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Yet another very belated update as still suffering from the effects of the pipeline and I have finally had to accept that with the permanent damage to the land that I have got to cut down the number of ponies here drastically. I have now got to feed them hay all the year round so the ponies are happily munching through my savings!
I am very anxious that the ponies that are sold will, when possible, go to homes where the females will have the chance some time in their life of breeding an odd foal and so help to preserve some of the old bloodlines they carry. I also have a yearling colt who I'd prefer to sell to someone who had the facilities to run him on as a possible stallion but if no one interested or he is not good enough he would be gelded.
There will be a completely new sales list in the next few days!
Competitions have been limited as not really had a schooled young pony to show this year and now I cannot run fast enough anymore most of the babies have stayed at home.
Summer qualified again for the London and SE Dressage to music championships and was placed in both her classes at the final. Sadly the competitions were marred by a very bad sound system so without exception everybody's music was distorted and hardly recognisable, so not many people went home happy.
I also did a few Walk Trot Dressage competitions on Herb Robert and despite being a bit shocked at some of the places I took him to he did consistently well and qualified for two local championships, but I abandoned taking him anymore as I have now only a horrid little Movano horsebox and whilst he travelled well he hated being left on his own in it and it was not worth the worry of having a problem if I was on my own, a real shame as he has super natural paces. As he is a special pony he has not been sold but is leant to a very competent person who lives close to me and who I can trust 100%.
This has been the first year I have had no foals although Rebecca has been living with Ronay, he needs a permanent wife for company, she lost it late last year, a fluke I knew as if she had been outside and it was tiny the foxes would have removed it pronto but she had it on one of the few times she was in a stable. No other mares had been covered. Rightly or wrongly Ronay had two wives this year so fingers crossed there will be babies in the late spring.
Here we have Fleetmead Herb Robert at a Christmas Show at a Riding School. Proving to be very relaxed and having a great time taking part in some of the classes with Lucy and her friends, I missed the fancy dress class with Lucy's little boy riding him dressed as an elf! They all had a great day with super support and Herb came home with two rosettes.


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Edna Mae Burnam () is one of the most respected names in piano pedagogy. She began her study of the instrument at age seven, with lessons from . Step By Step Piano Course – Book 1 sheet music – Piano/Keyboard sheet music by Edna-Mae Burnam: Willis Music. Shop the World's Largest Sheet Music. Burnam, Edna Mae Dozen A Day Mini Book. The Dozen a Day books are universally recognized as one of the most remarkable technique series on the market.
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Burnam Piano Method
Willis Softcover with CD Author: Example 2 – Jones: I do wish though that the books were sturdier. A Dozen a Day Book 1 Series: Read reviews that mention edna mae piano course step by step mae burnam year old use year playing the piano step by step piano learning to play playing the piano great way book was a great piano lessons course book series of books students learn student practice teacher.
Read our Privacy Policy. Vurnam it a good teaching tool?
Step by Step Piano Course – Book 1
I figured plano was just her age and everyone who plays told me they also hated practicing so I assumed it was that. She began her study of the instrument at age seven, with lessons from her mother, and went on to major in piano at the University of Washington and Chico State Teacher's College in Los Angeles.
I totally recommend this to burnaj learning to play the piano, all ages young and old. They were decent enough to get me started.
Set up a giveaway. When they complete this series they really know how to If you do not wish to be contacted, leave it blank. Make a wish list for gifts, suggest standard repertoire, let students know which books to buy, boast about pieces you've mastered: I'm delighted Edna Mae Burnam's books are still available for new generations of pianists.
Typically, orchestra scores have the tuba linked to euphonium, but it does happen where Trombone is the principal instead.
Amazon Music Stream millions of songs. It's a bit more advanced than say the Faber primer book, but not as complicated as the Faber accelerated beginner book. Starts vurnam the names of notes and music theory from the start. The numbers represent only distinct parts, not the number of copies of a part.
He is learning more than to just play a song!
Easily share your music lists with friends, students, and the world. Used to contact you regarding your review. Each simple lesson adds a new note to learn and practice with easy children's songs.
This is a great book for the beginner. I wanted this to be something special we would learn together, not happening. I first went through the online free piano nanny tutorials. This method teaches students the rudiments of music in a logical order, for gradual and steady progress.
Customers who bought this item also bought. As an art teacher, I know how important that is.
Burnam Piano Method
You consent to our cookies and privacy policy if you continue to use this site. AmazonGlobal Ship Orders Internationally. The students do not feel intimidated by piaho much information at once. They just had tons of songs that I couldn't play.
Pieces to Play – Book 2: Pages with related products.

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Travel Channel Pitch Lands "Best in Food" Feature for Blueprint Creative client
When we were secured as the Agency of Record and event producer for the third annual Miami Gardens Wine & Food Experienced presented by the City of Miami Gardens, we had three months to pull it off – produce and manage an immersive experience that usually requires at least six months of planning. In other words, that's three months to secure food and liquor participants, secure sponsorship, conceptualize and design the entire event, managing sound and production, secure our celebrity chefs Michelle Bernstein and Chef Roble, AND sell tickets to the experience.
Like we always do, Blueprint Creative made magic happen and successfully produced an event that sold more tickets over last year. We also put our PR magic to work to secure a full episode on the Travel Channel's "Best in Food" series for the Sweet Freak Dessert competition at the event. The episode aired nationally on April 25, 2018 and showcased the fierce 20min baking competition between our three contestants.
Just to put this in magnitude, the City of Miami Gardens is a brand new city relatively speaking only incorporated in 2003. So there wasn't much of a track record or name appeal that could merit the magnitude of a Travel Channel pitch, but the right PR team can overcome nearly any challenge to yield brand impact.
We thank the Travel Channel for finding this event to be worthy to share with the world. You can watch the full episode below.


