An international team of astronomers led by Fabian Walter of the Max Planck Institute for Astronomy has managed for the first time to determine the distance of the galaxy HDF850.1, well-known among astronomers as being one of the most productive star-forming galaxies in the observable universe. The galaxy is at a distance of 12.5 billion light years. Hence, we see it as it was 12.5 billion years ago, when the universe was less than 10% of its current age. Even more of a surprise, HDF850.1 turns out to be part of a group of around a dozen protogalaxies that formed within the first billion years of cosmic history – only one of two such primordial clusters known to date. The work is being published in the journal Nature.
Figure 1: The region of the Hubble Deep Field where HDF850.1 is located. The cross indicates the submillimeter galaxy's position. For observations with ordinary, visible light telescopes such as the Hubble Space Telescope, the galaxy is completely invisible. Image credit: STScI / NASA, F. Walter (MPIA)
Figure 2: View of the Northern target area for the "Great Observatories Origins Deep Survey" (GOODS-N). The position of the Hubble Deep Field and, within that field, the position of the submillimeter galaxy HDF850.1, are shown separately. HDF850.1 is invisible for observations using ordinary, visible light. Image credit: GOODS-N, STScI / NASA, F. Walter (MPIA)
Figure 3: The Hubble Deep Field, with the position of the submillimeter galaxy HDF850.1 marked with contour lines. The lines represent the date of submillimeter observations of the galaxy; in visible light, it cannot be observed at all. Image credit: STScI / NASA, F. WalterThe galaxy HDF850.1 was discovered in 1998. It is famous for producing new stars at a rate that is near-incredible even on astronomical scales: a combined mass of a thousand Suns per year. For comparison: an ordinary galaxy such as our own produces no more than one solar mass's worth of new stars per year. Yet for the past fourteen years, HDF850.1 has remained strangely elusive – its location in space, specifically: its distance from Earth the subject of many studies, but ultimately unknown. How was that possible?
The "Hubble Deep Field", where HDF850.1 is located, is a region in the sky that affords an almost unparalleled view into the deepest reaches of space. It was first studied extensively using the Hubble Space Telescope. Yet observations using visible light only reveal part of the cosmic picture, and astronomers were quick to follow-up at different wavelengths. In the late 1990s, astronomers using the James Clerk Maxwell Telescope on Hawai'i surveyed the region using submillimeter radiation. This type of radiation, with wavelengths between a few tenths of a millimeter and a millimeter, is particularly suitable for detecting cool clouds of gas and dust.
The researchers were taken by surprise when they realized that HDF850.1 was the brightest source of submillimeter emission in the field by far, a galaxy that was evidently forming as many stars as all the other galaxies in the Hubble Deep Field combined – and which was completely invisible in the observations of the Hubble Space Telescope!
"The galaxy's invisibility is no great mystery. Stars form in dense clouds of gas and dust. These dense clouds are opaque to visible light, hiding the galaxy from sight. Submillimeter radiation passes through the dense dust clouds unhindered, showing what is inside. But the lack of data from all but a very narrow range of the spectrum made it very difficult to determine the galaxy's redshift, and thus its place in cosmic history," explains MPIA's Fabian Walter.
Now, an international group of researchers led by Fabian Walter of the Max Planck Institute for Astronomy has managed to solve the mystery. Taking advantage of recent upgrades to the IRAM interferometer on the Plateau de Bure in the French Alps, which combines six radio antennas that then act as a gigantic millimeter telescope, they identified the characteristic features ("spectral lines") necessary for an accurate distance determination. "It is the availability of more powerful and sensitive instruments recently installed on the IRAM interferometer that allowed us to detect these weak lines in HDF850.1, and finally find what we had been unsuccessfully looking for, during the past 14 years," explains Pierre Cox, Director of IRAM.
The result is a surprise: The galaxy is at a distance of 12.5 billion light-years from Earth (z ~ 5.2). We see it as it was 12.5 billion years ago, at a time when the universe itself was only 1.1 billion years old! HDF850.1's intense star-forming activity thus belongs to a very early period of cosmic history, when the universe was less than 10% of its current age.
A combination with observations obtained at the National Science Foundation's Karl Jansky Very Large Array (VLA) then revealed that a large fraction of the galaxy's mass is in the form of molecules – the raw material for future stars. The fraction is much higher than what is found in galaxies in the local universe.
Once the distance was known, the researchers were also able to put the galaxy into context. Using additional data from published and unpublished surveys, they were able to show that the galaxy is part of what appears to be an early form of galaxy cluster – one of only two such clusters known to date.
The new work highlights the importance of future, more powerful interferometers operating at millimeter and submillimeter wavelengths. Both NOEMA, the future extension of the Plateau de Bure interferometer, and ALMA, a new interferometer array currently being built by an international consortium in the Atacama desert in Chile, will cover these wavelengths in unprecedented detail. They should allow for distance determinations and more detailed study of many more galaxies, invisible at optical wavelengths, that were actively forming stars in the early universe.
The "Hubble Deep Field", where HDF850.1 is located, is a region in the sky that affords an almost unparalleled view into the deepest reaches of space. It was first studied extensively using the Hubble Space Telescope. Yet observations using visible light only reveal part of the cosmic picture, and astronomers were quick to follow-up at different wavelengths. In the late 1990s, astronomers using the James Clerk Maxwell Telescope on Hawai'i surveyed the region using submillimeter radiation. This type of radiation, with wavelengths between a few tenths of a millimeter and a millimeter, is particularly suitable for detecting cool clouds of gas and dust.
The researchers were taken by surprise when they realized that HDF850.1 was the brightest source of submillimeter emission in the field by far, a galaxy that was evidently forming as many stars as all the other galaxies in the Hubble Deep Field combined – and which was completely invisible in the observations of the Hubble Space Telescope!
