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Colin Clark

Phone:+49 511 762-17491Fax:+49 511 762-2784
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Dr. Holger J. Pletsch

Research Group Leader
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Dr. Benjamin Knispel

Press Officer AEI Hannover
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Dr. Elke Müller

Press Officer AEI Potsdam
Phone:+49 331 567-7303Fax:+49 331 567-7298

Publication

1.
C. J. Clark, H. J. Pletsch et al.
PSR J1906+0722: An Elusive Gamma-Ray Pulsar
2.
C. J. Clark, H. J. Pletsch et al.
PSR J1906+0722: An Elusive Gamma-Ray Pulsar

Further information

Einstein@Home Discovery

Hidden in Plain Sight

Max Planck Scientists Discover Elusive Gamma-ray Pulsar with Distributed Computing Project Einstein@Home

August 05, 2015

Gamma-ray pulsars are remnants of explosions that end the lives of massive stars. They are highly-magnetized and rapidly rotating compact neutron stars. Like a cosmic lighthouse they emit gamma-ray photons in a characteristic pattern that repeats with every rotation. However, since only very few gamma-ray photons are detected, finding this hidden rhythm in the arrival times of the photons is computationally challenging. Now, an international team led by researchers at the Max Planck Institute for Gravitational Physics (Albert Einstein Institute, AEI) in Hannover, Germany, has discovered a new gamma-ray pulsar hidden in plain sight in data from the Fermi Gamma-ray Space Telescope. The improved, adaptive data analysis methods and the computing power from the distributed volunteer computing project Einstein@Home were key to their success.
<em>Fermi-LAT</em> sky map with the celestial neighborhood of the newly discovered pulsar&nbsp;<span>PSR J1906+0722 featuring several other gamma-ray pulsars (not labeled). The color scale shows the gamma-ray intensity. The dashed square at the centre encloses the position of the pulsar and the part of the sky shown in more detail in the figure below.</span> Zoom Image
Fermi-LAT sky map with the celestial neighborhood of the newly discovered pulsar PSR J1906+0722 featuring several other gamma-ray pulsars (not labeled). The color scale shows the gamma-ray intensity. The dashed square at the centre encloses the position of the pulsar and the part of the sky shown in more detail in the figure below. [less]

Searching for an Elusive Gamma-ray Pulsar
The gamma-ray source in which the discovery was made was thought to be a pulsar from the year 2012 on, based on the energy distribution of the gamma-ray photons observed by the Large Area Telescope (LAT) on board the Fermi Gamma-ray Space Telescope. For years, it was one of the brightest Fermi-LAT catalogue sources without a known association. “Everyone believed that the source now known as PSR J1906+0722 was a pulsar. The tricky part was to show that the gamma-ray photons carry the imprint of the pulsar's rotation and arrive according to that hidden rhythm. Many had tried that before, but to no avail,” says Holger Pletsch, leader of an independent research group at the AEI and co-author of the paper that now appeared in The Astrophysical Journal Letters.

The Fermi-LAT observations cover a total time of more than six years now. For every single gamma-ray photon received from the pulsar, the AEI scientists had to identify during which of the up to billions of pulsar rotations it was emitted. Since a priori there is very little knowledge about the pulsar's rhythm and its other properties, vast parameter spaces have to be searched very finely – otherwise the hidden signal would be missed. “It's a lot like searching the proverbial needle in haystack, except that beforehand we don't even know what our needle exactly looks like,” says Colin Clark, PhD student in Pletsch's group and lead author of the paper.

An Adaptive Search as Crucial Ingredient
Fermi-LAT's gamma-ray sky resolution is limited, so the sky position is not known well enough beforehand; but an offset in the sky position affects how the arrival times of the photons are reconstructed and whether the correct pulsar rotation phase can be identified for each photon. “We therefore have to search over a grid in the sky around the Fermi-LAT catalogue position. To make sure we do not miss the pulsar, we included a safety margin in our search grid,” explains Clark. “More importantly, we also made our search algorithm adaptive – even if the source was at the edge of the analyzed sky patch, the search algorithm could ‘walk away’ and still find the pulsar.”

