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|ELBURG SHIPMANAGEMENT PHILS., INC. is an international provider of crewing and ship management services.
In Elburg, we bring together our experience, our commitment to quality and continual quest for improvement with the readiness to cope with the diversified demands and needs of our clients in accordance with regulatory requirements to deliver the best possible service.
Based in Makati City, Philippines, we are currently providing Filipino officers and crew to major shipping companies worldwide. Our seafarers are properly trained and certified to meet the requirements of the International Maritime Organization (IMO), Standards of Training, Certification and Watchkeeping (STCW), and other international regulations.


text: At 2:00 PM -0400 4/22/97, Doug Jensen wrote: > I have some personal confusion regarding the adaptiveness of CAM >photosynthesis. It is usually portrayed as a pathway that decreases >photorespiration, and, as such, it is presented an alternative to C-4 >photosynthesis. To decrease photorespiration, there should be a mechanism to >decrease [oxygen] in the region of the chloroplasts. I don't see that. It >appears to me that the primary purpose of CAM is water conservation. > > Am I missing something here? Doug, I think you understand this pathway correctly! The plant faces declining CO2 levels through the day as the malate (or whatever) stored in the vacuole is depleted. At the same time oxygen levels are increasing as stomata are closed and light reactions release it into the trapped gas spaces. Reducing photorespiration might have been a selective force for the evolution of C-4, but I don't think the same is true of CAM. Worse, to operate the C-4 pump at night, the CAM plant must run respiration to supply the PEP. This is like spinning your wheels...it may look and maybe even sound impressive, but it is not very efficient...not much forward momentum. Day photosynthesis decreased by photorerspiration and night respiration used to drive photosynthesis... it isn't efficient at all. This makes CAM plants among the SLOWEST growing species on earth. On the other hand, the ability to close the stomata in daytime and still run photosynthesis while gaining carbon dioxide at night when it is cool via open stomata permits CAM plants to be VERY competitive in extremely dry habitats. As far as I can think, the stomatal reversal is the adaptive feature and C-4 photosynthesis provided the survival mechanism to permit it. Thus, water availability was the likely selective pressure for the evolution of CAM from C-4 in my opinion. ross _______________________________________________________________ Ross Koning | koning at ecsu.ctstateu.edu Biology Department | http://koning.ecsu.ctstateu.edu/ Eastern CT State University | phone: 860-465-5327 Willimantic, CT 06226 USA | fax: 860-465-4479 ____________________________|__________________________________

subset: commoncrawl


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Victoria's Purrrrfect Treasures
Victoria ~ Proprietress, New Germany, NS Canada
This is a lovely quality hand tooled vintage leather belt with repeat heart pattern. The buckle is stamped Solid Brass . In good vintage condition. Measures 1 inch wide by 35 inches long . The buckle is about 2 inches by 1 1/2 inches. 5 punched holes present for size adjustment.
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Pix Theater
319 Main Street,
No one has favorited this theater yet
Showing 4 comments
@Teecee…Jim Thatcher's post is incorrect. The building at the RIGHT of the view is the old Pix Newsreel, NOT the building at the left with the Pizza Center on the first floor. The Pix was already closed and vacant (but still surviving as a theater) as late as the 1960's. This is not the same as the Embassy, which was located several blocks west. The Palace was several blocks east on the opposite side of Main Street.
I have an address of 139 Main.
My 1950 edition of Film Daily Yearbook gives a street address of the Pix Newsreel Theatre as 319 Main Street. The Embassy Theatre at 347 Main St had 1,915 seats.
1951 FDY lists an Embassy Theater at 347 Main Street. Is this the same theater?


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Religion and politics collided once again this month as religious groups — led by Catholic bishops — objected to requirements to provide contraceptive-covering insurance in President Obama's health insurance rules. America's widely varying levels of religious commitment, even within denominations, makes the outcome of such firestorms hard to predict.
It's turned into quite the campaign issue, which has pollsters wondering whether religion can really tip the scales. Catholics represent about one in four adults in America, which makes the backlash from bishops to Obama's new regulations potentially consequential. The rules — which Obama later modified — would have required religiously affiliated institutions to provide health plans that cover birth control, a practice with which they have a moral disagreement. Alienating such a large group could severely endanger his chances at reelection in November.
But Catholics, like Protestants and other religious groups in the United States, are far from monolithic. Only one in three self-identified Catholics reported attending Mass every week in a January Washington Post-ABC News poll. And even that figure may be an overestimate — given Americans' tendency to say they are more churchgoing than they actually are.
Obama's popularity among Catholics hasn't taken a big hit, at least in the short term. His overall approval rating among Catholics in Gallup polls ticked down from 49 to 46 percent amid the controversy, a change within the margin of sampling error. While most Catholics in a Pew poll released this week said religiously affiliated employers should not be required to pay for contraceptives, just 15 percent said they believe using contraceptives is morally wrong.
So how much could this affect the 2012 campaign? Catholics represent just one aspect of America's complex religious and political calculus. Among Protestants, white evangelicals are a cornerstone of the Republican base, while white mainline (or non-evangelical) Protestants represent a key swing-voting group. Black Protestants are overwhelmingly Democratic.
For white evangelicals, religion seems to be making more of a difference in the Republican primary than it will when Obama is on the ballot. Romney has struggled to win evangelicals in early primary contests in Iowa and South Carolina, but national polls show evangelicals overwhelmingly back Romney in a matchup against Obama.
For many religious voters, specific religious issues may play less of a role than long-held partisan loyalties. And in the General Election, one key factor will be how voters with no religion cast their ballots. This group has grown and voted increasingly Democratic over the past two decades, and backed Obama over McCain by a 52-point margin in 2008, according to exit polls. More than six in 10 religiously unaffiliated voters approved of Obama in a Washington Post-ABC News poll released last week, marking a stark shift from November last year, when just as many disapproved as approved.
For some perspective, it's interesting to look at how America's religiosity compares with that of other countries. Most nations tend to gravitate toward either end of the spectrum — either highly religious or overwhelmingly secular. The United States falls in the middle. Roughly six in 10 Americans say religion is "very important" in their lives. That's about three times the number of Britons who gave religion such prominence in Pew surveys in recent years, and nearly double the number of Canadians who say the same. The story is similar for Germany (where 25 percent say religion is "very important"), Italy (24), Spain (23), France (13) and Sweden (8). Compared to Europe, the United States is God's own country.
But Americans profess less religious zeal than people living in the Middle East and sub-Saharan Africa. About eight in 10 Egyptians see religion as very important, a number that rises even higher in Rwanda (90) and Senegal, where religious commitment surges to 98 percent.
American politicians are well aware of voters' religious commitment. Nearly every member of Congress professes a religious faith, and Democrats have worked hard to shed the stereotype that they are less friendly toward religion than Republicans. For candidates looking to connect with voters in 2012, "God bless America" is a good refrain.
Foreign policy Wednesdays: Most Wednesdays we will feature a special poll watcher analysis of American public opinion on foreign policy. The series will be cross-posted at Foreign Policy Magazine's Election 2012 page.
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About Alamid
starting in 1993 from the ashes of athenas curse alamid are; gary ignacio = vocals dexter facelo- guitar jun pineda - bass gene mitra - keyboards jex herradura drums for info and bookings on the band contact us @ alamid.ph.tripod.com we play rock and new wave music Read more about Alamid on Last.fm.
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Alamid's Songs
Thomas Alvarez Vilchez and 1 more
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coma and 2 more


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GENEVA / VEVEY, SWITZERLAND – Nestlé and Lidl, two of the giants in the food industry, said Monday they are recalling products marked with beef in which traces of horsemeat have been found. The Swiss company is recalling pasta with meat products from Italy and Spain, while Lidl's recall covers Sweden, Finland, Denmark and Belgium.
"We are now suspending deliveries of all our finished products produced using beef supplied by a German firm, H.J. Schypke, a subcontractor of one of our suppliers, JBS Toledo N.V.
"Our tests have found traces of horse DNA in two products made from beef supplied by H.J. Schypke. The levels found are above the one percent threshold the UK's Food Safety Agency uses to indicate likely adulteration or gross negligence. We have informed the authorities accordingly.
"There is no food safety issue, but the mislabeling of products means they fail to meet the very high standards consumers expect from us."


