Contact

Priv.-Doz. Dr. habil. Jürgen Kerp
Phone:+49 228 73-3667
Email:jkerp@...

Argelander-Institut für Astronomie der Universität Bonn

Dr. Benjamin Winkel
Phone:+49 2257 301 167

Max-Planck-Institut für Radioastronomie, Effelsberg

Dr. Norbert Junkes
Press and Public Outreach
Phone:+49 228 525-399

Max-Planck-Institut für Radioastronomie, Bonn

Original Paper

Links

HI4PI: A new all-sky survey of neutral hydrogen

High-resolution map of the full sky by combining Effelsberg and Parkes observations at 21 cm wavelength

October 20, 2016

Two of the world's largest fully steerable radio telescopes, the 100-m dish at Effelsberg/Germany and the 64-m Parkes/Australia telescope, mapped the detailed structure of neutral hydrogen across the Northern and Southern hemispheres. Today, the complete survey, HI4PI, is released to the scientific community. It discloses a wealth of fine details of the large scale structure of the Milky Way's gas distribution. HI4PI is the product of a joined effort of astronomers of many countries and will be a mile stone for the decades to come.

The results are published in the current issue of “Astronomy & Astrophysics”.
<p><em>The entire sky in the light of neutral atomic hydrogen (HI) as seen by the Parkes and Effelsberg radio telescope. Our host galaxy, the Milky Way, appears as a luminous band across the sky with the Galactic Center in the middle. The Magellanic Clouds (Large and Small Magellanic Cloud) are prominently visible in orange colors below the Galactic plane. They are surrounded by huge amounts of gas, which was forcefully disrupted from their hosts by gravitational interaction. The HI emission of the Andromeda galaxy (M31) and its neighbor, Triangulum (M33), is also easy to spot as bright purple ellipses in the South-western part of the map. The gas motion is color coded with different hue values, and the visual brightness in the image denotes the intensity of the received HI radiation.</em></p> Zoom Image

The entire sky in the light of neutral atomic hydrogen (HI) as seen by the Parkes and Effelsberg radio telescope. Our host galaxy, the Milky Way, appears as a luminous band across the sky with the Galactic Center in the middle. The Magellanic Clouds (Large and Small Magellanic Cloud) are prominently visible in orange colors below the Galactic plane. They are surrounded by huge amounts of gas, which was forcefully disrupted from their hosts by gravitational interaction. The HI emission of the Andromeda galaxy (M31) and its neighbor, Triangulum (M33), is also easy to spot as bright purple ellipses in the South-western part of the map. The gas motion is color coded with different hue values, and the visual brightness in the image denotes the intensity of the received HI radiation.

[less]

Atomic hydrogen is the most abundant element in space. It is the prime constituent in almost all astronomical objects such as stars, galaxies, and even clusters of galaxies. Hydrogen consists of a single proton and is the simplest element in space. It was already formed during the big bang nucleosynthesis. If the proton is combined with an electron, it is called neutral atomic hydrogen, abbreviated as HI. In addition to the well-known hydrogen spectral lines at visual wavelengths, extremely faint hydrogen line emission can be observed at radio wavelengths, the so-called 21-cm line. Even though the emitted energy is tiny, the sheer amount of hydrogen in space makes the 21-cm line emission observable in nearly all galactic environments, even far beyond the stellar population of galaxies.

In 1951 three independent research groups from the United States, the Netherlands and Australia announced the first detection of HI 21-cm line emission. Now, 65 years later, an international collaboration of scientists from all over the world announced the release of a new full-sky 21-cm spectral line survey, called HI4PI. HI4PI is an acronym for HI across the whole sky (the surface area of the full sphere corresponding to 4*PI steradian). The HI4PI collaboration, led by a German team from Bonn University and Max Planck Institute for Radio Astronomy (MPIfR), is publishing the results in the current issue of "Astronomy and Astrophysics".

