJ/Graduate University for Advanced Studies, Japan), Kotaro Kohno (University of Tokyo, Japan), Hideki Umehata (ESO, Garching, Germany; University of Tokyo, Japan), Bunyo Hatsukade (NAOJ, Japan), Masanori Iye (NAOJ, Japan), Yuichi Matsuda (NAOJ/Graduate University for Advanced Studies, Japan), Takashi Okamoto (Hokkaido University, Japan) and Yuki Yamaguchi (University of Tokyo, Japan).
The Atacama Large Millimeter/submillimeter Array (ALMA), an international astronomy facility, is a partnership of ESO, the U.S. National Science Foundation (NSF) and the National Institutes of Natural Sciences (NINS) of Japan in cooperation with the Republic of Chile. ALMA is funded by ESO on behalf of its Member States, by NSF in cooperation with the National Research Council of Canada (NRC) and the National Science Council of Taiwan (NSC) and by NINS in cooperation with the Academia Sinica (AS) in Taiwan and the Korea Astronomy and Space Science Institute (KASI).
ALMA construction and operations are led by ESO on behalf of its Member States; by the National Radio Astronomy Observatory (NRAO), managed by Associated Universities, Inc. (AUI), on behalf of North America; and by the National Astronomical Observatory of Japan (NAOJ) on behalf of East Asia. The Joint ALMA Observatory (JAO) provides the unified leadership and management of the construction, commissioning and operation of ALMA.
ESO is the foremost intergovernmental astronomy organisation in Europe and the world's most productive ground-based astronomical observatory by far. It is supported by 16 countries: Austria, Belgium, Brazil, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Poland, Portugal, Spain, Sweden, Switzerland and the United Kingdom, along with the host state of Chile. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world's most advanced visible-light astronomical observatory and two survey telescopes. VISTA works in the infrared and is the world's largest survey telescope and the VLT Survey Telescope is the largest telescope designed to exclusively survey the skies in visible light. ESO is a major partner in ALMA, the largest astronomical project in existence. And on Cerro Armazones, close to Paranal, ESO is building the 39-metre European Extremely Large Telescope, the E-ELT, which will become "the world's biggest eye on the sky".
- Research paper - http://www.
eso. org/ public/ archives/ releases/ sciencepapers/ eso1620/ eso1620a.
- Photos of ALMA - http://www.
eso. org/ public/ images/ archive/ search/ ?adv= &subject_name= Atacama%20Large%20Millimeter/ submillimeter%20Array
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