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Lionel Richie makes up for late start with hits-stuffed Summerfest show — and lots of pandering
Richie played his first Milwaukee concert in 19 years at Summerfest's American Family Insurance Amphitheater, with Michael McDonald as his opener.
Lionel Richie makes up for late start with hits-stuffed Summerfest show — and lots of pandering Richie played his first Milwaukee concert in 19 years at Summerfest's American Family Insurance Amphitheater, with Michael McDonald as his opener. Check out this story on jsonline.com: https://www.jsonline.com/story/entertainment/festivals/summerfest/2019/07/03/lionel-richie-makes-up-late-start-hits-stuffed-summerfest-show-milwaukee/1625188001/
Piet Levy, Milwaukee Journal Sentinel Published 12:29 a.m. CT July 3, 2019 | Updated 7:24 a.m. CT July 3, 2019
See photos of Lionel Richie, A Boogie Wit Da Hoodie, CHVRCHES and more a...
Lionel Richie headlines the American Family Insurance Amphitheater on July 2, 2019. Hannah Schroeder/Milwaukee Journal Sentinel
A Boogie With Da Hoodie basks in the crowd at the U.S. Cellular Connection Stage on July 2, 2019. Courtesy of Summerfest
Michael McDonald opens for Lionel Richie at the American Family Insurance Amphitheater on July 2, 2019. Hannah Schroeder / Milwaukee Journal Sentinel
Chaka Khan performs at Summerfest's BMO Harris Pavilion on July 2, 2019. Hannah Schroeder/Milwaukee Journal Sentinel
Chaka Khan performs at the BMO Harris Pavilion on July 2, 2019. Colin Boyle/Milwaukee Journal Sentinel
Chvrches performs at the Miller Lite Oasis on July 2, 2019. Colin Boyle/Milwaukee Journal Sentinel
Liz Phair performs at the Briggs & Stratton Big Backyard on July 2, 2019. Colin Boyle/Milwaukee Journal Sentinel
Young The Giant performs at the Uline Warehouse on July 2, 2019. Colin Boyle/Milwaukee Journal Sentinel
Milwaukee native Jacob Latimore performs at the U.S. Cellular Connection Stage on July 2, 2019. Rick Wood/Milwaukee Journal Sentinel
Milwaukee native Jacob Latimore performs at the U.S. Cellular Connection Stage on July 2, 2019. Rick Wood, Milwaukee Journal Sentinel
Big Gigantic performs at the Harley-Davidson Roadhouse on July 2, 2019. Colin Boyle/Milwaukee Journal Sentinel
Milwaukee's MT Twins perform at the U.S. Cellular Connection Stage on July 2, 2019. Rick Wood / Milwaukee Journal Sentinel
Patrick Park performs at Briggs & Stratton Big Backyard on July 2, 2019. Courtesy of Summerfest
Good Boy Daisy performs at the Uline Warehouse on July 2, 2019. Courtesy of Summerfest
Allman Betts Band performs at the Johnson Controls World Sound Stage on July 2, 2019. Courtesy of Summerfest
Coin performs at the Uline Warehouse on July 2, 2019. Courtesy of Summerfest
Fast Company performs at the BMO Harris Pavilion on July 2, 2019. Courtesy of Summerfest
Stupid storms.
Not only did they interrupt Summerfest Tuesday — and cause some sets to end early and start late last Thursday — they nearly cost us Lionel Richie.
Starting a half-hour late at the American Family Insurance Amphitheater Tuesday, Richie claimed that his flight from Chicago was grounded due to the weather. He also claimed he was told he couldn't make it to Milwaukee, but he insisted on it.
Safe money suggests that part was just hyperbole to make himself into the hero. He didn't need it Tuesday, nor did he need to pander to the audience quite so much.
Festival goers at Summerfest on Tuesday sing their favorite songs by Lionel Richie before his show that night. Colin Boyle, Milwaukee Journal Sentinel
Fans appeared on the big screen for practically every song of the 100-minute set — including Don Smiley, CEO of Summerfest parent company Milwaukee World Festival Inc., who was doing his best to emulate the title subject of the Commodores tune "Fancy Dancer."
Richie also feigned astonishment at the crowd singalong for "Hello" — letting the fans sing the chorus for him the first two go-rounds. He gave fans rounds of applause, said they were "out of control," and claimed he hadn't seen dancing this good since 1978.
The crowd ate all this up — and tongue-in-cheek between song bits, like when Richie took a sip of an apparently potent vodka with cranberry juice, or his advice for men hoping for a happy night with their dates ("Just put your arms around her and say, 'Isn't he amazing?'").
But Richie hardly coasted on goodwill. Despite a poor vocal mix for "Truly," where Richie's voice was totally drowned out by the bombastic band, his melodramatic expressions justified the fireworks display playing on the big screen behind him.
Lionel Richie headlines the American Family Insurance Amphitheater on July 2, 2019. (Photo: Hannah Schroeder/Milwaukee Journal Sentinel)
Along with his smoking sax player, Richie held out a money note for the Commodores "My Love," taking a comical look at his watch.
"That was pretty spectacular if I say so myself," Richie told him — and this time, it wasn't hyperbole.
Richie was dripping with sweat strutting the stage for "Dancing on the Ceiling," extending his mic to his bassist and guitarist, only to yank it away and hog the spotlight.
But the band really got to show off though during a blend of the Commodores' funky and frisky "Brick House" and "Fire," and Richie finally got to show off his vocal skills with a proper mix for the tender "Three Times a Lady" and "Just to Be Close to You."
Here are the highlights and lowlights of the first 5 days of the World's largest music festival. Bill Schulz, Milwaukee Journal Sentinel
Near the end of the night, he started chatting up the audience again, but this time, what he said was quite poignant.
He talked about his experience on stage, how he sometimes sees people laughing during sad songs and crying during happy songs. (A couple of women were actually crying heavily just in front of me.)
"I'm trying to figure out for the life of me what's going on, and I figured it out," he said. "It's memories. You're remembering family, friends, parties, schools, graduation, births, deaths, where you were, what you were doing and who you were doing it with. ... I do not take it for granted."
But fans weren't just cherishing old memories at Richie's show Tuesday. At his first Milwaukee concert in 19 years, they were clearly making new ones.
Michael McDonald opens for Lionel Richie at the American Family Insurance Amphitheater on July 2, 2019. (Photo: Hannah Schroeder / Milwaukee Journal Sentinel)
Richie didn't bother playing any songs he made after 1986. But during his 75-minute opening set, Michael McDonald included a newer tune, "Just Strong Enough," from 2017's "Wide Open," his first album of original material in 17 years. It's doubtful many in the amphitheater knew it, but McDonald and his six piece band won over the crowd with escalating musical force, the tension snapping with the sound of Mark Douthit's sharp sax squeals.
But like Richie's set, this was a hits-filled affair, from the Doobie Brothers' toe-tapping "Minute by Minute" to a Sunday service-inspired "Takin' It To The Streets," led by testifying vocalist Drea Rheneé. Other classics were covered too, including Marvin Gaye's "What's Going On," with McDonald encouraging the audience to sing along.
Thankfully no one obligated. Who'd want to distract from such a soulful singer?
Photos: Looking back on 50 years of Summerfest
A view of the Summerfest crowd in 1972, two years after it moved to a 15-acre site on the lakefront, where the festival is still held each year. Milwaukee Journal Sentinel
George Carlin is arrested by Milwaukee police at Summerfest on July 21, 1972, on obscenity charges after performing his "Seven Words You Can't Say on Television." It was a landmark moment for comedy, Carlin's career and the Milwaukee festival. Mark Goff
Among the various attractions held at Summerfest was a daily hang gliding show in 1974. Henry A. Koshollek / Milwaukee Journal Sentinel
The late, legendary jazz artist Ella Fitzgerald played Summerfest in 1975. Stephen C. Liljegren / Milwaukee Journal Sentinel
"The Father of Rock 'n' Roll," Chuck Berry, performs at Summerfest in 1977. Lynn Howell / Milwaukee Journal Sentinel
Phil Donahue (right) hosted his syndicated talk show from Summerfest for a few years in the '70s. His guest, pictured here during a 1977 taping, is the late legendary comedian Bob Hope, one of the first major Summerfest headliners in 1969. Lynn Howell / Milwaukee Journal Sentinel
Emmylou Harris sings on the Summerfest Main Stage in 1980. Benny Sieu / Milwaukee Journal Sentinel
Kenny Loggins sings at Summerfest in 1980. Journal Sentinel files
Late Milwaukee Mayor Henry Maier leads a singalong for the opening day of Summerfest in 1981. Maier had the original vision for Summerfest, which officially began in 1967, following a trip to Munich during Oktoberfest. William Meyer / Milwaukee Journal Sentinel
The Allman Brothers Band was arguably the biggest act that played the Summerfest Main Stage in 1981. Rick Wood / Milwaukee Journal Sentinel
The "Queen of Soul" Aretha Franklin was a main headliner at Summerfest '81. Jack Orton / Milwaukee Journal Sentinel
Crooner Tony Bennett sings on the Main Stage at Summerfest in 1981. John Terhune / Milwaukee Journal Sentinel
The late Al Jarreau, a seven-time Grammy winner, headlined Summerfest's Main Stage in his hometown of Milwaukee in 1982. His song "Girls Know How" is part of a funny scene in "The Lego Batman Movie." Mary Jones / Milwaukee Journal Sentinel
Milwaukee music scene veteran Paul Cebar performs on Summerfest's Folk Stage in 1982. Journal Staff Photo
Milwaukee native and Rock and Roll Hall of Famer Steve Miller played his hometown festival in 1982. Scott Sharpe / Milwaukee Journal Sentinel
The Commodores topped the bill on Summerfest's Main Stage in 1982. It was one of the funky soul band's last concerts with Lionel Richie (center). Rick Wood / Milwaukee Journal Sentinel
'80s heartthrob Rick Springfield rocks out at Summerfest in 1983. Michael Sears / Milwaukee Journal Sentinel
Guitar great Eric Clapton plays Summerfest's Main Stage in 1983. Layne Kennedy / Milwaukee Journal Sentinel
The crowd goes wild listening to the band Barry's Truckers at Summerfest in 1984. Karen Sherlock / Milwaukee Journal Sentinel
Belinda Carlisle performs with the Go-Gos at Summerfest in 1984. Gary Porter / Milwaukee Journal Sentinel
A view of the Summerfest grounds, facing south, on a packed day in 1985. Milwaukee Journal Sentinel files
A Summerfest fan rocks out on the grounds in the mid-1980s. Milwaukee Journal Sentinel files
"Weird Al" Yankovic playfully promotes a Summerfest hat and brat while playing the Rock Stage in 1984. Bill Alkofer / Milwaukee Journal Sentinel
A view of the Summerfest grounds, facing north, in 1985. Karen Sherlock / Milwaukee Journal Sentinel
The late Roy Orbison, a perennial favorite at Summerfest, performs on the Pabst Festival Stage in 1986. Douglas Smyth / Milwaukee Journal Sentinel
A photo of the Summerfest grounds in the mid-'80s features the site of the festival's old Miller Jazz Oasis stage. Milwaukee Journal Sentinel files
Dolly Parton performs for more than 20,000 people at the Marcus Amphitheater in 1987, the first year the amphitheater was open. Larry Mishkar / Milwaukee Journal Sentinel
Duran Duran was one of the first acts to headline the Marcus Amphitheater's inaugural Summerfest season in 1987. The Beach Boys, Paul Simon, Run-DMC, Jimmy Buffett and John Denver with the Milwaukee Symphony Orchestra also performed at the amphitheater that year. Marcia Rules / Milwaukee Journal Sentinel
Whitney Houston sings at a sold-out Marcus Amphitheater for Summerfest's closing night in 1987. Benny Sieu / Milwaukee Journal Sentinel
A storm breaks out behind the rides on the Summerfest grounds on June 25, 1988. Jack Orton / Milwaukee Journal Sentinel
John Cougar Mellencamp performs at Summerfest in 1988. Todd Endorf / Milwaukee Journal Sentinel
Summerfest Entertainment Director Bob Babisch poses for a photograph on the festival's last day in 1989. He's been in charge of the Big Gig's bookings since 1978. Terry Person / Milwaukee Journal Sentinel
Stevie Nicks (with John McVie on bass) performs with Fleetwood Mac in the Marcus Amphitheater in 1990. Michael Sears / Milwaukee Journal Sentinel
An aerial view of downtown Milwaukee and Henry Maier Festival Park, the Summerfest logo visible on the roof of the Marcus Amphitheater, in 2000. GARY PORTER / Milwaukee Journal Sentinel
Prince performs at the Marcus Amphitheater on June 28, 2001, his second to last concert in Milwaukee. Benny Sieu / Milwaukee Journal Sentinel
Summerfest hosted other events besides music during its 50 years, including a once annual bodybuilding competition. In this photo, Daniel Kloss of Menomonee Falls (left) and Zico Buhaissi of Milwaukee square off on June 29, 2002. David Joles / Milwaukee Journal Sentinel
Summerfest Director Bo Black rides the Summerfest Skyglider on July 6, 2003. Joining Summerfest as its executive director in 1983, Black was the public face of Summerfest and instrumental to its growth until she stepped down as president in 2003. Dale Guldan / Milwaukee Journal Sentinel
Tom Petty performs with the Heartbreakers at the Marcus Amphitheater on June 29, 2006. Petty has played Summerfest's biggest stage more than any other headliner. JEFFREY PHELPS / Milwaukee Journal Sentinel
Bon Jovi performs "Bad Name" at the Marcus Amphitheater on the opening night in 2009. RICK WOOD / Milwaukee Journal Sentinel
Stevie Wonder (left) and John Legend perform at the Marcus Amphitheater on June 28, 2009. Wonder, who seemed distraught during portions of the show, paid tribute to Michael Jackson, who had died three days earlier. RICK WOOD / Milwaukee Journal Sentinel
A baby-faced Justin Bieber makes his Milwaukee debut at the Marcus Amphitheater on June 27, 2010. Rick Wood / Milwaukee Journal Sentinel
Kanye West performed only a handful of shows in the summer of 2011, following the release of his widely acclaimed album, "My Beautiful Dark Twisted Fantasy." Summerfest was one of them. Jeff Sainlar / Milwaukee Journal Sentinel
Katy Perry's first headlining tour in arenas and amphitheaters stopped at Summerfest's Marcus Amphitheater on July 7, 2011. Rick Wood / Milwaukee Journal Sentinel
Joey Bartman of the Milwaukee Bucks Rimrockers flys high into the air as he slams a dunk shot during a Summerfest exhibition in 2013. Rick Wood / Milwaukee Journal Sentinel
Riders on the Summerfest Skyglider get a front-row seat for the annual fireworks display on July 1, 2014. Rick Wood / Milwaukee Journal Sentinel
Arguably Summerfest's greatest booking coup was the Rolling Stones in 2015. The Marcus Amphitheater was by far the smallest venue the Stones played during its 15-date "Zip Code" North American tour. Rick Wood / Milwaukee Journal Sentinel
One-time tabloid magnet Paris Hilton performs at the Harley-Davidson Roadhouse at Summerfest on June 28, 2015. Hilton's booking sparked some backlash, including a Change.org petition urging her removal from the lineup, but she performed for a packed crowd anyway. Katie Klann / Milwaukee Journal Sentinel
Paul McCartney headlines his first Summerfest at a sold-out Marcus Amphitheater July 8, 2016. Rick Wood / Milwaukee Journal Sentinel
Fireworks rain down in the distance during Summerfest on July 3, 2016. Calvin Mattheis / Milwaukee Journal Sentinel
The Waukesha-born Americana band BoDeans, featuring co-founder Kurt Neumann (center), performs at the BMO Harris Pavilion during the city's annual Independence Day fireworks display on July 3, 2016. Calvin Mattheis / Milwaukee Journal Sentinel
THE SET LIST
1. "Running with the Night"
2. "Easy"/"My Love"
3. "Penny Lover"
4. "Truly"
5. "You Are"
6. "Stuck On You"
7. "Dancing on the Ceiling"
8. "Three Times a Lady"
9. "Sail On"
10. "Fancy Dancer"
11. "Sweet Love"
12. "Lady (You Bring Me Up)"
13. "Just To Be Close To You"
14. "Endless Love"
15. "Brick House"/"Fire"
16. "Hello"
17. "Say You, Say Me"
18, "We Are The World"
19. "All Night Long (All Night)"
RELATED: Summerfest 2019: A Boogie wit da Hoodie, Chaka Khan and more of the best and worst from the side stages on Day 6
RELATED: From Lizzo to Lonely Island, here's the best and worst of Summerfest 2019 in Milwaukee so far
RELATED: Not sure what to see at Summerfest 2019? Plan your visit with our interactive schedule.
Contact Piet at (414) 223-5162 or plevy@journalsentinel.com. Follow him on Twitter at @pietlevy or Facebook at facebook.com/PietLevyMJS.
Piet also talks concerts, local music and more on "TAP'd In" with Jordan Lee. Hear it at 8 a.m. Thursdays on WYMS-FM (88.9), or wherever you get your podcasts.
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Gems from the archives 86
At 11 am on 11 November 1918, "the eleventh hour of the eleventh day of the eleventh month", a ceasefire was declared and negotiations were soon started to terminate the Great War or World War One A number of persons from St. Kitts, Nevis and Anguilla had enlisted and served in the various regiments.
At the outbreak of the First World War, activists like Marcus Garvey encouraged West Indians to volunteer arguing that loyalty to the Empire would earn them the right to be treated as equals. The need for soldiers quickly outweighed the reluctance of the Secretary of State to allow them to join the British Forces. In 1915 the British West Indies Regiment was formed. Thousands enlisted, 105 men enlisted in St. Kitts. The four hand-written pages record their names and the person to whom they wanted a separation allowance sent during their service. At this stage we do not know how many of them returned.
However Equality eluded them and when the various battalions of the BWIR were brought together in Taranto, Italy, conditions had degenerated so much that a mutiny took place. The mutiny was crushed but at a meeting of sixty Non-Commissioned Officers an organization called the Caribbean League was formed to work towards black rights and self-determination in the West Indies.
The return of these men to the Caribbean, helped fuel the resentment being felt in the islands and increased demands for self-government. Albert St. Clair Podd was a founding member of the Union (Universal Benevolent Association) in St. Kitts. It came into existence just 6 days before his enlistment. His war time experiences, however, took a toll on his health. On his return he spoke at the Mutual Improvement Society of the injustices that he and his comrades endured. These links tell more of the story of the BWIR. https://www.iwm.org.uk/history/the-story-of-the-british-west-indies-regiment-in-the-first-world-war https://libcom.org/history/british-west-indies-regiment-mutiny-1918
To complete the picture of those who served in WW1, we are also including a list of service men who had joined other regiments and women who served as nurses. It notes a number of casualties. This was published in the St. Kitts-Nevis Daily Bulletin of the 21st January 1919.
You can also view this item on out website at
http://www.nationalarchives.gov.kn/1304
or on Instagram part 1 https://instagram.com/p/Bp9inB9Bzbp/
and part 2 https://instagram.com/p/Bp9ibmAhMku/
Tourism Month Kicks Off With A Strong Environmental Message
PUBLIC INVITED TO ATTEND REMEMBRANCE DAY SERVICE IN HONOUR OF THE COUNTRY'S FALLEN WAR VETERANS

