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Beyond The Fog Of Time Most Distant Galaxy Ever Unvieled
by Staff Writers
Paris, France (ESO) Oct 21, 2010

Astronomers using ESO's Very Large Telescope (VLT) have measured the distance to the most remote galaxy so far, UDFy-38135539, existing when the Universe was only about 600 million years old (a redshift of 8.6). At this early time, the Universe was not fully transparent and much of it was filled with a hydrogen fog that absorbed the fierce ultraviolet light from young galaxies. The transitional period when the fog was still being cleared by this ultraviolet light is known as the era of reionisation, illustrated with this still from a representative scientific simulation. Credit: M. Alvarez (, R. Kaehler, and T. Abel

A European team of astronomers led by Paris Observatory CNRS Director of Research Matthew Lehnert using ESO's Very Large Telescope (VLT) has measured the distance to the most remote galaxy so far. By carefully analyzing the very faint glow of the galaxy they have found that they are seeing it when the Universe was only about 600 million years old (a redshift of 8.6), or 4.4% of its present age of 13.7 billion years.

These are the first confirmed observations of a galaxy whose light is clearing the opaque hydrogen fog that filled the cosmos at this early time. The results will be presented at an online press conference with the scientists on 19 October 2010, and will appear in the 21 October issue of the journal Nature.

"Using the ESO Very Large Telescope we have confirmed that a galaxy spotted earlier using Hubble is the most remote object identified so far in the Universe" [1], says Matt Lehnert (Observatoire de Paris) who is lead author of the paper reporting the results.

"The power of the VLT and its SINFONI spectrograph allows us to actually measure the distance to this very faint galaxy and we find that we are seeing it when the Universe was less than 600 million years old."

Studying these first galaxies is extremely difficult. By the time that their initially brilliant light gets to Earth they appear very faint and small. Furthermore, this dim light falls mostly in the infrared part of the spectrum because its wavelength has been stretched by the expansion of the Universe - an effect known as redshift.

To make matters worse, at this early time, less than a billion years after the Big Bang, the Universe was not fully transparent and much of it was filled with a hydrogen fog that absorbed the fierce ultraviolet light from young galaxies.

The period when the fog was still being cleared by this ultraviolet light is known as the era of reionization [2]. Despite these challenges the new Wide Field Camera 3 on the NASA/ESA Hubble Space Telescope discovered several robust candidate objects in 2009 [3] that were thought to be galaxies shining in the era of reionization.

Confirming the distances to such faint and remote objects is an enormous challenge and can only reliably be done using spectroscopy from very large ground-based telescopes [4], by measuring the redshift of the galaxy's light.

Matt Lehnert takes up the story: "After the announcement of the candidate galaxies from Hubble we did a quick calculation and were excited to find that the immense light collecting power of the VLT, when combined with the sensitivity of the infrared spectroscopic instrument, SINFONI, and a very long exposure time might just allow us to detect the extremely faint glow from one of these remote galaxies and to measure its distance."

On special request to ESO's Director General they obtained telescope time on the VLT and observed a candidate galaxy called UDFy-38135539 [5] for 16 hours.

After two months of very careful analysis and testing of their results, the team found that they had clearly detected the very faint glow from hydrogen at a redshift of 8.6, which makes this galaxy the most distant object ever confirmed by spectroscopy. A redshift of 8.6 corresponds to a galaxy seen just 600 million years after the Big Bang.

Co-author Nicole Nesvadba (Institut d'Astrophysique Spatiale) sums up this work, "Measuring the redshift of the most distant galaxy so far is very exciting in itself, but the astrophysical implications of this detection are even more important. This is the first time we know for sure that we are looking at one of the galaxies that cleared out the fog which had filled the very early Universe."

One of the surprising things about this discovery is that the glow from UDFy-38135539 seems not to be strong enough on its own to clear out the hydrogen fog.

"There must be other galaxies, probably fainter and less massive nearby companions of UDFy-38135539, which also helped make the space around the galaxy transparent. Without this additional help the light from the galaxy, no matter how brilliant, would have been trapped in the surrounding hydrogen fog and we would not have been able to detect it", explains co-author Mark Swinbank (Durham University).

Co-author Jean-Gabriel Cuby (Laboratoire d'Astrophysique de Marseille) remarks: "Studying the era of reionization and galaxy formation is pushing the capability of current telescopes and instruments to the limit, but this is just the type of science that will be routine when ESO's European Extremely Large Telescope - which will be the biggest optical and near infrared telescope in the world - becomes operational."


[1] An earlier ESO result ( reported an object at a larger distance (a redshift of 10). However, further work failed to find an object of similar brightness at this position, and more recent observations with the NASA/Hubble Space Telescope have been inconclusive. The identification of this object with a galaxy at very high redshift is no longer considered to be valid by most astronomers.

[2] When the Universe cooled down after the Big Bang, about 13.7 billion years ago, electrons and protons combined to form hydrogen gas. This cool dark gas was the main constituent of the Universe during the so-called Dark Ages, when there were no luminous objects. This phase eventually ended when the first stars formed and their intense ultraviolet radiation slowly made the hydrogen fog transparent again by splitting the hydrogen atoms back into electrons and protons, a process known as reionization. This epoch in the Universe's early history lasted from about 150 million to 800 million years after the Big Bang. Understanding how reionization happened and how the first galaxies formed and evolved is one of the major challenges of modern cosmology.

[3] These Hubble observations are described at:

[4] Astronomers have two main ways of finding and measuring the distances to the earliest galaxies. They can take very deep images through differently colored filters and measure the brightness of many objects at different wavelengths. They can then compare these with what is expected of galaxies of different types at different times in the Universe's history. This is the only way currently available to discover these very faint galaxies and is the technique employed by the Hubble team. But this technique is not always reliable. For example, what may seem to be a faint, very distant galaxy can sometimes turn out to be a mundane, cool star in our Milky Way.

Once candidate objects are found more reliable estimates of the distance (measured as the redshift) can be obtained by splitting the light from a candidate object up into its component colors and looking for the telltale signs of emission from hydrogen or other elements in the galaxy. This spectroscopic approach is the only means by which astronomers can obtain the most reliable and accurate measurements of distance.

[5] The strange name indicates that it was found in the Ultra Deep Field search area and the number gives its precise position on the sky.

This research is presented in a paper, "Spectroscopic confirmation of a galaxy at redshift z=8.6," Lehnert et al., to appear in Nature on 21 October 2010. The team is composed of M. D. Lehnert (Observatoire de Paris - Laboratoire GEPI / CNRS-INSU / Universite Paris Diderot, France), N. P. H. Nesvadba (Institut d'Astrophysique Spatiale / CNRS-INSU / Universite Paris-Sud, France), J.-G. Cuby (Laboratoire d'Astrophysique de Marseille / CNRS-INSU / Universite de Provence, France), A. M. Swinbank (Durham University, UK), S. Morris (University of Durham, UK), B. Clement (Laboratoire d'Astrophysique de Marseille / CNRS-INSU / Universite de Provence, France), C. J. Evans (UK Astronomy Technology Centre, Edinburgh, UK), M. N. Bremer (University of Bristol, UK) and S. Basa (Laboratoire d'Astrophysique de Marseille / CNRS-INSU / Universite de Provence, France).


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