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The City's First Time Homebuyer program provides zero percent (0%) deferred loans to first-time homebuyers purchasing a property in the City of El Paso. The buyer selects their own eligible property to purchase and meets with one of the participating lenders to pre-qualified for a mortgage loan.
If being a first-time homebuyer is a part of your american dream. fort Worth, TX Fort Worth, Texas moved up 10 spots from last year's list to claim the title as the best city for first-time.
Usda Rd Income Limits USDA Home Loans Zero Down Eligibility; Qualify in 2019 – USDA Home Loan Income Limits. Guaranteed loans are available to "moderate" income earners, which the USDA defines as those earning up to 115% of the area's median income. For instance, a family of four buying a property in Orange County, California can earn up to $110,750 per year. The income limits are generous.Federal Housing Loans 23 ways Federal Budget 2019 could affect your wallet – The federal government is highlighting new measures to help make home ownership into a more affordable dream for first-time buyers, reduce student loan payments and help low-income seniors keep more.
The First Time Homebuyers Workshop is designed to assist low to moderate-income families with the home buying process. Completion of this class entitles qualified families with down payment and closing cost assistance.
Common Questions From First Time Home Buyers. A first-time home buyer is someone who has not bought a house in the last three (3) years. If you previously bought and owned a house but haven't done so in the last 3 years, you're considered a first time home buyer; even though you are not a first time home owner.
· 6 First-Time Home Buyer Mistakes to Avoid. Buying a home for the first time? Help ensure a smoother and less stressful experience by avoiding these common mistakes made by first time home buyers.
Usda Loan Property Eligibility Map Housing Authority Mesquite Tx Mesquite Housing Division, TX | Section 8 – Closed: Mesquite, Texas (homelessness) housing choice Voucher Waiting List. The Mesquite Housing division (mhd): section 8 housing Choice Voucher waiting list is currently closed.It was last open for homeless applicants for one day in April 2017.It was last open for the general public for one day in January 2016, and before that in 2008.Standard Home Loans FHA vs Conventional Loan Comparison Infographic | The Lenders. – When FHA Home Loans are Better than Conventional Loans.. conventional mortgages have more options than just the standard 30-year fixed-rate mortgage.USDA Launches Changes to USDA Property Eligibility Maps – In essence, the USDA property eligibility areas are becoming more restricted, particularly in the Northeast. Some areas that were previously in eligible USDA loan zones may now be excluded. For example, parts of Rhode Island will be excluded from these USDA loans. You can access the USDA site to view the future affected areas.Texas Homestead Services Property Tax Exemptions – Home Comptroller.Texas.Gov – Property tax in Texas is a locally assessed and locally administered tax. There is no state property tax.Property tax brings in the most money of all taxes available to local government to pay for schools, roads, police and firemen, emergency response services, libraries, parks and other services provided by local government.
According to First American's report, instead of focusing on Millennial buying power, attention needs to be shifted towards housing supply. "As the surge of Millennial demand begins to hit shore,
Tarrant County Housing Partnership – Classes in English and Spanish (817) 924-5091 Lenders & Realtors. HAP partners with participating Lenders and Realtors to assist first-time home buyers. If you are interested in becoming a participating Lender or Realtor, two-hour certification classes are available throughout the year.
Loan programs for first-time home buyer can make the process easier, especially if you've had credit issues or found it hard to save up a big The Texas Department of Housing and Community Affairs, or TDCHA, offers first-time home buyer programs to assist qualified borrowers in the lone star state.
This program is designed for homebuyers to purchase a home anywhere in Travis. Affairs' My First Texas Home's Taxable Mortgage Program (TMP) offers down. Homebuyers Assistance Program · First Time Home Buyer Down Payment.
Mortgage Loan Information Low Down Payment Mortgage – Affordable Loan Solution® from Bank of America Our Affordable Loan Solution® mortgage offers a competitive rate with a down payment as low as 3% (income limits apply). Learn how this fixed-rate loan could help make buying a home more affordable. affordable mortgage, low down payment mortgage


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Installation FAQ
Over our many years of helping homes and businesses like yours, we have had the pleasure of building close relationships with over 400 installers nationwide. This means that wherever you are, we will typically have an installer near you, should you require their service.
Our installers are contracted to professionally assemble your game table at the best possible price.
Please note that remote locations may incur additional costs. If an installer deems your location is remote, we will inform you before processing your order. Installations during weekends and/or holidays will also incur additional costs that will have to be covered by the customer. Regular installation hours are between 8am-4pm, Monday to Friday.
After assembly, installers will require your sign-off to make sure you are 100% satisfied with their work.
There are generally two levels of installation:
1. Regular Installation
The game table is shipped to your address, whereupon you move it yourself into a room of choice where the table will be installed. The installer arrives at a later day or time to professionally assemble it for you. This method is cost effective if you need installation only.
Before setting up the installation date, please make sure that you have received all boxes. The installers will not be able to complete the installation if you are missing parts.
2. White Glove Installation
The game table is shipped to your address. You are responsible for offloading the table; however some manufacturers may offer garage delivery, please inquire. The installers will arrive at a later day or time to move your game table into a room of choice and then professionally assemble it. This is a more involved and costly process, albeit far more convenient.
Please note that the responsibility to ensure a clear installation pathway falls on you, the customer, so as to ensure the installers will be able to navigate your table into the room of choice. If you are not 100% sure that your table can fit into a room or hallway, let us know prior to processing the order and we will send a professional installer to check the location. There is a non-refundable charge of $79 for this service. If the installation pathway is changed in any way after the installer has cleared the original location pathway, you will be responsible for any extra charges that may be incurred as a result of the change.
Should you require room-of-choice delivery & professional installation, please choose the option on the product page. Alternatively, feel free to inquire via chat!