redpajama_set_name: RedPajamaCommonCrawl


Country music is mourning the death of one of its most important voices this morning, with the passing of veteran Merle Haggard, aged 79.
Boasting a recording CV including more than 36 US country no.1s in a six decade-spanning career, Merle's gritty, no-nonsense outlook was forged by difficult formative years. His father died when Haggard was a child, and he would go on to serve time in San Quentin. Indeed, it was reportedly hearing Johnny Cash play at the prison that spurred Haggard on to pursue a career in music on his release in 1960.
Merle's breakthrough came with The Fugitive in 1966 and his most famous song is perhaps the typically forthright Okie from Muskogee, adopted as an anthem by conservative middle Americans on its release in 1969.
Haggard returned to prominence in 2015 with Django & Jimmie, a collaboration with fellow country legend Willie Nelson. Nelson led tributes last night, tweeting a picture of the pair laughing together, with the message "he was my brother, my friend. I will miss him."


Today marked the first annual Memphis NodeBots event.
Once everyone's robots were assembled and working, a soccer tournament was held and my cousin dominated with seven goals!
NodeBots day was held in the Fedex Institute of Technology on the same day as a codecrew hackathon so some of Memphis's best and brightest kids got to come by and cheer on during the soccer match. It was really exciting to see such a diverse group of tech enthusiasts and innovators in one place.


