text:
Beoga coming to San Juan Capistrano
Beoga features Niamh Dunne, Damian McKee, Seán Óg Graham, Eamon Murray and Liam Bradley.
With St. Patrick's Day less than a month away, there are a number of Irish music concerts coming to Orange County.
One of the most anticipated Celtic concerts is coming courtesy of Beoga, a five-member traditional group based in County Antrim, Ireland.
Beoga (an Irish word meaning "lively") will perform two shows in San Juan Capistrano as part of the Music at the Library concert series on Saturday evening, March 1.
The group traces its inception to a music jam session in August 2002, which brought together button accordion players Seán Óg Graham and Damian McKee with bodhrán master Eamon Murray and pianist Liam Bradley.
That foursome released the wonderful "A Lovely Madness" CD in 2004, which was greeted with critical acclaim throughout Ireland, as well as Europe and America.
With the later addition of Irish singer Niamh Dunne, the group continued its artistic climb with the recording of 2007's "Mischief."
Beoga's sophomore CD features thrilling jigs ("Kick'n the Box," "Ryan's Air"), instrumental reels ("Cu Chullain's Despair"), traditional folk songs ("Factory Girl," "A Delicate Thing") and even a reworked cover of the Steely Dan classic "Dirty Work" and the 1920s swing-styled standard "Please Don't Talk About Me When I'm Gone."
It's no wonder that "Mischief" was praised by Irish Music Magazine and the U.S. publication the Celtic Connection as one of the best albums of 2007.
Beoga is truly able to blend a wealth of traditional folk styles together whether performing original material or revised classics.
Beoga will perform at San Juan Capistrano Regional Library, 31495 El Camino Real, San Juan Capistrano, playing at 6:30 and 8:30 p.m. on March 1.
Tickets are $10 for adults and $5 for children under age 12.
Third Day, The Myriad impress in Anaheim show
Outside it was cold and raining, but inside the House of Blues Anaheim on Thursday night, Feb. 21, 2008, a capacity-crowd was warmed by a strong set from headliner Third Day and a groundbreaking appearance from relative newcomer the Myriad.
One of Christian music's most successful rock outfits, Third Day came to Anaheim as part of a short six-date club tour to gear up for a full-fledged spring tour. So while the band only played 75 minutes, fans were treated to the band's best-known hits, as well as some particularly promising songs set for release on the band's next studio release.
Third Day has honed a Southern rock sound that is rooted in the territory of Lynyrd Skynyrd but also boasts a heavy guitar crunch associated with neo-grunge bands such as Three Doors Down and Creed. That doesn't tell the full story, since Third Day's material is always melodic and features uplifting choruses that draw comparisons to U2's approach.
The band explored the full range of its sonic territory, playing the scorching "Rockstar," midtempo material such as "Who I Am" and praise songs ("King of Glory," "God of Wonders") that had many in the audience lifting their arms into the air.
Singer Mac Powell sang with power and conviction throughout the night, his baritone showcased on the soaring "Tunnel" and "My Hope Is You."
The group also played several new songs, with "Call My Name" especially effective with its undeniable chorus.
The Myriad is a young, up-and-coming band out of Seattle whose sound draws comparisons with the Cure, Radiohead and Snow Patrol, but is unique enough to warrant the band's growing buzz.
"A Clean Shot," one of the six songs performed by the band, was a highlight of the 30-minute set. But the lush and artful sound made by the quintet is as much a part of the Myriad as the songs themselves. Following the lead of Sigur Ros, the band even used a violin bow on the electric guitar at times to dramatic effect.
The Myriad is set to release "With Arrows, With Poise" on Koch Records in April and based on the group's wonderful set in Anaheim, it should rank on one of the most anticipated rock albums of 2008.
The night's opening group Revive performed a short set of four songs. The Australian group is one of the Christian rock's emerging voices and has a strong card in lead singer Dave Hanbury, whose impressive voice was especially forceful on the riff rock-styled "Can't Change Yesterday."
Michael Ubaldini returns to play his 'Americana' songs
Since its opening in 1980, acclaimed modern rock artists such as the Call and Brother have recorded concerts for commercial release at the Coach House in San Juan Capistrano.
Now one of Orange County's best-known artists is going to chronicle a special full-length concert for release as a combo DVD-CD collection. Fountain Valley-based Michael Ubaldini will headline at the San Juan Capistrano venue on Thursday night, Feb. 21, performing Americana-styled material from across his acclaimed discography.
"We're going to do stuff off every record," explained Ubaldini in a recent interview. "Some songs I'll just play acoustically with guitar and harmonica. Then the band will play with me on the other songs."
The cast of sonic players slated to join Ubaldini on stage includes Gavin Jones (bass), Larry Green (guitar), Mitch Ross (drums), Jimmy Zeiger (saxophone), Chris Lawrence (pedal steel guitar), TJR (keyboards), and Tricia Freeman and Deanie Wood on backing vocals.
"All are great musicians in their own right and it's a pleasure to be back together for this special event," Ubaldini said.
And while Ubaldini and his talented band have been rehearsing in anticipation of the upcoming show at the Coach House, he has also been going into the studio to record new material. Many of the songs are destined to appear on an upcoming acoustic collection, while more up-tempo material will be included on a forthcoming rock album.
"It has been a good year for songs," Ubaldini said.
Ubaldini, the Fallen Stars and Niki Smart will perform at 8 p.m. Thursday, Feb. 21 at the Coach House, 33157 Camino Capistrano, San Juan Capistrano. Admission to this special concert recording event is $10.
Michael Ubaldini returns to play his 'Americana' s...


text:
Since 2022, Lindsay Lohan is possibly single
by admin | Jan 19, 2023 | interracial-dating-central-inceleme visitors
Lindsay Lohan is good 35-year-dated American Motion picture Actress regarding Bronx, Nyc, U . s .. She was created to your Wednesday, July 2, 1986. Are Lindsay Lohan partnered otherwise unmarried, and you will who is she relationships now? Why don't we discover!
Lindsay Dee Lohan is actually an american actress, businesswoman, developer and you may musician. Born and increased for the New york, Lohan is actually signed so you can Ford Patterns once the a kid. Which have appeared while the a consistent for the Other World from the interracial dating central nedir decades ten, the lady discovery was available in Disney Pictures' The newest Moms and dad Trap (1998). The fresh film's success triggered appearances in a sequence of its televised video clips together with theatrical Slutty Tuesday (2003). She began their elite group career since a Ford model from the age around three.
Fun Fact: On the day off Lindsay Lohan's birth, "There will be Sad Musical (To get you to Scream)" from the Billy Ocean was the number 1 tune to the Billboard Gorgeous 100 and Ronald Reagan (Republican) try new You.S. President.
Lindsay Lohan's Boyfriend
Lindsay Lohan is solitary. She actually is perhaps not dating some body already. Lindsay got no less than 79 matchmaking in the past. Lindsay Lohan could have been engaged to help you Egor Tarabasov (2016) and you can Wilmer Valderrama (2004). In the 2004 she dated actor Wilmer Valderrama. She dated artist and you can DJ Samantha Ronson away from 2008 to help you 2009. She came into this world so you can Michael and you will Dina Lohan. She's got five siblings called Cody, Ali, Ashley, Michael and you will Landon. She had interested to help you Egor Tarabasov within the 2016, nevertheless they after split up. Based on the details, she's got no college students.
Like other celebs and celebs, Lindsay features this lady individual and you may sex-life personal. Glance at right back often even as we will continue to revision this site having this new dating information. Let us take a look at Lindsay Lohan past relationship, ex-men and you can past hookups.
Lindsay Lohan's birth sign was Cancers. Cancer tumors are extremely sensitive and compassionate. A cancers generally rushes drops crazy falls easily along with an extremely noisy thud that is less inclined to bail when the fresh supposed becomes rough. Cancers are loyal and calculated to work anything out. The absolute most suitable cues which have Disease are often considered to be Taurus, Virgo, Scorpio, and you will Pisces. The least compatible cues having Malignant tumors are reported to be Aries and you may Libra. Lindsay Lohan likewise has a dominating entire world of Moonlight.
Prior Relationships
Lindsay Lohan has been in relationship which have Denis Papageorgiou (2016), Gavin Doyle (2012), Adam Senn (2009 – 2010), Samantha Ronson (2008 – 2009), Heath Ledger (2007 – 2008), Riley Giles (2007), Calum Top (2007), Robbie Williams (2006 – 2007), Harry Morton (2006), Courtenay Semel (2006 – 2008), Jamie Burke (2006), Damien Fahey (2003 – 2004) and you may Aaron Carter (2002 – 2003). She has also had experiences which have Matt Nordgren (2013), Maximum George (2012), Voodoo (2012), Philipp Plein (2011), Oscar Lusth (2011), Zac Efron (2011), Child Berryman (2011), Nico Tortorella (2011), fifty Cent (2010 – 2011), Danny Cipriani (2010), Ryan Phillippe (2010), Evan Peters (2010), Jason Segel (2009), Petey Wright (2009), Gerard Butler (2009), Alessandro Di Nunzio (2008), Dario Faiella (2008), Edoardo Costa (2008), Criss Angel (2007), Travis Barker (2007), Scott Storch (2007), Garrett Hedlund (2007), Joe Francis (2007), Stavros Niarchos (2006), Brody Jenner (2006), Brett Ratner (2006), Brandon Jack James (2006), Benicio Del Toro (2006), Jamie Dornan (2006), Joaquin Phoenix (2006 – 2010), Sean Lennon (2006), Justin Timberlake (2006), Adam Levine (2006), Harry Judd (2005), Colin Farrell (2004), Lukas Haas, Orlando Flower, Ashton Kutcher, Josh Mond, Ryan Rottman and Aaron Voros. This lady has been interested in order to Egor Tarabasov (2016) and you can Wilmer Valderrama (2004). Our company is currently in procedure of looking up more information on the previous dates and you will hookups.
Lindsay Lohan Bio
Lindsay Lohan was given birth to towards next away from July from inside the 1986 (Millennials Age group). The original age group to reach adulthood regarding brand new century, Millennials would be the more youthful technical professionals who prosper for the the new innovations, startups, and working regarding coffee shops. These people were the youngsters of your own 90s who have been created roughly ranging from 1980 and 2000. These 20-somethings so you're able to early 29-year-olds provides expanded the latest place of work. Big date mag titled him or her "The latest Me Myself Me personally Generation" because they are interested all the. He's labeled as convinced, entitled, and you will disheartened.
Lindsay Lohan is preferred to be a motion picture Celebrity. Celebrity exactly who very first gained detection to have portraying Annie James and Hallie Parker, twins separated once beginning, regarding 1998 Disney funny New Parent Pitfall. She acquired numerous MTV Movie Honors for her featuring part for the Imply Females in 2004 and you can she in addition to played direct positions in the Herbie: Totally Stacked and you will Nasty Friday. She played alongside Rachel McAdams from inside the Imply People. Lindsay Dee Lohan attended Cooler Spring Harbor High school, Cooler Spring Harbor, Nyc, Sanford H. Calhoun Highschool, Merrick, New york, Homeschooled.
Lindsay Lohan is actually flipping thirty-six from inside the
Lindsay was born in new 1980s. The latest 1980s was the fresh new a decade out-of big locks, larger mobile phones, pastel serves, Cabbage Plot Infants, Rubik's cubes, Yuppies, Heavens Jordans, neck shields and you will Pac Child. For the Eighties, Berlin Wall crumbled, the newest computers innovation emerged and smash hit clips and MTV reshaped pop culture.
The fresh 35-year-dated American was born in the season of one's Tiger and you may belongs to Millennials Generation
Centered on Chinese Zodiac, Lindsay was born in the entire year of one's Tiger. People born in the year of the Tiger are brave and you can separate. He could be recognized for their deep advice and you can daring tips, however, possibly showcase whenever accomplishing one thing.

redpajama_set_name: RedPajamaCommonCrawl


The high-end phablet will supposedly come with the new Kirin 950 SoC.
Will yet another Huawei phablet launch alongside or shortly after the Mate 8? Leaked details from benchmarking application AnTuTu suggest that the P9 Max phablet may soon be ready for an official reveal.
According to the source, the P9 Max (model P950S) will be a 6.2-inch phablet with a display resolution of 2560 x 1600 pixels. The device will supposedly ship with Android 6.0 and carry the recently announced 16 nm FF+ Kirin 950 SoC and integrated Mali-T880 MP4 GPU. RAM and storage space are expected to be 4 GB and 64 GB, respectively. Smartphones running Marshmallow are slowly creeping up the charts according to Google.
In AnTuTu, the alleged P9 Max scores just under 74000 points with a 3D score of about 17000 points. In comparison, Huawei claimed a top score of 83000 points for the Kirin 950 during its reveal.
Huawei has been rising in the ranks worldwide. The Chinese manufacturer has surpassed Xiaomi in China and was selected by Google to manufacture the lauded Nexus 6P phablet.


