Monday, September 24, 2007

MIT model could improve some drugs' effectiveness


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24hoursnews-In this image, a fragment of the antibody Erbitux (cetuximab) binds to its target, a fragment of epidermal growth factor receptor (EGFR). The blue ribbon at the top is the backbone of the EGFR fragment, and the red and gray ribbons at the bottom are the backbone of the antibody fragment. The licorice sticks and the balls in the central portion represent protein side chains making close interactions between the antigen (EGFR) and the antibody, with the balls representing one of the mutations designed computationally.


MIT researchers have developed a computer modeling approach that could improve a class of drugs based on antibodies, molecules key to the immune system. The model can predict structural changes in an antibody that will improve its effectiveness.


The team has already used the model to create a new version of cetuximab, a drug commonly used to treat colorectal cancer, that binds to its target with 10 times greater affinity than the original molecule.


The work, which will appear Sept. 23 in an advance publication of Nature Biotechnology, results from a collaboration using both laboratory experiments and computer simulations, between MIT Professors Dane Wittrup and Bruce Tidor.


"New and better methods for improving antibody development represent critical technologies for medicine and biotechnology," says Wittrup, who holds appointments in MIT's Department of Biological Engineering and Department of Chemical Engineering. Tidor holds appointments in Biological Engineering and the Department of Electrical Engineering and Computer Science.


Antibodies, which are part of nature's own defense system against pathogens, are often used for diagnostics and therapeutics. Starting with a specific antibody, the MIT model looks at many possible amino-acid substitutions that could occur in the antibody. It then calculates which substitutions would result in a structure that would form a stronger interaction with the target.


"Combining information about protein (antibody) structure with calculations that address the underlying atomic interactions allows us to make rational choices about which changes should be made to a protein to improve its function," said Shaun Lippow, lead author of the Nature Biotechnology paper.


"Protein modeling can reduce the cost of developing antibody-based drugs," Lippow added, "as well as enable the design of additional protein-based products such as enzymes for the conversion of biomass to fuel." Lippow conducted the research as part of his thesis work in chemical engineering at MIT, and is now a member of the protein engineering group at Codon Devices in Cambridge, Mass.


"Making drugs out of huge, complicated molecules like antibodies is incredibly hard," said Janna Wehrle, who oversees computational biology grants at the National Institute of General Medical Sciences, which partially supported the research. "Dr. Tidor's new computational method can predict which changes in an antibody will make it work better, allowing chemists to focus their efforts on the most promising candidates. This is a perfect example of how modern computing can be harnessed to speed up the development of new drugs."


Traditionally, researchers have developed antibody-based drugs using an evolutionary approach. They remove antibodies from mice and further evolve them in the laboratory, screening for improved efficacy. This can lead to improved binding affinities but the process is time-consuming, and it restricts the control that researchers have over the design of antibodies.


In contrast, the MIT computational approach can quickly calculate a huge number of possible antibody variants and conformations, and predict the molecules' binding affinity for their targets based on the interactions that occur between atoms.


Using the new approach, researchers can predict the effectiveness of mutations that might never arise by natural evolution.


"The work demonstrates that by building on the physics underlying biological molecules, you can engineer improvements in a very precise way," said Tidor.


The team also used the model with an anti-lysozyme antibody called D44.1, and they were able to achieve a 140-fold improvement in its binding affinity. The authors expect the model will be useful with other antibodies as well.


The research was funded by the National Science Foundation and the National Institutes of Health.


Wittrup and Tidor also co-teach a class focusing on connecting fundamental molecular and cellular events to biological function through the use of mathematical models and computer simulations




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Friday, September 14, 2007

Stars caught in bizarre death-dance



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24hoursnews


The low-mass companion in SWIFT J1756.9-2508 may have a mass just a few times greater than Jupiter, but up close, it would probably look nothing like a planet. The object is probably dominated by helium gas. Even though it is much larger than the pulsar, the pulsar is at least 100 times more massive. Image / Aurore Simonnet, Sonoma State University


In this artist depiction of the SWIFT J1756.9-2508 system, the foreground object is the planet-mass object. The pulsar, located at the upper right, is tidally distorting the companion into a teardrop-shaped object, and ripping gas from it. This material flows in a stream toward the pulsar and forms a disk around it. Eventually, enough gas builds up in the disk to produce an outburst bright enough to make the system visible from Earth. Image / Aurore Simonnet, Sonoma State University



NASA astronomers have found a bizarre Planet-Mass orbiting a neutron star.