"The galaxy's invisibility is no great mystery. Stars form in dense clouds of gas and dust. These dense clouds are opaque to visible light, hiding the galaxy from sight. Submillimeter radiation passes through the dense dust clouds unhindered, showing what is inside. But the lack of data from all but a very narrow range of the spectrum made it very difficult to determine the galaxy's redshift, and thus its place in cosmic history," explains MPIA's Fabian Walter.
Now, an international group of researchers led by Fabian Walter of the Max Planck Institute for Astronomy has managed to solve the mystery. Taking advantage of recent upgrades to the IRAM interferometer on the Plateau de Bure in the French Alps, which combines six radio antennas that then act as a gigantic millimeter telescope, they identified the characteristic features ("spectral lines") necessary for an accurate distance determination. "It is the availability of more powerful and sensitive instruments recently installed on the IRAM interferometer that allowed us to detect these weak lines in HDF850.1, and finally find what we had been unsuccessfully looking for, during the past 14 years," explains Pierre Cox, Director of IRAM.
The result is a surprise: The galaxy is at a distance of 12.5 billion light-years from Earth (z ~ 5.2). We see it as it was 12.5 billion years ago, at a time when the universe itself was only 1.1 billion years old! HDF850.1's intense star-forming activity thus belongs to a very early period of cosmic history, when the universe was less than 10% of its current age.
A combination with observations obtained at the National Science Foundation's Karl Jansky Very Large Array (VLA) then revealed that a large fraction of the galaxy's mass is in the form of molecules – the raw material for future stars. The fraction is much higher than what is found in galaxies in the local universe.
Once the distance was known, the researchers were also able to put the galaxy into context. Using additional data from published and unpublished surveys, they were able to show that the galaxy is part of what appears to be an early form of galaxy cluster – one of only two such clusters known to date.
The new work highlights the importance of future, more powerful interferometers operating at millimeter and submillimeter wavelengths. Both NOEMA, the future extension of the Plateau de Bure interferometer, and ALMA, a new interferometer array currently being built by an international consortium in the Atacama desert in Chile, will cover these wavelengths in unprecedented detail. They should allow for distance determinations and more detailed study of many more galaxies, invisible at optical wavelengths, that were actively forming stars in the early universe.
Contact information
Fabian Walter (lead author)
Max Planck Institute for Astronomy
Phone: (+49|0) 6221 – 528 225
Email: walter@mpia.de
Markus Pössel (Public relations)
Max Planck Institute for Astronomy
Heidelberg, Germany
Phone: (+49|0) 6221 – 528 261
Email: pr@mpia.de
Background information
The work described here will be published as F. Walter et al., "The Intense Starburst HDF850.1 in a Galaxy Overdensity at z = 5.2 in the Hubble Deep Field" in the June 14th, 2012, issue of the journal Nature.
The authors are Fabian Walter (Max Planck Institute for Astronomy [MPIA] and National Radio Astronomy Observatory [NRAO], Socorro), Roberto Decarli (MPIA), Chris Carilli (NRAO and Cambridge University), Frank Bertoldi (University of Bonn), Pierre Cox (IRAM), Elisabete Da Cunha (MPIA), Emanuele Daddi (CEA Saclay), Mark Dickinson (NOAO, Tucson), Dennis Downes (IRAM), David Elbaz (CEA Saclay), Richard Ellis (Caltech), Jacqueline Hodge (MPIA), Roberto Neri (IRAM), Dominik Riechers (Caltech), Axel Weiss (Max Planck Institute for Radio Astronomy [MPIfR]), Eric Bell (University of Michigan, Ann Arbor), Helmut Dannerbauer (University od Vienna), Melanie Krips (IRAM), Mark Krumholz (UCSC), Lindley Lentati (Cambridge University), Roberto Maiolino (INAF-Osservatorio Astronomico di Roma and Cambridge University), Karl Menten (MPIfR), Hans-Walter Rix (MPIA), Brant Robertson (University of Arizona), Hyron Spinrad (UC Berkeley), Dan Stark (University of Arizona), and Daniel Stern (Jet Propulsion Laboratory).
The work described here will be published as F. Walter et al., "The Intense Starburst HDF850.1 in a Galaxy Overdensity at z = 5.2 in the Hubble Deep Field" in the June 14th, 2012, issue of the journal Nature.
The authors are Fabian Walter (Max Planck Institute for Astronomy [MPIA] and National Radio Astronomy Observatory [NRAO], Socorro), Roberto Decarli (MPIA), Chris Carilli (NRAO and Cambridge University), Frank Bertoldi (University of Bonn), Pierre Cox (IRAM), Elisabete Da Cunha (MPIA), Emanuele Daddi (CEA Saclay), Mark Dickinson (NOAO, Tucson), Dennis Downes (IRAM), David Elbaz (CEA Saclay), Richard Ellis (Caltech), Jacqueline Hodge (MPIA), Roberto Neri (IRAM), Dominik Riechers (Caltech), Axel Weiss (Max Planck Institute for Radio Astronomy [MPIfR]), Eric Bell (University of Michigan, Ann Arbor), Helmut Dannerbauer (University od Vienna), Melanie Krips (IRAM), Mark Krumholz (UCSC), Lindley Lentati (Cambridge University), Roberto Maiolino (INAF-Osservatorio Astronomico di Roma and Cambridge University), Karl Menten (MPIfR), Hans-Walter Rix (MPIA), Brant Robertson (University of Arizona), Hyron Spinrad (UC Berkeley), Dan Stark (University of Arizona), and Daniel Stern (Jet Propulsion Laboratory).