It turned out that the new adaptive search method was exactly what was needed to get to the bottom of the riddle of PSR J1906+0722. Its actual sky position is outside the conservatively large region covered by the sky grid, which is why earlier (non-adaptive) searches did not find it. The new methods are also more efficient: They can analyze larger parameter spaces at the same computing costs.

Einstein@Home Contributes Computing Power
Still, the computing costs required for the search are enormous: Blind searches like this one would take several dozens of years on a regular laptop. Therefore, another crucial ingredient for the discovery was the use of the distributed computing project Einstein@Home. Each week, tens of thousands of volunteers from all around the word donate otherwise idle compute cycles on their laptops and desktop computers to the project. “We are very grateful to all Einstein@Home volunteers. Their valuable contributions have made our discovery possible,” says Pletsch.

The pulsar (artist's impression) in the center of the image and its celestial neighborhood. The supernova remnant (magenta) nearby is shown towards the bottom left in <em>Chandra</em> space telescope images. The molecular clouds (green and red) are shown in <em>WISE</em> images. For the&nbsp;<em>Fermi-LAT</em> the supernova remnant and the pulsar merged into a single source which complicated the pulsar discovery. Zoom Image
The pulsar (artist's impression) in the center of the image and its celestial neighborhood. The supernova remnant (magenta) nearby is shown towards the bottom left in Chandra space telescope images. The molecular clouds (green and red) are shown in WISE images. For the Fermi-LAT the supernova remnant and the pulsar merged into a single source which complicated the pulsar discovery. [less]

Supernova Remnant and Star Quake
After their discovery far from the catalogue position, the scientists had an even closer look at the Fermi-LAT data, to find the reason for the offset. By analyzing only those gamma-ray photons received while no pulsed radiation from the pulsar was detected, they were able to identify a second gamma-ray source nearby. In the Fermi-LAT catalogue it had been lumped together with the pulsar into a single source offset from the true pulsar position.

“From our follow-up analysis it appears that the nearby gamma-ray source could be the shock front of a different supernova remnant slamming into a neighboring molecular cloud and generating gamma-rays in the process,” explains Clark.

Upon closer inspection, it also became apparent that the pulsar had suffered a so-called glitch in the year 2009. After the glitch, the pulsar suddenly spun more rapidly than previously and is still settling back to its old rotation rate. This sudden shift also affected the gamma-ray photon arrival times, and complicated the data analysis.

Pulsar glitches are thought to be linked to quakes in the neutron star's crust and their study might provide insights into their interior structure.

<p>A pulsar is a compact neutron star that accelerates charged particles to relativistic speeds in its extremely strong magnetic field. This process produces gamma radiation (violet) far above the surface of the compact remains of the star, for example, while radio waves (green) are emitted over the magnetic poles in the form of a cone. The rotation moves the emission regions across the terrestrial line of sight, making the pulsar light up periodically in the sky.</p> Zoom Image

A pulsar is a compact neutron star that accelerates charged particles to relativistic speeds in its extremely strong magnetic field. This process produces gamma radiation (violet) far above the surface of the compact remains of the star, for example, while radio waves (green) are emitted over the magnetic poles in the form of a cone. The rotation moves the emission regions across the terrestrial line of sight, making the pulsar light up periodically in the sky.

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Finding otherwise Invisible Pulsars with “Blind” Searches
PSR J1906+0722 is not detectable in radio nor in X-ray observations conducted before and after the discovery. “This shows the importance of these ‘blind’ pulsar searches in Fermi-LAT gamma-ray data. Only with these searches that do not require exact prior knowledge will we be able to discover otherwise invisible pulsars. This is an important contribution towards a more complete view of the Galactic pulsar population,” says Pletsch. The combination of new data analysis methods developed at the AEI and the improved ‘Pass 8’ data recently released by the Fermi-LAT collaboration has made these blind searches more sensitive than ever before.

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