Microsoft has fixed a problem with a Windows 10 update that inadvertently deleted user documents. Oddly the problem had been highlighted in early testing, but doesn't seem to have been fixed.
The issue received widespread attention when the October 2018 Update started rolling out to the wider public. That's the second of the two big annual updates that bring new features to Windows 10, a system that replaces the old set-up of having service packs rolled out every few years.
Some users discovered that after the update, everything they had stored in their Documents folders had disappeared. Some were able to restore the files using specialist recovery software, but in many cases if the user didn't have a backup, the files were gone forever.
It appears that the bug affected users who have redirected standard folders such as "Desktop", "Documents" or "Downloads" to another location, rather than storing these folders (by default) on the C drive.
For example, on some machines the C drive might be a solid state drive (SSD) to store Windows, while a traditional drive (the D drive) is used for storing user data. In this case, the Desktop, Documents and Downloads may have been stored on the D drive (but only if it was configured by the user to do so).
The unintended deletion came from two separate mistakes by Microsoft. The first came earlier this year when it discovered the redirection was sometimes creating duplicate folders that had the same name but were empty.
The second mistake came with the recent update which was designed to automatically delete the duplicate folders but, with some set-ups, was actually deleting the folders which contained the files.
Do you know anyone who's been affected by this problem? Do you backup these folders (or your entire hard drive) as a matter of habit? Are you surprised Microsoft didn't fix the issue before rolling out the update?
Give your article title writer a smack upside the head!
What does that title say? That the update is fubar, don't install it. So then in the very first line of the article you contradict the title!
Microsoft has fixed a problem with a Windows 10 update that inadvertently deleted user documents.
This contradiction makes the article seem like click bait.
Don't say it was just an "oops". I've seen too much of this trend of misleading article titles in the computer industry.
Sorry, but I disagree. The title does not say "don't install the update" - it says that the update deleted user data; in this case, it happened to multiple users, hence the word "deletes" was used. So to say that the "Windows 10 October Update Deletes User Documents" is in fact correct - even if it happened a few days ago, because we have reports from multiple users stating exactly that. Microsoft also issued a fix - that is also a fact; mentioning it in first line should not matter. This was not meant as click bait. Take it for what you will.
It seems this is fixed. I hope it is because Dennis helped me redirect my personal files to an SSD d drive a couple years ago. Just in case it isn't fixed though, he also set up Macrium image backups for me, so worse case, I would be able to restore a deleted Documents folder from that. Because of those backups, I assume I am also well protected from the growing threat of ransomware.
You will be protected from ransomware IF your backup drive is physically disconnected from your PC when not backing up or at least turned off with the auto wake on LAN feature disabled if it exists.
Don't click "Check for Updates"
The best advice, it seems, is never click "Check for updates". If you do this, you are a guinea pig.
I had an interesting thing happen to me with the Oct update, I can not switch from my speakers to my headphones on my desktop. I have to go into my settings and change it back and forth from speakers to headphones, I can control the volume of the device from the taskbar but I can't change the devices. Is it possible to get this back as before?
Windows 10 'Deleting User Documents'... surely this is a 'Major Flaw' rather than a 'Bug' let alone a 'Glitch' as described by Microsft ... Not only unnerving for anyone of using Win10, let alone thinking of upgrading to Win 10 .. or should than be downgrading to a huge, intrusive, unreliable and dangerous OS.


Jarod Lamantagne - Computer Press Releases - Submit your news and press release. Computer / Internet / IT Industry.
Sales Training... Fact or perhaps Fiction?
When Accidents Happen in the Workplace: Are Companies Responsible?


text:
Q: Updating Todo list via mobx with react and typescript Hi guys i was just trying out mobx today and made a Todo List with it, the problem is the list isn't updating here after the item is removed from the list even though i had made observer and observable. You can also directly check my code here at CodeSanbox .It's a basic todo app
Store.js
import { observable, action, computed, reaction } from "mobx"
import { createContext } from "react"
import { v4 as uuidv4 } from 'uuid';
export interface Todo {
  id?: string;
  title: string;
  completed: boolean;
}

class TodoStore {
  constructor() {
    reaction(() => this.todos, _ => console.log(this.todos.length))
  }

  @observable todos: Todo[] = [
    { id: uuidv4(), title: "Item #1", completed: false },
    { id: uuidv4(), title: "Item #2", completed: false },
    { id: uuidv4(), title: "Item #3", completed: false },
    { id: uuidv4(), title: "Item #4", completed: false },
    { id: uuidv4(), title: "Item #5", completed: true },
    { id: uuidv4(), title: "Item #6", completed: false },
  ]

  @action addTodo = (todo: Todo) => {
    this.todos.push({ ...todo, id: uuidv4() })
  }

  @action toggleTodo = (id: string) => {
    this.todos = this.todos.map(todo => {
      if (todo.id === id) {
        return {
          ...todo,
          completed: !todo.completed,
        }
      }
      return todo
    })
  }

  @action removeTodo = (id: string) => {
      console.log(id)
    this.todos = this.todos.filter(todo => todo.id !== id)
    console.log(this.todos)
  }

  @computed get info() {
    return {
      total: this.todos.length,
      completed: this.todos.filter(todo => todo.completed).length,
      notCompleted: this.todos.filter(todo => !todo.completed).length,
    }
  }
}

export default createContext(new TodoStore())

TodoList.js
import React, { useContext } from "react";
import TodoStore from "../stores/TodoStore";
import { observer } from "mobx-react-lite";

const TodoList = () => {
  const todoStore = useContext(TodoStore);
  const { todos, toggleTodo, removeTodo } = todoStore;
  return (
    <>

              Title
              Completed?
              Actions

            {todos.map(todo => (

                {todo.title}
                {todo.completed ? "✅" : ""}

                  <button
                    className="btn btn-sm btn-info"
                    onClick={_ => toggleTodo(todo.id!)}
                  >
                    Toggle
                  </button>
                  <button
                    className="btn btn-sm btn-danger"
                    onClick={_ => removeTodo(todo.id!)}
                  >
                    Remove
                  </button>

            ))}

    </>
  );
};

export default observer(TodoList);

So as i click remove button, the action "removeTodo" gets fired up the todo is removed from the list i can check that on console but it istn't updating in the UI part

A: With Mobx v6 simply setting decorators is not enough anymore. You also need to call makeObservable or makeAutoObservable in the class constructor.
  import { observable, action, computed, reaction,makeAutoObservable } from "mobx"

  constructor() {
    makeAutoObservable(this)
    reaction(() => this.todos, _ => console.log(this.todos.length))
  }

Sandbox demo

redpajama_set_name: RedPajamaStackExchange


Our Volkswagen dealer in NH is proud to serve shoppers in the Nashua and Merrimack area. We offer new and used Volkswagen sales, service, and parts in an environment that is so welcoming that it is one-of-a-kind. The professional staff that makes our dealership run are dedicated to customer satisfaction, and we will always take the time to help you have the best possible car buying or maintaining experience.
Whether you are looking for a budget-friendly Volkswagen Jetta or a capable Volkswagen Tiguan, we've got the model for you at our New Hampshire dealership serving Nashua, Merrimack and surrounding areas. In fact, we carry the entire lineup of VW cars in our lot, so chances are that we have exactly what you are looking for. We even have a wide variety of dependable used cars for you to consider during your search. These are perfect for those looking for performance and style with a lower price point.
We know that there are many locations to choose from in New Hampshire, that is why we work hard to earn your business. Pay us a visit and we will prove to you why we are set apart from the rest!


A zoo that is not just for kids.
Living Desert Zoo and Gardens, formerly the Living Desert Museum, is a botanical garden and a zoo all in one. It's located at the top of the hill in Palm Desert, about 20 minutes south of Palm Springs in Riverside County.
If you are coming from Los Angeles take the 10 freeway, exit at Palm Springs, drive through town, and make a right on Pines to Palm Highway (#74).
If your near Lake Elsinore you can take the 74 highway over the mountains and the zoo is just a few minutes off the highway.
The facility was established in 1970 as a 360-acre wilderness preserve by the Palm Springs Desert Museum. They started with only a fox, tortoises, lizards, and two sheep. In the mid 1970's the area was rebuilt, and additional facilities were added, including greenhouses, model trains, and improved gardens. New animals included: gazelles, mountain lions, bobcats, badgers, cheetahs, warthogs, hyenas, giraffes and ostriches.
The Living Desert now provides a large variety of interactive attractions, entertaining shows, and educational shows. Camel Rides, Giraffe feedings, and other animal encounters are the must-see events. It's important to know that The Living Desert is a private zoo that operates as a non-profit.
Most people that attend the zoo are from out of town, and are in town for the weekend or longer vacation.
There are so many wonderful places to stay in Palm Desert, Rancho Mirage, or Palm Springs. The areas offers some of the most luxurious hotels, moderatly priced hotels and motels, themed motels, and of course there are many homes for rent anytime of the year.
Often people with large families or groups chose to travel by Party Bus to and from the various events of the day. This way they can pack the bus with all their needs for the day and not have to rent multiple cars.
If you are in need of any transportation in Riverside county, contact us for assistance.