It's an insidious practice: upscale restaurants are increasingly serving small plates in lieu of properly portioned entrées. If the trend continues, a generation of diners will be permanently saddled with the palates of dilettantes and the appetites of Lilliputians. Fine dining in the traditional sense will go the way of the Princess rotary-dial phone.
I confess to being a dinosaur: When setting out for a night on the town, my destination is invariably a top-tier chophouse: dim lighting, white linen tablecloths, a full glittering bar, and food portions that guarantee I'll walk out groaning.
At this point, reading at my desk, I grew faint. The next thing I knew, my assistant was waving smelling salts under my nose and helping me off the floor.
The trend toward small-plate, prix fixe menus is incontrovertible. Such celebrated establishments as Benu, Chez Panisse, and The French Laundry all follow the despotic formula of "you'll get what the chef gives you, and that's that." But then, so does the state prison at San Quentin.
I have to ask myself, Has the restaurant world gone completely mad?
I was beginning to think yes—that is, until last weekend, when my travels took me to Santa Cruz, CA, for a wine-bottling weekend high in the mountains. On Sunday we had a late-afternoon plane to catch, and this gave my traveling companions and me the opportunity to grab an early lunch near the airport.
The restaurant we quite inadvertently stumbled upon in downtown San Jose was Original Joe's Italian Restaurant, a descendant of the Original Joe's founded in San Francisco in 1937.
Low lighting, crescent leather booths, white linen tablecloths under a cavernous ceiling—this was a real restaurant. Our server, Jose Luis, wore a tuxedo. He was perhaps 60. In his 29 years at Original Joe's, he had personally tasted every one of the menu's 117 items. He wasn't so fond of the sweetbreads or the liver, he said, but the spaghetti, lasagna, and minestrone soup were excellent.
"The prime rib is ready to be served," Jose Luis added. It was 11:30 in the morning.
At Original Joe's, the omelets are made with four eggs. Order bacon and eggs, and you get crispy stout steak fries and a truckload of bacon with your scrambled eggs. The Bloody Marys arrive nearly colorless at the top. And the sheer girth of the club sandwiches being portaged through the dining room made our eyes pop. Imagine what dinner must be like.
My advice to those of you in the iPhone generation who are putting down a credit card and waiting two to three months for a table at some small-plate, prix fixe nirvana of gustatory endeavor: Cancel your reservation. Use what you save to spring for an Uber. Go to Original Joe's in San Jose, where a gentlemanly server in a tuxedo will unobtrusively attend to your every need. You'll eat what you want and you won't go away hungry.
Chew on that with your minuscule plate of Buffalo octopus, chef Brian Malarkey. ##.
Eric Peterson is the author of The Dining Car, a contemporary novel about a former college football player who enlists as bartender and personal valet to a curmudgeonly food writer and social critic who travels the country by private railroad car.
Breaking News: Peterson's novel is a finalist in the Independent Book Publishers Assn's 29th annual Benjamin Franklin Awards 2017.


Finding relief from your chronic pain can feel like a never-ending struggle filled with debilitating suffering that makes going about your day nearly impossible. You're not alone — thousands of Canadians suffer from chronic pain caused by a wide range of disabilities and diseases. Medication might help but it's not a fix-all for your pain.
A floating session is a simple and natural way to find relief from your chronic pain by allowing your body to relax, rejuvenate and begin to heal itself.
The float pod is filled with water containing over a thousand pounds of dissolved epsom salts which create a level of buoyancy that provides your body a break from the effects of gravity. The epsom salts also contain essential minerals like magnesium which are absorbed through your skin and dramatically increase blood flow throughout your entire body. Your muscles receive greater amounts of oxygen, pressure on your joints is minimized, and your mind begins to enter a theta brainwave state — one step before deep sleep, an optimal state for healing.
The benefits to your brain are magnified as all external stimuli are completely removed. No light and no sound can enter the pod which creates an ideal environment for your brain to turn its focus inward and greater communication between the left and right hemisphere occurs. Endorphins are released naturally, the stress hormone cortisol is reduced and relief from stress, anxiety and depression comes flooding in.


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Police ordered to reveal payments to known informant
FLORIDA--Once a court has revealed the identify of a confidential informant, the police must disclose information about the amount of…
FLORIDA–Once a court has revealed the identify of a confidential informant, the police must disclose information about the amount of money they paid him, a unanimous state appeals court in Tampa ruled in mid-September.
However the appeals panel sent the case back to trial court ordering the judge to personally inspect records to ensure that information that might reveal the informant's connection to other, specific cases would be withheld.
The city of St. Petersburg in September 1997 refused to give an attorney from the public defender's office in Clearwater records showing payment to longtime police and sheriff's informant Leon McCullough. The city cited an exemption in the state open records law for information "revealing the identity" of a confidential source.
But attorney Stephen Romine, who had watched McCullough testify in a public courtroom against his client, said that his request concerning McCullough's compensation would not reveal anyone's identity. He filed a FOI request for the information in circuit court in Clearwater and the court in November 1997 ruled in his favor.
The city appealed, saying that if it gave out the information, anyone could find out if an individual was an informant or not simply by seeking compensation records.
However, Romine said the public is entitled to know something about the relationship between the city and McCullough, who claimed in a deposition to have worked as an informant in nearly 1800 cases since 1988, receiving personal maintenance as well as cash from the law enforcement agencies.
The appeals panel said that disclosure of payments to McCullough would not reveal his status as an informer because that had already been made public. (City of St. Petersburg v. Romine; Counsel: Stephen Romine, Clearwater, pro se)
Appeals court upholds ruling that allows police to withhold some reports on rapist
Police must release incident reports involving juveniles
Court sets guidelines for determining informant confidentiality
FBI to release records on secret informant Ernest Withers
Police reports not always exempt from disclosure, court rules


The penultimate regular-season home weekend didn't go as planned for the Shreveport Mudbugs, but head coach Karlis Zirnis is adamant two games won't define the stellar 2017-18 season and added a little perspective.
Last weekend, the Mudbugs (40-10-6, 86 points) needed just a single victory against Corpus Christi, a nemesis during Shreveport's brief time in the NAHL, on George's Pond at Hirsch Coliseum – a place they'd won 19 of their previous 20 games -- to clinch the South Division, but were swept.
Tuesday, Mudbugs captain Dominic Procopio said the team spent the prior two days off the ice, and had an opportunity to celebrate teammate Brendan VanSweden's birthday.
An up-tempo practice preceded Tuesday's media luncheon, and set the stage for another opportunity to clinch the division at The George. The defending NAHL champion Lone Star Brahmas come to town for a pair of games that close out the 2017-18 home schedule.
The Brahmas have won 10 straight games and have shut out Shreveport in their past three meetings – all on a smaller sheet of ice in North Richland Hills, Texas.
The Mudbugs need a single point (at least an overtime/shootout loss) to claim their first division title in two seasons of NAHL play, and first since the franchise did it as a member of the Central Hockey League 10 years ago.
Zirnis was happy with the "compete level" against IceRays last weekend, and is thrilled his team could soon be closer to full strength. Defenseman Jack Clement (missed four games) and forward Warren Natyshak (missed three games) could return to action this week, and so could goaltender Gustavs Grigals.
Grigals suffered a shoulder injury during a Feb. 24 brawl against Kenai River. He was expected to miss at least six weeks.
Defenseman Jonatan Asplund may need some more time to heal after injuring his shoulder Friday. Forward Kieran Durgan is out for the season.
The division crown offers home-ice advantage through the first two rounds of the postseason – something that could be important as the Mudbugs still have their ultimate goal – a North American Hockey League Robertson Cup – in focus.
"At the end of the day, it's been a really successful regular season," Procopio said. "You play 60 (regular-season games) to win nine (playoff games). At the end, you can look back at the team who finishes first in the South Division, but it doesn't mean anything if you bounce the first round. We have our expectations high, but we don't want to look too far ahead.


That's might be a bit of an idea of how to explain the purpose and the idea of a Hungarian designer named Tamás Jakus - while combining the figure of Kawasaki J-Concept with the latest Z1000.
Kawasaki J-Concept itself had horrendous global world of two wheels since it first appeared in the Tokyo Motor Show 2013. The figure is touted as 'alien' is indeed a very radical view yet futuristic. While the latest Z1000 born for the first time with a super radical face after the past few years has not changed massively.
But what happens when both futuristic and radical figure is 'making out' then the result is a look that is very unpredictable, really extreme. Tamás Jakus imagination arising and making very creative motorcycle concept called Kawasaki Z1000 J-Style.


text:
Bodies and Clothing
Kōrero: Clothes
In the late 19th century feminists argued that women should abandon corsets and long skirts in favour of more practical, comfortable clothing. In the 2000s informal dress was common, with everyone sporting jeans and T-shirts.
He kōrero nā Fiona McKergow
Te āhua nui: Evening dress, early 1900s
Children's clothes
Clothing and identity
Māori women dress reformers, 1906
Tailoring service, Kirkcaldie & Stains, early 1900s
Children with bare feet, early 20th century
School uniforms, 2005
Māori in traditional and European dress, 1864
19th-century women wore long dresses, corsets and hats. Fashion was based on styles from London and Paris. From the 1850s home sewing machines and paper dressmaking patterns were available. In the late 19th century feminists promoted practical clothes such as knickerbockers (baggy knee-length trousers) for women.
Clothes were lacy and feminine in the 1900s, then simpler and looser in the 1920s. New clothing was rationed during the Second World War.
From the 1950s trousers for women were more common. Miniskirts were fashionable in the 1960s, and in the 1970s women began wearing jeans and T-shirts.
Men's clothes have mostly been made from strong fabrics in limited colours – black, blue, brown, white and grey. Men's fashion has changed less over time than women's fashion.
19th-century men wore shirts, waistcoats, trousers and coats. Suits were worn through the 20th century, although farmers or labourers often had just one suit for special occasions. Jeans, based on working men's clothes, became popular with young men from the 1950s.
In the 19th century both boy and girl babies wore robes. Later in the century boys wore knickerbocker suits, while girls wore dresses. Hand-knitted garments became popular, and from the later 20th century stretchy knit fabrics were widely used for most children's clothes. New Zealand children have often gone barefoot.
New Zealand secondary schools generally had uniforms, while primary schools did not. From the early 20th century girls wore gym frocks. In the 1960s girls' uniforms became more varied. Boys often wore grey shirts with short trousers, sometimes with a tie. In the 2000s uniforms were more unisex. Some primary schools had adopted uniforms while some secondary schools no longer had them.
Some adults, such as nurses and members of the armed forces, also wore uniforms.
As Europeans settled in New Zealand, Māori began wearing European clothing. Some outfits combined Māori and European styles. In the 2000s traditional Māori cloaks were worn on official occasions such as royal tours.
Clothes can be a way of expressing identity or group membership. For instance, gay men and lesbians have sometimes dressed differently from heterosexuals. People with particular religious or political beliefs may also show this through clothing.
Whai muri: Whārangi 1. Women's clothes Whai muri
Fiona McKergow, 'Clothes', Te Ara - the Encyclopedia of New Zealand, http://www.TeAra.govt.nz/mi/clothes (accessed 29 January 2022)
He kōrero nā Fiona McKergow, i tāngia i te 5 Sep 2013
Te Tinana me ngā Kākahu
Kākahu Māori


text:
Ogniwo Sopot – polski klub rugby z siedzibą w Sopocie założony 23 czerwca 1966 przez Mieczysława Opiekę i Zbigniewa Kulenty jako sekcja rugby wielosekcyjnego MKS Ogniwo Sopot. Jeden z najbardziej utytułowanych klubów rugby w Polsce. Jedenastokrotny mistrz Polski i dziesięciokrotny zdobywca Pucharu Polski. Obecnie gra w Ekstralidze.