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Latest Comments
"Hi kate, the link doesn't work, do you happen to know anywhere else I can get the step by step directions"
"I would love to be able to make this although since it is only available on Raverly I will NOT be able to download this. Once Raverly decided to put politics into their crocheting/Knitting pattern site, I will no longer give them the time of day. Looks like a wonderful pattern though."
"I can't get the Blue rose ripple pattern I need a new copy of it . I have lost my old one of this same pattern . I can't get this copy need help please"
Trio Blanket
We are adding the pattern to your Afghan Patterns.
This project has been added to your afghan patterns.
Click here to view your crochet patterns.
"Made with three Scheepjes Whirls, the yarn does all the work with this simple, repeating stitch pattern. All this colorplay and only six ends to weave! I provide lots of suggestions for color combos that might suit your style and space. This is the kind of pattern with its 2 row repeat that allows you to relax, binge Netflix, or tend to littles while you crochet something that will wow your friends. I hope you enjoy it!"
Crochet HookG/6 or 4 mm hook
Yarn Weight(2) Fine (23-26 stitches to 4 inches)
Finished Size• Sample A Blanket: 33" X 64" (84cm X 162cm) • Sample B Blanket: 38" X 50" (97cm X 128cm)
Materials List
- Scheepjes Whirl (3 cakes)
- G (4mm) hook
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Oct 27, 2018
This changing color effect can only be achieved by using this kind of yarn. It cannot be done using the ordinary worsted yarn in solid colors.
mulberrygalprinces s
Mar 04, 2018
What a pretty blanket. And the instructions are very well written and easy to follow. Now I have to just find the yarn and decide on a color. I hope it's available in my area. These can be put aside for Christmas and I will have some presents out of the way early.
Feb 28, 2018
The designer has made this in more than one color combination. I do not know which one I like the best. It can be really hard to make a decision when there are so many options. For a baby I guess I would go with the lighter version but you cannot go wrong with the darker color either. So many yarn colors so little time.
Delphine Bryant
Feb 28, 2018
I first thought that Scheepjes Whirl was a new crochet technique until I read the material list, lol. What a beauty. By using this type of yarn and knowing how to make a few basic crochet stitches this could be yours to gift or keep for yourself. It is almost one of those blankets that make itself. Thanks for the free pattern.
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Hi There! Is this Your First Time?
Did you know if you Register you have access to free search tools including the ability to save listings and property searches? Did you know that you can bypass the search altogether and have listings sent directly to your email address? Check out our how-to page for more info.
- Price$299,000
- Beds3
- Baths2
- SQ. Feet1,627
- Acres0.06
- Built1983
17019 Knots Landing, Addison
Stunning Remodel in Coveted Addison Place Neighborhood! This Immaculate Home Features White and Gray Quartzite Counters in the Kitchen, Metallic Epoxy Flooring, Designer Lighting, Custom Shaker Cabinets with Soft Close Doors and Drawers, White Farm Sink, Black Stainless Steel Samsung Appliances, Refrigerator to Stay! Rare Separate Utility Room For This Neighborhood With Custom Cabinetry! Luxury Vinyl Plank Flooring in Living and Dining! Beautiful Plantation Shutters Downstairs! Wood Look Tile in Guest Suite and Downstairs Bath! Refinished Baths With Custom Mirrors and Faucets! Professional Epoxy Floor in Garage! Zero Maintenance Back Yard with Aritficial Turf! HOA Maintains the Front! Move in Ready! Must See!
Essential Information
- Price$299,000
- Bedrooms3
- Bathrooms2.00
- Full Baths2
- Square Footage1,627
- Acres0.06
- Year Built1983
- TypeResidential
- Sub-TypeSingle Family
- StyleTraditional
- StatusActive Contingent
- UtilitiesCity Sewer, City Water, Concrete, Curbs, Individual Water Meter, Sidewalk, Underground Utilities
- FeaturesClub House, Comm Sprinkler System, Community Pool
- # of Garages2
- Garages2-Car Single Door, Attached, Covered, Garage, Garage Door Opener, Opener, Rear, Epoxy Flooring, Other Parking/Garage
- Exterior FeaturesCovered Porch(es), Gutters, Patio Covered, Sprinkler System
- Lot DescriptionInterior Lot, Landscaped, Subdivision, No Backyard Grass
- WindowsDouble Pane Windows
- RoofConcrete
- ConstructionBrick, Frame/Brick Trim, Siding, Stucco
- FoundationSlab
Listing Details
- Listing AgentLaura Teague
- Listing OfficeFirehouse Real Estate Services
Community Information
- Address17019 Knots Landing
- AreaADDISON/FAR NORTH DALLAS AREA (10)
- SubdivisionAddison Place Rev
- CityAddison
- CountyDallas
- StateTX
- Zip Code75001-5033
- Interior FeaturesCable TV Available, Decorative Lighting, High Speed Internet Available, Plantation Shutters, Wet Bar, Window Coverings
- AppliancesBuilt-in Microwave, Convection Oven, Dishwasher, Disposal, Oven - Electric, Drop-In Range/Oven-Elec, Refrigerator, Water Line to Refrigerator
- HeatingCentral Air-Elec, Central Heat-Elec
- # of Stories2
- Stories2
School Information
- DistrictDallas ISD
- ElementaryJerry Junkins
- MiddleWalker
- HighWhite
Users may not reproduce or redistribute the data found on this site. The data is for viewing purposes only. Data is deemed reliable, but is not guaranteed accurate by the MLS or NTREIS.
Listing information last updated on March 29th, 2020 at 4:00pm CDT.


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Event Information
Date and Time
About this Event
Join us on the third Sunday of the month at 11 am for services led by our Minister Reverend Carla Maurer. Services are in the Reformed tradition of the the Swiss Protestant Church, with an ecumenical outlook.
The sermon is in English.
Hymns are are in German, French and English, accompanied on our wonderful Swiss Späth organ, played by our Director of Music, Peter Yardley-Jones
You are very welcome to stay after the Service for light refreshments or a light meal and to join in conversation.
The Church building was constructed in 1855 and renovated in 2009 by award winning Swiss achitects Christ and Gantenbein.
The Swiss Church in London is rooted in the Reformed tradition but people from all denominations, faith groups or none, are welcome.


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Hair Care Shampoo
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Mix a small amount in the hands with water to create lather. Massage into the scalp and rinse thoroughly. Follow with Moisture Conditioner.
1. Vitamine E enhanced A natural hair product
2. Coconut Oil - is known for easy absorption to heal, protect and beautify your skin
3. Vitamin complex A, C and E - to help retain moisture and protect against dryness
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8. Silicon Oil - makes hair shiny and soft
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1. aloe 2. gardenia 3. coconut 4. sweet almod 5. olive 6. jasmine
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17. watermelon 18. tea tree 19. lemon 20. vanilla 21. chamomile 22. blackpeper 23. kiwi fruits 24. white citrus 25. strawberry
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Hair Care Shampoo Images


