text:
10-year Plan
U astronomers tackle decade's biggest questions.
Astronomers and astrophysicists at the University of Utah have been driving discoveries in the field for years. The innovative research from the Department of Physics & Astronomy is making an impact in all areas that the national community has determined as priorities in a once-in-a-decade report that guides the direction of astro-research for years to come.
This Decadal Survey was commissioned by the National Academies of Sciences, Engineering and Medicine to identify goals and challenges for the exploration of the cosmos. Unraveling the secrets of the universe requires vision and extensive planning—astronomers and astrophysicists use massive ground observatories and sophisticated space telescopes for projects that need years of preparation. The guidance of the decadal survey is crucial to this effort.
Released in early November, the decadal survey highlights three key research areas ripe for discovery: "Worlds and Suns in Context" focuses on stars and planets; "Cosmic Ecosystems" describe galaxies and the cosmic web they form; and "New Messengers and New Physics" provides a new view of the universe through high-energy particles, gravitational waves, and deep sky surveys. Scientists in the U's Department of Physics & Astronomy are leaders in each of these areas.
Kyle Dawson
"Over the past several decades, department faculty pushed forward on an increasing number of research areas in astronomy, astrophysics and particle physics. Now these separate initiatives are coming together, in focus, and beautifully aligned with the decadal survey's top priorities."
Kyle Dawson, professor of physics and astronomy, will chair the Astronomy and Astrophysics Advisory Committee (AAAC) in the first full year following the release of the decadal survey. The AAAC is a national panel of experts who advise the National Science Foundation, NASA, and the Department of Energy toward issues within the fields of astronomy and astrophysics that are of mutual interest. "We meet regularly with leadership from the federal agencies that sponsor research in astronomy and astrophysics. The decadal survey gives our panel a guide to work with those agencies to assess progress toward new programs that will allow the United States to maintain its role as a leader in astronomy and astrophysics research."
Over the past several decades, department faculty pushed forward on an increasing number of research areas in astronomy, astrophysics and particle physics, notes Professor Dawson. "Now these separate initiatives are coming together, in focus, and beautifully aligned with the decadal survey's top priorities."
Worlds and Suns in Context
The sun hosts a rich system of planets, from the massive gas giant Jupiter and the icy dwarf planet Pluto, to Earth, the only body in the universe known to sustain life. Recent observations from space and the ground have revealed thousands of other worlds around distant stars. Some are so large as to dwarf Jupiter, others appear to be exotic water worlds. A precious few may even harbor life. A key priority of the decadal survey is to understand the nature and origin of these worlds and the stars that host them. Driving this quest is a profound question, whether we are alone in the cosmos.
Mock-ups from a fast-migration sim (Jupiter through a massive pebble disk) w/planets + host star added.
The Sloan Digital Sky Survey, (SDSS), an international effort to chart the cosmos, is mapping stars across our galaxy, the Milky Way. Scientists at the U are in leadership roles in this large-scale, on-going collaboration. With detailed measurements of millions of stars, SDSS will provide an understanding of their chemical composition, how the elements are spread throughout the galaxy, and the connection between stars, their composition and the planets they host. This world-class project is integral to the decadal survey's scientific goals.
Research at the U also focuses on planet formation, how worlds emerge from the gas and cosmic dust that encircle all observed young stars. Simulations run on high-performance computers track this process, how planetary building blocks come together, sometimes through violent collisions, to grow into the planets like those in our solar system and around other stars in the cosmos.
Cosmic Ecosystems
Looking beyond the stars visible in the night sky, astronomers have discovered a wealth of exotic objects, including neutron stars, with the mass of the sun packed into a region the size of a small city, and black holes, where matter is so concentrated that space and time warp to form an event horizon, from which nothing, not even light, can escape. Telescopes also reveal galaxies, like our own Milky Way, with hundreds of billions of stars, even supermassive black holes in their centers, strewn across space. Neighboring galaxies, drawn together by gravity, form enormous clusters, the most massive objects in the universe. They are permeated by dark matter, an unidentified, ethereal substance known only through its gravitational influence. Together with galaxies and galaxy clusters, the dark matter sea forms patterns – knots, sheets and walls in a vast cosmic web. A second top priority of the decadal survey is to understand this cosmic web, the structures it contains, and how these structures formed out of the hot, dense early universe.
At the U, researchers are studying the ecosystems that produced this diversity of cosmic structure. With theoretical and computer studies, as well as observations from the ground and space, Utah faculty are probing the nature of galaxies, the central supermassive black holes they harbor, and how stars, gas, and dark matter interact to produce the cosmic structures we observe today. Research on nearby small galaxies, including satellites of our Milky Way and other nearby massive galaxies, will help us understand their formation histories and the role of dark matter in that formation. Upcoming observations with NASA's James Webb Space Telescope, the most sophisticated observatory ever launched, will help university researchers discover supermassive black holes in the central regions of galaxies to learn how these exotic beasts formed. At larger distances and earlier times, large clouds of gas – the precursors of galaxies– provide key diagnostics for researchers at Utah to identify the underlying physics of galaxy formation. Galaxy clusters, with up to thousands of galaxies bound together, are also in focus at Utah as researchers take advantage of NASA's NuSTAR mission to study the hot X-ray emitting gas trapped in these massive objects. These separate research threads are weaving together a more complete and compelling picture of cosmic structure formation.
New Messengers and New Physics
Studies of the universe began with optical telescopes, using our eyes to capture the signal from distant sources. As technology advanced, we used cameras to record this light, thus allowing for longer integrations and deeper insights into the cosmos. We soon began to explore the cosmos with light not visible to our eyes, from radio waves to X-rays to light with even higher energies. The scientific community has continued to add new messengers from the cosmos beyond the electromagnetic spectrum: High energy particles, neutrinos, and gravitational waves. Combining these multiple messengers is key to understanding the underlying physics of the most extreme events in the cosmos such as stellar explosions, collisions between black holes or neutron stars, and the dramatic forces in the regions surrounding supermassive black holes. Our understanding of the universe has advanced with each new way of observing the sky.
Bryce canyon skies. photo: Anil Seth
The faculty at Utah helped introduce some of these new messengers to the field of astrophysics. The Telescope Array, near Delta, Utah, is the most recent in a series of Utah experiments to study very high energy particles. The highest energy particle on record was detected from this sequence of experiments in Utah. The Utah faculty round out the full suite of messengers with significant contributions to the LIGO interferometer that is used to detect gravitational waves, the IceCube Neutrino Observatory at the South Pole, and the Veritas and HAWC (High-Altitude Water Cherenkov) observatories, and the future CTA and SWGO observatories used to detect the highest energy photons. The Utah faculty also leverages national facilities to use everything between radio and X-rays to explore the physics behind the most dramatic events in the universe.
This theme within the decadal survey also includes new physics, particularly the unknown physical natures of dark matter and dark energy. The possibility for discovering new fields, new particles, new laws for gravity, or new particle interactions motivated the construction of the Vera C. Rubin Observatory in Chile and the Dark Energy Spectroscopic Instrument in Arizona. Faculty in Utah use the data from these observatories to constrain models of fundamental physics and hunt for the signatures of new physics. Faculty in Utah are also making theoretical predictions for new signatures that dark matter or other new physics may introduce into the full suite of astronomical detectors that are used to track the multiple messengers from the cosmos.
Utah Faculty Researchers
John Belz - Studies the composition of the highest-energy cosmic rays, and investigated the use of novel instruments for their detection. He also uses computational techniques to model extreme spacetimes at the threshold of black hole formation, work complementary to the studies carried out by the Utah gravitational wave physics group.
Douglas Bergman - Uses observations of ultra high energy cosmic rays to test fundamental physics at the highest energies and to explore where extreme acceleration mechanisms exist in the local universe.
Benjamin Bromley - Explores the formation of planets using supercomputer simulations. This work identifies the conditions necessary for a star to host a planet like Earth.
Joel Brownstein - The head of data for the Sloan Digital Sky Survey (SDSS). He uses the distribution of luminous matter and dark matter to explore cosmic ecosystems.
Kyle Dawson - Co-spokesperson who sets priorities for cosmological studies within the 500-member, Dark Energy Spectroscopic Instrument (DESI) collaboration. He uses these spectroscopic data to search for new physics such as dark energy, new theories of gravity, and new fields that affect the evolution of the cosmos.
Paolo Gondolo - Studies theoretical models for new physics related to the nature of dark matter, and uses multi-messenger observational and experimental data to test them.
Charles Jui - Uses ultra high energy cosmic rays as a messenger to explore where extreme acceleration mechanisms exist in the local universe.
David Kieda - Leads multi -messenger astrophysics observations using high energy gamma rays as a messenger to explore particle acceleration around supernova remnants, neutron stars and black holes. Head of US development effort for ultra-high resolution interferometric observations of stars and binary systems.
Tanmoy Laskar - Uses light across the electromagnetic spectrum to investigate new physics in distant cosmic explosions.
Yao-Yuan Mao - Searches for galaxies in the nearby universe that are much smaller than the Milky Way and studies their roles in the cosmic ecosystems and their connection to dark matter.
John Matthews - Uses ultra high energy cosmic rays as a messenger to explore where extreme acceleration mechanisms exist in the local universe.
Carsten Rott - Studies neutrinos as a member of the IceCube collaboration, an observatory built into the pristine ice of the South Pole.
Pearl Sandick - Studies possible explanations for the dark matter in the Universe, how to confirm its nature experimentally, and how it affects our understanding of particle physics.
Anil Seth - Uses NASA's recently launched James Webb Space Telescope, the Hubble Space Telescope, and other national facilities to study cosmic ecosystems and supermassive black holes.
Wayne Springer - Uses very high energy gamma rays as a messenger to explore particle acceleration around supermassive black holes.
Daniel Wik - Takes a broad view of cosmic ecosystems by exploring clusters of galaxies and their wells of hot gas.
Gail Zasowski - Uses positions, motions, ages, and chemical makeup of millions of stars in the Milky Way and nearby galaxies to better understand today's worlds and suns.
Yue Zhao - Leads the Utah gravitational wave physics group in the Laser Interferometer Gravitational-Wave Observatory (LIGO).
Zheng Zheng - Studies the connection between galaxies, the dark matter halos in which they live, and the gas that flows in and out of these dark matter halos.


