From University of Sydney (AU): “Sydney Institute for Astronomy (SIfA)”

U Sidney bloc

From University of Sydney (AU)

Siding Spring Observatory, Coonabarabran, Warrumbungle National Park, NSW. Siding Spring Mountain [Mount Woorat] with Anglo-Australian Telescope dome visible near centre of image at an altitude of 1,165 m (3,822 ft).

ESO VLT at Cerro Paranal in the Atacama Desert, •ANTU (UT1; The Sun ),
•KUEYEN (UT2; The Moon ),
•MELIPAL (UT3; The Southern Cross ), and
•YEPUN (UT4; Venus – as evening star).
elevation 2,635 m (8,645 ft) from above Credit J.L. Dauvergne & G. Hüdepohl atacama photo.

Mauna Kea Observatory, Hawaii USA, altitude 4,213 m (13,822 ft).

The Sydney Institute for Astronomy (SIfA) is a national and international leader in Astronomy and Astrophysics.

Through cutting edge theoretical and observational research and the application of new technology for the next generation of instruments and telescopes. As well as being a research leader, SIfA is committed to excellence in postgraduate training and research-led undergraduate training.

SIfA scientists conduct research in many exciting frontline areas including exoplanets, asteroseismology, stellar and plasma astrophysics, black-hole binaries, supernovae, transient sources, the interstellar medium, and the Galactic Centre. We carry out detailed studies of the Local Group of galaxies, including the Milky Way, Andromeda and the Magellanic Clouds. At greater distances, we study active galaxies & quasars, clusters of galaxies, gravitational lensing, and cosmology. Our scientists perform supercomputer simulations of galaxy formation and evolution of large-scale structure.

SIfA has leadership or key involvement in several major surveys including the Kepler K2GAP survey, the Galactic Archaeology (GALAH) survey of a million stars, the Southern Stellar Stream Spectroscopic Survey (S5), the SAMI Galaxy Survey, the OzDES galaxy survey, the FLASH survey of radio galaxies, the MAGPI survey of galaxies in the cosmic “middle-ages” and the VAST survey for radio transients on the Australian SKA Pathfinder (ASKAP) telescope.

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Our Galaxy’s spiral arms – similar to the ones in this photo of NGC 6744 – can push stars into new orbits. Credit: ESO.

SIfA is one of three institutions that make up the Australian Astronomical Optics (AAO) consortium. We run the Sydney Astrophotonic Instrumentation Labs (SAIL) and invent new technologies for astronomy and industry, develop cubesats for space launch, and build instruments for Australian and international telescopes, including the next generation of Extremely Large Telescopes.

SIfA is a host institution for the Australian Research Council (ARC) Centres of Excellence; All Sky Astrophysics in 3D (ASTRO-3D) and Dark Matter Particle Physics (DMPP). We are affiliated with the ARC Centre for Gravitational Wave Discovery (OzGrav) and a member of the GROWTH telescope network based at Caltech, U.S.A.. SIfA is also a host institution for the Danish-led Stellar Astrophysics Centre (SAC) and a member of the Stellar Oscillations Network Group (SONG).

In 2017, Australia joined the European Southern Observatory (ESO) as a partner. Since then, SIfA has been a major recipient of observing time with the Very Large Telescope. We obtain data from major international facilities on the ground and in space, and receive large allocations of observing time on the Anglo-Australian Telescope (optical) and the Australia Telescope National Facility (radio). Each year, SIfA astronomers are also awarded several million hours of supercomputer time.

See the full article here .

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Please help promote STEM in your local schools.

Stem Education Coalition

University of Sydney (AU)
Our founding principle as Australia’s first university, U Sydney was that we would be a modern and progressive institution. It’s an ideal we still hold dear today.

When Charles William Wentworth proposed the idea of Australia’s first university in 1850, he imagined “the opportunity for the child of every class to become great and useful in the destinies of this country”.

We’ve stayed true to that original value and purpose by promoting inclusion and diversity for the past 160 years.

It’s the reason that, as early as 1881, we admitted women on an equal footing to male students. Oxford University didn’t follow suit until 30 years later, and Jesus College at Cambridge University did not begin admitting female students until 1974.

It’s also why, from the very start, talented students of all backgrounds were given the chance to access further education through bursaries and scholarships.

Today we offer hundreds of scholarships to support and encourage talented students, and a range of grants and bursaries to those who need a financial helping hand.