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  • richardmitnick 5:04 pm on February 15, 2023 Permalink | Reply
    Tags: "MeerKAT discovers a distant galaxy has very large hydrogen atoms", A Rydberg atom is an excited atom with one or more electrons that have a very high principal quantum number., , , , , Located in the constellation Sagittarius PKS1830-211 is a very distant quasar 11.1 billion light years away., PKS 1830-211 is a hot spot for studying astrochemistry and one of the brightest radio sources in the sky., PKS 1830-211has gas clouds made up of some of the largest hydrogen atoms in the universe-Rydberg atoms., SKA SARAO – South African Radio Astronomy Observatory (SA)   

    From SKA SARAO – South African Radio Astronomy Observatory (SA): “MeerKAT discovers a distant galaxy has very large hydrogen atoms” 

    From SKA SARAO – South African Radio Astronomy Observatory (SA)

    2.15.23

    Kimberly Emig
    kemig@nrao.edu,

    Neeraj Gupta
    ngupta@iucaa.in

    1
    Gravitational lensing. Credit: ESA + K. Emig.

    While using the MeerKAT radio telescope to study a distant galaxy towards PKS 1830-211, scientists discovered something unexpected: gas clouds made up of some of the largest hydrogen atoms in the universe, Rydberg atoms. It is the first time scientists observed these hydrogen atoms in a distant galaxy. What’s more, they believe the large atoms are spread throughout the galaxy in ionized interstellar gas clouds. The discovery could help researchers to understand the nature and evolution of interstellar gas in galaxies and how Rydberg atoms are formed in space.

    A Rydberg atom is an excited atom with one or more electrons that have a very high principal quantum number.

    3
    Figure 1: Electron orbital of a Rydberg atom with n=12. Colors show the quantum phase of the highly excited electron.
    Credit: Berndthaller

    An article reporting this discovery was recently published in The Astrophysical Journal [below].

    Located in the constellation Sagittarius PKS1830-211 is a very distant quasar 11.1 billion light years away (redshift 2.5). However, it is one of the brightest radio sources in the sky since the high-power jet from its super massive black hole is pointed directly at Earth. PKS 1830-211 is a hot spot for studying astrochemistry in the universe. The light from PKS 1830-211 passes through a foreground galaxy 7.3 billion light years distant (redshift 0.89) on its way to Earth, illuminating molecular chemistry in the spiral arms of the foreground galaxy. This rare alignment has allowed the large Hydrogen atoms to be observed.

    A Rydberg atom refers to an atom with an electron in a high energy state. Radio light amplifies the Rydberg atoms. Under just the right conditions, the atoms become naturally occurring lasers, and light becomes brighter at the radio wavelengths emitted by the atoms. Finding just the right conditions for this to occur in distant galaxies has been a long standing mystery. But next-generation radio telescopes observing the Universe at cm to meter wavelengths are making it possible for the first time.

    The South African MeerKAT radio telescope is currently the most sensitive radio telescope observing at these wavelengths. Large surveys that cover the sky using wide bandwidth receivers have high enough precision to look for spectral fingerprints from many wavelengths simultaneously. The MeerKAT Absorption Line Survey (MALS; https://mals.iucaa.in/) is one such survey which observes at 18 to 52 cm wavelengths. Because MALS is targeting the brightest radio sources in the sky, it is currently the most sensitive survey for detecting absorption signatures from hydrogen atoms (in the ground state) and molecules like OH – and unexpectedly, also the large Rydberg atoms.

    Using the MALS survey, scientists found 44 fingerprints from Rydberg atoms. “We used hydrogen Rydberg atoms to study the physical and dynamic structures in a galaxy 7.3 billion light years away towards PKS 1830-211. The Rydberg atoms could be coming from large clouds of gas that are ionized by the radiation from young massive stars. These atoms tell us that interstellar gas in this galaxy is much more dense than what is found in the Milky Way,” says Kimberly Emig, a Jansky Fellow at the National Radio Astronomy Observatory (NRAO) of USA and lead author of the paper.

