I decided to start with the pegboard over the general use bench, which sees everything from sharpening on the grinder to rewiring lamps for the wife. This area had really gotten pretty bad with a fair amount of "stuff" hung randomly over the last few years.
I stripped the board completely, determined to not hang anything on it which I would not absolutely NEED or USE in that area. Time for some brutally honest reflection. I do NOT need to hang EVERY screwdriver and EVERY pair of pliers I own above this bench. Only a 4-in-1 and a ratcheting screwdriver were hung in a central location within easy reach. A wooden holder containing various tips for the ratcheting screwdriver, along with it's flexible shaft and the extra long bit holder accompanies the tool for which they are intended. There is a mechanic's style tool chest on the left end of the bench containing wrenches, sockets, drive handles and all manner of pliers, all within easy reach. No need to hang any of those in this area. I put the excess of these in a box for redeployment elsewhere either in the shop or house.
It's amazing how much space gets freed up for other items one actually needs, IF it is limited to ONLY items that will be used in that area. Like the soldering iron, plus a holder for it's attendant solder and flux. Or the staple gun plus a wire holder for the staples to go in it. How about the wire stripper that always seemed to be lost before now? Oh, and I now ALWAYS know where I put my shop reading glasses, now. There is a wire holder for the hard plastic eyeglass case. It's not just roaming around the bench top anymore.
So far, I'm very pleased with the new "work station" approach, wherein only the tools used and needed in that area are kept handy. Nothing inspires like success, so I can't wait to get out there and get more area organized !!!
Sounds like you are taking control of the clutter. Good for you. I need to follow suit and revisit some of my clutter!
I have never seen a "actual working shop" that stayed totally clutter free!
Only in the magazine pictures do hey look that organized!
I clicked the post, thinking I'd see pegboard in the dumpster, lawl.
Congrats on organizing progress, I need to do the same thing and actually started some cleanup over the weekend as the weather cooperated a bit. There's a lot to be said for getting rid of what hasn't brought us joy in years. Shops have scraps that will never be used for projects, tools that are redundant, and clutter that stands in the way of efficiency.
Since I began this reorganization project, two side benefits have presented themselves: First, I have been able to repurpose some items that have been lurking around the shop for hanging tools and/or supplies. (For instance, a few quick snips with diagonal cutters and a couple of bends have transformed a wide wire drawer organizer into two "pockets" for tools. Another long, thin drawer organizer became the pocket to hold the shop reading glasses in their hard plastic case. The wire mesh pencil cup was flattened slightly on one side, and held in place with two 1/8 plastic anchors and screws (Which I had on hand) Pencils, a box cutter, the paint can opener now live in this stabilized container. Being a "scrounge" at heart, I'm glad to be able to find new life for these things that have been kicking around for awhile. (The wife has sent some of her crap to the garage. I my domain, I consider it "fair game" for reusing to my purposes…..) It's pretty amazing what you can hang on pegboard with a little imagination.
The second benefit is the surprising amount of hardware I have unearthed. Screws, nuts, bolts, hinges, mending brackets, etc. I've been putting these in a shoe sized box so they're all in one place, and can be sorted out later. This will save some time and money at the hardware store, that's for sure.
Your way ahead of me…I live in southern Maryland and with the break in the weather I just completed getting the first inspection for power being run to what is going to be my new shop. Wish it was done and I was doing the "organizing"!!!!
One last comment about reorganizing the pegboard. The natural inclination is to have everything hanging flat up against the wall. But if you look at some of the factory made hooks, some of them can be pretty long. Since the bench in question is 24 inches, having some of the items stick out three or four inches doesn't hurt anything. With some hooks made out of coat hanger wire added sideways to a long hook, things like large tin snips can be hung at 90 degrees to wall. This takes up less wall space while not interfering with the main work area. Just make sure these items are placed in an area where there is no risk of bumping your head on them !
Hey, I'm what the outsiders call a "Southern Maryland Inbred" (or S.M.I.B.) myself ! I ve just been displaced up here around Frederick.
Small world … I was born in Frederick. We moved to Virginia when I was just a few months old. My dad is now back in Frederick, just north of the Monocacy National Battlefield.
You will have to take some photos once you reorganization is complete.