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Go Create! offers children from 0-12 years old the opportunity to get creative at our purpose built studio. Whether it's painting, drawing, colouring, making something using the vast choice of materials we stock. Using clay or paper mache.
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if you cut and paste the Latex output into your own documents, or if you don't. The error message indicates that your TeXLive installation is corrupted or incomplete. It shows that the programs latex and dvips were indeed. JaxoDraw is a Feynman graph plotting tool written in Java. of JaxoDraw's main features is the possibility to create LATEX files which make.
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On Unix like systems, make sure that you have write permission to the directory where JaxoDraw creates temporary files usually the JaxoDraw home directory. This is dvips k 5.
This is a workaround that we used ourselves when working with axodraw. What should I do? We use maven to build our web site. Under Windows, you have to do basically the same as under Linux. If you are not sure, you should post a question to the JaxoDraw discussion mailing list. The number of undo steps can be configured jaxodrwa the Preferences. It is not necessary to install axodraw4j in order to run JaxoDraw. iaxodraw
RPM resource jaxodraw-latex
Older versions were written and maintained with Java version 1. General What is JaxoDraw? Refer to the appendix of the User Guide for more information. The documentation for axodraw4j. Post as a guest Name.
I am using "jaxodraw But I don't know what are the paths. I have a question that is not addressed here. Please see the Prerequisites document. On which platform does it run? They should have been created by a standard install of TeXLive in the following locations: Does it run on Mac OS X? How do I do this and that with JaxoDraw? For Java 5 there are a few minor points to notice, see this news entry. This is described in the Instructions section of the source download document. How can I run JaxoDraw from any location I like?
We shall only outline here how you make axodraw available on your system and how you use it with the LaTeX output from JaxoDraw. After that latex and dvips should work.
JaxoDraw was initially meant to be a graphical user interface for J. You have to install axodraw4j. Linux instructions For installation, you have two options: Vermaseren's axodraw LaTeX package. This package is derived from J. I'd recommend you to make this a full installation, and take the default options.
I have no idea what is the exact path for them! Sign up using Facebook. I ran the generated latex code using jazodraw "texmaker". How is the JaxoDraw web site built? I have installed Texlive Vanilla following the instructions given here: Thanks a lot, it did work after installing the new version and up[stream of the texlive, although there seems to be another problem not related to jaxodraw.
Home User Guide Plugins Sitemap.
Or try to jaxodra your feature yourself and send us some patches. If these resources don't help you with your problem, or if you think that you found a bug that is not yet documented, you should contact us. You can also try to pay us. Post Your Answer Discard By clicking "Post Your Answer", you acknowledge that you have read our updated terms of service jzxodraw, privacy policy and cookie policyand that your continued use of the website is subject to these policies.
Installing axodraw4j system wide is very easy.
For other features, please check the Overview document. First put your axodraw4j. The Reference section and the user guide contain some detailed and comprehensive documentation about JaxoDraw.


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Maybe it is because we have a lot of people moving into our area from out of state, or people just don't pay attention.ut I have noticed the following: Four out of every 10 cars do not turn on their headlights during rain and fog. It's the law - not their parking, fog or running lights. Six out of 10 do not give turn signals, and most of those who do, do not give them as required, 200 feet before turning.
Last Saturday I witnessed a sheriff's deputy - I will not cite the car number due to fear of retaliation - make two turns with no signal, and on Tuesday morning the same car was driving on Lewiston Road in Columbia County, in the rain and fog, with no lights on.
Send a letter to the editor
It will not cease until these people start getting tickets. Nobody is perfect, and that of course includes me, but I try to follow the law as best as I can.
I hope Columbia County Sheriff Clay Whittle tries to make sure I do not receive retaliation for this note. I'm only trying to make people aware.
Don Turner


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TagHair Fair 2014
Turning of the Rose
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I swung by KOT Stables to see if my centaur avatar had an update and decided it was the perfectContinue Reading
Darcy CogsWorth
Steamy heaven abounds! Remarkable Oblivion released these steam emitting highly detailed and ornate horns at The Secret Affair. The hornsContinue Reading
"We are not always what we seem, and hardly ever what we dream." ― Peter S. Beagle, The Last UnicornContinue Reading


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Professional Development Meetings
Title: An Introduction to FHWA's Quadrant Roadway Intersection Informational Guide
Date and Time: Thursday, April 9, 2020; 2:00 – 4:00 PM ET
Description: Alternative intersections and interchanges offer the potential to improve safety and reduce delay at a lower cost and with fewer impacts than traditional solutions. In 2014, the Federal Highway Administration published informational guides for four innovative designs: the Median U-Turn (MUT), Displaced Left Turn (DLT), Restricted Crossing U-Turn (RCUT), and Diverging Diamond Interchange (DDI). Recently, a fifth guide has been developed to provide information on the Quadrant Roadway Intersection (QRI).
The QRI concept uses a roadway in one intersection quadrant and three coordinated, signalized intersections to eliminate direct left turns at the main juncture. This allows a reduction in signal phases to improve intersection safety, capacity, and efficiencies. In addition to vehicular operational and safety improvements, the QRI has many multimodal benefits, including shorter and safer crossings for pedestrians and bicycles.
FHWA is pleased to offer this webinar to all Federal, State, Municipal, and Consultant transportation practitioners responsible for or interested in providing innovative solutions at intersections in need of operational, safety, and/or multimodal improvements. The webinar presentation will introduce the QRI Guide and review the information presented in the guide, focusing on intersection operations, safety, various geometric forms, and planning and design criteria to consider when evaluating the QRI as a potential intersection improvement alternative. The presentation will also include information provided from several DOTs that have constructed a QRI in recent years. Certificates of completion for professional development hours (PDHs) will be provided upon request.
Presenters: Jeff Shaw, FWHA Office of Safety Technologies, Guide Technical Manager; Jonathan Reid, Arcadis, Lead Author; Joseph E. Hummer, NCDOT State Traffic Management Engineer; and representatives from State DOTs having implemented the QRI.
Registration: Registration is free and open to everyone. Please forward this invitation to others who might be interested. Space is limited so please register as soon as possible. Once you register you will receive an email with login instructions. To register:
- Visit https://collaboration.fhwa.dot.gov/dot/fhwa/WC/Lists/Seminars/DispForm.aspx?ID=2310 and choose the "Register Yourself for Seminar" button.
- Log in with your Webconferencing system name and password. If you don't already have an account or you have forgotten your password, please click on the appropriate links to create an account or reset your password. To set up a new account, please visit https://collaboration.fhwa.dot.gov/FBA/MembershipRequest.aspx to request one.
- Once logged in, complete the registration process.
The Professional Development Committee is seeking input on training topics to be offered by NCITE. If you have any suggestions, please contact the Professional Development Committee.
If you are aware of an upcoming transportation-related professional development opportunity, please contact the Professional Development Committee to have it added to this list.