    Scientists hope to discover more of these oddball atoms. Emig explains, “We were excited to discover these high-excitation hydrogen atoms in such a distant galaxy. It gives a new way to observe our Universe and possibly study the evolution of interstellar gas in galaxies over cosmic time. They could also help us to understand how interstellar gas drives and inhibits the activity of super massive black holes.”

    PKS 1830-211 was the first target of MALS. Its observations helped to characterize the performance of the new MeerKAT telescope. The large volumes of MALS data (1.6 petabytes) are processed using an automated pipeline utilizing the task and tools based on the Common Astronomy Software Applications (CASA) package of NRAO, at a dedicated high performance computing facility setup at the Inter-University Centre for Astronomy and Astrophysics (IUCAA), India.

    The MALS survey primarily uses a transition of atomic hydrogen at 21 cm wavelengths and transitions from the hydroxyl (OH) molecule at 18 cm wavelengths in order to determine the occurrence of atomic and molecular gas in and around galaxies. “Only a small number of these transitions have been detected in distant galaxies so far due to technical limitations. If we detect a large number (several 100) of these transitions then we can assess the physical conditions of cold gas which serves as fuel for star formation in galaxies. Studying ionized gas through hydrogen Rydberg atoms is highly complementary to studying interstellar gas in its atomic and molecular phases and would help us to explain the changes in the properties of galaxies at different ages of the Universe,” explains Neeraj Gupta, astronomer at IUCAA and lead investigator of the MALS project.

    Making this discovery has been a team effort. The South African Radio Astronomy Observatory operates the MeerKAT telescope. An international collaboration from India, Europe, South Africa, North America, and Australia carries out the MeerKAT Absorption Line Survey. Data from the observations is processed through tools of the National Radio Astronomy Observatory, Inter-University Centre for Astronomy and Astrophysics, and Thoughtworks Technologies India Pvt Ltd, among others.

    The Astrophysical Journal
    See the science paper for instructive material with images.

    See the full article here.

    Comments are invited and will be appreciated, especially if the reader finds any errors which I can correct. Use “Reply”.

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    Please help promote STEM in your local schools.

    Stem Education Coalition

    The South African Radio Astronomy Observatory (SARAO), a facility of the National Research Foundation, is responsible for managing all radio astronomy initiatives and facilities in South Africa, including the MeerKAT Radio Telescope in the Karoo, and the Geodesy and VLBI activities at the HartRAO facility. SARAO also coordinates The African Very Long Baseline Interferometry Network (AVN) for the eight SKA partner countries in Africa, as well as South Africa’s contribution to the infrastructure and engineering planning for the Square Kilometre Array Radio Telescope. To maximize the return on South Africa’s investment in radio astronomy, SARAO is managing programmes to create capacity in radio astronomy science and engineering research, and the technical capacity required to support site operations.

    About SKA

    The Square Kilometre Array (AU) 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 Organization, with its headquarters at Jodrell Bank Observatory, near Manchester, UK, was established in December 2011 as a not-for-profit company in order to formalize relationships between the international partners and centralize the leadership of the project.

    SKA Pathfinder – LOFAR location at Potsdam via Google Images.

    The Square Kilometre Array (SKA) project is an international effort to build the world’s largest radio telescope, led by SKA Organization. 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.
    Members

    In February 2021, the members of the SKAO consortium were:

    Australia: Department of Industry and Science
    Canada: National Research Council
    China: National Astronomical Observatories of the Chinese Academy of Sciences
    France: French National Centre for Scientific Research
    Germany: Max-Planck-Gesellschaft
    India: National Centre for Radio Astrophysics
    Italy: National Institute for Astrophysics
    Portugal: Portugal Space
    South Africa: National Research Foundation
    Spain: Institute of Astrophysics of Andalusia
    Sweden: Onsala Space Observatory
    Switzerland: École Polytechnique Fédérale de Lausanne
    The Netherlands: Netherlands Organization for Scientific Research
    United Kingdom: Science and Technology Facilities Council

    As of December 2022, there were 16 countries involved in the project. SKA Organization 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.

