text:
2015 North Carolina General Statutes
Chapter 41A - State Fair Housing Act.
§ 41A-4 - Unlawful discriminatory housing practices.
41A-4. Unlawful discriminatory housing practices.
(a) It is an unlawful discriminatory housing practice for any person in a real estate transaction, because of race, color, religion, sex, national origin, handicapping condition, or familial status to:
(1) Refuse to engage in a real estate transaction;
(2) Discriminate against a person in the terms, conditions, or privileges of a real estate transaction or in the furnishing of facilities or services in connection therewith;
(2a), (2c) Repealed by Session Laws 2009-388, s. 1, effective October 1, 2009.
(3) Refuse to receive or fail to transmit a bona fide offer to engage in a real estate transaction;
(4) Refuse to negotiate for a real estate transaction;
(5) Represent to a person that real property is not available for inspection, sale, rental, or lease when in fact it is so available, or fail to bring a property listing to his attention, or refuse to permit him to inspect real property;
(6) Make, print, circulate, post, or mail or cause to be so published a statement, advertisement, or sign, or use a form or application for a real estate transaction, or make a record or inquiry in connection with a prospective real estate transaction, which indicates directly or indirectly, an intent to make a limitation, specification, or discrimination with respect thereto;
(7) Offer, solicit, accept, use, or retain a listing of real property with the understanding that any person may be discriminated against in a real estate transaction or in the furnishing of facilities or services in connection therewith; or
(8) Otherwise make unavailable or deny housing.
(b) Repealed by Session Laws 1989, c. 507, s. 2.
(b1) It is an unlawful discriminatory housing practice for any person or other entity whose business includes engaging in residential real estate related transactions to discriminate against any person in making available such a transaction, or in the terms and conditions of such a transaction, because of race, color, religion, sex, national origin, handicapping condition, or familial status. As used in this subsection, "residential real estate related transaction" means:
(1) The making or purchasing of loans or providing financial assistance (i) for purchasing, constructing, improving, repairing, or maintaining a dwelling, or (ii) where the security is residential real estate; or
(2) The selling, brokering, or appraising of residential real estate.
The provisions of this subsection shall not prohibit any financial institution from using a loan application which inquires into a person's financial and dependent obligations or from basing its actions on the income or financial abilities of any person.
(c) It is an unlawful discriminatory housing practice for a person to induce or attempt to induce another to enter into a real estate transaction from which such person may profit:
(1) By representing that a change has occurred, or may or will occur in the composition of the residents of the block, neighborhood, or area in which the real property is located with respect to race, color, religion, sex, national origin, handicapping condition, or familial status of the owners or occupants; or
(2) By representing that a change has resulted, or may or will result in the lowering of property values, an increase in criminal or antisocial behavior, or a decline in the quality of schools in the block, neighborhood, or area in which the real property is located.
(d) It is an unlawful discriminatory housing practice to deny any person who is otherwise qualified by State law access to or membership or participation in any real estate brokers' organization, multiple listing service, or other service, organization, or facility relating to the business of engaging in real estate transactions, or to discriminate in the terms or conditions of such access, membership, or participation because of race, color, religion, sex, national origin, handicapping condition, or familial status.
(e) It is an unlawful discriminatory housing practice to coerce, intimidate, threaten, or interfere with any person in the exercise or enjoyment of, on account of having exercised or enjoyed, or on account of having aided or encouraged any other person in the exercise or enjoyment of any right granted or protected by this Chapter.
(f) It is an unlawful discriminatory housing practice to:
(1) Refuse to permit, at the expense of a handicapped person, reasonable modifications of existing premises occupied or to be occupied by the person if the modifications are necessary to the handicapped person's full enjoyment of the premises; except that, in the case of a rental unit, the landlord may, where it is reasonable to do so, condition permission for modifications on agreement by the renter to restore the interior of the premises to the condition that existed before the modifications, reasonable wear and tear excepted.
(2) Refuse to make reasonable accommodations in rules, policies, practices, or services, when these accommodations may be necessary to a handicapped person's equal use and enjoyment of a dwelling.
(3) Fail to design and construct covered multifamily dwellings available for first occupancy after March 13, 1991, so that:
a. The dwellings have at least one building entrance on an accessible route, unless it is impractical to do so because of terrain or unusual site characteristics; or
b. With respect to dwellings with a building entrance on an accessible route:
1. The public and common use portions are readily accessible to and usable by handicapped persons;
2. There is an accessible route into and through all dwellings and units;
3. All doors designed to allow passage into, within, and through these dwellings and individual units are wide enough for wheelchairs;
4. Light switches, electrical switches, electrical outlets, thermostats, and other environmental controls are in accessible locations;
5. Bathroom walls are reinforced to allow later installation of grab bars; and
6. Kitchens and bathrooms have space for an individual in a wheelchair to maneuver.
(g) It is an unlawful discriminatory housing practice to discriminate in land-use decisions or in the permitting of development based on race, color, religion, sex, national origin, handicapping condition, familial status, or, except as otherwise provided by law, the fact that a development or proposed development contains affordable housing units for families or individuals with incomes below eighty percent (80%) of area median income. It is not a violation of this Chapter if land-use decisions or permitting of development is based on considerations of limiting high concentrations of affordable housing. (1983, c. 522, s. 1; 1989, c. 507, s. 2; 1989 (Reg. Sess., 1990), c. 979, s. 3; 2009-388, s. 1; 2009-533, s. 1.)
Disclaimer: These codes may not be the most recent version. North Carolina may have more current or accurate information. We make no warranties or guarantees about the accuracy, completeness, or adequacy of the information contained on this site or the information linked to on the state site. Please check official sources.


text:
[Resolved] Quikr — Quicker job is fake and fraud
DDosani Gani
I am applying in quicker jobs for get a electrical engineering job and also I received one SMS from quicker is like this
VK - QKRJOB[protected]
congratulation.. Your profile Has Been selected for NESTLE LTD sal 17500 to 35000.call HR PALLAVI [protected]Job by HR Solution...
And then I call to miss. Pallavi. She say me you come in new Delhi, you take one interview and after you select... I followed all processer but I not get Electrical engineering job at still now.. that prove quicker jobs is fraud and fake...