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Q: Arcpy: creating a line on an existing line based on points' coordinates I have a point which is some meters away from an existing line:

This point should be snapped to the line (to the closest part) and then, based on the points' new coordinates, a new line Feature Class should be created, which is on the existing line 1,5 meters left and 1,5 meters right (so 3 meters total) of the point. Therefore it should look like the following picture:

Existing Datasets shouldn't be used, the result should be in a new FC.
Here is the code is used so far:
    import arcpy
    arcpy.env.workspace = arcpy.GetParameterAsText(0)
    point_feature = arcpy.GetParameterAsText(1)
    line_feature = arcpy.GetParameterAsText(2)

    # Make backup copy of point feature class, since modification with
    #  the Editing tools below is permanent

    arcpy.CopyFeatures_management(point_feature, "point_feature_backup")

    # Snapping-Tool

    arcpy.Snap_edit(point_feature,[[line_feature,"EDGE","50 METERS"]])

    # Getting the coordinates of the new snapped Point

    with arcpy.da.SearchCursor(point_feature, ['SHAPE@XY']) as cursor:
        print ("Coordinates of the snapped point: {}".format(row[0]))

    # Creating the new line, I used phantasy coordinates here, it was just a test, the new Coordinates should be on the already existing line 1,5m left and 1,5m right of the snapped point
    cursor = arcpy.da.InsertCursor(line_feature, ["SHAPE@"])

    array = arcpy.Array([arcpy.Point(1823123.213, 6139654.819),
                         arcpy.Point(1823123.244, 6139654.869)])

    polyline = arcpy.Polyline(array)

    cursor.insertRow([polyline])

The hardest part for me is to find out how to get the 1,5m on both sides...which tools could be used to do that or is there an alternative way?

A: There are two answers depending on your definition of distance: bird's flight or along the road. they wil be identical on a straight line but differ on curves or broken lines.
bird's flight
you could create a buffer around your point, then intersect the buffer geometry with the line. You can do this for all your points at once using the geoprocessing tool on the feature class or work on the geometry objects within a cursor.
with arcpy.da.SearchCursor(point_feature, ['SHAPE@']) as cursor:
    for row in cursor:
        buffer = arcpy.Buffer_analysis(row[0], arcpy.Geometry(), "1.5 meters")[0]
        line_feature = arcpy.Clip_analysis(input_lines, buffer, arcpy.Geometry())[0]
#do what you want with the resulting geometry