2018-19 Printable School Calendar - UPDATED!
We engage, empower, and collaborate to educate and prepare every Bearcat for college, career, and life as a global citizen.
Full Day: 8:50 a.m. - 3:50 p.m.
Full Day: 7:30 a.m. - 2:40 p.m.
Full Day: 7:40 a.m. - 2:50 p.m.
Half Day: 7:40 a.m. - 10:40 a.m.
Half Day: 7:30 a.m. - 10:45 a.m.
Full Day: 9:00 a.m - 3:00 p.m.
Half Day: 9:00 a.m. - 11:46 a.m.
Night School Program: 4:00 p.m. - 8:00 p.m.
Morning: 7:45 a.m. - 10:45 a.m.
Afternoon: 11:35 a.m. - 2:40 p.m.
Morning: 7:45 a.m. - 10:30 a.m.
Afternoon: 11:50 a.m. - 2:35 p.m.
12:00 p.m. - 3:15 p.m.
To begin the enrollment process or for more information, visit the BCPS Enrollment page.
Applications are NOW OPEN through April 5, 2019 and spaces are limited. To apply, click below or learn more at Fremont's page or BC STEM's page.
A world-class system providing a quality education that prepares all students to be productive and responsible citizens. Battle Creek Public Schools will ensure a quality education for all students through quality teaching and support from all staff.
Battle Creek Public Schools is an urban school district located in Calhoun County, Michigan. It serves a major portion of the City of Battle Creek, portions of Emmett Township, Pennfield Township, Bedford Township, and the City of Springfield. The district includes one high school, two middle schools, six elementary schools, including a STEM (Science, Technology, Engineering, and Mathematics) school, and a new Alternative High School housed at the W.K. Kellogg Middle School. There are four sites in the district for Early Childhood Education, the Battle Creek Area Math and Science Center, and an adult education program. The district also has one of the nation's few remaining Outdoor Education Centers located on beautiful Clear Lake in Dowling, Michigan.
EDUStaff has partnered with Battle Creek Public Schools to recruit, train, and provide qualified substitute teachers and paraprofessionals for Battle Creek Public Schools and Calhoun ISD.
The W.K. Kellogg Foundation announced a five-year, $51 million grant to Battle Creek Public Schools to help ensure that every child receives a quality education. Our goal is that every Battle Creek student graduates, and receives the preparation and support they need for college or a career.
Whether your child is entering kindergarten or is a senior in high school, every single student at every grade level in BCPS will benefit from these resources.
The grant will support opportunities in literacy, pre-K, new books and supplies, professional development for teachers, reduced class sizes, and investments in arts, music and athletics.


Re: Captain Planet Funko POP!
Jalcmkzv87 wrote: Earth! Fire! Wind! Water! Heart!
Different Chrome Planet for each one?
How come we don't have Captain Planet Funko POP! yet - I think that this is something that should have been fairly easy to knock out. I think it would be dope to have Captain Planet as a earth day exclusive through Box Lunch and have all of the different planeteers as well. Would you guys be interested in Captain Planet POP!?
Hahaha I just need their rings to glow in the dark.
Jalcmkzv87 wrote: Too many chromes .
chrome is hideous as it is in my opinion, but there is no way Captain Planet is a popular enough license to support needless variants like that anyway.
Gofunkoyourself wrote: Only if we can get the planeteers as a 5-pack! I love a good 5-pack. Captain planet could come to ECCC because he is green! Nailed it.
Thats what I'm talking about, I would be all over that.
Been wanting one for ages!
I think that Wall-E was a excellent choice for earth day last year... but I definitely think if they want to take it up another notch which Im sure Funko wants to do - They can go ahead and drop Captain Planet for Earth Day. It also would make sense for a Captain Planet to show up for Emerald City Comic Con - If it was me I'd drop Captain Planet first and drop the planeteers later based off of how well Captain Planet does.
Maybe this could be the chase version?
Semi-Chrome like Colossus Capt Planet would be awesome!
MsLafleur82 wrote: Semi-Chrome like Colossus Capt Planet would be awesome!


text:
Q: Unable to load Action class while deploying struts2.5 war file on weblogic 10.3.6 Unable to load Action error while deploying struts2 war file on weblogic 10.3.6
The above question is very similar to the issue I'm facing but there is no solution provided.
I have an application in struts2.5 which I have exported to a *.war file and trying to deploy it to weblogic 10.3.6(running on java7).
During deployment I get an error that the Action class is not found (when I can see it present in the war file's WEB-INF/classes).
As mentioned by user3898783 in above link- "What weblogic does during
WAR deployment(obviously it internally explodes) it puts all the files reside in web-inf/classes folder into jar called _wl_cls_gen.jar file and copies into web-inf/lib directory under domain stage folder." - similar is my problem.
I am currently using the wls:prefer-web-inf-classes"true" /wls:prefer-web-inf-classes configuration in my weblogic.xml file which hasn't really solved my problem.
Weblogic.xml
<?xml version="1.0" encoding="UTF-8"?>
<wls:weblogic-web-app xmlns:wls="http://xmlns.oracle.com/weblogic/weblogic-web-app" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://java.sun.com/xml/ns/javaee http://java.sun.com/xml/ns/javaee/ejb-jar_3_0.xsd http://xmlns.oracle.com/weblogic/weblogic-web-app http://xmlns.oracle.com/weblogic/weblogic-web-app/1.4/weblogic-web-app.xsd">
     <wls:container-descriptor>
        <wls:prefer-web-inf-classes>true</wls:prefer-web-inf-classes>
     </wls:container-descriptor>

    <wls:session-descriptor>
        <wls:cookies-enabled>true</wls:cookies-enabled>
     </wls:session-descriptor>