     
  • richardmitnick 12:53 pm on January 29, 2023 Permalink | Reply
    Tags: "Canadian researchers will have access to next-generation radio astronomy observatory", "SKA": The Square Kilometre Array, , , , , , SKA Murchison Widefield Array (AU), SKA SARAO – South African Radio Astronomy Observatory (SA), ,   

    From The Dunlap Institute for Astronomy and Astrophysics (CA) At The University of Toronto (CA): “Canadian researchers will have access to next-generation radio astronomy observatory” 

    From The Dunlap Institute for Astronomy and Astrophysics (CA)

    At

    The University of Toronto (CA)

    1.27.23

    Canada intends to proceed to full membership in the Square Kilometre Array Observatory (SKAO), a next-generation radio astronomy observatory bringing together nations from around the world to build and operate cutting-edge radio telescopes.

    ______________________________________________
    The Square Kilometre Array (SKA)– a next-generation telescope due to be completed by the end of the decade – will likely be able to make images of the earliest light in the Universe, but for current telescopes the challenge is to detect the cosmological signal of the stars through the thick hydrogen clouds.

    SKA SARAO Meerkat Telescope (SA), 90 km outside the small Northern Cape town of Carnarvon, SA.

    SKA Hera at SKA South Africa.


    SKA Square Kilometre Array low frequency at the Inyarrimanha Ilgari Bundara Murchison Widefield Array, Boolardy station in outback Western Australia on the traditional lands of the Wajarri peoples.

    EDGES telescope in a radio quiet zone at the Inyarrimanha Ilgari Bundara Murchison Radio-astronomy Observatory in Western Australia, on the traditional lands of the Wajarri peoples.

    SKA Pathfinder – LOFAR location at Potsdam via Google Images.
    ______________________________________________
    SKAO will operate two telescopes – one in Australia and one in South Africa – with headquarters in the United Kingdom. The facility will enable discoveries that will advance our understanding of the universe, the fundamental laws of physics and the prospects for life on other planets. Membership in the SKAO will allow Canada to develop strong scientific, technical and industrial capabilities and collaborations well into the future.

    The decision to proceed with full membership, announced this week by Innovation, Science and Industry Minister François‑Philippe Champagne, is expected to provide Canadian astronomers with a six per cent use-share of the SKAO and support establishing a domestic regional centre. The centre will provide direct connections to data collected with the SKA telescopes and science support to enable ground-breaking discoveries.

    “This is tremendously exciting news,” says Bryan Gaensler, director of the University of Toronto’s Dunlap Institute for Astronomy & Astrophysics in the Faculty of Arts & Science and former science director of the Canadian Square Kilometre Array, a global radio observatory. “Canadian membership in the SKAO was one of the marquee priorities in the Canadian Astronomy Long Range Plan for 2020-2030. Membership will open new opportunities for University of Toronto leadership at an international scale.”

    With full membership, U of T envisages significant involvement in a Canadian SKA Regional Centre as part of its recently established Data Sciences Institute.

    “The SKAO is a key part of U of T’s Strategic Research Plan for 2018 – 2023 and an important institutional priority,” says Leah Cowen, U of T’s vice-president, research and innovation, and strategic initiatives. “It is a brilliant example of a high-impact, interdisciplinary research collaboration that is a reflection of our incredible research community.”

    U of T also leads the $10-million Canadian Initiative for Radio Astronomy Data Analysis (CIRADA), a consortium of six Canadian universities, the National Research Council Canada and many international partners, whose goal is to establish Canadian capability for processing, archiving and sharing the enormous scientific data sets anticipated for the SKA.

    “I’m thrilled to congratulate everyone at U of T for their work over many years in bringing us to this historic commitment,” says Melanie Woodin, dean of the Faculty of Arts & Science. “It’s rewarding to know that the SKAO involves researchers from five Arts & Science units: the Dunlap Institute, the David A. Dunlap Department of Astronomy & Astrophysics, the Canadian Institute for Theoretical Astrophysics, the Department of Physics and the Department of Statistical Sciences.”