Distance along line
For distance along line you can use linear referencing tools. You'l first need to create measures on your lines, then you can locate the feature along the route and then create a route event by adding/removing 1.5m  from your point measured value. The created layer can be stored as a geometry if needed. (with arcpy copy )

redpajama_set_name: RedPajamaStackExchange


text:
Bowbrook Meadows
Kerry & Steven
Mon: 10am - 5pm
Tue: 10am - 5pm
Wed: 10am - 5pm
Thurs: 10am - 5pm
Off Mytton Oak Road, Shrewsbury, Shropshire, SY3 5BS
Book an appointment Download a brochure
Open daily 10am to 5pm
Price (highest to lowest) Price (lowest to highest) Bedrooms (lowest to highest) Bedrooms (highest to lowest)
The Arundel
The Oxford
The Durham
The Wimborne
About Bowbrook Meadows
Our stunning new development in Shrewsbury at Bowbrook Meadows has proven to be one of our most popular developments.
Located on the outskirts of Shrewsbury it offers plenty of open areas ideal for walking and views across green nature. Our final phase includes some of our classic homes; offering spacious rooms and family space.
This development has several phases, click here to view the other phase(s) development plan(s).
Note: This plan has been produced for plot identification purposes only. Layout, individual plots, housetypes and amenities may be subject to change. For latest information, including selected plots, please contact sales advisor. Overall development layout plan correct at time of publication.
Bowbrook Meadows just over 2 miles from Shrewsbury town centre and a few minutes' drive from the A5.
Wolverhampton is approximately 36 miles and Birmingham about 50.
The town has good bus and coach services with three park and rides.
Trains run from Shrewsbury Railway Station to Birmingham, Telford, Wolverhampton, Manchester, Cardiff and London Euston.
For air travel, Manchester and Birmingham Airports are both about 64 miles.
A trip to the shops
Shrewsbury has a great mix of popular high street stores alongside the quirky independents at Wyle Cop that offer everything from vintage clothing and jewellery to rare book and antiques.
The town's medieval passageways are home to a variety of boutiques, while latest fashion and chain stores can be found at the Darwin and Pride Hill shopping centres.
The Parade offers dozens of independent shops, while the Market Hall offers local produce, crafts and curios.
Dating back to 1074, Shrewsbury has a rich heritage with more than 660 listed buildings, a red sandstone castle, an abbey and a cathedral.
The birthplace of Charles Darwin, Shrewsbury was built alongside the River Severn and has nine bridges and many pretty riverside walks, a riverboat and the bankside Theatre Severn.
For history and culture, visit the impressive Shrewsbury Museum and Art Gallery and see St Chad's a round church close to the 29 acre, Quarry Park featuring The Dingle, a landscaped sunken garden.
The town has many sports clubs including cricket, rowing, rugby, running and motorsports, while Shrewsbury Sports Village is a modern sports centre. The Shropshire Hills, an Area of Outstanding Natural Beauty, are also with in easy reach.
There are a number of primary schools within one mile of Bowbrook Meadows including Oxon Primary, Woodfield Infant School, Saint George's Junior School and Radbrook Primary School.
For senior pupils there's The Priory, an Academy Trust rated outstanding by Ofsted, Meole Brace School Science College and Shrewsbury Sixth Form College.
The Shrewsbury College of Arts and Technology offers vocational courses.
This is a map of the local area
From M54
Exit the M54 at junction 7 continue onto the A5 passing through four roundabouts signposted A5
At the next roundabout take the 3rd exit onto Mytton Oak Road/B4386
Continue for approximately one mile and the development is on the right hand side.
Directions from your location:
Click on the marker to get directions to the development from any location or postcode
Sorry, Google maps are not working, please check your have javaScript enabled.
Request a viewing Download a brochure
5 bedroom detached
4 bedroom town house

redpajama_set_name: RedPajamaCommonCrawl


text:
Q: Am I allowed to ask for the OP's email in a comment to send him source codes? I met this situation here: the OP (who's new on SO) was looking for something that I've already done, but it's a (sure small but) real project and I can't put all the sources on the answer (JAVA, XML, properties, etc.).
How should I process then? May I ask his email in a comment?

A: If you do end up providing actual files to the OP in one manner or another you'll need to remember that the question itself is still going to remain long after they've sorted the problem themselves. The question remains because StackOverflow is a site for repositories of answers, not quick support fixes. It's conceivable that other people will have the same issues in future, search SO / Google for the problem and see this question and your answer. The fact that at one point in history you provided some actual (long deleted) files to the original asker of the question isn't going to be of any help to them though, making the answer worthless.
Really, if the answer requires so many files and examples to be of use then either a) the question itself is far too broad to fit the site so should be updated, or b) the answer should be structured so that just the relevant parts of the code are included thereby benefiting future visitors too.

A: When the problem is that you have code too big to include in the answer, assuming you're willing to make the code public, the best solution is usually to host it elsewhere and link to it. You can use a pastebin for this (such as pastebin.com, or, as we often use on Ask Ubuntu, paste.ubuntu.com — there are many others, of course).
If one of the reasons the source code should not be included in a post on a Stack Exchange site pertains to its licensing, and the code is in a pastebin, I recommend raising that point explicitly in your answer. (This may help to prevent others from editing some of it into your question, if their edits would be beyond the limits of fair use.) If the code is somewhere like Github, then presumably it's part of a source tree with a copyright statement...
In any case, it's advisable for every source code "file," whether it's a real file or simply a page in a pastebin that may or may not correspond to an actual file, to contain a prominent, visible copyright statement at the top, with licensing information if applicable. That advice doesn't really have anything to do with Stack Exchange--it's just good practice, generally. It's good practice even for source code that is not intended to be released to anyone at all. (Please note that you do not need a copyright notice for your source code to be copyrighted, however. Under U.S. law since the 1970's and international treaties, a work is copyrighted by its author automatically upon creation, and the copyright must be explicitly disclaimed in order not to exist. Oh, and I'm not a lawyer and nothing in this post is legal advice.)
(If the source code is public domain, then of course it should not have a copyright statement, but you can still have a statement indicating that it is public domain.)


text:
La Gran presa de Inga es un proyecto hidroeléctrico en el río Congo en la República democrática de Congo. Estaría situada en la proximidad de las cataratas de Inga en la provincia del Bajo-Congo, a una treintena de kilómetros al norte de la ciudad de Matadi. Dos embalses, Inga I y Inga II existen ya en la zona.

Hay otro proyecto para un tercer embalse, denominado proyecto Inga III, que se aprovechara de la existencia de los embalses Inga I y Inga II. El proyecto Gran presa de Inga es de otra naturaleza, ya que necesita de trabajos e inversiones complementarias a Inga I, II, e III.

