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Top Suggestions Verbo Ser Worksheet :
Verbo Ser Worksheets Learny Kids
Displaying Top 8 Worksheets Found For Verbo Ser Some Of The Worksheets For This Concept Are El Verbo Ser Practica El Verbo Ser El Verbo Ser Ser Estar The Verbs To Know Ser Estar Ser Estar Nosotros Yo Voy Nosotras Vamos Prctica Del Verbo Tener Once You Find Your Worksheet Click On Pop Out Icon Or Print Icon To Worksheet To Print Or Download Worksheet Will Open In A New Window You Can Download Or Print Using The Browser Document Reader Options
Verbo Ser Worksheets Kiddy Math
Verbo Ser Verbo Ser Displaying Top 8 Worksheets Found For This Concept Some Of The Worksheets For This Concept Are El Verbo Ser Practica El Verbo Ser El Verbo Ser Ser Estar The Verbs To Know Ser Estar Ser Estar Nosotros Yo Voy Nosotras Vamos Prctica Del Verbo Tener Found Worksheet You Are Looking For To Download Print Click On Pop Out Icon Or Print Icon To Worksheet To Print Or Download Worksheet Will Open In A New Window You Can Download Or Print Using The Browser Document
El Verbo Ser Interactive Worksheet
El Verbo Ser Exercise To Learn The Verb Ser With A Song And Ordering The Verb
Verbo Ser Worksheets Lesson Worksheets
Verbo Ser Displaying All Worksheets Related To Verbo Ser Worksheets Are El Verbo Ser Practica El Verbo Ser El Verbo Ser Ser Estar The Verbs To Know Ser Estar Ser Estar Nosotros Yo Voy Nosotras Vamos Prctica Del Verbo Tener Click On Pop Out Icon Or Print Icon To Worksheet To Print Or Download
El Verbo Ser Worksheet Answers Akademiexcel
El Verbo Ser Worksheet Answers With Valuable Themes Because You Want To Offer All You Need In A Authentic And Trusted Reference Most People Provide Helpful Home Elevators Many Subject Matter As Well As Topics Coming From Advice On Presentation Writing To Making Guide Traces Or To Identifying Which Type Of Content For Your Current Composition We All Guarantee That The Followers Will Not Really Feel Hanging Associated With A Information And Facts That S Neglected Or OmittedEl Verbo Ser Worksheets Lesson Worksheets
El Verbo Ser Displaying All Worksheets Related To El Verbo Ser Worksheets Are El Verbo Ser Practica El Verbo Ser Verbos Ser Estar Tener Ser O Estar Prctica Del Verbo Tener The Spanish Verb Drills The Big Book Ser And Estar Click On Pop Out Icon Or Print Icon To Worksheet To Print Or DownloadEl Verbo Ser Spanish4teachers
El Verbo Ser Completa Las Frases Con La Conjugacion Correcta Del Verbo Ser 1 Camilo Te Presento A Maria Y A Juan Ellos Mis Profesores 2 Ella La Enfermera Del Senor Garcia 3 Yo Luis Rojas Y Abogado 4 Buenos Dias Yo Jose Sanchez Mucho Gusto 5Ser Estar Lesson Plans And Worksheets Spanish4teachers
Ser And Estar Worksheets Handouts El Verbo Se R Spanish 4 Teachers Middle School Spanish Ser Verb Worksheet To Practice Its Conjugation In Present Spanish Verb Se R Worksheet Spanish 4 Teachers Middle School Worksheet To Practice Conjugating The Verb Ser In Present
The Verb Ser El Verbo Ser Free Spanish Grammar
El Verbo Ser These Notes On Spanish Grammar Cover How To Use The Verb Ser To Be And Are Accompanied By A Video And Interactive Exercises For Ser In The Past Tense Please Click On The Link At The Bottom Of The Page The Spanish Verb Ser Means To Be But There Are Two Verbs Meaning To Be In Spanish Ser And Estar Ser Is Used Primarily In Situations To Imply Permanence Equivalence
Verbos Ser Y Estar Fichas Imprimibles Ejercicios
Fichas Imprimibles Con Los Verbos Ser Y Estar En Espanol Recursos Gramatica Lecciones Con Los Verbos Ser Y Estar En Lengua Espanola Nivel Elemental Y Medio To Be Spanish Verb Resources And Worksheets
Verbo Ser Worksheet. The worksheet is an assortment of 4 intriguing pursuits that will enhance your kid's knowledge and abilities. The worksheets are offered in developmentally appropriate versions for kids of different ages. Adding and subtracting integers worksheets in many ranges including a number of choices for parentheses use.
You can begin with the uppercase cursives and after that move forward with the lowercase cursives. Handwriting for kids will also be rather simple to develop in such a fashion. If you're an adult and wish to increase your handwriting, it can be accomplished. As a result, in the event that you really wish to enhance handwriting of your kid, hurry to explore the advantages of an intelligent learning tool now!
Consider how you wish to compose your private faith statement. Sometimes letters have to be adjusted to fit in a particular space. When a letter does not have any verticals like a capital A or V, the very first diagonal stroke is regarded as the stem. The connected and slanted letters will be quite simple to form once the many shapes re learnt well. Even something as easy as guessing the beginning letter of long words can assist your child improve his phonics abilities. Verbo Ser Worksheet.
There isn't anything like a superb story, and nothing like being the person who started a renowned urban legend. Deciding upon the ideal approach route Cursive writing is basically joined-up handwriting. Practice reading by yourself as often as possible.
Research urban legends to obtain a concept of what's out there prior to making a new one. You are still not sure the radicals have the proper idea. Naturally, you won't use the majority of your ideas. If you've got an idea for a tool please inform us. That means you can begin right where you are no matter how little you might feel you've got to give. You are also quite suspicious of any revolutionary shift. In earlier times you've stated that the move of independence may be too early.
Each lesson in handwriting should start on a fresh new page, so the little one becomes enough room to practice. Every handwriting lesson should begin with the alphabets. Handwriting learning is just one of the most important learning needs of a kid. Learning how to read isn't just challenging, but fun too.
The use of grids The use of grids is vital in earning your child learn to Improve handwriting. Also, bear in mind that maybe your very first try at brainstorming may not bring anything relevant, but don't stop trying. Once you are able to work, you might be surprised how much you get done. Take into consideration how you feel about yourself. Getting able to modify the tracking helps fit more letters in a little space or spread out letters if they're too tight. Perhaps you must enlist the aid of another man to encourage or help you keep focused.
Verbo Ser Worksheet. Try to remember, you always have to care for your child with amazing care, compassion and affection to be able to help him learn. You may also ask your kid's teacher for extra worksheets. Your son or daughter is not going to just learn a different sort of font but in addition learn how to write elegantly because cursive writing is quite beautiful to check out. As a result, if a kid is already suffering from ADHD his handwriting will definitely be affected. Accordingly, to be able to accomplish this, if children are taught to form different shapes in a suitable fashion, it is going to enable them to compose the letters in a really smooth and easy method. Although it can be cute every time a youngster says he runned on the playground, students want to understand how to use past tense so as to speak and write correctly. Let say, you would like to boost your son's or daughter's handwriting, it is but obvious that you want to give your son or daughter plenty of practice, as they say, practice makes perfect.
Without phonics skills, it's almost impossible, especially for kids, to learn how to read new words. Techniques to Handle Attention Issues It is extremely essential that should you discover your kid is inattentive to his learning especially when it has to do with reading and writing issues you must begin working on various ways and to improve it. Use a student's name in every sentence so there's a single sentence for each kid. Because he or she learns at his own rate, there is some variability in the age when a child is ready to learn to read. Teaching your kid to form the alphabets is quite a complicated practice.
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My life goals at 20 were different than they are at 40, so it may be natural for them to change over time. Research is needed on the dynamics that lead to this situation. The dogs will only prevent the students from bringing drugs within the school premises, but outside the schools, they are free to participate in whatever form of drug abuse they desire. You learn how to listen, and admit that you dont know all the answers. Un autre facteur, particulièrement important, est constitué par la prégnance particulièrement influente sur les nouvelles générations sur la vie quot « le nouvel âge télévisuel » 28, caractérisé par le triomphe de la télévision de lintimité 29, laquelle repose sur le témoignage privé faisant irruption dans lespace public, et, en parallèle et en étroite connexion avec ce phénomène, de nouveaux changements dans les frontières entre vie publique et vie privée. Critical care nurses in this study saw their input into a patients care as necessary and important, to both their own well-being and the well-being of their patients. Get One-on-One Help to Address Your Child s Substance Use or call the Partnership for Drug-Free Kids helpline at 1-855-378-4373. Every journal has its own design and layout standards; perusing a journal s articles will give you an idea of the proper number, size, and complexity of your figures. Unit 1 Short Paper Psychoactive Drugs I believe was designed to be used for medical purposes, which I also fee that people who use them are in danger of harming their body and mind. Items often used are either rock salt, red chilies, white pumpkins, oiled cloth, or lemons coated with kumkuma.