Please help me ... I am in big Stress
Please help me.
Complaint marked as Resolved 2017-03-15 01:34:01
Complaint Status
[Feb 10, 2017] Quikr customer support has been notified about the posted complaint.
Verified SupportQuikr Customer Care's response Feb 12, 2017
Hi Dosani,
We're sorry for your experience. We shall check this with our support team and they'll get back to you.
Thank you.
- Team Quikr
|30 Comments Updated:

subset: commoncrawl


text:
Learn more about Scribd Membership
Discover everything Scribd has to offer, including books and audiobooks from major publishers.
For the second year, Deutsch LA's Invention team journeyed to CES and SXSWi to wade through hundreds of new products and services. What follows is an exploration into the emerging trends and lessons, culled from that adventure, that brand marketers can apply to their own businesses.
About This Report
Invention began at Deutsch LA with the mission to solve complex business problems through means that fall outside the comfortable mold of advertising deliverables. Our team is charged with developing disruptive offerings, relationships, and business models for our clients. With that in mind, we attended two of the leading conferences relevant to our industry - CES and SXSWi - to examine startups and products that build on or extend emerging behaviors and technologies.
Startups and burgeoning products represent emerging bets at the intersection of technology and culture. Any product that a company produces is inherently a prediction for the future. CES and SXSWi represent a rare opportunity to view hundreds of those predictions in a single location, all vying for attention and adoption. From these bets, we've collected an overall view of rising trends and what brands and marketers can learn from those trends.
The Big Trend: The Rise of the Hardware Startup
CES, which is typically a conference for major hardware brands, was showcasing more and more startups in the hardware space this year. Conversely, SXSW Interactive, which has in the past been the launching pad for applications and software, this year showcased a number of startups (and brands) emerging in the hardware space. So why this marked attention and activity among hardware startups? We have three theories:
1. More Accessible 3D Printing: 3D printers were on
everyone's list of top disruptions this year and we've begun to see a plethora of consumer-grade entrants.
2. The Internet of Things: The internet is no longer contained to just a smartphone or a computer. We're entering an era where pretty much any object can turn into a Wi-Fi- enabled, data-sharing, communicating device.
3. Crowdfunding: The cost of prototyping has decreased but the cost of mass production is still high. Thankfully, platforms like Kickstarter and IndieGoGo allow entrepreneurs to share ideas with the world and get funding all without meeting a single VC.
CC-BY-NC-ND 3.0 - Deutsch LA 2013
Authored by: Bud Caddell, Charlotte Myerberg, and Rachel Mercer
Page 2 of 10
AliveCor Beam Technologies Bia Brainbot Breathometer Coco Controller Double Robotics Dropcam Fabule Fabrications Flomio Focus Formlabs Good Night Lamp Grippity Helio Hiku InteraXon Leap Motion LIFX Lightup Makerbot Makible Makie Labs Memoto Misfit Wearables Molecule Synth Ninja Blocks Nomiku Olloclip Ouya Pebble PetHub Pinnochio POWERLeap Rest Devices Sensus / Canopy Spark StickNFind Tagstand Twine U Grok It
2013 Hardware Startup Trends
Emerging hardware startups and the trend categories they fall into.
3D Printing
DIY Technology
Health and Wellness
The Internet of Things
Mobile Accessory
Quantified Self
Toys and Games
Wearable Technology
Page 3 of 10
From 2012 to 2013, theres been a significant increase in hardware startups at major tech conferences.
Key Trends (cont'd)
The CubeX is a new consumer-friendly competitor to the Makerbot.
CubeX 3D: Makerbot isn't the only product of its kind on the market. One competitor is the CubeX 3D, which won CNET's Best of CES award. This high-end printer, aimed at both enthusiasts and professionals, can print 15% larger objects than any other printer currently on the market. [Retails at $2,499]
Startups built on 3D Printing
Makie: A startup from the UK, Makie, creates custom dolls for young girls and a winner of the SXSW Accelerator competition. Makie allows doll they want online and have it produced just for them. Years ago, a venture like this would be almost impossible because of time and resources, but 3D printing makes it easy to make personalized creations quickly, and at a lower cost than typical manufacturing processes.
Peeko: From Rest Devices, the Peeko Monitor is the next-level baby monitor, a onesie for babies that tracks their breathing, activity, temperature, and noises. Parents can access this data on their mobile phone with an accompanying app. Peeko showcased their product at CES with 3D-printed (thanks to Makerbot) prototypes for customers to experience.
Internet of Things
In 2007, the world was wowed when the iPhone power of a computer in our pocket. Moore's Law has since been chugging away and now storage smaller and smaller things. As a result, we're starting to see a whole new era of connected devices, giving our houseplants the ability to tweet and our glasses the ability to project location-based information onto our retinas.
This new wave of hardware-based products launching at major conferences is leading to a shift in marketing tactics as well. Flashy booths in conference halls and free T-shirts are one thing, but hardware startups are looking for more creative ways of getting the actual product into lets you refocus images after you take them, rented out their devices to SXSW attendees for 24 hours so they could play with the product in real-world scenarios.
Google Products
Google Talking Shoes: Last year at SXSW, everyone was talking about the Nike Fuelband, a hardware product from Nike that tracks your everyday movement and helps you visualize your progress online. This year, Google took of talking sneakers that tracked activity and motivated you to keep moving with audible words of encouragement.
Page 5 of 10
Google Glass: Toward the end of the conference, Google hosted a demonstration of Google Glass, essentially a wearable, voice- controlled smartphone that lives in the lens of eye glasses. Seeing the presenter and members of the audience wearing the device felt like a glimpse into a very distant future.
The Memoto can be clipped on to record all the moments in your day.
Memoto: Accelerator, Memoto, is a tiny, wearable camera that takes a picture every second. It takes lifestream to a whole new level. The camera also serves as a GPS so it can organize photos by location. By connecting the camera to your computer, you can browse, search, and share (quite literally) your life.
Pebble: While we're all hearing about the rumors that Samsung and Apple will soon release "smart watch" devices, it turns out that some scrappy startups beat them to it. The Best in Show award at CES went to Pebble, an e-ink watch that can sync with your phone, and is easily customizable based on the users demand. The watch can be used for anything from monitoring a golf swing to controlling a music playlist.
