Galaxy 'Hunting' Made Easy

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Galaxy 'Hunting' Made Easy

The European Southern Observatory (ESO) press release is reproduced below:

ESO 40/07 - Science Release

14 September 2007
For Immediate Release

Galaxy 'Hunting' Made Easy

Galaxies found under the Glare of Cosmic Flashlights

Astronomers using ESO's Very Large Telescope have discovered in a single pass about a dozen otherwise invisible galaxies halfway across the Universe. The discovery, based on a technique that exploits a first-class instrument, represents a major breakthrough in the field of galaxy 'hunting'.

Images of the region around the 14 quasars where a previously hidden galaxy was detected via its hydrogen emission using the SINFONI instrument on ESO's Very Large Telescope. The contours show the quasars, while the arrow represents 1 arcsecond (~ 26 000 light-years at the distance of these galaxies, which is roughly 7 700 million light-years). North is up, East is left, and the colour-coding reflects the relative hydrogen fluxes of the sources.

The team of astronomers led by Nicolas Bouché have used quasars to find these galaxies. Quasars are very distant objects of extreme brilliance, which are used as cosmic beacons that reveal galaxies lying between the quasar and us. The galaxy's presence is revealed by a 'dip' in the spectrum of the quasar - caused by the absorption of light at a specific wavelength.

The team used huge catalogues of quasars, the so-called SDSS and 2QZ catalogues, to select quasars with dips. The next step was then to observe the patches of the sky around these quasars in search for the foreground galaxies from the time the Universe was about 6 billion years old, almost half of its current age.

"The difficulty in actually spotting and seeing these galaxies stems from the fact that the glare of the quasar is too strong compared to the dim light of the galaxy," says Bouché.

This is where observations taken with SINFONI on ESO's VLT made the difference. SINFONI is an infrared 'integral field spectrometer' that simultaneously delivers very sharp images and highly resolved colour information (spectra) of an object on the sky.

Artist's impression showing a galaxy located between an observer on Earth and a background quasar that acts as a beacon. The light that travels from the quasar is intercepted by the foreground galaxy on its sightline, carrying out the galaxy's signature all the way to the observer. The sketch shows a side-on view of the system. The inset shows a face-on view of it, the same view captured (albeit with less detail) by the images taken with the SINFONI instrument on ESO's Very Large Telescope (see ESO 40a/07).

With this special technique, which untangles the light of the galaxy from the quasar light, the team detected 14 galaxies out of the 20 pre-selected quasar patches of sky, a hefty 70% success rate.

"This high detection rate alone is a very exciting result," says Bouché. "But, these are not just ordinary galaxies: they are most notable ones, actively forming a lot of new stars and qualifying as 'starburst galaxies'."

"We discovered that the galaxies located near the quasar sightlines are forming stars at a prodigious rate, equivalent to 20 suns per year," adds team member Celine Péroux.

These findings represent a big leap forward in the field, setting the stage for a very promising era of galaxy 'hunting'.

The astronomers now plan to use SINFONI to study in more detail each of these galaxies, by measuring their internal motions.

Note

SINFONI is a combination of a novel infrared 'integral field spectrometer' (SPIFFI) and a special adaptive optics module (MACAO). The integral field module SPIFFI gives detailed colour, or spectral, information for each of 2000 spatial points on the sky, arranged over a contiguous two dimensional field of 32 times 64 pixels. SINFONI was developed and built by an international consortium consisting of the Max Planck Institute for Extraterrestrial Physics, Garching, Germany, ESO, and NOVA, Leiden, the Netherlands (see ESO PR 21/04).

More Information

This research is presented in a paper in press in the Astrophysical Journal ("The SINFONI Mg II Program for Line Emitters (SIMPLE): discovering starbursts near QSO sightlines" by N. Bouché et al.). The team is composed of Nicolas Bouché, Richard Davies, Frank Eisenhauer, Natascha M. Förster Schreiber, and Linda Tacconi (Max Planck Institute for Extraterrestrial Physics, Garching, Germany), Michael T. Murphy (Swinburne University of Technology, Australia), and Céline Péroux (ESO).

Contacts

Nicolas Bouché
Max Planck Institute for Extraterrestrial Physics, Garching, Germany
Phone: +49 89 30000 3830
Email: nbouche (at) mpe.mpg.de

Céline Péroux
ESO, Garching, Germany
Email: cperoux (at) eso.org

Michael T. Murphy
Centre for Astrophysics & Supercomputing
Swinburne University of Technology, Australia
Phone: +61 (0)3 9214 5818
Email: mmurphy (at) swin.edu.au

Source: ESO Press Release pr-40-07