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Astronomers have spotted a 40 billion solar mass black hole in the Abell 85 cluster of galaxies. They found the behemoth using spectral observations with the Very Large Telescope (VLT.) There are only a few direct mass measurements for black holes, and at about 700 million light years from Earth, this is the most distant one.Continue reading "There's a New Record for the Most Massive Black Hole Ever Seen: 40 Billion Solar Masses"
Some Quasars Shine With the Light of Over a Trillion Stars
Quasars are some of the brightest objects in the Universe. The brightest ones are so luminous they outshine a trillion stars. But why? And what does their brightness tell us about the galaxies that host them?
To try to answer that question, a group of astronomers took another look at 28 of the brightest and nearest quasars. But to understand their work, we have to back track a little, starting with supermassive black holes.Continue reading "Some Quasars Shine With the Light of Over a Trillion Stars"
Astronomers Find a Supermassive Black Hole That's Feasting on a Regular Schedule, Every 9 Hours
Astronomers have found a supermassive black hole (SMBH) with an unusually regular feeding schedule. The behemoth is an active galactic nucleus (AGN) at the heart of the Seyfert 2 galaxy GSN 069. The AGN is about 250 million light years from Earth, and contains about 400,000 times the mass of the Sun.Continue reading "Astronomers Find a Supermassive Black Hole That's Feasting on a Regular Schedule, Every 9 Hours"
A Monster Black Hole has been Found with 40 Billion Times the Mass of the Sun
If contemplating the vast size of astronomical objects makes you feel rather puny and insignificant, then this new discovery will make you feel positively infinitesimal.
It's almost impossible to imagine an object this large: a super massive black hole that's 40 billion times more massive than our Sun. But there it is, sitting in the center of a super-giant elliptical galaxy called Holmberg 15A. Holmberg 15A is about 700 million light years away, in the center of the Abell 85 galaxy cluster.Continue reading "A Monster Black Hole has been Found with 40 Billion Times the Mass of the Sun"
Astronomers See Evidence of Supermassive Black Holes Forming Directly in the Early Universe
Super-Massive Black Holes (SMBH) are hard to explain. These gargantuan singularities are thought to be at the center of every large galaxy (our Milky Way has one) but their presence there sometimes defies easy explanation. As far as we know, black holes form when giant stars collapse. But that explanation doesn't fit all the evidence.Continue reading "Astronomers See Evidence of Supermassive Black Holes Forming Directly in the Early Universe"
This Star has been Kicked Out of the Milky Way. It Knows What It Did.
Every once in a while, the Milky Way ejects a star. The evicted star is typically ejected from the chaotic area at the center of the galaxy, where our Super Massive Black Hole (SMBH) lives. But at least one of them was ejected from the comparatively calm galactic disk, a discovery that has astronomers rethinking this whole star ejection phenomenon.Continue reading "This Star has been Kicked Out of the Milky Way. It Knows What It Did."
Here's What the First Images from the Event Horizon Might Look Like
The largest object in our night sky—by far!—is invisible to us. The object is the Super-Massive Black Hole (SMBH) at the center of our Milky Way galaxy, called Sagittarius A. But soon we may have an image of Sagittarius A's event horizon. And that image may pose a challenge to Einstein's Theory of General Relativity.
Continue reading "Here's What the First Images from the Event Horizon Might Look Like"
Evidence for Thousands of Black Holes Buzzing Around the Center of the Milky Way
Since the 1970s, astronomers have understood that a Supermassive Black Hole (SMBH) resides at the center of the Milky Way Galaxy. Located about 26,000 light-years from Earth between the Sagittarius and Scorpius constellations, this black hole has come to be known as Sagittarius A* (Sgr A*). Measuring 44 million km across, this object is roughly 4 million times as massive as our Sun and exerts a tremendous gravitational pull.
Since that time, astronomers have discovered that most massive galaxies have SMBHs at their core, which is what separates those that have an Active Galactic Nuclei (AGN) from those that don't. But thanks to a recent survey conducted using NASA's Chandra X-ray Observatory, astronomers have discovered evidence for hundreds or even thousands of black holes located near the center of the Milky Way Galaxy.
The study which described their findings was recently published in the journal Nature under the title "A density cusp of quiescent X-ray binaries in the central parsec of the Galaxy". The study was led by Chuck Hailey, the Pupin Professor of Physics and the Co-Director of the Columbia Astrophysics Laboratory (CAL) at Columbia University, and including members from the Instituto de Astrofísica at the Pontificia Universidad Católica de Chile and the Harvard-Smithsonian Center for Astrophysics.
Using Chandra data, the team searched for X-ray binaries containing black holes that were in the vicinity of Sgr A*. To recap, black holes are not detectable in visible light. However, black holes (or neutron stars) that are locked in close orbits with a star will pull material from their companions, which will then be accreted onto the black holes' disks and heated up to millions of degrees.
This will result in the release of X-rays which can then be detected, hence why these systems are called "X-ray binaries". Using Chandra data, the team sought out X-ray of sources that were located within roughly 12 light years of Sgr A*. They then selected sources with X-ray spectra similar to those of known X-ray binaries, which emit relatively large amounts of low-energy X-rays.
Using this method, they detected fourteen X-ray binaries within about three light years of Sgr A*, all of which contained stellar-mass black holes (between 5 and 30 times the mass of our Sun). Two of these sources had been identified by previous studies and were eliminated from the analysis, while the remaining twelve (circled in red in the image above) were newly-discovered.
Other sources which relatively large amounts of high energy X-rays (labeled in yellow) were believed to be binaries containing white dwarfs. Hailey and his colleagues concluded that the majority of the dozen X-ray binaries were likely to contain black holes, based on their variability and the fact that their X-ray emissions over the course of several years was different from what is expected from binaries containing neutron stars.
Given that only the brightest X-ray binaries containing black holes are likely to be detectable around Sgr A* (given its distance from Earth), Hailey and his colleagues concluded that this detection implies the existence of a much larger population. By their estimates, there could be at least 300 and as many as one thousand stellar-mass black holes present around Sgr A*.
These findings confirmed what theoretical studies on the dynamics of stars in galaxies have indicated in the past. According to these studies, a large population of stellar mass black holes (as many as 20,000) could drift inward over the course of millions of years and collect around an SMBH. However, the recent analysis conducted by Hailey and his colleagues was the first observational evidence of black holes congregating near Sgr A*.
Naturally, the authors acknowledge that there are other explanations for the X-ray emissions they detected. This includes the possibility that half of the dozen sources they observed are millisecond pulsars – very rapidly rotating neutron stars with strong magnetic fields. However, based on their observations, Hailey and his team strongly favor the black hole explanation.
In addition, a follow-up study conducted by Aleksey Generozov (et al.) of Columbia University – titled "An Overabundance of Black Hole X-Ray Binaries in the Galactic Center from Tidal Captures" – indicated that there could be as many as 10,000 to 40,000 black holes binaries at the center of our galaxy. According to this study, these binaries would be the result of companions being captured by black holes.
In addition to revealing much about the dynamics of stars in our galaxy, this study has implications for the emerging field of gravitational wave (GW) research. Essentially, by knowing how many black holes reside at the center of galaxies (which will periodically merge with one another), astronomers will be able to better predict how many gravitational wave events are associated with them.
From this, astronomers could create predictive models about when and how GW events are likely to happen, and well as discerning what role they may play in galactic evolution. And with next-generation instruments – like the James Webb Space Telescope (JWST) and the ESA's Advanced Telescope for High Energy Astrophysics (ATHENA) – astronomers will be able to determine exactly how many black holes reside near the center of our galaxy.
Further Reading: NASA
The Gaia Mission Could Moonlight as a Gravitational Wave Detector
In February of 2016, scientists working for the Laser Interferometer Gravitational-Wave Observatory (LIGO) made the first-ever detection of gravitational waves. Since that time, multiple detections have taken place, thanks in large to part to improvements in instruments and greater levels of collaboration between observatories. Looking ahead, its possible that missions not designed for this purpose could also "moonlight" as gravitational wave detectors.
For example, the Gaia spacecraft – which is busy creating the most detailed 3D map of the Milky Way – could also be instrumental when it comes to gravitational wave research. That's what a team of astronomers from the University of Cambridge recently claimed. According to their study, the Gaia satellite has the necessary sensitivity to study ultra-low frequency gravitational waves that are produced by supermassive black hole mergers.
The study, titled "Astrometric Search Method for Individually Resolvable Gravitational Wave Sources with Gaia", recently appeared in the Physical Review Letters. Led by Christopher J. Moore, a theoretical physicist from the Center for Mathematical Sciences at the University of Cambridge, the team included members from Cambridge's Institute of Astronomy, Cavendish Laboratory, and Kavli Institute for Cosmology.
To recap, gravitational waves (GWs) are ripples in space-time that are created by violent events, such as black hole mergers, collisions between neutron stars, and even the Big Bang. Originally predicted by Einstein's Theory of General Relativity, observatories like LIGO and Advanced Virgo detect these waves by measuring the way space-time flexes and squeezes in response to GWs passing through Earth.
However, passing GWs would also cause the Earth to oscillate in its location with respect to the stars. As a result, an orbiting space telescope (such as Gaia), would be able to pick up on this by noting a temporary shift in the position of distant stars. Launched in 2013, the Gaia observatory has spent the past few years conducting high-precision observations of the positions of stars in our Galaxy (aka. astrometry).
In this respect, Gaia would look for small displacements in the massive field of stars it is monitoring to determine if gravitational waves have passed through the Earth's neighborhood. To investigate whether or not Gaia was up to the task, Moore and his colleagues performed calculations to determine if the Gaia space telescope had the necessary sensitivity to detect ultra-low frequency GWs.