Healthcare Products
Sure Response: A new service from Verizon, Sure Response is essentially a system that lets you keep track of an elderly parent, or any loved one who might need assistance. Users can push a help button and automatically deliver location information in the event of an emergency to a set caretaker, to a 911 response.
HealthID: Another product from Verizon, powered wristband that contains important personal information that you can have on you wherever you go. Your medical record, allergy, and pre-existing condition information can be wirelessly transferred to an emergency responder from the device.
Canopy's Sensus Case lets users add touch functionality on the back and sides of their smartphone devices
Smart Device Cases
Sensus: A new product from Canopy, the Sensus Case adds touchscreen functionality to the back and right-hand side of your Apple mobile device. This lets users interact with any experience on screen without blocking the view of the screen in a more comfortable and relaxed position.
Page 6 of 10
"world's thinnest watch." After raising over $500K on Kickstarter, it went on to win many of the Best in Show awards across CES.
The CST-01's E-Ink Display
Product Add-Ons
Olloclip: Focusing on the increasingly-popular photography space, Olloclip is a 3-in-1 lens that wide-angle, and macro options. Olloclip had a big presence at SXSW, but it wasn't exactly making its debut. It started raising money in 2011 on Kickstarter and gained enough ground to make a big splash at the tech conference this year.
StickNFind: StickNFind are Bluetooth stickers that you can put on devices so that you never lose them. The stickers come with a partnered iPhone app which serves as a sort of RADAR for these commonly misplaced items. A smart simple idea that solves a real consumer unmet need.
Connecting Digital to Physical
The Meter Plug:
Supermechanical's Twine
Page 8 of 10
What brands can learn from these trends (cont'd)
Experiment in New Spaces
Sometimes the best way for a brand to evolve is to nudge themselves into new territories that expand their business and their offerings. case, building data and phone networks) and applying it to the health space. Whether or not their products (Sure Response and HealthID) become an integral part of their business, it shows that these types of ventures can open new possibilities.
Smoke Testing as a Marketing Tool
Ideas are cheap. Execution is expensive. Just as startups use a clever video on Kickstarter to expose a new idea, we're beginning to see brands like Oreo and Budweiser launch proof-of-concept videos that test the social waters and validate a new idea. Organizations rarely get to market with their original idea in-tact, and it's time for brands and marketers to begin to test their assumptions before investing small fortunes in development.
Hardware Competition
Twenty years ago, monolithic companies like Xerox and IBM suddenly had to fear garage-based software startups like Apple and Microsoft. Today, with the advent of cheap 3D printing technologies and micro- funding, every business model is suddenly ripe for disruption from the garage-based hardware startup. The next few years will determine whether the infrastructure and distribution of large companies will overcome the grassroots funding and novelty of small-scale hardware developers.
The Innovation of Dead Tech
With rumors swirling that Apple and Samsung are both developing smart watches, we asked ourselves, "Who still wears a watch?" Plenty of people, it turns out. With the rise of the Internet of Things, every single device is suddenly a candidate for innovation. You may stare could be tweeting and sharing its way to a completely new price point.
"Disrupt yourself before someone does it for you." - Google
We believe that in order to survive,
organizations must myopically chase their own obsolescence. All businesses face an increasingly connected and therefore more uncertain world, and with it, we
all compete in a smaller pool,
full of more demanding and less
attentive consumers. Advertising
be a powerful driver of growth,
advertising alone cannot
steer a firm to future success.
That's why we've created a department of Inventionists – a
mix of researchers, creatives,
technologists, and entrepreneurs – to help our clients experiment with new tools, products, and business models.
Our group specializes in
concepting and developing pilot programs and products that disrupt the status quo, ignite culture, and create business
change. We also help brands find their social mission and work with
the larger advertising force at
Deutsch LA to pursue that mission through interactive ideas. If you're a business with an appetite for experimentation and marketing innovation, we'd love to partner with you.
in touch.
SVP, Invention
Page 10 of 10


text:
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text:
Re-Imagine Public Safety
We have a once in a lifetime opportunity to re-imagine how our society operates. I worked with Council President Martinez, Councimemember Wesson, and Councilmember Price on legislation that will create an unarmed model of crisis response that would divert non-violent calls for service (mental health crisis, substance abuse, neighbor disputes, etc.) away from LAPD to the appropriate non-law enforcement agencies. This legislation will completely change the role of law enforcement, buy it will take time to implement such sweeping reforms.
In the meantime, I introduced over 10 pieces of legislation to improve diversity, accountability and transparency within the LAPD. This progress is a result of residents making their voices heard and demanding better from our city. We have already implemented community-based public safety solutions in South Los Angeles that have proven to be effective. I will continue to fight for policies and actions that give our residents access to city services and reimagine safety protocols in our communities.
We need to invest in better approaches to crisis response and move forward with implementing the best practices of 21st-century public safety models. The legislation I introduced will do the following:
- Divert non-violent calls for service to non-law enforcement agencies
- Establish a culture of transparency and accountability within the LAPD
- Diversify LAPD to reflect more African American Officers
- Establish policies for responding to mass demonstrations
- Ban policies requiring predetermined citations, arrests, or investigative contacts
- Require officers to seek consent for search warrants
- Engage and expand multidisciplinary approaches to crisis response
- Develop an external reporting mechanism to combat African American attrition based on internal bias, racism and discrimination
Click here to read the details of all of the legislation introduced to improve public safety.


text:
Our AutoCav team is available to help with design and specification, quotes and estimates as well as technical product support. contact the team directly here.
AutoCav Residential Maintenance Checklist.pdf
Download zip file
Fit the auto head to the frame
Fit the door, connect the drive bar and tighten the belt
Connect the activation devices
SMC Connection
Remove the Controller
Refit the Controller
Run the Safety Beam Wires


text:
A Czech men's group is planning to encourage reflection on the dangers of alcohol again this year with the seventh edition of Dry February. The director of the League of Open Men, Josef Petr, said the rules were simple – not one drop of alcohol for the whole of the month.