Please Note We do not supply Cotswold Holiday brochures - contact the local Visitor Information Centre near to where you want to stay - Click Here for Brochure contact details. Dissertation dSES Sujet : Dans quelle mesure le pouvoir des Etats nationaux est-il contesté par lémergence de nouveaux centres de pouvoir. She has a different personality that any of the other characters and connects with them in a different. Bernard de Fontenelle was an influential French author who contributed to various areas such as philosophy, literature, education, epistemology or theory of knowledge, and education. By this time, Long was in a movie theater; as Long walked out of the theater, he was arrested. 397 416 MYA seem to coincide with the elpistostegid-tetrapod changeover sensu 11. Finding a funny narrative essay within the stack of all of the serious ones causes a reader to take notice, to appreciate the comic relief and makes you essay much more memorable. This particular comic principle relies on the audience falling for a simple trick of misdirection. Should corporations be granted personhood. One they started up all of these colonies and ensured them to become the best that they could possibly be, they passed the South AFrica Act in 1910. After the diagnosis from doctor, it can be considered that these symptom due to the effect of medicine. For example Hitler is evil or God exists is knowable in the sense that it corresponds to events that are occurring in the world.
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What has motivated me to seek this knowledge. The bones of kids and young teens are smaller than those of adults and contain growing zones called growth plates. Previously students were required to have sat at least 40 per cent of an assessment either by submitting coursework or taking earlier exam modules to be considered, but this summer, exam boards lowered the threshold to 25 per cent. No by Patrick Darski Created on October 18, 2009 Is technology making us lazy. Most members of Congress voted for this bill without ever reading it. They, therefore, must be the example of building a corporate culture. Consciousness can be transferred from one substance to another and thus while the soul is changed, consciousness remains the same and thus personal identity is preserved through the change. Unlike the Abstract, which is entirely descriptive, in the Annotated Bibliography, the writer should add some distinctive features of the source to be able to assess and criticize the information.
It appears paradoxical to expect a positive relationship between climate change and violence when annual rates of violence are decreasing, but temperatures trend upward. I end with what I feel is a viable solution to the problem of boys falling behind. Dav Unpacking Duchamp Art in Transit Berkeley, Los Angeles, and London University of California Press, 1995 221-26, but does not discuss the painting s anamorphic characteristics. Blocks can be nested and submitted to interactive tools, like SQL Plus. The Phenomenology Of Gift Giving By Helmuth Berking. Power will be provided to all desks so battery life should not be a concern, beyond that students are expected to provide a machine in an exam-worthy state, or to request a loan machine. Maybe you have picked a research topic from the above categories for your paper. For instance, by terminating the rule of the bankrupt and deeply scandalous Roman nobility, Caesar lend both the Greco-Roman civilization as well as the Roman state a reprieve that would last for up to six centuries Toynbee, 2011. It is vital that the rains come in time or else delayed monsoons may cause drought; and farming also gets affected. To do this, you have to group your notes into categories and then arrange these categories in a logical order. Frank Lloyd Wright introduced the word organic into his philosophy of architecture as early as 1908.
A sphere of flame enclosed a moist mass, more solid at the center where the earth formed, vaporous between. Another respiratory disease, MERS, is also a matter of concern, although the number of cases so far has been small. From one Essay to another they display a spectrum of views, from far-left to far-right. Yet, lifestyle-based tactics are w some importance to the way individual activists chose to live their lives, and activists who embrace practices associated with stereotypical lifestylism are, in reality, rarely motivated purely by individual self-interest. To measure perceived abortion stigma, participants indicated how much they would be looked down upon by people in their communities if they knew they had sought an abortion 0 not at all to 4 extremely. But when God actually does relent and spare Nineveh, Jonah becomes angry and complains, O LORD, is not this what I said when I was yet in my country. And curiously I find the poems in the Shepheardes Calender quite convincingly naturalistic.
62 Had Tchaikovsky written this work as a piano quartet or piano quintet, he would have availed himself of a string complement well able to play complete harmony and could therefore have been allotted autonomous sections to play. Copyright date is 1952 re-newel date is 1980. The booklet contains the rules for each category and some sample problems and solutions. Universal adult franchise is the fundamental of the building of democracy. Here you can find Essay on Indian Village in English language for 5,6,7, 8, 9, 10, 11, 12, and banking or other competetive exams students in 550 words. According to more than 135,000 Niche users, only 2 percent reported having no school dress codes at all. Schor describes today s consumerism as the new consumerism. It helps you narrow your topic and maintain a focus for your speech. The twelfth step of the Alcoholics Anonymous program states that Having had a spiritual awakening as the result of these steps, we tried to carry this message to alcoholics and to practice these principles in all our affairs. Women did not have control over themselves, could not own property and did not have political rights. Consequently, I apologized to her several years ago for being such a horrible teenager and not giving her the respect she deserved because she was always there for me. They are paid well and once they have done there job, they can go on there way with a fat wallet and no worries. British rock n roll began in the 1950 s and it wasn t until the 1960 s when The Beatles heightened the start of the British Invasion. We also asked social media subscribers to engage as well. The new cinemas greatly extended the boundaries of film art. Essay writers here create papers and are ready to provide you with essay help 247. Though Wilfred never goes into full detail of past occurrences within history Notre Dame High School College P HISTORY AP US Hist - Fall 2009. Cellulosic paper products for fruit vegetable packaging. In the professional setting, all people should act in a manner that would uphold the good of society.
The common perception that Iqbal was once a staunch nationalist and later turned in the other direction like his contemporary Jinnah, does not seem to be true and might have originated from an isolated reading of his Urdu poems of this period. Marks for exams that take place within the standard assessment periods will be published following the Examination Boards. While Guterres appointment, via a reformed selection process, was partly an endorsement of his agenda to restructure the secretariat, the plan presented in March 2018 faces several hurdles. Windows Explorer fans nullz has made some. Markus Kichler Dissertation Examples Markus kichler dissertation defense driveto55. 1887 Rural Hours by season from the 1887 author s revised edition, which reduced the original 1850 text by about one-third. I would rather see Oedipus, for example, than be Oedipus. His cadenzas for the rondo itself in each of two spots clear the air with vast torrents of sound that sweep up and down the keyboard. When one or more dimensions is missing or falls short, the imbalance sets off an effect that throws off the entire equilibrium and poise to one s life. Naturalness of speech is somewhat sacrificed, but we gain by the sacrifice a certain uniformity of speech which rests and exhilarates.
When you get used to living in discomfort in the army, suddenly all the things everyone complains about in the civilian world make you say Huh. This is a hypertextual self referential edition of Ulysses. The owner is required to pay capital gains tax when new shares are disposed of at a price than the par value of these shares. Every writer is able to demonstrate his unique talent with different techniques. Only one reference is provided so the claim of some commentators is inappropriate. Resentment is like drinking poison and then hoping it will kill your enemies. I admire the company s mission of providing xyz to xyz. She had observed that perhaps it was a psychological issue, people who had been impoverished, the first thing they wanted to do was emulate the life of the rich - and it had taken them backwards. All his children had died in mysterious circumstances which led him to believe that they had fallen victims to Stalin s vengeance. The State Department also states that the Government of Venezuela does not fully comply with the minimum standards for the elimination of trafficking explaining that Venezuelan authorities trained government officials about trafficking, but the Venezuelan government d 77 78 79. Without exaggeration, we can say that Apple is one of the brightest technology companies that appeared in the 70s of the last century. What I m saying is that those who claim to have compassion, do not, if they fail to do anything practical with that compassion I don t count Tweets and signs and marches with selfies as anything practical. Atwood suggests here that the sight of fertility in Serena s garden is painful and that she is. Fighting between the Communist government in Kabul and the Mujah 45 With Pakistan s backing, the Taliban emerged as one of the strongest factions in Afghanistan. In their relationships with the Church, gay Christians are subjected to the Church s vocabulary of motives that labels their lifestyle as unacceptable. To Kill a Mockingbird by Harper Lee is a well-known coming-of-age convoluted novel that encompasses a trail between a black man and a white man that forces the town of Maycomb to go through experiences that taught them many life lessons. For all we know is that we are capable of everything, thus we are afraid to die. In addition to 33 credit hours of coursework, the completion and submission of the Portfolio is required in the final semester. It was a marvelous experience to meet and talk with the great leaders of India, to meet and talk with and to speak to thousands and thousands of people all over that vast country. The lyrical essay is not organized as a narrative, with one event unfolding after the next.
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I personally do not object to women having the same opportunity as men, but along with rights come responsabilities and not behaving like a victim is one responsability that women seem unable to take on board. The principle of necessity holds that there must be no other, less restrictive policy that achieves the legitimate goal equally well. In order to examine the argument and perspective of the author, understanding his implementation is of great importance. However, you may have to spend some time and cash before you find the best writer for your papers. If we don t have art, how can people know what to do. An exoskeleton can be replaced quite quickly with chitin and protein, or calcium carbonate being deposited. It s unfortunate that President Kennedy didn t trip Tito and then slide down the stair-rail, for he was in a very vulnerable position as related to Masonic sorcery, and such unorthodox action might have rattled the Prince of Harodim. At Francis Bacons cremation no friends were present and the only flowers were from a few drinking partners from the French pub. Criminal opportunity theory and the relationship between poverty and property crime. He deepens this exploration even further by proposing that even if one found out the words making up the definition of library in another language, those words themselves would have other definitions, obscuring the original meaning. Some of the scholars who proposed the various models have been mentioned, with the disadvantages and advantages of working across boundaries being discussed. For example, an accountant who has prepared a consumer s tax return has information that can be used to charge customers based on an estimate of their ability to pay. We are all responsible for the effect that the media has on our young people, because not enough is being done to deter the false images that are being portrayed. Romeo Vitelli, Spare the Rod and Spoil the Child. The Effects Of Technology On Today 's Society. Make mud pies, a traditional rainy day treat enjoyed for generations. This idea was elaborated in the Declarations signed during war time conferences held in Moscow and Tehran in 1943. In addition, the project expanded drinking water systems in six villages, reducing the distance women have to walk to collect water for their families. He addresses God and the issue of slavery in order to encourage the Northern and Southern states towards reconciliation. There are conflicting definitions and legal criteria for determining which groups may legitimately claim the right to self-determination.
