text:
Q: LSTM model approach for time series (future prediction) I am new to tensorflow/tflearn and deep learning so these may be basic questions but I would appreciate any input.

*

*Question 1:  I have been able to successfully run a LSTM model using tflearn on a set of 2 years of time series data/sequence.  I can run the model via variations of "look_back" (e.g. 1 day, 7 days, 30 days) but it will output a single value at each iteration.  Running the LSTM for a larger look back improves the RMSE of my test data set.  Question I have is, if my goal is to to predict the "next 30 days" given a set of historical daily values, how do I modify the model?  I presume I need to either modify my OUTPUT tensor to be a sequence or somehow feed the decoder output at each iteration to be the input to the next?  Or do I modify the model to output a full sequence?  I cannot find any clear example of how this may be done.

*Question 2:  After a model is trained, how exactly do you productionize the model. Suppose in my case I trained/tested a model using a year of data to predict the next 30 days. How exactly can I now implement this so that as i get daily values they get integrated with the model. Again, any example of this would be great.

I have tried to go through the tensorflow tutorials but I am not sure they address these points.
Thanks

redpajama_set_name: RedPajamaStackExchange


I always find that it's easy to go for your basic reds and pinks when it comes to a manicure, but there's nothing more exciting than changing it up for once. Especially because summer is finally here, nothing screams "the warmer months have arrived!" than the perfect, punchy mani-pedi. Burgundies, deep reds, and darker tones are put away, and pops of bright colors galore take center stage. Here are some fun and unique summer nail ideas to get you inspired for your next trip to your next mani appointment.
Why choose one color when you can choose 10?! When it comes to chic summer nail trends, this is probably one of the easiest ones in the book. You can use polishes you already have at home to create dreamy color combinations.
Adding small sequins and gems is the perfect way to add some minimal sparkle to your look. After painting your nails with as many coats as you want, place the small gem or sequin to your nail bed using some tweezers. Seal it all in with a strong, clear topcoat.
Showing your natural nail and creating shapes out of negative space has been all the rage when it comes to the latest and greatest manicure trends. To get this look at home, tape off your nails using a thin manicure tape in any shape you'd like and then paint over the tape in multiple coats, letting the polish to fully dry before peeling.
For sparkle lovers who don't want their nails to be the least bit minimal, this is an easy way to get a crazy design just in time for festival season. Pair this look with a ton of rings and you'll be ready to dance the night away.
Although it's easy to get caught up in bright and detailed nail designs, a simple coat of lavender white keeps your nails looking clean and fresh and incorporates one of the season's hottest hues.
What are your favorite summer nail trends? Let us know in the comments below! And if you're interested in writing articles like this for College Fashionista, be sure to apply to be a Community Member today.


* The Startimer Pilot Manufacture from historical Swiss watch brand Alpina is the brand's limited edition Pilot watch with in-house movement, AL-710. The beautiful anthracite grey dial with sunburst effect features applied Arabic numerals and bold, luminous hands making readability in all light conditions simple. The unique date indicator is shown with the use of a small pointer sub-dial at the 6 o'clock position whilst the oversized crown and red triangle second hand add to the aesthetic qualities of this watch.
* This piece comes in mint/unworn condition and perfect working order. Box and papers dated 2015 are included.
* Current new RRP £2400 saving £750 (31%) on list price.


Monitoring wells and groundwater sensors were installed and monitored in and around Holts Landing State Park on the Indian River Bay, eastern Sussex County, Delaware, between October 2009 and August 2012. Data from test drilling, geophysical logging, geophysical surveys, and well testing characterized the hydrogeological framework and spatial and temporal patterns of water pressure, temperature, and salinity in the shallow, unconfined Columbia aquifer. The work revealed a plume of freshened groundwater extending more than 650 ft into the bay from the shoreline.


text:
Moure peut désigner :

Toponymie

au Portugal :
 Moure, paroisse civile de la municipalité de Barcelos ;
 Moure, paroisse civile de la municipalité de Felgueiras ;
 Moure, paroisse civile de la municipalité de Póvoa de Lanhoso ;
 Moure, paroisse civile de la municipalité de Vila Verde.

Patronyme

 Émile-Jules Moure (1855-1941), pionnier français de l'oto-rhino-laryngologie ;
 Jesus Moure (1912-2010), prêtre et entomologiste brésilien ;
 Pierre Moure (1983- ), acteur français.

Voir aussi

 Mourre

Patronyme français

redpajama_set_name: RedPajamaWikipedia


text:
Q: What app does macOS Mojave use for screen recording? I just upgraded to macOS Mojave on Macbook Air. I press command + shift + 5 on keyboard, it prompts a window where I select part of screen and then I begin recording my screen. The video quality is good and even the default microphone works well.
However, it is a little mysterious to me what program it is using for this. In the past, it would use QuickTime. However, I do not see QuickTime or any menu bar visible when this screen sharing utility launches. Also, after I save, and open it, it suggests to open in Quicktime.
Is it using QuickTime behind the scenes, albeit without a menu bar?

A: If you start screen recording then open the activity monitor.
You will see a process name screencapture.
Click process info botton will see more detail.
It seems like a system level functions and use intel quick sync to encode.


text:
SHIFTS by Powerhouse Company
Exhibition about the economic crisis and its consequences for architecture.
From 7 February to 25 May, the Danish Architecture Centre (DAC) in Copenhagen will host SHIFTS, an exhibition by Powerhouse Company and Hans Ibelings. SHIFTS will be part of the exhibition 'Will it Sustain?'.
The Danish Architecture Center, Strandgade 27B DK 1401 Copenhagen Denmark
February 7 to May 25, 2014 (Opening hours: Monday – Sunday 10:00 – 5:00 pm / Wednesday 10:00 – 9:00 pm)
http://www.dac.dk/en/front-page/
http://powerhouse-company.us6.list-manage.com
http://www.architectureobserver.eu
Doctoral Research Fellows in Art History and Visual Studies
PhD Funding
University of Oslo Department of Philosophy, Classics, History of Art and Ideas Two Doctoral Research Fellowships (SKO 1017) in Art History and Visual Studies are available at the Department of Philosophy, Classics, History of Art and Ideas, University of Oslo....
SAH | Places Prize on Race and the Built Environment
Applications are now being accepted for the SAH | Places Prize on Race and the Built Environment. The prize is a unique collaboration between the Society of Architectural Historians and Places Journal. The successful applicant will propose an original work of public...
Holt/Smithson Foundation 2022 Research Fellowship
The Foundation is calling for applications to the 2022 Research Fellowships. This program encourages new research on the work, ideas, and creative legacies of Nancy Holt and Robert Smithson. The second Fellowship season focuses on two topics: Earthwork Ethics and...
Webinar: "On Pedagogy: Islamic Art and Architecture in the Classroom," International Journal of Islamic Architecture Dialogues Series
Join the International Journal of Islamic Architecture (IJIA) for its Dialogues Series, an annual webinar that brings together scholars and practitioners from across varied disciplines for a discussion of critical contemporary issues that interrogate the boundaries...
Doctoral Fellowship in History and Theory of Architecture (2 positions)
Doctoral Program, Institute of History and Theory of Architecture (gta), Department of Architecture, ETH Zurich, Switzerland The doctoral program at the Institute of History and Theory of Architecture (gta), ETH Zurich, offers two fellowship positions to start on...
more news from the field
← Space-Time by Jorge Otero-Pailos at the MIT Keller Gallery National Preservation Conference – Call for Ideas and Proposals →