I am interested in obtaining some high temp silicone bellows like this.
Could you tell us where you obtained yours from?
Topic: My quick review of Kontax Ross-yoke model.
Re: My quick review of Kontax Ross-yoke model.
Sad to say i don't own either engine..
But glad to say i don't own any kind of apple (except the one in my lunchbox)..
Nice engine purchase though, they are a very sweet ride!!
That's an interesting approach. Turning things inside out could make for a very compact burner and heat exchange system..
Can you post some pictures and give a more detailed explanation of your 'piston problems'..


In great poetic figurative imagery, David describes God's response to his plea for help. The majesty and power of the Lord is described as He comes down from Heaven. God demonstrates His anger at evil by shaking the earth and thundering in the heavens with dark storms. The imagery is terrifying and awesome in its powerful wording. This passage is reminiscent of the Lord coming down on Mount Sinai in Exodus 19. There the mount was filled with dark clouds, smoke, thunder and lightning, as the mountain quaked violently with the presence and the voice of God.
Lord Jesus, I am amazed at Your mighty power and Your majesty. I am thankful for Your coming down from Heaven to help me and all Your people who cry out to You.


The Loan Away Inc. (we, us) website (Site) is offered to you conditioned on your acceptance without modification of the terms, conditions, and notices contained herein, as amended from time to time. Your use of the Site constitutes your agreement to all such terms, conditions, and notices. Site may only be accessed by those who are 13 years of age or older.
All contents of the Site are: Copyright 2014 by Loan Away Inc. and/or our affiliates. The names of actual companies and products mentioned herein may be the trademarks of their respective owners. Any rights not expressly granted herein are reserved.
THE INFORMATION, PRODUCTS, AND SERVICES INCLUDED IN OR AVAILABLE THROUGH THE SITE MAY INCLUDE INACCURACIES OR TYPOGRAPHICAL ERRORS. CHANGES ARE PERIODICALLY ADDED TO THE INFORMATION HEREIN. WE AND/OR OUR AFFILIATES MAY MAKE IMPROVEMENTS AND/OR CHANGES IN THE SITE AT ANY TIME.
WE AND/OR OUR AFFILIATES MAKE NO REPRESENTATIONS ABOUT THE SUITABILITY, RELIABILITY, AVAILABILITY, TIMELINESS, CURRENCY AND ACCURACY OF THE INFORMATION CONTAINED ON THE SITE FOR ANY PURPOSE. TO THE MAXIMUM EXTENT PERMITTED BY APPLICABLE LAW, ALL SUCH INFORMATION AND THE PRODUCTS AND SERVICES ARE PROVIDED "AS IS" WITHOUT WARRANTY OR CONDITION OF ANY KIND. WE AND OUR AFFILIATES HEREBY DISCLAIM ALL WARRANTIES AND CONDITIONS WITH REGARD TO THIS INFORMATION, PRODUCTS, SERVICES, INCLUDING ALL IMPLIED WARRANTIES OR CONDITIONS OF TITLE, NON-INFRINGEMENT, AND OF MERCHANTABILITY, FITNESS FOR A PARTICULAR PURPOSE. WE RESERVE THE RIGHT TO MODIFY AND/OR REMOVE SUCH INFORMATION AT OUR SOLE DISCRETION WITH NO FURTHER NOTICE.
The Site may contain links to other websites ("Linked Sites"). The Linked Sites are not under the control of the Site and we are not responsible for the contents of any Linked Site, including without limitation any link contained in a Linked Site, or any changes or updates to a Linked Site. We are not responsible for webcasting or any other form of transmission received from any Linked Site. We are providing these links to you only as a convenience, and the inclusion of any link does not imply our endorsement or any association with its operators.
Any ideas, proposals, and/or other information submitted or collected on the Site (excluding information provided pursuant to an application for credit) shall be considered non-confidential. By submitting information to the Site, or directly to us, you agree that we shall not be under any obligation of confidentiality or non-use, express or implied, with respect to any submissions, and we may disclose or use any submission for any purpose whatsoever, at our sole discretion, with no obligation, express or implied, to compensate or work with the person or entity that supplied the information, idea and/or proposal in any manner.


A new comprehensive study by the Center for Near East Policy Research and the Israel Resource News Agency, commissioned by the Simon Wiesenthal Center, highlights that there is an unprecedented level of incitement to terror in new Palestinian Authority school books used in UNRWA schools. How should the sixty-eight UNRWA donors react?
Rachel Avraham is a senior media research analyst at the Center for Near East Policy Research and a correspondent for the Israel Resource News Agency. She is the author of "Women and Jihad: Debating Palestinian Female Suicide Bombings in the American, Israeli and Arab media," published by the Gefen Publishing House. She received her BA degree at the University of Maryland at College Parkand, where she majored in Government and Politics, and her MA degree from Ben Gurion University of the Negev, where she majored in Middle Eastern Studies.
The Center for Near East Policy Research and the Israel Resource News Agency published a comprehensive study, commissioned by the Simon Wiesenthal Center, that provides numerous examples of how new Palestinian Authority textbooks, which are being used in UNRWA schools, incite terrorism against the Jewish people and State of Israel. What differentiates this study from previous studies of PA school textbooks — from the time that the PA began introducing its own schoolbooks into UNRWA schools in 2000 — is that this is the first time that all PA school books were examined in a comprehensive manner. The study argues that despite statements made to the contrary by the US State Department and others, incitement to terrorism remains a pivotal part of the Palestinian school curriculum.
Moreover, throughout the 2016-2017 textbooks, the name "Israel" was replaced by the phrase "Zionist occupation" and the Arab-Israeli conflict was referred to as "the Zionist-Arab conflict." The maps in the Palestinian textbooks do not show Israel on the map. Even major Israeli cities, such as Tel Aviv, do not appear on the maps in the Palestinian textbooks, as they were built by Jews. Instead, the textbooks call for the descendants of the Palestinian refugees to return to their former homes via armed struggle. A fifth grade textbook declares, "We are returning/ Returning to the homes, to the valleys, to the mountains/ Under the flag of glory, Jihad and struggle/ With blood, sacrifice, fraternity and loyalty/ We are returning." Even the math textbooks include questions that prompt students to support "Palestinian shahids." The question remains: should funding to UNRWA be made conditional upon reforms in the UNRWA educational system?
Dr. Arnon Groiss, the study's author, disagrees, stressing that documentation provided by the Center for Near East Policy Research shows that some UNRWA staff members have openly supported terrorism against Israel, as well as online antisemitic hate speech. In fact, some UNRWA teachers have even moonlighted as terrorists. For example, UNRWA's workers union publicized a poster featuring the map of "Palestine" (Israel is wiped off the map) accompanied with the following caption: "Oh UNRWA, we have a cause and our fight, jihad, resistance and struggle against those who usurped our land do not need neutrality." The UNRWA workers' union has been controlled by Hamas for many years. Some former UNRWA employees, including Suheil Al-Hindi, were actively part of Hamas while working for UNRWA. It took a very long time for UNRWA to get rid of Hindi.
Om Alaa, who identifies herself as an UNRWA teacher on her Facebook profile, published on social media a picture of Adolf Hitler and his "top" ten quotes. Eman Shammala, who identifies herself as an UNRWA teacher on her Facebook profile, published a photo on Facebook of a keffiyeh-clad Palestinian playing a knife like a violin, using a Palestinian "key of return" as a bow. At the Al Fakhoura Middle School (UNRWA), the Islamic Bloc organized an event honoring thirteen years since the martyrdom of senior level Hamas terrorist Sheikh Yassin. A sign featuring Sheikh Yassin and the Hamas flag waved outside of the school.
All of the documentation provided by the Center for Near East Policy Research and the Israel Resource News Agency demonstrates that the there is, in fact, an unprecedented level of incitement to terror in PA textbooks being used in UNRWA schools.
Yet, the question remains: How should the international community respond to this incitement? Disbanding UNRWA is not an option, as it can only be disbanded by the United Nations General Assembly.
Therefore, the only possible way to bring about change in UNRWA education is for donor states in the West to use their financial influence to insist that UNRWA's curriculum excludes the promotion of hate and violence and that its materials reflect the reality of a neighboring Jewish state. In addition, the new UN Secretary General and all nations committed to peace in the Middle East must demand that UNRWA end all incitement in their schools. Furthermore, all staff members—especially teachers—who are members of terror organizations and/or make statements in support of terrorism and/or demonstrate hate speech be immediately fired.
 Arabic Language, Grade 5, Part 1 (2017) p. 14; Social Studies, Grade 9, Part 1 (2017) p. 74.
 Arabic Language, Grade 9, Part 1 (2017) p. 61.
 Arabic Language, Grade 7, Part 1 (2017) p. 66.
 Our Beautiful Language, Grade 3, Part 2 (2016) p. 64.
 Our Beautiful Language, Grade 5, Part 1 (2015) p. 50.
 United Nations Relief and Works Agency for Palestine Refugees in the Near East, "Textbooks Used in UNRWA Schools in the Occupied Palestinian Territory," October 6, 2017.
 From an exclusive interview with the author or this article.
 The Center for Near East Policy Research, "Hamas continues to operate freely in UNRWA schools in Gaza," September 2017.
 From an exclusive interview with the author of this article.


Ken & his staff are really caring people. They really do a great job. They do their research and really put together a great trip. I have been on many of their trips. (New York, DC, Niagara Falls & many day trips) Keep up the good work.


Wayne (W6IRD) and Sharon (K6IRD) Spring show off their shack and workshop, manufacturer's day at the Atlanta Ham Radio Outlet, surface mount soldering, and more.
Hosts: Bob Heil (K9EID), Gordon West (WB6NOA), and George Thomas (W5JDX) Wayne (W6IRD) and Sharon (K6IRD) Spring show off their shack and workshop, manufacturer's day at the Atlanta Ham Radio Outlet, surface mount soldering, and more. Guest: Gary Pearce (KN4AQ) Download or subscribe to this show at http://twit.tv/hn. We invite you to read, add to, and amend our show notes at wiki.twit.tv. Thanks to Joe Walsh who wrote and plays the Ham Nation theme. Thanks to Cachefly for the bandwidth for this show.