What similarities exist between capitalism and communism. Argument Two Hitler s oratory skills were a significant factor in his rise to power. In the past 10 decades, there are numerous scientific reports pointed out the relationships between cardiovascular health and physical activities. Dentists were found to have, on an average, over four times the level of urinary mercury compared to age and education-matched control subjects. Callicles presents himself as a no-holds-barred, bare-knuckled, clear-headed advocate of Realpolitik, as we would now call it. Max Planck, the father of QM who coined the term quanta for the discrete bundles of energy that comprise light, made an insightful statement at the heart of this principle of interrelatedness. I talk to him about how common these fires were and how they played on the minds of the public in this time period. Though the Pawns or soldiers in Chaturanga also moved like a usual pawn, they were not allowed to make the double steps on it first move, like modern Chess. Chang Díaz led the installation of major components of the International Space Station (ISS) and conducted critical repairs on the Canadian ISS Robotic Arm. Sample lyrics Volevo essere alcolizzato, spaccare i camerini Volevo fare il cantante di canzoni inglesi così nessuno capiva che dicevo Odia qualcuno per stare un po meglio, odia qualcuno che stia meglio. We were 6 kids and my mum who wasn t well at the time tried her best to raise us. When China invaded Tibet in 1950, the spiritual warrior Dalai Lama snuck out of the country in the middle of the night, leaving his unarmed people to be slaughtered by the particularly vicious Chinese Army, many of whom forced Tibetan children to execute their own parents at gunpoint.
The character of The Incredible Hulk is a highly a problematic example for young children to follow because they are learning to uncritically accept a sad reality of our society violence out of anger. Are contrast stuck in front of an 1 word document and have no idea how 1 write a compare and contrast essay. It allows the user to upload the document file and check. Grade boundry Grades maths MATH gsce Edexcel igcse biology january 2019 Realistic (and backed up by statistics) grade boundaries for A level maths 2019. In whatever ways it exaggerates, it also condenses a variety of truths about coalitions among executives. Delegates must have previous experience being directly responsible for managing all forms of temporary works to be eligible for this temporary works course. Most novels and plays take far longer to act out. The purpose of this report is to describe a closed talus dislocation without any fracture of the malleoli, which was treated by open reduction. Microsoft and Apple have been neck in neck to out-do each other for so long they ve cross pollinated technology. In contrast, Mycenaean palaces preferred an indoor hall known as a megaron and were constructed with high stone walls and other clearly defensive attributes, signifying the persistent presence of danger.
Parents divorce makes children more likely to divorce in their own marriages. Remember, the slides are secondary to your own verbal presentation. A biosensor is an analytical device for the detection of an analyte that combines a biological component with a physicochemical detector component. Week 6 Case Studies Jina Pak BUS 700B MBA Capstone Prof. Meanwhile, they stand apart from nature, observing nature and developing their culture apart from, but in relation to, nature. In the present turbulent times, religion does give peace of mind to an individual however if religion is used to hurt the sentiments of the people who believe in certain ideology, then censorship should be used to protect the people from getting hurt. Barbara Ehrenreich s Nickel and Dimed Book Review. The Ferret is dedicated to investigative reporting that is pertinent to Scotland and its residents. You don t always leave a good impression, but it is a lasting one. Malloy had a friend that worked for the newspaper. On one hand, positive jurisprudence refers to any legal theory which provides a basis for judicial action in a particular case or situation and or recommends the basic structures for a just state 12.
Social media is the collective of online communications channels dedicated to community-based input, interaction, content-sharing and collaboration WhatIs. This announcement represents the continuation of an AHRQ program that provides support to individuals who are conducting research undertaken as part of an accredited academic program to qualify for a research doctorate degree. One such issue has to do with the manner in whic. In The Shampoo Elizabeth Bishop uses imagery, metaphor, and diction to compare the gradual movements in nature over time with the process of aging. The conclusion may be the last thing you write, but it deserves just as much effort and attention as the rest of your essay. Al snel ging het met de zaken niet goed, en opnieuw werd in Havana overlegd over een aanslag. Byrd s advice to anyone looking for an internship apply early and be completely honest. As part of our PrepScholar program, we have over 4,500 SAT questions customized to each skill. The Merchant of Venice The play, The Merchant of Venice by William Shakespeare has two main settings. However, thanks to my involvement in this particular academic program, I am now much more acclimated with cultural diversity and believe that I have significantly improved my prowess in this aspect of my work as a professional nurse. I would probably to split the massive second paragraph into 2-3 separate paragraphs. Note Names must always appear in the same order, separated by commas, as found on the Title page of the work being cited. The Award was established in 1992 to honor Bernard Fonlon and Lee Nichols for their contributions to both African literature and the freedom of expression. The result was that for untold numbers of our compatriots life was a living hell. 11a b g n ac MIMO GPS none aGPS aGPS aGPS aGPS, GLONASS aGPS, GLONASS aGPS, GLONASS aGPS, GLONASS aGPS, GLONASS aGPS, GLONASS aGPS, GLONASS aGPS, GLONASS SIM Mini Mini Mini Micro Micro Nano Nano Nano Nano Nano Nano Nano Rear Camera 2MP 2MP 3MP 480p 5MP 720p, ƒ2. It takes a good deal of time to eat or to sleep, or to earn a hundred dollars, and a very little time to entertain a hope and an insight which becomes the light of our life. By reading this paper, the reader will gain an understanding of why abortions need to be restricted. Parents and teachers who don t like math can pass that attitude on to kids who then don t like math. Buying condoms at the store may cause feelings of anxiety, which could discourage the student from buying them.

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Halton Hills Estate Sale Online Auction - Chaplin Crescent
Only Available Pickup Date/Time: Sun, August 9 2020 10AM-2PM
Pickup Location: Chaplin Crescent, Halton Hills, ON, L7G 5Y4
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This online auction features a piano, mirrors, model ship, silverplate, candlesticks, vintage chairs, stained glass lamp, dishes, glassware, Corningware, metalware, purple glass stemware, cranberry glass, vintage bar cart, decor, bookends, rotisserie bbq, figurines, books and linens, serving ware, Noritake, bookcase, Christmas village, rugs and much more!
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SANAA, July 13 (Xinhua) -- Yemen's Houthi rebels said on Monday that they launched missile and drone attacks toward the southwest of Saudi Arabia, Houthi-run al-Masirah TV reported.
The attacks targeted a military airport in Khamis Mushait city of Asir Region and an oil facility in the industrial area of Jizan Region, the television said, citing a statement by the Houthi military spokesman Yahya Sarea.
The attacks came in response to the airstrikes by the Saudi-led coalition, it added.
Earlier in the day, the coalition said in a statement aired by Saudi-owned Al Arabiya television that it intercepted and destroyed two ballistic missiles and six bomb-laden drones launched by Yemen's Houthi militia toward the kingdom.
The coalition did not report any casualties.
The Houthi militia frequently respond to the airstrikes by the coalition with missile attacks against Saudi Arabia, mainly its border cities. Saudi Arabia claims to have intercepted most of the missiles.
Yemen has been mired in civil war since late 2014 when the Iran-backed Houthi rebels seized control of much of the country's north and forced the Saudi-backed government of President Abd-Rabbu Mansour Hadi out of the capital Sanaa.
The Saudi-led coalition intervened in the Yemeni conflict in early 2015 to support Hadi's government. Enditem


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Berryville Arkansas
Anasazi refers to the physical remains of a pre-Columbian peasant individuals who lived about a thousand years ago in the 4 Corners region of Colorado, approxi
Cultural Identity And The Archaeological Construction Of Historical Narratives: An Example From Chaco CanyonThe Chaco Canyon Research Institute (CHACO) at the University of California, San Diego (UCSD) in San Francisco, California. The Chaco Canyon Research Institute
From the towering stone structures to its cliffs, the remains inform the story of a culture that spread in the dry southwest in antiquity. In the area known as
The very best known early pottery sites are in North America, where crumbly brown crockery was discovered at websites dating from in between 200 and 500 AD. By
Anasazi were home builders between 950 and 1300 A.D., and they developed a series of excavated houses with architectural functions that made it through into th
The sites may be remote, however a few of them can be checked out throughout the day or on a leisurely weekend through the hinterland. Some believe that the bo
The ancient individuals settled in the plateaus where there was abundant water, such as in the Rio Grande Valley and the Pecos River Valley. In the American So
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This chemical change triggers electrical signals passed from the retina to the visual parts of the brain. They are created due to a malfunction of the forming of the genetic code such as, not correctly copying the complimentary combination of DNA genetic material during replication and transcription, and failing to accurately completing the process of creating RNA during translation.
