Discovering Teenage Galaxies Billions Of Light Years Away

The team, led by Martin Haehnelt of the University of Cambridge, UK, Michael Rauch and George Becker of the Observatories of the Carnegie Institution, USA, and Andy Bunker of the Anglo-Australian Observatory, reports their results in the 1 March 2008 issue of the Astrophysical Journal.

"The farther we look back into space the farther we see back in time," explained Rauch." We were actually trying to measure a faint signal from intergalactic gas caused by the cosmic ultraviolet background radiation. But as often happens in science, we got a surprise and found something we weren't looking for--dozens of faint, discrete objects emitting radiation from neutral hydrogen in the so-called Lyman alpha line, a fundamental signature of protogalaxies."

A popular theory of galaxy formation predicts that the gas accreted forming smaller protogalaxies, which then collided and merged to become the massive galaxies seen today. The new discovery lends strong support to this theory.

During the 1990s there was mounting evidence in favor of this hierarchical picture of galactic evolution, including measurements of distant quasars by Rauch and collaborators that showed how the properties of cosmic gas clouds--the reservoir of matter for galaxy formation--fit within that scheme.

"Most of those gas clouds are dark and visible only as foreground objects, which cast something of a shadow against a bright background quasar," Becker said. "Intriguingly, one class of these shadows--known as damped Lyman alpha systems--was suspected to arise when those small, protogalactic building blocks intersect the line-of-sight to the quasar. For many years, these shadows were our only hint that a population of numerous early galaxies existed."

"This is the first time that the sky has been searched to this depth and the unrivalled sensitivity of the picture taken with the VLT was key to succeeding," says Haehnelt.

"Previous attempts have usually been frustrated by the difficulty of detecting extremely faint objects: the amount of time required even with an 8-metre class telescope like the VLT considerably exceeds typical observing time awards. We have thus exploited the periods of less good weather with the FORS2 spectrograph at the VLT, taking advantage of the service observing mode," says Becker.

In service mode, ESO staff astronomers at Paranal are responsible for carrying out the actual observations, taking all the specific requirements into account.

"We were actually trying to measure a faint signal from intergalactic gas caused by the cosmic ultraviolet background radiation. But as often happens in science, we got a surprise and found something we weren't looking for--dozens of faint, discrete objects emitting radiation from neutral hydrogen in the so-called Lyman alpha line, a fundamental signature of protogalaxies," explains Rauch.

The same small patch of sky, centred on a quasar, was observed between 2004 and 2006 for an unprecedented 92 hours, the equivalent of about 12 complete nights, allowing the astronomers to obtain a spectrum of the Universe when it was only 2 billion years old.

The result of this search is the detection of 27 faint objects. The weak light signal that the team has detected from these distant objects implies low star formation rates and a small amount of chemical enrichment, suggesting that they are indeed at an early stage of formation.

"The properties of the emitters seem to provide an excellent match to those of 'Damped Lyman Alpha Systems', the main reservoir of neutral hydrogen in the far Universe," says Andy Bunker. "This suggests that the objects found are the long-sought counterparts of the DLAS in emission. The new observations confirm theoretical research proposing that galaxies like our own have formed by the amalgamation of small proto-galaxies early on in the history of the Universe," he adds.

"What makes our discovery particularly exciting is that it opens the route to find large numbers of building blocks of normal galaxies and that we will now be able to study in detail how galaxies like our Milky Way have come together, " says Martin Haehnelt.

The results are reported in a paper in press in the Astrophysical Journal ("A Population of Faint Extended Line Emitters and the Host Galaxies of Optically Thick QSO Absorption Systems", by M. Rauch et al.). The team is composed of Michael Rauch and George Becker (Observatories of the Carnegie Institution of Washington, Pasadena, USA), Martin Haehnelt (Institute of Astronomy, Cambridge, UK), Andrew Bunker (Anglo-Australian Observatory and School of Physics, Exeter, UK), Francine Marleau (Spitzer Science Center, Caltech, USA), James Graham (University of California, Berkeley, USA), Stefano Cristiani (Osservatorio Astronomico di Trieste, INAF, Italy), Matt J. Jarvis (University of Hertfordshire, UK), Cedric Lacey, Simon Morris, and Tom Theuns (Durham University, UK), Celine Peroux (Observatoire Astronomique de Marseille-Provence, France), and Huub Röttgering (Leiden Observatory, The Netherlands)