Buy and Sell Used Torit. Bid on Equipment is the market leader for the online sale of used, second hand and surplus machinery.
Feb 17, 2014· Fixing a Panasonic Lumix DMC FS35 that has dust behind the lens.
Purchase Filter Bag Replacements For Dust Collector Systems Save Off Retail Prices With Baghouse America. Baghouse America manufactures dust collector bags with all different fabrics for your application. Our main staple are fiberglass filter bags for industrial boilers applications.
The Panasonic LUMIX DMC-GM1 Digital Camera is the first model to sit in the new Panasonic GM range of portable and lightweight compact system cameras and offers many of the advanced features found the larger G-series models.
PANASONIC DMC-FZ5PP SERVICE MANUAL Pdf Download.
Panasonic DMC-FZ5PP Service Manual. Hide thumbs ... HOW TO DEFINE THE MODEL SUFFIX (NTSC or PAL model) There are seven kinds of DMC-FZ5, regardless the colours. ... Removal of the EVF Unit To prevent unnecessary dust being entered, do not remove the CCD Unit except for servicing.
Find 800 dmc dryflo mc2000 for sale right now. Shop our full collection of 800 dmc dryflo mc2000 in stock on the internet.
VQT1P98 Before use, please read these instructions completely. This manual is based on the DMC-TZ15 model. Product illustrations and screens may vary.
VQT4W14 M0113KZ0 Operating Instructions for advanced features Digital Camera Model No. DMC-LZ30 Please read these instructions carefully before using this product, and save this manual for future use.
PANASONIC DMC-FS3P SERVICE MANUAL Pdf Download.
Denray 9600 48 x 96 Down Draft Table Recently Denray introduced a new tube filtration system. Dust is captured within the tube, and then falls into the drawer below once the machine is turned off.
Some cameras are available in a choice of colour, indicated by a suffix letter: K is black, S silver, A blue, R red, W white. Most lower-priced models have small sensors of about 10.2 mm / 1/2.5".
Model stitched over 2 threads on 32 Ct. Pixie Dust by Silkweaver fabrics using DMC floss, Kreinik #4 braid and Mill Hill Beads. Stitch count 123x193. 123Stitch.com ships via the U.S. Postal Service to anywhere in the world.
Dust forming on the lens doesn't normally impede performance or graphic quality, it's the dust that forms on the sensor - at the rear of the camera, that does This can be confirmed by taking a shot of a completely clean scene...say, a white sheet - or a cloudless blue sky.
Preparations Preparations Before use Camera handling Keep the camera away from excessive vibration, force, or pressure. The camera is not dust resistant, splash resistant, or waterproof. Avoid using the camera in places with excessive dust or sand, or where water can come into contact with the camera.
The advantages of DMC pulse jet dust collector : 1, the dust collector have strong abilities of ash and dust removal ,high efficiency, low emission concentration, air leakage rate is small, less energy consumption, less consumption of steel, covers an area of less, stable and reliable operation, good economic benefit.
Basic Operating Instructions Digital Camera Model No. DMC-TZ110/DMC-ZS110 DMC-TZ80/DMC-ZS60 DMC-TZ110/DMC-ZS110 DMC-TZ80/DMC-ZS60 Please read these instructions carefully before using this product, and ... The camera is not dust resistant, splash resistant, or waterproof.
Donaldson Torit , the dust/fume/mist collection equipment brand of Donaldson Company, Inc., is a leading worldwide provider of dust collectors and replacement filters.
Le Hoooked Ribbons XL de DMC est idéal pour réaliser des sacs, des écharpes, des peluches et de nombreux autres accessoires. C'est un fil à tricoter ou à crocheter 100 % recyclé.
The Dryflo® line of mist collectors from Donaldson ... DMC-MMA All Wet Dryflo Leaves the Competition. ... in-stock orders shipped within 48 hours, Donaldson Torit is your best, most reliable source for premium performance replacement parts. Visit us at www.donaldsondynamic.com.


There are many diseases that know no bounds, ages or types. The same thing can be said of those who crave the open road on two wheels. Cycle riders come in all shapes, sizes and from various backgrounds, and now, they are coming together for a good reason.
"We want to do two things. One, help find a cure for Type 1 Diabetes, and two, have a great rally!" said Chuck Price.
Plans are to gather at the market beginning at 9:30 AM, then kickstands up promptly at 11:00 AM for an impressive bike procession through the market, then on South to Albany. The route passes the State Capital, runs through Albany Rural Cemetery and passes many other sites around the region.
Registration proceeds will go to the Juvenile Diabetes Research Foundation. Those who register early, get a reduced registration fee and have the opportunity to add a commemorative shirt to their order.
"There are various levels of sponsorship available as well. All donations are 100 percent tax deductible so we are hoping for lots of support," said Price.
This is the fifth annual ride, and more are scheduled in the future. Price and his family have personal ties to this all important cause.
"My son was diagnosed with Type 1 Diabetes at age eight. This disease requires constant monitoring, and regular visits to a pediatric endocrinologist. The more we learn, the better the chance to fight and cure this disease," said Price.
Last year's rally made over $5,000.00 for the research foundation. Price wants to best that and then some this year.
"Come out; support a great cause for some great kids. It is also a way to meet and greet fellow riders," said Price. Two Scooter clubs and a Moped Club were formed as a direct result of the first Rally. All will be on hand for ATR 5.
Additional information, including ride route and registration forms are available at the website. Visit http://atownrumble5.eventbrite.com.


text:
MACJC to NFL
Archived Stats
Former Bulldog D.J. Montgomery inks unrestricted free agent contract with the Cleveland Browns
Former Holmes Community College wide receiver D.J. Montgomery of Durant has signed an unrestricted free agent contract with the National Football League's Cleveland Browns.
For the past two seasons, Montgomery played at the Austin Peay State University Governors. As a senior, he started all 11 games at wide receiver catching 42 passes for 797 yards for an 18.98 per catch average and 10 touchdowns. As a junior, he started all 11 games and caught 19 passes for 228 yards and three touchdowns. He had a long catch of 55 yards his senior season and 39 yards as a long his junior season. He is third in touchdowns all-time at APSU.
At Holmes as a sophomore, he caught 36 passes for 991 yards and 10 touchdowns. He averaged 27.5 yards per catch and 99.1 yards per game. He was named First Team All-State and was named the MVP Offensive Player for his play in Holmes' Graphic Edge Bowl win over Iowa Western, 28-21. He caught seven passes for 205 yards and two touchdowns, one from 54 yards in the second quarter and one from 30 yards in the third. Holmes finished the 2016 season ranked at No. 7 in the NJCAA.
As a freshman, he caught 11 passes for 291 yards and two touchdowns. He averaged 36.4 yards per catch.
At his pro day, Montgomery put up solid testing numbers with a 4.43 40-yard dash and 6.69 in the 3-cone.
Montgomery played his high school career at Madison Central High School.


81% of technology buyers say they cut providers from consideration when their sales reps can't answer their questions. In fact, based on thousands of interviews with B2B buyers, the quality of the sales interaction has more impact on vendor selection than price, features or brand.
accounts are an ideal match for your strengths and quickly exit those you can't win.
objections to learn how to explain your strengths in context with your buyers' needs.
deliver more credible responses than your competitors, earning their trust and business.
What Do Technology Buyers Have To Say?
What we often got was someone who seemed heavily invested in sales and wasn't really an expert. It was like pulling teeth because I felt that what we were asking was new to them.
I don't want anybody just walking in and trying to sell us something. There has to be a link to my industry. It seemed as though it was just a big sales job. Everybody's selling, but it turns people off.
The vendors need to be more honest with responses to the questions that come up, and candid in terms of what they can and can't do. Be honest with us.
Stop spending all of your sales training dollars on "generic how to" sales techniques that position your team as outsiders. Show your reps "why" your buyers make this investment so they can sell like an insider.
Ensure your sales team wins the deals they should.


text:
JTA Sections
Watch: De Blasio, Cuomo, Tiki Barber On Why They Love Israel
By Aaron Herman June 15, 2017 12:37 pm
Tens of thousands of people lined Manhattan's Fifth Avenue on Sunday, June 4, to show their support for Israel, turning the famed street into a sea of blue and white. The Celebrate Israel parade, which took place on the Upper East Side from 57th Street to 72nd Street, was held under the banner of "Celebrate Israel All Together." The parade also recognized 50 years of the reunification of Jerusalem.
Sign up for our newsletter to get must-read New York stories each day
An Evening with Naftali Bennett
Mon. Jan. 30, 2023 @ 7:30 PM EST Hosted by: Streicker Center Temple Emanu-El NYC
The Role of Mass Media in Holocaust Portrayal
Mon. Jan. 30, 2023 @ 7:30 PM EST Hosted by: UJA-Federation of New York
Wed. Feb. 01, 2023 @ 11:00 AM EST Hosted by: Jewish Telegraphic Agency (JTA)
More from New York
A Jewish initiative aims to support Asian New Yorkers following Monterey Park shooting
By Jacob Henry January 24, 2023 5:22 pm
7 ways NYC is marking International Holocaust Remembrance Day
By Julia Gergely January 24, 2023 10:32 am
NY federation CEO offers rare criticism of Israel's right-wing government
By Andrew Silow-Carroll January 23, 2023 3:09 pm
Jewish news from around the world
Brought to you by the Jewish Telegraphic Agency


text:
\section{Introduction}
\label{sec:intro}

The Weakly Interacting Massive Particles (WIMP) have been proposed as one of the leading particle dark matter candidates to explain the missing non-luminous matter of the universe \cite{Zwicky:1933gu,Bertone:2004pz,Steigman:1984ac}. The WIMP with masses in the mass range of a few GeVs to tens of TeV would get gravitationally attracted to the celestial body, scatter off the nucleons in the celestial bodies and lose energy. WIMP whose velocities become less than the escape velocity of the celestial body are then trapped in the gravitational potential well of the celestial body. The trapped WIMP eventually sink to the centre of the celestial body due to gravity where their concentration increases. Subsequent annihilations of WIMP is expected to produce neutrinos in their final states. These neutrinos are expected to come with an energy spectrum in the range $[0-m_\chi]$, where $m_\chi$ is the WIMP mass. These neutrinos can be detected in the neutrino detectors, providing an indirect evidence for the existence of WIMP dark matter. Such indirect detection signals for WIMP in the sun \cite{Aartsen:2016zhm,Choi:2015ara,Albert:2016dsy} and earth \cite{Aartsen:2016fep,Albert:2016dsy} have been looked for in the currently running neutrino detectors such as IceCube \cite{Aartsen:2016zhm}, Antares \cite{Albert:2016dsy} and Super-Kamiokande (SK) \cite{Choi:2015ara}. Since none of the detectors have recorded any positive signal for WIMP annihilations in the sun and earth, they have given exclusion limits in the WIMP scattering cross-section -- WIMP mass space.
\\

The magnetised Iron CALorimeter (ICAL) detector proposed to be built at the India-based Neutrino Observatory (INO) should be able to detect the neutrinos from WIMP annihilations if the WIMP indeed have masses in the few GeV to 100s of GeV range. In our previous work \cite{Choubey:2017vpr} we explored the prospects of indirect detection of WIMP annihilation in the sun at the ICAL detector at INO. In this work we study the prospect of indirect detection of WIMP at ICAL from their annihilations in the centre of the earth. As is well known, the WIMP annihilation cross-section can be related to the WIMP-nucleus scattering cross-section. The WIMP scattering on nucleons can proceed both via Spin Independent (SI) as well as Spin Dependent (SD) process, where the SI cross-section depends on the mass of the nucleus involved while the SD cross-section does not. Therefore, heavier target nuclei offer better sensitivity to SI cross-sections. As a result, the WIMP direct detection experiments, which look for the recoil energy of target nuclei due to WIMP scattering on them in dedicated terrestrial detectors, are more sensitivity to SI cross-sections owing to their heavier target nuclei. On the other hand, the indirect detection search for WIMP annihilation in the sun is more sensitive to the SD cross-sections since the sun mostly consists of hydrogen. The earth has heavier elements and hence can be sensitive to SI cross-sections. While the direct detection experiments continue to be several order of magnitude more sensitive for SI interactions, indirect searches provide a complementary probe to dark matter and are hence interesting.
\\

The organisation of the paper is as follows. In Section \ref{sec:capture} we calculate the signal neutrino spectra due to WIMP annihilation in the earth. In Section \ref{sec:event} we describe the detector and the event generation procedure. Thereafter, in Section \ref{sec:background}, we describe the atmospheric background suppression scheme. In Section \ref{sec:analysis} we describe our statistical analysis, present results in Section \ref{sec:results} and finally conclude in Section \ref{sec:summary}.