The object's minimum mass is only about seven times that of Jupiter, but instead of orbiting a normal star, this low-mass body orbits a rapidly spinning pulsar.


It orbits the pulsar every 54.7 minutes at an average distance of only about 230,000 miles (slightly less than the Earth-Moon distance).


MIT astronomers played a key role in discovering what NASA calls one of the most bizarre objects in space: a star "skeleton" of very low mass that is orbiting and being slowly consumed by a pulsar, or remains of a second massive star, that is itself spinning faster than a kitchen blender.


A NASA team led by Hans Krimm and Craig Markwardt at Goddard Space Flight Center and an MIT team led by Deepto Chakrabarty, an associate professor of physics in MIT's Kavli Institute for Astrophysics and Space Research, described the overall system (known by its abbreviation SWIFT J1756.9) in an article accepted for publication in the Astrophysical Journal Letters.


"While we already know of several cases of pulsars that have consumed or vaporized most of the mass in their companion star, SWIFT J1756.9 is possibly the most extreme example," said Chakrabarty.


Systems like SWIFT J1756.9 provide a rare opportunity for astronomers to examine how millisecond pulsars are spun up to such incredibly rapid speeds, and to determine their eventual fate, he added.


SWIFT J1756.9 was discovered earlier this year using NASA's Swift and Rossi X-Ray Timing Explorer (RXTE) satellites. The RXTE observations indicate that the pulsar, a type of neutron star, is spinning 182.07 times per second, even though it is believed to contain at least 1.4 times the mass of the sun but is only about 10 miles across. "This means that the surface of the star is moving at about 7000 miles per second, or roughly 4 percent the speed of light," Chakrabarty said.


The companion object was found to orbit the pulsar every 54.7 minutes at an average distance of only about 230,000 miles (slightly less than the Earth-Moon distance). It has what astronomers consider a very low mass: about seven times that of Jupiter. For comparison, the sun is over 1000 times more massive than Jupiter.


"This object is merely the skeleton of a star," says Markwardt. "The pulsar has eaten away the star's outer envelope, and all that remains is its helium-rich core."


The system is only the eighth millisecond pulsar observed to be pulling mass from a companion, and only one other such system has a companion with such a low mass. The companion in that system also has a minimum mass of about seven Jupiters.


The system probably formed several billion years ago, when it consisted of a very massive star and a smaller star. The more massive star evolved quickly and exploded as a supernova, leaving behind a pulsar. The smaller star eventually started to puff up as it aged, and the two objects became embedded in the extended stellar envelope. This drained orbital energy, causing the two stars to draw ever nearer.


Today, the two objects are so close to each other that the pulsar's powerful gravity produces a tidal bulge on its companion, siphoning off gas that flows into a disk that surrounds the pulsar. The flow eventually becomes unstable and dumps large quantities of gas onto the pulsar, causing an outburst like the one observed in June.


With an estimated distance of roughly 25,000 light-years, the system is normally too faint to be detected, and is only visible during an outburst. SWIFT J1756.9 has never been seen to erupt until this June, so as Markwardt points out, "We don't know how long it will slumber before it wakes up again."


In addition to Chakrabarty, the MIT team includes Jacob Hartman, a graduate student in physics who defended his Ph.D. thesis on August 2.


More



Bizarre planet-mass object orbiting neutron star detected




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Thursday, September 13, 2007

Silicon Storage Technology’s gets a boost,


24hoursnewsThursday, September 13th, 2007 at 3:38 pm in Silicon Storage Technology.


You have to forgive Silicon Storage Technology (ticker:SSTI) if it's feeling a bit down in the dumps lately. The Sunnyvale maker of flash storage products for consumer devices could use a friend right about now. It's struggling to sort out its potential backdated options problems, it's fighting delisting by Nasdaq because it hasn't filed financial statements in about a year, and its stock price has been hovering around $3 per share for the past few months.


On Thursday, SST got a big hug, but not necessarily the kind it wanted.


Los Angeles-based Riley Investment Partners filed a schedule 13-D indicating it now held about 6.1 percent of the company's stock after going on a stock buying binge starting in late July. At the end, the fund attached a love letter of sorts explaining its interests:


"RIM believes the shares of the Issuer to be significantly undervalued…In fact, when one backs out cash and investments, the market is valuing SST's NOR flash business, product pipeline and licensing revenue stream at only $60 million-which RIM believes to be an extremely low valuation by any measure."