Historia
En 1921 un estudio llevado a cabo por el  Servicio Geológico de Estados Unidos concluyó que la totalidad de la cuenca del río Congo poseía más de una cuarta parte del potencial de energía hidráulica del mundo. En 1960 se inició el proyecto denominado "Gran Presa de Inga" que construyó Inga I entre los años 1968 y 1972 con financiación del gobierno de la República Democrática del Congo. En 1982 se inauguró Inga II y comenzó a planificar la construcción de Inga III y buscar financiación para el mismo. En el año 2016 el Banco Mundial retiró su apoyo al proyecto Inda III por desacuerdos con el gobierno del Congo. En 2018 se designó a unas compañías  chinas y españolas como codesarrolladoras del proyecto, pero en un cambio político en la dirección del país prefirió un proyecto de menor tamaño al propuesto lo que hizo que la empresa española  ACS se retirara del proyecto en 2020.

En 2021 el empresario  australiano Andrew Forrest  mediante su compañía Fortescue Metals Group manifestó  que  tenía la intención de invertir 100.000 millones de dólares en el desarrollo de las principales plantas hidroeléctricas, solares y geotérmicas de África y estaba en negociaciones con el gobierno de la República democrática del Congo para impulsar el conjunto de proyectos Gran Inga, que completaría con otros  de  países vecinos.

La Fortescue Metals Group  manifestó su intención de convertirse en un importante productor de energía eléctrica renovable o limpia en África que destinaría a la producción de hidrógeno para su posterior venta en Europa. El gobierno del Congo  señaló  a la compañía Fortescue  como  única operadora de toda la Gran Inga.

Inga I, II, e III
Inga I, II, e III han sido o tendrían que estar construidos en el margen derecho del río, aprovechando al existencia de un valle seco, Nkokolo, antigua cama del río. Sus márgenes alcanzaban, antes de ser anegados, 150 metros de altura al nivel de las cataratas del Inga, paralelas al nivel del embalse. Está utilizado para alimentar de agua Inga I y Inga II, eventualmente Inga III.

Un embalse, el embalse de Shongo, ha permitido poner bajo agua el Nkokolo. El agua es captada a 10 kilómetros del embalse Inga II, a una altitud de 125 metros, para alcanzar 115 metros al nivel del bief que alimenta los embalses Inga I y Inga II. Un canal de una longitud de algunos centenares de metros, ubicado al oeste del embalse Inga I (45 metros de desnivel, 115-70 metros), alimenta el embalse Inga II (50 metros de desnivel, 115-65 metros). Un canal excavado aguas arriba de las otras dos presas permitiría que la presa Inga III se construyera debajo de las otras dos presas, beneficiándose así de una diferencia de elevación de 55 metros (115-60 metros). Los 3 embalses desarrollarían así una potencia total de 6 275 MW a potencia plena (Inga I e II funcionan actualmente a aproximadamente 20 % de su capacidad, y Inga III no existe todavía).

Gran Inga
La Presa gran Inga permitiría la constitución de una central de una potencia de 39 000 MW. El proyecto prevé la construcción de un embalse a contracorriente del apresamiento de agua de Nkokolo, que permitiría generar una represa de agua con una altitud de 200 metros (contra 125 metros actualmente al mismo sitio) en el valle del río Bundi, que sería vallada, algunos kilómetros más lejos por un embalse a la altura de su confluencia con el río Congo (actualmente a 45 metros de altitud). Entre la represa de agua y el río, a partir de ahora 155 metros de desnivel sobre el segundo río más potente del mundo. Una central construida allí tendría una potencia de 39 000 MW, con doble potencia que el embalse de las Tres-Gargantas en el río Yangzi, pero con una inversión y costes ecológicos sensiblemente menores que en las Tres-Gargantas, en Asuán o Itaipú.

In fina, el total del complejo de los embalses de Inga (a veces denominado como "Gran Inga") comprendería 4 unidades de producción, para una potencia total de 45 275 MW repartida como sigue:

 Inga I (funcionando actualmente al 20 % de sus capacidades, 45 metros de caída):
 Inga II (funcionando actualmente al 20 % de sus capacidades, 50 metros de caída): 1 424
 Inga III (en proyecto, 55 metros de caída) : 4 500
 Grande Inga  / central de la Bundi (en proyecto, 155 metros de caída) : 39 000

En 2015, los planes para ampliar el emplazamiento actual y para financiar el Inga III y el Grand Inga están todavía en la mesa de dibujo.

Oposición al proyecto
Ciertos observadores critican el proyecto por su elevado coste (estimado entre 80 y 100 mil millones de dólares) en un país conocido por su corrupción endémica, y que por lo tanto puede ser de poco beneficio para la población. Además, millares de hectáreas de bosque serían anegados, lo que perjudicaría la biodiversidad y los ecosistemas locales. Sin embargo, la respuesta es que el daño asociado al desarrollo del proyecto sería mucho menor que los beneficios que podría disfrutar una gran parte del África subsahariana.

Referencias

Enlaces externos
 Katembo Fotografías de los websites de Inga I e II en 2005

Represas de la República Democrática del Congo
Provincia de Bajo Congo

redpajama_set_name: RedPajamaWikipedia


EL PASO, Texas, April 12, 2019 /PRNewswire/ -- Church's Chicken® is celebrating the opening of its newest El Paso, TX location in the area loved by its former president of the Church's Independent Franchisee Association, David Newman, who passed away suddenly earlier this year. The Newman family is staying true to their patriarch's goal of extending the availability of the great taste of Church's—along with the community involvement the brand is known for—to El Paso.
The official grand opening is set to take place on April 13th from 11 a.m. till 2 p.m. at 13296 Socorro Rd. San Elizario, TX 79849.
"It's always a pleasure to bring high-quality food to my community. Texas is where Church's was born, so it's no surprise we have such a demand for delicious down-home flavor right here in El Paso," said long-time zone director Victor Cortez, who now assists and operates the restaurants for the family.
The restaurant is located at 13296 Socorro Rd. Guests will find the restaurant bears the attractive STAR Image Design, which includes Church's latest interior seating options, new exterior design and color palettes, and contemporary lighting inside and out.
Church's is world-renowned for their freshly-prepared original and spicy chicken and fresh-baked Honey-Butter Biscuits™ made from scratch daily. "At Church's, we are dedicated to providing great chicken experiences for every guest who walks in our doors," said Peter Servold, Executive Vice President of US Operations at Church's Chicken.
Founded in San Antonio, TX in 1952 by George W. Church, Church's Chicken® is one of the largest quick service restaurant chicken chains in the world. Church's® specializes in Original and Spicy Chicken freshly prepared throughout the day in small batches that are hand-battered and double-breaded, Tender Strips®, Honey-Butter Biscuits™ made from scratch and freshly baked, and classic, home-style sides all for a great value. Church's® (along with its sister brand Texas Chicken® outside the Americas) has more than 1,500 locations in 23 countries and international territories and system-wide sales of more than $1 billion. For more information, visit www.churchs.com. Follow Church's® on Facebook at www.facebook.com/churchschicken and Twitter at www.twitter.com/churchschicken.