    The initial phase of the SKAO consists of 197 radio dishes located in South Africa [MeerKat] and 131,072 antennas located in Australia. Construction on Phase 1 began in June 2021 and is expected to be completed by 2029.

    Canada was one of six founding members of the initial SKAO consortium in 2000 and has maintained substantial involvement and engagement in the SKAO project to date. Canadian astronomers are playing leading roles in designing marquee SKA science programs – including tests of gravity, low-frequency cosmology, cosmic magnetism, dark energy and detecting transient systems. They have multi-wavelength expertise in galaxy evolution, multi-messenger astronomy and planetary system formation.

    “Canada’s commitment to the SKA secures our position at the forefront of astrophysics for the next few decades. Everybody at U of T that has the slightest interest in astronomy should prepare to get absolutely blown away by what the SKA is going to find,” says Roberto Abraham, chair of the David A. Dunlap department of astronomy and astrophysics. “And what makes it extra exciting is that U of T’s leadership in the national consortium means that many of the most amazing discoveries will get made right here. What an exciting time to be an astronomer. To all the young people just getting into the subject: Hold on to your hats – it’s going to be a wild ride!”

    As well as working on many aspects of the SKA project itself, Canadian astronomers are developing a variety of new facilities and experiments aimed at testing the technology needed for the SKAO. Foremost amongst these is the Canadian Hydrogen Intensity Mapping Experiment (CHIME) of which U of T is a member.

    CHIME is a unique radio telescope that can detect fast radio bursts and is making a three-dimensional map of the dark energy that is accelerating the expansion of the universe.

    The NRC points out that for the SKAO, respecting Indigenous cultures and the local populations has been a key consideration from the start: “These core principles are fully aligned with the priorities of the Canadian astronomical community as expressed in the Canadian Astronomy Long Range Plan 2020-2030.”

    See the full article here .

    Comments are invited and will be appreciated, especially if the reader finds any errors which I can correct. Use “Reply”.


    five-ways-keep-your-child-safe-school-shootings

    Please help promote STEM in your local schools.

    Stem Education Coalition

    Dunlap Institute campus

    The Dunlap Institute for Astronomy & Astrophysics (CA) at the University of Toronto (CA) is an endowed research institute with nearly 70 faculty, postdocs, students and staff, dedicated to innovative technology, ground-breaking research, world-class training, and public engagement. The research themes of its faculty and Dunlap Fellows span the Universe and include: optical, infrared and radio instrumentation; Dark Energy; large-scale structure; the Cosmic Microwave Background; the interstellar medium; galaxy evolution; cosmic magnetism; and time-domain science.

    The Dunlap Institute (CA), Department of Astronomy & Astrophysics (CA), Canadian Institute for Theoretical Astrophysics (CA), and Centre for Planetary Sciences (CA) comprise the leading centre for astronomical research in Canada, at the leading research university in the country, the University of Toronto (CA).

    The Dunlap Institute (CA) is committed to making its science, training and public outreach activities productive and enjoyable for everyone, regardless of gender, sexual orientation, disability, physical appearance, body size, race, nationality or religion.

    Our work is greatly enhanced through collaborations with the Department of Astronomy & Astrophysics (CA), Canadian Institute for Theoretical Astrophysics (CA), David Dunlap Observatory (CA), Ontario Science Centre (CA), Royal Astronomical Society of Canada (CA), the Toronto Public Library (CA), and many other partners.

    The University of Toronto participates in the CHIME Canadian Hydrogen Intensity Mapping Experiment at The Canada NRCC Dominion Radio Astrophysical Observatory in Penticton, British Columbia(CA) Altitude 545 m (1,788 ft).


    The The University of Toronto (CA) is a public research university in Toronto, Ontario, Canada, located on the grounds that surround Queen’s Park. It was founded by royal charter in 1827 as King’s College, the oldest university in the province of Ontario.

