2013 CASS Student Symposium — Talk title: Searching for Fast
Radio Bursts in the High Time Resolution Universe Survey
A Faster Response Needed to See Fast
Radio Bursts in the Universe - an article I wrote for The Conversation
The ASKAP telescope in Australia found new fast
radio bursts in just three days — and it's not even fully operational yet.
An unknown object that appears close to an expanding cloud of matter from a supernova (top) spat out five strong
radio bursts in 2002 (bottom).
The origin of a fast
radio burst in this type of dwarf galaxy suggests a connection to other energetic events that occur in similar dwarf galaxies, said co-author and UC Berkeley astronomer Casey Law, who led development of the data - acquisition system and created the analysis software to search for rapid, one - off bursts.
Observing a fast
radio burst in conjunction with neutrinos would be a coup, helping establish source objects for both types of phenomena.
Not exact matches
It was a total surprise to them; the idea of
radio wave
bursts had been abandoned after scientists
in the»70s and»80s failed to locate such signals.
The number of wave crests arriving from Fast
Radio Bursts per second — their «frequency» — is in the same range as that of radio sig
Radio Bursts per second — their «frequency» — is
in the same range as that of
radio sig
radio signals.
Penn State University astronomers have discovered that the mysterious «cosmic whistles» known as fast
radio bursts can pack a serious punch,
in some cases releasing a billion times more energy
in gamma - rays than they do
in radio waves and rivaling the stellar cataclysms known as supernovae
in their explosive power.
Fast
radio bursts, which astronomers refer to as FRBs, were first discovered
in 2007, and
in the years since
radio astronomers have detected a few dozen of these events.
Was it the first step on the path to a paradigm shift
in radio astronomy, similar to pulsars or gamma ray
bursts?
«With abundant observational information
in the future, we can gain a better understanding of the physical nature of Fast
Radio Bursts,» said Peter Mészáros, Holder of the Eberly Family Chair
in Astronomy and Astrophysics and Professor of Physics at Penn State, the senior author of the research paper.
Discovery of the gamma - ray «bang» from FRB 131104, the first non-
radio counterpart to any FRB, was made possible by NASA's Earth - orbiting Swift satellite, which was observing the exact part of the sky where FRB 131104 occurred as the
burst was detected by the Parkes Observatory
radio telescope
in Parkes, Australia.
The team also analyzed the
radio waves
in a new way, revealing that what looked like individual
bursts were actually composed of many smaller sub-
bursts, says astronomer Andrew Seymour of the Universities Space Research Association at Arecibo.
«If you have young magnetars that have just been born
in supernova explosions, only a few decades old, they could be very bursty objects, have very violent youths, and that could give rise to repeating fast
radio bursts,» says astronomer Brian Metzger of Columbia University, who was not involved
in the new study.
Hessels thinks «the prospects are quite good» for figuring out what fast
radio bursts are
in the near future.
This artist's impression represents the
burst in different
radio wavelengths: blue is a shorter wavelength, red is longer.
Astronomers are racing to figure out what causes powerful
bursts of
radio light
in the distant cosmos
Although this neutron star's
radio waves don't come
in brief bright
bursts, they are also twisted, the researchers say.
«Since gamma ray
bursts are usually so well behaved, this really stood out,» says
radio astronomer Dale Frail of the National Radio Astronomy Observatory in Soccorro, New Me
radio astronomer Dale Frail of the National
Radio Astronomy Observatory in Soccorro, New Me
Radio Astronomy Observatory
in Soccorro, New Mexico.
Most short gamma - ray
bursts are visible
in X-rays and
radio waves right away and fade over time.
The change
in the
burst's brightness appears to be exactly the same at
radio and optical frequencies; this can happen, say Garnavich and his collaborators Avi Loeb and Kris Stanek from the Center for Astrophysics
in Cambridge, Massachusetts, only if part of the expanding ring passed behind a star located exactly between Earth and the ring itself.
«The discovery of a repeating FRB has not only narrowed down the possible astrophysical origins of FRBs,» says lead author Laura Spitler of the Max Planck Institute for
Radio Astronomy
in Bonn, Germany, «but we also have a better shot at unraveling their nature by being able to observe more
bursts from this source.»
Meanwhile, astronomers at the Very Large Array
radio telescope
in New Mexico were detecting the
burst's
radio - wave aftermath, another first.
A repeating
burst was discovered
in 2012, however, providing an opportunity for a team of researchers to repeatedly monitor its area of the sky with the Karl Jansky Very Large Array
in New Mexico and the Arecibo
radio dish
in Puerto Rico,
in hopes of pinpointing its location.
Those observations, published today
in Nature, reveal that the location of the
bursts coincides with a faint, remote galaxy that also hosts a faint, persistent source of
radio waves.