The price quoted for White Glove Delivery is for ground floor delivery, with direct access, meaning no stairs. Please note that that are exceptions that might increase the price of the White Glove Delivery, and they are as follows:
- 1 Set of Stairs
- 2 Set of Stairs
- 3 Set of Stairs
- Stairwell
- Window entry
- Basement/Bilco Entry
- Onsite Travel Path > 100ft
Thank you for choosing Foosball Planet!

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Happy New Year
Uploaded: January 01, 2006
Flower Burst
Nikkor 28-100mm lens
Hoya UV Filter
Nikon Picture Project Used For Effect
KV Day January 01, 2006Just beautiful #367420
Susan Weisensel January 01, 2006I just love this. What kind of lighting did you use, because it gave it A great color effect. Happy new year to you too. Keep up the good work. #2242971
Michael E. Quintana January 02, 2006Many thanks for the comment Susan.
Jessica Baldridge January 04, 2006great colors! #2253759
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Unavailable EXIF: If there is no other information but 'Unavailable' in the EXIF (meaning no EXIF data exists with the photo), the 'Unavailable' blurb is not displayed. If there is any info, it shows. Many photos have the EXIF stripped out when people modify the image and resave it, before uploading.
The following truth is one of the core philosophies of BetterPhoto:
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I do, I understand.
You learn by doing. Take your Nature and Landscape Photography up to a new level of understanding in my new online class - on sale now.
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Images may not be copied, downloaded, or used in any way without the expressed, written permission of the photographer.
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Simple Ivory Dupioni Silk Ring Pillow
Gorgeous Dupioni 100% Silk Ring Bearer Pillow In Ivory for your Wedding Day!
The Pillow Measures 8 inch square. The simplicity of this pillow works like a charm and suits many many Wedding Themes!
The Broad Satin Ribbon goes all the way to the back in a cross tie style.
Please note: Rings Must be tied to the thin ribbon only. The broad ribbon is purely for decoration!
Please Choose your Ribbon and mention in the "Note to Seller" Section during checkout.
1. Sunshine Yellow
2. Light Olive Green
3. Black
4. Navy Blue
5. Light Beige
6. Dark Olive
7. Light Pink
8. Coral
9. Maroon
10. Wine
11. Grey
12. Mauve
13. Purple
The Pillow will come packed in a sturdy cardboard box.
Would you like to further customize this product to suit your wedding theme! Write to me and lets get started!
Ships from Gurgaon, India within 3 to 5 days.
We Also Recommend


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Some information is missing or invalid below.
Victrola 6-in-1 Bluetooth Record Player
This product is not eligible for promotional offers and coupons. However, you are able to earn and redeem Kohl's Cash and Kohl's Rewards on this product.
Stylish with a nostalgic feel, this Victrola 6-in-1 Record Player is ready to play all of your vintage vinyls.
Gift Givers: This item ships in its original packaging. If intended as a gift, the packaging may reveal the contents.
- 6 ways to play your music
- 3-speed turntable plays 33 1/3, 45 and 78 RPM albums
- Built-in Bluetooth wirelessly streams music from most Bluetooth-enabled devices
- Aux-in jack lets you play music from any non-Bluetooth device
- All-in-one turntable, CD player, cassette player and AM/FM radio
- Record player
- 3.5mm cable
- 10.8"H x 14.4"W x 18.4"D
- Weight: 14.9 lbs.
- Cord length: 60 ft.
- Inputs/outputs: 3.5mm audio, RCA
- Wood, plastic
- Manufacturer's 1-year limited warranty
- For warranty information please click here
- For information about the modified return policy, please click here
- Model no. VTA-200B
Promotional offers available online at Kohls.com may vary from those offered in Kohl's stores.
WARNING: This product can expose you to chemicals including lead, which is known to the State of California to cause cancer. For more information go to www.P65Warnings.ca.gov.
Due to its contents, this product cannot be shipped via our Priority Service or sent to Alaska, Hawaii, P.O. boxes, and/or APO/FPO military addresses.


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Off the Ice
After 65 days on the ice the New Land 2013 Expedition to Ellesmere Island has come to an end. This morning at 9:45 a.m. we boarded our charter DeHavilland Twin Otter bound for Resolute and are now at the hotel in Resolute. We'd like to thank our primary sponsors Bergans of Norway, makers of technical outdoor clothing and equipment since 1908, and Devold, makers of wool long underwear and sweaters since 1853.
In total we skijored over 511 nautical miles, or roughly 608 street miles, on Ellesmere Island and Axel Heiberg Island. The ski conditions were totally awesome and the views were even better. To immerse ourselves in this land and travel through it at the beautiful pace set by sled dog and ski has been truly a special experience. We've fallen in love with our dogs and this landscape much in the same way that Otto Sverdrup and the men on the Second Fram Expedition did over 100 years ago.
Our wildlife encounters far exceeded our expectations. Here's the final numbers:
- We had over 60 wolf sightings
- We had 96 musk ox sightings
- We saw 116 rabbits
- Two polar bears
- 16 seals
- And five Arctic fox
We'll spend the next week in Resolute and Iqaluit and further south in Ottawa packing up and cleaning up before flying home. So this blog will continue as before in the near term. The expedition is over, but we have tons of work to do. We have got to shuffle through all of our video and photos and lots of post-expedition processing and we have to put together the documentary film.
We'd also like to thank all of our generous sponsors and supporters. We'd like to thank the wonderful staff of the Eureka Weather Station, our home team staff and our families. Without your support this project wouldn't be possible. So on behalf of Toby, Kyle, Hugh, Elle, Axel, Napu, Larry, and myself, thanks for following along, and we'll have some more blogs coming your way shortly.
Read the full post and listen to the audio dispatch on ForwardEndeavors.com
About the author:
During the late winter and early spring of 2007, John lived in Baffin Island, Canada, for 100 days. There he worked as expedition manager for the Global Warming 101 – Baffin Island Expedition. While documenting the local Inuit experience with climate change, the expedition connected school children in the States with their counterparts on Baffin Island.