Rochelle Rao is an Indian model and anchor. Rochelle was awarded the crown of "Femina Miss India International" in 2012. She has also appeared in Kingfisher Calendar several times. Rochelle joined Bigboss 9 as a participant in 2015. Rochelle Rao participated in the fifth Pantaloons Femina Miss India South Pageant in January 2012, where she was the first runner up.
After that she participated in "Femina Miss India" in 2012 and won the title. She also won three subtitles, "Miss glamorous Diva", "Miss Ramp Walk", "Miss Body Beautiful" etc.
In 2012, she represented India in Miss International 2012 pageant in Okinawa, Japan, where she was ranked ninth from 68 countries. In 2012, she was crowned for "Femina Miss India International". After that she was also a hosted "Indian Premier League Season 6".
Rochelle Rao is at #22 in this list.


text:
Michaël Belluau est stagiaire post-doctoral dans le laboratoire de Christian Messier et Alain Paquette et coordonnateur scientifique du réseau IDENT.
Laforest-Lapointe, I., Messier, C., Kembel, S.W. (2016) Tree phyllosphere bacterial communities: Exploring the magnitude of intra- and inter-individual variation among host species. PeerJ, 2016(8). (Scopus )
Background. The diversity and composition of the microbial community of tree leaves (the phyllosphere) varies among trees and host species and along spatial, temporal, and environmental gradients. Phyllosphere community variation within the canopy of an individual tree exists but the importance of this variation relative to amongtree and among-species variation is poorly understood. Sampling techniques employed for phyllosphere studies include picking leaves from one canopy location to mixing randomly selected leaves from throughout the canopy. In this context, our goal was to characterize the relative importance of intra-individual variation in phyllosphere communities across multiple species, and compare this variation to inter-individual and interspecific variation of phyllosphere epiphytic bacterial communities in a natural temperate forest in Quebec, Canada. Methods. We targeted five dominant temperate forest tree species including angiosperms and gymnosperms: Acer saccharum, Acer rubrum, Betula papyrifera, Abies balsamea and Picea glauca. For one randomly selected tree of each species, we sampled microbial communities at six distinct canopy locations: bottom-canopy (1-2mheight), the four cardinal points of mid-canopy (2-4 m height), and the top-canopy (4-6 m height). We also collected bottom-canopy leaves from five additional trees from each species. Results. Based on an analysis of bacterial community structure measured via Illumina sequencing of the bacterial 16S gene, we demonstrate that 65% of the intra-individual variation in leaf bacterial community structure could be attributed to the effect of interindividual and inter-specific differences while the effect of canopy location was not significant. In comparison, host species identity explains 47% of inter-individual and inter-specific variation in leaf bacterial community structure followed by individual identity (32%) and canopy location (6%). Discussion. Our results suggest that individual samples from consistent positions within the tree canopy from multiple individuals per species can be used to accurately quantify variation in phyllosphere bacterial community structure. However, the considerable amount of intra-individual variation within a tree canopy ask for a better understanding of how changes in leaf characteristics and local abiotic conditions drive spatial variation in the phyllosphere microbiome. © 2016 Laforest-Lapointe et al.
TITLE = { Tree phyllosphere bacterial communities: Exploring the magnitude of intra- and inter-individual variation among host species },
JOURNAL = { PeerJ },
VOLUME = { 2016 },
ABSTRACT = { Background. The diversity and composition of the microbial community of tree leaves (the phyllosphere) varies among trees and host species and along spatial, temporal, and environmental gradients. Phyllosphere community variation within the canopy of an individual tree exists but the importance of this variation relative to amongtree and among-species variation is poorly understood. Sampling techniques employed for phyllosphere studies include picking leaves from one canopy location to mixing randomly selected leaves from throughout the canopy. In this context, our goal was to characterize the relative importance of intra-individual variation in phyllosphere communities across multiple species, and compare this variation to inter-individual and interspecific variation of phyllosphere epiphytic bacterial communities in a natural temperate forest in Quebec, Canada. Methods. We targeted five dominant temperate forest tree species including angiosperms and gymnosperms: Acer saccharum, Acer rubrum, Betula papyrifera, Abies balsamea and Picea glauca. For one randomly selected tree of each species, we sampled microbial communities at six distinct canopy locations: bottom-canopy (1-2mheight), the four cardinal points of mid-canopy (2-4 m height), and the top-canopy (4-6 m height). We also collected bottom-canopy leaves from five additional trees from each species. Results. Based on an analysis of bacterial community structure measured via Illumina sequencing of the bacterial 16S gene, we demonstrate that 65% of the intra-individual variation in leaf bacterial community structure could be attributed to the effect of interindividual and inter-specific differences while the effect of canopy location was not significant. In comparison, host species identity explains 47% of inter-individual and inter-specific variation in leaf bacterial community structure followed by individual identity (32%) and canopy location (6%). Discussion. Our results suggest that individual samples from consistent positions within the tree canopy from multiple individuals per species can be used to accurately quantify variation in phyllosphere bacterial community structure. However, the considerable amount of intra-individual variation within a tree canopy ask for a better understanding of how changes in leaf characteristics and local abiotic conditions drive spatial variation in the phyllosphere microbiome. © 2016 Laforest-Lapointe et al. },
ART_NUMBER = { e2367 },
AUTHOR_KEYWORDS = { Bioindicator; Inter-individual variation; Interspecific variation; Intraindividual variation; Microbiome; Phyllosphere; Plant-bacteria interaction; Temperate forest },
DOI = { 10.7717/PEERJ.2367 },
URL = { https://www.scopus.com/inward/record.uri?eid=2-s2.0-84992051099&partnerID=40&md5=70d670d4ad690e62bb2c3d2e0bfe48f8 },

redpajama_set_name: RedPajamaCommonCrawl


The devil has been collecting souls for 200,000 years and still hasn't found his soulmate, but *raises glass* I'm glad you found yours. Congrats Tina and John.
Ran into a casual high school acquaintance I haven't seen in 10 years on NYC streets. Without saying a word she gives me a high five and keeps walking. Be like her.
I never know if the pain in my chest is from anxiety or french fries.
The abnormally high temperatures will continue through the end of the planet.
I love that "take out" means food, dating, and murder.
Me: was. Scooby doo. neutered.
school fundraisers were wild lol you would sell 100 dollars of merchandise and they'd give you a keychain. you. didn't. even. own. keys.
I've been hitting "remind me tomorrow" on a computer update for the last 68 years.


text:
Source: Tavon Austin, Rams agree on 4-year, $42 million extension
By Alden Gonzalez
DENVER -- The Los Angeles Rams locked up dynamic wide receiver Tavon Austin to a four-year, $42 million extension Saturday, a source told ESPN NFL Insider Adam Schefter.
The deal, which keeps Austin with the Rams through 2021, includes $30 million guaranteed, with incentives that could elevate the deal's value to $52 million, the source told Schefter.
Austin significantly increased his production in 2015, setting career highs in receptions (52), yards from scrimmage (907) and touchdowns (10), prompting the Rams to trigger his fifth-year option for 2017.
Austin, the eighth overall selection in the 2013 draft, carries a base salary of $2,143,773 in 2016 and is set to make $12,268,000 in 2017.
His role is expected to increase this season -- in the passing game and out of the backfield -- under Rob Boras and new passing game coordinator Mike Groh. Austin will also continue to return punts.
sportsespnextensionnflcontractlos angeles ramstavon austin


Sorry for missing all this time! I couldn't believe it was an entire week ago since my last post.
After getting things together at my childhood hometown, I drove back to my grown-up city with my parents in tow, where we proceeded to do more wedding things, cook ridiculous amounts of food, and spend too much time at stores, whether it was the fun kind (real shopping) or the "eh" kind (groceries).
Anyway, I decided to try and make my friend's bridal shower invitations extra special, so I took my best stab at calligraphy that my hand/attention span would allow. I'm pretty insanely happy with the result, considering my first hundred attempts were futile. I'm somewhat determined to become much more adept at the whole calligraphy thing someday.
Lovely penmanship! But I would not expect anything less!!!
Thanks Naomi! You're a sweetheart.