</wls:weblogic-web-app>

<May 23, 2019 1:00:02 AM CDT> <Error> <HTTP> <BEA-101165> <Could not load user defined filter in web.xml: org.apache.struts2.dispatcher.filter.StrutsPrepareAndExecuteFilter.
Unable to load configuration. - action - zip:/apps/bea/wls103/user_projects/domains/mydomain/servers/mymanagedserver/tmp/_WL_user/myapp/4bdx7o/war/WEB-INF/lib/_wl_cls_gen.jar!/struts.xml:16:97
        at org.apache.struts2.dispatcher.Dispatcher.init(Dispatcher.java:509)
        at org.apache.struts2.dispatcher.InitOperations.initDispatcher(InitOperations.java:73)
        at org.apache.struts2.dispatcher.filter.StrutsPrepareAndExecuteFilter.init(StrutsPrepareAndExecuteFilter.java:61)
        at weblogic.servlet.internal.FilterManager$FilterInitAction.run(FilterManager.java:343)
        at weblogic.security.acl.internal.AuthenticatedSubject.doAs(AuthenticatedSubject.java:321)
        Truncated. see log file for complete stacktrace
Caused By: Unable to load configuration. - action - zip:/apps/bea/wls103/user_projects/domains/mydomain/servers/mymanagedserver/tmp/_WL_user/myapp/4bdx7o/war/WEB-INF/lib/_wl_cls_gen.jar!/struts.xml:16:97
        at com.opensymphony.xwork2.config.ConfigurationManager.getConfiguration(ConfigurationManager.java:69)
        at org.apache.struts2.dispatcher.Dispatcher.getContainer(Dispatcher.java:957)
        at org.apache.struts2.dispatcher.Dispatcher.init_PreloadConfiguration(Dispatcher.java:463)
        at org.apache.struts2.dispatcher.Dispatcher.init(Dispatcher.java:496)
        at org.apache.struts2.dispatcher.InitOperations.initDispatcher(InitOperations.java:73)
        Truncated. see log file for complete stacktrace
Caused By: Action class [com.myapp.struts.actions.LoginAction] not found - action - zip:/apps/bea/wls103/user_projects/domains/mydomain/servers/mymanagedserver/tmp/_WL_user/myapp/4bdx7o/war/WEB-INF/lib/_wl_cls_gen.jar!/struts.xml:16:97
        at com.opensymphony.xwork2.config.providers.XmlConfigurationProvider.verifyAction(XmlConfigurationProvider.java:508)
        at com.opensymphony.xwork2.config.providers.XmlConfigurationProvider.addAction(XmlConfigurationProvider.java:457)
        at com.opensymphony.xwork2.config.providers.XmlConfigurationProvider.addPackage(XmlConfigurationProvider.java:572)
        at com.opensymphony.xwork2.config.providers.XmlConfigurationProvider.loadPackages(XmlConfigurationProvider.java:326)
        at org.apache.struts2.config.StrutsXmlConfigurationProvider.loadPackages(StrutsXmlConfigurationProvider.java:108)
        Truncated. see log file for complete stacktrace
>

I checked my struts.xml(struts.xml:16:97) - and it is pointing to the LoginAction action class mapping, which obviously its not able to find under the weblogic "../domains/../mymanagedserver/tmp/_WL_user/myapp/4bdx7o/war/WEB-INF/classes"
Thanking you in anticipation

A: Finally I was able to figure this out. The culprit has been the compiler compliance level in my eclipse project.  Although I was using jdk1.7 in my project buildpath, I should have also checked for the projects compiler compliance version in Eclipse which was 1.8 (proj right click> JavaCompiler> I set it to 1.7).
Also, I was using javax.servlet-api-3.0.1.jar - I switched to servlet2.5 as I read somewhere that weblogic10.3.x is only compliant upto servlet2.5.
I hope this helps someone looking for a solution to similar problem.

redpajama_set_name: RedPajamaStackExchange


text:
UK and Central America sign continuity agreement
UK Government | 18 July 2018
The UK government has signed a trade and political continuity agreement with Central America.
Trade between the UK and Central America was worth £1bn in 2018.
Agreement ensures British businesses and consumers benefit from continued access to the region after we leave the EU.
The UK and Costa Rica, El Salvador, Guatemala, Honduras, Nicaragua and Panama have signed the UK-Central America Association Agreement.
Ambassador Ross Denny signed the agreement in Managua, Nicaragua together with Trade and Economic Ministers from each of the six Central American countries.
The Agreement will ensure British businesses and consumers benefit from continued trade with Central America after we leave the European Union. It provides tariff-free trade of industrial products together with liberalisation of trade in agricultural food production and fisheries products.
Consumers in the UK will continue to benefit from lower prices on goods imported from Central American countries party to this agreement, such as prawns from Honduras and Costa Rican fruit. Consumers in Central America will continue to benefit from lower tariffs on products such as drinks and cars produced in the UK.
Trading on these preferential terms rather than on World Trade Organization terms will deliver significant savings and help to support British jobs. It will also help further strengthen the trading relationship between the UK and Central America, which was worth £1 billion in British exports and imports in 2018.
The Agreement provides a framework for cooperation and development through political dialogue, increased economic ties and our work on important issues like the environment and human rights, reaffirming Britain's commitment to a close relationship with Central America.
Welcoming the new Agreement, Foreign Secretary Jeremy Hunt said:
This agreement is of real importance as we prepare to leave the European Union and strengthen our ties with the rest of the world. It will help provide the certainty business need to be thrive and help turbocharge our economy into the future.
It has also been achieved thanks to the hard work of UK diplomats and I thank them for their work.
We look forward to building on our political and economic ties, with exporters and consumers having the certainty they need to continue trading freely and in confidence abroad.
This agreement replicates the existing EU-Central America trading relationship as far as possible and will ensure continuity in the trading relationship between the UK and Central America when the UK ceases to be a member of the EU.
The British Government is continuing to work intensively on securing continuity with other countries. We have secured agreements – either signed or agreed in principle - that account for 64% of the UK's trade with all the countries with which the UK is seeking continuity, should we leave the EU without a deal.
Wilson Del Socorro, Global Director of Government Affairs for Diageo PLC added:
Diageo warmly welcomes the news of a Central America-UK Association Agreement.
The free flow of international trade is vital to Diageo as it gives us the opportunity to reach more consumers and markets. Central America is an important export market for Diageo and for Scotch whisky.
We look forward to enhanced bilateral ties that support the future growth of trade in goods, services and cultural exchanges.
The UK-Central America Association Agreement will come into effect when the current Agreement between Central America and the EU ceases to apply. This will take place either following an implementation period if the UK leaves the EU with a deal, or on 31 October 2019 if the UK leaves the EU without one.
This agreement will now be subject to the domestic parliamentary procedures of all countries party to the agreement before it can be brought into force.
The UK will continue to be covered by the EU Central America Agreement while the UK is a member of the EU, and during an Implementation Period. This agreement is designed to take effect when the EU-Central America agreement ceases to apply to the UK.
The UK has signed or agreed in principle 13 trade continuity agreements with 38 countries, these include some of our biggest trading partners. A regularly updated list of all signed agreements is available on GOV.UK.
Total exports from the UK to Central American Countries party to this agreement were worth £346m in 2018. Total trade was worth £1bn.
Source of trade statistics: ONS: UK total trade: all countries, non-seasonally adjusted October to December 2018 release.
source: UK Government
Central America UK