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Court wants to quiz Campbell about plot
A LITHUANIAN court has said it wants to question Dundalk man Liam Campbell over his younger brother Michael, who was jailed for 12 years for a plot to smuggle arms from the Baltic state.
Justice Viktoras Kazys ruled that the testimony of Liam Campbell from Upper Faughart and another Irishman was key to an appeal launched by Michael Campbell against his prison term.
Judge Kazys said: "The court will take the necessary measures for them to be questioned. The court believes questioning is necessary."
Liam Campbell was found liable by a civil court for the 1998 Omagh bombing, which killed 29 people including a woman pregnant with twins.
In October 2011, a Lithuanian court convicted his younger brother Michael Campbell, aged 39, of attempted smuggling, aiding a terrorist organisation and illegal possession of arms.
However, Michael Campbell appealed. He claimed he was framed in a money-making scheme run by prosecution witness Robert Jardine - identified in court as a British MI5 agent posing as a smuggler.
Michael Campbell was arrested in January 2008 in Vilnius as he met a Lithuanian agent who posed as an arms dealer. He went on trial in August 2009.
Liam Campbell and another man, Brendan McGuigan, are suspects in a separate pre-trial investigation in the arms smuggling case by the Lithuanian authorities.
Michael Campbell's defence hailed the move to question Liam Campbell, but said it was belated.
Michael Campbell admits travelling to the Baltic state to buy weapons, but claims he did not intend to use them to arm dissident republicans.


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Under Armour Curry 3 Performance Review
After breaking the record for made 3 pointers in a season for the third year in a row, winning a second MVP by an unprecedented unanimous decision, getting to the NBA Finals (and blowing a 3-1 lead), and helping to sign the biggest free agent of the season, what else could Stephen Curry do to occupy his time? Release his third signature shoe, of course. Hot off of the success of his second shoe, the Under Armour Curry 2, the baby-faced assassin unveiled his newest kicks a few months ago, the Under Armour Curry 3. Sporting a drastically different design, new materials, and coming off of Curry and Under Armour's huge success with the Curry 1 and Curry 2, this was supposed to be a massive release. Rumors are that the Curry 3 hasn't sold very well, but does it perform well on the basketball court?
The Under Armour Curry 3 features a simple herringbone pattern with thin grooves, a pivot point in the forefoot, and a hard rubber compound. The traction is decent, on a clean court the stopping power is very good, probably a 9/10. However, this outsole attracts a ton of dust and since the grooves are close together, it is requires frequent and extensive wiping to get it out. When dust does inevitably get stuck to the outsole of the Curry 3, you experience some slipping and a definite loss of bite. Overall, the Sole Brothers give the traction on the Curry 3 a rating of 8/10.
Under Armour and Stephen Curry opted to use nearly the same cushioning setup that has been featured in every one of the Curry lineup, Charged foam. There are some minor tweaks this time around. The Charged midsole extends up in the heel area to form the heel counter (with a TPU counter inside), they used a thin insole, and they implemented a carbon fiber midfoot shank for tosional support that also extends above the midsole (more on this part later). The insole is not particulary special, its soft but since it is pretty thin, it doesn't do much to change the overall cushioning system. The Charged foam midsole, like in the Curry 2, provides excellent responsiveness, good court feel, minimal impact protection, and no bounce whatsoever. This setup is good for a player who is light on their feet, fast, and needs a responsive ride to execute shifty moves like a guard. Overall, the Curry 3's cushion earns a rating of 7/10.
The biggest change from last year's Curry shoe is the upper. The lateral side and toe area use a material called Threadborne, a woven material derived from paracord technology to be light and strong. The medial side and heel area are constructed with a body mapped, molded Anafaom piece for extra comfort and lockdown. As mentioned earlier, the carbon fiber wing that works as a midfoot shank in the midsole extends up the sides of the shoe between the heel and the arch of the foot to, as Under Armour puts it, "expressly support the joint that connects the ankle and heel bones for better balancing, pivoting, and shock absorption,". The upper is fit together in a half-bootie construction. The Threadborne material feels very thin and stiff and plastic-like at first, but once it is broken in it feels soft like a jacquard. The same goes with the Anafoam area, it is stiff at first but feels soft and supportive once it breaks in. The materials by themselves (implementation is a bit different) are amazing, earning a rating of 10/10.
Fit: The Curry 3 does not fit very well, there is a lot of dead space above your toes and feels a bit unstable as a result. It seems to fit a tad long (Sammy was testing a size 8 which is 1/2 of a size up for him which is probably why) so go true to size and the length issue should be good. The Curry 3 does fit wider than the Curry 2, which is disappointing since the Curry 2's fit is what made the Sole Brothers love it so much.
Support: This is a very supportive shoe. The materials do not stretch and the ankle support was so good that Sammy did not wear his ankle braces at all in the shoe. The height of the shoe (which is taller than last year's model) is surprisingly supportive without restricing movement at all.
Lockdown: The Curry 3 provides good lockdown, although it has the same quirk as the Curry 2 in the heel. In the heel area, your foot doesn't move or feel loose, but you just don't feel very locked in or secured. The forefoot lockdown was good, no issues to report. Overall, the Curry 3 earns a rating of 8/10 for fit/support/lockdown
Ventilation, Durability, and Aesthetics
Ventilation: The shoe felt very well ventilated, earning a rating of 9/10.
Durability: The Curry 3 should be a durable shoe, the outsole is hard and the materials were made to be super strong and durable. The Sole Brothers give the Curry 3 a rating of 9/10.
Aesthetics: Sammy said that this shoe has grown on him since he first saw it and says that they are dope, but Don and myself agree that this is a hideous shoe. The silhouette looks squarish and it simply looks like a boot rather than a basketball shoe. The black out colorway is the best looking one since it hides most of the hideousness of this shoe. Sammy gave this a rating of 9/10 on our scorecard, but I am making an executive decision to give it a rating of 4/10 for aesthetics.
The Under Armour Curry 3 in a size 8 weighs in at 12.87 ounces, which if Sammy gets a pair in his correct size shouldn't be very different than the Curry 2. The Curry 3 feels very light on the foot and quite minimal. Under Armour is selling this shoe at retail for $140 which is a $10 increase over last year's model and a $5 increase over the Curry 2.5. Sammy enjoyed the Curry 3 overall, but was disappointed in the traction and fit, if those had been better, this would have been a great shoe rather than simply a good shoe. Let us know what you think in the comments and be sure to check out our scorecard and Don and Sammy's discussion on the Curry 3 below.


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Commentary: Obama Does Not Believe Global Warming a Civil-War or World-War-II Scale Crisis
President Barack Obama evidently does not believe that fossil-fueled global warming is a nation-threatening crisis, despite repeated scientific warnings that a full-scale mobilization must be enacted now to avert global catastrophe. At the top of his list for accomplishments before the end of his term, instead of a redirection of the national and global economy towards rapid decarbonization, is the goal of beginning "the process of rebuilding the middle class and the ladders into the middle class."In response to The New Yorker's David Remnick's question of "what he felt he must get done before leaving office," Obama said:
I think we are fortunate at the moment that we do not face a crisis of the scale and scope that Lincoln or F.D.R. faced.
Abraham Lincoln and Franklin Delano Roosevelt were president at the start of the Civil War and World War II, respectively.
Obama's presidency has been marked by a backing away from a sense of urgency about the climate crisis. "Obviously there's great urgency in dealing with a threat to the entire planet," Obama said as a candidate in 2007. In an October 2007 speech, he called global warming "the planet's greatest threat," "the issue that will determine the very future of life on this Earth," "a fact that threatens our very existence," and "the most urgent challenge of this era."
"Global warming is not a someday problem, it is now," he said. He pledged "to phase out a carbon-based economy that's causing our changing climate." "As President, I will lead this commitment," he promised.
Six and half years later, global carbon pollution has continued to rise rapidly, fueled in no small part by Obama's "all of the above" support for increased oil drilling, fracking, and coal mining.
After years of near-to-total silence on the ravages of a polluted climate to the nation, Obama started his second term with a new promise for action.
"As a President, as a father, and as an American, I'm here to say we need to act," he said in June 2013.
It looks he doesn't actually feel the urgency of his own words.


