Thursday, May 9, 2013

Slacker lures 6 million new listeners, makes profit on both free and paid users

Slacker lures 6 million new listeners, bucks industry with profit on free and paid users

When Slacker launched its big software overhaul in February, many were skeptical that a refresh could bring it back to prominence. Apparently, all that doubt was misguided: Slacker says it's racked up 6 million new listeners in the past three months, 3.5 million of which are on mobile. They're more involved, too -- there are 100,000 new paying customers, iOS installs have tripled and members of all kinds tune in for an average of 25 percent longer. And did we mention that Slacker may even benefit from the rush? Where some peers face a constant fight to stay above water without enough premium customers, Slacker says both its ad-supported free radio and paid on-demand service are profitable. While there's no guarantee the company will hold on to those bedazzled new users, it's good to see renewed competition in a field with fewer and fewer participants.

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Source: Slacker

Source: http://www.engadget.com/2013/05/08/slacker-lures-6-million-new-listeners/?utm_medium=feed&utm_source=Feed_Classic&utm_campaign=Engadget

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Tuesday, May 7, 2013

Record-breaking star explosion is most powerful ever seen

Two NASA space telescopes have captured what appears to be the most powerful star explosion ever detected, a cosmic event so luminous that scientists dubbed it 'eye-wateringly bright' despite being 3.6 billion light-years from Earth.

By Miriam Kramer,?Space.com / May 6, 2013

The Swift space telescope caught sight of the most powerful star explosion ever recorded.

Stefan Immler / Swift / NASA

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Two NASA space telescopes have captured what appears to be the most powerful star explosion ever detected, a cosmic event so luminous that scientists dubbed it "eye-wateringly bright" despite being 3.6 billion light-years from Earth.

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On April 27, NASA's Swift Space Telescope and the Fermi Gamma-ray Space Telescope spotted the highest-energy gamma-ray burst (GRB) ? an explosion of a massive star in the last stage of its life ? ever before seen.

NASA scientists combined the observations into a video animation of the historic gamma-ray burst to illustrate the surprising brightness of this star explosion.

"We have waited a long time for a gamma-ray burst this shockingly, eye-wateringly bright," Julie McEnery, a project scientist for the Fermi Gamma-ray Space Telescope at NASA's Goddard Space Flight Center in Greenbelt, Md., said in a statement. "The GRB lasted so long that a record number of telescopes on the ground were able to catch it while space-based observations were still ongoing."

One of the gamma-rays emitted during the eruption ? seen in the constellation Leo ? was three times more energetic than any other gamma-ray burst recorded by Fermi's Large Area Telescope (LAT), the instrument on the spacecraft responsible for detecting these kinds of explosions.

The gamma-ray burst (named GRB 130427A) was also the longest ever recorded, NASA officials said.

"The GeV [energy] emission from the burst lasted for hours, and it remained detectable by the LAT for the better part of a day, setting a new record for the longest gamma-ray emission from a GRB," NASA officials added.

Gamma-ray bursts are the brightest explosions yet observed in the universe.

"Astronomers think most [gamma-ray bursts] occur when massive stars run out of nuclear fuel and collapse under their own weight," NASA officials said in a statement. "As the core collapses into a black hole, jets of material shoot outward at nearly the speed of light."

Swift's detection of this burst was delayed. The satellite was moving between cosmic targets at the time of the eruption, but the spacecraft captured the explosion less than a minute after it began. Swift also aided astronomers in placing the gamma-ray burst closer to Earth than most other star explosions of its kind, NASA officials said.

"This GRB is in the closest 5 percent of bursts, so the big push now is to find an emerging supernova, which accompanies nearly all long GRBs at this distance," Goddard's Neil Gehrels, principal investigator for Swift, said in a statement.

Scientists are hoping to find a supernova within the area of the explosion in order to trace the gamma-ray burst back to its origins.

Observatories on the ground are keeping an eye on GRB 130427A's area of the sky to locate the supernova by mid-May.

Follow Miriam Kramer on Twitter and Google+. Follow us on Twitter, Facebookand Google+. Original article on SPACE.com.

Copyright 2013 SPACE.com, a TechMediaNetwork company. All rights reserved. This material may not be published, broadcast, rewritten or redistributed.

Source: http://rss.csmonitor.com/~r/feeds/science/~3/iqJanFx1hxI/Record-breaking-star-explosion-is-most-powerful-ever-seen

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Saturday, May 4, 2013

Mathematicians help unlock brain function

May 3, 2013 ? Mathematicians from Queen Mary, University of London will bring researchers one-step closer to understanding how the structure of the brain relates to its function in two recently published studies.

Publishing in Physical Review Letters the researchers from the Complex Networks group at Queen Mary's School of Mathematical Sciences describe how different areas in the brain can have an association despite a lack of direct interaction.

The team, in collaboration with researchers in Barcelona, Pamplona and Paris, combined two different human brain networks -- one that maps all the physical connections among brain areas known as the backbone network, and another that reports the activity of different regions as blood flow changes, known as the functional network. They showed that the presence of symmetrical neurons within the backbone network might be responsible for the synchronised activity of physically distant brain regions.

Lead author Vincenzo Nicosia, said "We don't fully understand how the human brain works. So far the focus has been more on the analysis of the function of single, localised regions. However, there isn't a complete model that brings the whole functionality of the brain together. Hopefully, our research will help neuroscientists to develop a more accurate map of the brain and investigate its functioning beyond single areas."

The research adds to the recent findings published in Proceedings of the National Academy of Sciences in which the QM researchers along with the Department of Psychiatry at University of Cambridge analysed the development of the brain of a small worm called Caenorhabditis elegans. In this paper, the team examined the number of links formed in the brain during the worm's lifespan, and observed an unexpected abrupt change in the pattern of growth, corresponding with the time of egg hatching.

"The research is important as it's the first time that a sharp transition in the growth of a neural network has ever been observed," added Dr Nicosia.

"Although we don't know which biological factors are responsible for the change in the growth pattern, we were able to reproduce the pattern using a simple economical model of synaptic formation. This result can pave the way to a deeper understanding of how neural networks grow in more complex organisms."

The Complex Networks group at Queen Mary is headed by Professor Vito Latora. Aside from theoretical research about the structure and function of complex networks, the group is working on the characterisation of multi-layer brain networks, aimed at reconciling and integrating different brain signals to produce a more informative picture of the human brain.

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The above story is reprinted from materials provided by Queen Mary, University of London.

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Journal Reference:

  1. Vincenzo Nicosia, Miguel Valencia, Mario Chavez, Albert D?az-Guilera, Vito Latora. Remote Synchronization Reveals Network Symmetries and Functional Modules. Physical Review Letters, 2013; 110 (17) DOI: 10.1103/PhysRevLett.110.174102

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Disclaimer: This article is not intended to provide medical advice, diagnosis or treatment. Views expressed here do not necessarily reflect those of ScienceDaily or its staff.

Source: http://feeds.sciencedaily.com/~r/sciencedaily/top_news/~3/9MZnfezMlkE/130503132954.htm

David Rakoff