With modern radio telescopes, HI is fairly easy to detect towards any direction on the sky. Mapping the whole sky is nevertheless time consuming and costly in terms of manual labor. To map the whole sky demanded more than a million individual observations with two of the World's largest radio telescopes, the 100-m telescope at Effelsberg, Germany, and the Parkes 64-m telescope in Australia. In total, dozens of Tera-bytes of raw data have been recorded. The raw data sets were processed by Astronomers in Bonn, yielding the final data product. “Besides a careful calibration of the data, we also had to remove man-made noise from the data. This so-called radio frequency interference (RFI) is, for example, produced by telecommunication and broadcast stations, or military RADAR and pollutes the faint emission of the astronomical sources”, explains Benjamin Winkel from MPIfR, responsible for the data acquisition and processing in the HI4PI collaboration. “The computational effort for the data processing was huge, adding to the thousands of hours of observations thousands of hours of computing time.”

The new observations were only possible because the technical equipment at radio telescopes was hugely improved in the last decade. On the one hand, new receiving systems utilizing multi-pixel feeds increased the mapping speed by an order of magnitude. On the other hand, extremely capable spectrometers based on state-of-the-art digital processors became available. Previously, state-of-the-art HI data came from the Leiden-Argentine-Bonn survey (LAB), which is based on observations with 30-m class telescopes. The new HI4PI survey has twice the sensitivity and four times better angular resolution compared to the LAB survey.

Because HI is ubiquitous in the universe, HI4PI will serve as a major resource for researchers working with observational data at all wavelengths. As an example, X-ray and Gamma ray photons are partly absorbed, scattered or re-emitted at other wavelengths by Milky Way hydrogen during their journey from outer space to our telescopes. Therefore, the distribution of HI in the Milky Way significantly alters the incoming signal observed by high-energy telescopes. The HI4PI data set allows the scientists to correct for these disturbing effects, cleaning our window to the distant universe.

Also, for astrophysicists studying the Milky Way gas distribution itself, HI4PI will be a valuable new resource. Owing to the increased sensitivity and angular resolution much finer structures of the interstellar medium are now revealed. “Many studies that use pre-release data of the HI4PI survey have already been published in the last years, providing a wealth of new insights and amazing scientific results”, says Peter Kalberla from Bonn University, the leading senior scientist in the project.

“HI4PI sets a benchmark for the decades to come”, concludes Jürgen Kerp, also from Bonn University, the project coordinator and principal investigator of the Effelsberg survey. “Although upcoming new instruments such as the Square Kilometer Array (SKA) will push sensitivity and angular resolution to new realms, being radio interferometers they are by design insensitive to diffusely distributed HI gas. The HI4PI will be the prime resource to add this missing information to the SKA data.”

HI4PI data will be freely accessible on request from interested persons all over the world via CDS, the Strasbourg data center.

<p><em>Two of the largest radio telescopes in the world, utilized for HI4PI, the high-resolution map of the full sky in the light of neutral hydrogen. Effelsberg 100-m radio telescope near Bonn, Germany (left) and Parkes 64-m radio telescope 400 km west of Sydney/Australia (right).</em></p> Zoom Image

Two of the largest radio telescopes in the world, utilized for HI4PI, the high-resolution map of the full sky in the light of neutral hydrogen. Effelsberg 100-m radio telescope near Bonn, Germany (left) and Parkes 64-m radio telescope 400 km west of Sydney/Australia (right).

[less]

-----------------------------------------------

The team comprises the HI4PI Collaboration: N. Ben Bekhti, L. Flöer, R. Keller, J. Kerp, D. Lenz, and B. Winkel, moreover  J. Bailin, M. R. Calabretta, L. Dedes, H. A. Ford, B. K. Gibson, U. Haud, S. Janowiecki, P. M.W. Kalberla, F. J. Lockman, N. M. McClure-Griffiths, T. Murphy, H. Nakanishi, D. J. Pisano, and L. Staveley-Smith.

 

 
loading content