text:
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Inc. announced today that it has launched its GRID360™
Distribution Manager-a new, network modeling and simulation software
application that enables utilities to build, analyze, simulate, and
optimize distribution networks.
The GRID360 Distribution Manager enables utilities to address the
challenge of unpredictable power flow in the power grid due to
distributed generation, renewable integration, micro-grids, and demand
response. The application represents a breakthrough in network modeling
and simulation technology to improve network visibility by identifying
network topology and SCADA measurement errors using advanced state
estimation techniques that deliver the most accurate network model. The
application runs on Nexant's advanced GRID360
platform with industry-proven network
modeling, generalized state estimation and power flow software, and
leveraging open Common Information Model (CIM) standards.
Nexant GRID360 enables power system engineers to build, monitor,
analyze, and perform "what if" scenarios in a collaborative environment.
It is built with a highly sophisticated N-tier open architecture to
easily address security, interoperability, extensibility, and
"To make the grid 'smarter' and capable of addressing the need to
decarbonize generation sources and enable end-user energy efficiency,
utilities will have to improve observability and controllability of
their networks, while transforming them into geodesic structures that
intersperse a variety of distributed energy resources-some owned and
operated by consumers," according to Zarko Sumic, Vice President and
Distinguished Analyst, Gartner (News - Alert), Inc. in his July 2012 report, Hype
Cycle for Smart Grid Technologies.
Nexant will be demonstrating GRID360 Distribution Manager at the
DistribuTECH conference in San Diego, on January 29-31 for utility
distribution operations and planning professionals. To arrange a
demonstration contact: email@example.com.
Nexant offers a comprehensive suite of best-in-class energy enterprise
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energy value chain.
[ Back To TMCnet.com's Homepage ]
ITEXPO: January 28 - 31, 2019 | Fort Lauderdale, Florida
IoT Evolution Expo : January 28 - 31, 2019 | Orlando, Florida


text:
Please keep all discussion of tonight's episode in this thread, at least until 1:00 a.m. E.S.T.
Thanks and enjoy the show!!!
Please keep all discussion of tonight's episode in this thread, at least until 1:00 a.m. E.S.T.
Thanks and enjoy the show!!!
Where's the thread? Where's the thread? *pulls hair out frantically*
Oh. Here it is.
Jenny saying Kim has no class
Okay people. Give us poor impatient West Coasters some info.
the first skirt looked HORRIBLE on that skant.
Changes outfit from HO to semi HO
Wow, Kim went SO conservative with that outfit!! NOT!!
"I can do all things through Him who strengthens me!"
Kimberly was asked on tonight's first date (to an art gallery) and she is confronted by Anitra and Jenny (I think) 'cause Kimberly is dressed in a sexy way.
Anitra and Jenny tell Kimberly that she's dressed "too hot" for the date.
Jenny says, "Here's trash, here's class -- she was somewhere in the middle."
Jenny describes Kimberly: Here's trash... here's class... here's Kimberly somewhere in the middle.
Charlie, of course, likes her slutty outfit.
Never let the things you want make you forget about the things you have.
Jenny still saying Kim has no class. I think that is what she was going for. They are going to an art gallery . These two do not have a clue about art


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Bala Ji Temple :-
Tirupati is located in Andhra Pradesh. Tirupati is an ancient Hindu temple town having historical references in Puranas. The temple of Lord Venkateswara is located on the Tirumala hill and Tirupati is at the foot steps of the Tirumala hills. Every day around 1 lakh people visit this place. It has great reputation for famous temples. The newly created "Greater Tirupati" covers a large area with a population of over 10 lakhs, covering geographical area from Srikalahasti in the north to Puttur in the south, which is about 1400 sq km. Tirupati has one international airport, and is head quarters to six universities. The National Atmospheric Research Laboratory (NARL) of the Indian Space Research Organisation (ISRO) is located at Gadanki near Tirupati. NARL is engaged in fundamental research related to atmospheric and space sciences and developing various types of radars and lidars for atmospheric studies. Temples located in and around Tirupati include: 1. Sri Padmavathi Devi temple at Tiruchanooru (Alamelu Mangapuram) 2. Kalyana Venkateswara Swamy Temple at Srinivasa Mangapuram. According to legend, Lord Venkateswara stayed here after his marriage with Sri Padmavathi Devi, before proceeding to Tirumala. 3. Govindaraja Swamy Temple in Tirupati adjacent to the railway station (Lord Vishnu in Anantasayanam pose). Saint Ramanujacharya consecrated this temple in 1130 AD. 4. Kapila Teertham in Tirupati town at the base of Tirumala Hills dedicated to Lord Siva 5. Sri Kodandaramaswami Temple, Tirupati built by Chola kings during the tenth century AD 6. Sri Kalahasteeswara Temple at Srikalahasti 7. Sri Kalyana Venkateswaraswami temple at Narayanavanam (40 km from Tirupati). Lord Sri Venkateswaraswami and Sri Padmavathi Ammavaru, daughter of Akasa Maharaja were married here.