redpajama_set_name: RedPajamaCommonCrawl


text:
OnePlus 7 to be unveiled on May 14
Sagar 23 April 2019
OnePlus Android
OnePlus has announced that it will launch its 2019 smartphones - OnePlus 7 and 7 Pro - next month on May 14.
Renders of OnePlus 7 and 7 Pro
The launch event will be held in New York at Pier 94 and will commence at 11am EDT. And, like previous events, it will be open to fans who can attend it by purchasing tickets from OnePlus.com.
Early bird tickets will be available starting April 25 at 11am for 48 hours at a discounted price of $20, with the Standard and Plus One tickets going on sale afterwards.
OnePlus will also be holding launch events in London, UK and Bangalore, India simultaneously at 4pm BST and 8:15pm IST, respectively; and there will be a separate event for its home country China on May 16 at Yanqi Lake, Beijing at 2pm PST.
OnePlus 7 case renders show off notch-less display and triple rear cameras
OnePlus 7 shines in CAD renders again, but this time without a pop-up camera
OnePlus 7 Pro could have a QHD+ 90Hz display, stereo speakers
OnePlus 7 Pro camera details leak: 3x zoom and ultra-wide camera
Just having a beer
They may have it, but they will not review it until it is released. It ia a fair play I would say. Every news have to have some standards...
vGu
THIS! The SAR limits were chosen that way.
2Au
I doubt it. But if they already have it. They can't release it yet due to news or press embargo.


Camden is not what people think of when they read "Garden State" on New Jersey license plates. But that could change this year, when a 78,000-square-foot, warehouse-style building starts to rise in a weed-strewn field in the 1500 block of Broadway.
The New Yorker's Ian Frazier spent months getting to know our team and visiting our farms and customers. His impressions are thoughtful and incisive.
After years of experimentation, Silicon Valley may finally be making urban farming viable.


Don't want the Windows 10 Upgrade? Getting tired of it constantly asking you to install? Microsoft delivered this notification through a program which is installed through Windows update. The upgrade assistant is named GWX.exe in C:\Windows\System32\GWX.
If you are not interested in Windows 10, you can remove this program from your PC. Go to Windows Update->Installed updates, remove KB3035583. Also, you will need to hide the update again in windows updates to prevent it from auto installing again since this is marked "important".
Next → Next post: How can I change my email address password using Mailbox Manager?


text:
पात्रा के अनमोल रतन 💩- Ep56 #TheDeshBhakt with Akash Banerjee
Akash Banerjee
Unsubscribe from Akash Banerjee?
Often blamed for single handedly lowering the level and logic of TV debates - Sambit Patra turns 44 today and to mark his momentous occasion .... #TheDeshBhakt wants to thank #SambitPatra for the entertainment, the drama and volume levels - that kept kids away from stuff like BiggBoss & Naagin.
44 gems from Patra's unlimited repository to show you his talent / range and sheer brilliance. Have a good laugh and send a tweet thanking Patra for keeping our democracy in a humorous condition! Support #TheDeshBhakt & Join The Desh Bhakt Toli!
Patreon - https://www.patreon.com/akashbanerjee
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Twitter: - @akashbanerjee
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Facebook - @akashbanerjee.in
Clip Credits -
https://www.youtube.com/watch?v=jOR5D...
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A Little Egret was just N of Sollas township, North Uist early this afternoon.
In the late afternoon Joan MacInnes phoned to say she had taken a photo of an all white heron-like bird with a yellow bill that was by the cattle on her croft at Stoneybridge, South Uist. From her description undoubtedly a Cattle Egret and presumably the same bird that was present at Daliburgh on the 21st.
A large arrival of Redwings on Barra today, roughly 800 birds around the island. The small Canada Goose was still on Borve Point with c150 Barnacle Geese. Around 15 Chiffchaffs and 5 Blackcaps were still around the island.