Historia
Początki sekcji rugby sięgają 1963, kiedy do zarządu MKS Ogniwo wpłynął wniosek o powołanie drużyny. Sopocki klub został przyjęty do Polskiego Związku Rugby dopiero 23 czerwca 1966. Data rejestracji w związku uważana jest za powstanie sekcji rugby Ogniwa. W 1967 drużyna rozegrała swój pierwszy ligowy sezon. Po dwóch latach występów sekcja została rozwiązana. W 1971 drużyna zostaje reaktywowana. Wraz z zatrudnieniem w 1976 Edwarda Hodury, rozpoczyna się złoty okres klubu. Juniorzy i kadeci zdobywają pod wodzą Hodury medale mistrzostw Polski. W 1983 seniorzy trenowani przez Hodurę awansowali do I ligi. Od 1 kwietnia 1984 do 4 czerwca 2011 Ogniwo występowało nieprzerwanie w ekstralidze. W 1987 seniorzy zdobywają pierwsze mistrzostwo oraz puchar kraju.

W 2011 po przegranych barażach o utrzymanie w ekstralidze z Juvenią Kraków drużyna Ogniwa spadła do I ligi. W 2013 ponownie awansowała do ekstraligi, w 2017, 2018, a następnie w 2022 sięgnęła po wicemistrzostwo Polski, a w 2019 i 2021 po mistrzostwo.

Sukcesy

Seniorzy
 Mistrzostwo Polski:  1987, 1989, 1990, 1991, 1992, 1993, 1997, 1999, 2003, 2019, 2021
 Wicemistrzostwo Polski:  1988, 1994, 1995, 1996, 1998, 2001, 2017, 2018, 2022
 Trzecie miejsce:  2002, 2016
 Puchar Polski:  1987, 1988, 1989, 1991, 1993, 1995, 1998, 1999, 2001, 2020

Juniorzy
 Mistrzostwo Polski:  1971, 1972, 1974, 1975, 1976, 1977, 1978, 1986, 1989, 1990, 1991, 1996, 2003, 2004, 2005, 2007, 2009

Rugby 7
 Mistrzostwo Polski:  1996, 1997
 Wicemistrzostwo Polski:  1998
 Trzecie miejsce:  2003

Przypisy

Linki zewnętrzne
 Oficjalna strona MKS Ogniwo Sopot

Polskie drużyny rugby union
Sport w Sopocie
Karlikowo (Sopot)

redpajama_set_name: RedPajamaWikipedia


Where is Europe on its way to 100% Renewable Energy?
How do you know that the world is changing? The following facts might give you an indication: Renewable energy broke another record last year, accounting for over 60% of net addition to the world's power capacity, providing more than 19% of the global final energy consumption (REN21 Renewables 2015 Global Status Report). Since 2000, renewable energy capacity has grown 120% (IRENA) and the number of countries with renewable energy targets and policies increased again in 2014: At least 164 countries have renewable energy targets, and an estimated 145 countries have renewable energy support policies in place. World leaders, including the G7 and Pope Francis call for a phase out of fossil fuels and the divestment movement is growing almost on a daily basis. While this is already great news, you see even stronger evidences of change when looking at the local level: Hundreds of local governments across the world have 100% renewable energy or electricity targets in place, with many municipalities already achieving such targets. The leaders of this local movement are mainly European cities and municipalities.
June 26, 2015 Comments Off on Where is Europe on its way to 100% Renewable Energy?
Six key recommendations on how to enable a local regenerative transition are highlighted in the new report Imagine A Regenerative City.


Thinking about starting Home Health Aide training in Sikeston, MO? Find both classroom and online CNA and HHA classes here. Search by zip code.
There has never been a greater time to begin Home Health Aide Training in Sikeston, MO. As the median age of the United States' population gets higher, the need is greater than ever for certified Home Health Aide professionals. As healthcare technology becomes increasingly more accessible and less expensive, many individuals elect to be cared for in the home instead of nursing facilities and hospitals. In many cases the care required encompasses monitoring vital signs and assisting with every day activities such as preparing food and housecleaning. Ultimately, obtaining your HHA Certification in Sikeston, MO can be a fulfilling and empowering process that might change your life, as well as the individuals you care for.
Why Pursue a Career as an HHA in Sikeston, MO?
In general a home health aide (HHA) provides caregiving assistance that make it possible for patients to remain in their home as opposed to being cared for in a health care facility. HHA's provide basic caregiving services including monitoring a patients' vital signs and medication schedule, preparing meals, personal grooming, light housekeeping tasks, and companionship. It can be a challenging job, and for that reason the turnover tends to be high. So why would you want to go after such a professional?
Below are a few reasons why this career might be ideal for you.
As baby boomers age, it is predicted that more and more seniors will choose to remain in their own homes as long as possible. This is increasing demand for caregivers to offer care in domestic settings, assisted living facilities, as well as adult day care programs. The U.S. Department of Labor's Bureau of Labor Statistics rates the job outlook for home health aides as "excellent." In fact, it's the second-fastest growing vocation in the U.S. (following registered nurses). Careerinfonet.org predicts job availibility for Home Health Aides will grow by 69% or over 700,000 more jobs dueing the ten year period 2010 to 2020.
Home health aides perform tasks which might be required on various schedules. This means you are often permitted the option for a flexible or non-traditional job schedule. For example, you might visit a patient in their home daily, weekly, or on some other schedule. You can also choose to work overnight shifts for clients who require over-night monitoring. Home health aides in Sikeston, MO can easily work part-time or full-time. This can be very helpful if you are searching for a job that will allow you to accommodate child care obligations, continuing education, or any other responsibilities.
Being a home health aide means you will have several employment paths to choose from based on your work preferences. HHAs are employed by home health care organizations, assisted living facilities, adult day care programs, nonprofit organizations, and private parties (families). You'll see a different degree of benefits, support, and work environment based on the kind of employer. Many caregivers opt to be independent and do private-duty work so they have more control over their schedule and patients.
For anyone who is contemplating a health care career, training to be a home health aide is an excellent entry point. This enables you to acquire practical experience in the field, and even to keep working, while you pursue becoming a CNA, licensed practical nurse, RN, or any other occupation in the health care industry.
Typically you will find enough demand in the local community that home health aides will not need to travel far for work, unless they so desire. If you wish to be able to easily relocate, the demand is such that you shouldn't have any trouble doing so. Keep in mind, training and certification requirements will differ from state to state so you might want to check that you have the necessary education to satisfy local requirements.
Lastly, and most significantly, this career will allow you to do work which could make a difference in the lives of the patients you serve. If you happen to be a caring person that values the chance to help people live their lives with dignity, working as a home health aide in Sikeston, MO is likely the ideal career for you!
Thanks for sharing such a great site. I was able to get some info about the various schools in my area and found one that works for me. Now I'm ready to begin my classes and can't wait to become a Certified Home Health Aide.


text:
Johannes Groß oder Johannes Gross ist der Name folgender Personen:

* Johannes Groß (1564–1654), deutscher Theologe, siehe Johannes Major (Theologe)
 Johannes Groß (Politiker) (1879–1954), deutscher Politiker (Zentrum)
 Johannes Gross (1932–1999), deutscher Publizist, Aphoristiker und Journalist
 Johannes Heinrich Groß (1916–2008), deutscher Theologe, siehe Heinrich Groß (Theologe)

Siehe auch:
 Johann Groß
 Hans Groß


awaiting silver flats: I had my eye on these last week, and thank to stacking coupon codes and Old Navy rewards, I got them for a steal! If you use the code 'sale' and '25lucky' you can get them down to $53 instead of $110. Win. excited about a long weekend in st. louis: I'm headed home to spend Memorial Day with my family at my parents' country home, which means relaxation, no internet, and tons of free space for pup. Plus pretty scenery and no awkward social encounters while taking blog photos. wearing men's graphic tees: Why doesn't anyone make NASA or Captain America lady's tees? Until they do, I'll just be wearing my perfectly slouchy tees borrowed from the boys, with sneakers and boyfriend jeans on the weekend, or heels and a blazer for the office. using pacifica blood orange hand cream: This hand cream smells deliciously summery, and doesn't leave any of that greasy residue many other hand creams do. Let's be honest though, I bought it for the packaging :) craving avocado hummus: Imagine guacamole meets hummus, only tastier. It's delicious on pita chips, tostadas, or dolloped on a taco salad. I've made it a couple times, and the necessary ingredients are on my grocery list because I think of it longingly every time I'm hungry. Yes, it's that delicious. wanting to try origins active charcoal mask: I've read that this is kind of like the poor man's GlamGlow mud mask, so I'm curious about the results. Have any of you savvy readers tried the Origins mask? Or how about the GlamGlow mask? Happy Wednesday!