text:
aerospace engineer salary california
Analyzes results of stress tests on various craft and missile parts and conducts research to determine flight characteristics. Competitive salary. Being an Aerospace Engineer I may concentrate in a single aerospace discipline such as flight mechanics, guidance, and control systems, propulsion systems, robotics, or aerodynamics. The average salary for an Aerospace Engineer in Los Angeles, California is $89,338. 1,094 of the 6,987 Aerospace & Aeronautical Engineering degrees awarded last year were given by schools in California. An Aerospace Engineer in your area makes on average $51 per hour, or $1.17 (2%) more than the national average hourly salary of $49.44. Not the job you're looking for? Average salaries can vary and range from $42,563 to $191,439. Individualize employee pay based on unique job requirements and personal qualifications. Verified employers. Salaries can vary considerably depending on whether the employer is a private, government, or educational institution. Work is closely managed. Aerospace Engineer Jobs in Visalia, California&Aerospace Engineer job openings in Visalia, California. CPI AEROSTRUCTURES INC, DORIAN LPG LTD, Howmet Aerospace Inc. Aerospace Engineer I Salaries by Percentile, Aerospace Engineer I's Average Annual Base Salary. The Greater Los Angeles Area and the San Francisco Bay Area are the nation's second and fifth most populous urban regions, with 18.7 million and 9.7 million residents respectively. Salaries for Related Job Titles. Entry Level Salary for Aerospace Engineers. Verified employers. No data is available based on your input. The range for our most popular Aerospace Engineer positions (listed below) typically falls between $64,380 and $157,275. The average Aerospace Engineer I salary in California is $84,661 as of November 25, 2020, but the range typically falls between $76,519 and $90,561. Aerospace engineers design primarily aircraft, spacecraft, satellites, and missiles. The average salaries of aerospace engineers in 10 major industry sectors are shown in Table 2. 2021 Best Colleges with Aerospace Engineering Degrees in California About this List Explore the best colleges with aerospace engineering degrees. Search aerospace engineer jobs in California. How do aerospace engineer salaries compare to similar careers. Aerospace engineering and mechanical engineering are the most common majors for people with jobs as aerospace engineers. Aerospace Engineer salaries vary drastically based on experience, skills, gender, or location. The average salary for aerospace engineers in California is around $122,960 per year. Additionally, Aerospace Engineer I typically reports to a supervisor or manager. Brisbane, CA, PDS Tech, Inc. - Salaries range from 64,100 USD (lowest) to 199,000 USD (highest).. The state capital is Sacramento. Salary estimation for Aerospace Engineer I at companies like : Aerospace Design Engineer $77K. In addition, they earn an average bonus of $4,240. Salary estimates are based on 1,125 salaries submitted anonymously to Glassdoor by Aerospace Engineer employees. Compensation data tools, salary structures, surveys and benchmarks. Salary ranges can vary widely depending on the city and many other important factors, including education, certifications, additional skills, the number of years you have spent in your profession. Browse job listings for Aerospace Engineer in Visalia, California or refine your search by selecting a specific city. The average Aerospace Engineer II salary in California is $104,920 as of October 28, 2020, but the range typically falls between $93,223 and $116,052. The average salary for "aerospace engineer" ranges from approximately $62,633 per year for Controls Engineer to $131,570 per year for Senior System Engineer. Full-time, temporary, and part-time jobs. Find the aerospace engineering … The U.S. is known for producing some of the best engineers in the world, who gain top degrees at some of the most prestigious American universities. The average Aerospace Engineer salary in the United States is $110,828 as of October 28, 2020. ...More. On average, they make less than software engineers but more than To be an Aerospace Engineer I typically requires 0-2 years of related experience. Other states where you may have better chances of earning an above-average salary as an aerospace engineer are Texas, Colorado, and California. Average Salary: $103,720 Expected Lifetime Earnings: $4,330,000. The Aerospace Engineer I works on projects/matters of limited complexity in a support role. 9 LinkedIn members shared this salary. Salary ranges can vary widely depending on the city and many other important factors, including education, certifications, additional skills, the number of years you have spent in your profession. Salaries typically start from $75,300 and go up to $200,785. Average Aerospace Engineer Salary By Location. Read more from. Wages typically start from $75,300 and go up to $200,786. The average salary for an entry level Aerospace Engineer is $69,041. Get the right aerospace engineer job with company ratings & salaries. Full-time, temporary, and part-time jobs. 78% above national average ● Updated in 2018. The average Aerospace Engineer I salary in California is $84,518 as of October 28, 2020, but the range typically falls between $76,396 and $90,414. Analyze the market and your qualifications to negotiate your salary with confidence. A person working as an Aerospace Engineer in United States typically earns around 128,000 USD per year. An experienced Aerospace Engineer makes about $112,143 per year. Visit PayScale to research aerospace engineer salaries by city, experience, skill, employer and more. California is a state in the Pacific Region of the United States. Los Angeles is California's most populous city, and the country's second most populous, after New York City. See user submitted job responsibilities for Aerospace Engineer I. Salary.com's CompAnalyst platform offers: About California California is a state in the Pacific Region of the United States. Support simulation analysis and development for composite part manufacturing and structural performance. The 68,510 aerospace engineers in the U.S. earn an average salary of $112,010 per year or $58.85 per hour according to the Bureau of Labor Statistics. Salaries estimates are based on 174 salaries submitted anonymously to Glassdoor by Aerospace Engineer employees in Los Angeles, CA. Source: Wikipedia (as of 04/11/2019). How to Apply for a Job During the Coronavirus Pandemic, Supplier Management Solutions, LLC - Throughout the U.S., the average salary for an aerospace engineer is roughly $104,176 per year, which boils down to $50.09 per hour. Anaheim, CA, Midcom - This salary estimate is based on salaries at similar … Aerospace engineers in West Virginia and Wisconsin, on the other hand, reported an average annual wage that was below the $90,000 mark. Requires a bachelor's degree. With 39.6 million residents, California is the most populous U.S. state and the third-largest by area. In addition, they test prototypes to make sure that they function according to design. The highest paying industry sector for aerospace engineers occupations is the federal, state, and local government sector with an annual salary $118,050. PayScale presents a typical early career salary for aerospace engineers as $68,700 per year, and the average mid-career pay as $113,900 per year. SkillsetGroup - Professional Staffing Solutions -. This is 25% higher (+$22,162) than the average aerospace engineer salary in the United States. The median salary of a vice president of engineering … 3,131 open jobs for aerospace engineer. Get the latest market price for benchmark jobs and jobs in your industry. Apply to System Engineer, Avionics Engineer, Mechanical Designer and more! Competitive salary. Search and apply for the latest Aerospace engineer (program manager) jobs in California. Aerospace engineers earn about the same as related careers in California. We note that the salaries vary considerably within different industry sectors. Get hired! According to the BLS, aerospace engineers made salaries of $108,750 or more working the states of California, Alabama, Virginia and Maryland. A new graduate with a degree in aerospace engineering can expect a starting salary in the range of $60,000 or more¹. Aerospace Engineering. The national average salary for a Aerospace Engineer is $79,714 in United States. With cutbacks in space exploration the Department of Labor expects that the need for aerospace engineers will grow at 2% over the next few years, a slower pace than the average job market. What are the average salary ranges for jobs in the Aerospace and Defense?There are 152 jobs in Aerospace and Defense category. Wages typically start from $68,289 and go up to $176,573.. 78 % above national average Updated in 2019 Search more salaries here: Aerospace Engineer I Salaries with a Bachelor's Degree, Aerospace Engineer I Salaries with a Master's Degree or MBA, Aerospace Engineer I Salaries with a JD, MD, PhD or Equivalent, 10th Percentile Aerospace Engineer I Salary, 25th Percentile Aerospace Engineer I Salary, 50th Percentile Aerospace Engineer I Salary, 75th Percentile Aerospace Engineer I Salary, 90th Percentile Aerospace Engineer I Salary, Detailed skills and competency reports for specific positions. ranks number 1 out of 50 states nationwide for Aerospace Engineer salaries. Visit PayScale to research aerospace engineer salaries by city, experience, skill, employer and more.
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There will be no Islamic School on November 25th and 26th in the masjid. This is due to the program and visiting scholars we will be having in the masjid that weekend. School will resume normally the following weekend.
Please note that Islamic weekend school for girls starts on Saturdays at 10 AM. For boys it is on Sunday at 9AM. The earlier time is due to the fact there is only one teacher, the Imam for all the boys. The community needs volunteer instructors for the school. If you are interested in volunteering for either the boys or girls, please contact the Imam. You must be able to read and write in the Arabic language.
The khutbah on November 10 will start at 12:20PM due to the time change last weekend.


Holdings: Postcard, To: Frida Heilshorn From: Gerhard Hauschild, July 29, 1915.
Postcard, To: Frida Heilshorn From: Gerhard Hauschild, July 29, 1915.
1 photo postcard . Collected in album: Postcards sent to Frida Heilshorn from Gerhard Hauschild during World War I. Photograph of 4 German soldiers in barracks.


Serena Dyer, on stage with her father Dr. Wayne Dyer, discusses what it was like growing up with Dr. Wayne Dyer as a father and how living the 10 Secrets for Success and Inner Peace effected their day to day lives.
In her new book, Don't Die with the Music Still in You, Serena sets out to explain what it was like to grow up with spiritual parents. She touches upon all ten of her dad's original secrets, imparting her own experiences with them and detailing how they have affected the way she approaches various situations in life. She shares stories, struggles, and triumphs-and Wayne, in turn, contributes his own perspective.


text:
Jose Aldo sees nothing controversial about UFC 251 title shot: 'I deserve to be here'
By Danny Segura, John Morgan July 8, 2020 3:30 pm
By Danny Segura and John Morgan | July 8, 2020 3:30 pm
ABU DHABI – Jose Aldo sees nothing controversial about his title shot at UFC 251.
Aldo, the former UFC featherweight champion, fights Petr Yan for the vacant bantamweight title in the co-main event Saturday. Aldo (28-6 MMA, 10-5 UFC) is coming off an unsuccessful bantamweight debut where he lost a split decision to Marlon Moraes in December. Although it was a controversial defeat, many didn't agree with the merits of Aldo's title shot as other top contenders coming off wins were available.
Aldo, the third fighter in UFC history to fight for a title off two consecutive non-title losses, is not concerned with the critics, though. He firmly believes he should be fighting for the vacant belt.
"I'm not worried about that," Jose Aldo told MMA Junkie through a translator during a media scrum Wednesday. "I won that fight. Even the judges afterwards said they agree with me. I beat Marlon, who's the No. 1 contender, so it doesn't bother me at all. I deserve to be here."
Video: UFC 251 'Countdown' for Jose Aldo vs. Petr Yan
Jose Aldo: Weight cut to 135 pounds 'has actually been a lot easier than it was at 145'
Whether or not the title shot was warranted, there's no denying Aldo's achievements and impact on the sport. Despite his success, the Brazilian is not ready to reminisce on his accolades as he still has work to do.
"It was always a dream of mine to be a champ in two different divisions," Aldo said. "At first, I thought I was going to have to go up to lightweight, but now I'm down to bantamweight. I really do think one day when I stop fighting I'm going to be able to look back and see everything that I did."
Aldo feels confident in his second drop to 135 pounds and, as of now, has no plans of returning to featherweight. All of his focus is on bantamweight.
Breaking, Jose Aldo, UFC 251, News, UFC, Videos