redpajama_set_name: RedPajamaCommonCrawl


text:
Dead hedgehog very sad
Date posted: Friday 9th October 2020
A very sad discovery of this dead hedgehog lying on someone's plot this Tuesday. Flora and I were both concerned that the animal looked to be in a healthy bodily condition – we thought it might be the victim of eating slugs that had ingested metaldehyde based slug pellets. But Rose later suggested that the hedgehog might have died after being accidently pierced by a fork while someone was turning a compost heap. There was a suppurating hole on the body and initially we thought it was where crows had started pecking, but more likely it was an injury caused by a garden fork. At this time of year not many people are putting in new plants that would require slug pellets around them. In all the time I've had my plot I've only ever seen three hedgehogs on our site. The first had been strimmed and sustained a leg injury; it was taken to a rescue centre but didn't survive. The second was a large, healthy looking animal that was dead, in full view near the Seed Store. And now this one… Very sad, as they're now officially categorised as 'vulnerable to extinction' – a far cry from a few decades ago when hedgehogs were commonly seen all over the UK. A group called 'Hedgehog Street' has initiated a campaign to mitigate the loss of hedgehogs in urban areas:
'The decline in hedgehogs flags up concerns about the environment that affects us all. Although they have some national and European protection under Schedule 6 of the Wildlife and Countryside Act (WCA) 1981, which prohibits killing and trapping by certain methods, and the Wild Mammals (Protection) Act 1996 and Appendix III of the 'Bern' Convention, they are still at risk. In 2011, PTES and BHPS started the Hedgehog Street campaign to reverse this decline
by inspiring the British public to help protect hedgehogs. Together we've recruited over 47,000 Hedgehog Champions to help conserve hedgehogs.
British gardens are becoming poorer homes for wildlife with increased paving, decking and reduced plant life. And with more roads and housing developments being built, we're seeing a huge loss of connectivity between green spaces, leaving hedgehogs isolated. Hedgehog Street is improving urban areas for hedgehogs, with:
►more gardens and green spaces linked with 'Hedgehog Highways' in fences
►more wild areas and log piles in gardens for insects and other wildlife
►more hedgehog houses and feeding stations in gardens
We're inspiring the British public to make their gardens hedgehog-friendly and recruit their neighbours to create Hedgehog Streets in their community. BHPS and PTES are also working with academics to research the reasons for hedgehog decline, as well as lobbying developers and land owners to mitigate for hedgehogs and help create hedgehog-friendly housing. Chris Grayling MP, Secretary of State for Transport, has been appointed as the Species Champion for hedgehogs to help promote their conservation in Parliament. A ten-year strategy is in place for
national hedgehog conservation until 2025.' (www.britishhedgehogs.org.uk>pdf>sobh-2018)
There are commercially available slug pellets that aren't based on metaldehyde which is toxic to wildlife; 'Slug killers based on aluminium sulphate are not strictly organic, but they are environmentally friendly. They kill slugs and snails on contact with minimal risk to other wildlife or pets. Commercially available products using aluminium sulphate as active ingredient include Growing Success and Fertosan.' (RSPB).
On a more positive note with which to end as we were walking back in the dusk yesterday evening a little owl flew across the site, uttering that distinctive call – a joy to see it but it flew past too quickly to get the camera out!


We recommend this comprehensive range of cast iron manufactured by the excellent Chasseur factory in the Ardennes region of France. Complementing their superb heavy duty frying pans and grill pans the Chasseur cast iron casseroles are ideal for food requiring long slow cooking. The back enamel coating is durable and easy to clean. Super quality ridged grill pan.