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Turkey announces 2016 guarantees for generation from local coal
Turkey announced Tuesday details of the 2016 purchasing program for state power buyer and trading company Turkiye Elektrik Ticaret ve Taahhut AS (TETAS) for power generated by private power plants burning domestic coal.
The Turkish cabinet has decided that this year TETAS would buy a total of 6 TWh of power generated from locally produced coal for which it will pay Lira 185/MWh ($62.1/MWh), according to an announcement in Turkey's official state gazette Tuesday.
Generating companies have the right to sell up to 3% of their annual generation on application to TETAS within 60 days, after which TETAS will draft a purchase agreement designating how much power will be purchased and when it will be supplied, according to the announcement.
In future the decision by the cabinet as to how much power generated by local coal TETAS will buy and the price to be paid will be announced in October of the preceding year, with TETAS allowed to increase or decrease the volume by 10% as deemed necessary, the announcement said.
Similarly the cabinet will also announce each October how much power generated by coal-fired plants belonging to state generator EUAS that TETAS will buy and the price to be paid.
Turkey has 29 power plants totalling 9,842 MW burning locally produced coal, with a further six totalling 1,606 MW licensed and under development and another seven totalling 1,619.5 MW holding pre-licenses, which guarantee that a full generating license will be issued once finance for the development of the plant has been secured.
Turkish officials said earlier this year that Turkey would begin offering incentives to power plants burning local coal and were no longer in favor of developing plants burning imported coal. Last week Turkey said it would impose import duties of $15/mt on coal imported for power generation.
Source: Platts


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Photo Design Within Reach
1 break the rules, just for fun
Of course Design Within Reach (dwr.com) is big enough to contain many homes' worth of beds, chairs, rugs, funky bar stools, mid-century-inspired coffee tables, leather seats and storage options, shelves to wire bins. But today is about focusing on what helps us to actually see it all: good lighting, of course. DWR has plenty of modern and contemporary options in many personalities and for many purposes. Need overhead lighting? How about a drop light? Love your reading chair but squinting at the words in front of you? Spotlight floor lamps to the rescue. Burning the midnight oil and cramming for a big presentation at work? Turn to focused task lighting with a sleek desk lamp. DWR, founded in 1998, loves authentic modern design in all of its sleekness. DWR has a weakness for the work of iconic designers, and it's up to you to see the advantage of this.
2 making time for a romance
Within Stamford's Antique and Design district, you'll find plenty of stylish lighting, lampshades and other home accessories—everything from Nest candles and leather-and-velvet pillows to shiny gold serving trays and a Burmese Rattan basket in a honey brown that is both dreamy and practical. You're wandering The Accessory Store (stamfordshades.com), coming up with ideas left and right. This contemporary place is the bright idea of Mark Candido and Ron Scinto, cofounders of The Antique & Artisan Center; you're in good hands. A cool place, it was launched to help design-savvy customers and interior designers who were wearing out their high-end shoes running from place to place to source the finishing touches for their home- renovations and staging projects. The newer place carries the largest selection of lampshades in the Northeast.
3 honoring today's artisan tradition
You might have stopped into a store thinking you needed a platter for an upcoming party or a pretty candle for a hostess gift, but then you might quickly notice the sophisticated pendant lighting, and another one, and another one. Yes, Juliska (juliska.com) has a flagship store in Stamford and the lighting is worth the stop in and of itself. The pendants and chandeliers are simply beautiful, and made so by master glass blowers in the Czech Republic. Husband-and-wife Capucine and David Gooding founded the store in 2001 to offer artisan mouth-blown glasses. They fell in love with Bohemian glassware in Europe and built a brand known for quality and style. See it for yourself in the well-lit store on Canal Street. All of the pendants at the design shop are available for order for next-day pick up or complimentary home delivery. (P.S. The Factory Outlet is right next door—be sure to drop in.)


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Have you figured out your costume yet? A couples costume? For you? For your kids? Well, here's more inspiration and tutorials! (Part 1, Part 2, Part 3)
- The Swell life has a fun take on a Deviled Egg costume.
- A great tutorial on making costume armor out of felt! Perfect for your little knight… (via Craftgossip)
- Easy/Cute Baby Costumes (via Craftgossip)
- Homemade Exoskeleton
- A little Elvis! at Geekcrafts.com.
- Geekcrafts also brings us the ever popular Yip Yip Aliens from Sesame Street! (I actually like this version, which we saw at last years dragoncon, better — And there is an instructable to make your own, here.
- An adorable gnome, found at Craftzine
- And how to make your own sushi headdresses, also from Craftzine.
- Make quick homemade character costumes for kids (in this example Boba Fett, but good principles for any similar costume)
- Pippi Longstocking Braids
- Egyptian costume how to at Craftster
- Jeff sends us this fun list of 50 Cheap and Easy Halloween Costumes for Adults & Children – I love the idea of the Progressive Insurance girl!
If you missed it yesterday: Halloween Costumes, Star Wars Style!
From my own photo collection, here are some other great (mostly homemade) costumes from parties of years past, for your inspiration! Click to see larger…


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Gerald "Jerry" Rietveld, age 87, of Neenah, passed away unexpectedly on Thursday, March 5, 2020. Jerry was born on August 17, 1932 in Nuenen, Holland son of the late Peter and Bertha (Gietman) Rietveld. Jerry married Margie Kemps on September 18, 1954 at St. Margaret Mary Catholic Church in Neenah. They enjoyed 65 ½ years of marriage until his death. He worked for American Can/James River for many years until retirement.
Jerry and Margie were constant companions doing many things together. You could catch them at the local watering holes, casinos and family gatherings. Jerry enjoyed having a good time and was always up for a party.