text:
Danny Reed
Photo by Dave Adamson on Unsplash
COLUMBUS, Ohio – Rooting for Ohio-based NFL teams typically leads to stress and anxiety—but could relief soon be on the way?
As funny as it may sound, the Ohio Medical Board will soon issue an actual ruling on whether or not simply being a fan of the Cleveland Browns or Cincinnati Bengals is a qualifying condition for medical cannabis. Residents are able to submit petitions for additional qualifying conditions for cannabis use. Most of the twenty-eight petitions received by the Ohio Medical Board were related to serious medical conditions such as pain, opioid dependence, and autism. However, there was one proposed condition that stood out, being a fan of the Browns or Bengals.
The Browns and Bengals have combined for zero playoff wins in the past twenty-five years and are routinely among the worst teams in the league. Unfortunately, fans are not likely to receive an off the field win anytime soon either. Even when it comes to serious conditions, Ohio regulators have been hesitant to add any new qualifying conditions for medicinal cannabis. Last year, approximately 100 petitions were submitted, with none of them being approved by the board.
According to the medical board's website, successful petitions must include "relevant medical or scientific evidence" and "information from experts who specialize in the study of the disease or condition." While disgruntled fans may think it's a compelling case, we anticipate the board will cry foul.
"The Medical Board received twenty-eight petitions for potential new qualifying conditions during the 2019 petition window. Medical Board's Medical Marijuana Committee is anticipated to meet February 12," the board said on its website. "At that meeting, the committee will decide which petitions will be considered. A final vote on new qualifying conditions is expected this summer."
The NFL has come under intense scrutiny for its substance use policy. Although THC and CBD have become popular for pain relief among current and former athletes, the NFL still has a zero-tolerance cannabis policy. Although it is unlikely Ohio regulators would approve fandom as a qualifying condition this season, it's still possible that NFL fans will be allowed to medicate for stress related to watching football before players can medicate for pain related to playing football.
The next petition period will be November 1 to December 31, 2020.
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by Demetris	 January 1, 2019 September 23, 2019
The graph objective is to understand which factors may have driven shot success by LeBron James and Stephen Curry during the 2014/2015 NBA season.
There are several factors that could determine the success of a shot in a basketball game. Distant shots could qualify for a 3-pointer but are less likely to be made. The distance of 2-pointer shots may be closer but the nearer you get to the hoop the more likely you are to be guarded more closely. The shot clock plays an important role, with less seconds left on the clock forcing a less calculated shot. The defender distance is clearly also a factor. Touch time and dribbles can be influential too. Many coaches advocate (at least in Greece where I learnt the game) that the best shot is taken from a stationary position, following a pass and a small step to balance the shot. Dribbling too much can throw you off balance. All of the above, of course, are not necessarily the case for professionals who specialise in niche situations.
The data is sourced from the NBA API.
I reduce the data to just two players: LeBron James and Stephen Curry, and the 2014/2015 season. I also remove certain extreme values that indicate extraordinary shooting situations such as taking shot with distance more than 30 feet and having no defendant in a proximity of 11 feet.
The analysis looks at the variation of a number of potential factors with differing scales, e.g. shot clock measured in seconds, dribbles measured in numbers, shot distance measured in feet. Therefore, a key data management step is to standardise the range of variation of these variables.
Given my choice of using parallel coordinates to contrast this variation (as I explain below), it is best to standardise by dividing each variable through its maximum value.
For each basketball player, I plan to contrast the variation of six variables: shot success, shot clock, touch time, dribbles, defender distance, shot distance. Shot success is a binary variable, but the rest are quantitative interval-ratio variables.
Therefore, I need a five dimensional coordinate system for the quantitative variables that could be encoded twice for the binary classification. I choose to use the parallel coordinate system, whereby the scale of the five dimensions will be shown parallel to each other. This is why it is best to standardise the range of the scale, as explained just above.
A parallel coordinate system encodes the point visual implantations on the parallel axes and then connects the points using lines across the axes. In this way, the points encode the location on the scale, from smallest to largest, and the lines encode the direction of transition from one variable to the next.
The binary classes of shots made versus shots missed is encoded using the colour retinal variable. I choose to encode the two classes using a bight yellow hue and a bright blue hue.
There are close to 1,000 shots taken by each player which means that there will be 1,000 lines intersecting hence the need to be drawn very thin. The thinner the line the more difficult is to be seen using unsaturated colours. Therefore, saturated colours compensate for the loss of thickness (i.e. the size retinal variable).
The colour retinal variable is internally identified using a legend that is placed inside the plot region to save space. The legend also identifies the number of shots made and missed by each player.
The parallel axes scales are externally identified as going from Zero to Max. I am not interested in identifying detailed scales for two reasons: the graph is not meant to facilitate a detailed table look-up, and everyone knows what is Zero and what is Max for shot clock, touch time, dribbles, defender distance and shot distance.
External identification also includes a title describing the graph objective and a note acknowledging the data source.
Given the many parallel axes it is important to maintain a wide aspect ratio to allow for easier decoding of the many sloping lines.
Information from fully saturated colours cannot be easily perceived in white or bright color backgrounds. So it is important to switch to dark background.
Here is my proposed solution, first for LeBron James:
I decode first the positions of the point implantations on the parallel axes. The shots taken by LeBron James have a great deal of variation in terms of shot clock and shot distance, but he mostly maintains a low touch time and number of dribbles. In terms of shot success, he seems to make more shots with more time on the clock and shorter shot distance, while surprisingly the defender distance does not seem to be play a defining role.
Next, I decode the directions and density of the line implantations connecting the points. Many shots are made with more time on the clock, low touch time, low number of dribbles, and medium defender distance, and almost half are very close to the basket and the other half far away.
Here is how this looks for Stephen Curry:
It is remarkable that the two players have nearly identical number of shots made and missed, and the patterns in the parallel coordinates graph look remarkably similar.
The data suggests similar patterns for Stephen Curry as with LeBron James, but with the key difference that Stephen Curry has a much more tight variation in shot clock, touch time and dribbles. Specifically, Stephen Curry likes to take shots with more time on the clock whereas LeBron James also takes last second many shots. It is also surprising (to me at least), to see that Stephen Curry, although being a point guard, he keeps the ball much less than LeBron James.
Download the Stata code for reproducing this analysis: nba.do
Demetris Christodoulou
Tags: Basketball, Dribbles, LeBron James, National Basketball Association, NBA, Shot distance, Shots made, Shots missed, Stephen Curry, Touch time
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FAMILY SCIENCE PROJECT TOPICS AND MATERIALS
PERCEIVED FAMILY SUPPORT AND SELF CARE PRACTICES AMONG WOMEN OF MENOPAUSAL AGEGROUP ATTENDING GENERAL OUTPATIENT CLINIC, FEDERAL MEDICAL CENTRE, OWO.
ladychampionz January 13, 2022 FAMILY SCIENCE PROJECT TOPICS AND MATERIALS, PROJECT TOPICS No Comments
: 100 Pages
Menopause is a major burden and a daunting challenge among women. The beneficial effect of family support in overall health promotion and care of the patient has been documented. There is virtually no information on integrated health care among Nigerian menopausal women especially in areas of family support, self- care practices and other health related quality of life. Therefore this study was conducted to investigate the role of perceived family support and self-care in women of menopausal age group attending the GOP clinic, Federal Medical Centre Owo.
This was a descriptive cross-sectional hospital based study which utilized systematic sampling technique to select 404 women within ages 40-60 years who attended General Outpatient Clinic Federal Medical Centre Owo. A pre-tested, semi-structured interviewer administered questionnaire was used to obtain information from respondents. Data was analyzed using SPSS version 21.
The mean age of the respondents was 50.5 ±6.3years with the highest among women aged 55 years and above. The knowledge of menopause related symptoms was poor as 64% of the respondent did not know any menopause related symptoms. The prevalence of menopause related symptoms were more among the peri-menopausal and postmenopausal respondents in the 6 symptom domains
assessed. The use of screening services was poor as 4% of the respondents had done half of the 8
"recommended" health related screening within the stipulated period. The perceived family support among the respondents was low as 47.8% of the family had good family support. There was no significant association between family support and the self-care practices (health screening and treatment options).
This study has revealed gaps in the knowledge of menopause related symptoms, self-care practices and family support among the menopausal women. In addition, perceived family support did not play a role in the self-care practices among menopausal women. Opportunities for public enlightenment and health education interventions is needed to address these gaps among the study population.
DECLARATION………………………………………………………..……………………i
ACKNOWLEDGEMENTS………………………………………..………………………..ii
DEDICATION……………………………………………..…………………………...........iii
CERTIFICATION………………………………..……………………………………….…iv
TABLE OF CONTENTS…………………….………………………………………..…….v
LIST OF TABLES……………….………………………………………………………….vii
LIST OF FIGURES…………………………………………………………………............viii
APPENDICES…………..…………………………………………………………………...ix LIST OF ABBREVIATIONS………………………………………………………….........x SUMMARY………..………………………………………………………………………....1
CHAPTER 1: Introduction………………………………………………………..………….2
Rationale for the study…………………….……………………………………..….7
Aim and Objectives of the study……………………………………………………10
Literature Review…….………………………………………………………………...13
Materials and Method.…….…………………………………………………………... 46 CHAPTER 4 Results……………………………………………………………….......... 63
CHAPTER 5 Discussion…….……………………………………………………………86 Limitations of the study…..…………….………………………………………………...100
Conclusion………………………………………………………………………….......................
....101
Recommendations………………………………………………………………………………...
References…………………….………………………………………………………...............1
Menopause is a physiological process occurring with ovarian failure and marks the end of a woman's reproductive life. 1 The average age of menopause is 51 ± 3years worldwide.2 Dane and Seigal categorized menopause into three time periods. These are pre-menopausal, peri-menopusal and post-menopausal periods.3 The peri-menopausal period also known as climacteric is immediately prior to the post-menopause, at which time the endocrinological, biological and clinical features of approaching menopause commenced. It precedes the final menses by 2 to 8 years (median of 3.8 years). Postmenopausal state is the complete cessation of menstrual periods for 12 consecutive months, however the term menopause is commonly used for both events.3
Natural menopause is a gradual process that occurs for most women between ages of 45- 55 years,4 premature menopause occurs in a woman younger than 40 years and menopause is considered late if it occurs in a woman older than 55 years.4 Menopause occurs at a point when other life events are taking place simultaneously. The woman is faced with the task of adjusting to the physiological symptoms of the personality changes, job anxiety, career changes, maintaining an economic standard of living, managing a home, adjusting to children growing or leaving home.5
In 1960, the world population of women aged 60 years and above was below 250 million, but it is estimated that by the year 2030, 1.2 billion women will be peri- or post menopausal and this total will increase by 4.7 million every year.1 The average woman in the developed world expects to spend an approximately one third of her life in post- menopausal state.6 Presently in Nigeria, women have higher life expectancy than men with male: female of 51.63:53.66 years respectively according to 2014 estimate.7,8 This implies that women in their postmenopausal period make up majority of elderly
population.8
Menopause occurs due to regression of ovarian function, leading to decrease in estrogen level with resultant variability in menstrual cycle (peri-menopausal) and permanent caessation of menses (post-menopausal).4 With general increase in life expectancy, many women are likely to live for more than 20 years after menopause, spending about one quarter of their lives or more in a state of estrogen deficiency.9 Owing to lack of estrogen, a woman may experience target organ response involving the cardiovascular, urogenital, central nervous system, bone and skin resulting in decreased physical and mental wellbeing, hence post -menopausal woman could be considered at risk population.10 Most women going through menopause experience one or more of these symptoms in a varying degree of intensity from mild (discomforting), moderate, and severe (extreme and life changing).
The overall health and well-being of middle-aged women have become major public health issues around the world.11 Ten years prior to the caessation of menses, a woman receives signal that her reproductive organs are changing. More than 80% of women present with physical symptoms in the years approaching menopause with various distresses in their lives leading to a decrease in quality of life.11 This situation is worsened by women's overall limited knowledge about the potential health problems associated with menopause and the necessary preventive measures indicated by their low participation in screening programmes for chronic diseases coupled with their unhealthy lifestyle (physical inactivity, low consumption of fruits, vegetables and food rich in calcium) which impede a better overall health related quality of life.3
Population based studies have shown that reported health symptoms at 47 years tend to cluster into 4 main groups: vasomotor symptoms such as hot flushes and cold night sweat; somatic symptoms such as headaches, muscle and joint pain; psychological symptoms such as anxiety- depression and sexual discomfort. Non-specific somatic and psychological symptoms including tiredness, irritability, insomnia, palpitations, memory or concentration difficulties, mood swings, or depression have been commonly reported.12 As a result of these predicted changes in population structure, physicians are beginning to see that menopause is not a negligible phenomenon but a major health problem.1
Menopausal status seems to have an impact on attitude. Avis and Mckinlay found that surgical menopausal women held more negative attitude towards menopause than those going through the normal transition.13 Attitude refers to feelings, beliefs and reactions of an individual towards an event, phenomena, object or person, they are not innate attributes of mankind, but are learnt responses.14 Fishbien and Ajzen remarked that attitude is considered to be individualistic, an abstracted entity, a kind of intervening variable imposed in order to explain regularities in behavioural responses. In this study, attitude is used to explain the behaviours of Nigerian women towards menopause within an individual and influenced by situation and circumstances.14
The decision on how to deal with menopausal symptoms leads to perception and attitude of women towards menopause. If the knowledge of menopause is not enough, it will be perceived wrongly or negatively which can lead to negative or neutral attitude towards menopause. However, if the knowledge about menopause is adequate and understandable, there would be correct or right perception which can lead to positive attitude towards menopause. Perception as regards to this study therefore means ability of women to have the knowledge of menopause, understand menopausal signs and symptoms and to cope with it. Menopausal symptoms are found to be less common in societies where menopause is viewed as a positive rather than negative event.12
Self -care is a key component of current policies to manage long term conditions. Although most people with long term health problems care for themselves within an illness referral system, consultation rates for long term un-differentiated illness remain high. While most women seem to view menopause as a biological event and place it within the context of their developmental milestones15 or even accept it as a marker of old age. Some of these women place it as a time frame within their lifespan,16 a significant majority nevertheless resort to numerous prescribed and nonprescribed self-care actions to relieve menopause related symptoms through this transition.16–19 The need and choice of these self -care actions, particularly those that are non-prescribed, however vary from region to region and women to women depending on the educational level, attitude towards menopause, psychological and economic factors and even availability of access to medications.17 Promotion of self-care in these individuals requires an understanding of their selfcare practices and need to be understood in the context of health care pluralism.17
Individual based care known as self-care can be broadly defined as those that are practiced by the individual and directed at relieving symptoms, maintaining health or preventing ill health. 18 Rogers and Hay19 view self-care activity as a continuum with those efforts made solely by the individual at one end and those shared with professionals at the other. The interactions between sectors of care, particularly self-care/professional care (notably primary care) interface are increasingly demanding attention in research.20 Studies have predominantly investigated selfmanagement interventions relating to specific diseases or long term conditions particularly diabetes, asthma, and arthritis.20 In contrast, self-care practices adopted by people with less well defined health problems are little understood, despite the prevalence of such problems and the challenges they pose to the General Practitioners.21
Family support is an important factor in conceptualizing primary health care patient problems. Numerous examples of how the family system determines the course of chronic illness have been influential in the development of collaborative medical care.22 By understanding how the family influence health, the Family Physician has the opportunity to anticipate and reduce the adverse effects of family stress and use the family as a source of care of the patients. Family oriented approach to health care is based on the biopsychosocial model that emphasizes the relationship among biologic, interpersonal and social factors in health.22
The beneficial effect of family support in overall health promotion and chronic illness have been reviewed and how to use family as a valuable resource and support in the care of the patient have been discussed. Understanding how family can influence health can assist the Physician in working more effectively with patients and families. Integrated health care, which involves management and delivery of health services so that clients receive a continuum of preventive and curative services, according to their needs over time and across different levels of the health system is becoming an important issue.23 There is virtually no data on integrated health care among Nigerian menopausal women especially in areas of family support, self- care practices and other health related quality of life despite the identified problems mentioned inter alia in this group and little is known about the complex relationship between perceived family support and psychological distress in these mixed middle aged primary care patients.22
1.1 RELEVANCE OF THE STUDY
There is paucity of information in the area of family support and self-care practices in menopausal women in Africa including Nigeria. Studies have predominantly investigated self-management interventions relating to specific diseases or long term conditions particularly hypertension, diabetes, asthma, arthritis, but none have addressed areas concerning family support and self-care in menopausal women in Nigeria. There still exist a strong adherence to traditional and cultural practices in Nigeria where the way of life places a lot of demand on the women in the running of the household. Whereas women with mild menopausal symptoms are able to cope with the symptoms without seeking for medical treatment, women with moderate and severe menopausal symptoms consider them important health problems and may seek treatment for these symptoms.24
Assessing the awareness, knowledge and perception of menopause will give an idea of the kind of attitude towards ageing and managing symptoms of menopause in these women. It will also identify patient's expectation and fears about menopause thereby revealing most immediate needs and concern which could be biomedical, cultural or psychosocial.25 It would also identify their coping strategies and areas that would require support from the health care professional in order to improve their health related quality of life in menopause. 25
The most reported symptom(s) experienced by these women were based on the menopausal status and factors that affect health promotion, prevention and treatment which could provide most immediate needs and relieve concerns.25 How healthy are the patient's lifestyle in terms of diets, exercise, smoking, alcohol use, and intake of the counter medications give an idea of how much thought and effort has been put into taking care of themselves. This would improve patient-doctors relation where common ground are agreed upon in other to facilitate treatment and correct negative perceptions as they transit through menopause. 25 One of the important issues that may vary from one group to another is in determining whether menopause is considered a 'sickness' or a natural process of ageing. In many societies, the 'culture of silence' about some of the important aspects affecting reproductive health status also gives rise to concern about physiological changes that could be easily explained to the individual to relieve her of unnecessary stress. The way in which the social beliefs and norms have shaped the ideas and reactions of females to the discomfort and apprehension associated with reproductive changes will also affect their treatment seeking behaviour. 26
The beneficial effect of family support in health promotion in chronic diseases across the age groups irrespective of gender has been discussed, however the investigator is interested in how the family support promotes self-care practices in these women at menopause. In addition, biopsychosocial effect of family support on un-differentiated non-specific somatic and psychological symptoms including tiredness irritability, memory and concentration, poor sleep problem which have been described in most studies but poses challenges in medical practice will be looked unto. This would enable the logical planning and empowerment in areas that would have the greatest impact in promoting self-care practices and health related quality of life in these group of women as the investigator doubts the degree of contributions of the support received from the family, friends and relation including the community in their quest to maintaining health during after their reproductive period.
Over the past 2 decades, an expanding body of literature has documented links between a woman's age at menopause and health.27 Menstrual cycle patterns, as markers of physiologic functions and through their potential associations with the age at menopause, have also been investigated for their links to health outcomes.28 Early menopause has been associated to a number of negative outcomes including a higher risk of cardiovascular diseases, osteoporosis and higher all-cause mortality and the late age of menopause has been associated with higher risk of breast and endometrial cancer.29 Menstrual cycle characteristic most notably, length of inter-menstrual interval have also been identified as risk factors for a variety of health conditions including polycystic ovary syndrome, coronary heart disease, and risk of fracture.30 The concerns expressed 35years ago that "even": a minor shift from self-care to doctor care could make intolerable demands on the general-practitioner on services have continued to be voiced by General Practitioners and are now being taken a step further by National Health Service (NHS) policies that promote self-care support as a potential mechanism for reducing the element for medical care.22 Documenting women's use of self-care actions will help better understanding of the menopausal transitions and may serve as a platform to detect gaps in the integrative health care among this group of women. This may provide an opportunity for further studies on the role of family support and self -care practices since very little information is available on this issue in Nigeria, the focus being on family support, self -care practices, and common non-specific symptoms that are difficult to treat with medical interventions but which are amenable to other self-care. This could enable hypothesis generation for further research and to inform the development of methods of supporting women with menopause related symptoms in our environment.
1.2 AIM AND OBJECTIVES
The aim of this study is to investigate the role of perceived family support and self-care practices in women of menopausal age group attending the General Outpatient (GOP) Clinic of Federal Medical Centre, Owo, with the purpose of improving the knowledge of menopause related problems and reducing potential health related problems within this age group.
To determine the knowledge, prevalence and pattern of menopause related symptoms among women of menopausal age group attending GOP clinic, FMC Owo.
To assess the perceived family support among women in menopausal age group attending GOP clinic, FMC Owo
To assess the self-care practices among women in menopausal age group attending GOP clinic, FMC Owo.
To determine the role of family support on self-care practices among women of menopausal age group attending GOP clinic, FMC Owo.
1.3 SOME DEFINITIONS USED IN THIS STUDY
Menopause- This covers the events of peri-menopausal (climacteric) a time of changing ovarian function to post-menopausal (complete cessation of menstrual period for 12 consecutive months)
Menopausal women-This refer to women that are peri-menopausal and or post- menopausal.
Menopausal age group-This refer to women aged 40- 60 years in this study irrespective of symptoms or gynaecological history.
Menopausal status-This refer to whether the respondent is premenopausal, perimenopausal and post-menopausal in the absence of any medical or gynaecological procedures that can induce menstrual irregularity or complete cessation of menses. Menstrual status- This refers to perceived self-reported menstrual characteristic based on the last menstrual pattern.
Bio-psychosocial well-being- This involves the biological, psychological and social dimensions of health. It is an integrated mind-body approach which leads to overall health, better treatment outcome, enhanced satisfaction and well- being.
Biological well-being- These are physical changes a woman undergoes due to cessation of ovarian follicular activity. Biological changes includes hot f1ushes, joint or musculoskeletal pain
Social well-being- This refers to the ability of individual to function in society where she lives. Social change includes lack of interest to new relationship, work satisfaction.
Family support- This refers to the support received by the respondent from spouse, siblings, children, parents and relatives. These include informational support, emotional support and financial assistance as measured by the family APGAR.
Social support- This refers to the various types of support that people receive from others and is generally classified into three major categories: emotional, instrumental and informational support Family- This is defined in this study as a specific group of people who share common ancestors that may be made up of partners, children, parents, aunts, uncles, cousins and grandparents
NUTRITIONAL STATUS AND ACADEMIC PERFORMANCE OF URBAN AND RURAL PRIMARY SCHOOL CHILDREN IN OBAFEMI – OWODE LOCAL GOVERNMENT AREA, OGUN STATE
AN ASSESSMENT OF THE QUALITY OF EMERGENCY OBSTETRIC CARE SERVICES IN GOVERNMENT-OWNED SECONDARY HEALTH FACILITIES IN ENUGU STATE
EPIDEMIOLOGICAL SURVEY OF AN OUTBREAK OF SUSPECTED CHOLERA IN LAGUN
ladychampionz