    Originally controlled by the Church of England, the university assumed its present name in 1850 upon becoming a secular institution.

    As a collegiate university, it comprises eleven colleges each with substantial autonomy on financial and institutional affairs and significant differences in character and history. The university also operates two satellite campuses located in Scarborough and Mississauga.

    The University of Toronto has evolved into Canada’s leading institution of learning, discovery and knowledge creation. We are proud to be one of the world’s top research-intensive universities, driven to invent and innovate.

    Our students have the opportunity to learn from and work with preeminent thought leaders through our multidisciplinary network of teaching and research faculty, alumni and partners.

    The ideas, innovations and actions of more than 560,000 graduates continue to have a positive impact on the world.

    Academically, The University of Toronto is noted for movements and curricula in literary criticism and communication theory, known collectively as the Toronto School.

    The university was the birthplace of insulin and stem cell research, and was the site of the first electron microscope in North America; the identification of the first black hole Cygnus X-1; multi-touch technology, and the development of the theory of NP-completeness.

    The university was one of several universities involved in early research of deep learning. It receives the most annual scientific research funding of any Canadian university and is one of two members of the Association of American Universities outside the United States, the other being McGill University [Université McGill] (CA) .

    The Varsity Blues are the athletic teams that represent the university in intercollegiate league matches, with ties to gridiron football, rowing and ice hockey. The earliest recorded instance of gridiron football occurred at University of Toronto’s University College in November 1861.

    The university’s Hart House is an early example of the North American student centre, simultaneously serving cultural, intellectual, and recreational interests within its large Gothic-revival complex.

    The University of Toronto has educated three Governors General of Canada, four Prime Ministers of Canada, three foreign leaders, and fourteen Justices of the Supreme Court. As of March 2019, ten Nobel laureates, five Turing Award winners, 94 Rhodes Scholars, and one Fields Medalist have been affiliated with the university.

    Early history

    The founding of a colonial college had long been the desire of John Graves Simcoe, the first Lieutenant-Governor of Upper Canada and founder of York, the colonial capital. As an University of Oxford (UK)-educated military commander who had fought in the American Revolutionary War, Simcoe believed a college was needed to counter the spread of republicanism from the United States. The Upper Canada Executive Committee recommended in 1798 that a college be established in York.

    On March 15, 1827, a royal charter was formally issued by King George IV, proclaiming “from this time one College, with the style and privileges of a University … for the education of youth in the principles of the Christian Religion, and for their instruction in the various branches of Science and Literature … to continue for ever, to be called King’s College.” The granting of the charter was largely the result of intense lobbying by John Strachan, the influential Anglican Bishop of Toronto who took office as the college’s first president. The original three-storey Greek Revival school building was built on the present site of Queen’s Park.

    Under Strachan’s stewardship, King’s College was a religious institution closely aligned with the Church of England and the British colonial elite, known as the Family Compact. Reformist politicians opposed the clergy’s control over colonial institutions and fought to have the college secularized. In 1849, after a lengthy and heated debate, the newly elected responsible government of the Province of Canada voted to rename King’s College as the University of Toronto and severed the school’s ties with the church. Having anticipated this decision, the enraged Strachan had resigned a year earlier to open Trinity College as a private Anglican seminary. University College was created as the nondenominational teaching branch of the University of Toronto. During the American Civil War the threat of Union blockade on British North America prompted the creation of the University Rifle Corps which saw battle in resisting the Fenian raids on the Niagara border in 1866. The Corps was part of the Reserve Militia lead by Professor Henry Croft.

    Established in 1878, the School of Practical Science was the precursor to the Faculty of Applied Science and Engineering which has been nicknamed Skule since its earliest days. While the Faculty of Medicine opened in 1843 medical teaching was conducted by proprietary schools from 1853 until 1887 when the faculty absorbed the Toronto School of Medicine. Meanwhile the university continued to set examinations and confer medical degrees. The university opened the Faculty of Law in 1887, followed by the Faculty of Dentistry in 1888 when the Royal College of Dental Surgeons became an affiliate. Women were first admitted to the university in 1884.