Please note this article was first published in 22 Jan 2010. Its content may now be out of date. We recommend taking a look at more recent website building blog posts or check out our comprehensive support pages. If you are looking for information on our 14 day free website builder trial we have a large number of webpages that guide you throug the process.
In our last Blog we looked at the marketing benefits of offering Gift Vouchers. In this tutorial, we'll look at how to issue money off vouchers and savings. Everyone loves a saving or a bargain and these days, online shoppers have even come to expect it when shopping online. Gift certificates and discount vouchers are a great way to improve and encourage customer loyalty and in turn this can increase repeat and ongoing business and sales. As a website builder you can up your game when it comes to your competitors by offering sales and money off vouchers to both new and existing customers.
Your DotGO shopping basket works in partnership with an award winning ecommerce system called Mals Ecommerce. They've been working very hard on developments to their system in recent months and one of their recently new and improved features is an incredibly simple voucher system. You can now offer Money off Vouchers, Gift Vouchers and Discount Coupons to your customers in a matter of minutes and best of all… this facility will cost you NOTHING! That's right, there is no cost to use the voucher system, the only cost to you is the discount your are providing your customers. Well, it only seems fair that you should get a bargain too once in a while!!
Whatever you use your vouchers for, make sure they generate the maximum number of sales possible and also that they encourage loads of new and future business for you.
If you already have an active shopping basket, you'll also have a Mals Ecommerce account. Log into your Mals account using the login details you would have been provided with when you initially set your shopping basket up. Don't worry if you've forgotten your details, there's a handy system, which can send them to you within seconds. Just go to www.mals-e.com and click the Forgotten Your Details link.
Once you've logged in, click on "Cart Setup" > "Discounts" > "Discount Vouchers".
You'll now see the new "Add a New Voucher" panel, which you can see here.
The first option deals with the Voucher Code. This is the code provided to the customer, which they enter at the checkout stage. This code works with the system and amends their final checkout total to include their discount. You can choose to create one yourself or let the system create one for you. You may have certain product codes or unique reference numbers associated with existing discounts and sales and so creating your own code here will work nicely with any existing discount activities you may have. Alternatively, let the system create one for you and just make a note of it to help you keep track of them all.
The types of voucher available include: A percentage of the order value, a fixed value (or amount) or Free Shipping (Postage). The value of discount coupons is added onto any other discount you may have in an order. Fixed value vouchers appear in the totals under the line Vouchers. Free shipping coupons simply reduce the shipping amount to zero. Choose which type of voucher you want to offer and then enter the amount of discount you are offering.
You can also set a minimum order value for which the vouchers can be used, which means that customers have to spend a certain amount of money in order to qualify for the discount.
You can add an expiry date to your voucher if you wish. Simply leave this option's boxes blank to make the voucher timeless. One last option is to set the voucher to have a onetime use only.
The cart does not keep a record of which coupons have already been used so you do need to check them carefully when you receive an order. However, by using the expiration date sensibly and by altering the range from time to time, you should be able keep the number of valid coupon codes quite small and easy to manage.
If you choose to use coupons then a text box appears in cart where they can enter their number. It doesn't specify what the voucher is for, it's assumed that customer already knows. This important, it's so that your customers who don't have discount coupons don't feel they are paying more than they need to. Instead, most will assume the box is for gift coupons only.
If you have any questions relating to this tutorial, please send us a message by clicking the comments link below.
Please remember, this article was first published 22/01/2010. The content may be out of date and you cannot post comments any more. Please check out our new blog.


text:
Goodwill Partners with the U.S. Census Bureau to Achieve Accurate Count in 2010
Rockville, MD. — Goodwill Industries International has announced that it will partner with the U.S. Census Bureau to achieve a complete and accurate count of the U.S. population in 2010. The partnership is part of a larger effort by the Census Bureau to increase participation in the 2010 Census.
As an organization that provides vital employment services to people in local communities across the country, Goodwill has a unique relationship to the people it serves. By participating in the Census Bureau partnership program, Goodwill continues to demonstrate its connection with and commitment to those communities.
"The count for the U.S. Census is critical to the people who seek our help through job training programs, employment placement services and overall support services," said Jim Gibbons, president and CEO of Goodwill Industries International. "Goodwill is proud to reach out to program participants, employees, donors, shoppers and volunteers to stress the importance of completing Census forms to better determine a complete count."
Every year, the federal government distributes more than $400 billion to state, local and tribal governments based on Census data.
"Through their unique roles in their individual communities, Goodwill agencies can help deliver the 2010 Census message to every corner of the nation," said Robert Groves, director, U.S. Census Bureau.
More than 140,000 organizations supported Census 2000 as partners, including community- and faith-based organizations, schools, state, local and tribal governments, media, businesses and others. Goodwill will be doing its part through PSAs, educational seminars and donation drives.
Census forms will be delivered or mailed to households in March 2010; households should complete and mail back their forms upon receipt. Census workers will visit households that do not return forms to take an in-person count. Information shared with the Census Bureau is completely confidential. By law, the Census Bureau cannot share an individual's personal information with anyone, including other federal agencies and law enforcement entities.
For more information about the 2010 Census, visit 2010census.gov.


text:
TARACHI GOLD CORP ANNOUNCES LORNE WARNER AS PRESIDENT AND CEO
Mr. Martin Bajic reports
Tarachi Gold Corp. has appointed Lorne Warner, professional geoscientist, as president, chief executive officer and a director. "I am thrilled to be leading Tarachi Gold Corp and working closely with the Board and all of our team to continue the progress made to date at the Tarachi project, and to be focused on achieving the Company's strategic goals to build Tarachi into a large gold resource in the shadow of the two producing mines in the region," stated CEO Lorne Warner.
About Lorne Warner
Lorne McLeod Warner graduated from the University of Alberta in 1986 with a BSc in Geology. Lorne is a registered professional geologist in B.C, NWT and Nunavut with over 30 years experience in mineral exploration, underground and open pit mining with Noranda Exploration and Placer Dome Inc. His career started in mineral exploration in British Columbia but has now worked throughout the Americas, Africa, Asia and Australia. As the vice president of several junior mining companies his team discovered the western extension of the Detour Lake gold deposit, now in production in Ontario. As well, the Falea North Zone - Uranium, Silver, Copper Deposit and the Fatou Main Gold Deposit in Mali. In conjunction with the appointment of Mr. Warner, Michael Konnert will be stepping down from the Board of Directors but will be staying with the company as an Advisor to the Board. Leighton Bocking will remain as a Director of the Board. The team would like to thank Mr. Konnert and Mr. Bocking for their service to the Company. About the Tarachi Project Tarachi has an option to acquire 100% of a group of concessions in the Sierra Madre gold belt known as the Tarachi projects. The Project is approximately 220 kilometres ("km") by air east of the City of Hermosillo, and 300km south of the border between the United States of America and Mexico. The Tarachi projects include the El Jabali past producing gold mine, consisting of 70 hectares located in east Sonora in the Mulatos gold belt. The property is located only six km west from Alamos Gold Inc.'s "Mulatos" gold-and silver-producing heap-leach mine.
Lorne Warner, P.Geo, a consultant of the company is a qualified person as defined by National Instrument 43-101, has reviewed and approved the scientific and technical disclosure in this news release.
We seek Safe Harbor.


text:
Q: C++ std::getline error I'm new to C++, could someone please explain to me why I received the below errors when I do use "std::getline"?  Here's the code:
#include <iostream>
#include <string>

int main() {

  string name;  //receive an error here

  std::cout << "Enter your entire name (first and last)." << endl;
  std::getline(std::cin, name);

  std::cout << "Your full name is " << name << endl;

  return 0;
}

ERRORS:
te.cc: In function `int main()':
te.cc:7: error: `string' was not declared in this scope
te.cc:7: error: expected `;' before "name"
te.cc:11: error: `endl' was not declared in this scope
te.cc:12: error: `name' was not declared in this scope

However, the program would run and compile when I used "getline" with "using namespace std;" instead of std::getline.
#include <iostream>
#include <string>

using namespace std;

int main() {

  string name;

  cout << "Enter your entire name (first and last)." << endl;
  getline(cin, name);

  cout << "Your full name is " << name << endl;
  return 0;
}

Thank you!

A: The errors are not from std::getline.  The error is you need to use std::string unless you use the using namespace std.  Also would need std::endl.

A: You need to use std:: on all the identifiers from that namespace. In this case, std::string and std::endl.  You can get away without it on getline(), since Koenig lookup takes care of that for you.

A: #include <iostream>
#include <string>

int main()
{
    std::string name;  // note the std::

    std::cout << "Enter your entire name (first and last)." << std::endl; // same here
    std::getline(std::cin, name);

    std::cout << "Your full name is " << name << std::endl; // and again

    return 0;
}

You just needed to state the namespace for various elements that are in the std namespace (alternatively, you can remove all the std::s and place a using namespace std; line after your includes.)

A: Try this:
 #include <iostream>
#include <string>

int main()
{
     std::string name;

      std::cout << "Enter your entire name (first and last)." <<
      std::endl;

      while(getline(std::cin, name))
      {
            std::cout <<"Your name is:"<< name << '\n';
     }

  return 0;
}

redpajama_set_name: RedPajamaStackExchange


text:
Celebrity Watch Spotlight - Kevin Hart
This week in the Everest Celebrity Spotlight, we take a look at America's favorite funnyman - Kevin Hart. Hart's style is effortless, and his taste in watches definitely proves this. From Audemars Piguet to Richard Mille, the comedic genius has something for every occasion - whether he be on stage performing, at an awards show, or at home with the family.
In a 2015 interview withHaute Time,Kevin stated that his collection started with a classic standard - the Rolex Submariner. He has alsosaid that the collection he has grown to today is full of"the bonuses that come with life after hard work." This shows, as his next watch purchase after his initial Sub - one that he still wears to this day - was a Stainless Steel Daytona. He has since expanded upon this and has been seen wearing a50th Anniversary Rolex Cosmograph Daytona in Platinum with a blue dial, theEverose Daytona, a yellow goldPaul Newman, plus some classic models such as the stainless steel white dial, and yellow gold black dial.
On the AP front, Hart has a few different Royal Oaks to choose from. With a standard Stainless Steel, an enviable Rose Gold, and some more coveted ones like the QE II CUP 2016 Limited Edition, the Platinum Tourbillion Chronograph, and the Tourbillion Concept GMT, his collection is anything but small.
When it comes to Richard Mille, Kevin Hart knows what's up - he has been seen wearing such beauties as the Richard Mille RM 11–01 "Roberto Mancini", a white Richard Mille RM035 Gold Toro, and a Limited Edition (of only 50) of Richard Mille's manually wound RM 035 Americas Rafael Nadal.
In his Patek Philippe collection, the two that stand out the most are his Celestials. Hart has both the 6102R and the 6104-001 Celestial models, and both are complete stunners. Both part of the Master Complication Collection - meaning they are handcrafted by one person from start to finish - the two watches ooze elegance, but definitely not simplicity. With a sky-chart of the Milky Way, phases and orbit of the Moon, the watches are a sight to see on their own - but these two are especially beautiful. The 6102R brags an 18k rose gold case, while the 6014-001 is encased in solid platinum with a factory-set bezel of baguette diamonds. The night sky would be jealous.
These watches may just be the tip of the iceberg for self-proclaimed watch-guy Kevin Hart's collection, so make sure to keep up with him!
Which watch in his collection is your favorite? Let us know below!


text:
\section{Introduction}

The standard map is an important object in studies in nonlinear
dynamics, mainly because it is often used to describe the local
behavior of other more complicated symplectic
maps~\cite{C78,C79,LL92}. What is more, it serves as an important
independent mechanical and physical paradigm~\cite{C96,M92}.
General properties of the standard map, often in interrelation
with those of the separatrix map, Fermi map and other fundamental
maps, were considered and studied in detail
in~\cite{C78}--\cite{VC98}, and many other works.

