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  • richardmitnick 12:15 pm on December 23, 2018 Permalink | Reply
    Tags: , , , , , , HIRAX South African astronomy project, New fellowships, ,   

    From Perimeter Institute: “New fellowships to fuel fundamental physics with radio telescopes in Canada” 

    Perimeter Institute

    From Perimeter Institute

    December 20, 2018

    Perimeter Institute and Canada’s National Research Council have created a pair of postdoctoral fellowships for exceptional emerging radio astronomers.

    As radio astronomy enters a transformative new era, Perimeter Institute and Canada’s National Research Council (NRC) have launched two new fellowships to accelerate the research of young scientists conducting theory, data analysis, or instrument development.

    The new initiative is a collaboration between Perimeter and NRC’s Dominion Radio Astrophysical Observatory (DRAO), the site of Canada’s revolutionary Canadian Hydrogen Intensity Mapping Experiment (CHIME) Telescope.

    CHIME Canadian Hydrogen Intensity Mapping Experiment -A partnership between the University of British Columbia, the University of Toronto, McGill University, Yale and the National Research Council in British Columbia, at the Dominion Radio Astrophysical Observatory in Penticton,British Columbia

    Instruments like CHIME and forthcoming experiments possess unprecedented statistical power, promising to open new windows into fundamental physics questions, including dark matter, gravity, and neutrinos. These instruments will be used to tackle new challenges in data analysis and high-performance computing, and will help scientists resolve deep astronomical puzzles, such as the origin of fast radio bursts (FRBs).

    The Perimeter-DRAO partnership will bring together theorists, data analysts, and instrumentalists at the leading edge of this very exciting field.

    One of the postdoctoral fellows will be based at the DRAO, with the other at Perimeter Institute; each will be encouraged to spend time at the other institution to deepen the partnership and strengthen the connections between the institutions.

    Perimeter Institute is part of a number of radio astronomy collaborations, including CHIME/FRB, HIRAX (Hydrogen Intensity and Real-time Analysis Experiment), and the EHT (Event Horizon Telescope), among others.

    SKA HIRAX prototype dishes at Hartebeesthoek Astronomy Observatory near Johannesburg.

    EHT map

    EHT APEX, IRAM, G. Narayanan, J. McMahon, JCMT/JAC, S. Hostler, D. Harvey, ESO/C. Malin

    Perimeter researchers associated with these initiatives include Avery Broderick, Ue-Li Pen, Will Percival, Daniel Siegel, Kendrick Smith, and Neil Turok.

    In addition to hosting CHIME in British Columbia and several other radio telescopes, DRAO features laboratories and specialized equipment for the design and construction of all aspects of radio-frequency instrumentation, from highly sensitive antennae and receiver systems to high-speed digital signal processing hardware and software. This national facility is home to astronomers, astrophysicists, engineers, and technologists, as well as visiting researchers and students from universities and astronomical observatories around the world.

    The deadline to apply for the fellowships is January 31, 2019. Find more information and apply here.

    See the full article here .


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    About Perimeter
    Perimeter Institute is the world’s largest research hub devoted to theoretical physics. The independent Institute was founded in 1999 to foster breakthroughs in the fundamental understanding of our universe, from the smallest particles to the entire cosmos. Research at Perimeter is motivated by the understanding that fundamental science advances human knowledge and catalyzes innovation, and that today’s theoretical physics is tomorrow’s technology. Located in the Region of Waterloo, the not-for-profit Institute is a unique public-private endeavour, including the Governments of Ontario and Canada, that enables cutting-edge research, trains the next generation of scientific pioneers, and shares the power of physics through award-winning educational outreach and public engagement.

     
  • richardmitnick 5:27 pm on August 23, 2018 Permalink | Reply
    Tags: , , , , HIRAX South African astronomy project,   

    From SKA via SPACE.com: “New Telescope Chases the Mysteries of Radio Flashes and Dark Energy -Not a SKA Project 


    From SKA

    via

    SPACE.com

    South African HIRAX prototype dishes at Hartebeesthoek Astronomy Observatory near Johannesburg.

    South Africa is becoming one of the world’s most important radio astronomy hubs, thanks in large part to its role as co-host of the Square Kilometre Array (SKA). Now a new telescope is being unveiled that will be built at the SKA South Africa site in the Karoo. This is not a part of SKA but it will benefit from SKA. The Hydrogen Intensity and Real-time Analysis eXperiment (HIRAX) project is an international collaboration being led by scientists from the University of KwaZulu-Natal. The Conversation Africa chatted to project leader Professor Kavilan Moodley about HIRAX’s scientific goals.

    What will HIRAX do, and how?

    It’s an interferometer array that will be made up of 1024 6-metre dishes. Interferometer arrays are really cool because they combine signals from many telescopes to provide the resolution of a larger telescope.

    HIRAX has two main science goals: to study the evolution of dark energy by tracking neutral hydrogen gas in galaxies, and to detect and localise mysterious radio flashes called fast radio bursts.

    Dark energy is a mysterious force driving the accelerated expansion of our universe. HIRAX can study it using a unique cosmic ruler provided by nature, called baryon acoustic oscillations. These were generated in the very early universe, which was a hot and dense soup of particles and light. Small irregularities gave rise to sound waves in this primordial soup.