Jerry is survived by his wife Margie, his children: Nancy (Jay) Stadler, Deb (Russ) Sova, Tammy (Gregg) Jansen and Rob (Jen) Rietveld. He is also survived by his grandchildren: Amber (Shaun) Jones, Karissa (Tommy) Clohessy, Becky (Mike) Wittman, Scott Sova (Yvonne Pulido-Gonzalez), Jeff Jansen (Lauren Bond), Kyle Rietveld, Brittney Rietveld (Brian Hendricks); great-grandchildren: Jordan, Phoenix, Bradley, Zayden, Skye, Amelia, Mason, Jada, Kyra, Penelope and Oscar; great-great grandchildren Landon and Laken. Jerry is further survived by his brothers, John Rietveld, and Tony (Donna) Rietveld. He was preceded in death by his parents and brothers Frank, Pete, Ray, Arie, Teddy, and one sister Riet.
The family would like to thank the paramedics, Gold Cross Ambulance, the compassionate care from Theda Clark Medical Center (a special thanks to his nurses in ICU especially Hannah, Brett, Lynn and Luke for the care they gave to not only Jerry, but the entire family) and Kessler Funeral Home.
A gathering of family and friends and Celebration of Life for Jerry will be held from 4:00 p.m. until 6:00 p.m. on Monday, March 9, 2020 at the Kessler Funeral Home, 304 S. Commercial St., Neenah. A memorial is being established.
To send flowers to Gerald's family, please visit our floral store.


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let's sum up. the grinding balls diameter determined by the bond formula has a recommendatory character and serves as a starting point for calculating the necessary proportion grinding media feeding a new mill. more precisely adjust the ball load in the mill can only by industrial test performing.
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the first two grinding efficiency measurement examples are given to show how to calculate wio and wioc for single stage ball mills. figure 1. the first example is a comparison of two parallel mills from a daily operating report. mill size 5.03m x 6.1m 16.5 x 20 with a id of 16 .
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ball mill power calculation example #1. a wet grinding ball mill in closed circuit is to be fed 100 tph of a material with a work index of 15 and a size distribution of 80% passing ¼ inch (6350 microns). the required product size distribution is to be 80% passing 100 mesh (149 microns).
to accelerate the math or calculation you can use the shortened formula: d m <= km * d^0.5where km =6 log dk is taken from figure 5 according to the fineness of the finished product dk. these formulas are applicable to the case of feeding a mill with only single-sized balls and not a mixture without consideration for ball wear.
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Applies to: Microsoft Teams.
The Wiki tab is a smart-text editor that moonlights as a communication machine where you draft, edit, and chat all in one area.
In this article
Write content for your Wiki tab
Create a Wiki tab
Every channel accompanies a Wiki tab.
To add a completely new Wiki tab, select Add a tab beside the other tab names in the channel. Choose Wiki from the tab gallery. Label the tab and begin writing.
Write content for your Wiki tab
A Wiki tab is equipped with each of the usual formatting options, such as bold, italic, and underlined text, highlighting, headers, and lists.
Every document in your Wiki tab is named a page and every page is composed of various sections. To start working, label your page and then begin authoring sections. Whenever you seek to append a new section, simply hover over the left side of the page and press Add a new section here.
On the left side of your screen, you'll notice a table of contents. This assists you to navigate swiftly between pages or even do some organising.
Note: A standard channel's Wiki tab can be accessed by anyone on your team. A private channel's Wiki tab is accessible only by members of that channel.
Link to a section
Hover over the section title and press More options > Get link.
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@mention someone in a section
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We measure the energy emitted by extensive air showers in the form of radio emission in the frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger Observatory, we obtain a radiation energy of 15.8 \pm 0.7 (stat) \pm 6.7 (sys) MeV for cosmic rays with an energy of 1 EeV arriving perpendicularly to a geomagnetic field of 0.24 G, scaling quadratically with the cosmic-ray energy. A comparison with predictions from state-of-the-art first-principle calculations shows agreement with our measurement. The radiation energy provides direct access to the calorimetric energy in the electromagnetic cascade of extensive air showers. Comparison with our result thus allows the direct calibration of any cosmic-ray radio detector against the well-established energy scale of the Pierre Auger Observatory.
The Auger Engineering Radio Array (AERA) is part of the Pierre Auger Observatory and is used to detect the radio emission of cosmic-ray air showers. These observations are compared to the data of the surface detector stations of the Observatory, which provide well-calibrated information on the cosmic-ray energies and arrival directions. The response of the radio stations in the 30 to 80 MHz regime has been thoroughly calibrated to enable the reconstruction of the incoming electric field. For the latter, the energy deposit per area is determined from the radio pulses at each observer position and is interpolated using a two-dimensional function that takes into account signal asymmetries due to interference between the geomagnetic and charge-excess emission components. The spatial integral over the signal distribution gives a direct measurement of the energy transferred from the primary cosmic ray into radio emission in the AERA frequency range. We measure 15.8 MeV of radiation energy for a 1 EeV air shower arriving perpendicularly to the geomagnetic field. This radiation energy -- corrected for geometrical effects -- is used as a cosmic-ray energy estimator. Performing an absolute energy calibration against the surface-detector information, we observe that this radio-energy estimator scales quadratically with the cosmic-ray energy as expected for coherent emission. We find an energy resolution of the radio reconstruction of 22% for the data set and 17% for a high-quality subset containing only events with at least five radio stations with signal.