text:
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6. GOVERNING LAW. These Terms shall be governed by and construed in accordance with the law of the Commonwealth of Pennsylvania, and the federal laws of the United States of America, as an agreement made therein, without reference to any conflicts of laws provisions or policies. The United Nations Convention on Contracts for the International Sale of Goods shall not apply to these Terms. Any dispute between the parties that cannot be amicably resolved shall be determined by one arbitrator in binding arbitration administered by the American Arbitration Association pursuant to its Commercial Arbitration Rules. All hearings will be conducted, and all evidence will be entered, by audio conference and video conference. The award of the arbitrator shall be final and binding on the parties, and may be entered and enforced in any court or tribunal of competent jurisdiction.
7. ENTIRE AGREEMENT. The parties hereto acknowledge that the Service Agreement (where applicable) and these Terms, including any Schedules, are the complete and exclusive statement of agreement respecting the subject matter hereto and supersede all prior understandings and other communications between the parties relating hereto. Except as expressly stated in these Terms, any additional or contradictory terms or conditions of any purchase order, accounting report or communication between the parties, or any other document, shall be of no effect unless signed in hard copy by both parties.
8. EFFECTIVE DATE. These Terms are effective as of December 1, 2016, and supersede any prior sets of Terms.
Privacy Policy
1. About this Privacy Policy.
This Privacy Policy is a statement by BuyerMLS, LLC, the operator of the Buyside service ("Buyside") that describes how we collect, store, process, and share personal information in connection with our website and online services. Most of the information we collect we do so on behalf of our customers (each, an "Organization"), but this Privacy Policy does not address the privacy practices of any other person or entity, including any provider of data to us, or any user of our Products. Accordingly, for each entity, site and service other than Buyside, you should contact them regarding their privacy practices.
2. Definitions. The following terms have the following meanings.
"Administrator" means the person authorized by an Organization to make decisions on behalf of that Organization.
"Buyside" or "we" or "us" or "our" means BuyerMLS, LLC.
"Cookie" means a small digital file containing a string of characters that is stored on your computer when you visit a website.
"Member" means each person who obtains access to Buyside's Products through an Organization.
"Non-Personal Information" is any information that we collect, store, process or share, that does not identify an individual person, even if the information is collected from a person.
"Organization" means the person, company or organization that has entered into a contract with Buyside for access to the Products.
"Personal Information" (also known as "personally-identifiable information") is any information that we collect, store, process or share, and which identifies an individual person.
"Privacy Policy" means this statement of data privacy practices, as it may be updated and revised from time to time.
"Products" means any goods or services provided by Buyside.
"Site" means the Buyside website at www.GetBuyside.com.
"You" and "your" mean each Organization, Administrator, and Member.
3. Overview: How We Protect your Privacy
Buyside is an information service that combines data you provide with data from third parties and publically-available data. We can then report information back to you that helps you rent and sell properties.
All non-confidential information entered at Buyside is used by Buyside and its affiliates for the purpose of facilitating Buyside's Site and Products, including the buyer management and listing process.
Email messages may be reviewed for compliance and security.
All buyer contact information is confidential and is never shared by us on the public site or to any subscribers of Buyside, rather it is only accessible by the agent listing that specific buyer ("Buyer Agent"), the Buyer Agent's business associates, and anyone with whom the Buyer Agent chooses to share the buyer contact information.
Credit card information is never stored by Buyside. After a transaction is processed by Buyside, all credit card information is deleted from Buyside's servers. Credit card information will be stored by credit card processing companies, banks and other financial institutions.
Buyside uses 128 bit data encryption and Secure Sockets Layer (SSL) to better protect online transactions.
Buyside data is protected by and complies with the Payment Card Industry (PCI) Data Security requirements of Visa, MasterCard, American Express & Discover, although we do not store credit card information.
We don't share your Personal Information with third parties for marketing purposes, but we do share Non-Personal Information with third parties for marketing purposes.
Account information is password-protected. Please keep your password safe.
We are not responsible for, nor have any control over, the privacy policies of any third party websites, and encourage all users to read the privacy policies of each and every website visited.
4. Data We Collect
For each Organization, Administrator and Member, we collect Personal Information, including name, user name and password, and contact information such as email address and telephone number. Each of these different types of information is used to provide the Buyside Site and Products. Personal Information is also used to authenticate users, for service-related communications, and as an integral component of the Products. In some cases, contact information will be sent to third party syndication partners who have the ability to anonymize email addresses.
We sometimes collect email address for purposes such as sending self-publishing and confirmation emails, authenticating user accounts, providing subscription email services, registering for forums, and other communications.
We sometimes collect your phone number for account authentication purposes, and may transmit it to a third party service for tele-robotic verification.
Buyside does not store credit card information. Credit card transactions are transmitted to a financial gateway, and we endeavor to protect the security of your payment information during transmission by using Secure Sockets Layer (SSL) technology.
We may collect Personal Information if you provide it to us, or if you contact us directly. Please do not post any Personal Information in any correspondences or emails that you expect to keep private.
Our web logs collect standard web log entries for each page served, including your IP address, page URL, and timestamp. Web logs help us to diagnose problems with our server, to administer the Buyside Site, and to otherwise provide our service to you.
We allow third-party companies to collect certain Non-Personal Information and other anonymous information when you visit our Site. These companies may use Non-Personal Information during your visits to this and other websites in order to provide advertisements about goods and services likely to be of greater interest to you. These companies typically use a cookie or a third party web beacon to collect this information. To learn more about this behavioral advertising practice, you can visit www.networkadvertising.org.
5. Data We Store
We store all buyer listings in our database. Even after "deletion" from our database, we continue to store buyer listings, and they may be archived elsewhere. Our web logs and other records are stored indefinitely.
Active Members can access and update their account information through the account homepage.
All user Organization, Administrator and Member contained within the Products remain the Organization's property. We will continue to make that data available to the Organization as long as the Organization is a customer, and make that data available to the Organization upon the termination of its relationship with Buyside.
If at some point Buyside sells all or a portion of its assets, or merges with another entity, all Personal Information and other data are assets that may be transferred or acquired by a third party. We will use commercially reasonable efforts to notify all affected Organizations, Administrators and Members of any such transaction, and each will have the opportunity to retrieve their Personal Information and cease usage of the Site and Products. After such a transaction, the third party that becomes the custodian of the Personal Information would have the right to continue using the Personal Information solely as set forth in this Privacy Policy or any policy that may replace it where the new policy is instituted in accordance with the provisions of this Privacy Policy.
6. Spam
We do not tolerate spam. To report spam or spoof emails to Buyside, please forward the email to firstname.lastname@example.com. You may not use our communication tools to send spam or otherwise send content that would violate our Terms of Service or Service Agreement. We automatically scan and may manually filter messages to check for spam, viruses, phishing attacks and other malicious activity or illegal or prohibited content, but we do not permanently store messages sent through these tools.
7. Share This
When you use the "Share This" link to bookmark and share our Products and Site, you will be taken to a third party site. Please note that the third party sites' privacy policies (and not this Privacy Policy) govern the collection and use of the information collected on those sites.
8. Changes to this Privacy Policy.
We may update this Privacy Policy from time to time. Any changes that we make to this Privacy Policy will be effective thirty days after the sooner of providing a copy of the revised Privacy Policy or posting the revised version of this Privacy Policy. The date shown in this Privacy Policy indicates the date that we last revised this Privacy Policy. BY CONTINUING TO ACCESS OR USE THE BUYSIDE SITE OR PRODUCTS AFTER SUCH DATE, YOU WAIVE ANY OBJECTION TO THE REVISED VERSION OF THIS PRIVACY POLICY. If you cease using Buyside before the effective date of a particular revised version of this Privacy Policy, then you remain subject to the terms of the most recent version of this Privacy Policy in effect while you were using the Products. If we make any material changes to this Privacy Policy, we may provide a more prominent notice of our choosing. We encourage you to periodically review this Privacy Policy to be informed of how we are collecting, using, sharing and otherwise handling your Personal Information.
9. Your Opt-Out Rights
As an Organization, Administrator, or Member, you have the right to opt out of receiving marketing communications (whether through mail, telephone or email) from us or any of our affiliates or vendors regarding other products, services and promotions available from us. To opt out of all marketing emails, please click the link contained in any such emails sent by us or our affiliates or vendors. If you have difficulties opting out of such emails, or if you would like to opt out of receiving marketing communications through the mail or telephone, please contact us (see Contact Us section below). In your request (whether by mail, telephone or email), please specify the type of communication (mail, telephone or email) that you would like to stop receiving from us. We will take commercially reasonable measures to comply with your request within a commercially reasonable time.
10. Security of Your Personal Information.
The security of your Personal Information is important to us. We and the vendors that help us host and administer each Site and Product, and maintain the servers through which we provide each Site and the Products, take reasonable measures to secure your Personal Information from unauthorized alteration, access, use and disclosure. We follow generally-accepted industry standards to protect the Personal Information submitted to us, both during transmission and once we receive it. When you enter Personal Information on the Site, we encrypt that information using secure socket layer technology (SSL).
We use a third party credit card processing company. We will only share with them (via SSL) your Personal Information that is needed to process your credit card payments, and they are prohibited from using your Personal Information for any other purpose.
No method of transmission over the Internet, or method of electronic storage, is completely secure. While we strive to use commercially-acceptable means to protect your Personal Information, we cannot guarantee its security.
If you are registered on the Site, your Personal Information is accessible through entry of your Member name (email address) and password on the Site. We recommend that you refrain from divulging your login identification or password to anyone. We will not ask you for your login identification or password during an unsolicited phone call or in an unsolicited email. Please keep in mind that whenever you disclose information online that information can be collected and used by others. Ultimately, you are responsible for maintaining the confidentiality of your login identification, password and other Personal Information.
11. Editing and Removing Your Information; Information Retention.
Subject to the written agreement between Buyside and the applicable Organization, and the provisions of this section, you may review and request modification and deletion of your Personal Information. If you are registered with us, you may do so by logging into your account on the Site or Product, and following the instructions provided on the screen.
We make requested changes and deletions to your Personal Information within a commercially reasonable time, but it may be impossible to remove your Personal Information completely, since it may remain in our backup files or logs. Please note that, if you request deletion of your Personal Information, you may be unable to utilize certain features of the Site and the Products.
Notwithstanding the above, we may preserve information about you, including your Personal Information, in response to a legal demand or request if we believe that the law requires us to do so. We may also preserve information about you, including your Personal Information, when we believe it is necessary to detect, prevent and address fraud and other illegal activity; to protect ourselves, you and others, including as part of investigations; and to prevent death or imminent bodily harm. Information we receive about you, including your Personal Information, may be retained for an extended period of time when it is the subject of a legal request or obligation, governmental investigation, or investigations concerning possible violations of our terms or policies, or otherwise to prevent harm.
12. Non-Personal Information.
When you access or use a Site or Product, we may collect Non-Personal Information from you, including (but not limited to) your Internet Protocol (IP) address, browser type, domain names, access times and referring website addresses. To gather Non-Personal Information, we may use common tracking tools such as cookies. We use cookies to help you personalize your online experience, to enable us to provide quality Products through each Site and to provide general statistics regarding use of each Site and Product.
The purpose of a cookie is to tell a web server that you have returned to a specific page. For example, if you register with a Site or a Product, a cookie copied to your local device helps us to recall your specific information on subsequent visits. When you return to the Site, the information you previously provided can be retrieved to enhance the Products that we provide to you. You may also get cookies and other tracking technologies from third parties with links on a Site or Product, as described in the Third Party Websites & Links section below. We do not control cookies and other tracking technologies employed by third parties.
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You have the ability to accept or decline cookies from each Site or Product. Most web browsers automatically accept cookies, but you can usually modify your browser setting to decline cookies if you prefer. If you choose to decline cookies, you may not be able to fully experience the interactive features of a Site or a Product.
14. Disclosure.
We may disclose aggregated Non-Personal Information that has been collected from you and others to our existing or potential vendors or other third parties, or in response to a government request or demand. We may also share Non-Personal Information, including aggregated and de-identified demographic data, with third parties to enable the provision of targeted information, promotions, offers and discounts on our Products.
15. Third Party Websites & Links.
We cannot control, and are not responsible for, any third party's use of cookies, web beacons or other tracking technology that collect information about you or others. Advertising agencies, advertising networks, and other companies who place advertisements on websites, email messages and on the Internet may use this or other technology to collect information about you. We encourage you to review the privacy policies of websites you choose to link to from website links that we provide through the Site or the Products, so that you can understand how those websites collect, use and share your information. We are not responsible for privacy or security policies or practices of any third parties or their other websites.
16. Children's Privacy.
The Site is not directed at children under 13 years of age, and we do not seek or knowingly collect any personal information about children under 13 years of age. If we become aware that we have unknowingly collected any personal information from a child under the age of 13, we will make commercially reasonable efforts to delete such personal information from our systems. If you are a parent or legal guardian and think your child under 13 has personal information to us, please contact us (see Contact Us section) and we will delete it.
17. Visitors Residing Outside the United States.
The Sites and the Products are hosted and managed in the United States of America, and are subject to United States laws, which may be different than laws in other countries. If you reside outside the United States, then the privacy laws and regulations in your country may be more protective of your Personal Information than those of the United States. We make no representation or warranty that this Privacy Policy and/or our privacy or security practices comply with the laws of any country outside of the United States.
18. Contact Us.
We welcome your comments regarding this Privacy Policy and our privacy practices. If you have any questions or complaints about our privacy practices or this Privacy Policy, please contact us via email at firstname.lastname@example.com or first class mail sent to the following address:
BuyerMLS, LLC
PO Box 1821
Southeastern, PA 19399
We will use commercially reasonable efforts to answer any questions, promptly evaluate any complaints, determine if any violations have occurred and remedy any problems as appropriate.