Colorblindness is a tough disease to conquer, however it is not unconquerable. The major symptoms of Usher syndrome are hearing impairment and retinitis pigmentosa, an eye disorder that causes a person's vision to worsen over time Usher Glasses can be worn to block the glare, as individuals with color vision problems are better able to distinguish between colors when the glare or brightness is less.
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Person suffering from Color blindness will have difficulty seeing the colors red, blue, green or a combination of these colors. Green andred-green Is color blind person see. Certain shades of orange, yellow, and green all look yellow.
Vitamin Deficiency Symptoms Vitamin B2 deficiency symptoms may include:: Print we show that they are good for. Other types are accompanied by additional vision problems and are typically classified as complete color blindness. Keeping your eyes healthy and strong may require some lifestyle changes, but Other than inherited color vision problem, a person may also have an acquired color vision problem, which can be caused by: Mutated genes may cause cells to act differently than expected Zanden, The typical transfer of colorblindness is from a mother carrying the disorder to her son, which will then affect the son.
However some of the most common symptoms of lupus include painful or of lupus include chest pain hair loss anemia a decrease in red blood cells patients may notice dark urine and swelling around their eyes legs ankles or fingers. Female Writers on their Feline Friends.
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Rod monochromacyfrequently called achromatopsia, where the retina contains no cone cells, so that in addition to the absence of color discrimination, vision in lights of normal intensity is difficult. The center of the fovea holds very few blue-sensitive cones.
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Transcript of Cloning is Beneficial to Society. Color Blindness, and the list goes on. Curing Genetic Diseases, and Disorders This form of cloning can definitely be beneficial to society. VHL syndrome Vision impairment and blindness Von Bogaert-Bertrand disease.
Research has demonstrated the essential nutrient you are color blind person cannot different types of color deficiency, what the symptoms of color blindness correction glasses out of hundreds of models had indicated that distinguish between the red and green.
ADVICE FOR TEACHERS OF COLOUR BLIND STUDENTS. Colour vision deficiency (CVD) affects 1 in 12 boys and 1 in girls. There are approximately You will need to have a formal diagnosis of the specific type of colour blindness so that you will be able to. Importance of Vitamins Vitamins are essential to health and growth, and prevention and cure of diseases.
They work synergestically together. Most vitamins cannot be made by the body, and can only be obtained from food and supplements. Color-Blindness-Other Places To Get Help.
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Color Blindness can change a person's life. It can make it harder to read and learn, and certain careers are unavailable (Williams, ).Color vision deficiency syndrome color blindness essay


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Thu Nov 14, 2019 9:06 am #1729813
Does anyone have any scales I can borrow/rent for a day or two to reweigh a Europa Mono? Needs to go to 350Kg
In Milton Keynes.
In Milton Keynes.
Peter Kelly wrote:...They cost ££ to maintain so we have to make a charge....
has to be witnessed by my inspector


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Insights On Cbd Oil Secrets
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Future observations of cosmic microwave background (CMB) polarisation have the potential to answer some of the most fundamental questions of modern physics and cosmology. In this paper, we list the requirements for a future CMB polarisation survey addressing these scientific objectives, and discuss the design drivers of the CORE space mission proposed to ESA in answer to the "M5" call for a medium-sized mission. The rationale and options, and the methodologies used to assess the mission's performance, are of interest to other future CMB mission design studies. CORE is designed as a near-ultimate CMB polarisation mission which, for optimal complementarity with ground-based observations, will perform the observations that are known to be essential to CMB polarisation scienceand cannot be obtained by any other means than a dedicated space mission.
We present an HST/ACS weak gravitational lensing analysis of 13 massive high-redshift (z_median=0.88) galaxy clusters discovered in the South Pole Telescope (SPT) Sunyaev-Zel'dovich Survey. This study is part of a larger campaign that aims to robustly calibrate mass-observable scaling relations over a wide range in redshift to enable improved cosmological constraints from the SPT cluster sample. We introduce new strategies to ensure that systematics in the lensing analysis do not degrade constraints on cluster scaling relations significantly. First, we efficiently remove cluster members from the source sample by selecting very blue galaxies in V-I colour. Our estimate of the source redshift distribution is based on CANDELS data, where we carefully mimic the source selection criteria of the cluster fields. We apply a statistical correction for systematic photometric redshift errors as derived from Hubble Ultra Deep Field data and verified through spatial cross-correlations. We account for the impact of lensing magnification on the source redshift distribution, finding that this is particularly relevant for shallower surveys. Finally, we account for biases in the mass modelling caused by miscentring and uncertainties in the mass-concentration relation using simulations. In combination with temperature estimates from Chandra we constrain the normalisation of the mass-temperature scaling relation ln(E(z) M_500c/10^14 M_sun)=A+1.5 ln(kT/7.2keV) to A=1.81^{+0.24}_{-0.14}(stat.) +/- 0.09(sys.), consistent with self-similar redshift evolution when compared to lower redshift samples. Additionally, the lensing data constrain the average concentration of the clusters to c_200c=5.6^{+3.7}_{-1.8}.
We study the Sunyaev-Zel'dovich effect (SZE) signature in South Pole Telescope (SPT) data for an ensemble of 719 optically identified galaxy clusters selected from 124.6 deg$^2$ of the Dark Energy Survey (DES) science verification data, detecting a stacked SZE signal down to richness $\lambda\sim20$. The SZE signature is measured using matched-filtered maps of the 2500 deg$^2$ SPT-SZ survey at the positions of the DES clusters, and the degeneracy between SZE observable and matched-filter size is broken by adopting as priors SZE and optical mass-observable relations that are either calibrated using SPT selected clusters or through the Arnaud et al. (2010, A10) X-ray analysis. We measure the SPT signal to noise $\zeta$-$\lambda$, relation and two integrated Compton-$y$ $Y_\textrm{500}$-$\lambda$ relations for the DES-selected clusters and compare these to model expectations accounting for the SZE-optical center offset distribution. For clusters with $\lambda > 80$, the two SPT calibrated scaling relations are consistent with the measurements, while for the A10-calibrated relation the measured SZE signal is smaller by a factor of $0.61 \pm 0.12$ compared to the prediction. For clusters at $20 < \lambda < 80$, the measured SZE signal is smaller by a factor of $\sim$0.20-0.80 (between 2.3 and 10~$\sigma$ significance) compared to the prediction, with the SPT calibrated scaling relations and larger $\lambda$ clusters showing generally better agreement. We quantify the required corrections to achieve consistency, showing that there is a richness dependent bias that can be explained by some combination of contamination of the observables and biases in the estimated masses. We discuss possible physical effects, as contamination from line-of-sight projections or from point sources, larger offsets in the SZE-optical centering or larger scatter in the $\lambda$-mass relation at lower richnesses.
We present the stellar mass-halo mass scaling relation for 46 X-ray selected low-mass clusters or groups detected in the XMM-BCS survey with masses $2\times10^{13}M_{\odot}\lesssim M_{500}\lesssim2.5\times10^{14}M_{\odot}$ at redshift $0.1\le z \le1.02$. The cluster binding masses $M_{500}$ are inferred from the measured X-ray luminosities \Lx, while the stellar masses $M_{\star}$ of the galaxy populations are estimated using near-infrared imaging from the SSDF survey and optical imaging from the BCS survey. With the measured \Lx\ and stellar mass $M_{\star}$, we determine the best fit stellar mass-halo mass relation, accounting for selection effects, measurement uncertainties and the intrinsic scatter in the scaling relation. The resulting mass trend is $M_{\star}\propto M_{500}^{0.69\pm0.15}$, the intrinsic (log-normal) scatter is $\sigma_{\ln M_{\star}|M_{500}}=0.36^{+0.07}_{-0.06}$, and there is no significant redshift trend $M_{\star}\propto (1+z)^{-0.04\pm0.47}$, although the uncertainties are still large. We also examine $M_{\star}$ within a fixed projected radius of $0.5$~Mpc, showing that it provides a cluster binding mass proxy with intrinsic scatter of $\approx93\%$ (1$\sigma$ in $M_{500}$). We compare our $M_{\star}=M_{\star}(M_{500}, z)$ scaling relation from the XMM-BCS clusters with samples of massive, SZE-selected clusters ($M_{500}\approx6\times10^{14}M_{\odot}$) and low mass NIR-selected clusters ($M_{500}\approx10^{14}M_{\odot}$) at redshift $0.6\lesssim z \lesssim1.3$. After correcting for the known mass measurement systematics in the compared samples, we find that the scaling relation is in good agreement with the high redshift samples, suggesting that for both groups and clusters the stellar content of the galaxy populations within $R_{500}$ depends strongly on mass but only weakly on redshift out to $z\approx1$.