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This Month's Content
ASIS International Gets Together with ISSA
It's another step along the convergence path. ASIS International has signed a memorandum of understanding with the Information Systems Security Association. ISSA serves information security and risk professionals with more than 138 chapters and members in 70 countries, ranging from the first-year systems administrator to the senior-most information security executive. ISSA is the second industry organization to align with ASIS in 2009.
The vision of this relationship is to increase collaboration in and among organizations that have access to the disciplines and thought leadership surrounding Enterprise Security Risk Management. Providing a foundation where the respective organizations and their members can actively collaborate in the development of education content through research, demonstrated best practices, principles and approaches involving ESRM is the immediate objective.
The ASIS approach was initiated in 2008 in response to the development and evolution of an Enterprise Security Risk Management body of knowledge. ESRM is the practice of integrating all the areas of an organization that involve the protection of people, property and information. A key component of Enterprise Risk Management—which considers the entire risk universe, including financial, strategic and operational—ESRM is where security professionals ensure that multiple disciplines and business units communicate effectively and work together to identify, prioritize and mitigate risk.
"Our involvement with the ISSA is in the interest of rapid advancement and development of the ESRM body of knowledge," says ASIS' Chief Executive Officer Michael J. Stack. "This relationship allows for periodic discussions regarding common strategic, tactical or operational opportunities or partnerships that would be mutually beneficial to each member's organizations."
According to the terms of the agreement, members of ASIS and ISSA will meet regularly to identify joint strategic and operational opportunities. They will also collaborate on developing educational content for each other's domestic and international programs. Additionally, ASIS and ISSA will cooperate to provide mutual member discounts on fees to attend ASIS/ISSA educational programming, provide access to member's only content on websites and support global evolution of security standards and guidelines.
"As the worlds of logical security, physical security and compliance converge, we need to continually equip our members, and our profession, with the skills to present a holistic view of security risks," says ISSA's President Howard A. Schmidt. "Working together with ASIS provides our chapters and members access to an array of educational events, as well as an extended network of security professionals, that will help prepare us for the next generation of security risk challenges."
Earlier this year, ASIS formalized a relationship with the Open Security Exchange, a group dedicated to accelerating convergence of IT and physical security.
Security eNewsletter & Other eNews Alerts
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text:
<?php
namespace Spot\Relation;

use Spot\Mapper;
use Spot\Entity;
use Spot\Entity\Collection;

/**
 * Relation object for HasMany relation
 *
 * @package Spot
 */
class HasMany extends RelationAbstract implements \Countable, \IteratorAggregate, \ArrayAccess
{
    /**
     * Constructor function
     */
    public function __construct(Mapper $mapper, $entityName, $foreignKey, $localKey, $identityValue)
    {
        $this->mapper = $mapper;

        $this->entityName = $entityName;
        $this->foreignKey = $foreignKey;
        $this->localKey = $localKey;

        $this->identityValue = $identityValue;
    }

    /**
     * Set identity values from given collection
     *
     * @param \Spot\Entity\Collection
     */
    public function identityValuesFromCollection(Collection $collection)
    {
        $this->identityValue($collection->resultsIdentities());
    }

    /**
     * Build query object
     *
     * @return \Spot\Query
     */
    protected function buildQuery()
    {
        $foreignMapper = $this->mapper()->getMapper($this->entityName());

        return $foreignMapper->where([$this->foreignKey() => $this->identityValue()]);
    }

    /**
     * Map relation results to original collection of entities
     *
     * @param string Relation name
     * @param Spot\Collection Collection of original entities to map results of query back to
     *
     * @return Spot\Collection
     */
    public function eagerLoadOnCollection($relationName, Collection $collection)
    {
        // Get relation object and change the 'identityValue' to an array
        // of all the identities in the current collection
        $this->identityValuesFromCollection($collection);
        $relationForeignKey = $this->foreignKey();
        $relationEntityKey = $this->entityKey();
        $collectionRelations = $this->query();

        // Divvy up related objects for each entity by foreign key value
        // ex. comment foreignKey 'post_id' will == entity primaryKey value
        $entityRelations = [];
        foreach ($collectionRelations as $relatedEntity) {
            $entityRelations[$relatedEntity->$relationForeignKey][] = $relatedEntity;
        }

        // Set relation collections back on each entity object
        foreach ($collection as $entity) {
            if (isset($entityRelations[$entity->$relationEntityKey])) {
                $entityCollection = new Collection($entityRelations[$entity->$relationEntityKey]);
                $entity->relation($relationName, $entityCollection);
            }
        }

        return $collection;
    }

    /**
     * SPL Countable function
     * Called automatically when attribute is used in a 'count()' function call
     *
     * @return integer
     */
    public function count()
    {
        $results = $this->execute();

        return $results ? count($results) : 0;
    }

    /**
     * SPL IteratorAggregate function
     * Called automatically when attribute is used in a 'foreach' loop
     *
     * @return \Spot\Entity\Collection
     */
    public function getIterator()
    {
        // Load related records for current row
        $data = $this->execute();

        return $data ? $data : [];
    }

    // SPL - ArrayAccess functions
    // ----------------------------------------------
    public function offsetExists($key)
    {
        $this->execute();

        return isset($this->result[$key]);
    }

    public function offsetGet($key)
    {
        $this->execute();

        return $this->result[$key];
    }

    public function offsetSet($key, $value)
    {
        $this->execute();

        if ($key === null) {
            return $this->result[] = $value;
        } else {
            return $this->result[$key] = $value;
        }
    }