The standard map is given by the equations

\begin{eqnarray}
     y_{i+1} &=& y_i + \frac{K}{2 \pi} \sin (2 \pi x_i) \ \ \ (\mbox{mod } 1), \nonumber \\
     x_{i+1} &=& x_i + y_{i+1} \ \ \ (\mbox{mod } 1),
\label{stm}
\end{eqnarray}

\noindent where $K$ is the so-called stochasticity
parameter~\cite{C78,C79}.

In Ref.~\cite{S04c} we studied three major characteristics of the
chaotic dynamics of the standard map, namely, the measure $\mu$ of
the main connected chaotic domain (MCCD), the maximum Lyapunov
exponent $L$ of the motion in this domain, and the dynamical
entropy $h = \mu L$, as functions of the stochasticity parameter
$K$. The perturbations of the domain due to the birth and
disintegration of islands of stability, upon variations of $K$,
were considered in particular. By means of extensive numerical
experiments, we showed that these perturbations are isentropic, at
least approximately: the dynamical entropy follows the smooth
dependence $h(K) = \ln {K \over 2} + {1 \over K^2}$, and does not
fluctuate about it with changing the stochasticity parameter,
while local jumps in $\mu$ and $L$ due to the birth and
disintegration of regular islands are significant.

On the other hand, recently Baldovin~\cite{B04} and Baldovin et
al.~\cite{BBT04} introduced the notion of the ``dynamical
temperature'' for the standard map, defining it as the variance of
the momentum:

\begin{equation}
T \equiv \langle (y - \langle y \rangle )^2 \rangle - \frac{1}{12}
= \langle y^2 \rangle - \langle y \rangle^2 - \frac{1}{12},
\label{TB}
\end{equation}

\noindent where the angle brackets signify ensemble average; the
constant addend is the normalizing shift, introduced for
convenience. This choice of normalization gives $T=0$ for the case
of the uniform ensemble~\cite{B04,BBT04}. Henceforth we use
different normalization:

\begin{equation}
T \equiv 12 \langle (y - \langle y \rangle )^2 \rangle = 12
(\langle y^2 \rangle - \langle y \rangle^2).
\label{T}
\end{equation}

\noindent This gives $T=1$ for the case of the uniform ensemble.
This normalization is used in calculating $T$ in what follows. In
practice, the measurement of $T$ is performed by averaging over an
iterated trajectory in the chaotic domain, i.e., we assume that
the ensemble average is equal to the time average. This is
justified in the considered situation, when the regular islands
are small and the motion is almost completely ergodic on the phase
plane. The relation between ensemble and time averages for
low-dimensional symplectic maps in the opposite case of extended
borders between chaotic and regular components of the phase space
were considered and analyzed in Ref.~\cite{B04}.

In this paper, we investigate the behavior of two state variables
of the MCCD of the phase space of the standard map: namely, the
volume $\mu$ and the dynamical temperature $T$, both as functions
of the stochasticity parameter $K$. At moderate values of $K$ (at
approximately $K < 4$), the non-monotonic (spike) variations in
$\mu(K)$ and $T(K)$ are conditioned by the process of absorption
of minor chaotic domains by the MCCD, while $K$ increases; at
larger values of $K$ (at approximately $K > 4$), they are
conditioned by the process of birth and disintegration of
stability islands. In other words, the perturbations of the
chaotic domain at high values of $K$ are due to the birth and
disintegration of islands of stability, upon small variations of
$K$. By means of extensive numerical experiments, we show that the
variations of $\mu$ and $T$ due to this process obey simple
analytical relations.

\section{Numerical experiments}

The traditional ``one trajectory method''
(OTM)~\cite{C78,C79,SM03,S04c} has been used for calculation of
$\mu$. This method consists in computing the number of cells
explored by a single trajectory on a grid exposed on the phase
plane. A strict but computationally much more expensive approach
for measuring $\mu$ consists in calculating the values of the
coarse-grained area of the chaotic component for a set of various
resolutions of the grid, in order to find the asymptotic value of
$\mu$ at the infinitely fine resolution (see~\cite{UF85}). In some
cases the ``LCE segregation method''
(LCESM)~\cite{C78,C79,SM03,S04c} has been employed for
verification of the obtained values of $\mu$. In this method, a
numeric criterion is used for separation of the regular and
chaotic trajectories. The criterion is provided by an analysis of
the differential distribution of the values of the finite-time
Lyapunov characteristic exponents (LCEs) computed on a set of
trajectories with the starting values randomly generated on the
phase plane or specified on a regular grid on the phase plane. In
the distribution, the peak corresponding to the regular
trajectories is movable: if one increases the LCE computation
time, the peak moves to the left on the abscissa axis, because the
computed LCEs for the regular trajectories tend to zero; while all
the peaks corresponding to the chaotic domains stay immovable, on
condition that the computation time is long enough. By increasing
the computation time one can make the movable and immovable peaks
completely distinct, and in this way determine the ``finite-time
LCE'' value separating the regular and chaotic trajectories for
the given computation time. The OTM and LCESM were both proposed
and used by Chirikov~\cite{C78,C79} in computations of $\mu$ for
the standard map. Analogous methods were used in Ref.~\cite{SM03}
in computations of the chaotic domain measure in the
H\'enon--Heiles problem, and in Ref.~\cite{S04c} for computations
of $\mu$ for the standard map. A detailed description of the
currently used versions of the methods is given in
Ref.~\cite{S04c}.

In Figs.~1--4, we present the obtained numerical data on the
measure $\mu$ and the dynamical temperature $T$ of the MCCD, and
their interrelations. Fig.~1 shows $\mu(K)$ and $T(K)$ for a
perturbation of the MCCD due to the birth and disintegration of
the regular islands corresponding to a 2-periodic solution (at $K
\in (11.9, 12.6)$) and to an accelerator mode (at $K \in (12.6,
13.3)$). An accelerator mode represents a 1-periodic solution on
the torus $x, y \in [0, 1] \times [0, 1]$. Theoretical ranges in
$K$ for the existence of both types of solutions are given
in~\cite{C79}; the narrow ``windows'' of their existence follow
with the period of $2 \pi$ in $K$, and with increasing $K$ they
become more and more narrow. In Fig.~2, the same plots are
constructed for a perturbation conditioned by the birth and decay
of the islands due to a 4-periodic solution at $K \approx 9.21
\div 9.45$.

The OTM has been used for calculating $\mu$; the grid is $5000
\times 5000$ pixels on the square $x, y \in [0, 1] \times [0, 1]$.
The map has been iterated $n_{it} = 10^9$ times at each value of
$K$. The step in $K$ is equal to $0.005$ (Fig.~1) and $0.001$
(Fig.~2). Each value of $T$ has been computed simultaneously with
the value of $\mu$ for the same trajectory.

No error bars are shown in the Figs.~1 and 2, since the typical
errors appear to be rather low. One can estimate them in the
following way. Consider first the calculation of $\mu$. The main
uncertainty in the measured $\mu$ value, at sufficiently long
iteration times $n_{it}$, is conditioned by the resolution of the
grid imposed on the phase plane. We designate the number of pixels
at each side of the square $x, y \in [0, 1] \times [0, 1]$ by $l$;
so, $l = 5000$. Consider the model case of a round islet (the
choice of geometries is not principal for our estimate by the
order of magnitude). The relative uncertainty $\varepsilon$ in the
measured area of the disk is given approximately by one half of
the ratio of the area of the chain of the pixels at the disk
border and the disk area $S$. It is straightforward to show that
$\varepsilon = l^{-1} (\pi / S)^{1/2}$. This is the relative error
by which the island area can be overestimated by the OTM. For the
accelerator modes the maximum area of one island scales as $0.19
K^{-2}$~\cite{C96}; so, one has $\varepsilon \approx 4 K l^{-1}$.
For the accelerator mode in Fig.~1 this formula gives $\varepsilon
\approx 0.010$. This is the relative uncertainty in the measure
$\mu_{reg}$ of the regular component of the phase space. Hence the
absolute uncertainty in $\mu$ (in the ordinate in Fig.~1) is equal
to $2 \cdot 10^{-5}$; i.e., the error is smaller than the size of
the data point symbols in the Figure. Practically the same error
values are derived in the case of the plot in Fig.~2, i.e., in the
case of the 4-periodic solution.

In what concerns the errors in calculation of $T$, they seem to be
controlled only by the computation time $n_{it}$. If one decreases
this time, the ``noise'' appears in the plot: instead of the
smooth long-range (in comparison with the step in $K$) variations,
$T$ varies irregularly at each step in $K$; the amplitude of these
irregular one-step variations gives the typical error in the
estimation of $T$. From the fact of the absence of such variations
in Figs.~1 and 2, one concludes that the errors are typically
smaller than at least one-half of the distance in $\mu$ between
each two consecutive points on the plots, i.e., they are
insignificant in the given case of $n_{it} = 10^9$.

\section{Analytical relations between volume and dynamical
temperature}

The local minima in $\mu(K)$ seen in Figs.~1 and 2 clearly
correspond to local extrema in $T(K)$. The observed amplitudes of
the volume and temperature variations are apparently
commensurable, namely, their ratios represent some integer or
half-integer numbers. This suggests the existence of the power law
relations with rational exponents. We verify this hypothesis by
constructing the ``$\mu$--$T$'' graphs in Figs.~3 and 4. All the
points present in Figs.~1 and 2 are depicted in Figs.~3 and 4; in
the latter Figures, each pair of neighbors in $K$ are connected by
straight segments.

For all $K > 5$ the islands are small, i.e., $\mu$ is close to 1;
this is discussed in detail at the end of this Section. In this
context, it clearly follows from Figs.~3 and 4 that the relation

\begin{equation}
T = 1 - \gamma (1 - \mu)
\label{Tmu}
\end{equation}

\noindent takes place with three different values of the $\gamma$
constant. Namely, $\gamma = -1$ in the case of the 2-periodic
solution, $\gamma = 2$ for the accelerator mode, and $\gamma =
1/2$ for the 4-periodic solution.

Among 320 data points present in Fig.~3 there are 10 (i.e.,
$\approx 3$\%) that notably (by more than $0.0005$) deviate from
the dotted lines given by Eq.~(\ref{Tmu}) with $\gamma = -1$ and
$2$; among 350 data points in Fig.~4 there are 8 (i.e., $\approx
2$\%) that notably (by more than $0.0002$) deviate from the dotted
line given by Eq.~(\ref{Tmu}) with $\gamma = 1/2$. In other words,
the percentage of notable deviations is rather low. The deviating
points apparently correspond to those values of $K$ at which
secondary resonance chains separate from the outer borders of the
islands; these phenomena manifest themselves in the secondary
peaks in the curves $\mu(K)$ and $T(K)$. In such situations the
measuring of both $\mu$ and $T$ are subject to additional
uncertainties: the thin chaotic layers between the islands and the
surrounding resonance chains can be unresolved in the adopted grid
of pixels, and, besides, the enhanced sporadic sticking of the
chaotic trajectories to the islands may lead to increasing the
contribution of the ``temperature on the islands'' (this notion is
considered below) in the total measured temperature value.