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Discussion in 'Critique Forum Archives' started by mentos_007, Feb 28, 2005.
what do you think?
Something is missing with the mountins but still very cool pick.
haha I'm almost sure you wanted to see the top of the mountain me too
Oh, I love it. It's gorgeous! (We don't see things like that in Texas)
yeah!!! Finally I've got something that's not in America!!! yeah!!! Europe rulez!!
Separate names with a comma.


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The Maui Hill
Welcome To The Maui Hill
Maui Hill condominium resort sits on a lushly landscaped slope overlooking the clear blue of the Pacific, just minutes from the premier resort area of Wailea. It's a perfect alternative to the more expensive Wailea super-resorts.
With extra-spacious one- and two- bedroom units, you'll have plenty of room to kick back and relax. Our luxurious two-story, three-bedroom units are the perfect vacation choice for families and larger parties. All suites come with fully equipped kitchens, washer/dryers, and large furnished balconies or lanai, where you can relax and enjoy the cool breeze from the beach. All suites feature tropical garden or ocean views.
Some see Maui Hill as a private oasis, but don't let that fool you. While it's certainly relaxing, you'll also have easy access to the Kamaole Beach Parks, world class golf courses, the Wailea resort area, and numerous fine shops and restaurants. From the beach, you'll even be able to see the islands of Lanai and Kahoolawe in the distance.
Take advantage of the resort's many amenities, including daily complimentary continental breakfast, swimming pool, jet spa, tennis court, putting green, shuffleboard, and outdoor barbecues. When it's time to go home, Kihei is just 10 miles from the Kahului Airport.
More Information On The Maui Hill
- Year-round children's program, Camp Kaanapali (available at all Maui RQH properties)
- Near Beach
- FREE High speed internet access
- Weekly continental breakfast
- Weekly manager's mai tai party
- Personalized service and attention
- Free parking
All Maui Hill Reservations processed through Blue Hawaii Vacations © 2009 Blue Hawaii Vacations


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Hello everybody on OSM Community! :relaxed:
New forums , new adventures , new era for the OSM planet and of course lots of new entries with managers and visitors of the OSM forums from all around the world. So my friends I thought it would be nice to have a specific topic for anyone that wishes to introduce himself/herself . Please, feel free to share a few words with the rest of us in here or simply say a ... Hello ! :wink:


text: Harry Putnam <firstname.lastname@example.com> wrote: > I hope someone might be able to help me with installing debian as > guest by way of vmware. > I downloaded the iso DVD (4.4 GB what a hefty download) If you've got network access you're probably far better off with one of the netinst images, and using the network to bring in recent editions of the packages you're actually going to use. > Also, I wasn't really sure if I'm getting the right one. The hardware > is (intel) i7 Q820 multiple cores with windows 7 64 bit. The host hardware's largely irrelevant. What is important is the virtual hardware offered within the VM. I successfully run a 686 based kernel, here. Chris


text: By now most of you have read that Garrosh survives his defeat at the hands of the players in the Siege of Orgrimmar raid. I won't dive into an in-depth analysis here, but I will say that this is a good thing! A good story needs its villains, and one of the biggest problems that WoW has had is that it kills its villains off too readily. Of course, when villains appear in multiple places (see: Kaelthas, though that was handled kinda poorly story-wise so that people didn't see it coming) people complain about things being reused. Check out this WoWInsider article for a lengthier analysis of this effect, but simply put I am happy that Garrosh has survived. Are you?


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A King County Sheriff's deputy was taken to Valley General Hospital with minor neck and back injuries tonight after a vehicle he was pursuing accelerated into his patrol car, sheriff's spokeswoman Cindi West said.
The 34-year-old female suspect, in a small red car, was driving when she saw a deputy behind her and accelerated, West said.
The deputy tried to stop the woman, who was driving in a reckless manner, West said.
The woman made her way to Highway 167 and exited to 15th Street Northwest, where she hit a car that was going east, West said.
The crash turned the car 180 degrees, facing the ramp it had just used to exit. The driver then drove head on into another deputy helping with pursuit, who suffered the minor injuries, West said.
The suspect was booked into jail for investigation of felony eluding and vehicular assault, West said.


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Otterspool Way
Easter Opening Times
|Friday 30th March 2018
|10am - 4pm
|Saturday 31st March 2018
|9am - 5pm
|8am - 4.30pm
|8am - 1pm
|Sunday 1st April 2018
|Monday 2nd April 2018
|10am - 4pm
Contact Watford Audi for some of the very best customer service and Audi expertise in the Hertfordshire area, from one of the biggest Audi dealerships in the UK. Whatever your Audi need, whether it be a new car, a scheduled service or a set of floor mats, we will do our utmost to help you in any way we can. You can contact Watford Audi by email, with the links provided below, or by calling any of the Watford Audi phone numbers. You would also be very welcome to come in to see us. We're open six days a week; just take a look at our Watford Audi opening hours.
Our 16-car showroom is the perfect place to view the outstanding range of new Audi cars, whilst our exceptional approved used Audis are available to view any time. If you're already an Audi owner and want someone to look after your car, Watford Audi offers the full range of servicing products, such as Audi servicing and Audi MOT, from our state-of-the-art 20-bay workshop and our Audi bodyshop and repair centre. We can also supply the full range of Audi genuine parts and accessories.
From the Audi A1 to Audi A8, with Audi Sport models, the Q family and stylish Black Editions in between, almost every model we sell is available with some excellent Audi business lease deals and private Audi finance offers, and we're Motability accredited. We also always have some great deals on ex-demonstrator Audis. Just contact our helpful sales team to find out more about what we have on offer, or to arrange a test drive.
This won't take long...
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When you give us your contact details, Group 1 Automotive companies, our authorised dealer network or our agents may use your data to email or phone you about Group 1 Automotive products, services and offers which we believe may be of interest to you. We may also contact you to conduct market research, so we can improve our service to you. We never sell or share your information with third party organisations.