The group's dedicated website offers tips on exercises and alternative non-alcoholic drinks, as well as advice from psychologists. Czechs rank among the top five nations in the world in terms of annual per capita consumption of pure alcohol.


text:
Client Reviews Search All Homes For Sale
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text:
AMA CPT® Assistant - 2017 Issue 4 (April)
Surgery: Integumentary System (Q&A) (April 2017)
April 2017 page 9a Surgery: Integumentary System Question: What are the appropriate codes to report for a bilateral subcutaneous brow lift with full facelift corset platysmaplasty? Answer: It is appropriate to report code 15824, Rhytidectomy; forehead, for the brow lift procedure, and code 15825, Rhytidectomy; neck with platysmal tightening (platysmal flap, P-flap), for the facelift corset platysmaplasty procedure. For the bilateral brow lift, append modifier 50 to code 15824. Question: A surgeon performs complex closures of the large dead space left following mastectomy, which double the operating time in most cases as these are meticulous and complex closures. Is...
To read the full article, sign in and subscribe to the AMA CPT® Assistant.
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text:
There's much more that goes into packaging than you think. The appearance and feel can influence the buyer's experience a lot from shelf visibility to the design and label and opening it at home.
Packages are more than just a box or a bag. It's the storefront of your brand and the driving force of buying behavior. Here are five reasons why packaging is more important than the product in it.
Customers See the Packaging Before the Product
Whether you realize it or not, how you package and present your product is a part of your overall marketing strategy. As soon as shoppers step into a store, you and other brands are competing for shelf visibility and brand recognition.
First impressions are important because they're everlasting and help customers form an immediate decision. Whatever the packaging portrays (i.e. boring, cheap, or flimsy), those qualities will automatically be attributed to the product it holds.
Let your package do the talking. Use it as leverage over your competition by making it an interesting talking point. After all, your packaging is the deciding factor in whether your product is purchased.
Provides Protection During Shipping and Storage
As a standard, packages serve to protect the product from the manufacturing facility to the retail shelf. To ensure products remain intact, your packaging must be durable and secure.
It would be best if you also use seals and locks. It prevents tampering and ensures the safety and integrity of the product.
Unboxing Is an Experience on Its Own
A lot of custom packaging made by Deepking Labels and other companies focuses on how it would look when you open it. Hauls and unboxing videos are so popular because customers are drawn to the anticipation and satisfaction of opening packages.
Keep in mind that unboxing is part of your brand and product presentation. Packages that are difficult to open can communicate how sturdy and well kept the product is, but on the other hand, it's not ideal for people who need assistance. If you use ribbons or other soft materials, it conveys a sense of fineness and fragility.
Brand Recognition
Brand recognition or brand awareness is the customer's ability to identify a specific brand over others. Certain colors, shapes, and other attributes can conjure familiarity with popular logos such as Apple, Coca Cola, and Walmart.
The same applies to packages. It has to be attractive, but it should also be easy to identify from a crowd or a distance. Don't be afraid to do something different. While a polished and professional look is the little black dress of the marketing world, use a little imagination to make your brand, packaging, and product memorable.
Sustainability and Reusability
Research by Trivium Packaging shows that nearly three-fourths of customers will pay more for sustainable packaging. That's because buyers are making more conscientious choices on where their money goes.
Sustainable packaging doesn't have to be limited to biodegradable or recyclable materials. Your packaging can be anything from refillable, reusable, or serve more than one function. Not only does the format, design, and materials showcase what your product is about, but it also exposes your stance on environmental concerns.
Final Thoughts
As a company, you enhance your brand presence and marketing strategy when you invest in smart, high-quality packaging suitable for your product. Keep in mind that your packaging has to be easy to transport, durable, and make a great impression from the warehouse to the shelves of your local retailers.


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wrestling / News
CHIKARA and The Wrestle Factory Cut Ties With Rory Gulak For 'Misconduct'
Both CHIKARA and The Wrestle Factory have announced that they are cutting ties with Rory Gulak due to 'misconduct.' It's unknown what the specific allegations are, but it seems it was enough for both promotions to end the relationship. Gulak was one of the trainers at the Wrestle Factory and has been with CHIKARA since 2017. His profile was removed from Wrestle Factory's website. While it can still be found at CHIKARA's website, he's not listed on the roster page and his photo was removed.
The statement reads: "Last week, both CHIKARA, Inc. and The Wrestle Factory, LLC severed ties with Rory Gulak
We take allegations of misconduct very seriously.
In accordance with this, we cooperate completely and transparently with all law enforcement agencies. Our priority is and always will be the safety of our fans, cast and crew.