Why "the snip" gets the short shrift.
It's not just a niche topic among DIYers. Ken Bone, the 34-year-old, red-sweater-clad internet sensation made infamous by his presidential debate appearance, recently sang the praises of his own medical sterilization on a Reddit Ask Me Anything thread, concluding that the procedure was painless, his sexual satisfaction is way up, and his wife loves it, too.
It seems like maybe vasectomies are going mainstream. But the reality is that vasectomy rates in the U.S. are actually much lower than in other countries. Female sterilization is twice as popular in the U.S., but in Canada and the U.K., it's almost the complete opposite. The reason is likely a combination of a few things: the cultural expectation that women should take on all the family planning responsibilities, and the fact that under the Affordable Care Act, vasectomies are not required to be covered like so many forms of female birth control (including sterilization) are. The procedure's nickname, "the snip," also makes it sound barbaric, when in fact, it's a generally safe, low-risk procedure.
While men are starting to catch on, vasectomies are still not the cultural norm in the U.S. "Vasectomies are still the fourth most common form of contraception, after oral contraceptives, condoms, and tubal ligation," Puneet Masson, M.D., assistant professor of urology and the director of male fertility at the University of Pennsylvania, tells SELF. But when comparing family planning options, male sterilization is one of the safest, cheapest, and most effective.
A vasectomy is a quick, low-risk procedure, with permanent—yet reversible—results.
Most vasectomies can also be reversed. The chance of a successful reversal varies depending on how the original procedure was done, but ranges anywhere from around 40 percent to over 90 percent.
Vasectomies aren't always 100 percent effective, but the failure rate is lower than even the most effective methods of female contraception.
Depending on the technique used, the chance a vasectomy will fail (aka, the man will get someone pregnant post-surgery) is anywhere from 0.3 percent to 9 percent in the first six months after the procedure. That's usually because it takes a few months for sperm to be fully out of the system—doctors suggest using another form of birth control until a follow-up analysis shows there's no sperm left in the seminal fluid. After that, the failure risk is between 0.04 percent and 0.08 percent (about 1 in 2,000).
The failure rate of an IUD, one of the very best forms of reversible birth control available to women, is between 0.2 and 0.8 percent—an order of magnitude higher. After a tubal ligation, nearly 1 percent of women will get pregnant in the first year, according to the Mayo Clinic, which is not just inconvenient, but dangerous. If you conceive after having the procedure, it can result in an ectopic pregnancy, a complication that's life-threatening for the woman if it's not caught early. Tubal ligation can also cost up to six times as much as a vasectomy, though it is more likely to be covered by insurance.
As of now, getting a vasectomy is the one good way men can take on the family planning responsibility.
While they're still trying to find a male birth control that works and is worth the side effects, vasectomies remain the one solid way a man can take on the medical responsibilities of family planning.
Vasectomies aren't just for couples who are done having kids. They're also an option for those committed to living child-free. Historically, there was a stigma about men who were child-free and opting for a vasectomy, Masson says. "Perhaps there was the belief that they would engage in unprotected sexual relations with multiple partners or that they were making an immature and rash decision about future family planning."
Masson explains that today, it's understood that some men and couples have decided on a child-free life or suffer from medical conditions that would make childbearing highly complicated and/or life-threatening to the mother or child. "For this reason, as a society, we are respecting a person's ability to make his or her own healthcare decisions. I have personally performed many vasectomies on men and/or couples who have decided that they are not interested in having children," says Masson.
A study conducted at Northwestern University shows that in challenging economic times, particularly when unemployment rates go up, there are higher rates of vasectomies. It makes sense—vasectomies cost anywhere from a couple hundred to about $1,500, and sometimes are covered by insurance. Kids cost much more than that.
Some doctors say they are seeing more men asking for vasectomies—a sign that maybe things are shifting, albeit slowly.
Masson says that he's performing more vasectomies annually and believes that the reason is because there is greater awareness about the safety and availability of the procedure. "Men are having these conversations with their friends. Additionally, there seems to be a greater public awareness for men's health, especially with men taking responsibility for their own reproductive health," he says. There are about 50 million men who've undergone vasectomies worldwide and approximately 500,000 in the U.S. who undergo a vasectomy every year.
Vasectomies are common enough that "VasMadness" has been coined to describe one of the most popular times for the procedure: during the NCAA basketball tournament. Masson says that because men are advised to relax on the couch with an ice pack (or bag of frozen peas) on their groin after a vasectomy, there has been an appeal to have one performed during one of the popular televised sporting events of the year. "I personally do a high volume of vasectomies during the entire March Madness season. I actually opened up extra days specifically for this procedure to accommodate the demand and men reserve these days months in advance," he says. He sees the same interest around Super Bowl and Thanksgiving football games, too. With all of that ball talk, it certainly seems appropriate.
And still, as ob/gyn Jen Gunter writes, only 5 percent of American men have had a vasectomy, while 15 percent of American women have had their tubes tied—and many, many more rely on IUDs, implants, diaphragms, rings or birth control pills (not to mention emergency contraception and abortion) to control their reproductive futures. As equality in parenting becomes increasingly normalized, here's hoping that men will start to take on a greater role in not parenting, too.


On This England, revealing that this 'heritage' quarterly which favours cottages, steam engines, choirboys, and old shephered's smocks, also has a toxic undercurrent connecting it to the far right.
columnist, shortly after the murder of Jamie Bulger.
Published as the 'Monday Profile' in the Guardian, 27 February 1993.


Whether you are looking for replacement elements, original elements, original filter assemblies, European & Japanese replacements or machine tool replacement elements B-Line Filter is your one stop shop!
®The names listed above are registered trademarks of their respective companies. No warranties are expressed or implied.


Cancer is a group of more than 100 different diseases. Benign tumours are not cancer; malignant tumours are cancer. most cancers are named for the type of cell or the organ in which they begin. When cancer spreads (metastasizes), the new tumour has the same name as the original (primary) tumour. Skin cancer is the most common type of cancer for both men and women. The second most common cancer in men is prostate cancer, in women it is breast cancer. Lung cancer is the leading cause of death from cancer for both men and women in the U.S. Cancer is NOT contagious.


text:
Efficiency & Environment, Technology, Top Stories
Overhead electric lines help emissions reductions keep on truckin'
Siemens' eHighway technology has been put into action on a 6.2-mile stretch of the autobahn in Germany
Image: Siemens
Overhead lines to power electric trucks have been put into action on a 6.2-mile stretch of the autobahn in Germany.
The German Government says the first test of the eHighway system on a public road began earlier this week – developed by Siemens, the technology allows trucks with special equipment mounted on their roofs to connect to overhead electrified lines while driving at speeds up to 56 miles per hour.
The section of road links Frankfurt airport, a global freight hub and a nearby industrial park – there are plans to launch the technology on two other stretches of autobahn in the near future.
The trucks run on electric motors when connected to the overhead lines and use a hybrid system when they disconnect, resulting in a significant reduction in emissions of carbon dioxide and nitrogen dioxide over the course of their journey.
Siemens says the model can be integrated with existing road infrastructure, making it a practical way to reduce emissions and energy consumption, and predicts the system means a truck operator could save around €20,000 (£17,200) on fuel costs over 62,000 miles travelled.
electric electrification germany overhead Siemens trucks


one bedroom apartments in dc one bedroom apartments in mo with utilities included for modern house new apartments under in dc one bedroom apartments nw dc.
small apartment living room furniture living room for small apartment home step living room design and decorating on budget small apartment living room furniture arrangement.
small apartment decorating ideas living room medium size of living apartment decorating ideas living room small scale sectional sofas small apartment living room decorating ideas pictures.
apartments near washington dc two and three bedroom apartments dc craigslist basement apartments washington dc.
2 bedroom apartments nyc large size of bedroom apartments full size bedroom ideas awesome apartments 2 bedroom apartments for sale in manhattan nyc.
interior design ideas for small apartments medium size of living studio apartment design simple interior design for small house interior design ideas for small apartments in india.
interior design living room apartment medium size of living living room furniture apartment living room layout apartment ideas interior design ideas living room apartment india.
one bedroom apartment washington dc bedroom amazing one bedroom apartment dc intended for h street apartments in d c 2 bedroom apartments in washington dc all utilities included.
1 bedroom apartments for rent nyc 2 bedroom apartments for rent new one bedroom apartments for rent 1 bedroom apartment 1 bedroom apartments in new york for rent.
1 bedroom apartments in dc wonderful 1 bedroom apartments dc low income 1 bedroom apartments in washington dc.