Original 2004 29&1/2 x 19&1/2 (appx.) oil on masonite board painting (professionally framed under UV-filtering plexiglas in a hand-painted carved wood frame) by the one and only Stanley Mouse.
Painting has also been SIGNED and dated and features an AWESOME rendition of an eagle flying out of a radiant sun... a SUPREMELY cool design, somewhat reminiscent of the Phoenix image Stanley created for the Grateful Dead in 1979. As this is a framed piece of original art (originally obtained directly from the artist's studio), a letter grade doesn't really apply here but overall the piece is in GREAT shape.
A VERY unique opportunity, as original Mouse art of this magnitude does not surface very often... and this one is a real gem.


text:
Lagoa Cimidor is a small coastal lagoon in the southeastern part of the island of Maio in Cape Verde. It is situated 3.5 km northeast of the village Ribeira Dom João and 13 km east of the island capital Cidade do Maio. It is part of a  protected area (Reserva Natural da Lagoa Cimidor) which also includes the adjacent coast.  One of the largest permanent bodies of water on the island, it is an important area for birds and turtles.

See also
List of lakes in Cape Verde
List of protected areas in Cape Verde

References

Bodies of water of Cape Verde
Geography of Maio, Cape Verde
Protected areas of Cape Verde


text:
You are here:News•Successful birth after ovarian tissue transplantation
Successful birth after ovarian tissue transplantation
33-year-old woman from Sweden successfully gave birth to a child after transplantation of her own frozen ovarian tissue.
Ten years ago 23-year-old Lotte was diagnosed with a malignant tumor. The woman was prescribed chemotherapy, which could not but lead to infertility. But doctors at the Department of Reproductive Medicine of Karolinska University Hospital in Stockholm had frozen healthy ovarian tissue of the woman before chemotherapy.
Lotte has successfully undergone a course of treatment from cancer, and in summer 2012 her own ovarian tissue was transplanted to her. After a course of hormonal stimulation and procedure of artificial insemination the woman successful got pregnant. And on the last Monday in the Mälarsjukhuset hospital of the city Eskilstuna the daughter of Lotte and her husband Magnus was born. The girl was named Freya.
According to the doctor who performed the transplantation of ovarian tissue, Kenya Rodriguez-Wallberg, there are only 25 children all over the world that were born after a similar operation.


text:
Q: How to flatten a dictionary> in linq and keep the key in the results How do you achieve the following in linq?  I feel there should be a Linq alternative.
    var foods = new Dictionary<string, List<string>>();
    foods.Add("Cake", new List<string>() { "Sponge", "Gateux", "Tart" });
    foods.Add("Pie", new List<string>() { "Mud", "Apple" });
    foods.Add("Roll", new List<string>() { "Sausage" });

    var result = new List<Tuple<string, string>>();
    foreach (var food in foods)
    {
        foreach (var detail in food.Value)
        {
            result.Add(new Tuple<string, string>(food.Key, detail));
        }
    }

ie
cake <sponge, gateux>
pie <apple>

to

cake, sponge
cake, gateux
pie,  apple

thank you

A: You can use SelectMany extension method:
var result= foods.SelectMany(f=>f.Value.Select(s=>new Tuple<string, string>(f.Key, s)))
                 .ToList();

A:  var result = (from food in foods
               from detail in food.Value
               select new Tuple<string, string>(food.Key, detail)).ToList();

A: Linq is a query.  That is what the 'q' stands for.  You are adding items into a dictionary.  Try this
            Dictionary<string, List<string>> foods = new Dictionary<string, List<string>>()  {
               {"cake",  new List<string>() {"Sponge", "Gateux", "Tart"}},
               {"Pie",  new List<string>() {"Mud", "Apple"}},
               {"Roll",  new List<string>() {"Sausage"}},
            };


Wide territory in the Horn of Africa (extended not much more than the double of Italy) without a true state, without institutions, without services.
At the present time there are two declared independent Republics (the Somaliland and the Puntland) under the control of armed militias of Egal and Ahmad.
The consequence of that all is war, armed bands, thousand of refugees.


text:
Who is the 2012 Money in the Bank winner?
In the main event, John Cena won the Money in the Bank ladder match for a WWE Championship match contract, while in the opening bout, Dolph Ziggler won the other Money in the Bank ladder match for a World Heavyweight Championship match contract.
Which Money in the Bank did CM Punk win?
John Cena Fired?! WWE Money in the Bank has come and gone, and it may very well be the best PPV of the year, surpassing Extreme Rules in that category. The show delivered in every aspect, and may go down as one of the best PPVs ever.
Who has cashed in Money in the Bank and lost?
John Cena, Damien Sandow, Baron Corbin, and Braun Strowman are the only Money in the Bank contract holders to cash in and fail to gain a championship.
Who was Mr Money in the Bank 2011?
Daniel Bryan won the SmackDown Money in the Bank Ladder Match. Eight of SmackDown's most gifted Superstars battled for the coveted Money in the Bank briefcase, but a tenacious Daniel Bryan was the man who walked away with the future in the palm of his hands.
Who won Money in the Bank 2013?
Randy Orton Wins WWE Championship Money in the Bank Match.
Who is the current Money in the Bank holder 2021?
In the main event, Roman Reigns defeated Edge to retain the Universal Championship. Additionally, Big E and Nikki A.S.H. won their respective men's and women's Money in the Bank ladder matches.
Who is the current Mr Money in the bank?
MITB winner is determined by a special Money in the Bank ladder match involving six or more wrestlers….Men's Winners.
Event & Date
Money in the Bank (May 19, 2019)
Held For
Cash In Date Event & Date
Extreme Rules(14 July 2019)
Cash in Against
Seth Rollins(Universal Championship)
Who was the first woman to win 2 Money in the Bank matches?
Women's Winners
1. Carmella Money In The Bank (June 18, 2017)
2. Carmella Money in the Bank
3. Alexa Bliss Money in the Bank (June 17, 2018)
4. Bayley Money in the Bank (May 19, 2019)
When did money in the Bank 2012 take place?
It took place on July 15, 2012, at the US Airways Center in Phoenix, Arizona. Money in the Bank featured seven professional wrestling matches that involved different wrestlers from pre-existing feuds or and storylines that played out on WWE's primary television programs.
What were the reviews of money in the bank?
Money in the Bank received generally positive reviews. The Baltimore Sun called the pay-per-view "Strong, if unspectacular"; they praised the WWE title match calling it a "fun ride" and that "The no disqualification stipulation really added to the contest". Both Money In The Bank matches were well received. 411 mania awarded the pay-per-view a 7.
When did Daniel Bryan Cash in his money in the bank?
Daniel Bryan cashes in his Money in the Bank contract at WWE TLC 2011 Daniel Bryan shocked the WWE Universe when he won the SmackDown Money in the Bank Ladder Match on July 17, 2011, then followed it up with an equally surprising announcement: He would cash in his title opportunity on The Grandest Stage of Them All, WrestleMania XXVIII.
What was the main event of the money in the bank?
The main event was the Money in the Bank Ladder match for a WWE Championship contract involving John Cena, Big Show, Chris Jericho, Kane and The Miz. Cena performed an Attitude Adjustment on Big Show through a broadcast table and then the other wrestlers buried Big Show under several ladders.
Is Chevy Cobalt a reliable car?
What is an archaeological site for kids?