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Middle School Robotics places 2nd; Advances to State Event
Dec 12 2017 3:20 PM
If people at the 10th annual First Lego League Qualifying Tournament didn't know who Wilbraham & Monson Academy was when the competition started, they sure knew who Coach Luke Pelletier and his five students were by the end of the day.
Competing against 22 middle school teams from Western Massachusetts, the Titans won one category and placed second in two others Dec. 9 at Agawam High School to advance to the state event.
"The team worked extremely well with each other," Coach Pelletier said. "The five core kids really worked outstandingly together. They came in with no experience and they left with a tremendous amount of experience. Yuzuki, the program she made was beautiful."
The five WMA Middle School students who competed at the nine-hour event were Gabe Dziura '24, Brady Gouin '23, Michelle Itkin '22, Yuzuki Yamaoka '23 and Jinyu "Melody" Zhan '22.
WMA placed second in the overall category, which included how its robot performed and how well the students presented to judges in three areas: their project on urban water cycles, how they worked together, and how well they knew the robot and the programming. The presentations were given without assistance from coaches.
"It showed they knew what they were doing," Coach Pelletier said.
The meet didn't start as planned for the Titans, who struggled in their first two (of five) attempts in the Robot Performance portion due to an issue with the table.
"They figured it out, and without my help," Coach Pelletier explained. "The three (attempts) after the first two were perfect. It was good for them to feel good, I felt good as a coach because I didn't tell them what to do, and the parents saw it. They figured it out so well that we beat everyone in the afternoon at the bracket competition."
While the judges were calculating scores, the students competed in a friendly head-to-head competition with all of the other participants, which WMA won.
Approximately 400 teams competed in qualifying tournaments at various events throughout the state. Massachusetts hosts two state meets, with WMA earning a trip to Worcester Polytechnic Institute Dec. 16.