text:
Now Representing Sebastian ErraZuriz
R & Company is pleased to announce representation of Sebastian ErraZuriz. Renowned for his innovative approach as an artist, designer, and activist, ErraZuriz challenges traditional definitions of art and design–mixing genres, techniques, and disciplines. ErraZuriz's experimental practice is informed by his desire to provoke conversation and awareness even if these elicit controversy. His expansive body of work ranges from provocative public art to functional sculpture and furniture design. As such, ErraZuriz's interdisciplinary approach subverts conventional categorization, and invites the viewers to consider the ways in which any work can be simultaneously both conceptual and functional.
"We are thrilled to represent Sebastian's mechanical furniture and conceptual lighting," states Evan Snyderman, co-founder of R & Company. "His meticulous craftsmanship, which is mostly executed in his Brooklyn studio, paired with his unique brand of conceptual design epitomizes the exceptional quality, storytelling and visionary thinking we look for in an artist."
ErraZuriz states, " R & Company is always willing to experiment and try new things while challenging the artists and designers they represent to push their own boundaries. This push to break through the barriers of what is expected from an artist's repertoire represents a common passion we share with R & Company. In the same manner as I find it fascinating to question the limits of technical craftsmanship and mechanical ingenuity, I also feel compelled to break free from the traditional palette of materials an artist is expected to work with."
Born in Chile and raised in London, NY based artist and designer Sebastian ErraZuriz earned a degree in design in Santiago and a Master of Fine Arts from New York University. ErraZuriz's work has been exhibited internationally and resides in an array of permanent museum collections from the Cooper Hewitt, National Design Museum in New York to the Kiasma Museum of Contemporary Art in Helsinki.
"Sebastian's work is saturated with the history of art," notes James Zemaitis, Director of Museum Relations. "His 2014 retrospective at the Carnegie Museum of Art was a dazzling portrait of a young designer willing to try anything, and our intent at R & Company is to collaborate with him on several specific categories in his design practice, such as his ingenious mechanical furniture and its connections to European furniture makers of the 17th and 18th Centuries."
Sebastian ErraZuriz will premier his Bird Series at R & Company's booth at Expo Chicago from September 27 – 30. ErraZuriz states "The series places a focus on a body of work that has always captivated audiences. Like a precarious juggling act, these avary lamp sculptures manage to juggle between the absurd and the humorous, the morbid and the disgusting, the prohibited and the naif."
A selection of ErraZuriz's functional sculptures and experimental furniture designs can now be found at R & Company.


text:
Q: Make elements show above carousel I have a carousel, using owlCarousel, and I'm trying to make the elements in the carousel to expand on hover. The way it's implemented, is it's simply displayed: none by default, then on hover, it's displayed to block. Nothing fancy.
It's taken out of the flow by an absolute positioning, this way the carousel will not expand on element hover.
The problem is, when the element get's hovered, the details, expanded element doesn't show. I tried giving it a high z-index, but it doesn't seem to fix the problem. Here's the code:
CodePen FIle

$('.owl-carousel').owlCarousel({
  loop: true,
  margin: 10,
  nav: true,
  responsive: {
    0: {
      items: 1
    },
    600: {
      items: 3
    },
    1000: {
      items: 5
    }
  }
})
body {
  background-color: teal;
}

.owl-carousel {
  background-color: orange;
}

.owl-carousel .item:hover .details {
  display: block;
}

.owl-carousel .item-inner-wrapper {
  position: relative;
}

.owl-carousel h4 {
  background-color: yellow;
  height: 100px;
}

.owl-carousel .details {
  background-color: pink;
  height: 300px;
  position: absolute;
  top: 100%;
  bottom: 0;
  right: 0;
  left: 0;
  display: none;
  z-index: 20;
}
<link href="https://cdnjs.cloudflare.com/ajax/libs/OwlCarousel2/2.3.4/assets/owl.theme.default.css" rel="stylesheet" />
<link href="https://cdnjs.cloudflare.com/ajax/libs/OwlCarousel2/2.3.4/assets/owl.carousel.css" rel="stylesheet" />

1

        This is some crazy cool details that you will have to know about

2

        This is some crazy cool details that you will have to know about

3

        This is some crazy cool details that you will have to know about

4

        This is some crazy cool details that you will have to know about

5

        This is some crazy cool details that you will have to know about

6

        This is some crazy cool details that you will have to know about

7

        This is some crazy cool details that you will have to know about

8

        This is some crazy cool details that you will have to know about

9

        This is some crazy cool details that you will have to know about

10

        This is some crazy cool details that you will have to know about

11

        This is some crazy cool details that you will have to know about

12

        This is some crazy cool details that you will have to know about

A: See if this will work for you:

*

*Set .owl-carousel .item to your content height + detail height (I used 200px)

*Set margin-top of .owl-carousel.owl-theme .owl-nav to -(detail height) + 10px (it was originally 10px)

$('.owl-carousel').owlCarousel({
  loop: true,
  margin: 10,
  nav: true,
  responsive: {
    0: {
      items: 1
    },
    600: {
      items: 3
    },
    1000: {
      items: 5
    }
  }
})
body {
  background-color: teal;
}

.owl-carousel {
  background-color: orange;
}

.owl-carousel .item {
  height: 200px;
}

.owl-carousel .item:hover .details {
  display: block;
}

.owl-carousel .item-inner-wrapper {
  position: relative;
}

.owl-carousel h4 {
  background-color: yellow;
  height: 100px;
}

.owl-carousel .details {
  background-color: pink;
  height: 100px;
  position: absolute;
  top: 100%;
  right: 0;
  left: 0;
  display: none;
}

.owl-carousel.owl-theme .owl-nav {
  margin-top: -90px;
}
<link href="https://cdnjs.cloudflare.com/ajax/libs/OwlCarousel2/2.3.4/assets/owl.theme.default.css" rel="stylesheet" />
<link href="https://cdnjs.cloudflare.com/ajax/libs/OwlCarousel2/2.3.4/assets/owl.carousel.css" rel="stylesheet" />

1

        This is some crazy cool details that you will have to know about

2

        This is some crazy cool details that you will have to know about

3

        This is some crazy cool details that you will have to know about

4

        This is some crazy cool details that you will have to know about

5

        This is some crazy cool details that you will have to know about

6

        This is some crazy cool details that you will have to know about

7

        This is some crazy cool details that you will have to know about

8

        This is some crazy cool details that you will have to know about

9

        This is some crazy cool details that you will have to know about

10

        This is some crazy cool details that you will have to know about

11

        This is some crazy cool details that you will have to know about

12

        This is some crazy cool details that you will have to know about

A: You can try not giving a top value, and instead a height of auto to .details

$('.owl-carousel').owlCarousel({
  loop: true,
  margin: 10,
  nav: true,
  responsive: {
    0: {
      items: 1
    },
    600: {
      items: 3
    },
    1000: {
      items: 5
    }
  }
})
body {
  background-color: teal;
}