A rare find on one of Calgary's most sought after streets. Fabulous two-storey split on Willow Park Green, backing on Willow Park Golf & Country Club. An exclusive home with private south back yard, magnificent view of the Golf Course and has a triple attached, heated garage. Main floor boasts open living with gas fireplace, dining area with vaulted ceiling, spectacular kitchen and eating area designed by Empire Kitchens, family room with wood burning fireplace, library, office, powder and laundry rooms. Kitchen appliances are high quality with separate Sub Zero stand up and sliding drawer fridge/freezer units and wine storage. Wolf 48' dual fuel range with French cooktop. Integrated main floor Bank and Olufsen audio system "powerful and distinctive looking". Four bedrooms up and three full baths including 5-piece master en-suite (travertine tiles & Corian countertop). Basement fully developed with rec room/wood burning fireplace, hot tub room, bedroom, office, full bath. Two new high efficiency furnaces.


Let me begin: I live in the south, and more specifically, in the Ozark Hills of Arkansas where idyllic outdoorsy wonderlands began. We are people accustomed to humidity, mosquitoes, tornadoes, and flip flops. Winter is simply the novelty month that stitches together the cool crisp colors of autumn with the rainy green squishy-ness of spring. Our winter has us reveling in making a pot of chili and building our one fire in the fireplace. Snow flurries usually send many of my fellow southerners into a frenzy, scavenging for the last supplies of bread and milk in the region. I've still no idea what we do with all that milk and bread, but we buy it in bulk before every predicted snow like its our job, much like the way we all grow tomatoes in summer when we have no need for three truckloads of tomatoes. Its our DNA. We can't help it.
A southern snow storm is an event that last, at most, 24 hours. A few hours of "oh, the pretty flakes" are followed by nervous drives to work, ending with hours of discussion with co-workers which detail every moment of our snow-bound journey to the office through one inch of snow. Blow. By. Blow. The snow melts somewhere in the middle of the fifth telling of our tale, and the drive home is clear and warmer. Such is the pattern of a southern snow storm. It goes faster than our stories.
But this year -- oh, this year -- has us lost in utter confusion. Winter began on December 5 with several inches of snow and has taken few breaks since then. We haven't seen the grass in over a week. It's been below freezing for nearly a month, and our faucets are set on perpetual trickle to prevent frozen pipes.
We are tired of eating chili and know no other wintertime food because we never needed to know more than chili. Winter has never lasted this long before. Shivering people wander the grocery store aisles, muttering from beneath seven layers of clothing, and habitually grab milk and bread from the shelves. We don't even understand why we do it anymore. We do it because it's all we know to do. This winter has dished out more than we can handle. We are not equipped for this. We are a lost people. Covered in snow with perpetually frosted extremities, we wander through our days reminiscing about what the sun used to look like and fondly remember how it felt to wear shorts.
Our snow shoveling skills are improving, much to our dismay. We never yearned for such skills and used to shake our heads at television news reports showing New Englanders pushing show with metal-ended sticks. Give us a tornado, and we know how to respond quickly, like a well-choreographed ballet. Give us 100+ degree temperatures, and we open the fire hydrants and break out the swimsuits. But we don't do winter well.
So here I sit at the end of yet another week of frozen existence where a walk to the mailbox is a life or death choice. More snow is predicted for next week, and I have run out of cheery banter about the frigidness of our weather. It's not funny anymore. This morning I dreamed of mosquitoes. That is a sure sign of mental anguish over this whole winter thing.
Stella and George's eyes say it all: "Mom, these sweaters are getting old."
It's only February 7, and winter has five official weeks left but we, as a people, are dwindling fast. Nerves are frayed, tempers are short, and our southern charm ran out three weeks ago. Near-stampedes have occurred as we run outside for the five minutes of sunlight that peaks through the gray skies. We are desperate. And cold. We're really cold. Deliriously cold. C'mon -- I dreamed of mosquitoes. We are deliriously cold! It may be too late for us.
You cannot move a tropical creature to the Arctic and expect no consequences. You cannot surround a southerner with unrelenting winter weather and expect the same person at the end as when you began. We are not cut out for this. We have met our match. Old Man Winter has won. He beat us.
Wait . . . what's that? It's snowing again? Oh, crap . . .
oh my goodness....stay warm dear!!


text:
An elliptical set from the Mountain Goat(s)
By Richard Cromelin
May 31, 2004 12 AM PT
Times Staff Writer
"I am a mole, sticking his head above the surface of the earth," John Darnielle sang during his show at Spaceland on Friday. The lyric had a dual role in this case, describing not only the psychological state of the character in the song, but also the physical setting at the club, where Darnielle's seated position left him eye to eye with the fans in front of the stage and barely visible to those farther back.
It was an apt posture for someone whose music is often elliptical and elusive. Darnielle, who records and performs under the group name the Mountain Goats, has moved to the forefront of indie-rock's singer-songwriter cadre, and while the spare setting of Friday's show left things musically monochromatic -- his acoustic guitar strum was accompanied only by a bassist -- Darnielle kept the faithful enraptured with his sharp, powerful singing and manic conversation.
As he talked about the pitfalls of playing in his old home (the North Carolina-based performer hails from nearby Claremont) and diagramed the neuroses behind his fear of playing a new song, Darnielle was both cheerily engaging and slightly precious. As a singer, he evokes such artists as Jonathan Richman, Frank Black and David Byrne, wrapping them up into a sort of anti-Dashboard Confessional persona -- with the same sort of intimate intensity, but often dark and mordant rather than relentlessly encouraging.
The prolific Darnielle mixed older songs with some compelling vignettes from the Mountain Goats' new album, "We Shall All Be Healed." In such songs as "Palmcorder Yanja," about a bad night at a Travelodge with a group of speed freaks, Darnielle showed that he's a deft, detailed chronicler of a generation in a state of drift and uncertainty. A fuller musical palette onstage would have served that vision better. It wasn't until he was joined at the end by drummer Alianna Kalaba, from the opening act We Ragazzi, that these Mountain Goats truly kicked.