    public function offsetUnset($key)
    {
        $this->execute();
        unset($this->result[$key]);
    }
}

redpajama_set_name: RedPajamaGithub


The efficiency of the coronagraph can be measured by comparing images of the same object respectively on-axis and off-axis (Fig. 3). When the star is set off-axis by 4 or 5 times the distance of the first Airy ring (this is about 2 arcsec here) the nulling process no longer applies. Thus as shown in Fig. 3 (image on the left), the photometry of the star is available through the twin images (the summed energy in the twin images is half the energy reaching the beamsplitter). When the star is on-axis a halo of residual energy appears (as shown in Fig. 3). Basically the ratio of the energy in the residual halo to the incident energy determines the extinction capabilities, and this led to the criterion: normalised integrated residual energy. In the following we use this criterion to evaluate the effect of AIC on AO typical images. We also compare two reduction techniques for AIC images and we show how AIC reaches a higher close-sensing capability than does the Lyot coronagraph.
where D is the diameter of the telescope, r0 is the Fried parameter in the visible and pJ is a coefficient depending on J, the index of the last Zernike polynomial corrected.
In Fig. 4 we plot the value of the integrated residual intensity gJversus the factor for a sample of data collected during the observation run. The filled circles stand for gJ measured when adding the whole set of images of a star and the squares stand for gJ measured when adding only selected best images of a star. The selected best images for each target represent between 8% and 15% of the total number of images (in Sect. 4.2 we have explained why the number of images varies from quality-class to another). The best regression lines (whole set and selected set) are also drawn. They yield respective estimates of pJ via the expression: . For the whole set of images we find pJ=0.009 (solid line in Fig. 4) while for the selected images pJ=0.0065 (dashed line in Fig. 4). The theoretical coefficient pJ for BOA is 0.0025. In comparison the AO acts as if it was an AO completely efficient up to radial mode N=7 (36 polynomials). The error bars show the 1 dispersion. Vertically the precision has been estimated taking into account the temporal variation of the extinction and of the total energy collected w0. Horizontally the limitations come mainly from the temporal variation of the r0 during the observations. This variation of r0 is estimated from the BOA measurements taken on each star.
We have to take into account the shape of the halo because it makes the detection capability variable with the location of the image of a companion. In addition we want to visualize the shape of the halo of residual light effectively obtained from the observational data. For that matter we consider the case where AIC has given its best results (here ). In Fig. 5 we show profiles of the normalised flux pertaining respectively to the diffraction pattern of the telescope, central obscuration taken into account (profile a), to the observed image without coronagraph and where AO provides a Strehl Ratio of 90% in K band (profile b, 150 images), to the residual light averaged over the whole set of images (profile c, 1200 images) and to the residual light averaged over the set of selected best images (profile d, 150 out of 1200 images). In Paper I, we suggested that the residual energy is spread over an extended halo, what is effectively found from our data. Unsurprisingly the coronagraphed profile from the selected set is lower and less extended than the profile from the whole set. This change brings in a reduction of the integrated energy from 7.5% to 5.5% that is a lowering factor of 0.73 and reduces the height of the central peak from 2.6% to 2.1% that is a lowering factor of 0.8. Those numerical figures illustrates the interest of a selection process and the presented profiles show where and how the situation is thus improved.
However, we should have observed a depression at the origin in the coronagraphed profiles, as expected from the analysis in Paper I. and this is clearly not confirmed by our profiles from data. This discrepancy between expected and observed profiles is well explained on the theoretical ground by unstabilities affecting OPD (see Paper I) and this situation has been clearly met in our observations, as commented in Sect. 3.2 (specific conditions of observation). In addition, the central hole expected from the theoretical extinction profile can yield full extinction only over an area smaller than the pixel size. Therefore a small fraction of the residual energy is constantly present and prevents the "full darkening" of the central pixel. This also contributes to the observed central peak (but significantly less than OPD variations do).
In this section, to demonstrate more quantitatively the effect of AIC, we compare the magnitude difference ( ) detectable at a given angular resolution with AIC and without AIC. The values correspond to the lower limit of the detectable flux of the companion at the level of 3 . The noise is evaluated by integration of the energy over a patch (Paper I, Close et al. 1998) and this patch is radially moved to determine the variation of the noise level versus the angular distance to the axis. The total flux of the companion is determined by the energy enclosed within the patch centered on each image of the companion. One must notice that the total flux recorded from the companion depends also on the angular separation but the effect of the dependency is visible only close to the star (see Paper I). Roughly AIC diminishes the flux from the companion when this one is closer to the star than 0.18'' while there is practically no attenuation beyond.
In Fig. 6 we show the accessible from raw data without and with AIC (curve a curve b) for typical conditions of turbulence ( ). Substracting the comparison star from the target star profile (both obtained without AIC) yields the curve c. It is apparent from the graph that curve b and c correspond to nearly the same detection sensitivity, what means that working with raw data of AIC is as good as working with "cleaned'' data without AIC. Such a situation shows that processing raw data is necessary to improve the detectivity and ultimately to recover the expected performance.
