Andrew Yee[_1_]
May 8th 08, 05:15 AM
ROYAL ASTRONOMICAL SOCIETY PRESS INFORMATION NOTE
Issued by RAS Press Officers:
Dr Robert Massey
Tel: +44 (0)20 7734 3307 / 4582
Anita Heward
Tel: +44 (0)1483 420904
NATIONAL ASTRONOMY MEETING PRESS ROOM (31 MARCH - 4 APRIL ONLY):
Tel: +44 (0)2890 975262 / 975263 / 975264
NAM 2008
http://nam2008.qub.ac.uk
Royal Astronomical Society
http://www.ras.org.uk
CONTACTS
Dr Sebastien Foucaud
School of Physics and Astronomy
University of Nottingham
University Park
Nottingham NG7 2RD
Tel: (+44) (0) 115 846 8857
Fax: (+44) (0) 115 846 6070
Dr. Omar Almaini
School of Physics and Astronomy
University of Nottingham
University Park
Nottingham NG7 2RD
Tel: (+44) (0) 115 846 79 01
Fax: (+44) (0) 115 846 60 70
Prof. Andy Lawrence
Institute for Astronomy
Royal Observatory
Blackford Hill
Edinburgh EH9 3HJ
Phone: +44 (0)131 668 8346 (direct)
EMBARGOED UNTIL 0001 BST, 4 April 2008
Ref.: PN 08/30 (NAM 21)
Witnessing the formation of distant galaxies
UK astronomers have produced the most sensitive infrared map of the distant
Universe ever undertaken. Combining data over a period of three years, they
have produced an image containing over 100,000 galaxies over an area four
times the size of the full Moon. Some of the first results from this project
will be presented by Dr Sebastien Foucaud from the University of Nottingham
on Friday 4th April at the RAS National Astronomy Meeting in Belfast.
Due to the finite speed of light, these observations allow astronomers to
look back in time over 10 billion years, producing images of galaxies in the
Universe's infancy. The image is so large and so deep that thousands of
galaxies can be studied at these early epochs for the first time. By
observing in the infrared, astronomers can now peer further back in time,
since light from the most distant galaxies is shifted towards redder
wavelengths as it travels through the expanding Universe.
"I would compare these observations to the ice cores drilled deep into the
Antarctic," said Dr Foucaud. "Just as they allow us to peer back in time,
our ultra-deep image allows us to look back and observe galaxies evolving at
different stages in cosmic history, all the way back to just 1 billion years
after the Big Bang."
One of the key aims is to understand when the rarest, most massive galaxies
form in the distant Universe, which is a long-standing unsolved problem in
astronomy. "We see galaxies 10 times the mass of the Milky Way already in
place at very early epochs. Now, for the first time, we are sampling a large
enough volume of the distant Universe to be able to see them in sufficient
numbers and really pin down when they were formed."
The image was obtained using the United Kingdom Infrared Telescope (UKIRT)
in Hawaii. The results presented today form part of the Ultra-Deep Survey
(UDS), led by Dr Omar Almaini at the University of Nottingham. The UDS is
one element of a five-part project, the UKIRT Infrared Deep Sky Survey,
which commenced in 2005. Professor Andy Lawrence, Principle Investigator of
UKIDSS from the University of Edinburgh, said "As we keep taking images over
the next few years, we will see ever more distant galaxies."
IMAGES
The image is available at:
http://www.nottingham.ac.uk/~ppzsf/foucaud_press_release_nam08.jpg
Caption: Zooming into a small fraction of the UKIDSS UDS field, the deepest
infrared image ever obtained over such a large area. The zoom shows a
relatively nearby spiral galaxy. Many of the faint red objects in the
background are massive galaxies at distances of over 10 billion light years.
LINKS
* The UKIDSS Ultra-Deep Survey
http://www.nottingham.ac.uk/astronomy/UDS/
* UKIDSS
http://www.ukidss.org
* UKIRT
http://www.jach.hawaii.edu/UKIRT/
* Nottingham Astronomy group
http://www.nottingham.ac.uk/astronomy/
NOTES FOR EDITORS
RAS NATIONAL ASTRONOMY MEETING
The RAS National Astronomy Meeting (NAM 2008) is hosted by Queens University
Belfast. It is principally sponsored by the RAS and the STFC. NAM 2008 is
being held together with the UK Solar Physics (UKSP) and Magnetosphere,
Ionosphere and Solar-Terrestrial (MIST) spring meetings.
UKIRT
The world's largest telescope dedicated solely to infrared astronomy, the
3.8-metre (12.5-foot) UK Infrared Telescope (UKIRT), is sited near the
summit of Mauna Kea, Hawaii, at an altitude of 4194 metres (13760 feet)
above sea level. It is operated by the Joint Astronomy Centre in Hilo,
Hawaii, on behalf of the UK Science and Technology Facilities Council.
Further information about the UK Infrared Telescope:
http://outreach.jach.hawaii.edu/articles/aboutukirt/
SCIENCE AND TECHNOLOGY FACILITIES COUNCIL
The Science and Technology Facilities Council is an independent,
non-departmental public body of the Office of Science and Innovation which
itself is part of the Department of Innovation, Universities and Skills. It
was formed as a new Research Council on 1 April 2007 through a merger of the
Council for the Central Laboratory of the Research Councils (CCLRC) and the
Particle Physics and Astronomy Research Council (PPARC) and the transfer of
responsibility for nuclear physics from the Engineering and Physical
Sciences Research Council (EPSRC). It is one of seven national research
councils in the UK.