Apart from these casual deviations, the sticking phenomenon does
not influence the temperature measurements. (This is contrary to
the case of the diffusion coefficient, which, as it is well known,
diverges in the presence of the accelerator modes,
see~\cite{C79,C96}.) If a trajectory constantly sticks to an
accelerator mode island, the temperature tends to the
``temperature on the island'' value, which is finite, because the
temperature~(\ref{TB}) and (\ref{T}) is defined in the factored
phase space: $y$ is taken modulo 1.

If one puts Eq.~(\ref{Tmu}) in the form $\frac{\Delta T}{T} =
\gamma \frac{\Delta \mu}{\mu}$ and integrates, one has

\begin{equation}
T = \mu^\gamma.
\label{plgamma}
\end{equation}

\noindent Eqs.~(\ref{Tmu}) and (\ref{plgamma}) are practically
equivalent for any application. At $K=9.24$, the MCCD area $\mu
\approx 0.995$; and the values of $T$ given by Eqs.~(\ref{Tmu})
and (\ref{plgamma}) at this value of $\mu$ differ by only $2.5
\cdot 10^{-5}$. For smaller islands, emerging at greater values of
$K$, the difference is smaller.

We have considered the behavior of the standard map at two
definite intervals of $K$. Now let us look at the problem in a
global perspective. In Fig.~5, the dependences $\mu(K)$ and $T(K)$
are presented in a broad range: $K \in [4, 30]$. The values of
$\mu(K)$ and $T(K)$ are calculated as previously, except that a
lower grid resolution ($2000 \times 2000$ pixels) and shorter
trajectories ($n_{it} = 10^8$) are used. The step in $K$ is equal
to $0.01$. The observed $\mu(K)$ dependence (Fig.~5) at large
values of $K$, i.e., at $K$ approximately greater than $6$,
represents the basic line $\mu = 1$ interrupted by periodic
sequences of sharp narrow minima whose depth diminishes with $K$.
The most prominent of these sequences correspond to the 2-periodic
solutions and accelerator modes (at $K_m \approx 2 \pi m$; $m=1,
2, \ldots$) and the 4-periodic solutions (at $K_m \approx 2 \pi
\left(m + \frac{1}{2} \right)$; $m=1, 2, \ldots$). The less
pronounced sequences of minima correspond to periodic solutions of
higher order. The observed minimum values of $\mu$ for these three
basic cases of periodic solutions agree with the semi-analytical
scaling $\mu_{reg} = 0.38 K^{-2}$ derived by Chirikov~\cite{C96}
for the maximum area of the accelerator mode islands. The
difference is within $(1 \div 2) \cdot 10^{-4}$. This agreement
verifies the good accuracy of our measurements of $\mu$. Note that
recently Giorgilli and Lazutkin~\cite{GL00} rigorously derived the
inversely quadratic law of decay with $K$ of the area of the main
regular islands, i.e., the islands emerging at $K \approx \pi n$
($n=2, 3, \ldots$).

The variations with $K$ in the standard map behavior due to the
2-periodic solutions and accelerator modes repeat themselves at
$m=2, 3, \dots$, only the amplitude of the variations diminish.
The same is true for the 4-periodic solutions. So, it is natural
to expect that the laws~(\ref{Tmu}) and (\ref{plgamma}) are
universal for all $m$. We have performed recomputation of our
plots taking $K \in [18.4, 19.3]$ (a 2-periodic solution and an
accelerator mode, $m=3$) and $K \in [15.58, 15.67]$ (a 4-periodic
solution, $m=2$). As expected, the values of $\gamma$ have been
found to reproduce the cases analyzed above.

\section{Theoretical explanation}

Finally, we consider a tentative explanation for the observed
relations~(\ref{Tmu}) and (\ref{plgamma}). In Ref.~\cite{S04c}, we
showed that the dynamical entropy  $h = \mu L$, where $L$ is the
maximum Lyapunov exponent of the motion in the MCCD, follows the
smooth dependence $h(K) = \ln {K \over 2} + {1 \over K^2}$, and
does not fluctuate about it with changing $K$, while local jumps
in $\mu$ and $L$ due to the birth and disintegration of regular
islands are significant. In other words, the $h(K)$ function
normalized by the ``long-term'' trend $\ln {K \over 2} + {1 \over
K^2}$ is constant and thus represents an invariant with respect to
$K$. Could a similar invariant be found in the case of the
dynamical temperature? Note that the dynamical entropy  $h = \mu
L$ is nothing but the maximum Lyapunov exponent averaged over the
whole phase space, because the maximum Lyapunov exponent is zero
on the islands. Since the dynamical temperature is, generally
speaking, non-zero on the islands, an analogous temperature
invariant, which is the dynamical temperature averaged over the
whole phase space including the chaotic sea and the islands, would
have the form $\Theta = \mu_{sea} T_{sea} + \mu_{isles} T_{isles}
= 1$ in our normalization of $T$. For the sake of clarity we
designate $\mu_{sea}\equiv\mu$, $T_{sea}\equiv T$; $\mu_{isles}$,
equal to $1-\mu$, is the measure of the islands; $T_{isles}$ is
the temperature on the islands, i.e., the quantity~(\ref{T})
calculated for the initial data on the islands. From this equality
one has

\begin{equation}
T = \frac{1 - \mu_{isles} T_{isles}}{1 - \mu_{isles}} = 1 +
\mu_{isles} (1 - T_{isles}) + O(\mu_{isles}^2) .
\label{Tth}
\end{equation}

\noindent Comparing Eqs.~(\ref{Tmu}) and (\ref{Tth}) with the
precision of $O(\mu_{isles}^2)$, we find

\begin{equation}
\gamma \approx T_{isles} - 1.
\label{gm}
\end{equation}

\noindent The quantity $T_{isles}$ is determined by the $y$
location of the islands in the phase space. The data on the
location of the islands is available in~\cite{C79} (for the
2-periodic solutions and accelerator modes) and in~\cite{C78} (for
the 4-periodic solutions). The temperature is straightforwardly
calculated by Eq.~(\ref{T}), and it has the values: $T_{isles}
\approx 0$, $3$, and $3/2$ for the 2-periodic solutions,
accelerator modes, and 4-periodic solutions, respectively; i.e.,
$\gamma \approx -1$, $2$, and $1/2$, respectively, in accord with
our analysis of the plots in Figs.~3 and 4.

\section{Conclusions}

Let us summarize the main results. The measure $\mu$ of the main
connected chaotic domain (MCCD) of the standard map and its
dynamical temperature $T$ have been studied as functions of the
stochasticity parameter $K$ by means of extensive numerical
experiments. The process of the birth and disintegration (upon
small variations of $K$) of the islands of stability inside the
chaotic domain result in local variations (spikes) in $\mu(K)$ and
$T(K)$. It has been shown that the variations of $\mu$ and $T$ are
connected by certain dependences~(\ref{Tmu}). Since the island
areas are small, these dependences are equivalent to power
laws~(\ref{plgamma}): $T = \mu^\gamma$, with $\gamma = -1$ and $2$
for the 2-periodic solutions and accelerator modes respectively
and $\gamma = 1/2$ for the 4-periodic solutions. It is interesting
to note that the value of $\gamma$ for the 4-periodic solutions is
the arithmetic mean of the values for the 2-periodic solutions and
accelerator modes.

If the newly found relations are confirmed analytically in a
rigorous way, they would provide an efficient instrument for
estimating the measure of chaotic domains by means of
computing the dynamical temperature. Such a method would be more
efficient than the OTM or LCESM, since any direct measurement of
$\mu$ is a tedious and time-consuming task, subject to a number of
uncertainties.

The author is thankful to anonymous referees for advice and
remarks which led to significant improvement of the manuscript.
This work was supported by the Russian Foundation for Basic
Research (project \# 05-02-17555) and by the Programme of
Fundamental Research of the Russian Academy of Sciences
``Fundamental Problems in Nonlinear Dynamics''. The computations
were partially carried out at the St.\ Petersburg Branch of the
Joint Supercomputer Centre of the Russian Academy of Sciences.

redpajama_set_name: RedPajamaArXiv


text:
\section*{Abstract}

We use {\em ASCA}\/\ data to obtain two-dimensional maps of the gas temperature in
three clusters: A754, A3558 and Triangulum Australis (the maps of A2256,
A2319, A2163 and A665, also presented at the conference, have since appeared
in [5]). All clusters from our sample show considerable temperature decline
with radius at $r\sim 0.5-1\,h^{-1}$ Mpc, most prominently in distant A2163
and A665. The three clusters presented here also feature asymmetric spatial
temperature variations, which may be naturally attributed to the effects of
a subcluster merger. As an example, we show that the Triangulum Australis gas
temperature and density maps indicate recent nonadiabatic heating,
presumably by merger shocks. Unlike most of the clusters, the systems in
our sample lack cooling flows (with the possible exception of a weak one in
A3558), thus we may be probing the younger members of the cluster
population.

\vspace{7mm}

Spatially resolved measurements of the gas temperature in clusters of
galaxies can provide valuable information on the dynamical history of these
systems, pointing to those clusters with recent or ongoing merger activity
(e.g., [8]). The present-day cluster merger rate is dependent on
cosmological parameters, with more mergers in higher-$\Omega$ models.
Simulations show that cluster radial temperature profiles are also sensitive
to the underlying cosmology (e.g., [2]). Thus, measurements of the cluster
temperature structure are of significant interest. Such measurements for hot
(and therefore massive) clusters have become possible now with the advent of
{\em ASCA}\/.

{\em ASCA}\/\ temperature maps of A2256, A2319, A2163 and A665 were presented in
[5] (see also [1]). In this paper, we present our results for A754, A3558
and Triangulum Australis (all three have $z\simeq 0.05$). To reconstruct
their temperatures, we employed the technique described in [5,6], using
{\em ROSAT}\/\ images as a brightness template and modeling {\em ASCA}\/\ mirror
scattering, modifying the technique for the cD region in A3558 [7].