\section{Neutrino flux from WIMP annihilation in the earth}
\label{sec:capture}

The number of WIMP ($N$) inside the earth as a function of time $t$ is given by the following differential equation \cite{Jungman:1995df},
\begin{equation}\label{eq:1}
 \frac{dN }{ d t}= C-C_{A} N^2-E N
 \,,
\end{equation}
where the terms on the right-hand side correspond to capture of WIMP inside the earth ($C$), annihilation in the core ($C_{A}$) and evaporation from its surface ($E$), respectively. In this work we neglect the
effect of evaporation from the earth assuming that it is not significant for reasonably heavy WIMP \cite{Spergel:1984re,Gould:1987ju,Krauss:1985aaa,Griest:1986yu}.
Each annihilation reduces the number of WIMP by two units and hence the rate of depletion of WIMP is twice the annihilation rate in the earth,
\begin{equation}\label{eq:4}
\Gamma_{A}=  \frac{1}{2} C_{A}N^2
\,.
\end{equation}
The quantity $C_{A}$ depends on $\langle\sigma_{A}v\rangle$ which is the total WIMP annihilation cross-section times the relative velocity of the WIMP.
Solving Eq.~(\ref{eq:1}) for $N$, we find the annihilation rate at any given time as,
\begin{equation}\label{eq:5}
    \Gamma_{A}=\frac{1}{2}C\tanh{^2}(t/\tau)
    \,,
\end{equation}
where $\tau=(CC_{A})^{-1/2}$ is the time required for equilibrium to be established between the capture and annihilation of WIMP in the earth. If $t \gg \tau$, equilibrium is seen to be established and we have $\Gamma_A = C/2$. Since the capture rate $C$ depends directly on the WIMP-nucleon scattering cross-section, we get a direct relation between the annihilation rate and the WIMP-nucleon scattering cross-section. However, for the case of the earth it is seen that equilibrium has not reached and hence there is no simple proportionality between the annihilation rate and WIMP-nucleon scattering cross section. Nevertheless, $t/\tau$ can be related to the capture rate $C$ and annihilation cross-sections $\langle \sigma_{A}v \rangle$ via the following relation:
\begin{equation}\label{eq:6}
   \frac{t_{\oplus}}{\tau_{\oplus}} = 1.9\times 10^{4} \bigg (\frac{C}{s^{-1}} \bigg)^{1/2} \bigg( \frac{\langle \sigma_{A}v \rangle}{cm^3 s^{-1}} \bigg)^{1/2} \bigg( \frac{m_{\chi}}{10GeV} \bigg)^{3/4}
\end{equation}
where $t = t_{\oplus} \sim 4.5 \times 10^{9}$ years is the age of the earth. For a fixed value of $\langle \sigma_{A}v \rangle$, $C_{A}$ is constant and a direct proportionality between $\Gamma_{A}$ and
$C$ can be established. Hence, the annihilation of WIMP in earth can be related to the
WIMP-nucleon scattering cross section. The scattering of the WIMP could proceed via both Spin Dependent (SD) and Spin Independent (SI) processes. The SI scattering cross-section depends on the number of nucleons present in the nucleus and hence is dominant for heavy nuclei. Since the earth comprises mainly heavy nuclei, the SI WIMP-nucleon scattering is dominant and is given by \cite{Gould:1991hx,Jungman:1995df}:
\begin{equation}
\label{eq:2}
 C = c \left(\frac{1~\textup{GeV}}{m_\chi}\right)
  \left( \frac{\rho_{local}}{0.3~ \textup{GeV}/\textup{cm}^{3}}  \right)  \left(\frac{270~ \textup{km}/\textup{s}}{\bar v_{\textup{local}}} \right) \sum_{i} F_{i}(m_{\chi})
  \sigma_{SI}^i f_{i}\phi_{i}\frac{S(m_{\chi}/m_{Ni})}{m_{Ni}/(1~{\rm GeV})}
 \,,
\end{equation}
where $c$ is a constant with value $4.8\times 10^{15}$ s$^{-1}$ for the case of earth and $m_\chi$ is the mass of WIMP.  $\rho_{local}$ and $\bar v_{\textup{local}}$ are the local DM density and velocity dispersion in the halo respectively. The summation in Eq.~(\ref{eq:2}) has to be carried out over all the nuclei in the earth where $F_i(m_\chi$) is the form-factor suppression for the capture of a WIMP of mass $m_\chi$ with the $i^{th}$ nucleus. For the $i^{th}$ nuclear species with mass $m_{N_i}$ (in GeV), $f_{i}$ and $\phi_i$ are its mass fraction and distribution in the earth respectively. $\sigma_{SI}^i$ is the cross-section for elastic scattering of the WIMP on $i^{th}$ nuclear species via SI interaction in units of $10^{-40}$ cm$^2$. For the capture of the WIMP on $i^{th}$ nuclei, $S(m_\chi / m_{N_i})$ gives the corresponding kinematic suppression factor. The cross-section for interaction of WIMP $\sigma_{SI}^i$ with $i^{th}$ nucleus can be related to WIMP-nucleon interaction cross-section $\sigma_{SI}$ by the following expression :
\begin{equation}\label{eq:7}
 \sigma^{i}_{SI} = \sigma_{SI} A^{2}_{i} \bigg( \frac{\mu_{\chi N_{i}} }{\mu_{\chi p}} \bigg)^{2}
\end{equation}
where for the $i^{th}$ nucleus: $A_i$ is the atomic number, $\mu$ is its reduced mass and $m_{N_{i}} \approx A_{i}m_{p}$, $m_{p}$ being the proton's mass. We assume here that proton mass to be equal to the neutron mass.
\begin{figure}[tbp]
\centering
\includegraphics[width=.75\textwidth,origin=c]{Plots/eps/EarthCapture.pdf}
\caption{\label{fig:1} SI capture rate for WIMP in the earth as a function of WIMP mass $m_{\chi}$. The enhanced capture rate due to resonance scattering on various nuclei is also shown.}
\end{figure}
The annihilation of WIMP produce standard model particle antiparticle pairs. Subsequently, hadronisation and/or decay of these pair products can give rise to neutrinos.
Due to WIMP annihilation in the earth, the differential neutrino flux arising at the detector is given by:
\begin{equation}
 \frac{dN_{\nu}'}{d\Omega dt dE_{\nu}} = \frac{\Gamma_{A}}{4\pi R^{2}} \sum_{j=1} {\rm BR}_j \frac{dN_{j}}{dE_{\nu}}
 \,,
 \label{diffflux}
\end{equation}
where $\Gamma_A$ and $C$ are related as discussed above, $R$ is the distance travelled by the neutrinos between the point of creation in the earth's core and detection at the detector. $dN_j/dE_\nu$ is the differential neutrino flux for a given WIMP annihilation channel $j$ such as $W^+W^-$, $b\bar b$, $c\bar c$, $\tau^{+}\tau^{-}$ etc. The sum in Eq.~(\ref{diffflux}), which is over all possible channels $j$, has to be weighted with the branching ratio ($BR_{j}$) of the particular channel $j$. Considering a generic WIMP scenario, we take one annihilation channel at a time and assume 100\% branching ratio for each of the channels. For a specific model predicting a different $BR_{j}$, the above fluxes would be simply mixture of different channels scaled linearly.\\\\
The annihilation of WIMP into standard model particle-antiparticle pairs in the centre of the earth, followed by the propagation of the produced neutrinos up to the detector is done using the WIMPSIM \cite{Blennow:2007tw,Edsjo:2007xyz} package. WIMPSIM uses Nusigma \cite{Edsjo:2007abc} for simulation of neutrino-nucleon interactions. For the hadronisation, decay and production of
neutrinos it uses PYTHIA \cite{Sjostrand:2006za}. We consider WIMP mass in the range $(10-100)$ GeV for both $b\bar ~b$ and $\tau^{+}\tau^{-}$ annihilation channels. The propagation of neutrinos through earth matter involves neutrino oscillations which has been incorporated in a full three flavour neutrino framework with the oscillation parameters given in Table~\ref{tab:1}. Throughout our analysis, we consider normal mass hierarchy. \\

\begin{table}[tbp]
\centering
\begin{tabular}{|lr|c|}
\hline
Paramter & Best-Fit Value\\
\hline
$\theta_{12}$ & $34^{\circ}$ \\
$\theta_{13}$ & $9.2^{\circ}$ \\
$\theta_{23}$ & $45^{\circ}$ \\
$\delta$ & $0$ \\
$\Delta m^2_{21}$ & $7.5\times 10^{-5} \textup{eV}^2$ \\
$\Delta m^2_{31}$ & $2.4\times 10^{-3} \textup{eV}^2$\\
\hline
\end{tabular}
\caption{Oscillation parameters used in the Simulation}\label{tab:1}
\end{table}