Official, joint statement from CHIKARA and The @WrestleFactory_ pic.twitter.com/rVFJIWLISd
— CHIKARA (@CHIKARApro) January 6, 2020
Official, joint statement from The Wrestle Factory and @CHIKARApro pic.twitter.com/R4a0QEimNG
— The Wrestle Factory (@WrestleFactory_) January 6, 2020
More Trending Stories
- People in WWE Reportedly Unhappy With How Velveteen Dream's TV Return Was Handled
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- Chris Jericho on AEW's Creative Process, The Only Thing The NFL Took Issue With In Stadium Stampede
- Velveteen Dream's Second Accuser Makes Statement Following Dream's Return to NXT


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Education for the 21st Century: Time for Open Schools to Raise their GameNational Institute for Open Schooling (NIOS)21 November 2010
Address to the General Body of the Commonwealth Open Schools AssociationEducation for the 21st Century:Time for Open Schools to Raise their GameSir John DanielCommonwealth of LearningIntroductionIt is a pleasure to be with you. I apologise for having to talk to you today rather than during your conference proper tomorrow, but as you know, COLs big biennial event, the 6th Pan-Commonwealth Forum on Open Learning begins in Kochi this week and we have organised a series of pre-conference events that require my attendance. Your meeting also falls into that category and we are very grateful to NIOS for hosting it. I value the opportunity to address you because in the last two years I have become much better acquainted with open schooling than I was before. I shall start by explaining the personal journey that stimulated that interest and led directly to my new book Mega-Schools, Technology and Teachers: Achieving Education for All, which was published in English and Chinese earlier this year.As I wrote that book I came to the conclusion that those of you who work in open schools are far too modest about the role that open schools should play in 21st century education systems. Maybe you have toiled for so long in a part of the education system that has low status that you have failed to observe how things have changed. For large parts of the world the 21st century belongs to open schools, so my purpose today is to encourage you all to hold your heads higher and be more ambitious. Thats why Ive titled this address: Education for the 21st Century: Time for Open Schools to Raise their Game.I shall suggest several ways in which you should be more ambitious. First, open and distance learning, or ODL, is booming. You shouldnt let university people have a monopoly on research into this vital phenomenon of our times. I suspect there are ten papers maybe even a hundred published on ODL in higher education for each one on open schooling. Yet at the moment research on open schooling is more important and more interesting than adding extra embroidery onto the already considerable literature of higher distance learning. Second, you should take on a more central role in curriculum development for your national school systems. Open schools are national leaders in translating curricula into learning materials, which can be useful in the regular schools as well as for the open school pupils. You should arrange to be involved on a permanent basis in the processes by which your national curricula evolve. This would at least avoid the situations that some of you have experienced where a major curriculum change was announced and your open schools were left high and dry with quantities of obsolete materials that had to be scrapped.But your central role in contemporary education goes wider than curriculum. In nearly all countries, even very small ones, the education system is terribly compartmentalised. Different ministries and departments often do not coordinate their efforts and institutions at different levels of education live in their own solitudes. To be effective we need to take inspiration from biology and think of education in terms of an ecosystem. Open schools should a major node in such a system.So that is my agenda. Lets go back to the beginning. Why will the 21st century belong to open schools?Three key imperatives for educationThere are always plenty of challenges in education, both nationally and globally, but three stand out as being of overwhelming importance for the next 20 years. Open schools have a role to play in addressing all of them.The Secondary SurgeThe first is what I call the secondary surge. For the last twenty years and for some years to come the major educational preoccupation of developing country governments and international agencies has been the campaign for Universal Primary Education or UPE. I know this campaign well because from 2001 to 2004 I was Assistant Director-General for Education at UNESCO and that campaign defined much of my work. Our problem was that we were all so focussed on achieving UPE that we didnt spend much time thinking about what would happen if we were successful. And we have been successful. Thanks to the UPE campaign and huge efforts by many national governments, when it comes to getting children into primary school many developing countries have achieved in two decades what took a century for todays rich countries. There are still countries, notably Nigeria and Pakistan, that will be challenged to meet the goal of UPE by 2015, but most are well on the way.The result, of course, is that a tidal wave of millions of children actually hundreds of millions of children is now heading for secondary schooling. One researcher estimated a few years ago that 400 million children between the ages of 12 and 17 were not in secondary school (Binder, 2006).There is no chance whatsoever that the majority of these children will be accommodated by the expansion of conventional models of secondary education: the numbers are just too huge. Every possible alternative must be used to let them continue their education. Open schooling is by far the most promising of the available alternatives because it is scalable at reasonable cost.Climate changeSecondary schooling is important. We have expended so much energy in the last 20 years on promoting the importance of primary education that the case for secondary education has been neglected. Primary education is good, but both parents and children know that what will really make a difference to their opportunities in life is the education people receive after primary school. Secondary schooling for girls has a very special importance because it is humankinds best weapon against climate change. The primary driver of climate change is population. The reason that the world has a climate problem is that since the industrial revolution 200 years ago, the earths population has increased by a factor of seven. Moreover, since that time the demands that each person makes on the planets resources has also increased by a factor of seven, meaning that the impact of humankind on this world has grown by a factor of 50 times.If we want to stop or slow climate change the first thing we must do is slow population growth. This is where the secondary education of girls is so important. Women with secondary education have, on average around the world, 1.5 fewer children than those without secondary schooling (Cohen, 2008). A difference of just one child per woman means 3 billion more or fewer people on the planet by 2050. Secondary education for girls must be a priority.Teacher ShortageThe third challenge that I wish to flag is the teacher shortage. This is worldwide problem, not just a developing country problem, and has several causes. The rich world is seeing a massive wave of teacher retirements and, in some cases, horrendous attrition among new teachers. In the USA 50% of teachers leave the profession within five years of qualifying to join it. As well as attrition through retirement, many developing countries have to cope with a high death rate of teachers from AIDS at a time when they need many more teachers to complete the drive to universal primary education and expand secondary education.I am not proposing open schooling as a solution to the teacher shortage, although it does help countries to deploy teachers and teaching assistants in better ways. However, the curriculum development and delivery systems of open schools can be very helpful in expanding the in-service education of teachers on which so much depends. This is part of what I mean by saying that open schools are a major node in an educational ecosystem for the 21st century that also includes the ministries of education and the teacher education institutions.Open Schooling: raising the game The framework for education in the next two decades will reflect those three key educational challenges: the secondary surge; secondary schooling for girls; and the teacher shortage. Against that background let me return to my main theme, namely that it is time for open schools to raise their game. I start with research.ResearchThe memory of certain experiences stays with you a long time. I remember a cold day in January 2007 when I visited the World Bank with my COL colleague Mohan