Issued by RAS Press Officers:
Dr Robert Massey
Tel: +44 (0)20 7734 3307 / 4582
Anita Heward
Tel: +44 (0)1483 420904
NATIONAL ASTRONOMY MEETING PRESS ROOM (31 MARCH - 4 APRIL ONLY):
Tel: +44 (0)2890 975262 / 975263 / 975264
NAM 2008
http://nam2008.qub.ac.uk
Royal Astronomical Society
http://www.ras.org.uk
CONTACTS
Dr Sebastien Foucaud
School of Physics and Astronomy
University of Nottingham
University Park
Nottingham NG7 2RD
Tel: (+44) (0) 115 846 8857
Fax: (+44) (0) 115 846 6070
Dr. Omar Almaini
School of Physics and Astronomy
University of Nottingham
University Park
Nottingham NG7 2RD
Tel: (+44) (0) 115 846 79 01
Fax: (+44) (0) 115 846 60 70
Prof. Andy Lawrence
Institute for Astronomy
Royal Observatory
Blackford Hill
Edinburgh EH9 3HJ
Phone: +44 (0)131 668 8346 (direct)
EMBARGOED UNTIL 0001 BST, 4 April 2008
Ref.: PN 08/30 (NAM 21)
Witnessing the formation of distant galaxies
UK astronomers have produced the most sensitive infrared map of the distant
Universe ever undertaken. Combining data over a period of three years, they
have produced an image containing over 100,000 galaxies over an area four
times the size of the full Moon. Some of the first results from this project
will be presented by Dr Sebastien Foucaud from the University of Nottingham
on Friday 4th April at the RAS National Astronomy Meeting in Belfast.
Due to the finite speed of light, these observations allow astronomers to
look back in time over 10 billion years, producing images of galaxies in the
Universe's infancy. The image is so large and so deep that thousands of
galaxies can be studied at these early epochs for the first time. By
observing in the infrared, astronomers can now peer further back in time,
since light from the most distant galaxies is shifted towards redder
wavelengths as it travels through the expanding Universe.
"I would compare these observations to the ice cores drilled deep into the
Antarctic," said Dr Foucaud. "Just as they allow us to peer back in time,
our ultra-deep image allows us to look back and observe galaxies evolving at
different stages in cosmic history, all the way back to just 1 billion years
after the Big Bang."
One of the key aims is to understand when the rarest, most massive galaxies
form in the distant Universe, which is a long-standing unsolved problem in
astronomy. "We see galaxies 10 times the mass of the Milky Way already in
place at very early epochs. Now, for the first time, we are sampling a large
enough volume of the distant Universe to be able to see them in sufficient
numbers and really pin down when they were formed."
The image was obtained using the United Kingdom Infrared Telescope (UKIRT)
in Hawaii. The results presented today form part of the Ultra-Deep Survey
(UDS), led by Dr Omar Almaini at the University of Nottingham. The UDS is
one element of a five-part project, the UKIRT Infrared Deep Sky Survey,
which commenced in 2005. Professor Andy Lawrence, Principle Investigator of
UKIDSS from the University of Edinburgh, said "As we keep taking images over
the next few years, we will see ever more distant galaxies."
IMAGES
The image is available at:
http://www.nottingham.ac.uk/~ppzsf/foucaud_press_release_nam08.jpg
Caption: Zooming into a small fraction of the UKIDSS UDS field, the deepest
infrared image ever obtained over such a large area. The zoom shows a
relatively nearby spiral galaxy. Many of the faint red objects in the
background are massive galaxies at distances of over 10 billion light years.
LINKS
* The UKIDSS Ultra-Deep Survey
http://www.nottingham.ac.uk/astronomy/UDS/
* UKIDSS
http://www.ukidss.org
* UKIRT
http://www.jach.hawaii.edu/UKIRT/
* Nottingham Astronomy group
http://www.nottingham.ac.uk/astronomy/
NOTES FOR EDITORS
RAS NATIONAL ASTRONOMY MEETING
The RAS National Astronomy Meeting (NAM 2008) is hosted by Queens University
Belfast. It is principally sponsored by the RAS and the STFC. NAM 2008 is
being held together with the UK Solar Physics (UKSP) and Magnetosphere,
Ionosphere and Solar-Terrestrial (MIST) spring meetings.
UKIRT
The world's largest telescope dedicated solely to infrared astronomy, the
3.8-metre (12.5-foot) UK Infrared Telescope (UKIRT), is sited near the
summit of Mauna Kea, Hawaii, at an altitude of 4194 metres (13760 feet)
above sea level. It is operated by the Joint Astronomy Centre in Hilo,
Hawaii, on behalf of the UK Science and Technology Facilities Council.
Further information about the UK Infrared Telescope:
http://outreach.jach.hawaii.edu/articles/aboutukirt/
SCIENCE AND TECHNOLOGY FACILITIES COUNCIL
The Science and Technology Facilities Council is an independent,
non-departmental public body of the Office of Science and Innovation which
itself is part of the Department of Innovation, Universities and Skills. It
was formed as a new Research Council on 1 April 2007 through a merger of the
Council for the Central Laboratory of the Research Councils (CCLRC) and the
Particle Physics and Astronomy Research Council (PPARC) and the transfer of
responsibility for nuclear physics from the Engineering and Physical
Sciences Research Council (EPSRC). It is one of seven national research
councils in the UK.