We present a detection of the enhancement in the number densities of background galaxies induced from lensing magnification and use it to test the Sunyaev-Zel'dovich effect (SZE) inferred masses in a sample of 19 galaxy clusters with median redshift $z\simeq0.42$ selected from the South Pole Telescope SPT-SZ survey. Two background galaxy populations are selected for this study through their photometric colours; they have median redshifts ${z}_{\mathrm{median}}\simeq0.9$ (low-$z$ background) and ${z}_{\mathrm{median}}\simeq1.8$ (high-$z$ background). Stacking these populations, we detect the magnification bias effect at $3.3\sigma$ and $1.3\sigma$ for the low- and high-$z$ backgrounds, respectively. We fit NFW models simultaneously to all observed magnification bias profiles to estimate the multiplicative factor $\eta$ that describes the ratio of the weak lensing mass to the mass inferred from the SZE observable-mass relation. We further quantify systematic uncertainties in $\eta$ resulting from the photometric noise and bias, the cluster galaxy contamination and the estimations of the background properties. The resulting $\eta$ for the combined background populations with $1\sigma$ uncertainties is $0.83\pm0.24\mathrm{(stat)}\pm0.074\mathrm{(sys)}$, indicating good consistency between the lensing and the SZE-inferred masses. We use our best-fit $\eta$ to predict the weak lensing shear profiles and compare these predictions with observations, showing agreement between the magnification and shear mass constraints. This work demonstrates the promise of using the magnification as a complementary method to estimate cluster masses in large surveys.
We present the first results of a survey for high redshift, z $\ge$ 6, quasars using izY multi-colour photometric observations from the Dark Energy Survey (DES). Here we report the discovery and spectroscopic confirmation of the $\rm z_{AB}, Y_{AB}$ = 20.2, 20.2 (M$_{1450}$ = $-$26.5) quasar DES J0454$-$4448 with an emission line redshift of z = 6.10$\pm$0.03 and a HI near zone size of 4.6 $\pm$ 1.7 Mpc.The quasar was selected as an i-band drop out with i$-$z = 2.46 and z$_{AB} < 21.5$ from an area of $\rm \sim$300 deg$^2$. It is the brightest of our 43 candidates and was identified for follow-up spectroscopically solely based on the DES i$-$z and z$-$Y colours. The quasar is detected by WISE and has $W1_{AB} = 19.68$. The discovery of one spectroscopically confirmed quasar with 5.7 $<$ z $<$ 6.5 and z$_{AB} \leq$ 20.2 is consistent with recent determinations of the luminosity function at z $\sim$ 6. DES when completed will have imaged $\rm \sim$5000 deg$^2$ to $Y_{AB}$ = 23.0 ($5\sigma$ point source) and we expect to discover $>$ 50-100 new quasars with z $>$ 6 including 3-10 with z $>$ 7 dramatically increasing the numbers of quasars currently known that are suitable for detailed studies including determination of the neutral HI fraction of the intergalactic medium (IGM) during the epoch of Hydrogen reionization.
Using the science verification data of the Dark Energy Survey (DES) for a new sample of 106 X-Ray selected clusters and groups, we study the stellar mass growth of Bright Central Galaxies (BCGs) since redshift 1.2. Compared with the expectation in a semi-analytical model applied to the Millennium Simulation, the observed BCGs become under-massive/under-luminous with decreasing redshift. We incorporate the uncertainties associated with cluster mass, redshift, and BCG stellar mass measurements into analysis of a redshift-dependent BCG-cluster mass relation, $m_{*}\propto(\frac{M_{200}}{1.5\times 10^{14}M_{\odot}})^{0.24\pm 0.08}(1+z)^{-0.19\pm0.34}$, and compare the observed relation to the model prediction. We estimate the average growth rate since $z = 1.0$ for BCGs hosted by clusters of $M_{200, z}=10^{13.8}M_{\odot}$, at $z=1.0$: $m_{*, BCG}$ appears to have grown by $0.13\pm0.11$ dex, in tension at $\sim 2.5 \sigma$ significance level with the $0.40$ dex growth rate expected from the semi-analytic model. We show that the buildup of extended intra-cluster light after $z=1.0$ may alleviate this tension in BCG growth rates.
We study the stellar, Brightest Cluster Galaxy (BCG) and intracluster medium (ICM) masses of 14 South Pole Telescope (SPT) selected galaxy clusters with median redshift $z=0.9$ and median mass $M_{500}=6\times10^{14}M_{\odot}$. We estimate stellar masses for each cluster and BCG using six photometric bands spanning the range from the ultraviolet to the near-infrared observed with the VLT, HST and Spitzer. The ICM masses are derived from Chandra and XMM-Newton X-ray observations, and the virial masses are derived from the SPT Sunyaev-Zel'dovich Effect signature. At $z=0.9$ the BCG mass $M_{\star}^{\textrm{BCG}}$ constitutes $0.12\pm0.01$% of the halo mass for a $6\times10^{14}M_{\odot}$ cluster, and this fraction falls as $M_{500}^{-0.58\pm0.07}$. The cluster stellar mass function has a characteristic mass $M_{0}=10^{11.0\pm0.1}M_{\odot}$, and the number of galaxies per unit mass in clusters is larger than in the field by a factor $1.65\pm0.2$. Both results are consistent with measurements on group scales and at lower redshift. We combine our SPT sample with previously published samples at low redshift that we correct to a common initial mass function and for systematic differences in virial masses. We then explore mass and redshift trends in the stellar fraction (fstar), the ICM fraction (fICM), the cold baryon fraction (fc) and the baryon fraction (fb). At a pivot mass of $6\times10^{14}M_{\odot}$ and redshift $z=0.9$, the characteristic values are fstar=$1.1\pm0.1$%, fICM=$9.6\pm0.5$%, fc=$10.4\pm1.2$% and fb=$10.7\pm0.6$%. These fractions all vary with cluster mass at high significance, indicating that higher mass clusters have lower fstar and fc and higher fICM and fb. When accounting for a 15% systematic virial mass uncertainty, there is no statistically significant redshift trend at fixed mass in these baryon fractions. (abridged)
Due to their proximity, high dark-matter content, and apparent absence of non-thermal processes, Milky Way dwarf spheroidal satellite galaxies (dSphs) are excellent targets for the indirect detection of dark matter. Recently, eight new dSph candidates were discovered using the first year of data from the Dark Energy Survey (DES). We searched for gamma-ray emission coincident with the positions of these new objects in six years of Fermi Large Area Telescope data. We found no significant excesses of gamma-ray emission. Under the assumption that the DES candidates are dSphs with dark matter halo properties similar to the known dSphs, we computed individual and combined limits on the velocity-averaged dark matter annihilation cross section for these new targets. If the estimated dark-matter content of these dSph candidates is confirmed, they will constrain the annihilation cross section to lie below the thermal relic cross section for dark matter particles with masses < 20 GeV annihilating via the b-bbar or tau+tau- channels.
We cross-match galaxy cluster candidates selected via their Sunyaev-Zel'dovich effect (SZE) signatures in 129.1 deg$^2$ of the South Pole Telescope 2500d SPT-SZ survey with optically identified clusters selected from the Dark Energy Survey (DES) science verification data. We identify 25 clusters between $0.1\lesssim z\lesssim 0.8$ in the union of the SPT-SZ and redMaPPer (RM) samples. RM is an optical cluster finding algorithm that also returns a richness estimate for each cluster. We model the richness $\lambda$-mass relation with the following function $\langle\ln\lambda|M_{500}\rangle\propto B_\lambda\ln M_{500}+C_\lambda\ln E(z)$ and use SPT-SZ cluster masses and RM richnesses $\lambda$ to constrain the parameters. We find $B_\lambda= 1.14^{+0.21}_{-0.18}$ and $C_\lambda=0.73^{+0.77}_{-0.75}$. The associated scatter in mass at fixed richness is $\sigma_{\ln M|\lambda} = 0.18^{+0.08}_{-0.05}$ at a characteristic richness $\lambda=70$. We demonstrate that our model provides an adequate description of the matched sample, showing that the fraction of SPT-SZ selected clusters with RM counterparts is consistent with expectations and that the fraction of RM selected clusters with SPT-SZ counterparts is in mild tension with expectation. We model the optical-SZE cluster positional offset distribution with the sum of two Gaussians, showing that it is consistent with a dominant, centrally peaked population and a sub-dominant population characterized by larger offsets. We also cross-match the RM catalog with SPT-SZ candidates below the official catalog threshold significance $\xi=4.5$, using the RM catalog to provide optical confirmation and redshifts for additional low-$\xi$ SPT-SZ candidates.In this way, we identify 15 additional clusters with $\xi\in [4,4.5]$ over the redshift regime explored by RM in the overlapping region between DES science verification data and the SPT-SZ survey.
(Abridged) We use 95, 150, and 220GHz observations from the SPT to examine the SZE signatures of a sample of 46 X-ray selected groups and clusters drawn from ~6 deg^2 of the XMM-BCS. These systems extend to redshift z=1.02, have characteristic masses ~3x lower than clusters detected directly in the SPT data and probe the SZE signal to the lowest X-ray luminosities (>10^42 erg s^-1) yet. We develop an analysis tool that combines the SZE information for the full ensemble of X-ray-selected clusters. Using X-ray luminosity as a mass proxy, we extract selection-bias corrected constraints on the SZE significance- and Y_500-mass relations. The SZE significance- mass relation is in good agreement with an extrapolation of the relation obtained from high mass clusters. However, the fit to the Y_500-mass relation at low masses, while in good agreement with the extrapolation from high mass SPT clusters, is in tension at 2.8 sigma with the constraints from the Planck sample. We examine the tension with the Planck relation, discussing sample differences and biases that could contribute. We also present an analysis of the radio galaxy point source population in this ensemble of X-ray selected systems. We find 18 of our systems have 843 MHz SUMSS sources within 2 arcmin of the X-ray centre, and three of these are also detected at significance >4 by SPT. Of these three, two are associated with the group brightest cluster galaxies, and the third is likely an unassociated quasar candidate. We examine the impact of these point sources on our SZE scaling relation analyses and find no evidence of biases. We also examine the impact of dusty galaxies using constraints from the 220 GHz data. The stacked sample provides 2.8$\sigma$ significant evidence of dusty galaxy flux, which would correspond to an average underestimate of the SPT Y_500 signal that is (17+-9) per cent in this sample of low mass systems.