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How Mars Petcare Uses Data To Connect The Dogs
by Ryan Joe // Monday, February 19th, 2018 – 6:45 am
You probably don't think of Mars Petcare as a center for startup incubation.
It owns a lot of brands you can buy at a local grocery store, including Pedigree and Whiskas. But in 2000, it bought Royal Canin, a pet food brand focused on health care, and, more recently, a string of veterinary clinics.
So, while Mars Petcare originated as a provider of packaged pet products – one with little direct insight into clients – it now had a direct line into pet owners. The trick, however, is bringing those products, services and insights together.
That's where Leonid Sudakov – the US president of Mars Petcare Connected Solutions – comes in.
"All of our core businesses will have to go through a true transformation in the next decade to future-proof their brands," Sudakov said.
That means establishing a direct line to consumers – not only to send messages them, but also to sell to them.
"Where my division is really engaged, is how do we become a real force for good for the future of our category?" Sudakov said. "How do we become the partner of choice for every disruptor, whether that's a person with an idea, a startup trying to scale or someone in the core business trying to do something different?"
For instance, in 2016, Mars Petcare acquired Whistle, the so-called "Fitbit for dogs." In so doing, Mars Petcare gained insight into the activities of dogs across the nation.
Sudakov, who owns a cat, four donkeys, four horses and four ponies, spoke with AdExchanger at the IAB Leadership Conference last week about orienting these very different departments around a single goal.
AdExchanger: Many of your recent acquisitions – from Whistle to pet health clinics – give you a direct line to the animal owner.
LEONID SUDAKOV: Exactly. For 70 years, since we first got into pet food in 1936, we've been primarily a grocery pet food business. When we acquired Royal Canin in the early 2000s, it opened the door to therapeutic nutrition, which you sell to the vets. That brought us closer to the world of health.
The idea is that the more you understand the health conditions of your pets, the more you can design products and services, starting with pet food but not exclusively, to fit their needs.
I can't imagine that every acquisition is used to sharing data. How do you get them invested in doing that?
The competitive aspect of our business is that we have so many touch points that allow us to serve consumers.
Ensuring the entire organization understands that and sees the value and benefit of data is a massive priority. [The pet care] industry historically is not data-centric. There are no unified disease codes. It's about the doctors making the right decisions on the spot, not about saving or using data for the future.
We've defined our dual strategy as better care and better business. If we can match our primary care data from Banfield with our specialty emergency care data from Blue Pearl with activity data from Whistle, we can actually create a data platform that can add years to pets' lives.
That lets you win over all the doctors and all the industry opinion leaders. You're not trying to mine the data to get more value, you want to do something to help the industry transform.
How are we going to buy pet food in 10 years?
Like any other consumer goods industry, I believe a lot of the engagement will happen digitally. Half of the category growth is online. You'll be guaranteed to have the right food in the right quantity, delivered when you need it.
Amazon does that, Chewy does that. Is that something you need to build?
I don't believe there will be one solution. We've partnered very closely with Amazon, Petco and PetSmart to figure out what will happen from those channels.
If you build a direct-supply model, that's a great opportunity if you can own that buying portal.
We're in it already. I'm so excited about our Royal Canin flagship store [in China], which is about learning how to build a direct-to-consumer business. We need to continue to scale it. It's important to move from business innovation in the abstract to living it day in and day out. That's where we are.
How about in the US?
We have quite a few live projects in the US. It's a market where we have fantastic and strong leading brands, so I see us operating various models in the US as well.
GDPR will bring more restrictions around collecting consumers' data. But if you know that Bob Jones' cat has kidney issues, is that data about Bob Jones or about his cat?
In the case about the health of the cat, it's quite separate from the data of the pet owner. The critical part is that we're very conscientious of GDPR and protecting the privacy of our consumers. But we can use the insights in the data we have about pets to build better care. So, it's not just trying to know the pet owner, if you have medical records from a pet, you can predict the medical outcome better and be preventative.
Do you have the infrastructure to create that messaging?
That's what we're working on. We are about to launch this predictive analytics machine that will connect all of this. To create that, you need to have what Google has in the human world: a scale of data inputs to run a predictive diagnostic algorithm. That's where the scale of our business helps. We want to do this in the next three years.
What's the challenge now? Data collection?
We're engaging thousands and thousands of pet owners, distributing free devices and starting to build this data collection mechanism. Then we'll start matching what we get from the device, the type of behavior we see, so we can recognize what's a gait or tail wagging or a jump.
Magna: Digital Ad Spend Resilient In 2020 Despite Turmoil


Batman And Joker Drawing How To Draw Joker And Batman, Step By Step, Dc Comics, Comics. tagged: batman and joker drawing, batman and joker drawing easy, batman vs joker drawing... How to Draw The Joker Retro Vintage Style Easy Drawing Tutorial October 19, 2015 by admin Leave a Comment Learn how to draw a retro / vintage style Joker from an old-time cereal box.
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At home in Lancaster County, work in one of Pennsylvania's most cherished retirement communities.
If you seek fulfilling work with rewarding benefits, look into the jobs now available at Quarryville Presbyterian Retirement Community. As your fellow employees will tell you, it can become your second home.
We are currently seeking a Housekeeper to join our new Home Care team!
We are looking for a Companion Driver to join our Home Care team!
Position Summary: Works under the supervision of the Director of Home Care to provide companionship, transportation, and physical assistance to individual clients of Great Rock Home Care.
Great Rock Home Care provides non-medical home care to seniors in the comfort of their home. We are seeking compassionate, reliable, and dedicated caregivers to join our team!
We are currently seeking part-time Aides and Servers to join our Dining Services Team throughout our campus!
We currently have an opportunity available for a Cook to join our Dining Services Team! This is a full-time, every other weekend position. A qualified candidate will be dedicated, self-motivated, and have high volume and/or healthcare culinary experience.
We are seeking LPNs to join our Personal Care team!
We are seeking Personal Care Attendants to join our team!
QPRC is looking for a Memory Support Attendant to fill a second-shift position, 4 PM to 8 PM, three evenings per week and alternating every other Saturday and Sunday.
Responsibilities include: Provide activities of daily living for residents, document resident care, and provide afternoon activities programs. Previous experience with dementia care preferred.
We are seeking RNs/LPNs to join our Skilled Nursing Team!
We currently have part-time opportunities available for Certified Nursing Assistants (CNAs)!
We are currently seeking a Certified Nursing Assistant to join both our Skilled Nursing team and our Activities team! This is a full-time position in which the CNA would work in Activities (4 days biweekly) but also work in Skilled Nursing (6 days biweekly). Qualified candidates must have an up-to-date Pennsylvania CNA certification.