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Talks & Events
KICP Colloquia: 2008
Star Formation in Galaxies
Christopher McKee, UC Berkeley
Star formation is at the nexus of astrophysics: stars are believed to be responsible for the re-ionization of the universe, they created all the heavy elements, they control the formation and evolution of galaxies, and the formation of stars naturally leads to the formation of planets. It is therefore critical to understand the rate at which stars form. Observations of the star formation rate are encapsulated in the Kennicutt-Schmidt relations between the star formation rate and the amount of gas in a galaxy. Observations have also shown that star formation is inefficient. This inefficiency, and the Kennicutt-Schmidt relations, are naturally explained in the theory of turbulence-regulated star formation (Krumholz & McKee 2005). Star formation in turn is a major driver of turbulence in giant molecular clouds, the sites of star formation. The observed star formation rate is generally inferred from observations of the ionized gas produced by massive stars. However, massive stars can form only in regions of high surface density (~ 1 g/cm^2 or greater). This threshold for massive star formation leads to a truncation of the initial mass function at high masses in the outer parts of galaxies, and can account for the difference in the star formation rates inferred from observations of UV continuum emission by GALEX and of Halpha emission from ionized gas.
Magnetized Coronae of Stars and Accretion Disks
Dmitri A. Uzdensky, Princeton University
In this talk I will paint a general physical picture of magnetically-active astrophysical coronae, relevant to both stars and accretion disks. I first present a statistical theory of a turbulent accretion disk's magnetically-dominated corona, represented by an ensemble of loops. Each loop constantly evolves under the Keplerian shear, radnom footpoint motions on the disk surface, and reconnection with other loops. I construct and then solve numerically a kinetic equation for the loop distribution function. I use the resulting steady state solution to calculate the vertical distribution and the total amount of the magnetic energy in the corona, the overall coronal torque, etc. I demonstrate that these quantities grow strongly with increased strength of Keplerian shear relative to reconnection. This underscores the importance of reconnection in accretion disk coronae. In the second part of my talk I argue that recent advances in magnetic reconnection enable significant progress in understanding of magnetized coronae as self-regulating, marginally collisioness systems. I propose a novel view on the coronal heating problem, based on an interplay of two effects: (1) transition between the slow collisional and the fast collisionless reconnection regimes and (2) plasma evaporation from the star's or disk's surface due to coronal energy release. I show how these ideas work both for the solar corona and for the inner part of a black hole accretion disk corona.
The Importance of Lens Environments
Ann Zabludoff, Unversity of Arizona/Steward Observatory
Analyses of strong lensing galaxies have provided constraints on quantities as important and varied as the Hubble constant and substructure in the dark matter halos of galaxies. However, the environments in which most lens galaxies lie are not well-known and may contribute significantly to the lensing potential. Not including the environment in lens models can introduce uncertainties and biases of 5-20%, preventing lensing constraints from competing with those derived from CMB or distance ladder measurements. I will describe results from our theoretical modeling of environment effects and from our five-year observational survey of the fields of 70 lenses. We find that the majority of lenses lie in overdense environments -- poor groups or rich clusters of galaxies -- that perturb lens models. We are using these data not only to identify "golden lenses" whose properties provide useful cosmological constraints, but also to measure the evolution of groups and clusters over the large redshift range probed by our sample. I will discuss some of our recent results measuring the baryon content of nearby groups and clusters, which suggest that our lens survey will ultimately allow us to explore baryon evolution in such common environments.
X-ray binaries: puzzle bonanza
Natalia Ivanova, The University of Toronto, CITA
The abundance of X-ray binaries in our and other galaxies and their brightness at many wavelengths make them key to our understanding of different physical processes (accretion and gravitational waves radiation) and of advanced questions in stellar evolution (the origin and evolution of binary systems, the final stages of massive stars, the formation of compact objects). Within the next decade, observations at existing and planned facilities in almost all wavelengths will put a heavy demand on further studies of compact binaries. In my talk, I will discuss what is our current knowledge of X-ray binaries formation and evolution, where we had a progress and where we have failed, what are new breakthrough ideas. Specific attention will be given to globular clusters, where dynamical interactions between objects lead to the enhanced formation of X-ray binaries. Their study surprisingly helped to understand the field population of X-ray binaries and millisecond pulsars better. Other topics to be discussed are whether we can put constraints on the stellar evolution by comparing the observed populations and theoretical results, which uncertainties in the theory seem to play the most important role and what questions must be answered in the future.
The Highest Redshift Quasars and the End of Reionization
Xiaohui Fan, University of Arizona
Luminous quasars at high redshift provide direct probes of the evolution of supermassive black holes (BHs) and the intergalactic medium (IGM) at early cosmic time. Over the last six years, more than 20 quasars have been discovered at z>6 from various wide-field surveys. Two main results emerge from the studies of these quasars. Detections of such objects indicate the existence of billion M_sun BHs merely a few hundred Myrs after the first star formation in the Universe.
Theyare surrounded by metal-enriched gas and young galaxies with intense star formation, providing the strongest constraints on early growth of supermassive BHs and co-evolution with their host galaxies.
Meanwhile, Absorption spectra of the highest redshift quasars reveal complete Gunn-Peterson absorption, indicating a rapid increase in the IGM neutral fraction, marking the end of the reionization epoch at z~6, suggesting a peak of reionization activity and emergence of the earliest galaxies and AGNs at 6
The echo of Einstein's greatest blunder
Martin White, UC Berkeley
The coupling of baryons and photons by Thomson scattering in the early universe leads to a rich structure in the power spectra of the cosmic microwave background photons and the matter. The study of the former has revolutionized cosmology and allowed precise measurement of a host of important cosmological parameters. The
study of the latter is still in its infancy, but holds the potential to constrain the nature of the dark energy believed to be causing the accelerated expansion of the universe. I will discuss how we can measure this cosmic sound, and the theoretical developments that need to be made before we can realize the promise of future missions.
Measuring CMB Polarization
James J Bock, California Institute of Technology
The Inflationary paradigm has been remarkably successful in passing observational tests, largely from Cosmic Microwave Background temperature anisotropy measurements. Gravitational waves produced during the epoch of Inflation may imprint a detectable polarization signal in the CMB. This polarization signal, which has a distinctive 'B-mode' pseudo-vector field that cannot be duplicated by matter over/under-densities, depends on the physics of Inflation and thus can be used to distinguish among Inflationary models.
We have developed the BICEP (Background Imaging of Cosmic Extragalactic Polarization) experiment to measure degree-scale CMB polarization in a search for evidence of an inflationary gravitational wave background. I discuss the unique design of the receiver and its performance after two seasons of observations from the South Pole. Recent advances in antenna-coupled TES bolometers will enable significant improvement in system sensitivity. We are developing two new instruments based on these new detectors, SPIDER to measure large-scale polarization from a long-duration balloon, and BICEP2 to deeply integrate in a small region of the sky with low Galactic foregrounds from the ground. These measurements will ultimately culminate in a space-borne measurement with large detector arrays, NASA's Einstein Inflation Probe.
Star Formation in Turbulent Molecular Clouds
Andreas Michael Burkert, University of Munich
Star formation, despite its importance, is not well understood up to now. This situation is however changing quickly. High-resolution observations now provide detailed insight into the complex structure of the turbulent interstellar medium and its various gas phases. The star formation history of molecular cloud regions like Taurus and Orion has now been investigated in great details. At the same time, numerical simulations have achieved enough resolution and complexity in order to explore the origin of turbulent molecular clouds and their fragmentation into stars and stellar clusters in great details.
At the moment the physics of star formation is still in an early phase of exploration. A major step forward has recently been made by identifying several key questions which need to be solved to make progress. I will discuss some of the most puzzling and challenging questions. I then will present recent ideas and and new numerical simulations that have the potential to solve some of these puzzles and by this provide crucial steps towards a consistent theory of star formation.
Searching for Dark-Matter Axions
Leslie Rosenberg, University of Washington
The axion is a hypothetical elementary particle whose existence would explain the baffling absence of CP violation in the strong interactions. It's properties make it a good dark-matter candidate. Even though dark-matter axions would make up the overwhelming majority of mass in the universe, they are extraordinarily difficult to detect. We have developed a detector of dark-matter axions that is at heart an exquisitely sensitive detector of microwave radiation. This colloquium will briefly review the role of axions in particle and astrophysics, and will describe the progress we've made in the experimental search.
New CMB Polarization Results from QUaD
Clement Pryke, The University of Chicago
Measurements of the intensity fluctuations of the Cosmic Microwave Background have already taught us an enormous amount about the nature of the Universe in which we live. Polarization measurements have the potential to tell us even more. After briefly reviewing the motivation for polarization measurements I will move on to the QUaD experiment at South Pole, which is currently the world's most sensitive CMB polarimeter in the multipole range 200 to 2000. I will describe the instrument, observation strategy, analysis and newly released results. Finally I will mention a new project called SPUD and the push to detect the gravitational wave B modes.
CN-cycle Solar Neutrinos and the Solar System Metalicity
Wick C Haxton, INT, University of Washington
The CN-cycle plays a modest role in solar energy generation, but produces a significant flux of neutrinos that will be measured in SNO+ and other future detectors. Because past measurements have precisely calibrated other conditions in the solar core -- and because of progress made in constraining neutrino flavor physics -- I argue this new measurement will determine the primordial solar core abundances of C and N to 10%. This will eliminate a key assumption in the standard solar model, and address the current conflict between helioseismology and photospheric abundance determinations. I discuss the possibility that this conflict is real and associated with late-stage metal differentiation in the solar-system disk associated with planetary formation -- and point to observational implications.
Indeterminacy of Holographic Quantum Geometry
Craig Hogan, The University of Chicago
Theoretical motivations will be reviewed for the idea that spacetime is holographic: there is a minimum time or length in nature, and the third dimension of space emerges in quantum theory from time evolution, in the normal direction to a light sheet. A new phenomenon will be described that arises in such holographic geometry: "holographic noise", caused by an indeterminacy of transverse position. It will be shown that currently operating interferometric gravitational-wave detectors have the capability to detect holographic noise. These experiments provide a zero-parameter test of the holographic hypothesis. In a holographic world, they provide a direct, precise measurement of the fundamental minimum interval of time.
The Chirality of Life: From Phase Transitions to Astrobiology
Marcelo Gleiser, Dartmouth College
Life is chiral. Amino acids that make up biomolecules are left-handed, while all sugars are right-handed. And yet, when synthesized in the laboratory, the solutions come out 50-50. Is life's chirality simply an accident, or is it the result of dynamical processes that occurred in early Earth, during prebiotic times? If life exists elsewhere in the Universe, will it choose the same chirality? In this talk, I will address these and other questions of interest in astrobiology, using techniques from nonequilibrium statistical mechanics and field theory. In particular, I will argue that life's chirality might be due to a symmetry-breaking phase transition. Exploring this possibility, I will obtain bounds on possible processes that may have selected life's chirality here and possibly in other life-bearing planetary platforms. Coupling the polymerization reactions to a simple model of the early-Earth environment, we conclude that Earth's chirality was selected randomly. A large sample of planetary platforms with stereochemistry will have a 50-50 chiral distribution.
Cosmological Inhomogeneities and Dark Energy
Eanna Flanagan, Cornell University
The issue of whether the backreaction of inhomogeneities can mimic the effects of dark energy has been a subject of much debate. I review the evidence on both sides of this issue and discuss what needs to be done to resolve it. I also discuss the extent to which inhomogeneities perturb high precision measurements of dark energy.
Early results from the Fermi gamma-ray space telescope
Julie McEnery, NASA/GSFC
The Fermi Gamma-ray Space Telescope, recently launched in June 2008, is a satellite based observatory to study the high energy gamma-ray sky.
There are two instruments on Fermi: the Large Area Telescope (LAT) which provides coverage from 20 MeV to over 300 GeV, and the Gamma-ray Burst Monitor (GBM) which provides observations of transients from 8 keV to 30 MeV. Since its launch, Fermi has detected over one hundred gamma-ray bursts (three above 100 MeV), dozens of flaring AGN, a couple of Galactic transients, radio-loud and radio-quiet pulsars, and is enabling a detailed study of the many other persistent sources in the high energy gamma-ray sky. In this talk, I will review the early results from Fermi, and discuss the current status and future plans for the observatory.
Clustering, Quenching, and Feedback: Galaxies and AGN at z=1
Alison Coil, University of California, San Diego
Roughly half of the red elliptical galaxies observed today have formed since z=1. I will present galaxy clustering results from the DEEP2 Redshift Survey that strongly constrain the mechanism responsible for the quenching or cessation of star formation in these galaxies. I will show where this quenching is occurring on large scales and how it can not be due primarily to cluster-specific physics. I will also present results on the clustering of optically-bright quasars and X-ray selected AGN and show how AGN accretion correlates with the star formation activity in galaxies at z=1. I will also show new results on the prevalence of outflowing galactic winds at z=1 and discuss their role in quenching star formation. Finally, I will present a new wide-area prism survey that will allow further studies of galaxy evolution to z=1 with the largest faint galaxy survey to date.