Earlier, {\em ROSAT}\/\ PSPC data suggested the existence of gas temperature
variations over the face of A754 [4]. The cluster galaxy distribution and
its X-ray image indicate the ongoing subcluster merger, and the temperature
nonuniformity supports this hypothesis. Our GIS+SIS results for A754,
presented in Fig.~1 (and in more detail in [3]), are in general agreement
with earlier findings while having a much better accuracy. We detect a spur
of hot gas along the cluster elongation axis. Cooler gas resides in the
north-eastern outskirts, and, according to [4], in the region of the
brightness peak. The temperature and brightness maps of A754 are strikingly
similar to the results of a simulation of a merger with the nonzero impact
parameter [2]. If the analogy with the simulation is correct, the eastern
and western subunits seen in the image are infalling from North and South,
respectively. The elongated plume of cool gas near the X-ray brightness peak
is then the stripped atmosphere, and perhaps even a cooling flow, belonged
to the eastern subunit.

\begin{figure}[t]
\begingroup\pst@ifstar\pst@picture(0,8.9)(14.5,20)

\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}[tl]{0}(-0.4,19.8){\epsfysize=7.4cm
\epsffile{754map_gray.ps}}

\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}{0}(-0.5,16.5){\def\pst@par{}\pst@object{psframebox}*{\white \rule{5mm}{5mm}}}

\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}[tl]{0}(-0.35,12.8){\epsfxsize=8.5cm
\epsffile{754temps.ps}}

\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}[tl]{0}(7.1,19.8){\epsfysize=7.4cm
\epsffile{3558map.ps}}

\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}[tl]{0}(7.3,12.8){\epsfxsize=7.5cm
\epsffile{3558temps.ps}}

\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}{0}(3.9,19.85){A754}
\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}{0}(11.4,19.85){A3558}

\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}[cl]{0}(5.5,12.1){\def\pst@par{}\pst@object{psframebox}*{\white \rule{12mm}{1mm}}}
\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}[cl]{0}(13,12.1){\def\pst@par{}\pst@object{psframebox}*{\white \rule{11mm}{1mm}}}
\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}[cl]{0}(3.2,9.25){\def\pst@par{}\pst@object{psframebox}*{\white \rule{11mm}{1mm}}}
\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}[cl]{0}(10.8,9.25){\def\pst@par{}\pst@object{psframebox}*{\white \rule{11mm}{1mm}}}
\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}[cl]{90}(0.1,10.5){\def\pst@par{}\pst@object{psframebox}*{\white \rule{11mm}{1.5mm}}}
\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}[cl]{90}(7.6,10.5){\def\pst@par{}\pst@object{psframebox}*{\white \rule{11mm}{1.5mm}}}

\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}{0}(3.9,9.25){region \#}
\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}{0}(11.4,9.25){region \#}
\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}{90}(0.2,11){$T_e$, keV}
\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}{90}(7.7,11){$T_e$, keV}
\endpspicture

Fig.~1---Temperature maps of A754 and A3558. Contors show {\em ROSAT}\/\ PSPC
surface brightness; grayscale shows {\em ASCA}\/\ temperatures. For A754, regions
are 5$^\prime$\ boxes and sectors of the $r=16'$ circle. For A3558, the regions
are an $r=2.5'$ circle centered on the cD galaxy and sectors of the two
annuli $r=8-18'$ around the cluster centroid.  Regions are numbered and
their temperatures are shown in the lower panels.  Two spectral components
are shown for the cD region in A3558. Horizontal lines correspond to the
average temperature in A754 and average temperatures within each annulus for
A3558. All errors are 90\%.
\end{figure}

A3558 is a core member of the Shapley supercluster. Its X-ray image suggests
that the cluster may have experienced a merger and more are to happen. The
temperature map and radial profile of A3558 are shown in Figs.~1 and 3. A
fit to the cD galaxy region required at least two spectral components, with
the additional hot thermal component preferred over a physically meaningful
power law [7]. There is a slight radial temperature decline, which is
asymmetric. The asymmetry is present in both SIS and GIS data fitted
separately, although with marginal significance. We interpret this asymmetry
as a merger signature.

A {\em ROSAT}\/\ image of the Triangulum Australis cluster shows that there is an
underdense region east of center (Fig.~2; region 2). From the image alone,
one expects this region to have a higher temperature to maintain a pressure
similar to the adjoining sectors, assuming the cluster gravitational
potential is reasonably smooth. Our temperature map indicates that the
cluster core has a higher temperature, and the temperature in the
low-brightness sector is indeed slightly higher than the average at that
radius, just enough to balance the gas pressure.  However, its specific
entropy, which is a useful diagnostic of shock heating or any other
nonadiabatic heating, is significantly higher than that in other regions at
the same radius (Fig.~2). The entropy in the core is also higher than that
expected in an isothermal model, which is a kind of distribution a cluster
gas is expected to approach if left to itself, particularly if thermal
conduction is effective. The simplest explanation of such pressure and
entropy distribution would be that the gas in the cluster center was heated
by the passage of a merger shock. The same event might have heated and
ejected the gas in region 2 from the center, which then adiabatically
expanded to its present density. Hydrodynamic simulations of a head-on
merger [8] predict a hot core and an asymmetric temperature structure not
unlike the observed one.

\begin{figure}[t]
\begingroup\pst@ifstar\pst@picture(0,8)(14.5,20)

\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}[tl]{0}(-0.1,20.2){\epsfysize=7.5cm
\epsffile{trimap_gray.ps}}

\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}[tl]{0}(7.6,20.13){\epsfxsize=7cm
\epsffile{tritemps90.ps}}

\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}[tl]{0}(7.6,16.3){\epsfxsize=7cm
\epsffile{trientro90.ps}}

\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}[cl]{0}(10.9,8.5){\def\pst@par{}\pst@object{psframebox}*{\white \rule{15mm}{2mm}}}
\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}{0}(11.5,8.4){region \#}

\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}[tl]{0}(-0.1,12.6){
\begin{minipage}{7.4cm}
Fig.~2---Temperature map of Triangulum Australis, overlaid on the {\em ROSAT}\/\
image. {\em ASCA}\/\ regions are concentric annuli with $r=3-12-23'$, with the
outer annuli divided into 5 and 4 sectors, respectively (two sectors poorly
covered by {\em ASCA}\/\ are not shown.)  Right panels show temperature, gas
pressure and specific entropy in these regions.  Horizontal line in the
second annulus corresponds to an average over regions 4, 5 and 6. Dashed
line shows entropy for an isothermal $\beta$-model with $T_e=8$ keV.
\end{minipage}
}
\endpspicture
\end{figure}

\vspace{5mm}

Of the eight clusters for which the temperature was reconstructed so far
using our method, all but one exhibit a radial temperature drop at $r\sim
0.5-1\,h^{-1}$ Mpc (the exception is nearby AWM7, for which our analysis
covered only $r<0.25\,h^{-1}$ Mpc and resulted in a constant profile [7]).
Fig.~3 shows the radial temperature profiles of those clusters which are
relatively symmetric. Of the five clusters reasonably well resolved by
{\em ASCA}\/\ (A2256, A2319, A754, A3558 and Triangulum Australis), three,
presented here, show asymmetric temperature structure suggestive of a recent
or ongoing merger. The other two, A2256 and A2319, although not showing the
characteristic temperature asymmetries [5], are probably starting to merge
with the subunits which are apparent in their X-ray images, but the process
may have not yet disturbed the bulk of gas.

An eventual drop of the gas temperature at some distance from the cluster
center is expected intuitively and is predicted by simulations (e.g., [2]).
However, in the clusters we studied, the temperature appears to decline even
steeper than expected in the standard cosmological models. The most extreme
case of A2163 is discussed in [6]. Generally, steeper temperature profiles
are predicted in either the models with low $\Omega$ (due to the steeper
density profiles), or in the models with significant galaxy feedback [2]. In
open models, present-day clusters are relaxed and there are few mergers
among them.

However, our cluster sample is quite likely to be biased towards younger
systems, because of our selection of objects without cooling flows to
minimize the effects of the uncertain {\em ASCA}\/\ PSF. Cooling flows may be
disrupted by mergers, and merging clusters are expected to have peaked
temperature profiles [8]. As our sample expands and becomes more
representative, it may become possible to derive cosmological constraints
from it.

\begin{figure}[t]
\begingroup\pst@ifstar\pst@picture(0,6.6)(14.5,20)

\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}[tl]{0}(0.4,20.4){\epsfysize=7cm
\epsffile{2256tprof.ps}}

\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}[tl]{0}(7.1,20.4){\epsfysize=7cm
\epsffile{2319tprof10.ps}}

\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}[tl]{0}(0,13.6){\epsfysize=7cm
\epsffile{3558tprof.ps}}

\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}[tl]{0}(5.75,13.6){\epsfysize=7cm
\epsffile{665tprof.ps}}

\begin@psput{\pst@getref{\pst@getrputrot{\end@psput\rput@i}}}[tl]{0}(10.2,13.6){\epsfysize=7cm
\epsffile{2163tprof1.ps}}
\endpspicture

Fig.~3---Radial temperature profiles of five clusters. For A2163,
temperatures in three-dimensional shells are shown (from [6]), while other
temperatures are projected on the image plane. For A2256 and A665, also
shown are {\em ROSAT}\/\ PSPC results from [5,7].
\end{figure}

\vspace{1pc}

\re
1. Churazov, E., Gilfanov, M., Forman, W., \& Jones, C. 1996, these proceedings
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In July of 2015 we bought a female puppy from breeder Jeanette Häkämies Karlsson in Sweden, from kennel Vildingarnas. She is from an exciting combination and has a different genetic background than what our female Frigg has. She has so far been an excellent addition to our family, and I look forward to train and become better acquainted with her. She will be used a great deal in agility as she grows older.
Her name is also from Norse mythology, from «Vilje and Ve» brothers of the God Odin. The name is used on a male in the mythology, but is commonly used on the female gender today.
See more photos of Vilje in her gallery!


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ARCA Championship: Third Place Finisher Tom Hessert Reflects On 2010
The 2010 ARCA season will be remembered for including one of the best championship battles the series has seen in a long time, involving three contenders. In the end, Tom Hessert finished third, 85 points behind Craig Goess, who finished second. "It was an awesome year," Hessert told the ARCA Racing Network. "Obviously, I'll say that this was the best season in my career to this point. I'm a little disappointed to not win after we came from such a difference after the first eight races - 220 points down - to lead the championship for a couple of hours (laughing), at least, after Salem. We got our first win and had a bunch of top-10s and top-fives, so I'm pretty pleased." The first win is a moment that many refer to as the highlight of&...
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By Ashley McCubbin – December 23, 2010
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LanYFP is a basic (constitutively fluorescent) green/yellow fluorescent protein published in 2013, derived from Branchiostoma lanceolatum. It has very low acid sensitivity.
Most newly cloned green and yellow fluorescent proteins are not subjected to additional engineering simply because of their lack of improved properties relative to existing proteins. Thus, we were intrigued that a yellow fluorescent protein from B. lanceolatum (LanYFP) exhibits an unusually high quantum yield (∼0.95) and extinction coefficient (∼150,000 M−1 cm−1), making it a very attractive candidate for additional development.