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Canon, Latest Technology

Canon’s Cinema EOS System EOS C300 cinema camera honored with Design for Asia Silver Award

November 21, 2013
Canon Inc.

TOKYO, Japan, November 21, 2013—Canon Inc. announced today that the company’s EOS C300 professional cinema camera (launched in January 2012), part of the company’s Cinema EOS System1 lineup of professional digital cinematography products, was recognized for design excellence by the Hong Kong Design Centre2 with the 2013 Design for Asia Silver Award.


The Cinema EOS System EOS C300
(Shown alongside EF Cinema Lenses)

Launched in 2003, the Design for Asia (DFA) Awards celebrate design excellence, honoring and acknowledging outstanding designs that have the potential to increase the quality and vibrancy of life in Asia and create globally sustainable ideas. Winners of 2013 DFA Awards, including the DFA Grand, DFA Special and DFA Gold and Silver Awards, were selected from among the approximately 970 entries representing designs that were launched between January 1, 2011, and July 31, 2013, in one or more Asian markets.

The launch of the Cinema EOS System lineup of cinema cameras and lenses in January 2012 marked Canon’s entry into the motion picture production industry. The EOS C300, winner of this year’s DFA Silver Award, was the first Cinema EOS System camera introduced and combines exceptional imaging performance with outstanding mobility and expandability to meet the demanding production needs of the motion picture industry.

The Design for Asia accolade, Canon’s first, was achieved following the company’s first-ever submission to the DFA Awards. To date, in addition to being selected as a finalist for an International Design Excellence Award (U.S.A.), the EOS C300 has been recognized with a range of prestigious industry awards, including an iF design award (Germany), a Good Design Award (Japan), and a Machine Design Award (Japan).

Encouraged by this latest industry recognition, Canon will continue striving to create products that combine the highest levels of performance and design excellence.

1
The Cinema EOS System comprises digital cinema cameras, including the EOS C300, and EF Cinema Lenses that deliver high optical performance to support the recording of 4K video and realize the operability required by the film and television production industries.
2
A publicly funded, non-profit organization established in 2002 with the support of the design industry.

 Japan

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Evidence of jet in Milky Way’s black hole

Nov. 20, 2013 — Astronomers have long sought strong evidence that Sagittarius A* (Sgr A*), the supermassive black hole at the center of the Milky Way, is producing a jet of high-energy particles. Finally they have found it, in new results from NASA's Chandra X-ray Observatory and the National Science Foundation's Very Large Array (VLA) radio telescope.

Previous studies, using a variety of telescopes, suggested there was a jet, but these reports -- including the orientation of the suspected jets -- often contradicted each other and were not considered definitive.

"For decades astronomers have looked for a jet associated with the Milky Way's black hole. Our new observations make the strongest case yet for such a jet," said Zhiyuan Li of Nanjing University in China, lead author of a study appearing in an upcoming edition of The Astrophysical Journal and available online now.

Jets of high-energy particles are found throughout the universe, on large and small scales. They are produced by young stars and by black holes a thousand times larger than the Milky Way's black hole. They play important roles in transporting energy away from the central object and, on a galactic scale, in regulating the rate of formation of new stars.

"We were very eager to find a jet from Sgr A* because it tells us the direction of the black hole's spin axis. This gives us important clues about the growth history of the black hole," said Mark Morris of the University of California at Los Angeles, a co-author of the study.

The study shows the spin axis of Sgr A* is pointing in one direction, parallel to the rotation axis of the Milky Way, which indicates to astronomers that gas and dust have migrated steadily into Sgr A* over the past 10 billion years. If the Milky Way had collided with large galaxies in the recent past and their central black holes had merged with Sgr A*, the jet could point in any direction.

The jet appears to be running into gas near Sgr A*, producing X-rays detected by Chandra and radio emission observed by the VLA. The two key pieces of evidence for the jet are a straight line of X-ray emitting gas that points toward Sgr A* and a shock front -- similar to a sonic boom -- seen in radio data, where the jet appears to be striking the gas. Additionally, the energy signature, or spectrum, in X-rays of Sgr A* resembles that of jets coming from supermassive black holes in other galaxies.

Scientists think jets are produced when some material falling toward the black hole is redirected outward. Since Sgr A* is presently known to be consuming very little material, it is not surprising that the jet appears weak. A jet in the opposite direction is not seen, possibly because of gas or dust blocking the line of sight from Earth or a lack of material to fuel the jet.

The region around Sgr A* is faint, which means the black hole has been quiet in the past few hundred years. However, a separate Chandra study announced last month shows that it was at least a million times brighter before then.

"We know this giant black hole has been much more active at consuming material in the past. When it stirs again, the jet may brighten dramatically," said co-author Frederick K. Baganoff of the Massachusetts Institute of Technology in Cambridge, Mass.

Astronomers have suggested the giant bubbles of high-energy particles extending out from the Milky Way and detected by NASA's Fermi Gamma Ray Telescope in 2008 are caused by jets from Sgr A* that are aligned with the rotation axis of the galaxy. The latest results from Chandra support this explanation.

The supermassive black hole at the center of the Milky Way is about four million times more massive than our Sun and lies about 26,000 light-years from Earth. The Chandra observations in this study were taken between September 1999 and March 2011, with a total exposure of about 17 days.

NASA's Marshall Space Flight Center in Huntsville, Ala., manages the Chandra Program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory controls Chandra's science and flight operations from Cambridge, Mass.

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Nokia Music is now Nokia MixRadio, comes with an updated app

Nokia Music for Windows Phone 8 got rebranded in the latest update. The ad-free music streaming service is now called Nokia MixRadio.

The name of the service puts the accent on its free of charge, ad-free music streaming feature. The app has been updated too – it is now centered around a personalized stream, based on the user’s favorite artists.

For $4 a month, users can still gain access to unlimited downloads. Improved audio streaming quality is also included in the price.

Nokia Lumia owners need to update their Nokia Music app to access MixRadio.

Source | Via