Menon. We had gone to the World Bank to talk about open schooling and, although Mohan was in charge of teacher education at COL at that time I took him along because, as a former chairman of NIOS, he knew a lot about open schools.Our address to the World Bank officials covered the issue that I raised earlier the secondary surge and urged them to take an interest in open schooling. They admitted that they hadnt given enough thought to the consequences of success in the campaign for Universal Primary Education and that they needed to do so. However, development agencies like the World Bank are hugely invested in traditional ways of doing things, which their economists have researched for years. In the case of secondary schooling, the research, which has been well summarised by Professor Keith Lewin (Lewin, 2008) shows that the difference in unit costs between primary and secondary schooling is much greater in developing countries than in the OECD countries. In the richer countries the unit costs of secondary are less than double those of primary, whereas in Africa secondary costs from 3 times to 8 times as much as primary. Lewin concluded that a country will never achieve universal secondary education unless it can get its national cost ratio down below two.You might think that such results would have spurred the development agencies to look for ways of lowering the costs of secondary schooling. In a way they have, but always within the classroom paradigm. For example, Lewin notes that some


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Read Rabbi Knopf's Recent Posts
- A New Prayer for the United States of America July 15, 2020
- Statement of Moral Outrage at Police Violence and Systemic Racism July 9, 2020
- Justice Demands RISC June 15, 2020
- Message to the Class of 2020 June 14, 2020
- Richmond's Wailing Wall June 12, 2020
Tag Archives: interfaith
'We can be so much more when we live in love': Two area faith leaders share thoughts of hope, help during COVID pandemic
The following are thoughts that David Dwight, Lead Pastor of Hope Church in Richmond, and I shared with the Richmond Times-Dispatch on helping people through the difficulties of life in COVID-19. (The questions and responses have been edited for length … Continue reading
Posted in Articles and Op-Eds, Public Statements, Reflections Tagged coronavirus, covid-19, culture, current-events, faith, health, healthcare, interfaith, personal, religion, society, spirituality Leave a comment
Renewing our Vows: A New Approach to Intermarriage
Recently, my congregation's lay leadership voted to permit its clergy to officiate at marriages between a Jewish individual and a partner from another background (with some important conditions), if and when the Conservative movement's Rabbinical Assembly and the Cantorial Assembly … Continue reading
Posted in Articles and Op-Eds Tagged Conservative Judaism, conservative rabbis, Conversion, interdating, interfaith, intermarriage, religion, society Leave a comment
Why I'm Still a Conservative Jew
My name is Michael Knopf. I grew up at a Conservative synagogue; I spent my summers at Camp Ramah in New England, a Conservative movement camp; as a teen, I was president of my Atlanta chapter of United Synagogue Youth, … Continue reading
Posted in Articles and Op-Eds Tagged Conservative Judaism, Denominations, interdating, interfaith, intermarriage, USY Leave a comment


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We have seen plenty of promotional material for Mission: Impossible - Rogue Nation, with plenty of talk about the film, with the movie being officially described as "Ethan and team take on their most impossible mission yet, eradicating the Syndicate - an International rogue organization as highly skilled as they are, committed to destroying the IMF."
As well as starring Jeremy Renner and Tom Cruise, the rest of the cast of Mission: Impossible - Rogue Nation includes the likes of Simon Pegg, Alec Baldwin, Rebecca Ferguson, and Ving Rhames, among others. Mission: Impossible - Rogue Nation is directed by Christopher McQuarrie and is set to hit the big screen on July 31 in both the US and the UK.
With still a few more months left to wait until the movie finally hits the big screen, we expect that we will get plenty more promotional material between now and then but, while we wait for that release date, why not sit back, relax and take a couple of minutes to enjoy the new Mission: Impossible - Rogue Nation trailer, below. It is certainly a good one.


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Cosmic Microwave Background Polarisation: foreground contrast and component separation
We evaluate the expected level of foreground contamination to the
cosmic microwave background (CMB) polarised radiation, focusing on
the diffuse emission from our own Galaxy. In particular, we perform a
first attempt to simulate an all sky template of polarised emission
from thermal dust. This study indicates that the
foreground contamination to CMB modes is likely to be relevant
on all frequencies, and even at high Galactic latitudes.
We review the recent developments in the design of data analysis techniques dedicated to the separation of CMB and foreground emissions in multi-frequency observations, exploiting their statistical independence. We argue that the high quality and detail of the present CMB observations represent an almost ideal statistical dataset where these algorithms can operate with excellent performance. We explicitly show that the recovery of CMB modes is possible even if they are well below the foreground level, working at the arcmin. resolution at an almost null computational cost. This capability well represents the great potentiality of these new data analysis techniques, which should be seriously taken into account for implementation in present and future CMB observations.
1 Introduction
Among all cosmological observables, the Cosmic Microwave Background (CMB) polarisation stores cosmological perturbations in the smartest way. The Stokes parameters and are non-locally combined to get the and modes, featuring opposite parity relations; as for total intensity (), modes are activated by all cosmological perturbations, and indeed the two are strongly correlated (); on the other hand, modes are excited by vectors and tensors only; since no significant power is experted from vectors, a detection of modes would be a strong indication of the presence of cosmological gravitational waves. For a comprehensive review of the CMB physics, see Hu et al. (1998) and references therein.
On the observation side, we are right now in the epoch in which the CMB is revealing its finest structure. The Wilkinson Microwave Anisotropy Probe (WMAP) satellite111map.gsfc.nasa.gov released recently the first year CMB data, for and , unveiling all sky anisotropies with about arcmin. resolution on a frequency range between and 90 GHz (see Bennett et al., 2003, and references therein); balloon-borne and ground-based observations cover angular scales from a few arcminutes to tens of degrees, and also aim at measuring CMB and modes (see Kovac et al., 2002, for a first mode detection). The Planck satellite222astro/estec.esa.nl/SA-general/Projects/Planck will provide total intensity and polarisation full sky maps with resolution and a sensitivity of a few K, on nine frequency channels between 30 and 857 GHz.
This work focuses on the foreground contamination to the CMB polarised emission. This issue is gathering greater and greater attention as the importance of the CMB polarisation measurements increases (see De Zotti, 2002, for reviews). In Section 2 we estimate the expected strength of foreground polarised emission with respect to the CMB; in Section 3 we describe the recent progresses in the design of data analysis tools designed to reduce such a contamination; in Section 4 we make some concluding remarks.
2 Foreground contamination to the CMB
We focus on the diffuse emission from our own Galaxy. Indeed, at microwave frequencies, the contamination from Galactic, extra-Galactic radio and infrared sources (see De Zotti, 2002, and references therein), as well as the polarised Sunyaev-Zel Dovich emission (see White, 2003, proceedings of this conference), are likely to be relevant for the damping tail of the CMB power spectrum, i.e. at arcmin. angular scales, corresponding to multipoles of the order 1000, which sets the limit of validity for our analysis.
The main diffuse foreground at low microwave frequencies, say
GHz is expected from Galactic synchrotron.
The available high resolution data in the radio band, approximately
arcmin., are at low and medium Galactic latitudes,
(Duncan et al., 1999; Uyaniker et al., 1999); degree resolution data (Brouw & Spoelstra, 1976) cover
about half of the sky and reach high latitudes. These templates have been
used to evaluate the angular power spectrum of synchrotron in the radio
band, up to arcmin. scale
(Tucci et al., 2000; Baccigalupi et al., 2001; Giardino et al., 2002; Tucci et al., 2002; de Oliveira-Costa et al., 2003, proceedings of this conference).