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Both our McHi Mariachi Oro and Rowe HS Mariachi Azteca advanced to the State Finals after putting on exceptional performances and receiving straight "Division 1 Superior" ratings from all three judges at Area competition just a few weeks ago. They will be competing at the State Finals tomorrow, February 4, 2017 at the South San Antonio HS Performing Arts Complex! We are extremely proud of all of our talented student musicians for their hard work, dedication, passion, and love for the music! They will be representing their individual schools as well as McAllen ISD out in San Antonio, TX!
McHi Mariachi Oro takes the stage at 7:00pm & Rowe HS Mariachi Azteca goes on at 8:40pm!


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Skip to comments.Newark Mayor Cory Booker: $80.4B Food Stamp Program Not a Government Handout
Posted on 12/10/2012 11:00:28 AM PST by Olog-hai
Newark, N.J. Mayor Cory Booker says the federal governments Supplemental Nutrition Assistance Program (food stamps), which spent $80.4 billion in fiscal 2012, is not a government handout.
I hope and understand that people are getting a better recognition that this is a program that really helps America, helps families in need, Booker said on Friday, while describing his fourth day of living on a SNAP budget.
"Its not a government handout, he said. If anything, its a safety net that helps people through difficult times and bridges them towards stability.
(Excerpt) Read more at cnsnews.com ...
It's a handout-——idiot.
If I had to make a pie-in-the-sky guess, I would say less than 15% of the people on food stamps actually need them. The other 85% are lazy moochers who want their free food, big screen TV with cable, and leased luxury cars.
Don't forget their free phones!
How discriminatory of em. After all, "bears" refers to a certain segment of the gay community and all . . .
I wonder if he just got back from Seattle.
Up is down. Bad is good. Black is white. In is out...ad infinitum. These DIMocRATs are tooooooo much! Am I missing something...are the recipients of this HANDOUT paying for this stuff??????? Is this mayor's head misshapen?????
I don't care. I'm supporting this guy for Gov. We need to stop Fat RINO stupid Christie from being the 2016 nominee.
You forgot the Party-approved "war is peace, freedom is slavery, ignorance is strength" . . .
Maybe even back to 2010.
I really do need to go to the reeducation camp for a while...don't I?
Why don't you, Mayor, ask WHY these people have to have this government "safety net" IOW, welfare instead of working to support themselves?
Where are the great jobs that Newark had in the 40s, 50's and 60's?
Why can't people SUPPORT THEMSELVES?
Where are the jobs Obama promised?
This ignorant turd is beyond belief.
I'm often reminded of what happened in Manhattan, NYC, which used to be one of the country's biggest manufacturing centers in the 50s (if you can believe that). Along came Mayor Robert F. Wagner, who instituted all sorts of government programs, and the consequence was so many manufacturing jobs fleeing the city that he had to expand government services (a self-perpetuating disease). Of course, NYC was one of the first cities that instituted total government control of the mass transit systems, forcing the private subway companies to hold down fares to unprofitable levels until they eventually had to sell out to the city (the city-owned IND came along as unfair "competition" as well); expansion came to a standstill after that. Such policies rapidly expanded to neighboring cities such as Newark, of course, with even worse ramifications.
Maybe it helps Americans, maybe it helps families in need, maybe it's a safety net that yadda yadda yadda ... but none of those changes the fact that it's a government handout.
This reminds me of the people who say Social Security isn't an "entitlement" because they're entitled to it.
No, it's Reparations, right Cory?
Disclaimer: Opinions posted on Free Republic are those of the individual posters and do not necessarily represent the opinion of Free Republic or its management. All materials posted herein are protected by copyright law and the exemption for fair use of copyrighted works.


text: A university lecturer's elderly father pays a prostitute to leave her profession and live with him, then accidentally kills her, kicking off a series of events with the only common link being those implicated attempting to do one good dead. The university lecturer attempts to find the prostitute's estranged daughter, who is at the same time being chased by authorities in different countries because of her political activities. Set in Germany and Turkey, and told in several languages, this is a truly international film that focuses on a search for meaning and purpose in an otherwise mundane existence. The scenery plays a central role in the many quiet scenes, often conveying intense emotions. While difficult to watch, this is a film that is not easily forgotten, making it both powerful and beautiful.


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|p. 1
|The nature of illegal immigration in the United States
|p. 5
|Purpose, history and function of the United States Border Patrol
|p. 19
|The issue of migrant deaths
|p. 31
|Preventing migrant deaths : ethics, policy and the utility of situational crime prevention
|p. 39
|Impact of border safety initiative policy
|p. 55
|Understanding the circumstance and situational nature of migrant deaths
|p. 95
|Implications for policy, practice and future research
|p. 143
|Table of Contents provided by Blackwell. All Rights Reserved.


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100% Ilayaraja Tamil MP3 songs site. Collection of Ilayaraja hits and melodies songs are available for free download. Download old, new and latest Tamil mp3 music for free. A.R. Rahman songs, other Tamil music directors songs, Tamil actress movie gallery and Tamil videos are coming up in the future!
Monday, March 15, 2010
Pillai Nila (1985)
Album: Pillai Nila
Cast: Mohan
Music: Illayaraja
Year: 1985
Director: Manobala
Ilayaraja Hits
1. Azhake
Malaysia Vasudevan, S. Janaki
2. Raja Magal (Child)
S. Janaki
3. Raja Magal (Female)
K.S. Chitra, S. Janaki
4. Rajamagal (Male)
P. Jayachandran, K.J.Yesudas
1 comment:
- BharaniOctober 16, 2011 at 8:04 AM
Hey.. Thanks a lot for this songs.. i was searching for a long time for "Raja Magal" song Male version. Thanks once again!!ReplyDelete
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text:
Print editions may be delayed
The Daily Democrat is continuing to experience problems getting our editions out due to a major breakdown at the newspaper's press plant.
Deliveries of print editions today and Tuesday may be delayed.
We continue to ask your understanding and patience, and thank you in advance for same.