Neutrinos in the cosmic ray flux with energies near 1 EeV and above are detectable with the Surface Detector array of the Pierre Auger Observatory. We report here on searches through Auger data from 1 January 2004 until 20 June 2013. No neutrino candidates were found, yielding a limit to the diffuse flux of ultra-high energy neutrinos that challenges the Waxman-Bahcall bound predictions. Neutrino identification is attempted using the broad time-structure of the signals expected in the SD stations, and is efficiently done for neutrinos of all flavors interacting in the atmosphere at large zenith angles, as well as for "Earth-skimming" neutrino interactions in the case of tau neutrinos. In this paper the searches for downward-going neutrinos in the zenith angle bins $60^\circ-75^\circ$ and $75^\circ-90^\circ$ as well as for upward-going neutrinos, are combined to give a single limit. The $90\%$ C.L. single-flavor limit to the diffuse flux of ultra-high energy neutrinos with an $E^{-2}$ spectrum in the energy range $1.0 \times 10^{17}$ eV - $2.5 \times 10^{19}$ eV is $E_\nu^2 dN_\nu/dE_\nu < 6.4 \times 10^{-9}~ {\rm GeV~ cm^{-2}~ s^{-1}~ sr^{-1}}$.
A measurement of the cosmic-ray spectrum for energies exceeding $4{\times}10^{18}$ eV is presented, which is based on the analysis of showers with zenith angles greater than $60^{\circ}$ detected with the Pierre Auger Observatory between 1 January 2004 and 31 December 2013. The measured spectrum confirms a flux suppression at the highest energies. Above $5.3{\times}10^{18}$ eV, the "ankle", the flux can be described by a power law $E^{-\gamma}$ with index $\gamma=2.70 \pm 0.02 \,\text{(stat)} \pm 0.1\,\text{(sys)}$ followed by a smooth suppression region. For the energy ($E_\text{s}$) at which the spectral flux has fallen to one-half of its extrapolated value in the absence of suppression, we find $E_\text{s}=(5.12\pm0.25\,\text{(stat)}^{+1.0}_{-1.2}\,\text{(sys)}){\times}10^{19}$ eV.
Contributions of the Pierre Auger Collaboration to the 33rd International Cosmic Ray Conference, Rio de Janeiro, Brazil, July 2013
BATATA is a hodoscope comprising three X-Y planes of plastic scintillation detectors. This system of buried counters is complemented by an array of 3 water-Cherenkov detectors, located at the vertices of an equilateral triangle with 200 m sides. This small surface array is triggered by extensive air showers. The BATATA detector will be installed at the centre of the AMIGA array, where it will be used to quantify the electromagnetic contamination of the muon signal as a function of depth, and so to validate, in situ, the numerical estimates made of the optimal depth for the AMIGA muon detectors. BATATA will also serves as a prototype to aid the design of these detectors.
One of the main impacts of the JEM-EUSO mission will come from its unprecedented exposure. This feature creates, for the first time in the field, the possibility of studying individual UHECR sources. However, the intrinsic characteristics of the sources and the injection mechanism, as well as the presence of intervening magnetic fields, present challenges to the identification of isolated sources and to the extraction of their relevant spectral information from the data. We discuss here these aspects in a quantitative way and give an overview of what can be achieved in this regard under different astrophysical scenarios.
JEM-EUSO, on board of the Japanese Exploration Module of the International Space Station, is being proposed as the first space observatory devoted to UHECR. Its privileged position at 430 km above the Earth surface, combined with a large field of view, innovative optics and a high efficiency focal surface, results in an unprecedented exposure which significantly surpasses that of the largest ground observatories. The large number of events expected above the GZK threshold for photo-pion production by protons will allow the directional identification of individual sources and the determination of their spectra, i.e., doing astronomy and astrophysics through the particle channel. Similar goals can be achieved in the case of light UHECR nuclei. Furthermore, the atmospheric target volume ($\sim 10^{12}$ ton) makes the possibility of neutrino observation a highlight of the mission. Other exploratory objectives include the detection of extreme energy gammas and the study of Galactic magnetic fields as well as global observations of the earth's atmosphere, including clouds, night-glows, plasma discharges, and meteors. In this contribution we will describe the scientific objectives of JEM-EUSO.
The Pierre Auger Collaboration intends to extend the energy range of its southern observatory in Argentina for high quality data from 0.1 to 3 EeV. The extensions, described in accompanying papers, include three additional fluorescence telescopes with a more elevated field of view (HEAT) and a nested surface array with 750 and 433 m spacing respectively and additional muon detection capabilities (AMIGA). The enhancement of the detector will allow measurement of cosmic rays, using the same techniques, from below the second knee up to the highest energies observed. The evolution of the spectrum through the second knee and ankle, and corresponding predicted changes in composition, are crucial to the understanding of the end of Galactic confinement and the effects of propagation on the lower energy portion of the extragalactic flux. The latter is strongly related to the cosmological distribution of sources and to the composition of the injected spectrum. We discuss the science motivation behind these enhancements as well as the impact of combined HEAT and AMIGA information on the assessment of shower simulations and reconstruction techniques.
The fluorescence technique has been successfully used to detect ultrahigh energy cosmic rays by indirect measurements. The underlying idea is that the number of charged particles in the atmospheric shower, i.e, its longitudinal profile, can be extracted from the amount of emitted nitrogen fluorescence light. However the influence of shower fluctuations and the very possible presence of different nuclear species in the primary cosmic ray spectrum makes the estimate of the shower energy from the fluorescence data analysis a difficult task. We investigate the potential of shower size at maximum depth as estimator of shower energy. The detection of the fluorescence light is simulated in detail and the reconstruction biases are carefully analyzed. We extend our calculations to both HiRes and EUSO experiments. This approach has shown some advantages to the reconstruction of the energy when compared to the standard analysis procedure.
Along the years HiRes and AGASA experiments have explored the fluorescence and the ground array experimental techniques to measure extensive air showers, being both essential to investigate the ultra-high energy cosmic rays. However, such Collaborations have published contradictory energy spectra for energies above the GZK cut-off. In this article, we investigate the acceptance of fluorescence telescopes to different primary particles at the highest energies. Using CORSIKA and CONEX shower simulations without and with the new pre-showering scheme, which allows photons to interact in the Earth magnetic field, we estimate the aperture of the HiRes-I telescope for gammas, iron nuclei and protons primaries as a function of the number of simulated events and primary energy. We also investigate the possibility that systematic differences in shower development for hadrons and gammas could mask or distort vital features of the cosmic ray energy spectrum at energies above the photo-pion production threshold. The impact of these effects on the true acceptance of a fluorescence detector is analyzed in the context of top-down production models.