    These waves carried matter as they travelled until a time when matter and light separated, distributing matter in a very characteristic pattern. Neutral hydrogen gas is a great tracer of the universe’s matter distribution. This neutral hydrogen emits a signal at 1420 MHz, which is in the range of frequencies used by cellular networks and UHF television channels; the signal gets stretched to lower frequencies as the universe expands.

    HIRAX will operate between 400 and 800 MHz allowing it to map neutral hydrogen in the universe between 7 to 11 billion years ago. Studying the characteristics of dark energy during this time has the potential to unravel its properties, as this is a vital time when dark energy became the primary component in the universe and accelerated its expansion.

    The second focus area involves mysterious bright, millisecond flashes that scientists call fast radio bursts. Scientists do not know what causes these. They’re also hard to detect and localise since they’re so brief and most telescopes only observe a small region of the sky.

    HIRAX’s large field of view will allow it to observe large portions of sky daily – so when the flashes happen, the instrument will be more likely to see them. We expect that it’ll see up to a dozen of these flashes a day; to put that in perspective, only a few dozen in total have ever been observed.

    And HIRAX will add the unique capability of being able to figure out exactly where in the sky these fast radio bursts occur, by working with several other Southern African countries to build 8-dish outrigger arrays. These, in combination with the main array, will help localise these bursts to within their hosting galaxies.

    It sounds like HIRAX will be collecting huge amounts of data?

    It will need to collect large amounts of data at a rate of around 6.5 Terabits per second. That’s comparable to all of Africa’s international bandwidth. For that, HIRAX needs to design and manufacture high precision dishes, receivers and other instrumentation; we’re working with local companies on this challenge.

    Then the team will need to figure out smart ways to compress, store and analyse this data. That will require big data hardware and software.

    We hope that the design and manufacturing abilities required to equip HIRAX properly will open up many opportunities for local industries in the region around the SKA project.

    Is this an SKA project, or entirely separate but using space and technology at the SKA?

    The project originated as a response by UKZN and its partner institutions to a call for institutional flagship projects by the National Research Foundation. So it’s independent from the SKA and its precursor, the MeerKAT – but will benefit greatly from the South African investment in the SKA project, which gives it access to excellent infrastructure hosted by the South African Radio Astronomy Observatory.

    By sharing a location with MeerKAT on the SKA South Africa site, HIRAX will be able to conduct science in “radio-clear” skies across its wide frequency range; legislation has been introduced to limit radio frequency interference on the SKA SA site. It’s also a great space because it allows access to the southern sky covered by other cosmological surveys and, in turn, more of the galaxy where we’ll find pulsars.

    Being part of the “Karoo radio park” will allow HIRAX to add to South Africa’s radio astronomy engineering and infrastructure. This infrastructure and the resulting science will increase South Africa’s reputation as a global leader in radio astronomy.

    HIRAX will also contribute to training the next generation of scientists for the SKA; students working on the project will be trained in all aspects of the telescope, from engineering to science. Students who build hardware are also involved in data analysis, which provides a special environment for training upcoming radio astronomy experts.

    Finally, there are strong scientific synergies with MeerKAT (which was officially launched in July 2018). If HIRAX discovers any interesting new pulsars, for instance, MeerKAT can conduct follow-up timing observations at higher frequencies.

    See the full article here .

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    Please help promote STEM in your local schools.

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    SKA ASKAP Pathefinder Telescope

    SKA Meerkat telescope, 90 km outside the small Northern Cape town of Carnarvon, SA


    SKA Meerkat Telescope

    Murchison Widefield Array,SKA Murchison Widefield Array, Boolardy station in outback Western Australia, at the Murchison Radio-astronomy Observatory (MRO)


    SKA Murchison Wide Field Array
    About SKA

    The Square Kilometre Array will be the world’s largest and most sensitive radio telescope. The total collecting area will be approximately one square kilometre giving 50 times the sensitivity, and 10 000 times the survey speed, of the best current-day telescopes. The SKA will be built in Southern Africa and in Australia. Thousands of receptors will extend to distances of 3 000 km from the central regions. The SKA will address fundamental unanswered questions about our Universe including how the first stars and galaxies formed after the Big Bang, how dark energy is accelerating the expansion of the Universe, the role of magnetism in the cosmos, the nature of gravity, and the search for life beyond Earth. Construction of phase one of the SKA is scheduled to start in 2016. The SKA Organisation, with its headquarters at Jodrell Bank Observatory, near Manchester, UK, was established in December 2011 as a not-for-profit company in order to formalise relationships between the international partners and centralise the leadership of the project.

    The Square Kilometre Array (SKA) project is an international effort to build the world’s largest radio telescope, led by SKA Organisation. The SKA will conduct transformational science to improve our understanding of the Universe and the laws of fundamental physics, monitoring the sky in unprecedented detail and mapping it hundreds of times faster than any current facility.

    Already supported by 10 member countries – Australia, Canada, China, India, Italy, New Zealand, South Africa, Sweden, The Netherlands and the United Kingdom – SKA Organisation has brought together some of the world’s finest scientists, engineers and policy makers and more than 100 companies and research institutions across 20 countries in the design and development of the telescope. Construction of the SKA is set to start in 2018, with early science observations in 2020.

     
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