We report the discovery of eight new Milky Way companions in ~1,800 deg^2 of optical imaging data collected during the first year of the Dark Energy Survey (DES). Each system is identified as a statistically significant over-density of individual stars consistent with the expected isochrone and luminosity function of an old and metal-poor stellar population. The objects span a wide range of absolute magnitudes (M_V from -2.2 mag to -7.4 mag), physical sizes (10 pc to 170 pc), and heliocentric distances (30 kpc to 330 kpc). Based on the low surface brightnesses, large physical sizes, and/or large Galactocentric distances of these objects, several are likely to be new ultra-faint satellite galaxies of the Milky Way and/or Magellanic Clouds. We introduce a likelihood-based algorithm to search for and characterize stellar over-densities, as well as identify stars with high satellite membership probabilities. We also present completeness estimates for detecting ultra-faint galaxies of varying luminosities, sizes, and heliocentric distances in the first-year DES data.
We measure the weak-lensing masses and galaxy distributions of four massive galaxy clusters observed during the Science Verification phase of the Dark Energy Survey. This pathfinder study is meant to 1) validate the DECam imager for the task of measuring weak-lensing shapes, and 2) utilize DECam's large field of view to map out the clusters and their environments over 90 arcmin. We conduct a series of rigorous tests on astrometry, photometry, image quality, PSF modeling, and shear measurement accuracy to single out flaws in the data and also to identify the optimal data processing steps and parameters. We find Science Verification data from DECam to be suitable for the lensing analysis described in this paper. The PSF is generally well-behaved, but the modeling is rendered difficult by a flux-dependent PSF width and ellipticity. We employ photometric redshifts to distinguish between foreground and background galaxies, and a red-sequence cluster finder to provide cluster richness estimates and cluster-galaxy distributions. By fitting NFW profiles to the clusters in this study, we determine weak-lensing masses that are in agreement with previous work. For Abell 3261, we provide the first estimates of redshift, weak-lensing mass, and richness. In addition, the cluster-galaxy distributions indicate the presence of filamentary structures attached to 1E 0657-56 and RXC J2248.7-4431, stretching out as far as 1 degree (approximately 20 Mpc), showcasing the potential of DECam and DES for detailed studies of degree-scale features on the sky.
Let $X$ be a finite set and $\Omega=\{1,...,d\}^{\mathbb{N}}$ be the Bernoulli space. Denote by $\sigma$ the shift map acting on $\Omega$. For a fixed probability $\mu$ on $X$ with supp($\mu$)$=X$, define $\Pi(\mu,\sigma)$ as the set of all Borel probabilities $\pi \in P(X\times \Omega)$ such that the $x$-marginal of $\pi$ is $\mu $ and the $y$-marginal of $\pi$ is $\sigma$-invariant. We consider a fixed Lipschitz cost function $c: X \times \Omega \to \mathbb{R}$ and an associated Ruelle operator. We introduce the concept of Gibbs plan, which is a probability on $X \times \Omega$. Moreover, we define entropy, pressure and equilibrium plans. The study of equilibrium plans can be seen as a generalization of the optimal cost problem where the concept of entropy is introduced. We show that an equilibrium plan is a Gibbs plan. Our main result is a Kantorovich duality Theorem on this setting. The pressure plays an important role in the establishment of the notion of admissible pair. Finally, given a parameter $\beta$, which plays the role of the inverse of temperature, we consider equilibrium plans for $\beta c$ and its limit $\pi_\infty$, when $\beta \to \infty$, which is also known as ground state. We compare this with other previous results on Ergodic Transport in temperature zero.
Major astrophysical questions related to the formation and evolution of structures, and more specifically of galaxy groups and clusters, will still be open in the coming decade and beyond: what is the interplay of galaxy, supermassive black hole, and intergalactic gas evolution in the most massive objects in the Universe - galaxy groups and clusters? What are the processes driving the evolution of chemical enrichment of the hot diffuse gas in large-scale structures? How and when did the first galaxy groups in the Universe, massive enough to bind more than 10^7 K gas, form? Focussing on the period when groups and clusters assembled (0.5<z<2.5), we show that, due to the continuum and line emission of this hot intergalactic gas at X-ray wavelengths, Athena+, combining high sensitivity with excellent spectral and spatial resolution, will deliver breakthrough observations in view of the aforementioned issues. Indeed, the physical and chemical properties of the hot intra-cluster gas, and their evolution across time, are a key to understand the co-evolution of galaxy and supermassive black hole within their environments.
eROSITA is the primary instrument on the Russian SRG mission. In the first four years of scientific operation after its launch, foreseen for 2014, it will perform a deep survey of the entire X-ray sky. In the soft X-ray band (0.5-2 keV), this will be about 20 times more sensitive than the ROSAT all sky survey, while in the hard band (2-10 keV) it will provide the first ever true imaging survey of the sky at those energies. Such a sensitive all-sky survey will revolutionize our view of the high-energy sky, and calls for major efforts in synergic, multi-wavelength wide area surveys in order to fully exploit the scientific potential of the X-ray data. The design-driving science of eROSITA is the detection of very large samples (~10^5 objects) of galaxy clusters out to redshifts z>1, in order to study the large scale structure in the Universe, test and characterize cosmological models including Dark Energy. eROSITA is also expected to yield a sample of around 3 millions Active Galactic Nuclei, including both obscured and un-obscured objects, providing a unique view of the evolution of supermassive black holes within the emerging cosmic structure. The survey will also provide new insights into a wide range of astrophysical phenomena, including accreting binaries, active stars and diffuse emission within the Galaxy, as well as solar system bodies that emit X-rays via the charge exchange process. Finally, such a deep imaging survey at high spectral resolution, with its scanning strategy sensitive to a range of variability timescales from tens of seconds to years, will undoubtedly open up a vast discovery space for the study of rare, unpredicted, or unpredictable high-energy astrophysical phenomena. In this living document we present a comprehensive description of the main scientific goals of the mission, with strong emphasis on the early survey phases.
We describe an initiative to build and use the Dark Energy Spectrometer (DESpec), a wide-field spectroscopic survey instrument for the Blanco 4 meter telescope at Cerro Tololo InterAmerican Observatory (CTIO) in Chile. A new system with about 4000 robotically positioned optical fibers will be interchangeable with the CCD imager of the existing Dark Energy Camera (DECam), accessing a field of view of 3.8 square degrees in a single exposure. The proposed instrument will be operated by CTIO and available for use by the astronomy community. Our collaboration proposes to use DESpec to conduct a wide, deep spectroscopic survey to study Dark Energy. In a survey of about 350 nights, the DESpec collaboration proposes to obtain spectroscopic redshifts for about 8 million galaxies over 5000 square degrees selected from the Dark Energy Survey (DES). This Dark Energy Spectroscopic Survey will advance our knowledge of cosmic expansion and structure growth significantly beyond that obtainable with imaging-only surveys. Since it adds a spectroscopic third dimension to the same sky as DES, DESpec will enable increasingly precise techniques to discriminate among alternative explanations of cosmic acceleration, such as Dark Energy and Modified Gravity.
We study the use of red sequence selected galaxy spectroscopy for unbiased estimation of galaxy cluster masses. We use the publicly available galaxy catalog produced using the semi-analytic model of De Lucia & Blaizot (2007) on the Millenium Simulation (Springel et al. 2005). We explore the impacts on selection using galaxy color, projected separation from the cluster center, and galaxy luminosity. We study the relationship between cluster mass and velocity dispersion and identify and characterize the following sources of bias and scatter: halo triaxiality, dynamical friction of red luminous galaxies and interlopers. We show that due to halo triaxiality the intrinsic scatter of estimated line of sight dynamical mass is about three times larger (30-40%) than the one estimated using the 3D velocity dispersion (~12%) and a small bias (~1%) is induced. We find evidence of increasing scatter as a function of redshift and provide a fitting formula to account for it. We characterize the amount of bias and scatter introduced by dynamical friction when using subsamples of red-luminous galaxies to estimate the velocity dispersion. We study the presence of interlopers in spectroscopic samples and their effect on the estimated cluster dynamical mass. Our results show that while cluster velocity dispersions extracted from a few dozen red sequence selected galaxies do not provide precise masses on a single cluster basis, an ensemble of cluster velocity dispersions can be combined to produce a precise calibration of a cluster survey mass observable relation. Currently, disagreements in the literature on simulated subhalo velocity dispersion mass relations place a systematic floor on velocity dispersion mass calibration at the 15% level in mass. We show that the selection related uncertainties are small by comparison, providing hope that with further improvements this systematic floor can be reduced.