\begin{figure}[tbp]
\centering
\includegraphics[width=.85\textwidth,]{Plots/eps/EarthFluxes.pdf}
\caption{\label{fig:2} The $\nu$ and $\bar{\nu}$ fluxes at ICAL due to annihilation of 25 GeV WIMP in the earth for channels $b \bar{b}$ and $\tau^{+} \tau^{-}$ channel
with $\sigma_{SI}=10^{-38}$ cm$^{2}$ and $\langle \sigma_{A}v \rangle = 3 \times 10^{-26}$ cm$^3$ s$^{-1}$.}
\end{figure}
Fig.~\ref{fig:2} shows the neutrino and antineutrino fluxes (in units of GeV$^{-1}$m$^{-2}\Omega^{-1 }$s$^{-1}$) at ICAL due to WIMP annihilations in the earth.
For each of the annihilation channels, we assume 100 \% BR.  We take $ \rho_{\textup{local}} =0.3~ \textup{GeV}/ \textup{cm}^3$ and $v_{\textup{local}}= 270 ~\textup{km}~ \textup{sec}^{-1}$ in our flux calculations. The fluxes shown in Fig.~\ref{fig:2} are for 25 GeV WIMP assuming a WIMP-nucleon scattering cross section $\sigma_{SI}=10^{-38}$ cm$^{2}$. We can see from the figure that the fluxes for
both neutrinos as well as antineutrinos are nearly same, with antineutrino fluxes being slightly higher than the neutrino fluxes. This feature seems to hold for nearly all WIMP masses. The maximum kinematically possible energy of neutrinos produced from annihilation of WIMP is set by the WIMP mass i.e. for a WIMP mass of 25 GeV, the produced neutrinos will have energies in the range $(0-25)$ GeV.
For the $\tau^{+} \tau^{-}$ channel, the neutrino fluxes fall by about 1 order of magnitude in the above range. However, for the $b \bar{b}$ channel, the fluxes fall sharply by many orders of magnitude and well before $E_\nu = 20$ GeV it becomes negligible. Therefore, stronger indirect detection bounds are expected with neutrino fluxes from $\tau^{+} \tau^{-}$ channel in comparison to $b \bar{b}$ channel.
The fluxes arising due to annihilation channels involving the other quark-antiquark pairs are even weaker. Hence we do not consider those channels while discussing the expected sensitivity to indirect detection of dark matter in ICAL. The individual BR for a particular channel depends on a specific model considered. We, however, take a model-independent approach in this paper and quote the expected sensitivity limits for the $\tau^{+} \tau^{-}$ and $b \bar{b}$ channels with 100 \% BR each, as mentioned above. For a specific WIMP model, the flux with mixed BR for these channels will be between these extremes and hence the corresponding bounds. The Fig.~\ref{fig:2} show fluxes for benchmark values of WIMP mass and cross-sections. The fluxes for other values of $\sigma_{SI}$ can be obtained by simply scaling with the value of the cross-section. The above mentioned features of fluxes from various annihilation channels hold for all WIMP masses.
\section{Event generation at ICAL}\label{sec:event}
India-Based Neutrino Observatory (INO) is a proposed underground research facility to be built in Theni district of Tamil Nadu which is in the southern part of India. INO, among a few other experiments, will host be a 50 kt Iron CALorimeter (ICAL) detector. ICAL will have 150 layers of glass Resistive Plate Chambers (RPCs) as an active medium. Each of these RPC layers will have iron plates between them which will act as an interaction medium whereby the muon neutrinos will interact with iron and produce muons. These muons will leave long tracks. Since the iron in the detector will be magnetised, $\mu^{+}$ and $\mu^{-}$ will bend in opposite directions giving ICAL a capability of charge identification  \cite{Kumar:2017sdq}.
ICAL, with its excellent angular resolution of muons, can be used to put limits on the WIMP annihilation from the earth, competitive with other indirect searches.\\\\
GENIE \cite{Andreopoulos:2009rq}, suitably modified for our purpose, has been used for generating neutrino events with an ICAL geometry comprising 50 kt iron mass and 150 layers of glass RPCs. We use fluxes calculated by Honda et al. \cite{PhysRevD.83.123001} for Theni site for the simulation of atmospheric neutrino background. Signal calculation is done with the fluxes as prescribed in Section \ref{sec:capture}. Events are generated for a benchmark WIMP-nucleon cross-sections of $\sigma_{SI}=10^{-40} ~cm^{2}$, assuming 100 \% BR for each of the annihilation channel, and then scaled appropriately for other WIMP-nucleon cross-sections. \\\\
We generate the signal and background events separately. Subsequently, we pass them through our reconstruction code whereby ICAL energy and angle resolutions,
reconstruction and charge identification efficiencies are applied to get the final events at the detector. The muons, in our analysis, are binned in reconstructed energy and zenith angle bins. We perform detector simulations for ICAL geometry with Geant4 \cite{Agostinelli:2002hh} and obtain the muon reconstruction efficiency, muon charge identification efficiency, muon zenith angle resolution and muon energy resolution values. We tabulate these resolutions and efficiencies in a two dimensional table implying that the muon energy and angle resolutions are a function of both muon energy as well as muon zenith angle and are described in detail in our previous work \cite{Choubey:2017vpr}.
After incorporating the efficiencies and resolutions, the number of reconstructed $\mu^{-}$ events in the $ij^{th}$ bin are:
\begin{equation} \label{eq:3}
 N'^{th} _{ij} =  \mathcal{N} \sum_{k} \sum_{l} K^{k} _{i} (E^{k} _{T}) M^{l} _{j} (\cos{\Theta^{l} _{T}}) \left( \varepsilon_{kl} \mathcal{C}_{kl} n_{kl} (\mu^{-}) + \bar{\varepsilon_{kl}} (1-
 \bar{\mathcal{C}_{kl}}) n_{kl} (\mu^{+}) \right) \,,
\end{equation}
where $\mathcal{N}$ is the normalisation that we require for a given exposure in ICAL. The summation in Eq.~(\ref{eq:3}) is over true muon energy and true muon zenith angle bins and are indicated by indices $k$ and $l$, respectively. $E_{T}$ and $\cos{\Theta_{T}}$ are the true (kinetic) energy and true zenith angle of the muon, respectively, whereas $E$ and $\cos{\Theta}$ are the corresponding reconstructed (kinetic) energy and zenith angle of reconstructed of $\mu^{-}$. Using the reweighting algorithm prescribed in \cite{Ghosh:2012px}, the raw $\mu^{-}$ and $\mu^{+}$ events from GENIE are folded with the three-generation oscillation probabilities and subsequently binned in terms of muon energy and zenith angles. The subsequent number of $\mu^{-}$ and $\mu^{+}$ events, in the respective $k^{th}$ true energy and $l^{th}$ true angle bin, are denoted by the quantities $n_{kl}(\mu^{-})$ and $n_{kl}(\mu^{+})$. For the $k^{th}$ energy and the $l^{th}$ zenith angle bin, the quantities $\varepsilon_{kl}$ and $\bar\varepsilon_{kl}$ are the reconstruction efficiencies of $\mu^{-}$ and $\mu^{+}$, respectively, and $\mathcal{C}_{kl}$ and $\bar{\mathcal{C}}_{kl}$ are the corresponding charge identification quantities.
\begin{figure}[tbp]
\centering
\includegraphics[width=.75\textwidth]{Plots/eps/BkgWithoutCuts.pdf}
\caption{\label{fig:3} $\mu^{-}$ event distribution at ICAL due to atmospheric neutrino background for 50 $\times$ 10 kt-years of ICAL exposure. ICAL has zero efficiency for horizontal tracks which is reflected in the bins around $\cos\theta =0$. Note that in ICAL convention $\cos\theta = 1$ represents upward going muons.}
\end{figure}
The reconstruction efficiencies as well as the charge identification efficiencies are the functions of the true muon energy $E_{T}$ and true muon zenith angle $\cos{\Theta_{T}}$. The
Gaussian resolution functions $K^{k}_{i}$ and $M^{l}_{j}$ are used to apply muon energy and angle smearing respectively and are given as:
\begin{equation}
  K^{k} _{i}= \int _{E_{L_{i}}} ^{E_{H_{i}}} dE \frac {1} {\sqrt{2\pi}\sigma_{E}} \textup{exp} \left( -\frac {({E^{k}_{T}-E})^{2}} {2\sigma^{2}_{E}} \right)\,,
\end{equation}
\begin{equation}  f
 M^{l} _{j}(\cos_{\Theta_{T}^{l}})  = \int _{\cos{\Theta_{L_{j}}}} ^{\cos{\Theta_{H_{j}}}} d\cos{\Theta} \frac {1} {\sqrt{2\pi}\sigma_{\cos_{\Theta}}} \textup{exp} \left( -\frac
 {({\cos{{\Theta}^{k}_{T}}-\cos{\Theta}})^{2}} {2\sigma^{2}_{\cos_{\Theta}}} \right)\,.
\end{equation}
The values of $\sigma_{E}$ and $\sigma_{\cos{\Theta}}$ are as given in appendix of \cite{Choubey:2017vpr}. Similar expressions can be written for the $\mu^+$ events and  $N'^{th}_{ij}(\mu^{+})$. All analysis in this work is done for 10 years of ICAL running.

\section{Atmospheric neutrino background suppression}
\label{sec:background}
The major source of background to the indirect searches from WIMP annihilation in the earth is due to the atmospheric neutrinos. However, unlike the neutrinos from WIMP annihilation which come from the direction of the earth core, the atmospheric neutrinos have a distribution over all zenith and azimuth angular bins and is comparatively well studied. We can exploit this feature and use it to suppress the atmospheric background considerably. Other source of neutrinos such a geothermal neutrinos coming from the core direction are in the MeV range and hence are not relevant here. The signal neutrinos, for the case of WIMP annihilation in the earth, will come from the direction of earth core. The signal search region for the WIMP annihilation in the earth is shown in Figure~\ref{fig:4}. These neutrinos on reaching ICAL will interact with the detector iron through charge current interaction and produce charged leptons, muons being the lepton of interest for ICAL. The scattered muon will make an angle ($\theta_{\nu \mu}$) with their parent neutrino, where ($\theta_{\nu \mu}$) is a function of parent $\nu$ energy and detector medium. Due to finite detector resolution there will be smearing effects. However, we choose to work with true muon direction rather than the reconstructed muon direction at the stage of background suppression. ICAL has an excellent muon angle resolution \cite{Choubey:2017vpr} for the considered energy range and hence this choice will not affect the final results significantly.\\\\
\begin{figure}[tbp]
\centering
\includegraphics[trim=10 10 10 10,clip,width=.45\textwidth]{Plots/eps/ConeCutEarth_v2.pdf}
\caption{\label{fig:4}  The cone regions where signal from the WIMP annihilations are expected for the earth.}
\end{figure}
We define $\theta_{90}$ to be the half angle of the cone that contains 90\% of the signal muons, the axis of the cone being in the direction of the earth's core. Harder channels like $\tau^{+} \tau^{-}$ with higher energy neutrinos will have a narrower $\theta_{90}$ in comparison to softer channels like $b \bar{b}$ with lower energy neutrinos which will have a broader $\theta_{90}$. Likewise, we expect that the $\nu$ spectra from annihilation of massive WIMP to have most of the associated muons in a narrower cones than neutrinos by lighter WIMP. Also, the heavier the WIMP, the closer it is to the centre of the earth and hence smaller cone opening. Using WIMPSIM and GENIE, we estimate $\theta_{90}$ for each WIMP mass and for a given annihilation channel. Figure~\ref{fig:5} shows the $\theta_{90}$ obtained for WIMP annihilation inside earth, as a function of WIMP mass ($m_{\chi}$), and for different annihilation channels.\\
\begin{figure}[tbp]
\centering
\includegraphics[width=.85\textwidth,origin=c]{Plots/eps/ConeCutEarth.pdf}
\caption{\label{fig:5} 90 \% cone cut values obtained for the earth. This is obtained using WIMPSIM and GENIE. A cone angle is estimated such that it contains 90\% of the signal events. The solid lines correspond to neutrinos and dashed lines correspond to anti-neutrinos for each of the annihilation channel.}
\end{figure}
\begin{figure}[tbp]
\centering
\includegraphics[width=.75\textwidth]{Plots/eps/EarthEvents.pdf}
\caption{\label{fig:8} Angular probability distribution of reconstructed $\mu^{-}$ at ICAL due to WIMP annihilations in the earth. A comparison for three WIMP masses has been shown and the region where signal is expected is marked. The probability distribution for the unsuppressed atmospheric background is also shown.}
\end{figure}

\begin{figure}[tbp]
\centering
\includegraphics[width=.45\textwidth,]{Plots/eps/Events5214GeV-ch5-ea.pdf}
\hfill
\includegraphics[width=.45\textwidth,origin=c]{Plots/eps/Events5214GeV-ch11-ea.pdf}
\caption{\label{fig:9} Muon event distribution at ICAL due to atmospheric neutrinos and signal neutrinos arising out of a WIMP annihilations in the earth. The plots are for fluxes arising due
to SI capture rate. A cross-section of $\sigma_{SI} =10^{-40} cm^{2}$ has been assumed for the signal neutrinos. The left plot is for the WIMP annihilating into the channel $b \bar{b}$ while
the right plot is for the annihilation channel $\tau^{+} \tau^{-}$. A 100 \% branching ratio has been assumed for each of the channels. Also shown are the corresponding events coming from the atmospheric
background after applying the suppression scheme as described in \ref{sec:background}. Atmospheric events have been simulated using Honda fluxes at Theni \cite{Honda:2015fha}.
The softer channel $b \bar{b}$ has more background than the harder channel $\tau^{+} \tau^{-}$.}
\end{figure}
The atmospheric neutrino background is then suppressed as follows. For each WIMP mass and annihilation channel, we accept only those muons whose zenith angle are within $\theta_{90}$ with respect to the earth core. These atmospheric background events that fall within this cone represents an irreducible background for we can not distinguish them from the neutrinos due to WIMP annihilation in the core. After applying this suppression scheme, we fold the background events with detector resolution and efficiencies as described in the previous Section~\ref{sec:event} to obtain the final reconstructed and suppressed background events which are then used for $\chi^{2}$ analysis.\\\\
Figure~\ref{fig:8} shows the angular probability distribution of $\mu^{-}$ due to WIMP annihilations in the earth for the $\tau^{+} \tau^{-}$ channel along with the distribution of the (unsuppressed) atmospheric background muon events at ICAL. A comparison for three WIMP masses $5$, $50$ and $100$ GeV has been shown. The above probability distribution, for each of the WIMP mass, has been obtained by normalising the reconstructed $\mu^{-}$ events in each bin by total number of reconstructed $\mu^{-}$ events for that WIMP mass. It can be noted that as WIMP mass increases, the angular probability distribution peaks towards the direction of the core. This is expected because of the reasons discussed above. The signal search is carried out in the region right of the vertical line represents $\theta_{90}$. We draw a line at $\sim 30^{\circ}$ from the earth centre $(\cos\theta=1)$ just for illustration. The actual values of $\theta_{90}$ for each WIMP mass and channel is taken from Figure~\ref{fig:5} while doing the analysis. Fig.~\ref{fig:9} shows the signal events due to a 52.14 GeV WIMP annihilating through $\tau^{+} \tau^{-}$ and $b \bar{b}$ channels. Also shown are corresponding suppressed atmospheric background events.