.owl-carousel {
  background-color: orange;
}

.owl-carousel .item:hover .details {
  display: block;
}

.owl-carousel .item-inner-wrapper {
  position: relative;
}

.owl-carousel h4 {
  background-color: yellow;
  height: 100px;
}

.owl-carousel .details {
    background-color: pink;
    position: absolute;
    bottom: 0;
    right: 0;
    left: 0;
    display: none;
    height: auto;
}
<link href="https://cdnjs.cloudflare.com/ajax/libs/OwlCarousel2/2.3.4/assets/owl.theme.default.css" rel="stylesheet" />
<link href="https://cdnjs.cloudflare.com/ajax/libs/OwlCarousel2/2.3.4/assets/owl.carousel.css" rel="stylesheet" />

1

        This is some crazy cool details that you will have to know about

2

        This is some crazy cool details that you will have to know about

3

        This is some crazy cool details that you will have to know about

4

        This is some crazy cool details that you will have to know about

5

        This is some crazy cool details that you will have to know about

6

        This is some crazy cool details that you will have to know about

7

        This is some crazy cool details that you will have to know about

8

        This is some crazy cool details that you will have to know about

9

        This is some crazy cool details that you will have to know about

10

        This is some crazy cool details that you will have to know about

11

        This is some crazy cool details that you will have to know about

12

        This is some crazy cool details that you will have to know about


How many times have you recalled a specific situation in your life and imagined what might have happened if it had played out differently than it actually had? What would have happened if you had introduced yourself to that one person? What if you took the other job offer you had? What if you could have experimented with these "what if" scenarios to see how they played out before they happened? If you were able to put yourself into the actual environment and were able to try different things, take different risks, even interact and exchange with other people (maybe even with other things) and know that you would be able to come back intact and unharmed at the end of it, how powerful would that be? Taking it a step further, once you found the outcome you liked best, you could make the decision to move forward? Wouldn't that be amazing? Think of it as Avatar meets Groundhog Day!
How many of us have dreamed of access to an augmented reality where we could control time, change how things happen, and experiment without the constraints of real world physics? The movement towards cloud technology is changing the level of abstraction we are operating in and IoT is completely transforming our environment; socially, technically and how we conduct business. Still, when it comes down to developing, integrating, testing and deploying electronics systems, we are often still challenged and frustrated by the scarcity of hardware to run on, inadequate tools for debugging and lack of automated tasks to produce seamless paths to collaborate cross our enterprise boundaries.
Imagine having your own virtual lab. We are hosting heterogeneous virtual systems where you can access, share and run software. You can experiment, develop, test, integrate and deploy virtual systems. It is cloud based, so no installation required. It scales efficiently and it's accessible from any device and from anywhere. It is user friendly, both in terms of the user experience and cost… based on a freemium model, anyone can have access to the basic service for free, so you can decide for yourself, at your own pace, what is worth paying for down the road. As an analogy of what Lab Cloud could do for software development, consider file sharing technologies such as Dropbox. Those types of offerings changed our behavior from sending files, to directly sharing and accessing files instead. Similarly, with Lab Cloud, you can enter a virtual workspace where you develop and run software on virtual target systems, and it can be shared with others who can also enter that virtual workspace. Or, to take another example – think about services like Spotify® and how it's changed the way we consume music. Now, we stream an endless pool of music instead of listening to a local file that we first had to acquire, which meant we had a pretty limited offering. With Lab Cloud you can consume unlimited numbers of virtual boards, instead of having to acquire, set up, manage, and maintain local, physical boards.
Now, Helix Lab Cloud won't make it possible to teleport yourself to a virtual world…we need more time for that However, it can transport you to a virtual lab, and we are so excited about it that we want to give folks access to an early preview. To find out how to create a free account, please visit this page. We are operating in an agile and continuous fashion, so new features and assets will be available frequently. I'm sure you will be pleasantly surprised with the new services we'll offer over time to our Lab Cloud users. Keep visiting Lab Cloud to see new capabilities as they become available.
Since our inception, Wind River has constantly changed how engineers, managers and companies think about their business. With Helix Lab Cloud, we believe that we are defining the future of system development in an IoT centric world!


text:
You are here: Home / IT & Infrastructure / Power Management & Distribution / Prysmian launches eco-friendly cabling technology
Prysmian launches eco-friendly cabling technology
July 2, 2019 By Louise Frampton Leave a Comment
Prysmian Group claims to have made a significant step in advancing cable technology to enable more efficient, reliable and eco-friendly power transmission over long distances.
After completing one-year qualification testing in accordance with international standards, the Group introduces two new 525 kV extruded land cable systems, one qualified with P-Laser and one with XLPE insulation. These cable systems are designed at a higher voltage level and with large conductor cross-sections to provide optimal technical solutions for long distance high power transmission with minimised land use.
P-Laser is described by the company as "the first 100% recyclable eco-friendly high-performance cable technology", utilising a 'zero-gas' process which reduces CO2emissions by up to 30%*. P-Laser is fully compatible with existing HVDC cables and accessories and has over 30,000 km manufacturing experience in other types of power cable networks.
The P-Laser qualified cable system employs a Prysmian in-house developed material, called HPTE (High Performance Thermoplastic Elastomer) offering increased thermal performance and higher intrinsic reliability. The XLPE qualified cable system uses a new insulation compound specific for HVDC applications. Both technologies have also successfully passed type tests at 600 kV and represent the next generation solutions for land cable systems that underpin Prysmian Group's ability to provide reliable systems for the challenges of power transmission.
"This new milestone is a significant step forward for power transmission systems and the development of innovative and sustainable cable solutions in the industry," declared Hakan Ozmen, EVP, Projects Business Unit, Prysmian Group. "The 525 kV cable systems can be an effective solution for the planned German HVDC Corridor projects, providing the TSOs (TenneT, 50Hertz, TransnetBW and Amprion)with two proven technologies able to connect the wind generation-rich regions of northern Germany to the major consumption areas in the South, reducing the required land usage and ensuring a lower environmental impact," concluded Ozmen.
Prysmian Group is playing a key role in the connection of German offshore wind farms to the mainland, having supplied and installed multiple turnkey HVDC & HVAC systems across the German waters, with a track record of 4,100 km of HVDC submarine and land cables and more than 1,000 installed cable accessories.
Filed Under: Power Management & Distribution
Is battery technology on the verge of a blue period?
Why a poor power factor is brewing business trouble
Market report shows increasing demand for data centre power equipment
Protecting a UPS during maintenance bypasses
Why UPS needs to be Li-ion ready
Colt announces expansion at London North data centre
Why make the switch to DC power?
Managing energy risk strategies