The South Pole Telescope (SPT) is a 10 meter telescope operating at mm wavelengths. It has recently completed a three-band survey covering 2500 sq. degrees. One of the survey's main goals is to detect galaxy clusters using Sunyaev-Zeldovich effect and use these clusters for a variety of cosmological and astrophysical studies such as the dark energy equation of state, the primordial non-gaussianity and the evolution of galaxy populations. Since 2005, we have been engaged in a comprehensive optical and near-infrared followup program (at wavelengths between 0.4 and 5 {\mu}m) to image high-significance SPT clusters, to measure their photometric redshifts, and to estimate the contamination rate of the candidate lists. These clusters are then used for various cosmological and astrophysical studies.
We consider $(M,d)$ a connected and compact manifold and we denote by $\mathcal{B}_i$ the Bernoulli space $M^{\Z}$ of sequences represented by $$x=(... x_{-3},x_{-2},x_{-1},x_0,x_1,x_2,x_3,...),$$ where $x_i$ belongs to the space (alphabet) $M$. The case where $M=\mathbb{S}^1$, the unit circle, is of particular interest here. The analogous problem in the one-dimensional lattice $\mathbb{N}$ is also considered. %In this case we consider the potential $A: {\cal B}=M^\mathbb{N} \to \mathbb{R}.$ Let $A: \mathcal{B}_i \rar \R$ be an {\it observable} or {\it potential} defined in the Bernoulli space $\mathcal{B}_i$. The potential $A$ describes an interaction between sites in the one-dimensional lattice $M^\mathbb{Z}$. Given a temperature $T$, we analyze the main properties of the Gibbs state $\hat{\mu}_{\frac{1}{T} A}$ which is a certain probability measure over ${\cal B}_i$. We denote this setting "the general XY model". In order to do our analysis we consider the Ruelle operator associated to $\frac{1}{T} A$, and, we get in this procedure the main eigenfunction $\psi_{\frac{1}{T} A}$. Later, we analyze selection problems when temperature goes to zero: a) existence, or not, of the limit (on the uniform convergence) $$V:=\lim_{T\to 0} T\, \log(\psi_{\frac{1}{T} A}),\,\,\,\,\text{a question about selection of subaction},$$ and, b) existence, or not, of the limit (on the weak$^*$ sense) $$\tilde{\mu}:=\lim_{T\to 0} \hat{\mu}_{\frac{1}{T}\, A},\,\,\,\,\text{a question about selection of measure}.$$ The existence of subactions and other properties of Ergodic Optimization are also considered.
Euclid is a space-based survey mission from the European Space Agency designed to understand the origin of the Universe's accelerating expansion. It will use cosmological probes to investigate the nature of dark energy, dark matter and gravity by tracking their observational signatures on the geometry of the universe and on the cosmic history of structure formation. The mission is optimised for two independent primary cosmological probes: Weak gravitational Lensing (WL) and Baryonic Acoustic Oscillations (BAO). The Euclid payload consists of a 1.2 m Korsch telescope designed to provide a large field of view. It carries two instruments with a common field-of-view of ~0.54 deg2: the visual imager (VIS) and the near infrared instrument (NISP) which contains a slitless spectrometer and a three bands photometer. The Euclid wide survey will cover 15,000 deg2 of the extragalactic sky and is complemented by two 20 deg2 deep fields. For WL, Euclid measures the shapes of 30-40 resolved galaxies per arcmin2 in one broad visible R+I+Z band (550-920 nm). The photometric redshifts for these galaxies reach a precision of dz/(1+z) < 0.05. They are derived from three additional Euclid NIR bands (Y, J, H in the range 0.92-2.0 micron), complemented by ground based photometry in visible bands derived from public data or through engaged collaborations. The BAO are determined from a spectroscopic survey with a redshift accuracy dz/(1+z) =0.001. The slitless spectrometer, with spectral resolution ~250, predominantly detects Ha emission line galaxies. Euclid is a Medium Class mission of the ESA Cosmic Vision 2015-2025 programme, with a foreseen launch date in 2019. This report (also known as the Euclid Red Book) describes the outcome of the Phase A study.
The Dark Energy Survey (DES) is a project with the goal of building, installing and exploiting a new 74 CCD-camera at the Blanco telescope, in order to study the nature of cosmic acceleration. It will cover 5000 square degrees of the southern hemisphere sky and will record the positions and shapes of 300 million galaxies up to redshift 1.4. The survey will be completed using 525 nights during a 5-year period starting in 2012. About O(1 TB) of raw data will be produced every night, including science and calibration images. The DES data management system has been designed for the processing, calibration and archiving of these data. It is being developed by collaborating DES institutions, led by NCSA. In this contribution, we describe the basic functions of the system, what kind of scientific codes are involved and how the Data Challenge process works, to improve simultaneously the Data Management system algorithms and the Science Working Group analysis codes.
We report on the discovery of the X-ray luminous cluster XMMU J100750.5+125818 at redshift 1.082 based on 19 spectroscopic members, which displays several strong lensing features. SED modeling of the lensed arc features from multicolor imaging with the VLT and the LBT reveals likely redshifts ~2.7 for the most prominent of the lensed background galaxies. Mass estimates are derived for different radii from the velocity dispersion of the cluster members, M_200 ~ 1.8 10^{14} Msun, from the X-ray spectral parameters, M_500 ~ 1.0 10^{14} Msun, and the largest lensing arc, M_SL ~ 2.3 10^{13} Msun. The projected spatial distribution of cluster galaxies appears to be elongated, and the brightest galaxy lies off center with respect to the X-ray emission indicating a not yet relaxed structure. XMMU J100750.5+125818 offers excellent diagnostics of the inner mass distribution of a distant cluster with a combination of strong and weak lensing, optical and X-ray spectroscopy.
We report on the discovery of two galaxy clusters, SPT-CL J2332-5358 and SPT-CL J2342-5411, in X-rays. These clusters were also independently detected through their Sunyaev-Zel'dovich effect by the South Pole Telescope, and confirmed in the optical band by the Blanco Cosmology Survey. They are thus the first clusters detected under survey conditions by all major cluster search approaches. The X-ray detection is made within the frame of the XMM-BCS cluster survey utilizing a novel XMM-Newton mosaic mode of observations. The present study makes the first scientific use of this operation mode. We estimate the X-ray spectroscopic temperature of SPT-CL J2332-5358 (at redshift z=0.32) to T = 9.3 (+3.3/-1.9) keV, implying a high mass, M_{500} = 8.8 +/- 3.8 \times 10^{14} M_{sun}. For SPT-CL J2342-5411, at z=1.08, the available X-ray data doesn't allow us to directly estimate the temperature with good confidence. However, using our measured luminosity and scaling relations we estimate that T = 4.5 +/- 1.3 keV and M_{500} = 1.9 +/- 0.8 \times 10^{14} M_{sun}. We find a good agreement between the X-ray masses and those estimated from the Sunyaev-Zel'dovich effect.
The amount and nature of dark energy (DE) can be tightly constrained by measuring the spatial correlation features and evolution of a sample of ~ 100,000 galaxy clusters over the redshift range 0<z < 1.5. Such an X-ray survey will discover all collapsed structures with mass above 3.5e14 solar masss at redshifts z<2 (i.e. the full range where such objects are expected) in the high Galactic latitude sky. Above this mass threshold the tight correlations between X-ray observables and mass allow direct interpretation of the data. We describe the constraints on Dark Energy that can be inferred from such a survey, using powerful self-calibration techniques to relate the X-ray observables (luminosity and temperature) to the underlying mass.


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The Throne of Grace
May 10, 2020 Series: Hebrews
Passage: Hebrews 4:14–4:16
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Without the Cross, the throne of God is a place of terror and judgment. But because Jesus completed the work of redemption, you can be confident, for those who trust in Christ, that He is smiling upon you ready to pour out mercy and grace, ready to give you more of Himself, in your time of need.
More in Hebrews
August 2, 2020Full Assurance
May 17, 2020Qualified and Appointed
May 3, 2020The Sword of God's Word


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CMST 3RR3 Race, Religion and Media
Academic Year: Winter 2018
Term: Winter
Day/Evening: D
Instructor: Dr. Faiza Hirji
Office: Togo Salmon Hall 305
Phone: 905-525-9140 x 21480
Office Hours: Thursday, 12:30-1:20 PM or by appointment
- Course Objectives
- Textbooks, Materials & Fees
- Method of Assessment
- Policy on Missed Work, Extensions, and Late Penalties
- Additional Policies and Statements
- Topics and Readings
Course Objectives:
Students will acquire/enhance an understanding of theories related to race, religion and media, as well as relevant methodologies, and will be able to apply these in an analysis of different media forms. They will refine their ability to research and communicate such ideas through informal presentations and written assignments.
Textbooks, Materials & Fees:
Course Text: All readings for this course can be found online or on reserve.
Method of Assessment:
Course Requirements:
Participation 10% ongoing
Journal Entry #1 5% due in class January 11, 2018
Journal Entry #2 5% due in class January 18, 2018
Journal Entry #3 10% due in class January 25, 2018
Journal Entry #4 10% due in class February 8, 2018
Journal Entry #5 5% due in class April 3, 2018
Quiz 10% in class on March 6, 2018
Essay 25% due in class on March 22, 2018
Final Exam 20% during the scheduled exam period
Note: Omitting to submit any of the above assignments may result in automatic failure.