\section{The statistical analysis}
\label{sec:analysis}
We estimate the 90 \% C.L. sensitivity limits on SI WIMP-nucleon cross-sections through a $\chi^{2}$ analysis. In our analysis, we generate prospective data at ICAL comprising atmospheric background events only. To this `data', we fit our hypothesis in which we consider combined events predicated at ICAL due to WIMP annihilation in the earth and atmospheric neutrino background. This choice is consistent with `no WIMP scenario' in the data and hence the limits calculated are the expected exclusion limits in the WIMP mass - WIMP SI cross-section plane from 10 years of running of ICAL.

We combine the $\mu^{+}$ and $\mu^{-}$ events while performing $\chi^2$ analysis.
A $\chi^2$ function is defined as
\begin{equation}
 \chi^2 = \chi^2(\mu^-) +  \chi^2(\mu^+)
\end{equation}
where
\begin{equation}
\chi^2(\mu^\pm) = \min_{\xi^\pm_k}\sum_{i=1}^{N_i}\sum_{j=1}^{N_j}
\bigg [ 2\bigg(N_{ij}^{\rm th}(\mu^\pm) - N_{ij}^{\rm ex}(\mu^\pm)\bigg ) +
2N_{ij}^{\rm ex}(\mu^\pm)\ln\bigg(\frac{N_{ij}^{\rm ex}(\mu^\pm)}{N_{ij}^{\rm th}(\mu^\pm)}
\bigg ) \bigg]
+ \sum_{k=1}^l {\xi^\pm_k}^2
\,,
\end{equation}
\begin{equation}
N_{ij}^{\rm th}(\mu^\pm) = {N'}_{ij}^{\rm th}(\mu^\pm)\bigg(1+\sum_{k=1}^l \pi_{ij}^k{\xi^\pm_k}\bigg)
+{\cal O}({\xi^\pm_k}^2)\,,
\end{equation}
where ${N'}_{ij}^{\rm th}(\mu^\pm)$ are the $\mu^\pm$ events that we `predict' and $N_{ij}^{\rm ex}(\mu^\pm)$ are the events `observed' at ICAL. For $k^{th}$ systematic uncertainty we have associated $\pi_{ij}^k$ correction factors with $\xi^\pm_k$ being the corresponding pull parameters. Similar to our previous analysis \cite{Choubey:2015xha}, we include 5 systematic errors as follows. We take 20~\% error on neutrino flux normalisation and 10~\% error on neutrino-nucleon cross-section. On the zenith angle distribution of atmospheric neutrino fluxes, we include a 5~\% uncorrelated error and 5~\% tilt error. Finally, we take a 5~\% overall error to account for detector systematics.
Minimisation over the pull parameters gives the individual contributions from $\mu^-$ and $\mu^+$ data samples. Thereafter, we add them up and calculate the $\chi^2$ for a given set of WIMP mass and WIMP-nucleon cross-sections.
\section{Results}
\label{sec:results}
\begin{figure}[tbp]
\centering
\includegraphics[width=.65\textwidth]{Plots/eps/SigmaVLimits.pdf}
\caption{\label{fig:10} The expected 90 \% C.L. sensitivity limits on $\sigma_{SI}$ for ICAL as a function of annihilation cross-section $\langle \sigma_{A}v\rangle$ for a $50 GeV$ WIMP annihilating through  $\tau^{+}$ and $\tau^{-}$ (red solid) and $b ~\bar{b}$ (red dashed). Also shown are upper limits at 90 \% C.L obtained by various experiments IceCube \cite{Aartsen:2016fep} $\tau^{+}$ and $\tau^{-}$ (green), ANTARES\cite{Albert:2016dsy} $\tau^{+}$ and $\tau^{-}$ (cyan), $b ~\bar{b}$ (light purple), $\nu_{\mu}\bar\nu_{\mu}$ (blue) and LUX\cite{Akerib:2016vxi} (black-dashed) have been shown for comparison.
For ICAL, systematics have been included.}
\end{figure}

\begin{figure}[tbp]
\centering
\includegraphics[width=.85\textwidth]{Plots/eps/INO-EarthLimits.pdf}
\caption{\label{fig:15} The expected 90\% C.L. sensitivity limits on $\sigma_{SI}$ as a function of WIMP mass, assuming a WIMP annihilation cross section
$\langle\sigma_{A}v\rangle= 3\times 10^{-26} cm^{3}s^{-1}$. The displayed sensitivity limits are for the local dark matter density $\rho =0.3 GeV cm^{-3}$. Among the indirect detection experiments,
ICAL provides the most stringent bound. The dip around 50 GeV in the limits obtained for Earth WIMP annihilation is a prominent feature in all experiments and is due to
resonant capture of WIMPs on Fe. ICAL 90\% C.L. sensitivity limits for $\tau^{+}$ and $\tau^{-}$ (red solid) and $b ~\bar{b}$ (red dashed) for WIMP annihilation in the Earth are shown; 90\% C.L. upper limits from SK\cite{Desai:2004pq} for $\tau^{+}$ and $\tau^{-}$ (brown), IceCube\cite{Aartsen:2016fep} $\tau^{+}$ and $\tau^{-}$ (blue) and ANTARES \cite{Albert:2016dsy}
$\tau^{+}$ and $\tau^{-}$ (black). Also, shown are the limits obtained from DARKSIDE \cite{Agnes:2014bvk} (dark green dotted), LUX (cyan), XENON-1T \cite{Aprile:2017iyp} (brown) and PANDA\cite{Tan:2016zwf} (light green dotted).}
\end{figure}

\begin{figure}[tbp]
\centering
\includegraphics[width=.85\textwidth]{Plots/eps/AnnihilationLimits.pdf}
\caption{\label{fig:11} The expected 90\% C.L. sensitivity limits on the annihilation rate ($\Gamma_{A}$) as function of WIMP mass ($m_{\chi}$) due to WIMPS annihilating into $\tau^{+}$ $\tau^{-}$
(red solid) and $b ~\bar{b}$ (red dashed) with 100\% branching ratio each. The limits are for 10 years of ICAL running. For comparison limits from various other experiments have been shown:
ANATARES\cite{Albert:2016dsy} $\tau^{+}$ $\tau^{-}$ (blue), $b ~\bar{b}$ (cyan), $\nu_{\mu}\bar\nu_{\mu}$ (black) , and IceCube\cite{Aartsen:2016fep} $\tau^{+}$ and $\tau^{-}$ for
$m_{\chi} <50 GeV$ and $W^{+} W^{-}$ for $m_{\chi} >50 GeV$ (green). We show these limits for a fixed $\langle\sigma_{A}v\rangle = 3 \times 10^{-26} cm^{3} s^{-1}$.}
\end{figure}

\begin{figure}[tbp]
\centering
\includegraphics[width=.85\textwidth]{Plots/eps/ICAL-Systematics.pdf}
\caption{\label{fig:12} The expected 90\% C.L. sensitivity limits for WIMP annihilation for different masses and two annihilation channels for WIMP annihilation in the earth are shown. The solid lines are the sensitivity limits calculated using detector systematics as described in Sec~\ref{sec:analysis}. The corresponding dotted lines are without systematics. The expected sensitivity limits for $\tau^{+}$ and $\tau^{-}$ are shown in red (with systematics) and orange-dotted lines (without systematics) and for $b ~\bar{b}$ in blue (with systematics) and azure-dotted lines (without systematics). The effect of systematics, as we expect, is to worsen the limits as expected.}
\end{figure}

We present the main results in this section. As mentioned in Section~\ref{sec:capture}, for the case of WIMP annihilation in the earth, the spin-independent WIMP nucleon cross sections $\sigma_{SI}$ and annihilation rate $\Gamma_{A}$ are related by Eq.~(\ref{eq:4}-\ref{eq:6}). The capture rate and the annihilation rate are not in equilibrium, and hence the annihilation rate depends on the $\sigma_{SI}$ as well as on the annihilation cross section $\langle\sigma_{A}v\rangle$. Figure~\ref{fig:10} shows our expected sensitivity upper limits at 90 \% C.L. in the $\sigma_{SI}$ - $\langle\sigma_{A}v\rangle$ plane for a WIMP mass of $50$ GeV. As shown in Figure~\ref{fig:1}, the capture rate for the WIMP masses closer to iron mass is greatly enhanced and hence we expect stronger bounds. It is evident that for a $50$ GeV WIMP, ICAL seems to put a stronger bound on $\sigma_{SI}$ for a given $\langle\sigma_{A}v\rangle$ for a given annihilation channel such as $\tau^{+}$ $\tau^{-}$. For the obvious reasons, described in earlier sections, the harder channel $\tau^{+}$ and $\tau^{-}$ gives a stronger limit in comparison to the softer channel $b ~\bar{b}$.\\\\
In Figure~\ref{fig:15} we present the expected 90 \% C.L. sensitivity limits on the WIMP-nucleon SI interaction cross-section as a function of WIMP mass for $500$ kt-years of ICAL exposure and compare it with the exclusion limits obtained from various other direct and indirect detection experiments. The direct detection experiment XENON-1T \cite{Aprile:2017iyp} gives the most stringent bound till date. Bounds from indirect searches are, in general, weaker in comparison to direct detection experiments. However, among the neutrino detectors, ICAL seems to give the most stringent bound for the chosen WIMP mass range. For the WIMP masses close to iron mass, there is a resonant capture and hence enhance event rates resulting in a stronger bound. \\\\
For calculating sensitivity limits on annihilation rate and $\sigma_{SI}$ in case of the earth, we assume an annihilation cross-section $\langle\sigma_{A}v\rangle =3 \times 10^{-26} cm^{3}s^{-1}$. As discussed in Section~\ref{sec:capture}, we have a relation between the annihilation rate $\Gamma_{A}$ and SI WIMP-nucleon cross-section $\sigma_{SI}$. Using the $\chi^{2}$ analysis described in Section~\ref{sec:analysis}, we derive limits on the $\sigma_{SI}$ as a function of WIMP mass $m_{\chi}$. Using Eq.~(\ref{eq:4}-\ref{eq:6}) from Section~\ref{sec:capture}, we transported these sensitivity limits from $\sigma_{SI} -m_{\chi} $ plane to $\Gamma_{A} -m_{\chi} $ plane. Figure~\ref{fig:11} shows the expected sensitivity limits at 90 \% C.L. calculated on the WIMP annihilation rate for annihilation in the earth through channels $\tau^{+}$ and $\tau^{-}$ and $b ~\bar{b}$. Results from other experiments are also shown for comparison\footnote{For SK latest preliminary results please see \cite{Frankiewicz:2017trk}.}. Again, we can see that for chosen WIMP mass range, ICAL presents a stronger bound on the WIMP annihilation rate for a given channel. Again, $\tau^{+}$ $\tau^{-}$ bounds are stronger than that of $b ~\bar{b}$. \\\\
Finally, in Figure~\ref{fig:12} we present the effect of systematic uncertainties on the expected 90 \% C.L. sensitivity limits on the WIMP-nucleon SI interaction cross-section. The dashed lines are the limits calculated while taking only statistical uncertainties. As expected, the effect of systematic uncertainties is to worsen the limits as can be seen from the figure.