To this end, Moore and his colleagues simulated gravitational waves produced by a binary supermassive black hole – i.e. two SMBHs orbiting one another. What they found was that by compressing the data sets by a factor of more than 106 (measuring 100,000 stars instead of a billion at a time), GWs could be recovered from Gaia data with an only 1% loss of sensitivity.
This method would be similar to that used in Pulsar Timing Arrays, where a set of millisecond pulsars are examined to determine if gravitational waves modify the frequency of their pulses. However, in this case, stars are being monitored to see if they are oscillating with a characteristic pattern, rather than pulsing. By looking at a field of 100,000 stars at a time, researchers would be able to detect induced apparent motions (see figure above).
Because of this, the full release of Gaia data (scheduled for the early 2020s) is likely to be a major opportunity for those hunting for GW signals. As Moore explained in a APS Physics press release:
"Gaia will make measuring this effect a realistic prospect for the first time. Many factors contribute to the feasibility of the approach, including the precision and long duration of the astrometric measurements. Gaia will observe about a billion stars over 5–10 years, locating each one of them at least 80 times during that period. Observing so many stars is the major advance provided by Gaia."
It is also interesting to note that the potential for GW detection was something that researchers recognized when Gaia was still being designed. One such individual was Sergei A. Klioner, a researcher from the Lorhrmann Observatory and the leader of the Gaia group at TU Dresden. As he indicated in his 2017 study, "Gaia-like astrometry and gravitational waves", Gaia could detect GWs caused by merging SMBHs years after the event:
"It is clear that the most promising sources of gravitational waves for astrometric detection are supermassive binary black holes in the centers of galaxies… It is believed that binary supermassive black holes are a relatively common product of interaction and merging of galaxies in the typical course of their evolution. This sort of objects can give gravitational waves with both frequencies and amplitudes potentially within the reach of space astrometry. Moreover, the gravitational waves from those objects can often be considered to have virtually constant frequency and amplitude during the whole period of observations of several years."
But of course, there's no guarantees that sifting through the Gaia data will reveal additional GW signals. For one thing, Moore and his colleagues acknowledge that waves at these ultra-low frequencies could be too weak for even Gaia to detect. In addition, researchers will have to be able to distinguish between GWs and conflicting signals that result from changes in the spacecraft's orientation – which is no easy challenge!
Still, there is hope that missions like Gaia will be able to reveal GWs that are not easily visible to ground-based interferometric detectors like LIGO and Advanced Virgo. Such detectors are subject to atmospheric effects (like refraction) which prevent them from seeing extremely low frequency waves – for instance, the primordial waves produced during the inflationary epoch of the Big Bang.
In this sense, gravitational wave research is not unlike exoplanet research and many other branches of astronomy. In order to find the hidden gems, observatories may need to take to space to eliminate atmospheric interference and increase their sensitivity. It is possible then that other space telescopes will be retooled for GW research, and that next-generation GW detectors will be mounted aboard spacecraft.
In the past few years, scientists have gone from making the first detection of gravitational waves to developing new and better ways to detecting them. At this rate, it won't be long before astronomers and cosmologists are able to include gravitational waves into our cosmological models. In other words, they will be able to show what influence these waves played in the history and evolution of the Universe.
Further Reading: Kavli Institute for Cosmology, APS Physics, Physical Review Letters
Supermassive Black Holes can Turn Star Formation On and Off in a Large Galaxy
In the 1970s, astronomers discovered that a particularly large black hole (Sagittarius A*) existed at the center of our galaxy. In time, they came to understand that similar Supermassive Black Holes (SMBHs) existed in the center of most massive galaxies. The presence of these black holes was also what differentiated galaxies that had particularly luminous cores – aka. Active Galactic Nuclei (AGN) – from those that didn't.
Since that time, astronomers and cosmologists have pondered what role SMBHs have on galactic evolution, with some venturing that they have a profound impact on star formation. And thanks to a recent study by an international team of astronomers, there is now direct evidence for a correlation between and SMBH and a galaxy's star formation. In fact, the team demonstrated that a black hole's mass could determine when star formation in a galaxy will end.
The study, titled "Black-Hole-Regulated Star Formation in Massive Galaxies", recently appeared in the scientific journal Nature. Led by Ignacio Martín-Navarro, a Marie Curie Fellow at the University of California Observatories, the study team also consisted of members from the Max-Planck Institute for Astronomy and the Instituto de Astrofísica de Canarias.
For the sake of their study, the team relied on data gathered the Hobby-Eberle Telescope Massive Galaxy Survey in 2015. This systematic survey used the 10m Hobby-Eberly Telescope (HET) at the McDonald Observatory to conduct an optical long-slit spectroscopic survey of over 1000 galaxies. This survey not only provided spectra for these galaxies, but also produced direct mass measurements of the central black holes for 74 of these galaxies.
Using this data, Martín-Navarro and his colleagues found the first observational evidence for a direct correlation between the mass of a galaxy's central black hole and its history of star formation. While astrophysicists have been operating under this assumption for decades, the proof was missing until now. As Jean Brodie, professor of astronomy and astrophysics at UC Santa Cruz and a coauthor of the paper, said in a UCSC press release:
"We've been dialing in the feedback to make the simulations work out, without really knowing how it happens. This is the first direct observational evidence where we can see the effect of the black hole on the star formation history of the galaxy."
Roughly 15 years ago, the correlation between a SMBHs mass and the total mass of a galaxy's stars was discovered, which led to a major unresolved question in astrophysical circles. While this correlation appeared to be a central feature of galaxies, it was unclear as to what could have caused it. How could the mass of a comparatively small and central black hole be related to the mass of billions of stars distributed throughout a galaxy?
One possible explanation was that more massive galaxies collected larger amounts of gas, thus resulting in more stars and a more massive central black hole. However, astrophysicists also believed their was a feedback mechanism at work, where growing black holes inhibited the formation of stars in their vicinity. In short, when matter accretes on a central black hole, it sends out a tremendous amount of energy in the form of radiation and particle jets.
If this energy is transferred to gas and dust surrounding the core of the galaxy, stars will be less likely to form in this region since gas and dust need to be cold in order to undergo areas of collapse. For years, feedback of this kind has been included in cosmological simulations to explain the observed star-formation rates in galaxies. According to these same simulations, minus this mechanism, galaxies would form far more stars than have been observed.
However, no direct evidence of this phenomena had previously been available. The first step to obtaining some was to reproduce the stellar formation histories of the 74 target galaxies used for the study. Martín-Navarro and his colleagues did this by subjecting spectra obtained from each of these galaxies to computational techniques that looked for the best combination of stellar populations to fit the data.
In so doing, the team was able to reconstruct the history of star formation within the target galaxies for the past 12.5 billion years. After examining these histories, they noticed some predictable results, but also some rather significant differences. For starters, as predicted, the regions of around the galaxies' central black holes demonstrated a clear dampening influence on the rate of star formation.
As predicted, there was also a clear correlation between the mass of the central black holes and stellar mass in these galaxies. However, the team also noted that in cases where stellar mass was slightly smaller than expected (relative to the mass of their central black holes), star formation rates were lower. In some other cases, galaxies had larger-than-expected stellar masses (again, relative to their black holes) and their star formation rates were higher.
This correlation was not only more consistent than that observed between black hole mass and stellar mass, it occurred independently of other factors (such as shape or density). As Martín-Navaro explained:
"For galaxies with the same mass of stars but different black hole mass in the center, those galaxies with bigger black holes were quenched earlier and faster than those with smaller black holes. So star formation lasted longer in those galaxies with smaller central black holes."
They also noted that this correlation extends into the deep past, where the galaxies with supermassive central black holes have been consistently producing a comparatively low rate of stars for the past 12.5 billion years. This constitutes the first strong evidence for a direct, long-term connection between star formation and the existence of a central black hole in a galaxy.
Another interesting takeaway from the study was the way it addressed possible correlations between AGN luminosity and star formation. In the past, other researchers have sought to find evidence of a link between the two, but without success. According to Martín-Navarro and his team, this may be because the time scales are incredibly different. Whereas star formation occurs over the course of eons, outbursts from AGNs occur over shorter intervals.
What's more, AGNs are highly variable and their properties are dependent on a number of factors relating to their black holes – i.e. size, mass, rate of accretion, etc. "We used black hole mass as a proxy for the energy put into the galaxy by the AGN, because accretion onto more massive black holes leads to more energetic feedback from active galactic nuclei, which would quench star formation faster," said Martin-Navarro.
Looking ahead, the team hopes to conduct further research and determine exactly how central black holes arrest star formation. At present, the possibility that it could be due to radiation or jets of gas heating up surrounding matter are not definitive. As Aaron Romanowsky, an astronomer at San Jose State University and UC Observatories, indicated:
"There are different ways a black hole can put energy out into the galaxy, and theorists have all kinds of ideas about how quenching happens, but there's more work to be done to fit these new observations into the models."
Part of determining how the Universe came to be is knowing what mechanisms were at play and the extent of their roles. With this latest study, astrophysicists and cosmologists can take comfort in the knowledge that they've been getting it right – at least in this case!