text:
Home> Top> Uk>Top 10 Special Occasion Dresses In Uk>Top 10 Special Occasion Dresses In Greater Manchester
City Channel:London, Greater Manchester, Birmingham, Liverpool, Cardiff, Glasgow, Cambridge, OxfordView All Cities
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Greater Manchester is a metropolitan county in North West England, with a population of 2.8 million. It encompasses one of the largest metropolitan areas in the United Kingdom and comprises ten metropolitan boroughs: Bolton, Bury, Oldham, Rochdale, Stockport, Tameside, Trafford, Wigan, and the cities of Manchester and Salford. Greater Manchester was created on 1 April 1974 as a result of the Local Government Act 1972; and designated a City Region on 1 April 2011.Greater Manchester spans 493 square miles, which roughly covers the territory of the Greater Manchester Built-up Area, the second most populous urban area in the UK. It is landlocked and borders Cheshire, Derbyshire, West Yorkshire, Lancashire and Merseyside . There is a mix of high-density urban areas, suburbs, semi-rural and rural locations in Greater Manchester, but land use is mostly urban — the product of concentric urbanisation and industrialisation which occurred mostly during the 19th century when the region flourished as the global centre of the cotton industry.
It has a focused central business district, formed by Manchester city centre and the adjoining parts of Salford and Trafford, but Greater Manchester is also a polycentric county with ten metropolitan districts, each of which has at least one major town centre and outlying suburbs.For the 12 years following 1974 the county had a two-tier system of local government; district councils shared power with the Greater Manchester County Council. The county council was abolished in 1986, and so its districts effectively became unitary authority areas. However, the metropolitan county has continued to exist in law and as a geographic frame of reference, and as a ceremonial county, has a Lord Lieutenant and a High Sheriff. Several county-wide services were co-ordinated through the Association of Greater Manchester Authorities until April 2011, when the Greater Manchester Combined Authority was established as the strategic county-wide authority for Greater Manchester, taking on functions and responsibilities for economic development, regeneration and transport. A further devolution of powers to Greater Manchester took place upon the election Andy Burnham as the inaugural Mayor of Greater Manchester on 4 May 2017Before the creation of the metropolitan county, the name SELNEC was used for the area, from the initials of "South East Lancashire North East Cheshire". Greater Manchester is an amalgamation of 70 former local government districts from the former administrative counties of Lancashire, Cheshire, the West Riding of Yorkshire and eight independent county boroughs. Since deindustrialisation in the mid-20th century, Greater Manchester has become known as an exporter of media and digital content, for its guitar and dance music and football clubs.
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text:
Flashbulb Games
Can Video Games Inspire the Next-Gen of Engineers?
Like racing? Love Sandbox games and designing new vehicles? Then you will love Trailmakers.
By Christopher McFadden
Trailmakers
Not all video games are about blowing stuff up! While such games can be fun, they don't necessarily teach you anything.
That is where games like Trailmakers come into play. By requiring players to design and build their own vehicles, it allows them not only to have a great time but also to learn some very important engineering principles. You also get to blow stuff up too...
RELATED: BATTERY-FREE GAME BOY RUNS FOREVER ON KINETIC ENERGY
Can video games inspire future engineers?
Video games have come a long way over the last few decades. They have become more technically challenging to play, the graphics are almost life-like, and, more importantly, a lot more people are playing them than ever before.
No longer are they the preserve of the old stereotype of gamers. Especially since the generation who grew up with Super Mario Brothers and Sonic the Hedgehog are now adults and parents.
But, some games are becoming more than just a way to spend the hours in the evenings. Sandbox games, purpose-built educational titles, and other creator-type games are providing a means for players to design and create their own things.
Whether that be vehicles, cities, or new alien life forms, video games are garnering love and aptitude for creativity in players.
Not only that but playing video games has been shown to provide some very interesting positive effects on players. Of course, there are some downsides, too, if players become addicted to gaming.
Video games are also increasingly being used as training tools for many professions, including engineering.
They may even be an excellent way to inspire the next generation of engineers. Games like Minecraft and Kerbal Space Program are excellent introductions to some complex engineering practices. They also make learning fun.
That's where games like Trailmakers might just be the perfect game for inspiring little engineers to start designing and building machines while having a blast at the same time.
What is Trailmakers?
Trailmakers, now available on Steam, is a creative vehicle-building sandbox and an exploration racing game at the same time. Players must use their imagination and creativity to build vehicles and test them out in various situations.
Test out your own innovative ideas with games like Trailmakers. Source: Trailmakers
Trailmakers' description reads, "Build a car, a plane, a boat, or maybe a… carplaneboat? With Trailmaker's intuitive builder, it is as easy as snapping together real building blocks. Take your machines on exciting rally races, dangerous exploration missions, or build the craziest contraptions you can imagine in our huge sandbox."
Trailmakers is both single-player and multiplayer. Source: Trailmakers
With the game's intuitive builder function, players can design their own creations, and once happy with the design, they can take their machines on dangerous exploration missions or breakneck rally races.
With Trailmakers, there is no limit to what you can build. For this reason, it is a great place to test out crazy machines and experiment with the physics engine.
You can make good use of the tons of different blocks, hinges, thrusters, and interactive vehicle parts to your heart's content.
The only limit is your imagination with games like Trailmakers. Source: Trailmakers
The main features of the game are, according to the creators:
Using modular blocks, you can build intuitively with endless possibilities.
The survival game mode "Stranded in Space" offers an open-world experience where you have to escape the planet you were stranded in.
You can go on breakneck rally races with the vehicle you've made according to your liking.
Your creations will have no constraints thanks to the two sandbox maps that are full of crazy obstacles.
You can race your creation even on the global leaderboards.
Trailmakers has a growing community which means there are tons of premade vehicles waiting for you to test them.
Design your own in Trailmakers! Source: Trailmakers
There is always something to do in Trailmakers. You can join the Trailmakers Rally, take on challenges, play in the sandbox, or race your friends. The game even comes with its own Discord channel, so you can chat with the game's designers or other players.
What are the game modes in Trailmakers?
As previously mentioned, the game comes with various modes to test your assembly contraptions. They are as follows.
1. "Stranded in Space" mode
As the name suggests, this part of the game allows players to design and assemble their very own spacecraft. It is a survival campaign that will test your designs to destruction.
Players are crash-landed on an alien world, and can only escape by building their own spacecraft from scrap parts. All the parts needed are scattered around on the planet, and players need to use their own ingenuity and resourcefulness to find and assemble them.
However, you are not alone on the planet, so be careful!
2. "Trailmakers Rally Campaign" mode
For those with a "need for speed", the game's "Trailmakers Rally Campaign" is an absolute must-play.
Players must go through a series of races that require them to compete with all sorts of different vehicles from simple go-karts and off-roaders to race cars and airplanes, and in the end, combinations of them all.
Source: Trailmakers
Players start the campaign with just a few basic building blocks and a go-kart track. Players progress through the rally by earning bronze, silver, or gold medals.
New blocks are unlocked after each race, and these can be used immediately to modify your racing vehicle. With ingenuity, racing skills, and perseverance, you will be putting jet engines in your car in no time.
A podracer. Source: Trailmakers
This portion of the game consists of 17 races, and once a player beats the "Golden Time", they get to compete against ghost players from the worldwide leaderboard.
Sadly this mode is currently only available as a single-player campaign, though racing ghosts of other real-life players are similar to a multiplayer experience.
3. "Sandbox" mode
Probably the best part of the game, its "Sandbox" mode, is a place designed for experimentation. All building blocks are available in this game mode with the exception of accessory blocks.
Create crazy contraptions with Trailmakers. Source: Trailmakers
Trailmakers states, "Each block has unique features like shape, weight, and functionality. They can be broken off, refitted, and used to build something new. Individually the blocks are fairly simple, but combined, the possibilities are endless."
Players are taken to an island built from different types of terrain with interesting built-in challenges. This mode is both single and multiplayer, which ensures future engineers will be enjoying the challenges thrown at them together.
So, if you are looking for a game that will keep your budding little engineers entertained while learning something new, why not check out Trailmakers today? Learning has never been this fun!
Neuromorphic Computing: How the Brain-Inspired Technology Powers the Next-Generation of Artificial Intelligence
Susan Fourtané
Stanford Scientists Shed Light on Next-Gen Energy Material
How Next-Generation Database Infrastructure Makes Data Mashups Easier
2D Material Helps Next-Gen Computer Chip Store, Process Data Like Neurons
Brad Bergan