    A devastating fire in 1890 gutted the interior of University College and destroyed 33,000 volumes from the library but the university restored the building and replenished its library within two years. Over the next two decades a collegiate system took shape as the university arranged federation with several ecclesiastical colleges including Strachan’s Trinity College in 1904. The university operated the Royal Conservatory of Music from 1896 to 1991 and the Royal Ontario Museum from 1912 to 1968; both still retain close ties with the university as independent institutions. The University of Toronto Press was founded in 1901 as Canada’s first academic publishing house. The Faculty of Forestry founded in 1907 with Bernhard Fernow as dean was Canada’s first university faculty devoted to forest science. In 1910, the Faculty of Education opened its laboratory school, the University of Toronto Schools.

    World wars and post-war years

    The First and Second World Wars curtailed some university activities as undergraduate and graduate men eagerly enlisted. Intercollegiate athletic competitions and the Hart House Debates were suspended although exhibition and interfaculty games were still held. The David Dunlap Observatory in Richmond Hill opened in 1935 followed by the University of Toronto Institute for Aerospace Studies in 1949. The university opened satellite campuses in Scarborough in 1964 and in Mississauga in 1967. The university’s former affiliated schools at the Ontario Agricultural College and Glendon Hall became fully independent of the University of Toronto and became part of University of Guelph (CA) in 1964 and York University (CA) in 1965 respectively. Beginning in the 1980s reductions in government funding prompted more rigorous fundraising efforts.

    Since 2000

    In 2000 Kin-Yip Chun was reinstated as a professor of the university after he launched an unsuccessful lawsuit against the university alleging racial discrimination. In 2017 a human rights application was filed against the University by one of its students for allegedly delaying the investigation of sexual assault and being dismissive of their concerns. In 2018 the university cleared one of its professors of allegations of discrimination and antisemitism in an internal investigation after a complaint was filed by one of its students.

    The University of Toronto was the first Canadian university to amass a financial endowment greater than c. $1 billion in 2007. On September 24, 2020 the university announced a $250 million gift to the Faculty of Medicine from businessman and philanthropist James C. Temerty- the largest single philanthropic donation in Canadian history. This broke the previous record for the school set in 2019 when Gerry Schwartz and Heather Reisman jointly donated $100 million for the creation of a 750,000-square foot innovation and artificial intelligence centre.

    Research

    Since 1926 the University of Toronto has been a member of the Association of American Universities a consortium of the leading North American research universities. The university manages by far the largest annual research budget of any university in Canada with sponsored direct-cost expenditures of $878 million in 2010. In 2018 the University of Toronto was named the top research university in Canada by Research Infosource with a sponsored research income (external sources of funding) of $1,147.584 million in 2017. In the same year the university’s faculty averaged a sponsored research income of $428,200 while graduate students averaged a sponsored research income of $63,700. The federal government was the largest source of funding with grants from the Canadian Institutes of Health Research; the Natural Sciences and Engineering Research Council; and the Social Sciences and Humanities Research Council amounting to about one-third of the research budget. About eight percent of research funding came from corporations- mostly in the healthcare industry.

    The first practical electron microscope was built by the physics department in 1938. During World War II the university developed the G-suit- a life-saving garment worn by Allied fighter plane pilots later adopted for use by astronauts.Development of the infrared chemiluminescence technique improved analyses of energy behaviours in chemical reactions. In 1963 the asteroid 2104 Toronto was discovered in the David Dunlap Observatory (CA) in Richmond Hill and is named after the university. In 1972 studies on Cygnus X-1 led to the publication of the first observational evidence proving the existence of black holes. Toronto astronomers have also discovered the Uranian moons of Caliban and Sycorax; the dwarf galaxies of Andromeda I, II and III; and the supernova SN 1987A. A pioneer in computing technology the university designed and built UTEC- one of the world’s first operational computers- and later purchased Ferut- the second commercial computer after UNIVAC I. Multi-touch technology was developed at Toronto with applications ranging from handheld devices to collaboration walls. The AeroVelo Atlas which won the Igor I. Sikorsky Human Powered Helicopter Competition in 2013 was developed by the university’s team of students and graduates and was tested in Vaughan.