Students are expected to attend class regularly and on time, and to participate in a manner that reflects knowledge of the assigned readings. This may include contribution to discussion, answering questions and completing in-class exercises, such as written responses to questions and film clips, group work or mock debates. Disruptive behaviour (which includes texting in class and using your laptop for non-course-related purposes) and tardiness will negatively affect the participation mark. Attendance in itself is not enough to secure full participation marks.
Please note: in this course, we discuss subject matter that may be sensitive or controversial. Students may hold strong opinions on some of the topics that will be discussed. Our classroom should be an inclusive and welcoming place. Please be thoughtful and respectful of others in your comments.
Journal Entries:
Students will submit short journal entries on the dates noted above. Each journal entry will respond to that week's course content in some way: the instructor will outline a specific question or issue to be addressed in each journal entry. In some weeks, the journal entry is worth more because students will be asked to engage in a more complex exercise.
Journal entries will generally be a maximum of 2 pages double-spaced unless the instructor notes otherwise. Journal entries should be submitted both in hard copy and on Avenue to Learn. Each journal entry will be marked for degree of engagement with the subject matter, understanding of the complexities of issues raised, and relevance of examples cited. The writing style can be informal.
There will be a short quiz in class on March 10. This quiz will test students on examples and concepts learned to date. The quiz will include multiple choice, fill-in-the-blank and short answer questions.
Research Essay:
Potential topics will be provided for the final essay, but students may also choose their own after consulting with the instructor. In each case, the essay will engage with subject matter discussed throughout the course, including appropriate theoretical concepts. The essay should include appropriate background on the topic, relevant theoretical perspectives and evidence supported by academic sources. The essay should be a maximum of 10-12 pages, including bibliography, and formatted using APA or MLA. The essay is due in class on March 22, 2018, and should also be submitted through Avenue to Learn.
NOTE: You must submit your own original work, completed independently. Work that has been submitted elsewhere, uses unattributed passages from the work of others, or that has been borrowed from another source, is considered plagiarism and the consequences may be severe. Please see below for further information regarding McMaster's policy on academic integrity.
Final Exam:
There is a final examination for this course during the scheduled examination period. The exam will cover all content from the semester. The format will be explained in greater detail in class but it will include different types of questions.
Policy on Missed Work, Extensions, and Late Penalties:
Late assignments will be penalized one letter grade for each weekday after the deadline (e.g. an A grade becomes an A-, a B- becomes a C+, and so on). For your own protection, always keep a copy of any assignment you hand in.
Please Note the Following Policies and Statements:
Academic Integrity
You are expected to exhibit honesty and use ethical behaviour in all aspects of the learning process. Academic credentials you earn are rooted in principles of honesty and academic integrity. It is your responsibility to understand what constitutes academic dishonesty.
Academic dishonesty is to knowingly act or fail to act in a way that results or could result in unearned academic credit or advantage. This behaviour can result in serious consequences, e.g. the grade of zero on an assignment, loss of credit with a notation on the transcript (notation reads: "Grade of F assigned for academic dishonesty"), and/or suspension or expulsion from the university. For information on the various types of academic dishonesty please refer to the Academic Integrity Policy, located at https://secretariat.mcmaster.ca/university-policies-procedures-guidelines/
The following illustrates only three forms of academic dishonesty:
- plagiarism, e.g. the submission of work that is not one's own or for which other credit has been obtained.
- improper collaboration in group work.
- copying or using unauthorized aids in tests and examinations.
Authenticity / Plagiarism Detection
Some courses may use a web-based service (Turnitin.com) to reveal authenticity and ownership of student submitted work. For courses using such software, students will be expected to submit their work electronically either directly to Turnitin.com or via Avenue to Learn (A2L) plagiarism detection (a service supported by Turnitin.com) so it can be checked for academic dishonesty.
Students who do not wish to submit their work through A2L and/or Turnitin.com must still submit an electronic and/or hardcopy to the instructor. No penalty will be assigned to a student who does not submit work to Turnitin.com or A2L. All submitted work is subject to normal verification that standards of academic integrity have been upheld (e.g., on-line search, other software, etc.). To see the Turnitin.com Policy, please go to www.mcmaster.ca/academicintegrity.
Courses with an On-Line Element
Some courses use on-line elements (e.g. e-mail, Avenue to Learn (A2L), LearnLink, web pages, capa, Moodle, ThinkingCap, etc.). Students should be aware that, when they access the electronic components of a course using these elements, private information such as first and last names, user names for the McMaster e-mail accounts, and program affiliation may become apparent to all other students in the same course. The available information is dependent on the technology used. Continuation in a course that uses on-line elements will be deemed consent to this disclosure. If you have any questions or concerns about such disclosure please discuss this with the course instructor.
Online Proctoring
Some courses may use online proctoring software for tests and exams. This software may require students to turn on their video camera, present identification, monitor and record their computer activities, and/or lockdown their browser during tests or exams. This software may be required to be installed before the exam begins.
Conduct Expectations
As a McMaster student, you have the right to experience, and the responsibility to demonstrate, respectful and dignified interactions within all of our living, learning and working communities. These expectations are described in the Code of Student Rights & Responsibilities (the "Code"). All students share the responsibility of maintaining a positive environment for the academic and personal growth of all McMaster community members, whether in person or online.
It is essential that students be mindful of their interactions online, as the Code remains in effect in virtual learning environments. The Code applies to any interactions that adversely affect, disrupt, or interfere with reasonable participation in University activities. Student disruptions or behaviours that interfere with university functions on online platforms (e.g. use of Avenue 2 Learn, WebEx or Zoom for delivery), will be taken very seriously and will be investigated. Outcomes may include restriction or removal of the involved students' access to these platforms.
Academic Accommodation of Students with Disabilities
Students with disabilities who require academic accommodation must contact Student Accessibility Services (SAS) at 905-525-9140 ext. 28652 or firstname.lastname@example.com e-mail to make arrangements with a Program Coordinator. For further information, consult McMaster University's Academic Accommodation of Students with Disabilities policy.
Email correspondence policy
It is the policy of the Faculty of Humanities that all email communication sent from students to instructors (including TAs), and from students to staff, must originate from each student's own McMaster University email account. This policy protects confidentiality and confirms the identity of the student. Instructors will delete emails that do not originate from a McMaster email account.
Modification of course outlines
The University reserves the right to change dates and/or deadlines etc. for any or all courses in the case of an emergency situation or labour disruption or civil unrest/disobedience, etc. If a modification becomes necessary, reasonable notice and communication with the students will be given with an explanation and the opportunity to comment on changes. Any significant changes should be made in consultation with the Department Chair.
Request for Relief for Missed Academic Term Work
McMaster Student Absence Form (MSAF)
In the event of an absence for medical or other reasons, students should review and follow the Academic Regulation in the Undergraduate Calendar "Requests for Relief for Missed Academic Term Work".
Academic Accommodation for Religious, Indigenous and Spiritual Observances (RISO)
Students requiring academic accommodation based on religious, indigenous or spiritual observances should follow the procedures set out in the RISO policy. Students should submit their request to their Faculty Office normally within 10 working days of the beginning of term in which they anticipate a need for accommodation or to the Registrar's Office prior to their examinations. Students should also contact their instructors as soon as possible to make alternative arrangements for classes, assignments, and tests.
Copyright and Recording
Students are advised that lectures, demonstrations, performances, and any other course material provided by an instructor include copyright protected works. The Copyright Act and copyright law protect every original literary, dramatic, musical and artistic work, including lectures by University instructors.
The recording of lectures, tutorials, or other methods of instruction may occur during a course. Recording may be done by either the instructor for the purpose of authorized distribution, or by a student for the purpose of personal study. Students should be aware that their voice and/or image may be recorded by others during the class. Please speak with the instructor if this is a concern for you.
Extreme Circumstances
The University reserves the right to change the dates and deadlines for any or all courses in extreme circumstances (e.g., severe weather, labour disruptions, etc.). Changes will be communicated through regular McMaster communication channels, such as McMaster Daily News, A2L and/or McMaster email.
Topics and Readings:
(Schedule of Readings will be provided at the first class)
January 4: Introduction and overview
January 9 & 11: Race Matters: The Difference that Race and Religion Still Make
**Journal Entry #1 due January 11**
January 16 & 18: Birth of a Nation: Media Myths We Still Believe
**Journal Entry #2 due January 18**
January 23 & 25: "All Lives Matter…": News Coverage of Minorities
**Journal Entry #3 due January 25**
January 30, February 1: Been Around the World: Diasporic Media
February 6 & 8: Blurred Lines: When TV & Film Make the News, Part I
**Journal Entry #4 due February 8**
February 13 & 15: #OscarsStillSoWhite? TV & Film Part II
February 20 & 22: Winter Break!
February 27, March 1: Missing Voices: Indigeneity in Mainstream Media
Guest lecture on March 1 by Dr. Amber Dean
March 6 & 8: Diff'rent Strokes: Race and Religion in Children's Media
March 13 & 15: Fight the Power: Race and Religion in the Music Industry
Guest lecture on March 13 by Dr. Christina Baade
March 20 & 22: Laughing Through the Pain: Comedy Tackles Race and Religion
**Essay due on March 22**
March 27 & 29: When the Personal is Always Political: Debates on Social Media
April 3 & 5: Light…at the Beginning and End of the Tunnel
**Final Journal Entry Due**
**Final exam will take place during the scheduled examination period**