\section{Summary}
\label{sec:summary}
The analysis presented in this work is a part of ongoing studies to probe the physics potential of the upcoming ICAL detector. Neutrinos arising out of WIMP annihilations in the earth could be used to probe dark matter signatures. Such searches would be complementary to direct searches for WIMP. We presented a study of prospects of detecting muon events at ICAL arising due to WIMP annihilation in the earth for $ \tau^+ \tau^- $ and $ b~\bar b$ annihilation channels. Employing an effective atmospheric background suppression scheme, the expected 90~\% C.L. sensitivity limits obtained for SI WIMP-nucleon cross-section for the case for the earth is better than any other indirect detection experiment.
\acknowledgements
We gratefully acknowledge INO collaboration for the support. We sincerely thank Amol Dighe for intensive discussions. We acknowledge the HRI cluster computing facility (http://cluster.hri.res.in). The authors would like to thank the Department of Atomic Energy (DAE) Neutrino Project under the XII plan of Harish-Chandra Research Institute. This project has received funding from the European Union's Horizon 2020 research and innovation programme InvisiblesPlus RISE under the Marie Sklodowska-Curie grant agreement No 690575. This project has received funding from the European Union's Horizon 2020 research and innovation programme Elusives ITN under the Marie Sklodowska- Curie grant agreement No 674896. This project has received funding from FONDECYT 3170845 (Chile).
\bibliographystyle{JHEP}

\section{User documentation}

This package provides a way to check if a document is being processed with \XeTeX. It may be loaded with

\bigskip
\begin{tabular}{l@{\quad}l}
{|\usepackage{ifxetex}|} & for \LaTeX, or \\
{|\input ifxetex.sty|} & for Plain \TeX.
\end{tabular}
\bigskip

\noindent
This defines the conditional \cmd\ifxetex\ that is used in the standard way:

\bigskip
|\ifxetex|\par
\hspace{2em}\meta{material for \XeTeX}\par
|\else|\par
\hspace{2em}\meta{material not for \XeTeX}\par
|\fi|
\bigskip

\noindent
Users of \LaTeX's \pkg{ifthen} package can also use it as |\boolean{xetex}|:

\bigskip
|\ifthenelse{ \boolean{xetex} }{|\texttt{\char`\%}\par
\hspace{2em}\meta{material for \XeTeX}\par
|}{|\texttt{\char`\%}\par
\hspace{2em}\meta{material not for \XeTeX}\par
|}|
\bigskip

\noindent
Finally, this package also defines the |\RequireXeTeX| command,
which tests for \XeTeX\ use and throws an error if a different engine
is being used. This is used for packages like \pkg{fontspec} that take
advantage of \XeTeX's new features and cannot be used otherwise.

\clearpage
\parindent=0pt
\section{Implementation}
\DocInput{ifxetex.sty}

\end{document}

redpajama_set_name: RedPajamaArXiv


I've wanted a dress form for years. They are expensive new and awkward and pricey to ship. I came across an idea online (here) on how to make your own. I blended two of their ideas together. I made a shell on myself out of duct tape (taping over a dress I didn't mind cutting up), cut up the front, took it off, and duct taped it back together. Then I put a first layer of paper mache. The beginning stage is pictured above.
I still need to put more layers of paper mache on. It's not perfect, but still should be great for sewing...it only cost me $4..the cost of the duct tape!


A land of rugged hills and deeply cut canyons with clear streams running over beds of solid limestone, the Hill Country is rich in regional species, from Sycamore-Leaf Snow Bell and Texas Barberry to Canyon Mock-Orange and Scarlet Leatherflower.
In the classic reference Wildflowers of the Texas Hill Country , Austin conservationist Marshall Enquist provides detailed descriptions and color illustrations of 427 wildflower species. Broad in scope, the book covers everything from the smallest meadow flowers to the largest flowering trees and shrubs.
A comprehensive guide to the flora of one of Texas' most beautiful regions, Enquist subdivides and provides brief explanations of three geological areas within the Hill Country: the Edwards Plateau, the Lampasas Cut Plains, and the Llano Uplift and the indigenous species of wildflowers that thrive in each locale.


'Seeking Infinity' released and new website launched!
Today, Pantheist has released its fifth full-length album, and first release in seven years, 'Seeking Infinity'. The album is a decisive return to the band's funeral doom roots, whilst still incorporating the atmospheric and progressive elements that have become an integral part of Pantheist's sound over the years. Comprising of six tracks and clocking in at just over 60 minutes, 'Seeking Infinity' is available on digipack CD from the band's own label Melancholic Realm Productions for £15 (including all postage costs) via the Merchandise page, and on doublefold 2xLP from the Spanish label The Vinyl Division.
In addition, 'Seeking Infinity' is available to listen to and purchase digitally on Bandcamp, and you can also order it on iTunes, or stream it on Spotify. People who buy the digital album on Bandcamp, as well as those subscribed to our mailing list will get the bonus track 'Warping Space-Time' for free. It can also be downloaded separately from Bandcamp (by subscribing to our mailing list as well). You can find out more about 'Seeking Infinity' on the Discography page, and check out the latest reviews of it on the Media page.
As you can see, to coincide with the release of the new album, we have also launched a new official Pantheist website! More content will continue to be added to the site in the coming weeks and months, so stay tuned for future updates. Finally, don't forget to sign up to the Pantheist mailing list if you would like to be the first to receive the latest news from the band in the future!


Villaviciosa de Odón is a municipality in the wastren zone o the Commonty o Madrid in Spain. The veelage is locatit 15 km wast Madrid's ceety centre, in the wastren zone o the metro aurie. Locatit athin the ceety is the Spainyie Air Force Museum an the Universidad Europea de Madrid.
Villaviciosa's quiet lifestyle an its proximity tae Madrid propitiatit rapid an extensive development durin the late 1990s an early 2000s. Acause o its proximity tae the Universidad Europea de Madrid, it haes become a varsity ceety, wi well-developed residential aurie an amenities for students. The toun conteens the Castle of Villaviciosa de Odón.
This page wis last eeditit on 11 Mairch 2018, at 11:22.


text:
lsu coach divorce rumors
Ed, 58, filed a divorce petition on Feb. 26 in East Baton Rouge Parish Family Court, according to the Baton Rouge Advocate.
SEC coach to film a PSA about coronavirus. Text us for exclusive photos and videos, royal news, and way more. Gave LSU Players Real Cash After National Championship Win, Joe Burrow Says.
All rights reserved (About Us). "Coach O" led the Tigers to a national championship in January and was named the AP Coach of the Year shortly after.
In the divorce filing, Orgeron says he wants exclusive use of the couple's home in Baton Rouge ... and claims to have no objection to letting Kelly have their house in Mandeville, La. LSU won the National Championship earlier this year. Louisiana State University football coach Ed Orgeron has reportedly filed for divorce from his wife Kelly after 23 years of marriage. Stay up to date on the latest vote tallies as compiled by The Associated Press' nationwide team, Princess Diana died when Harry was just 12 years old, The Sweetest Photos of Princes Harry with Diana, First-Time Voters Across the Country Share Why the 2020 Election Matters to Them. Louisiana State University football coach Ed Orgeron has reportedly filed for divorce from his wife Kelly after 23 years of marriage. The two had reportedly met on a blind date in 1996 ... and were married shortly after on Feb. 19, 1997, the docs say. If you would like to opt out of browser push notifications, please refer to the following instructions specific to your device and browser: LSU Football Coach Ed Orgeron Files for Divorce from Wife of 23 Years: Report. Note to readers: if you purchase something through one of our affiliate links we may earn a commission. Credit: In fact, the two were inseparable during Orgeron's victory celebration over Clemson on Jan. 13, sharing kisses and hugs as confetti rained down at the Superdome. Ed Missed the Birth of Their Twin Sons, Cody & Parker, Due to His Coaching Duties.
LSU Tigers football coach Ed Orgeron has filed for a divorce from his wife of 23 years, according to documents filed in February. until court proceedings mete out their situation. Ed Orgeron Filed for Divorce 1 Month After Signing $42 Million Contract at LSU.
LSU head football coach Ed Orgeron had one heck of a start to 2020. Ed Orgeron, a day after the SEC all on-campus events, practices and recruiting were suspended due to COVID-19, was the first SEC coach to film a PSA about coronavirus. All three boys share a love of football with the collegiate coach. Shortly after securing the victory, and accepting the Eddie Robinson Coach of the year award, it was confirmed that Ed had signed a new $42 million contract. Follow him on Twitter @Mark_Heim. — The Advocate (@theadvocatebr) April 2, 2020. "He has proven that he is not only a championship coach, but also a leader of a program committed to doing things the right way.". Get TMZ breaking news sent right to your browser! Orgeron filed the divorce Feb. 26 in East Baton Rouge Parish Family Court, per the report, stating he and his wife, Kelly, separated Feb. 24 "and have lived separate and apart without reconciliation since that date.", In the filing, the coach states he is entitled "to have the exclusive use and occupancy" of the couple's house in Baton Rouge. In the court documents, Ed said he wanted the exclusive use of the home they previously shared in Baton Rouge, and had no objection to Kelly being granted the exclusive use of another Louisiana home "until such time as the community property is settled either by conventional agreement or judicial partition," the outlet reported. Cody, a senior at McNeese State, is expected to return next year as the starting quarterback, and his brother served as a student assistant there last season, previously playing as a wide receiver. ALL RIGHTS RESERVED, Download the TMZ App on the Apple App Store, Download the TMZ App on the Google Play Store. Waiting for your permission to load the comments. LSU head coach Ed Orgeron, seen here with his wife Kelly celebrating after a win against Alabama in 2019 in Tuscaloosa, has filed for divorce after 23 years. Getty Composite Ed Orgeron is calling things off with his wife, Kelly... the LSU head coach filed for divorce a little more than a month after he led the Tigers to a National Championship. The couple has three sons, according to the Advertiser.
The 58-year-old filed the court docs in Louisiana back on Feb. 26, according to The Advocate ... and in them, he says he and Kelly officially split on Feb. 24.
Back in February, it was reported that the LSU football coach filed for divorce from his wife after 23 years of marriage. MORE: https://t.co/wCZIOmI8iZ. Orgeron had praised Kelly several times during LSU's championship run this past winter ... and had called her an inspiration multiple times in the years leading up as well.
White Crane Spiritual Meaning, Big Movie Ending Scene, Sceptre Z27 Monitor, Naval Observatory Time Hack, Strange Days (1995) 123movies, Brea Beal Parents, Quinone Vs Quinine, Boplicity Miles Davis Analysis, Devin White Parents, Knock On Wood Emoji, 667 Triangle écriture, Riverside County Probation Corrections Officer Practice Test, Richland Mall Sc, Anime Fortnite Creative Code, Welcome Home Bendy Roblox Id, Swallow The Air Essays, Is Italy Bigger Than Uk, Rêver De Chuchoter à Loreille Islam, Descendants Of Bernard Kroger, Sims 4 Superman, Comment Localiser Sa Nintendo Switch Perdu, Csgo Case Drop Rotation 2020, Alina Kabaeva Child, Reckoning Season 1 Netflix, Yamaha R6 Rear Shock Length, Physics Slope Calculator, Dark Night Of The Soul Twin Flame, 13 Ways Of Looking Perspective, Hershesons Almost Everything Cream Stockist, Harvey Specter Pen, Restaurant Grillades Laval, Feminine Wiles Reddit, Where Are Goodr Sunglasses Made, Mini Pc Ubuntu, My Soul Is At Rest Lyrics, Manchester Terrier For Sale Uk, Ice Breakers Mints Side Effects, Sarah Huffman Nike, Is Baileys A Fortified Wine, Troy Landry Sons, Playtone Productions Email Address, Modern Cat Tree Uk, Does Kissasian Have Viruses, Human Hearing Range, Who Is Holly Hamilton Mother, Fortnite Og Skins Recon Expert, John Woods Age, Bosch 500 Series Hmb5051, David Baker Forged In Fire Tattoo, Ascendant Argentavis Saddle Blueprint, What Is Needed To Pass Smog In California, Abyss Watchers Cheese, Tdr Capital Salary, Charleston Rambo Father, Elevation Map Ontario, Judge Emmet Sullivan Son, What Are The 7 Continents From Largest To Smallest, Audi Tdi Forums, Invader Movie 2020, How To Find People On Onlyfans, Oh Please Lyrics Sl, Steve Jobs Wife Yacht, Ron Tyson Net Worth, Is Whitney Cummings Vegan, Does Bryshere Gray Have Siblings, Clemson Fraternities Reputations, Faltu Full Movie 123movies, 2006 Chevy Silverado Wheel Hub Torque Specs, Alan Lee Beyblade, Cataraqui Golf And Country Club Menu, Nabhaan Rizwan Agent, Korean Short Stories Pdf, Polish Mp5 Gas Mask Filter, Anna Roisman Necklace,
lsu coach divorce rumors 2020