    The discovery of insulin at The University of Toronto in 1921 is considered among the most significant events in the history of medicine. The stem cell was discovered at the university in 1963 forming the basis for bone marrow transplantation and all subsequent research on adult and embryonic stem cells. This was the first of many findings at Toronto relating to stem cells including the identification of pancreatic and retinal stem cells. The cancer stem cell was first identified in 1997 by Toronto researchers who have since found stem cell associations in leukemia; brain tumors; and colorectal cancer. Medical inventions developed at Toronto include the glycaemic index; the infant cereal Pablum; the use of protective hypothermia in open heart surgery; and the first artificial cardiac pacemaker. The first successful single-lung transplant was performed at Toronto in 1981 followed by the first nerve transplant in 1988; and the first double-lung transplant in 1989. Researchers identified the maturation promoting factor that regulates cell division and discovered the T-cell receptor which triggers responses of the immune system. The university is credited with isolating the genes that cause Fanconi anemia; cystic fibrosis; and early-onset Alzheimer’s disease among numerous other diseases. Between 1914 and 1972 the university operated the Connaught Medical Research Laboratories- now part of the pharmaceutical corporation Sanofi-Aventis. Among the research conducted at the laboratory was the development of gel electrophoresis.

    The University of Toronto is the primary research presence that supports one of the world’s largest concentrations of biotechnology firms. More than 5,000 principal investigators reside within 2 kilometres (1.2 mi) from the university grounds in Toronto’s Discovery District conducting $1 billion of medical research annually. MaRS Discovery District is a research park that serves commercial enterprises and the university’s technology transfer ventures. In 2008, the university disclosed 159 inventions and had 114 active start-up companies. Its SciNet Consortium operates the most powerful supercomputer in Canada.

     
  • richardmitnick 11:22 am on December 3, 2022 Permalink | Reply
    Tags: "Extraterrestrial signal search is underway using the southern hemisphere’s biggest radio telescope", "Technosignatures": indicators of technology developed by extraterrestrial intelligence, , , , , SKA SARAO – South African Radio Astronomy Observatory (SA), This initiative expands the number of targets searched by a factor of 1000.   

    From SKA SARAO – South African Radio Astronomy Observatory (SA): “Extraterrestrial signal search is underway using the southern hemisphere’s biggest radio telescope” 

    From SKA SARAO – South African Radio Astronomy Observatory (SA)

    12.1.22

    Breakthrough Listen has begun observations of a million nearby stars with the MeerKAT Array [below].

    Breakthrough Listen – the initiative to find signs of intelligent life in the universe – announced today, at a conference organized by the South African Radio Astronomy Observatory (SARAO), the start of observations using a powerful new instrument deployed to the MeerKAT radio telescope in the remote Karoo region of South Africa. The new search for technosignatures – indicators of technology developed by extraterrestrial intelligence – expands the number of targets searched by a factor of 1000.


    Artist’s impression of the MeerKAT telescope in South Africa, and the Breakthrough Listen compute cluster, scanning the sky for possible signals (represented as binary codes) from extraterrestrial intelligence. One of the first targets to be observed by the new instrument will be the Alpha Centauri system, represented as the three stars towards the top right of the image. Credit: Danielle Futselaar / Breakthrough Listen / SARAO

    The astronomers and engineers on the Breakthrough Listen team have spent the last three years developing and installing the most powerful digital instrumentation ever deployed in the search for technosignatures, and integrating the equipment with the MeerKAT control and monitoring systems in cooperation with SARAO engineers. The new hardware complements Listen’s ongoing searches using the Green Bank Telescope in the USA, the Parkes Telescope in Australia, and other telescopes around the world. But while Listen’s programs at the GBT and Parkes involve moving these thousand-ton-plus dishes to point at targets all over the sky, the program on MeerKAT usually won’t mechanically move the antennas.