We all would like to hear we're worth more than everyone thinks, right? But this love is not unconditional:


"RIM has communicated this view to the Issuer's management… RIM's desire, at this point in time, is to work assiduously and aggressively with the current management team on behalf of all shareholders."


And here's the catch:


"RIM's sincere hope is that management and the Board of Directors share its sense of urgency…If they do not, it will force RIM to take a more proactive approach, one which will include, among other things, the nomination of new directors…communicating with other stockholders, making proposals to the Issuer concerning the capitalization and operations of the Issuer."


more from Silicon Storage Technology,>>


SST (Silicon Storage Technology, Inc., NASDAQ: SSTI), a leader in flash memory technology, today announced a new addition to the company's popular SuperFlash-based FlashFlex family of 8-bit, 8051-compatible microcontrollers, the SST89V54RD-33-C-QIF. Leveraging the company's innovative packaging technology, the new SST89V54RD is available in a 6mm x 6mm WQFN package, making it the smallest 8051-based microcontroller currently on the market. The device's miniature size and low power consumption are ideal for small form factor mobile applications, such as notebook PCs, MP3 players and GPS systems, as well as home entertainment devices including HDMI products. Additionally, the SST89V54RD supports in-system programming (ISP) and in-application programming (IAP), which provide a variety of benefits to device manufacturers and consumers alike.

"As the sophistication of mobile devices increases, size reduction and low power consumption become even larger issues for product design teams," said Paul Lui, senior vice president of the Standard and Special Product Group at SST and president of SST China. "The new thin and powerful SST89V54RD was designed to help our customers meet the size, power and performance requirements of next-generation portable consumer electronic devices."

In addition to a tiny 6mm x 6mm footprint, the WQFN package offers an extremely low-profile nominal package height of only 0.7mm (maximum total thickness of 0.8mm), making the new SST89V54RD well suited for height-constrained mobile applications.

In-Field Re-Programmability Through IAP and ISP
Like all of SST's FlashFlex microcontrollers, the SST89V54RD supports both IAP and ISP, enabling the user to update the flash device in the field or in an application. Both IAP and ISP lower cost and improve time-to-market for manufacturers, while bringing enhanced user experiences and convenience to consumers. These re-programming features also have a significant role in enabling increased functionality, such as remote diagnostics and product monitoring, in network- or Internet-enabled devices.


Pricing and Availability
Samples of the SST89V54RD-33-C-QIF FlashFlex microcontroller are available now. Pricing starts at $1.20 in 10K unit quantities. For more information about this or other SST products, please contact an SST sales representative, or visit the company's Web site at http://www.sst.com.


About Silicon Storage Technology, Inc.
Headquartered in Sunnyvale, California, SST designs, manufactures and markets a diversified range of memory and non-memory products for high volume applications in the digital consumer, networking, wireless communications and Internet computing markets. Leveraging its proprietary, patented SuperFlash technology, SST is a leading provider of nonvolatile memory solutions with product families that include various densities of high functionality flash memory components and flash mass storage products. The Company also offers its SuperFlash technology for embedded applications through its broad network of world-class manufacturing partners and technology licensees, including TSMC, which offers it under its trademark Emb-FLASH. SST's non-memory products include NAND controller-based products, smart card ICs, flash microcontroller and radio frequency ICs and modules. Further information on SST can be found on the company's Web site at http://www.sst.com.


Forward-Looking Statements
Except for the historical information contained herein, this news release contains forward-looking statements regarding flash memory and non-memory market conditions, SST's future financial performance, the performance of new products and SST's ability to bring new products to market that involve risks and uncertainties. These risks may include timely development, acceptance and pricing of new products, the terms and conditions associated with licensees' royalty payments, the impact of competitive products and pricing, and general economic conditions as they affect SST's customers, as well as other risks detailed from time to time in the SST's SEC reports, including the Annual Report on Form 10-K for the year ended December 31, 2005 and on Form 10-Q for the quarters ended March 31, June 30 and September 30, 2006.


For more information about SST and the company's comprehensive list of product offerings, please call 1-888/SST-CHIP. Information can also be requested via email to literature@sst.com or through SST's Web site at http://www.sst.com. SST's head office is located at 1171 Sonora Court, Sunnyvale, Calif.; telephone: 408/735-9110; fax: 408/735-9036.




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