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\section{Introduction}
Early-type galaxies are known to produce copious Lyman alpha photons due to their spatially extended gas distribution. In protogalactic halos gas transfers its gravitational binding energy to the excitation of hydrogen atoms which results in Lyman alpha emission \citep{2000ApJ...537L...5H,2006ApJ...649...14D,2006ApJ...649...37D}. Therefore, the gas in dark matter halos exceeding a virial temperature of $\sim10^4$~K may be detected in the Lyman alpha line emission. The presence of ionizing radiation sources may enhance the Lyman alpha flux as gas is photo-ionized, and and supernova feedback may further increase the escape fraction by generating a more clumpy structure. These ionization sources could be the first stars or mini-quasars. A luminous quasar can boost the emission of Lyman alpha photons by several orders of magnitude \cite{2001ApJ...556...87H}.

Many Lyman alpha blobs (LABs) have been observed at high redshift \citep{2009ApJ...693.1579Y,2009ApJ...696.1164O,2004AJ....128..569M,2000ApJ...532..170S}. In the light of recent detections at redshift $\rm > 7$ \citep{2010Natur.467..940L,2010arXiv1011.5500V}, it is of high interest to understand what drives the emission and how it is spatially distributed. A number of LABs have been observed whose most probable origin is cold accretion of gas onto dark matter halos \citep{2006A&A...452L..23N,2007MNRAS.378L..49S}.

Numerical simulations show that cooling by Lyman alpha radiation induces collapse in protogalactic halos. Moreover, baryons accumulate into the center of halos by penetration of cold streams of gas through the shock heated medium \citep{2001ApJ...562..605F,2008ApJ...682..745W,2009ApJ...696.1065J,2009MNRAS.396..343R,2009Natur.457..451D,2009MNRAS.395..160K,2010MNRAS.407..613G,2010MNRAS.tmp.1837L,2010MNRAS.402.1249S}. Cold streams with temperatures of $\sim10^4$~K could be potential sources of spatially extended Lyman alpha emission \citep{2009MNRAS.400.1109D}. \cite{2010MNRAS.tmp.1427J} found that Lyman alpha radiation can also be emitted during accretion of gas on black holes formed by direct collapse in the first galaxies. Such emission is potentially detectable with JWST\footnote{http://www.stsci.edu/jwst/instruments/nirspec/sensitivity}. Similarly, it allows to probe the starburst component through the enhanced emission in several recombination lines  \citep{2009MNRAS.399...37J}.

The presence of large columns of neutral hydrogen gas causes the trapping of Lyman alpha photons \citep{2006ApJ...652..902S,2010MNRAS.tmp.1837L,2010ApJ...712L..69S}, which was neglected in some of the previous studies. In this letter, we aim at a self-consistent modeling of Lyman alpha emission driven by accretion flows, including dynamics, non-equilibrium chemistry of H, $\rm H^{+}$, He, $\rm He^{+}$ and $\rm He^{++}$, detailed level populations of atomic hydrogen, as well as the trapping of hydrogen line photons due to large column densities. The prime objective of this work is to study the origin and spatial distribution of Lyman alpha emission, which is detectable with JWST.

\section {Modeling of the physics}
For our simulations, we employ an extended version of the adaptive mesh refinement (AMR) hydrodynamics code FLASH \citep{Dubey2009512}. FLASH is a module based Eulerian grid parallel simulations code. We use an AMR grid to achieve high dynamic resolution in the regions of interest. We employ the directionally split piece wise parabolic method (PPM) for hydrodynamic calculations, which is an improved form of the Godunov method \citep{1984JCoPh..54..174C}. This method is well suited for flows involving shocks and contact discontinuities. The dark matter is simulated based on the particle mesh (PM) method.
In order to create Gaussian random field initial conditions, we run the COSMICS package developed by \cite{1995astro.ph..6070B}. We start our simulation at redshift 100. Our computational periodic box has a comoving size of 10 Mpc. We perform our simulations in accordance to the $\rm \Lambda$CDM model with WMAP 5-years parameters. We select a $4\times 10^{9} M_{\odot}$ halo at redshift 7 and follow its collapse. We enforce 8 additional levels of refinement, which gives 15 levels of refinement in total. In this way, we obtain a dynamic resolution limit of 70pc (co-moving), and can still follow the further evolution until redshift $\rm z=4.7$. We impose the Truelove criterion by refining according to the Jeans length \citep{1997ApJ...489L.179T}. We resolve the Jeans length by at least 20 cells.Such resolution was shown to be sufficient for accurately resolving turbulent structures during
gravitational collapse (Federrath et al. 2010). When the highest refinement level is reached, we prevent artificial fragmentation via Jeans-heating. We assume a  primordial gas composition with $\rm 75 \%$ hydrogen and $\rm 25 \%$ helium by mass.

We have developed a chemical network for the non-equilibrium modeling of non-molecular species. For this purpose, we solve the rate equations of the following species $\rm H,H^{+},He,He^{+},He^{++}$ and $\rm e^{-}$ for non-equilibrium ionization. The rate equations for these species are solved using the backward difference formula (BDF) method of \cite{1997NewA....2..209A}. We adopt the chemical rates of \cite{1997NewA....2..181A} and \cite{2008A&A...490..521S}. We further solve for the level populations of atomic hydrogen up to the fifth electronically excited state, and model the non-equilibrium cooling including hydrogen line emission, collisional ionization cooling, recombination cooling, Bremsstrahlung cooling and Compton cooling/heating. The transition rates for the level populations are based on work of \citet{2001ApJ...546..635O}.
At an optical depth $\rm \tau_{0} > 10^{7}$, the photon escape time becomes longer than the gas free fall time. Because of the weak dependence of the photon escape time on the gas number density, $\rm t_{ph} \propto n^{-1/9}$, trapping becomes important important during the collapse since the latter scales as $\rm n^{-1/2}$. A detailed discussion of such line trapping effects is given by \citet{2001ApJ...546..635O, 2006ApJ...652..902S, 2010ApJ...712L..69S}. We have computed the Lyman alpha luminosity by determining the Lyman alpha emissivity and integrating it over the virial volume of a halo. Further details of the luminosity and flux calculation can be found in \cite{2006ApJ...649...14D}.

\begin{figure*}
\centering
\begin{tabular}{c c}
\begin{minipage}{8cm}
\includegraphics[scale=0.30]{Coldflow.ps}
\end{minipage} &
\begin{minipage}{8cm}
\includegraphics[scale=0.30]{Coldflow1.ps}
\end{minipage} \\  \\

\begin{minipage}{8cm}
\includegraphics[scale=0.30]{cftmp.ps}
\end{minipage} &

\begin{minipage}{8cm}
\includegraphics[scale=0.30]{ctmp12.ps}
\end{minipage}

\end{tabular}
\caption{The upper panels of this figure show the density slices through the center of the halo. The left panel is for redshift 4.7 and right panel for redshift 8. Velocity vectors are overplotted on the density slices. The bottom two panels show the corresponding temperatures. The figure shows the inner region of 20 kpc in comoving units.}
\label{figure1}
\end{figure*}

\section{Results and Conclusions}
The initial density perturbations decouple from the Hubble flow and begin to collapse via gravitational instabilities. The gas is shock-heated during the non-linear collapse of density perturbations. At redshift 10, the halo begins to virialize. In the process of virialization, part of its gravitational energy is converted into thermal energy. This heats up the gas and results in the emission of Lyman alpha photons. The gas is accreted into the center of the halo through cold streams of $\rm \sim 10^{4}$K as shown in figure \ref{figure1}. The upper panels of figure \ref{figure1} show the density at different redshifts while lower panels show corresponding temperatures. Typical number densities of the cold streams are of the order of 0.01-1 $\rm cm^{-3}$. Density and temperature radial profiles are depicted in the upper left and right panels of figure \ref{figure2}. We see that in the presence of hydrogen line emission the gas cools isothermally. The density profile of the halo is $\rm \sim r^{-2.3}$, which agrees with results of \cite{2008ApJ...682..745W}. The ionization degree of the gas is shown in the bottom left panel (HII abundance) of figure \ref{figure2}. We see that most of the gas remains neutral at $\rm 10^{4}$ K, ionized fraction goes down due to faster recombination at higher densities $\sim n^{-0.5}$. The gas radial velocity is depicted in the bottom right panel of figure \ref{figure2}. It can be seen from the figure that gas is falling into the center of the halo. The velocity profile also shows that gas is accreted onto the halo through accretion shocks. The cold streams have typical column densities of about $\rm 10^{19} cm^{-2}$. A radial profile of the column density is shown in figure \ref{figure3}. At columns above $\rm 10^{21} cm^{-2}$ the gas optical depth exceeds $10^{7}$ and Lyman alpha trapping becomes effective. The Lyman alpha emissivity is shown in figure \ref{figure3}. It can be seen from the figure that above columns of the order of $\rm 10^{22} cm^{-2}$, Lyman alpha photons are trapped and cooling through this line is completely suppressed. That is why the Lyman alpha emissivity sharply declines in figure \ref{figure3}. We explored the local density variations and found that the maximum variation of the column density does not exceed an order of magnitude. In this sense, our calculation should provide a conservative lower limit on the expected flux. In the presence of Lyman alpha trapping, cooling can proceed through higher electronic states of atomic hydrogen \citep{2010ApJ...712L..69S}. For comparison, the total emissivity from higher states of atomic hydrogen and recombination/Bremsstrahlung processes is shown in figure \ref{figure3}. The total emissivity plot shows that despite line trapping, cooling still proceeds through these higher states of atomic hydrogen, particularly through 2s-1s and 3-2 transitions, and the thermal evolution is approximately isothermal.
\begin{figure*}
\centering
\begin{tabular}{c c}
 \begin{minipage}{8cm}
\includegraphics[scale=0.23]{den3.ps}
\end{minipage} &

\begin{minipage}{8cm}
\includegraphics[scale=0.23]{tmp3.ps}
\end{minipage} \\  \\

\begin{minipage}{8cm}
\includegraphics[scale=0.23]{NewHII.ps}
\end{minipage} &

\begin{minipage}{8cm}
\includegraphics[scale=0.22]{Newvrad2.ps}
\end{minipage}

\end{tabular}
\caption{All panels in this figure are log log plots. The upper left panel shows the radial density profile of the halo. The radial temperature profile for the halo is depicted in the upper right panel. HII abundance is shown in the lower left panel. The radial velocity of the halo is depicted in the lower right panel.}
\label{figure2}
\end{figure*}

\begin{figure*}
\centering
\begin{tabular}{c c}
 \begin{minipage}{8cm}
\includegraphics[scale=0.23]{clom3.ps}
\end{minipage} &

\begin{minipage}{8cm}
\includegraphics[scale=0.23]{Total4.ps}
\end{minipage} \\  \\

\begin{minipage}{8cm}
\includegraphics[scale=0.23]{newlum3.ps}
\end{minipage} &

\begin{minipage}{8cm}
\includegraphics[scale=0.23]{newflux3.ps}
\end{minipage}

\end{tabular}
\caption{All panels in this figure are log log plots. The upper left panel shows column density plotted against the radius of the halo. Lyman alpha emissivity radial profile emerging from the halo is shown in the upper right panel. Lyman alpha luminosity is shown in the lower left panel. Lyman alpha flux is plotted against the radius of the halo in the lower right panel.}
\label{figure3}
\end{figure*}