text:
HomeBlogMore outrage over Catholic churches moving accused priests around
More outrage over Catholic churches moving accused priests around
On behalf of Soloff & Zervanos, P.C. Posted in Sexual Abuse on Wednesday, January 27, 2016.
In one of our posts last week, we wrote about an unfolding story in the Midwest involving a former Catholic archbishop. Although the incident did not happen here in Pennsylvania, similar incidents have happened here and in many other parts of the country.
In mid 2015, John Nienstedt resigned as the Archbishop of the Archdiocese of Minneapolis and St. Paul. There is much evidence to suggest that Nienstedt knew about credible sex abuse allegations against priests, yet failed to take any corrective or preventive action. Much of this evidence was revealed during the discovery period for numerous lawsuits against the archdiocese. Nienstedt continues to deny any wrongdoing.
Earlier this month, a priest in Michigan casually mentioned to parishioners that Nienstedt would be an occasional substitute at the church over the next six months while the regular priest attended to health issues. Nienstedt's recent and very controversial past was not mentioned, but it did not take long for the community to discover the truth.
Late last week, public outrage led to Nienstedt's removal from his temporary assignment. But the move was not enough to satisfy protest groups, including the Survivors Network of those Abused by Priests (SNAP). According to news sources, protestors want the local diocese to take several actions, including:
Holding a public meeting to talk about why Nienstedt was allowed to transfer there
Punishing the priest who invited Nienstedt to come without warning parishioners
Revealing whether there are any other "sexually troubled or complicit clerics" serving within the diocese
SNAP has long been instrumental in advocating for victims and holding the church accountable for its actions. But the fact that a group like SNAP even exists is evidence of just how pervasive clergy sexual abuse has been and continues to be. And while the Catholic Church is not the only religious institution affiliated with child sexual abuse, the church's top-down authority structure makes it especially difficult to hold offending priests accountable.
Hopefully, the outrage shown over this incident is a sign that American Catholics will no longer tolerate the institutional obstructionism that allows religious leaders to sexually abuse children.


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

The Galactic center region is one of the richest regions in sources of the Milky Way. Numerous X-ray~ binaries, massive stellar
clusters and supernova remnants (hereafter, SNRs) lie in this complex region, immersed in an extended high-temperature plasma which
heavily dominates the global soft X-ray~ emission \citep{c:koyama96}. Recently, a diffuse X-ray~ source, G0.570-0.018, was detected
with {\it ASCA}~ and confirmed with {\it Chandra}~ observations. The X-ray source has a ring-like structure, about 10$^{\prime\prime}$~in radius, with a
spectrum that can be fitted by a thermal emission model with a temperature of about 6\un{keV} \citep{c:senda02}. The high value
derived for N$_{H}$ ($\sim$ 10$^{23}$ cm$^{-2}$) is consistent with a source located near the Galactic center, at a distance of about
8 kpc. Based on the detection of an iron line with a high equivalent width at 6.5\un{keV} and a high Fe abundance (suggesting a recently
shocked plasma), the authors concluded that the origin must be a very young SNR with an age of $\sim$ 80 yr. However, based on
the analysis in the {\it Chandra}~ image of a faint east-west X-ray tail possibly related to G0.570-0.018, they conclude that it
could be about twice older. In a SNR scenario, we might expect non-thermal radio continuum emission from shock-accelerated electrons
and the presence of $\gamma$-ray~ lines associated with the decay of \titane{Ti}. This radioactive nucleus is thought to be exclusively
produced in supernova (hereafter, SN) explosions. It is primarily generated in the $\alpha$-rich freeze-out from nuclear statistical
equilibrium occurring in the explosive silicon burning stage of core-collapse SNe ({\it e.g.~} Woosley \& Weaver 1995), while a normal
freeze-out Si burning is at play in Type Ia SNe \citep{c:thielemann86}. The radioactive decay chain
\titane{Ti}$\longrightarrow$\titane{Sc}$\longrightarrow$\titane{Ca}, with a lifetime of about 87.5 yr \citep{c:wietfeldt99},
produces three $\gamma$-ray~ lines at 67.9\un{keV}, 78.4\un{keV} (from \titane{Sc}$^{\star}$) and at 1157\un{keV}
(from \titane{Ca}$^{\star}$) with similar branching ratios. It has been shown that \titane{Ti} may reveal young galactic SNRs
that could be hidden from our view at optical wavelengths due to heavy extinction in the Galactic plane region. \titane{Ti} $\gamma$-ray~
lines have been observed in the young SNRs Cassiopeia~A (Iyudin et~al.~ 1994; Vink et~al.~ 2001; Vink 2005) and RXJ~0856-4622
\citep{c:iyudin98}. Moreover, the radio data can provide information on the interaction of the blast wave with the circumstellar
and local interstellar media. G0.570-0.018 is then an ideal case to search for specific signatures of young SNe such as the
\titane{Ti} lines and the radio non-thermal radiation by combining both observations as early proposed by Silberberg et~al.~ (1993).

In this paper, based on the {\it INTEGRAL}~ (IBIS/ISGRI, section \ref{s:isgri}) and VLA\footnote[1]{The Very Large Array of the National Radio
Astronomy Observatory is a facility of the NSF operated under cooperative agreement by Associated Universities Inc.} (section
\ref{s:radio}) data, we investigate if G0.570-0.018 is indeed a young SNR. If this is the case, its possible type and characteristics
are discussed in section \ref{s:discuss} at the light of all available observationnal and theoretical material.