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I would say almost everyone has box full of video tapes that contain precious family memories. Video tape is known as an analog format and over time will slowly degrade and loose their picture quality and color. For several years now the service has been offered to transfer your old video tapes to DVD. When creating the DVD you have the option of having motion menus so you can access key scenes throughout the video and have an interactive menu. In order to capture your analog tapes, the company will play your tapes through the required format deck and digitize them into the computer.
This transfer process is done in real time. Once digitized, there are a few options, you can have the company edited your videos then make your DVD master or just have them output straight to DVD. When the DVD master is being created you do have the choice of making a menu that can list different areas of the video. This is a great way to skip through different parts of the DVD without having to watch the entire video. When your DVD master is complete I would recommend having a back up DVD made for safety purposes. DVD is a great way to preserve your memories, but if anything were to happen to your master DVD and you did not have a copy, you would need to start all over again. You could use a company that specializes in video to dvd transfers too.


text:
Embryolisse cream 365 firming body lotion 200ml£23.00
this treatment is specially formulated for complete hydration of the body while smoothing it and providing firmness.
The concentration of assets used in this treatment allows a triple action to feed, tone and firm, smooth and thin skin.
After using the skin is toned, elastic, plump, firm, soft and smooth.
It penetrates quickly and easily including grace its gel texture.
Applied all over the body previously cleaned and dried 1 to 2 times per day.
For effective action, it is important to ebien emphasise areas more released as the belly, thighs or arms.
365 laboratories Embryolisse body firming cream should be used within 6 months following its opening.
Hyaluronic acid, natural vegetable oils of sandalwood, Lige and barley, wheat proteins, extracts of guarana caffeine, Shea butter, beeswax-rich.Complex symdiol 68 paraben free preservative.
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text:
Empeiria Acquisition Corp. Announces Extension Of Tender Offer
Nov 27, 2012, 15:00 ET from Empeiria Acquisition Corp.
NEW YORK, Nov. 27, 2012 /PRNewswire/ -- Empeiria Acquisition Corp. (OTC BB: EPAQ; EPAQW; EPAQU) ("EAC") (or the "Company") today announced that its previously announced tender offer, as amended (the "Tender Offer"), has been extended until 12:00 Noon, New York City time, on December 13, 2012. Except for such extension, all of the terms and conditions set forth in the Tender Offer materials remain unchanged.
Stockholders who desire to own shares of the Company's common stock subsequent to the proposed acquisition of Integrated Drilling Equipment Company Holdings Inc. ("IDE") should not tender their shares of common stock in the Tender Offer. Stockholders who have previously tendered their shares of common stock do not need to take any other actions unless they desire to withdraw their shares, which they may do in accordance with the procedures described in the letter of transmittal and other related Tender Offer documents that EAC has filed with the SEC. As of November 26, 2012, based on information provided by the depositary for the tender offer, a total of 4,038,524 shares of the Company's common stock have been tendered and not withdrawn.
Each of Empeiria Investors LLC, EAC's sponsor, and EAC's officers and directors has agreed not to tender any shares of common stock pursuant to the tender offer.
Morrow & Co., LLC is acting as the information agent, and the depositary is Continental Stock Transfer & Trust Company. For questions and information, call the information agent toll free at (800) 667-0088 (banks and brokers call collect at (203) 658-9400).
This press release is neither an offer to purchase nor a solicitation of an offer to sell shares of EAC common stock. The solicitation of offers to buy shares of EAC common stock will only be made pursuant to the Offer to Purchase, dated October 19, 2012 (as may be amended or supplemented), the related Letter of Transmittal, and other related documents that EAC is sending to its securityholders. The tender offer materials contain important information that should be read carefully before any decision is made with respect to the tender offer. Those materials are being distributed by EAC to EAC's securityholders at no expense to them. In addition, all of those materials (and all other offer documents filed with the Securities and Exchange Commission ("SEC")) will be available at no charge on the SEC's website at www.sec.gov and from the information agent. Security holders of EAC are urged to read the tender offer documents and the other relevant materials before making any investment decision with respect to the tender offer because they will contain important information about the tender offer, the merger and the parties to the merger.
About EAC
EAC is a blank check company formed on January 24, 2011 for the purpose of acquiring one or more operating business or assets through a merger, capital stock exchange, asset acquisition, stock purchase, reorganization, exchangeable share transaction or other similar business transaction. On June 21, 2011, EAC consummated its public offering of 6,000,000 units, with each unit consisting of one share of common stock and one warrant to purchase one share of its common stock. Aggregate net proceeds of $61,200,000 from the public offering and its concurrent private placement were placed in trust pending completion of EAC's initial business transaction. If consummated, the merger with IDE would constitute EAC's initial business transaction.
Forward-Looking Statements
In addition to historical information, this release may contain a number of "forward-looking statements" as defined in the Private Securities Litigation Reform Act of 1995. Words such as "anticipate," "expect," "project," "intend," "plan," "believe," and words and terms of similar substance used in connection with any discussion of future plans, actions, or events identify forward-looking statements. Forward-looking statements relating to the proposed transaction include, but are not limited to: statements about the benefits of the proposed transaction involving EAC and IDE; EAC's and IDE's plans, objectives, expectations and intentions; the expected timing of completion of the transaction; and other statements relating to the transaction that are not historical facts. Forward-looking statements involve estimates, expectations and projections and, as a result, are subject to risks and uncertainties. There can be no assurance that actual results will not materially differ from expectations. Important factors could cause actual results to differ materially from those indicated by such forward-looking statements. These risks, as well as other risks associated with the transaction, are more fully discussed in the Schedule TO filed with the SEC in connection with the merger and tender offer. Additional risks and uncertainties are identified and discussed in EAC's reports filed with the SEC and available at the SEC's website at www.sec.gov. Forward-looking statements included in this release speak only as of the date of this release. Neither EAC nor IDE undertakes any obligation to update its forward-looking statements to reflect events or circumstances after the date of this release.
Alan B. Menkes
Chief Executive Officer
Empeiria Acquisition Corp
KCSA Strategic Communications
Rob Fink / Brad Nelson
212.896.1206 / 212.896.1217
email@example.com / email@example.com
SOURCE Empeiria Acquisition Corp.


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Chronicling is the ticket for keeping your child interested the writing process throughout the summer.
Create Pen and Ink Art from Photos
Use metallic pens to turn a photo into framable art
How To Knit Your Own Bracelets
Recently I helped out at the third graders knitting and crochet club
Watch A Bird Make It's Nest With Dyed Wool
My dyed wool project is an ideal activity for the whole family.
Create a Photo Collage Easter Egg
This Springtime craft project has always a big hit with my kindergarten students.


text: [ snip] >If people had spent the time that they spent posting messages arguing >against spending effort on CVSup actually configuring it, then it >would be done by now, and (once the public CVS access is working) we >would be able to boast more available means for accessing our source >code. You know, I think this is symptomatic of the disagreement. The issue at stake is whether ``working for some favoured ports'', (due to a crappy, for NetBSD's purposes, implementation) counts as a ``working' NetBSD service. Especially since there are no plans and no commitments to make the service generally avaiable. You obviously think it does. I don't. I think the onus to make it generaly available belongs with those who want it. I don't know what your take is there, but Greg's is, unabashedly, to declare that some ports are less equal than others. And I see *that* as contrary to the goals of the project.


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Wednesday's Racing Podcast - York Dante Festival Day One
The Dante Festival at York gets underway on Wednesday and the feature race on day one, the Musidora Stakes, sees So Mi Dar bid to enhance her Oaks credentials.
Assistant Trainer and William Hill Radio pundit, Sean Quinn, joins Mark Walton to look ahead to the action, previewing the first four races on the card.
Sean talks us through his thoughts in each and nominates his selections along the way.
Join Darren Owen, Gary Capewell and Ross Brierley on Racing Radio from 1.40pm.
Follow all the action - and get in touch with the team - on Twitter @willhillracing.


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Charting the coming ice age.
Friday, October 28, 2016
Videos of the River Work
On my walk by the Humber River, I like to keep track of the various projects. The first is a regular update on the erosion control project. The second is some new sewer work which is interesting.
I think when they open the sewer, I won't be walking there for a while. :)
Posted by
Harold Asmis
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text:
|Quickplot is a fast interactive 2D plotter with infinite zooming, value picking, pipe and regular file input, with unlimited simultaneous plots displayed per graph. Quickplot is meant for looking at your data quickly and of secondary importance is making static pictures of your data. It's a data viewer, not a plot editor. It reads ASCII text and sound files. It has lots of command line options, making it very shell script friendly. It currently runs on GNU/Linux systems and we hear it works on Mac OS X Darwin.
Quickplot is GNU GPL free software.
Quickplot is hosted by
To check-out the current source from the GitHub repository run:
git clone https://github.com/lanceman2/quickplot
This will create a directory named quickplot in the current directory.
Jan 03 2016 Moved the quickplot repository to GitHub.
Dec 11 2011 A complete re-write was done and there is a new release that requires the use of GTK+ version 3, without GTKmm. We consider this rewrite, version 0.10.*, much better than version 0.8.15 in many ways. See the new features list at about.html#features.
Nov 27 2013 Made a new release with some new options and minor bug fixes.
|About | Help|
|Quickplot Version 1.0.1rc