These
bursts of
radio waves have remained a mystery since the first one was discovered in 2007 by researchers scouring archived data from Australia's Parkes Radio Telescope in search of new pul
radio waves have remained a mystery since the first one was discovered
in 2007 by researchers scouring archived data from Australia's Parkes
Radio Telescope in search of new pul
Radio Telescope
in search of new pulsars.
At the VLA, he currently uses 24 computer central processing units (CPUs)
in parallel, both to record and search the data for brief
radio bursts.
SNATCHING SIGNALS Most of the fast
radio bursts seen to date have been recorded by the Parkes Radio Telescope in New South Wales, Austr
radio bursts seen to date have been recorded by the Parkes
Radio Telescope in New South Wales, Austr
Radio Telescope
in New South Wales, Australia.
Instead, they found a strange
burst of
radio noise recorded
in 2001 that appeared to originate well beyond one of the satellite galaxies that orbit the Milky Way.
This detection follows 11 previously recorded outbursts of
radio waves from the same location, the only known repeater
in a class of enigmatic eruptions known as fast
radio bursts.
The continuing barrage from this repeating source, roughly 3 billion light - years away
in the constellation Auriga, implies that whatever is causing some
radio bursts is not a one - time destructive
Last February a team of astronomers reported detecting an afterglow from a mysterious event called a fast
radio burst, which would pinpoint the precise position of the
burst's origin, a longstanding goal
in studies of these mysterious events.
A team studying data from a recent sky survey has spotted a huge
burst of
radio waves that came and went
in the blink of an eye and has not returned since.
It packed as much energy
in its mere 5 - millisecond duration as the sun puts out
in a month, making it by far the strongest, quickest signal
radio astronomers have observed, although it wasn't nearly as powerful as the elusive gamma ray
bursts that populate the universe.
Reporting online today
in Science, the researchers say they think only two phenomena could be behind the
radio burst they discovered: the merger of two neutron stars or the final evaporation of a black hole.
«The CHIME telescope
in Penticton, British Columbia, should be an excellent instrument for detecting fast
radio bursts and studying their polarization properties,» says Shriharsh Tendulkar, postdoctoral researcher at the McGill Space Institute.
But the authors also speculate that the twisting of the
radio bursts could be explained if FRB 121102 is located
in a powerful nebula (an interstellar cloud of gas and dust) or amid the remains of a dead star.
New detections of
radio waves from a repeating fast
radio burst have revealed an astonishingly potent magnetic field
in the source's environment, indicating that it is situated near a massive black hole or within a nebula of unprecedented power.
«A repeating fast
radio burst from an extreme environment: Extragalactic source of
radio - wave flashes resides
in a powerfully magnetized astrophysical region.»
The amount of twisting observed
in FRB 121102's
radio bursts is among the largest ever measured
in a
radio source, leading the researchers to conclude that the
bursts are passing through an extraordinarily strong magnetic field
in a dense plasma.
The observations by the Breakthrough Listen team at UC Berkeley using the Robert C. Byrd Green Bank Telescope
in West Virginia show that the fast
radio bursts from this object, called FRB 121102, are nearly 100 percent linearly polarized, an indication that the source of the
bursts is embedded
in strong magnetic fields like those around a massive black hole.
The Dutch and Breakthrough Listen teams suggest that the fast
radio bursts may come from a highly magnetized rotating neutron star — a magnetar —
in the vicinity of a massive black hole that is still growing as gas and dust fall into it.
Fast
radio bursts are brief, bright pulses of
radio emission from distant but so far unknown sources, and FRB 121102 is the only one known to repeat: more than 200 high - energy
bursts have been observed coming from this source, which is located
in a dwarf galaxy about 3 billion light years from Earth.
The nearly 100 percent polarization of the
radio bursts is unusual, and has only been seen
in radio emissions from the extreme magnetic environments around massive black holes, such as those at the centers of galaxies.
It has been instrumental
in tasks as diverse as monitoring near - Earth asteroids, watching for bright blasts of energy called fast
radio bursts and searching for extraterrestrial intelligence.
Another team of researchers announced
in August they'd detected an additional 14
bursts, and at higher
radio frequencies than ever observed before.
«The search for nearby fast
radio bursts offers an opportunity for citizen scientists to help astronomers find and study one of the newest species
in the galactic zoo,» says theorist Avi Loeb of the Harvard - Smithsonian Center for Astrophysics (CfA).
This article appeared
in print under the headline «Cosmic
radio burst tracked back to a dwarf galaxy»
That points to neutron stars — which form when short - lived massive stars
in stellar nurseries die — as the source of fast
radio bursts.