Tucci et al. (2000) estimated , regardless of the Galactic region considered; note that the same behavior was quoted for the first time by Tegmark et al. (2000). Baccigalupi et al. (2001) found the same result, regardless also of the Galactic latitude, up to the highest probed ; they also estimated the level of Faraday depolarisation to be important, but not such to mask substantially the true synchrotron emission; moreover, they estimated the power on super-degree angular scales, corresponding to multipoles , using the Brouw & Spoelstra (1976) data, finding a steeper behavior, . Giardino et al. (2002) estimated the power spectrum of the cosine and sine of the polarisation angle up to the arcmin. scale, and out of that constructed a spatial template assuming Gaussian distribution; the resulting pattern was then used to simulate templates for and out of the total intensity Haslam map at 408 MHz, assumed to be synchrotron dominated and theoretically polarised at ; they also estimated the synchrotron spectral index as inferred by multi-frequency radio observations. Tucci et al. (2002) extended the power spectrum analysis up to a few thousand multipoles, and de Oliveira-Costa et al. (2003) performed a detailed study of the and modes in the large scale data.
The CMB contamination from diffuse Galactic dust is much more uncertain. The main emission mechanism arises from the thermal emission of magnetized dust grains, which get locally aligned by the Galactic magnetic field (Lazarian & Prunet, 2002). Moreover, indications of a non-thermal dust emission, possibly connected with rapid rotations of the grains and extending to much lower frequencies, has been conjectured in several works, although in the WMAP data there is no evidence of such component (see Bennett et al., 2003, and references therein). In total intensity, a resolution all sky template of dust emission is available at 100 m, and on the basis of a correct interpretation it can be scaled at microwave frequencies and compared with the CMB (see Finkbeiner et al., 1999, and references therein). In polarisation, a great achievement has been obtained by Archeops (see Ponthieu et al., 2003, proceedings of this conference), which measured a polarised dust signal on the Galactic plane. On the basis of these two ingredients, we propose here a naively simulated template of the polarised dust emission, which agrees remarkably well with previous estimates (Lazarian & Prunet, 2002; Prunet et al., 2000). We assume perfect correlation between total and polarised intensity and a polarisation degree. Then we assume the same polarisation angle pattern of the synchrotron emission (Giardino et al., 2002). That is certainly quite drastic, but it corresponds to the assumption that the Galactic magnetic field is 100% efficient imprinting the polarisation direction to the dust and synchrotron emission.
The Stokes parameter template333Unless otherwise specified, the maps and power spectra we show are in Kelvin, antenna temperature. obtained by Giardino et al. (2002), hereafter , is shown in figure 1, together with the spectral index template, upper and lower left panels, respectively; we also show the template obtained rescaling to match the power spectrum predicted by Baccigalupi et al. (2001), upper right panel; we also show the template for the polarised thermal dust emission as described above, in the right lower panel. , and dust are shown in a non-linear scale in order to highlight the behavior at high Galactic latitudes; the corresponding template for is qualitatively equivalent; they have been extrapolated to 100 GHz, in antenna temperature, using the spectral index template for synchrotron and the latest recipe by Finkbeiner et al. (1999) for dust. By visual inspection, the model appear to be less structured on small angular scales with respect to the and the dust template; the latter has the sharpest decrease with Galactic latitude, as we discuss below.
Before quantifying the contamination to the CMB polarisation angular power spectrum, it is useful to give a look at the whole foreground statistics and sky distribution, plotted in figure 2; from top to bottom, the left and right panels represent signal distribution and root mean square as a function of for , and dust. The signal distributions are far from Gaussianity, and exhibit a marked super-Gaussian behavior, as the total intensity maps from which all these templates were derived. Also, as we anticipated, the dust and templates present the strongest and weakest dependence on the Galactic latitude, respectively. For the dust, the reason is the assumed perfect correlation between total and polarised intensity. For , as we see now more in detail, most of the power lies on the small angular scales, which propagate well outside the Galactic plane.
In Fig. 3 we report the power spectra of the ,
and dust templates, compared to the CMB444We realize a CMB
template according to the WMAP data: ,
also assuming a tensor to scalar ratio , rather close to the
current upper limit (see Bennett et al., 2003, and references therein)., on all sky
and with a Galactic cut excluding the region with latitude .
The plots are at 100 GHz, in antenna temperature. The synchrotron
frequency scaling according to the template in figure 1
is approximately , making the contamination
rapidly worse at lower frequencies. For the dust, the scaling is
given by Finkbeiner et al. (1999), which in the frequencies of interest here,
say the interval covered by WMAP and Planck, is approximately
, where and
are the Planck and Boltzmann constant, and the thermodynamical dust
temperature Kelvin; the departure from a pure
black body behavior is due to the heating that the interstellar
medium gets from stars (see Prunet et al., 2000, and references therein).
The CMB fluctuations in antenna temperature scale as the
derivative of the black body brightness
As a general feature, it can be noted how the Galactic emission has almost
equal power on and modes, according to the most natural expectation
for a non-cosmological signal (Zaldarriaga 2001).
On a full sky analysis, the polarised dust dominates. This is likely to be the case if the observed polarisation degree really holds for all scales and the polarisation angle statistics is not too far from the synchrotron one. On the other hand, this signal does show the most abrupt drop when the Galaxy is cut out, which cleans almost completely the CMB and modes, remaining however substantial for the ones; note that this case agrees remarkably well with the level quoted by Prunet et al. (2000) at intermediate Galactic latitudes.
On all sky, the synchrotron contamination is severe on large angular scales, almost covering the CMB reionization bump for and , being somewhat less important for . On , the signal drops rapidly below the CMB at a few tens in , while affects the first CMB acoustic oscillation. An important point is that the Galactic cut is not as effective as for the dust: the reason is the weaker Galactic latitude dependence for synchrotron, as it is evident in figure 2. As a result, the CMB modes are likely to be severely contaminated even when the Galaxy is cut out.