\section{{\bf INTEGRAL} \& VLA observations}
\label{s:obs}

The INTErnational Gamma-Ray Astrophysics Laboratory {\it INTEGRAL}~ \citep{c:winkler03} is an ESA mission carrying two main telescopes
based on a coded aperture imaging system: IBIS~ \citep{c:ubertini03} and SPI~ \citep{c:vedrenne03}. IBIS~, with its soft $\gamma$-ray~
(15\un{keV} - 1\un{MeV}) imager ISGRI~ \citep{c:lebrun03}, provides the finest imaging (13$^\prime$ ~FWHM) and the best line sensitivity up
to a few hundred\un{keV}. It is therefore best suited for a search for the two low energy \titane{Ti} lines and we only analyzed data
from this instrument. {\it INTEGRAL}~ is mainly devoted to the observation of galactic sources and spends considerable amount of time pointing
towards the Galactic plane and the Galactic center regions. We performed the analysis of data from the Galactic Center Deep Exposure
(GCDE) of the Core Program, acquired during the first two years of {\it INTEGRAL}~ operations. In a search for the radio counterpart for
G0.570-0.018, we have reprocessed archival VLA data at $\lambda$ 20\un{cm} and 6\un{cm} from different pointings where this source
was within the field of view. We have also analyzed the 90\un{cm} intermediate resolution VLA image of the Galactic center from
LaRosa et~al.~ (2000).

\section{Analysis and Results}
\label{s:res}

\subsection{$^{44}$Ti $\gamma$-ray~ lines}
\label{s:isgri}
\clearpage
\begin{figure*}[htb]
\epsscale{1.0}
\begin{center}
\includegraphics[scale=0.5, angle=0]{f1.eps}
\end{center}

\caption{IBIS/ISGRI contour map in Galactic coordinates of the combined significance
in the ranges of the two low energy \titane{Ti} lines. Contours are drawn from 3 to 100
using a square root scale. The continuum emission of several known bright sources is
clearly detected while there is no evidence of any emission coming from G0.570-0.018
above the 3$\sigma$ level.\label{f:44Ti_ima}}

\end{figure*}
\clearpage
Both {\it ASCA}~ and {\it Chandra}~ observations of G0.570-0.018 present a thermal X-ray~ spectrum, without any evidence of synchrotron radiation.
It is therefore highly improbable to detect this source with IBIS~ in the hard X-ray~ continuum, above 15\un{keV}. Besides, as revealed
by IBIS/ISGRI, the Galactic center region is a crowded area at hard X-ray~ energies \citep{c:belanger05}, making it more difficult to
precisely distinguish the part of the emission which could be associated with this source. In fact we did not find any evidence of
such emission in the 20-40\un{keV} mosaic presented in B{\'e}langer et~al.~ (2005). We analyzed pointings where G0.570-0.018 lies within
the field of view of IBIS~ ($\le$ 15$^\circ$), in the 65-71 and 75-82\un{keV} energy bands centered on the two low energy \titane{Ti}
$\gamma$-ray~ lines, using the Off-Line Scientific Analysis (OSA) software version 4.2 \citep{c:goldwurm03}. These narrow bandwidths take
full advantage of the ISGRI~ energy resolution ($\sim$ 6\un{keV} FWHM at 70\un{keV}). The critical point in the analysis of the
IBIS/ISGRI data is the background subtraction: we have generated background shadowgrams (detector image containing the shadow of the
coded mask onto the ISGRI~ detector) by analyzing and summing a large part of the high-latitude and empty field observations performed
during the first two years of the mission in 256 energy bands. The high total exposure time ($\sim$ 2\un{Ms}) warrants the best
removal of structures in the detector images \citep{c:terrier03}, mainly around the K$_{\alpha}$ and K$_{\beta}$ fluorescence lines of
the W (59 and 65\un{keV}) and Pb (75 and 85\un{keV}) located close to the two low energy \titane{Ti} astrophysical lines. This
method provides flat background-subtracted detector images in any desired energy band. Thus, the convolution of these shadowgrams
with a decoding array derived from the spatial characteristics of the coded mask produces good quality reconstructed sky images. We
finally obtained two mosaic images in these two energy bands and combined both to increase the signal-to-noise ratio. The resulting
mosaic is shown in Figure \ref{f:44Ti_ima}, with a final exposure time towards the source of about 4.3 Ms.

We found no evidence for any emission above 3$\sigma$ from G0.570-0.018 in the \titane{Ti} $\gamma$-ray~ lines range and estimated an
upper limit of 1.2 $\times$ 10$^{-5}$ cm$^{-2}$ s$^{-1}$ at the 3$\sigma$ confidence level. This can be converted into an upper limit
on the \titane{Ti} yield via the following equation:

\begin{equation}
Y_{44}=1.38\times{\left[\frac{F_{\gamma}}{\mathrm{cm}^{-2}~\mathrm{s}^{-1}}\times{\left(\frac{d}{1~\mathrm{kpc}}\right)^{2}}\times{e^{t/\tau_{44}}}\times{\frac{\tau_{44}}{1~\mathrm{yr}}}\right]\times{10^{-4}~\mathrm{M}_{\odot}}}
\end{equation}

where Y$_{44}$ is the \titane{Ti} yield, F$_{\gamma}$ the \titane{Ti} line flux and $\tau_{44}$ the \titane{Ti} lifetime $\sim$ 87.5 yr
\citep{c:wietfeldt99}. Assuming that G0.570-0.018 is located near the Galactic center region, a distance of 8 kpc is adopted
\citep{c:eisenhauer03}. Based on this assumption, we obtained the relation between the maximal \titane{Ti} yield and the age of
this source presented in Figure \ref{f:y_age}.
\clearpage
\begin{figure}[htb]
\epsscale{1.0}
\begin{center}
\includegraphics[scale=0.45, angle=0]{f2.eps}
\end{center}

\caption{3$\sigma$ upper limit on the \titane{Ti} yield (in units of
10$^{-4}$~$\mathrm{M}_{\odot}$) as a function of the age (in years).
The dashed region corresponds to the range of parameters excluded at
the 3$\sigma$ confidence level.\label{f:y_age}}

\end{figure}
\clearpage
For an age of 80 yr, our 3$\sigma$ upper limit on the \titane{Ti} ejected mass is $\sim$ 2 $\times$ 10$^{-5}$ $\mathrm{M}_{\odot}$.
One should notice that this value is $\sim$ 8 times lower than that of the youngest known SNR Cassiopeia~A (hereafter, Cas~A) derived
from {\it GRO}/COMPTEL \citep{c:iyudin94}, {\it BeppoSAX}/PDS \citep{c:vink01} and IBIS/ISGRI \citep{c:vink05} observations. This result is
discussed in detail in section \ref{s:discuss}.