The HiRes and AGASA Collaborations have published contradictory energy spectra for energies above the GZK cut-off. In this article, we investigate the acceptance of fluorescence telescopes to different primary particles at the highest energies. Using CORSIKA shower simulations without and with the new pre-showering scheme, which allows photons to interact in the Earth magnetic field, we estimate the aperture of the HiRes I telescope for gammas and protons primaries. We calculate the dependence of the telescope sensitivity to primary particle identity. We also investigate the possibility that systematic differences in shower development for hadrons and gammas could mask or distort vital features of the cosmic ray energy spectrum at energies above the photo-pion production threshold. The impact of these effects on the true acceptance of a fluorescence detector is analyzed in the context of top-down production models.
The surface detector technique has been successfully used to detect cosmic ray showers for several decades. Scintillators or Cerenkov water tanks can be used to measure the number of particles and/or the energy density at a given depth in the atmosphere and reconstruct the primary particle properties. It has been shown that the experiment configuration and the resolution in reconstructing the core position determine a distance to the shower axis in which the lateral distribution function (LDF) of particles shows the least variation with respect to different primary particles type, simulation models and specific shapes of the LDF. Therefore, the signal at this distance (600 m for Haverah Park and 1000 m for Auger Observatory) has shown to be a good estimator of the shower energy. Revisiting the above technique, we show that a range of distances to the shower axis, instead of one single point, can be used as estimator of the shower energy. A comparison is done for the Auger Observatory configuration and the new estimator proposed here is shown to be a good and robust alternative to the standard single point procedure.
The fluorescence technique has been successfully used to detect ultrahigh energy cosmic rays by indirect measurements. The underlying idea is that the number of charged particles in the atmospheric shower, i.e, its longitudinal profile, can be extracted from the amount of emitted nitrogen fluorescence light. However the influence of shower fluctuations and the very possible presence of different nuclear species in the primary cosmic ray spectrum make the estimate of the shower energy from the fluorescence data analysis a difficult task. We investigate the potential of shower size at maximum depth as estimator of shower energy. The detection of the fluorescence light is simulated in detail and the reconstruction biases are carefully analyzed. We extend our calculations to both Auger and EUSO experiments. This kind of approach is of particular interest for showers that are not fully contained inside the field of view of the detector.
The ultrahigh energy tail of the cosmic ray spectrum has been explored with unprecedented detail. For this reason, new experiments are exerting a severe pressure on extensive air shower modeling. Detailed fast codes are in need in order to extract and understand the richness of information now available. In this sense we explore the potential of SENECA, an efficient hybrid tridimensional simulation code, as a valid practical alternative to full Monte Carlo simulations of extensive air showers generated by ultrahigh energy cosmic rays. We discuss the influence of this approach on the main longitudinal characteristics of proton, iron nucleus and gamma induced air showers for different hadronic interaction models. We also show the comparisons of our predictions with those of CORSIKA code.
The air fluorescence technique has long been used to detect extensive air showers and to reconstruct its geometry and energy. The fluorescence photon yield of an electron in air is of main importance in the reconstruction procedure. Historically, the fluorescence yield used in the reconstruction of the showers is approximated at all energies by that of an electron with kinetic energy of 80 MeV, because these are the most abundant in a shower. In this paper, we calculate the fluorescence yield taking into account the energy spectrum of electrons in showers initiated by proton and iron nuclei as a function of height. We compare our results with previous calculations based on mono energetic electrons (80 MeV) and a difference in excess of 8% is found. Finally, the influence of a more realistic fluorescence yield in the shower energy reconstruction is also discussed.
Several facts regarding the structure of NGC 604 are examined here. The three main cavities, produced by the mechanical energy from massive stars which in NGC 604 are spread over a volume of 10$^6$ pc$^3$, are shown here to be undergoing blowout into the halo of M33. High resolution long slit spectroscopy is used to track the impact from massive stars while HST archive data is used to display the asymmetry of the nebula. NGC 604 is found to be a collection of photoionized filaments and sections of shells in direct contact with the thermalized matter ejected by massive stars. The multiple blowout events presently drain the energy injected by massive stars and thus the densest photoionized gas is found almost at rest and is expected to suffer a slow evolution.
Introducing a simple Galactic wind model patterned after the solar wind we show that back-tracing the orbits of the highest energy cosmic events suggests that they may all come from the Virgo cluster, and so probably from the active radio galaxy M87. This confirms a long standing prediction, as well as a theoretical model for the radio galaxy jet emission of M87. With this picture in hand, one clear expectation is that those powerful radio galaxies that have their relativistic jets stuck in the interstellar medium of the host galaxy, such as 3C147, will yield limits on the production of any new kind of particle, expected in some extensions of the standard model in particle physics.


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This is a basic introduction to the concepts rules and Best Practices of the typical Fiduciary/Caregiving roles. The course will introduce definitions, examples, and quizzes to test your knowledge. The goal of the course is to clearly define the terms, examine current cases and examples from your own experience and real life scenarios. These lessons will give you the tools and knowledge to be successful working directly with clients, loved ones or wards.
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· Understand the general duties and responsibilities of a fiduciary
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· Differentiate between the roles of a conservator of person and conservator of estate
· Develop a basic understanding of mental health disorders
· Understand the use of the "Strengths Perspective" when working in individuals
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- Module Two Introduction & Definitions
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- Video: Guardianship FREE PREVIEW
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- Activity: Case Study Part 1
- Activity: Case Study Part 2
- Module Two Quiz
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Michael Mackniak, JD
Senior Consultant
About the instructor
Michael Mackniak,JD is a "recovering attorney" who coaches and consults families and high performance professionals in decision-making and leadership roles. His work in the behavioral health field has garnered national recognition from groups such as the National Association of Social Workers, National Alliance on Mental Health, Probate Judges College and several others.