substracting the mean radial profile (radial process).
Substracting the mean radial profile is possible as soon as the correction by AO is good enough (Strehl Ratio (SR) larger than 50%) what is the case here. In Fig. 7 the is calculated as described in Sect. 5.2. In this figure we show for comparison the detectable from raw data (curve a in Fig. 7). The curves b and c (Fig. 7) shows the accessible respectively for the radial process and for the comparison process (both curves uses the whole set of images available for the target star and the comparison star).
For this configuration (star magnitude, number of frames, exposure time and high noise of the camera), the detectability is limited to beyond 1 arcsec separation. We can note that close to the star the radial process is more efficient than the comparison process. In fact, close to the star the shape of the profile is very similar to the theoretical radial profile (large SR). This leads to a shape of diffraction pattern very similar to the theoretical one. Since this pattern is radial the radial process works well. Besides, the comparison process is not very efficient close to the star because of the possible incidental on-axis pointing shift between the target star and comparison star. This slight angular shift makes the respective mean patterns unequal close to the axis, and limits the efficiency of the comparison process.
In the comparison process used far from the star the detectivity is reduced because noises from target and comparison contribution are added, then decreasing the detectable .
As described in Paper I one specific interest of AIC is its capabilities of detection close to the star. Then to study the efficiency of the AIC close to the star, we calculate the accessible with a selection of the best images of both target and comparison star for the two reduction processes we are interested in (curve d for radial process and curve e for comparison process, both in Fig. 7). When using the selection of best images we keep about 150 images while with the whole set of data we use 900 images.
Using a reduced number of images tends to decrease the detectable far from the star. Conversely, close to the star this is increased because the selection tends to favor images with the highest wavefront quality which results in removing residual energy around the axis first.
We have shown in this section that the selection of images helps increasing detectability of faint structures close to the axis. The use of reference stars does not seem necessary from the averaged radial curves we show. However, when searching for faint structures, one can be misled by fixed speckles mainly coming from aberrations in the wavefront sensor unit or in the optical set-up standing between the AO output beamsplitter and the AIC entrance. Reference sources are then still necessary.
To evaluate the close-sensing capability of AIC we have recorded images of several double stars of various angular separations. In Fig. 8 we present the case of the double star HD 221673 (72 Peg) where the separation is 1.4 times the angular distance of the first Airy ring (0.53 arcsec). From the recorded images (K band) we have estimated the magnitude difference between components at . Hipparcos (ESA 1997) gives a difference of magnitude of (Hipparcos magnitude Hp, visible-near infrared, Martin 1996).
Though, for this star, the magnitude difference to deal with is not very challenging it shows how AIC works. A more challenging star is HD 211073 for which we have to face magnitude differences (Hipparcos Catalogue ESA 1997), and (Ten Brummelaar et al. 1996) and a separation of 0.4'' (Hartkopf et al. 1996). For this star the best results have been obtained with the radial process, because the superimposition of target star and comparison star was not good enough. No faint companion appears clearly but at the position given by Hipparcos Catalogue (ESA 1997) and Hartkopf et al. (1996) two symmetrical bright speckles appear at the level of the residual fixed speckle noise. The difference of magnitude derived from the level of these speckles is . This result is not in agreement with a low mass companion hypothesis derived by Ten Brummelaar et al. (1996).
To show that the AIC can detect companions as close to the star as half of the distance of the first Airy ring we observed the star HD 213310 (5 Lac). The two components of the star are only about 0.11 arcsec appart (one third of the first dark Airy ring). This companion is too close to the star to be resolved by the telescope, but as shown in Paper I, it should be possible to detect this companion with AIC. Figure 9 shows that this possibility is effective and that a sensing of the environment as close as a third of the Airy angular radius has been achieved with AIC. Let us give few comments regarding this point. The image of a companion closer than the first Airy ring appears as two spots symmetrically located at 0.6 times the distance of the first dark Airy ring (Paper I), i.e. 0.22 arcsec here, even if the true separation is different. Actually the true separation governs the apparent flux, not the location of the image. The bright spots (twin images) from HD 213310 effectively appear at the expected location, with a Signal to Noise (SNR) of 5 (Fig. 9). Both the radial and comparison processes give the same result. The intensity ratio between the main star and these spots is 42. From this estimate and taking an average separation of 0.11 arcsec (Hartkopf et al. 1996) a magnitude difference is found. The uncertainty comes from the uncertainty regarding the angular separation and also from the low level of detection (SNR = 5). This magnitude difference is consistent with the spectral types of the 2 stars. Markowitz (1969) gives for these stars M0II+B8V (see also Ginestet et al. 1997 for more references on this star).
Classical Lyot coronagraph can not image a companion so close to the main star. Actually, the masks used in Lyot-type coronagraphs cover 2 to 10 times the distance of the first Airy ring (Malbet 1996) and most of the time they cover 4 or 5 times this distance (Beuzit et al. 1997; Mouillet et al. 1997). As we have shown in this section, AIC can image the faint companion at one third of this distance (first dark Airy ring).