text:
We are monitoring the impact of COVID-19 on Latin America Hyaluronic Acid Products Market Get in touch with us for detailed analysis Know More
Latin America Hyaluronic Acid Products Market
Latin America Hyaluronic Acid Products Market Rese . . . .
Latin America Hyaluronic Acid Products Market Research Report – Segmented By Product type, Application and Country (Brazil, Argentina, Chile, Mexico and Rest of Latin America) – Industry Size, Share, Trends and Growth Forecast (2021 to 2026)
Latin America Hyaluronic Acid Products Market Size (2021 to 2026)
The size of the Hyaluronic Acid Products Market in Latin America was around USD 0.82 Billion in 2021. It is expected to grow at a CAGR of 6.93% to reach USD 1.15 Billion by 2026.
The growing aging population is particularly vulnerable to incontinence, bone injuries, and fractures; hence the hyaluronic acid market caters to them. In Latin America, the aging or geriatric population is one of the essential hyaluronic acid-based products. In addition, manufacturers are developing hyaluronic acid-based supplements and injectables in response to the rising number of people with osteoporosis and rheumatoid arthritis. As a result of the increasing number of cases of bone and joint problems, the Latin American market for hyaluronic acid is expected to increase significantly during the forecast period.
Consumers have shifted toward the notion that prevention is better than cure as the frequency of lifestyle-related disorders has increased, driving the Latin American hyaluronic acid products market, particularly in sectors such as dietary supplements for joint health. The rise in chronic diseases and the rise in the cost of healthcare services are projected to drive the growth of the hyaluronic acid market during the forecast period. Furthermore, minimum surgical treatments and increased understanding of beauty and health are two elements that move the hyaluronic acid market forward. The increased use of hyaluronic acid in the cosmetics industry is fueling the market's expansion.
However, in countries such as Mexico and Brazil, the lack of competent specialists and the lack of dermal products limit the expansion of hyaluronic acid products. In addition, the hyaluronic acid market is expected to be hampered by adverse effects connected with treatment or therapy, such as redness and itching and an increase in the price of hyaluronic acid products during the forecast period.
Complications such as skin disorders, arthritis, inflammatory diseases, and ocular ailments become more common as people age. As a result, medicine for treating these indications has been in great demand among the greying population. In addition, hyaluronic acid products are an essential component in pain management and moisture restoration therapy for dry eyes and other conditions.
This research report on the Latin American hyaluronic acid products market has been segmented and sub-segmented into the following categories:
Latin America accounts for a moderate share of the worldwide hyaluronic acid market because of the thriving healthcare industry and rising awareness in emerging markets. In terms of innovation and product availability, the cosmetics sector in Mexico and Brazil is one of the most developed and mature. Furthermore, demand from the country's changing demographics is predicted to fuel the expansion of the hyaluronic acid products market by integrating its presence across various skin-related products. The anti-aging segment is projected to drive the hyaluronic acid market in Mexico. Gen Xers are looking for ageless items since they have the financial means to invest in a dependable solution for long-term use.
Throughout the forecast period, the rapid adoption of new skincare treatments and technologies will fuel the expansion of the hyaluronic acid market in the area. Because of the growing older population in Latin America, the hyaluronic acid industry is expected to increase significantly. Furthermore, the rising prevalence of osteoarthritis and ongoing improvements in healthcare facilities are expected to drive the hyaluronic acid market in the region to new heights in the coming years. Individual market affecting factors and changes in market regulation that impact present and future market trends are also provided in the nation section of the hyaluronic acid market analysis.
A few of the key companies operating in the Latin American hyaluronic acid products market are Allergan, Sanofi, Ferring B.V., Zimmer Biomet, Fidia Farmceutici, Salix Pharmaceutical, Anika Therapeutics, Seikagaku Corporation, Hoffmann-LA Roche Ltd, Alcon, Inc., Smith & Nephew plc and F.Merz Asthetics, Inc.
6.2 Brazil
6.4 Rest of Latin America
9.Competitive Landscape
10.Market Outlook and Investment Opportunities
Segment-level analysis in terms of Product Type, by Application along with market size forecasts and estimations to detect key areas of industry growth in detail
Latin America Hyaluronic Acid Products Market, By Product Type, From 2021 to 2026 (USD Million)
Latin America Single cycle injection products Market, By Region, From 2021 to 2026 (USD Million)
Latin America Three cycle injection products Market, By Region, From 2021 to 2026 (USD Million)
Latin America Five cycle injection produtcs Market, By Region, From 2021 to 2026 (USD Million)
Latin America Hyaluronic Acid Products Market, By Application, From 2021 to 2026 (USD Million)
Latin America Osteoarthritis Market, By Region, From 2021 to 2026 (USD Million)
Latin America Ophthalmic Market, By Region, From 2021 to 2026 (USD Million)
Latin America Dermal Fillers Market, By Region, From 2021 to 2026 (USD Million)
Latin America Vesicoureteral Reflux Market, By Region, From 2021 to 2026 (USD Million)
Brazil Hyaluronic Acid Products Market, By Product Type, From 2021 to 2026 (USD Million)
Brazil Hyaluronic Acid Products Market, By Application, From 2021 to 2026 (USD Million)
Argentina Hyaluronic Acid Products Market, By Product Type, From 2021 to 2026 (USD Million)
Argentina Hyaluronic Acid Products Market, By Application, From 2021 to 2026 (USD Million)
Mexico Hyaluronic Acid Products Market, By Product Type, From 2021 to 2026 (USD Million)
Mexico Hyaluronic Acid Products Market, By Application, From 2021 to 2026 (USD Million)
Rest of Latin America Hyaluronic Acid Products Market, By Product Type, From 2021 to 2026 (USD Million)
Rest of Latin America Hyaluronic Acid Products Market, By Application, From 2021 to 2026 (USD Million)


Mail servers start to send email alerts when the mail file size reaches 95% of the total space allowed; and will continue to do so as long as the situation is not resolved.
At this stage, the email functions normally. However, you should start to free space by deleting or archiving emails ASAP.
If failed to do so, you will not be able to receive or send messages when the mail file size exceeds the quota.
Please be aware that moving messages to folders does not free any space, only deletion and archiving does.
When deleting/archiving messages, it is most effective to select messages containing large attachments. To do so, first sort messages by size as shown below.
Then you can choose to delete or archive the messages. Or you can remove the attachment, but leave the message for future reference*.
Please empty the trash after deletion. Otherwise, no space will be freed until the deleted messages are automatically purged by the system in 48 hours.
Immediately after deletion/archive, freed space will be used for mail transaction right away. However, you will not see the change in the mail file properties until it is compacted over the weekend.
After deleting several messages; why don't I see a physical change in my mail file allocation?
*Double-click on the attachment you would like to save. Click on Save to save the attachment to a location on your hard drive.
To delete the message, select the attachment once and hit the Delete button on your keyboard or right-click the attachment and select Delete.


A friend recently commented on the playfulness of our family. I must say — the family fun is mostly attributable to Marathon. He has always been playful. He was the smarty-pants class clown in school (from what I've gathered) and that spirit is still in him today.
Playing and goofing off is one of his ways of unwinding. On days when he is working at home, we'll take an hour or so break and run around and play in the backyard — soccer, baseball, kickball, and recently, dodgeball on the trampoline.
In the evenings, after the kitchen has been cleaned, we have family time. For years we had story time with the kids – and still do that from time to time. But at some point last fall, we started playing family games in the evenings – pictionary, clue, blokus, Chinese checkers, crazy 8s…and we're still on the game circuit.
When Marathon is away during the day, I try to schedule a morning break to do something active outside with the kids. Sometimes, when I'm needing my space, I'll send them out in the backyard while I do Pilates indoors. I try to play, garden, or play a game with them each day. It's one of those things that I don't always want to do, but once I get going, I'm glad I did.
The family that plays together stays together? We'll see!


2 out of 10 people in the UK suffer from some form of hearing loss, and a large portion of these don't have the right hearing aids and equipment for these conditions. Here at Dove Hearing we're dedicated to bringing you the highest quality hearing services and products in the Lichfield area. In addition to our free in store hearing tests, we also offer home hearing tests in the Lichfield area.
Do you need a home hearing test in Lichfield?
These symptoms can drastically effect your communication and relationships with others, therefore it's imperative that you have a hearing test if you regularly suffer with these.
People often request our home hearing tests in Lichfield if they have problems with mobility, or they are particularly daunted by the prospect of having the test. A home hearing test in Lichfield can be an incredibly handy and quick way to begin the journey of hearing rehabilitation.
The home hearing test in Lichfield will consist of a few questions regarding your hearing restrictions and an audiometric test to distinguish which sounds you can hear. Once this is completed a member of our team will develop a plan for your best course of action – usually a hearing aid or other hearing treatment.
If you would like to learn more about our home hearing tests then please get in touch with our Lichfield centre. Our team will arrange a time to suit you, and can answer any questions you may have about the process.


Obama says that when (if) he's debating John McCain in the fall, people won't be questioning his patriotism but wanting to know his position on the issues.
I guess that's what he has to say publicly. But I hope he understands that--unfortunately--plenty of people will absolutely be questioning his patriotism. He can ask Michael Dukakis about that.


We are professional in wire mesh.
Friendly staff and good service, ready stock at all time. place very easy to locate.
reliable, efficient, and competitive price. highly recommended.
Variety choices, the quality is higher than expected, price cheap but quality not.