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The Genesis of Norms in Globalization
Prof. Dr. M. Mercè Darnaculleta i Gardella
Ph.D. Candidates
Lara Elena Knop
Thesis "Key concepts in interdisciplinary research contexts"
Jan Obracaj
Thesis "Kontingenzbewusstsein, Zivilgesellschaft und die Verteidigung der Demokratie – Philosophische Debatten zur politischen Legitimation"
Peter Scheiffele
Thesis "Haiti in der Weltordnung. Organisationaler Imperialismus und Autonomie"
Since the emergence of modernity, both the traditional forms of normative production and the classical regulative procedures and structures have been derived from one particular concept of state: a concept assuming the state's sovereignty over society. But in a time of globalization, new forms of normative genesis have emerged alongside their older counterparts; within them, the principle of sovereignty has been replaced by a principle of cooperation. A key question that here emerges is whether this development implies the state's withdrawal from the process of establishing norms.
In any event, at present we can observe the development of new normative systems running parallel to the state's generation of legal norms; these new systems are characterized by their societal—hence exclusively private or pseudo-state—origins, and by their global extension. In other words, the primacy of state regulation is being placed in question through new formulas for societal self-regulation with a global reach. Alongside the conditions of rule organized by the state, new hierarchies are surfacing that cross over political and cultural borders.