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This is a Journal entry by Saturnine
Saturnine Started conversation Jun 23, 2004
I'm getting snowed under with invites.
I have six more going, and it looks like I'll get more and more and more in the future. Email me if you want one (Egon and Croz, I know I owe you one if you haven't got one already).
SEF Posted Jun 23, 2004
What is it with all this Gmail peddling?! The people who have them don't need any more of them (yet more keep coming apparently) and the people who do want them don't get them (except from the people with too many).
egon Posted Jun 26, 2004
I await with baited breath <biggrin. You have my email address, don't you?
Saturnine Posted Jul 3, 2004
Egon - EMAIL ME. I have one invite to give out right now, and if you don't email me, I can't send you the invite.
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"The Hitchhiker's Guide to the Galaxy is a wholly remarkable book. It has been compiled and recompiled many times and under many different editorships. It contains contributions from countless numbers of travellers and researchers."


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BIRTHH is songwriter, producer and daydreamer Alice Bisi, for whom it's all about surprises. It's what gets her up in the morning – the never-ending promise of beauty, of a vast blue sky to lose yourself in each day. It's also seeped into the music she makes, with her forthcoming second album WHOA full of unexpected key changes, shifting tempos and playful twists and turns Bisi demoed in a nine month burst of creativity in her makeshift bedroom studio before finishing it with Solange collaborator Lucius Page and the Grammy-winning Robert 'LB' Dorsey.
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This deck requires heavy investment and Box resets, but having multiple Relinquished, along with the supports to summon him faster can be really strong. This is mostly an "all-in" version of the deck, without using cards like Interdimensional Matter Transporter to protect it, and focusing on its ability to get summon multiple Relinqsuihed.
|Harpies Hunting Ground
|Essential cards
|Budget - Expensive
(Box reset)
|The Ultimate Rising
|[Skill] description
|Harpies' Hunting Ground
Begin the Duel with the Field Spell Harpies' Hunting Ground on the top of your deck.
Sonic Bird, Senju of the Thousand Hands give you +1 hand advantage by just being summoned. Then you'll never run out of your hands. Once your opponent summons a monster to destroy them, use Sphere Kuriboh to defend and ritual summon Relinquished tributing Sphere Kuriboh in your graveyard.
There are 2 ways to use Relinquished, take control of your opponent's strong monster to beat their weaker ones, or take their weaker ones and attack into their stronger ones to deal damage. The latter only works if your opponent's LP is lower than yours, and if the damage that you take does not finish you off right away, while the former is good if you want to play offensively.
A common strategy that people sometimes do early in the duel, when your opponent only has 1 set monster and you can summon Relinquished, summon a monster, then summon Relinquished and take their set monster. This can potentially allow you to direct attack your opponent early. Having them at lower LP than you will give you quite a huge advantage in a Relinquished deck. You also don't have to be very conservative about using Sphere Kuriboh to defend, since you can use Sphere as the sacrifice material to get Relinquished out.
With only 3 Harpies in the deck, and no way to search for them, they won't be appearing as often, but the threat of Harpies' Hunting Ground field spell can make your opponent play more cautiously about their spell/trap cards.
Sonic Bird and Senju of the Thousand Hands will be summoned in preference to Harpies. Summoning Harpies to destroy a face-up spell/trap card like Mirror Wall and Skull Lair is the best. That's safer than destroying face-down spell trap cards since people often bring HHG counter cards like Security Orb, or Wild Tornado.
Additionally, in a Relinquished deck, Harpies can be used to destroy your Relinquished's equipped card instead of your opponent's spell/trap. Then your Relinquished can take a monster your opponent controls again.
Interdimensional Matter Transporter
|Banishing your Relinquished will make them untargetable and destroys the equipped monster.
|Mid Sept 2020
|Duelist Chronicle 5Ds: Fight for the Fortune Cup
|Duel Quest Event
|Late Sept 2020
|Yu-Gi-Oh Zexal Duel Links
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Seto Kaiba (DSOD) Lvl 40
Mokuba Kaiba (DSOD) Lvl 40
Scud (DSOD) Lvl 40
Sera (DSOD) Lvl 40
Joey Wheeler (DSOD) Lvl 40
|Available card boxes
|Card Trader
|Ranked Rewards
Card Trader
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Looking for a perfect party dip? My Healthy Everything Bagel Dip recipe is creamy and delish!
Hey guys!
We are heading into the holiday season faster than I'm ready to accept. Halloween is two weeks away and then I feel like we're just on a train of celebrations until January. It's such a wonderful time of year AND it never hurts to go into the busy season with a few new party recipes up your sleeve.
Today I'm sharing a fabulous new dip recipe that is not only a crowd-pleaser but only 4 INGREDIENTS! My Healthy Everything Bagel Dip recipe is perfectly creamy and tastes like everyone's favorite bagel!
Why you'll love this Healthy Everything Bagel Dip recipe…
This dip is basically everything a good dip should be.
Cheesy, savory, scoopable and totally addictive.
My Healthy Everything Bagel Dip recipe gets its flavor from the famous Trader Joe's Everything But the Bagel Seasoning (which they also now sell at ALDI!) You can buy yours OR make your own my homemade, DIY version I posted last week.
The combination of garlic, onion, sesame seeds and salt is perfection. If you even like everything bagel you are going to LOVE this.
The rest of the dip is a combination of whipped cream cheese and greek yogurt! You could do straight cream cheese but I love how the greek yogurt lightens it up, adds probiotics and keeps it a bit healthier. The texture of the light whipped cream cheese with the yogurt is nothing short of dreamy.
So what's in this Healthy Everything Bagel Dip recipe?
This recipe is SO easy! Only 4 ingredients! I already mentioned a few of them, but here's the rest.