    “MeerKAT consists of 64 dishes, which can see an area of the sky 50 times bigger than the GBT can view at once,” explained Breakthrough Listen Principal Investigator Dr. Andrew Siemion. “Such a large field of view typically contains many stars that are interesting technosignature targets. Our new supercomputer enables us to combine signals from the 64 dishes to get high resolution scans of these targets with excellent sensitivity, all without impacting the research of other astronomers who are using the array.”

    By operating in this “commensal” mode, Breakthrough Listen gains access to one of the world’s most capable and sensitive radio telescopes almost 24 hours a day, 7 days a week. The ability to scan 64 targets at a time within the main field of view also improves Listen’s ability to reject interfering signals from human technology such as Earth-orbiting satellites. The Listen team had to develop sophisticated targeting and scheduling software to ensure the survey goals could be met in the desired timeframe 1. They have also developed an automated data processing pipeline that scans through the data in near-real-time to search for interesting signals.

    Breakthrough Listen is also working with SARAO to develop research opportunities for astronomers and data processing experts in Africa on this cutting-edge program. The search for life in the Universe has become a major focus area for research internationally, and the Breakthrough Initiatives are leaders in the field.

    “I am very excited to be able to conduct a search for technosignatures using one of the most sensitive telescopes in the world,” remarked Dr. Cherry Ng, Breakthrough Listen’s Project Scientist for MeerKAT. “It will take us just two years to search over one million nearby stars. MeerKAT will provide us with the ability to detect a transmitter akin to Earth’s brightest radio beacons out to a distance of 250 light years in our routine observing mode.”

    Dr. Fernando Camilo, Chief Scientist for SARAO, the observatory that built and operates MeerKAT, is also excited about the new search.

    “MeerKAT has a remarkable combination of sensitivity and survey speed, which makes it a wonderful telescope for SETI,” said Camilo. “The telescope was planned and developed here in South Africa, and it’s very exciting that young South Africans will have the chance to be involved at the forefront of the search for life beyond Earth.”

    “One of the first targets we’ll be observing is our nearest neighbor star, Proxima Centauri, which appears to host two small rocky planets in the star’s habitable zone,” said Breakthrough Initiatives Executive Director, Dr. S. Pete Worden. “Routine observations with the Listen backend on MeerKAT are now underway, and the team looks forward to sharing the first science results in the coming months.”

    See the full article here.

    Comments are invited and will be appreciated, especially if the reader finds any errors which I can correct. Use “Reply”.

    five-ways-keep-your-child-safe-school-shootings

    Please help promote STEM in your local schools.

    Stem Education Coalition

    The South African Radio Astronomy Observatory (SARAO), a facility of the National Research Foundation, is responsible for managing all radio astronomy initiatives and facilities in South Africa, including the MeerKAT Radio Telescope in the Karoo, and the Geodesy and VLBI activities at the HartRAO facility. SARAO also coordinates The African Very Long Baseline Interferometry Network (AVN) for the eight SKA partner countries in Africa, as well as South Africa’s contribution to the infrastructure and engineering planning for the Square Kilometre Array Radio Telescope. To maximize the return on South Africa’s investment in radio astronomy, SARAO is managing programmes to create capacity in radio astronomy science and engineering research, and the technical capacity required to support site operations.

    About SKA

    The Square Kilometre Array (AU) 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 Organization, with its headquarters at Jodrell Bank Observatory, near Manchester, UK, was established in December 2011 as a not-for-profit company in order to formalize relationships between the international partners and centralize the leadership of the project.

    SKA SARAO Meerkat Telescope (SA), 90 km outside the small Northern Cape town of Carnarvon, SA.

    SKA Pathfinder – LOFAR location at Potsdam via Google Images.

    The Square Kilometre Array (SKA) project is an international effort to build the world’s largest radio telescope, led by SKA Organization. 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 Organization 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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