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Main content
Deprecated arithmetic
Current time:0:00Total duration:6:38
Thinking more about negative exponents
Video transcript
In the last video, we gave an argument for why 3 to the negative 2 power should be equivalent to 1 over 3 to the positive 2 power. I now want to do a very similar argument, but I want to do it for general bases and general exponents. So in particular, I want to think about what a to the b power, or in particular, what a to the negative b power should be equal to. So we know that we want to uphold the property that, if we have the base raised to an exponent and then that's being multiplied by that same base raised to another exponent, that we would just add the two exponents. So just to be clear, we want to maintain this property, that a to the b power times a to the negative b power should be equal to a to the b plus negative b power, which of course is going to be equal to a to the 0-th power. And as long as a does not equal to 0, this should be equal to 1. Let me write that-- for a does not equal 0. So in general-- actually I'll just copy and paste this-- a to the b times a to the negative b-- copy and paste-- should be equal to 1. So this right over here needs to be equal to 1. And so if we want think about, what does a to the negative b equal? We just divide both sides by a to the b. And we would get a to the negative b. I've kept the colors consistent this long. Gotta keep going. a to the negative b is equal to 1 over a to the b. And so I just want to review this. And it's really important to keep in mind because when you see something as a base to a negative exponent, there's a temptation to somehow introduce a negative number. But a negative exponent is really about taking the reciprocal. So you're taking the reciprocal of this number raised to the positive base. And we've just shown the argument that if we want this property be true-- and a lot of the properties of exponents are all about just keeping consistency, keeping the old properties continuing to be true as we introduce new definitions and new properties-- and we see that if we want this to be true, then a to the negative b should be 1 over a to the b. And in other videos we'll show other motivations for why a negative exponent is essentially defined this way. But now that we've seen this is true, for any non-zero a and any b, let's actually do some examples. And actually, let's think about the size of these numbers. So for example-- and let me introduce new colors right over here. I said I would introduce new colors, and I didn't-- if I were to take 5 to the third power, we know that's 5 times 5 times 5. That is equal to 125. It's a reasonably large number. Now what should 5 to the negative 3 power be? And I encourage you to pause this video and think about this before I tell you. Use what I just told you. What should 5 to the negative 3 power be? Well, I assume you've paused the video. So this is going to be equal to 1 over 5 to the positive 3 power, which is equal to 1/125. So this is really interesting. 5 to the third was a reasonably large number. While 5 to the negative 3, it wasn't a negative number. It's still a positive number, but it's a very small number. It's 1/125. Let's do two more examples. Let's say I were to take negative 1/2, and I were to raise this to the third power. What is that going to be? Well, it's negative 1/2 times negative 1/2 times negative 1/2, which is, of course, going to be equal to negative 1/8. Now what should negative 1/2 to the negative 3 power be, based on everything that we just talked about? And once again, I encourage you to pause this video and think about it. Well it should be equal to 1 over negative 1/2 to the positive 3 power. Well, we just figured out what that is. Negative 1/2 to the positive 3 power is negative 1/8. This thing right over here should be equal to negative 1/8. So it's going to be equal to 1 over negative 1/8. And what's that equal to? Well that's equal to 1 times the reciprocal of this denominator over here. So it's 1 times negative 8/1, which is going to be equal to negative 8. So this is interesting. Normally when you take a number whose absolute value is less than 1 and you take it to larger and larger exponents, it gets smaller and smaller and smaller. When you multiply either a positive or negative 1/2 times 1/2 times 1/2, its magnitude, its absolute value, is normally going to get smaller and smaller and smaller. But now, when you raise it to a negative exponent, it's absolute value is getting larger and larger and larger. And that's because, once again, you are taking the reciprocal. The important thing I want to emphasize here is that you shouldn't view this negative as when you think about negative multiplication. Notice, this negative did not change the sign of what the eventual value is. You've got negative 1/8. You got negative 8. What it did is, it changed the magnitude. So this is negative 1/8. When you took to the negative third power, you took the reciprocal of that, which is negative 8.