We conclude that our present knowledge of the diffuse Galactic polarisation emission indicate that CMB and modes are relatively clean, at least at medium and high Galactic latitudes and at frequencies around 100 GHz, while the modes are likely to be severely contaminated, at all frequencies and Galactic latitudes.
3 Component Separation
Despite of the severe foreground contamination, the CMB modes are expected to carry most important details on the nature of cosmological perturbations, as we stressed in the Introduction. For this reason it is worth to study data analysis techniques capable to clean the CMB from foreground contamination. This is feasible by exploiting the statistical differences of CMB and diffuse foregrounds, starting from a wide enough multi-frequency coverage of a given observation. The data can be sketched as
where represents the data at the frequencies, the components corresponding to each emission, and the instrumental noise; is the mixing matrix, scaling and mixing the emissions at any observed frequency, while is the number of pixels of the observation, or equivalently the number of harmonic coefficients if the analysis is performed in the spectral domain. Note that in general the angular resolution varies among the frequency channels. The target is to recover from ; as we saw in the previous Section, the problem is undetermined since we know A only partially, and the guesses on s are not reliable for stabilizing the inversion of the relation (1), either if the noise statistical properties are very well known, or even in a noiseless case. On the other hand, a well established expectation is that the CMB and foreground emission are statistically independent. It has been recently shown that this feature can be exploited to design "blind" component separation tools, i.e. able to recover even without any prior on s or A; a first algorithm of this class was proposed for use in astrophysical component separation by Baccigalupi et al. (2000) based on the novel concept in signal processing science, the Independent Component Analysis: that works by finding a matrix which applied to in (1) brings to . The criterion to find is to look for the statistically independent patterns in : that is clearly not unique and can be specialized for the problem at hand. A fast version (FastICA) adapted for satellite observations has been proposed by Maino et al. (2002); this technique has been further developed to account for any available and reliable prior, and successfully applied to the real COBE data by Maino et al. (2003). Recently, a different and promising blind technique based on a spectral matching of real and modeled data Delabrouille et al. (2003).
The first application of component separation to polarisation radiation
has been performed by Baccigalupi et al. (2003), with a FastICA approach:
separation is conducted on and Stokes parameters separately or
considered as a single signal provided that they obey the same statistics;
we refer to that work for any detail on the algorithm procedure. Here we
show a very simple application, with rather impressive results, to highlight
the potentialities of this technique. We consider a noiseless mixture of
polarised CMB and synchrotron , scaling uniformly in frequency,
at 50 and 80 GHz, on all sky and pixel size of about 3.5 arcmin.; note that
we do not refer to any operating or planned experiment, and choose the
frequencies among those in which CMB and synchrotron are roughly comparable.
The two channels are input to the FastICA to recover synchrotron and CMB
separately. Figure 4 show the input sky angular power
spectra for (left) and (right) together with the spectra of the
recovered CMB as output by FastICA. As it is evident, a CMB major cleaning
was achieved: the dotted line is the input sky power, while the
recovered CMB (solid) line is actually almost indistinguishable from the
input one (dashed). We stress that this is without the use of any prior, i.e.
not knowing any piece of A or . The algorithm knows only the
data at the two frequencies, and looks for the most statistically independent
components in those data. In addition, applying this technique in particular
is computationally free: the results in figure were obtained in about five
minutes on an ordinary single processor personal computer.
In particular, the CMB modes have been impressively cleaned: interpreting the foreground emission as noise, the signal to noise ratio is 0.1 or less, at all multipoles, as it can bee seen in the right panel of the figure. CMB modes have also been cleaned wherever the foreground contamination was relevant. The algorithm outputs also A, which differs from the real one by percent or less.
The reason of such an excellent performance is just the high level of detail of the underlying data. At arcmin. resolution, the maps are almost ideal datasets where the algorithm can look for the least statistically linked templates present into the maps themselves. Even if all the instrumental details were neglected, what we show here should be enough to gather attention on these new data analysis techniques, as we further stress in the next Section.
4 Concluding remarks
In this work we show that at frequencies around 100 GHz the diffuse Galactic polarisation emission is likely to be rather weak in comparison to the CMB and modes, at least at medium and high Galactic latitudes, while the ones are seriously contaminated on all sky. At lower and higher frequencies, the contamination gets rapidly worse because of the steep frequency behavior of synchrotron and dust, respectively.
We stress that the new concepts in signal processing science can be exploited in this context, to cancel or greatly reduce such a contamination. In particular, the statistical independence of CMB and foreground emission is suitable to achieve this goal: we give an impressive example based on the FastICA technique in polarisation (Baccigalupi et al., 2003), where CMB modes are recovered out of a foreground emission about ten times stronger, without any prior information but their statistical independence, and at an almost null computational cost.
These features represent the "nominal" capabilities of these algorithms, i.e. their performance on ideal datasets: cleaning the cosmological signal from substantial foreground contamination, exploiting only their natural diversity. This is in our opinion a great achievement, providing the basis on which the implementation to any particular observation can be built. The latter step, of course, presents challenging issues: the noise level, sky distribution and non-stationarity, as well as the non-uniform spectral index of the components to recover, are good examples. However, we have already the indications of a substantial stability of the nominal performance against instrumental features and systematics: Maino et al. (2002) and Baccigalupi et al. (2003), respectively for total intensity and polarisation, perform a whitening of simulated Planck data in order to get rid of the noise bulk in the FastICA separation process. Most importantly, the results of Maino et al. (2003) show that these techniques are flexible enough to be applied to real data, the COBE ones, getting outstanding results, namely the correct large scale CMB power spectrum amplitude and shape.
While waiting for the era of large scale CMB polarisation measurements, the next obvious target is a successful application to the WMAP data, meaning the recovery of CMB data on sky regions affected by Galactic contamination which are normally cut out.
The author warmly thanks Gianfranco De Zotti, Giovanna Giardino, Eric Hivon, Francesca Perrotta, George Smoot and Radek Stompor for useful discussions. The HEALPix pixelisation scheme, available at www.eso.org/healpix, by A.J. Banday, M. Bartelmann, K.M. Gorski, F.K. Hansen, E.F. Hivon, and B.D. Wandelt, has been extensively used.
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How We Live Together (2018 - 2020)
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