The radial profile of the enclosed Lyman alpha luminosity is shown in figure \ref{figure3}. If the emission originates preferentially from the center, an approximately flat profile would be expected, while for uniform emission, a power-law behavior as $\sim r^3$ would be expected due to volume effects. Here, we find the absence of emission in the central core, then a sharp increase in luminosity between radii of $\rm 10^{20.2}cm -10^{21} cm$ by four orders of magnitude, and a more modest increase between radii of $\rm 10^{21} cm -10^{22} cm$. This behavior reflects the generation of Lyman alpha emission through accretion shocks. JWST can confirm the presence of such a brightness profile. The total Lyman alpha luminosity from the halo is $\rm 10^{44} erg~s^{-1}$, which is consistent with observed Lyman alpha blobs \citep{2009ApJ...696.1164O,2010MNRAS.407..613G}.

The emerging flux from the halo is depicted in figure \ref{figure3}. We find a total flux of $\rm 5.0\times 10^{-17} erg~cm^{-2}~s^{-1}$. At redshift 4.7, the observed Lyman alpha wavelength is at 0.68 microns. This can be detected with the JWST-instrument NIRSpec for integration times of $10^{4}s$, with S/N=$10$ and R=$100$. JWST spectrograph NIRSpec will have angular resolution of 0.1 arc-sec for 2 micron, and NIRcam will be well-suited for higher angular resolution with field of view of 2.2x2.2 $\rm arcmin^{2}~and~ 4096^{2}$ pixels for shorter wavelength of 0.6-2.3 micro meter. The halo in our case will have an angular size of 0.5 arc-sec at redshift 4.7. It should be detectable with NIRcam/NIRSpec. For extended emission of Lyman alpha, it may need higher integration time ($\sim 10^{5}$ sec) to resolve the flux from extended sources. The total mass of our halo at redshift 4.7 is $\rm 2\times10^{10} M_{\odot}$, which is not extreme in any way. Selecting higher mass halos will produce higher fluxes as there is a power law relation between the mass of a halo and its luminosity $\rm L_{Ly\alpha}\propto M^{5/3}$ \citep{2009Natur.457..451D,2006ApJ...649...14D}. We stopped our simulation at a redshift of 4.7 as it becomes computationally too expensive to follow the further time evolution.

In this work, we assume that there is no X-ray/UV background flux. Its presence can heat the gas and may increase the Lyman alpha flux \citep{2008ApJ...678L...5S,2007MNRAS.375.1269Z}. We have compared our results with \citep{2006ApJ...649...14D} and found good agreement. We have assumed here that the halo is metal free. The addition of small amounts of dust can absorb Lyman alpha photons efficiently, unless the gas is inhomogeneous \citep{1999ApJ...518..138H}. However, in-falling gas may still be pristine for isolated halos. We have ignored $\rm H_{2}$ cooling, which is suppressed in the presence of a strong UV background ($\rm J_{21}> 100$) \citep{2004ApJ...601..666D,2009A&A...496..365C}. \cite{2010MNRAS.402.1249S} found that even $\rm J_{21} \sim 30$ will be sufficient to quench $\rm H_{2}$ formation for local variations in flux see \cite{2008MNRAS.391.1961D}. At higher redshifts, it is possible that $\rm H_{2}$ may form for more modest radiation backgrounds. Even then, we expect H$_2$ formation preferentially at the center of the halo, while the accretion at the virial radius may still include a gas phase at $10^4$~K. This supports our main conclusion that Lyman alpha radiation originates mostly from gas in halo envelope.

Some LABs are also  associated with massive star forming galaxies \citep{2006ApJ...640L.123M} where stellar feedback or an AGN could power Lyman alpha radiation. It is clear that starbursts and AGNs are also potential candidates to power or enhance the observed Lyman alpha luminosities. It is not fully clear if our results are also applicable to such situations, although we expect similar effects of line trapping in the centers of such galaxies if $\rm N_{H}/\Delta v \geq 10^{21} cm^{-2} km^{-1} s$,  with $\rm \Delta v$ the cumulative velocity difference along the atomic hydrogen column $\rm N_{H}$.Current modeling uncertainties concern both the star formation efficiency and the initial mass function. Both radiative feedback, leading to the formation of HII regions, as well as mechanical feedback, providing a more clumpy structure with higher escape fractions, need to be modeled self-consistently. Outflows if present may enhance the detectability of Lyman alpha emission in the outskirt of the halo,  5 \% of the emitted Lyman alpha photons could be directly transmitted to the observer along the line of sight \citep{2010MNRAS.408..352D}. In the future, cosmological radiative transfer simulations including feedback effects should be performed to obtain more robust results.

\section*{Acknowledgments}
The FLASH code was in part developed by the DOE-supported Alliance Center for Astrophysical Thermonuclear Flashes (ACS) at the University of Chicago. DRGS acknowledges funding via the European Community's Seventh Framework Programme (FP7/2007-2013) under grant agreement No. 229517 and via HPC-EUROPA2 (project number: 228398) with the support of the European Commission Capacities Area–Research Infrastructures Initiative. SZ thanks the ladt Davis foundation for support. We thank the anonymous referee for a careful reading of the manuscript and many insightful comments.

\label{lastpage}

redpajama_set_name: RedPajamaArXiv


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Walygator Parc - 4 Things to Know Before Visiting
Voie Romaine, 57280 Maizières-lès-Metz, France
Hotels near Walygator ParcMore Information
About Walygator Parc
Discover More Attractions in Grand Est
Walygator Parc is an amusement park in France that was located between Metz and Thionville in the Moselle. This amusement park currently operates four coasters, those being the aforementioned Anaconda and Comet, as well as Family Coaster and Monster. The park also used to operate Zig Zag. It was one of the nice location where you can spend your free time with your family.
Attractions Near Walygator Parc
Zoo d'Amnéville2.55km from Walygator Parc
The Amnéville Zoological Park is a French zoo in the Grand Est region located between Metz and the border with Luxembourg, near Amnéville. About 2000 animals 1 of 360 species are presented there on 18 hectares. It is one of the few French zoos to feature gorillas and orangutans. It is also the only one to present a show taming of tigers. A nice zoo which has a large collection of Wildlife and is kept in a serene environment.
Metz Cathedral11.77km from Walygator Parc
A beautiful majestic cathedral which was featured with fantastic stained-glass windows and Gothic features, built with yellow Jaumont limestone dates from the 13th century. One of the main pilgrimage centers in this area and also there are so many art collections and so more. It was built on the site of an ancient 5th-century church dedicated to Saint Stephen protomartyr.
La Petite Venise12.31km from Walygator Parc
The little Venice of Colmar is a picturesque old tourist area, in the district of Krutenau, in the southern suburb of the historic center of Colmar, in Haut-Rhin, in Alsace. It is named after Venice, Italy , in relation to the historical picturesque organization of the life of the district, around its canals of the Lauch. This place is, with its many charming hotels, restaurants, winstubs , pastry shops, and shops, one of the best preserved old medieval traditional sectors, picturesque, enhanced
Centre Pompidou-Metz13.16km from Walygator Parc
The Pompidou-Metz center is a public cultural cooperation 2 art establishment located in Metz, between the Parc de la Seille and the train station. Its construction is carried out as part of the development operation of the Amphitheater district. It is an art center dedicated to modern and contemporary art, whose cultural project is the presentation of temporary exhibitions and the programming of live shows, cinema sessions, and conferences in two dedicated rooms.
Mosel-Radweg Thionville14.93km from Walygator Parc
The German Moselle Cycle Route is a long -distance cycle route along the Moselle and is part of the international Velo Tour Moselle cycle route. The cycle route is a typical river cycle path with no significant inclines. The German part is on asphalt bike paths, either on its own route or alongside the road and is therefore also suitable for families.
Malbrouck Castle32.67km from Walygator Parc
A beautiful and majestic castle which was listed as a historical monument. It stands atop the wooded hill of Meinberg and was constructed between 1419 and 1434. , it was occupied by the Duke of Marlborough during the War of Spanish Succession. Now it was a tourist attraction and invites visitors to enjoy several historical and architectonical highlights. You can visit this castle for free and can enjoy this beautifully restored site.
Where is Walygator Parc
Discover More Attractions in Grand Est, Where Walygator Parc Is Located
Grand Est is a vast new region in Eastern France, the unification of the former historical regions of Champagne-Ardenne, Alsace, and Lorraine. Its geographical location – bordering Belgium, Luxembourg, Germany, and Switzerland – makes of the Grand Est an interesting cultural melting pot which can be clearly seen in its architecture and tasted in its gastronomy.