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HU's Stoffel earns NAIA women's XC scholar-athlete of year accolade
Thursday, February 6, 2020 8:25 AM
Huntington University junior Hannah Stoffel was named scholar athlete of the year for NAIA women's cross country by the United States track & field Cross Country Coaches Association.
Stoffel, the 2019 NAIA women's cross country champion, carries a 3.948 grade point average.
Stoffel and her teammates who competed at nationals were also tabbed an all-academic team by having a cumulative GPA of 3.75. That was the fourth-highest GPA of the 52 teams to receive the honor.
Individually, all seven of the HU harriers earned all-academic badges as well. Te be selected for this distinction, student athletes must carry a cumulative GPA of 3.25 on a 4.0 scale and qualify for the national championship meet.
HU athletes in addition to Stoffel receiving the honor included Isabel Hunter, Erin Manchess, Mara McFarland, Molly Mitchell, Saige Norris and Olivia Von Gunten.
On the men's side, the Foresters were among 44 teams deemed to be an all-academic team. The seven runners collectively claimed a team GPA of 3.31, well above the minimum 3.0 standard need for the honor.
Four individuals on Coach Nick Johnson's crew also received all-academic honors. They were Nick Childs, Aaron Hendryx, Mathew Hyter and Kent Yoder.


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The Kee football team brought its season to a close Friday, October 25 at Midland, but not before giving that host Eagle team fighting for extension of its own season a strong challenge that eventually waned away in the final frame to a 36-18 Hawk defeat. The Kee gridders answered Midland nearly blow-for-blow to just a 20-18 deficit through three full frames but had that pace derailed in the fourth quarter to result in a final 16-0 Eagle outburst that provided a majority of the game's final doubled-up margin.
The loss ends Kee's football season at a 2-7 overall record that included a mark of 2-5 that placed the Hawks sixth in the final eight-team standings of Eight-Man District 3. The Midland victory allowed the Eagles to improve to 7-2 overall and a third-place record of 5-2 in District 3 play that all proved to be good enough to land them one of the final State Play-Off seeds and a first-round date at HLV-Victor this Friday, November 1.
Third straight State Meet qualification ... The Waukon girls cross country team displays the banners signifying the team's qualification for the Class 2A State Meet after the Lady Indians ran to a second-place team finish at their State Qualifying Meet hosted by North Fayette Valley in West Union Thursday, October 24. Pictured above are: Left to right - Front row: Freshman Paige Hansmeier, sophomore Madelyn Helgerson and junior Annika Headington; Back row: Junior Skylar Garrett, seniors Ellec Armstead and Katelyn Benzing, and juniors Bailey Shafer, Regan Griffith and Maddy Waters. View and find out how to purchase this photo and many more by clicking on the Photo Galleries link on this website.
Waukon girls cross country team earns third consecutive qualification for Class 2A State Meet with runner-up finish at State Qualifier
For the third consecutive season the Waukon girls cross country team has proven itself among the Class 2A elite, running to its third straight State Meet qualification Thursday, October 24 at the Class 2A State Qualifying Meet hosted by North Fayette Valley High School in West Union. In an 11-team field where they were one of three ranked teams vying for a top-three finish to earn State Meet qualification, the 13th-rated Indians benefited from having all five of their scored runners finish within the top 23 individuals overall, and within the top 20 scored runners, to score 60 team points and firmly secure a runner-up team result and advancement to this year's season grand finale once again.
Despite the Waukon football team's Friday, October 25 final game of the regular season at North Fayette Valley featuring the already State Play-Off clinched Indians taking on a transitioning TigerHawk team bringing its season to a close, there was still plenty to play for besides the natural rivalry that seems to have developed between the two squads over the last several seasons. The Indians had a chance to gain further play-off advantage with a pending top billing in the final Class 2A State Play-Off seeding process resulting in hosting their first two postseason games and an even more historical motivation of being the first Indian grid squad in the Iowa high school football play-off era to complete an undefeated regular season and the first such season since the grid Tribe played to unblemished marks under Coach Walter "Red" Rixen in both 1953 and 1957.
Returning to State Meet with third consecutive qualification ... Members of the Kee girls cross country team display one of the banners they received signifying the team's qualification for the Class 1A State Meet after they ran to the team championship at their State Qualifying Meet hosted at Cedar Falls Thursday, October 24. Pictured above, left to right, are freshman Jaylyn Walleser, seniors Rachel Walleser and Makayla Peters, freshman Alison Wagner, sophomores Reagan Mudderman and Haley Meyer, and freshman Alaina Bakewell. Photo courtesy of the Kee High School Yearbook. View and find out how to purchase this photo and many more by clicking on the Photo Galleries link on this website.
Kee cross country girls run to third consecutive State Meet qualification in championship fashion; Junior Chris Wagner becomes first Kee boys State qualifier since 1994 season
A trip to the season grand finale was on the line at the Class 1A State Qualifying Cross Country Meet hosted by Cedar Falls High School Thursday, October 24, and for the first time since anyone can recall, and quite possibly ever, both the Kee girls and boys cross country programs will each be represented at the season-climaxing Class 1A State Cross Country Meet in the same year. The Hawk girls earned their third consecutive State Meet team qualification in championship fashion at the Cedar Falls State Qualifier, while the Hawk boys were headlined by the individual State Meet qualification earned by junior Chris Wagner.
Hauling one in ... Waukon football sophomore Braden Hemann looks in a pass for a catch in the Indians' 66-0 home victory over Anamosa Friday, October 18. Hemann hauled in two passes for 31 yards. View and find out how to purchase this photo and many more by clicking on the Photo Galleries link on this website.
A win this Friday would complete first undefeated regular season since the 1950s
The Waukon football team put on quite an offensive display for its hometown fans in the Tribe's final regular season game at home Friday, October 18, scoring on every one of its first-half possessions to bolt to a 60-0 lead by the halftime break on the way to a 66-0 victory over an Anamosa squad coming off its first win of the season last week. Those 66 points are the most scored by a Waukon football team since a 67-6 home victory over Fillmore Central out of Minnesota to start the Tribe's 2007 campaign and the most scored by a team under the guidance of Indian head coach Chad Beermann since his final season at Valley CEW, where his Tigers defeated Cedar Valley Christian by a 72-0 result in Eight-Man play during the 2012 season.
Wrapping up a Warrior ... Kee football senior Ryan Schulte wraps up a Central Elkader ball carrier in the Hawks' 72-6 home win over the Warriors Friday, October 18. Schulte posted a solo quarterback sack and assisted on three other tackles in the Kee victory, including one more tackle for a loss of yardage. Photo courtesy of the Kee High School Yearbook. View and find out how to purchase this photo and many more by clicking on the Photo Galleries link on this website.
Friday, October 18 was the final time the Kee football team would play in front of its hometown fans for this 2019 season, the final time this season's nine seniors would compete on their home football field. That final home stand of 2019 proved to be one to remember for both those fans and those seniors, as the Hawks erupted for the most points they've scored since the 2012 season, finding the end zone on all but two of its offensive possessions in the ballgame on the way to rolling to a 72-6 triumph in Eight-Player District 3 play over a Central Elkader team still in search of its first win of the season.
Setting up a swing ... Waukon volleyball junior Mia Strub pops up a set for her waiting teammates in the Indians' home loss to Charles City in three sets Tuesday, October 18. Strub assisted on 10 kills in the match while posting one each of kills and ace serves. View and find out how to purchase this photo and many more by clicking on the Photo Galleries link on this website.
The Waukon volleyball team wrapped up its regular season by solidifying sixth-place finishes in both its Northeast Iowa Conference (NEIC) regular season and at the NEIC Tournament this past week, completing both with 1-5 records against NEIC foes for sixth-place finishes in league play. That regular season effort was completed by a three-set sweep at home suffered at the hands of Charles City Tuesday, October 15, with the net Tribe then running through its NEIC opponents again all in one day at the NEIC Tournament hosted by New Hampton Saturday, October 19 to again defeat just one those six teams - the same winless Oelwein team the Indians beat during the regular season.
Haley Meyer and Chris Wagner each run to UIC Runner-Up honors; All five scored girls are All-UIC
The Kee cross country teams wrapped up their 2019 regular season schedule with the annual Upper Iowa Conference (UIC) Meet hosted by Clayton Ridge Thursday, October 17 in Guttenberg. Both the Hawks' girls and boys teams boasted the UIC individual runner-up in their respective races, with the Kee girls landing all five of their scored runners within the All-Conference top 15 in their respective races to return to the top of the team summit as this year's UIC team champions.
Team-high kills and blocks ... Waukon volleyball junior middle hitter Margaret Wacker blasts away for an attack in the Indians' three-set home loss to Crestwood Tuesday, October 8. Wacker shared the team-high kill total of 10 winners each with senior Leah Bulman and also paced Waukon's defense with three solo blocks. View and find out how to purchase this photo and many more by clicking on the Photo Galleries link on this website.
In its only competition scheduled for the week, the Waukon volleyball team hosted fellow Northeast Iowa Conference squad Crestwood in its annual "Think Pink" Night to raise awareness of October being designated as Breast Cancer Awareness Month. With both teams adorned in pink jerseys for the night, it was the Indians who ended up on the short end of a black-and-blue battle with the visiting Cadets, falling in straight sets by narrow scores of 22-25, 23-25 and 17-25.
Double-digit kill total ... Kee volleyball junior Jada Mitchell rises above the net to knock down a kill in the Hawks' loss at home in three sets to MFL/MarMac Thursday, October 10. Mitchell paced Kee's offensive and defensive efforts at the net with 10 kills and four solo blocks. Photo courtesy of the Kee High School Yearbook. View and find out how to purchase this photo and many more by clicking on the Photo Galleries link on this website.
The Kee volleyball team continued its trend of Upper Iowa Conference (UIC) match splits for another week, adding another UIC victory to its season record before having that fate reversed in a busy week of competition. The Lady Hawks first picked up that UIC win in four sets at Postville Tuesday, October 8 before falling at home to MFL/MarMac Thursday, October 10 in three sets. The Kee netters then traveled to Riceville Saturday, October 12 for their final weekend tournament of the season, winning three of four matches on the day to sweep their way into the championship bracket round of play before having their tournament day ended in the opening round of that bracket round.
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Casino Royale (Columbia, 1967). Spanish Language One Sheet (27" X 41"). James Bond. Starring Peter Sellers, Ursual Andress, ...Click the image to load the highest resolution version.
DescriptionCasino Royale (Columbia, 1967). Spanish Language One Sheet (27" X 41"). James Bond. Starring Peter Sellers, Ursual Andress, David Niven, Orson Welles, Joanna Pettet, Daliah Lavi, Woody Allen, Deborah Kerr, William Holden, Charles Boyer, John Huston, George Raft, Jean-Paul Belmondo. Directed by Val Guest, Ken Hughes, John Huston, Joseph McGrath, Robert Parrish. U-shaped tear in the top border that reaches into the image. Wear and tear along the edges. Minor cross fold separations. Faint creasing in the left side of the image. Fine.
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To God be the glory! LuoPads for women launched March 19, 2019. The documentary "Period. End of Sentence", which recently won an Oscar, is about the taboo of menstruation and lack of hygiene products in a small village in India. This village is like thousands in the world where women are ostracized and often prevented from leaving home or attending school during that time of the month. In many cases, women only have grass, leaves, or wood chips to use. A period should be the end of a sentence, and not the end of a girl's education.
The Sewing Bee Mission group is now sewing hundreds of washable and reusable feminine pads for women in need. These pads are combined with panties, a washcloth, safety pins, and waterproof bag to make a kit for a woman to use during menstruation at a cost of $9. You can help support this project with "Luo Pads" on the memo line of your gift to WUMC. Our 2019 goal is 200 kits.
We will continue to make dresses, shorts, and book bags. Our 2019 goals are 1000, 1000, and 1500, respectively. We are on target to make those goals. Since we started in 2014, we have distributed our products to 14 countries and 4 destinations in the United States. About 20 attend each sewing bee and 4 work exclusively from home.
Thanks to the dozens of people who volunteer their time and supplies to make this happen!


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Number 1 Unicorn
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