- Everything Bagel Seasoning
- Whipped Cream Cheese <— Light if that's your jam!
- Plain Greek Yogurt <— I like to use 0%.
- Onion powder <— Brings out all the flavors!
How to make this Healthy Everything Bagel Dip recipe…
This recipe is a no-bake, just stir dip! It could not be easier to throw together for a party.
- Carefully fold all the ingredients together.
- Top with extra Everything Bagel Seasoning
- Serve with crackers, veggies or pretzels. <— I found EVERYTHING BAGEL pretzels at ALDI. 🙂
This is such a fabulous recipe for any of the upcoming holidays! You could have as a hearty snack for Halloween, Thanksgiving or even Christmas. I can imagine making it for a group of friends.
I hope you love this Healthy Everything Bagel Dip recipe as much as I do.
Also try these dips…
- Healthy Buffalo Cauliflower Dip
- Creamy Lemon Garlic Feta Dip
- Healthy Creamy Black Bean Dip
- Avocado Feta Dip
- Healthier Jalapeno Popper Dip
Pin for later!
Healthy Everything Bagel Dip recipe
- 8 ounces whipped cream cheese
- 1/2 cup plain greek yogurt
- 1 teaspoon onion powder
- 2 tablespoons everything bagel seasoning, plus extra for topping
- Carefully fold together all the ingredients. Put in a bowl and top with extra everything bagel seasoning.
- Serve with bagel chips, pretzels, carrots or other crisp veggies!
Your turn!
What holidays do you cook for?


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What you get:
▪ Tea/Coffee Station set up with crockery cups
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Chef's selection Sweet treats
Assorted Cookies
Fruit Bowl
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A. Chef's Selection of savoury baked treats
B. Choice of sliders and sandwiches with
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I have lived in central PA for nearly 25 years. This is literally my home now. But I am not from here. My family and many friends from the previous parts of my life are back in the Midwest. So every year, we make the journey to Illinois, Wisconsin, Iowa and Minnesota. This year, it is uncertain, and that makes me sad.
Don't get me wrong. I love my life here. It is a beautiful place. Lemont and State College have much to offer between the resources of the university community, the advantages of a small town, the beauty of mountains and forests, the connection of our neighborhood. I can get milk in glass bottles from local cows, visit lots of local farmer's markets, talk with all sorts of people from a places all over the world, find a variety of interesting activities and events, and other than when there is football traffic, I can get anywhere in town in about 15 minutes. It is a rich life that suits me and my interests. But this isn't where I am from.
I am from a place with flat lands. Plains grasses. Rolling hills. Wide roads laid out in a grid. Great lakes. Chicago neighborhoods. Small town Wisconsin and small town Iowa. Meandering streams. The mighty Mississippi River. Friday fish fry. Friends who knew me when I was young. Classmates from high school and college and seminary. The places I knew and loved when I was a child.
Despite the risks because of Covid-19, it looks like we will make a careful trip to see my dad in Chicago this month. After driving west for 3 or 4 hours, somewhere in eastern Ohio, I'll realize we've left the lovely mountains behind. As I look out at farmland on all sides, I will take a deep breath and say, "I can see for miles." I have probably said that every year. It's become my way of saying, "I am going home."
The landscape of the places where I grew up and came of age speak to my spirit differently than the place I make my home now. There are huge skies, stormclouds like you cannot imagine, wind that never stops, rain and tornados you can see from miles away. People with my accent, and places that I remember from when I was very small.
Years ago, I talked about all this with a friend who lived and worked for decades in San Diego, California. There on the beach, with perfect weather almost every day, he lived in a paradise. Like me, he found his summer visits home, to the places he had grown up in Iowa, brought a kind of joy that other people couldn't quite understand. We agreed that for some of us, there is a landscape that is home to your heart.
This summer, may we all find time to spend in the place that is home.
God of every place,
You are with me everywhere I go.
I see you in the beauty of the mountains and the strength of the winds.
I find you in the gently waving prairie grass and farm fields.
I hear you in the songs of birds and the roar of the waves.
I know you are with me here.
I see you in the faces of my family and friends.
I find you in the presence of strangers and people I will never meet.
I hear you in the voices and music and traffic of the city, and the silence when I am alone.
I know you are with me here.


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With a relatively warm weekend coming up here in Charleston, I thought I'd share a smorgasbord of what I'm reading to get excited. Plus, for my Malaysian readers, there's a giveway! Scroll down for more details.
Major cities in Kuala Lumpur can now call on Food Panda to deliver from their favorite restaurants in the area. Delivery can be as low as RM 4 (just around $1.30 US). Do you think they'd deliver a pile of fresh roti canai (flatbread) and a teh tarik (pulled tea) to me here in Charleston? I'd probably pay a premium. Also, Food Panda is offering TEN of my lucky readers free delivery on their next order with Food Panda! Leave a comment below -- the first ten to respond with their complete e-mail will earn a voucher for free delivery.
Tristan, the restaurant where we got married nearly five years ago, is closing this April. Besides being utterly broken-hearted, I'm also concocting a plan to eat Chef Whiting's delicious hay-smoked, housemade pasta every week until then (budget and diet notwithstanding, of course).
Even though it's not the hubby's favorite, the kids and I have been inhaling this kale pesto -- it's easy to make and chock full of healthy, good stuff (I mean, besides the oodles of Parmesan, but that hardly counts when it's made of raw sheep's milk, right?)
I didn't start using crispy shallots regularly until we lived in Malaysia -- and this recipe is so easy, with a great suggestions to use them as a burger garnish.
A solid addition to the Charleston Asian food scene (which is, quite frankly, a desert wasteland); we went for Chinese New Year and had stellar scallion pancakes, Shanghai stir-fried noodles and sauteed eggplant (the other dishes were a little salty for our taste).
Here's a great story about reviving a South Carolina barbecue institution.