Handyman Painting Decorating Dartford DA | Quality Property Care Ltd.
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E – Knudsen, T.(4). DP – Oakland 1. LOB – Georgia Tech 4; Oakland 4. 2B – Wissmann, S.(1). HBP – Granger. SH – Piar. SB – Neff, T.(1); Judge.
Georgia Tech 1st – Coursey, F. struck out. Kumar, K. grounded out to p. Knudsen, T. struck out. 0 runs, 0 hits, 0 errors, 0 LOB.
Oakland 1st – Catanzaro popped up to ss. Utecht struck out looking. Granger grounded out to 3b. 0 runs, 0 hits, 0 errors, 0 LOB.
Georgia Tech 2nd – Wood, L. grounded out to ss. Donovan, K. struck out. Bartle, L. grounded out to 3b. 0 runs, 0 hits, 0 errors, 0 LOB.
Oakland 2nd – Burns walked. Seffens struck out. Evans grounded out to 2b; Burns advanced to second. Piar walked. Schulte struck out. 0 runs, 0 hits, 0 errors, 2 LOB.
Georgia Tech 3rd – Wissmann, S. doubled to center field. Hosier, A. struck out. Neff, T. singled to pitcher; Wissmann, S. advanced to third. Coursey, F. struck out. Kumar, K. grounded out to p. 0 runs, 2 hits, 0 errors, 2 LOB.
Oakland 3rd – Judge struck out looking. Catanzaro lined out to lf. Utecht grounded out to ss. 0 runs, 0 hits, 0 errors, 0 LOB.
Georgia Tech 4th – Knudsen, T. grounded out to 3b. Wood, L. grounded out to ss. Donovan, K. walked. Bartle, L. grounded out to 3b. 0 runs, 0 hits, 0 errors, 1 LOB.
Oakland 4th – Granger struck out looking. Burns flied out to cf. Seffens fouled out to 1b. 0 runs, 0 hits, 0 errors, 0 LOB.
Georgia Tech 5th – Wissmann, S. grounded out to 3b. Hosier, A. popped up to 2b. Neff, T. singled to second base. Neff, T. stole second. Coursey, F. grounded out to 3b. 0 runs, 1 hit, 0 errors, 1 LOB.
Oakland 5th – Evans singled to center field. McCoy pinch ran for Evans. Piar out at first 1b to 2b, SAC, bunt; McCoy advanced to second. Schulte struck out. Judge reached on a fielding error by ss; McCoy scored, unearned. Judge stole second. Catanzaro struck out. 1 run, 1 hit, 1 error, 1 LOB.
Georgia Tech 6th – Kumar, K. singled, bunt. Knudsen, T. reached on a fielder's choice; Kumar, K. out at second 3b to 2b. Wood, L. grounded into double play ss to 1b; Knudsen, T. out on the play. 0 runs, 1 hit, 0 errors, 0 LOB.
Oakland 6th – Utecht fouled out to lf. Granger hit by pitch. Hair pinch ran for Granger. Burns reached on a fielder's choice; Hair out at second 1b to ss. Seffens flied out to rf. 0 runs, 0 hits, 0 errors, 1 LOB.
Georgia Tech 7th – Granger to 1b for Hair. Donovan, K. grounded out to 3b. Bartle, L. grounded out to 3b. Wissmann, S. lined out to 3b. 0 runs, 0 hits, 0 errors, 0 LOB.


City Active Listings: There are a total of 301 properties actively on the market with the average price of $938,861 in Highland Park.
City Sold Listings: 36 properties closed last month in Highland Park with an average sales price of $526,511. The average time on market for these properties was 84 days.


Due to unforeseen sheduling conflicts, this event has been rescheduled to Saturday, May 4.
Experience wine like never before!
Find out why 4R insists on using Riedel glassware by diving into the history of the world-renowned glassmaking family and experience the impact that the shape and size of a wine glass has on your favorite wine. This tasting will be hosted by a professional Riedel representative.
Only 60 seats are available.