text:
Q: Counting occurences in a column within SQL Oracle This is what I have at the moment in terms of data:

Customer_id
Choco_type

100
Milk

544
Dark

74
White

100
White

544
Milk

82
Crisp

544
White

544
White

What I am looking to achieve is to find out for example is this:

Customer_id
Choco_type
Count

100
Milk
2

544
Dark
1

74
White
1

544
Milk
1

82
Crisp
1

544
White
2

A: Use GROUP BY to aggregate data. In this case you want a count, so...
select  id
       ,chocolate_type
       ,count(*)
from your_table
group by id
        ,chocolate_type
/

If you just want to know how many different types of chocolate each person has bought you would do this:
select  id
       ,count(distinct chocolate_type)
from your_table
group by id
/

You haven't posted your table structure, so I have made some assumptions. You will need to adjust my code examples to fit your actual situation.


If you habitually struggle with worry, this workshop is for you. We'll be looking at, what is worry, why we worry, and what can we do to break free from worry. A deeper understanding of how we get stuck in worrying, reveals insights that can help us on the path to breaking free. The workshop culminates to share with participants 3 steps to breaking free of worry, of which the THIRD step is using tools and strategies (some of which will be covered).
If you're stuck in habitually worrying, have been trying tools & coping to no avail, find out the steps you may be missing at the next Break Free from Worry workshop.


text:
Marilyn Rose Davenport/Morrett
Feb 16, 1929 July 31, 2014
Updated: Aug. 19, 2014, 1:45 p.m.
Marilyn Davenport passed away peacefully in Turlock on July 31st after a brave battle with lung disease. She was born and raised in Minneapolis, MN, then moved to California in 1950 upon marrying Henry Morrett and earning her nursing degree. She worked in hospitals for 19 years and another 10 years as an aerospace industry nurse in southern California. She highly valued her work as an ER nursing supervisor and enjoyed the variety of patients she served. She raised her two beloved sons, Hal and Bryan, mostly as a single mother, following the premature death of Henry in 1961. In 1988, Marilyn married a wonderful man named Harvey Davenport and they settled happily in Nevada City, CA. Upon the loss of Harvey a few years later, she moved to Turlock to be closer to her grandchildren and family.
Wherever she was, Marilyn was always very active in her church; most recently with Hughson United Methodist in their choir and chime choir. She enjoyed keeping the music and robes organized and was an enthusiastic musician. Marilyn was a skilled quilter and enjoyed teaching her grandchildren and others the fabric arts. With her gifted hands, she created many special heirlooms that will be treasured for generations to come. Marilyn liked being a member of the Friends of the Library and played cards with her friends on a regular basis. She passed her love of strategy games on to her grandchildren, teaching each of them how to play chess.
Marilyn was preceded in death by her parents, Clarence and Jeanette Donaldson of Minneapolis; her two husbands, Henry and Harvey; her brother, Forrest and her sister, Gladys; and her sons, Hal and Bryan. She is survived by her sister-in-law, Bette Donaldson, of Fort Collins, CO; her daughter-in-law, Carol Morrett, and three grandchildren Katherine, Zachary, and Michael Morrett, all of Hughson; her step sons, Larry and Lynn Davenport, of California and Maine, respectively, and their families; and her nieces and nephews in Colorado and Minnesota. A celebration of life will take place at 11:00 AM September 6th 2014 at Hughson United Methodist Church, 6th St. and Fox Rd., Hughson, ph. 883-4952.


text:
DG, CSIR launches Compendium of Indian Technologies for Combating COVID-19 to serve as a ready-reference for policy makers, industries, entrepreneurs, startups, MSMEs, research scholars, scientists and others
May 7, 2020 News
by Vipul Dhasmana, Digital Editor, www.dehradunsearchengine.com
A "Compendium of Indian Technologies for Combating COVID-19 (Tracing, Testing and Treating)" prepared by National Research Development Corporation (NRDC) was launched by Dr. Shekhar C. Mande, Director General, CSIR and Secretary, DSIR, Govt. of India at CSIR Headquarters, New Delhi.
The compendium carries information about 200 COVID-19-related Indian technologies, ongoing research activities, technologies available for commercialisation, initiatives and efforts taken by the Government of India, categorised under 3Ts of Tracking, Testing and Treating.
Most of these technologies are proof-of-concept (POC) tested and can help the entrepreneurs to take the product to market faster as they do not have to reinvent the wheel.
Dr. Mande appreciated the initiative of NRDC for bringing out the Compendium of Indian Technologies for Combating COVID-19 "as it is very timely and would benefit the MSMEs, Startups and the public at large".
Dr. H. Purushotham, CMD, NRDC, informed that team-NRDC has made an attempt to compile most relevant and emerging indigenously developed technological innovations, including those which are at research stage, to fight COVID-19 for the benefit of all stakeholders and this compendium will serve as a ready-reference for policy makers, industries, entrepreneurs, startups, MSMEs, research scholars, scientists and others. He also informed that several of the technologies compiled are approved by ICMR.
The information presented in the compendium is sourced from various government bodies and premier academic institutions including Department of Science and Technology (DST), Department of Biotechnology (DBT), Indian Council for Medical Research (ICMR), Ministry of Electronics and Information Technology (MeitY), Council of Scientific and Industrial Research (CSIR), Defence Research and Development Organisation (DRDO), Indian Institute(s) of Technology (IITs), Science and Engineering Research Board (SERB), Technology Development Board (TDB), National Innovation Foundation (NIF), Startup India and All India Council for Technical Education (AICTE), Sree Chitra Tirunal Institute for Medical Sciences and Technology (SCTIMST),and Indian Institute of Science (IISc).
For more information, including transfer of technology, one may reach NRDC, an enterprise of Department of Scientific and Industrial Research (DSIR), Ministry of Science & Technology, Govt.of India at cmdnrdc@nrdc.in.