\subsection{Radio emission}
\label{s:radio}
\clearpage
\begin{figure*}[htb]
\epsscale{1.0}
\begin{center}
\includegraphics[scale=0.8, angle=0]{f3.eps}
\end{center}

\caption{Radio images of a $\sim$ 7$^\prime$~field around G0.570-0.018 at
$\lambda$ 90\un{cm} {\bf (a)}, 20\un{cm} {\bf (b)} and 6\un{cm} {\bf (c)}.
The contours represent X-ray emission convolved with a gaussian beam
of 13$^{\prime\prime}$ $\times$ 8$^{\prime\prime}$. The greyscale varies between 0 and 150 mJy/beam
at 90\un{cm}, between -5 and 10 mJy/beam at 20\un{cm}, and between -10
and 40 mJy/beam at 6\un{cm}.\label{f:radio_im}}

\end{figure*}
\clearpage
The image at 20\un{cm} was obtained from archival data corresponding to observations carried out using the VLA in the hybrid CnB
configuration for about 1.5 hours on 2004 February. The data were processed under the MIRIAD software package \citep{c:sault95}
following standard procedures. The resulting synthesized beam is 13$^{\prime\prime}$ $\times$ 8$^{\prime\prime}$, PA=54.6, and the average rms noise of the order
of 2.5 mJy/beam. The largest scale structure accessible to this array is of about 5$^\prime$. A field around G0.570-0.018 is shown in Figure
\ref{f:radio_im}b, with a few contours superimposed representing the {\it Chandra}~ X-ray~ emission smoothed to the same angular resolution
as the radio image. Correction for primary beam attenuation was applied.

To produce the image at 6\un{cm} we used archival data from observations carried out with the VLA-D array during 45 minutes on 2003
April 30. The synthesized beam is 27$^{\prime\prime}$ $\times$ 11$^{\prime\prime}$, PA=-5.2 and the average rms noise in the field, about 2.2 mJy/beam. The
resulting image is displayed in Figure \ref{f:radio_im}c, again with {\it Chandra}~ X-ray~ contours overlapped.

The image shown in Figure \ref{f:radio_im}a at 90\un{cm} was extracted from the 4$^\circ$ $\times$ 4$^\circ$~image of the center of the Galaxy
obtained with the VLA B, C and D configurations (LaRosa et al. 2000). The angular resolution of these data is 48$^{\prime\prime}$ $\times$
48$^{\prime\prime}$~and the rms sensitivity of 5.9 mJy/beam. The largest angular scale to which this image is sensitive is approximately 45$^\prime$.

From these images, it is apparent that G0.570-0.018 lies on a region with tenuous, smooth radio emission. Not any conspicuous
radio feature can be associated with the X-ray~ source at any frequency up to the limit of the angular resolution and sensitivity
of these images. An upper limit for the flux densities at 90 and 20\un{cm} can be estimated by integrating the radio emission over a
region with the size of the outer X-ray~ contour. From this integration we estimate: S$_{\rm 90\un{cm}} \sim 0.23$ Jy and
S$_{\rm 20\un{cm}} \sim 0.066$ Jy. Although the flux contribution from large-scale structures was not added to these images, the flux
density estimates are reliable within observational errors because the size of the studied structure is smaller than the largest well
imaged structure at the respective frequencies. This is not the case for the emission at 6\un{cm}, thus it was not possible to
accurately estimate the flux density at this short wavelength.

\section{Discussion}
\label{s:discuss}

The X-ray~ morphology and spectra of G0.570-0.018 show a hot-temperature plasma distributed in a ring-like structure, two
characteristic features of young ejecta-dominated SNRs. In this context, we attempted to shed further light on the nature of this
source searching for  \titane{Ti} $\gamma$-ray~ lines and radio continuum emission. However, to our surprise neither the \titane{Ti}
$\gamma$-ray~ lines observations nor the radio continuum maps reveal any feature that can be ascribed to G0.570-0.018 at the levels of
sensitivity presented above.

Concerning SNe nucleosynthesis products such as \titane{Ti}, presupernova evolutions and calculations of explosive yields have a long
history. Recently, core-collapse SNe have been studied by Woosley \& Weaver (1995), Thielemann et~al.~ (1996), Rauscher et~al.~ (2002,
hereafter RHHW02) and Limongi \& Chieffi (2003, hereafter LC03) while nucleosynthesis in Chandrasekhar mass models for Type Ia SNe can
be found in Iwamoto et~al.~ (1999). The \titane{Ti} yields used in this paper were extracted from those obtained by RHHW02 and LC03
since their calculations include several improvements in stellar physics and revised nuclear reaction rates. Figure \ref{f:models}
shows these \titane{Ti} yields as a function of the energy of the explosion, for different masses of the progenitor with our
3$\sigma$ upper limit for the two possible ages of G0.570-0.018.
\clearpage
\begin{figure}[htb]
\epsscale{1.0}
\begin{center}
\includegraphics[scale=0.5, angle=0]{f4.eps}
\end{center}

\caption{\titane{Ti} yield (in units of 10$^{-4}$~$\mathrm{M}_{\odot}$)
versus the energy of the explosion (in units of 10$^{51}$ erg) for two
sets of nucleosynthesis calculations in Type II SNe: triangles represent
those of Limongi \& Chieffi (2003) and squares those of Rauscher et~al.~ (2002).
Each color is related to the mass of the progenitor. Horizontal lines
represent our 3$\sigma$ upper limit for two different ages of G0.570-0.018.
\label{f:models}}

\end{figure}
\clearpage
Explosive yields are sensitive to many details of the explosion and in the case of core-collapse SNe, \titane{Ti} is thought to
be created close to the mass-cut (the mass above which the matter falls back onto the compact remnant). From Figure \ref{f:models} it
can be seen that for each track of constant progenitor mass, the higher is the energy of the explosion, the larger is the ejected
mass of \titane{Ti}. For an age of 80 yr, our 3$\sigma$ upper limit is only compatible with few models of core-collapse SNe, where
the energy is unsufficient to eject an amount of \titane{Ti} above 2 $\times$ 10$^{-5}$~$\mathrm{M}_{\odot}$. We also considered the
expected \titane{Ti} yields in various Chandrasekhar mass models for SNIa explosions (Iwamoto et~al.~ 1999 and references therein). In
these models, explosive nucleosynthesis is calculated for a variety of deflagration speeds and ignition densities. We find that
``standards'' models (Nomoto et~al.~ 1984; Thielemann et~al.~ 1986) predict \titane{Ti} yields clearly below our 3$\sigma$ upper limit,
while delayed-detonation models with highly energetic explosions ($>$ 1.4 $\times$ 10$^{51}$ ergs) predict \titane{Ti} yields between
$\sim$ 3 and 4.5 $\times$ 10$^{-5}$~$\mathrm{M}_{\odot}$ which could be compatible only in the case where G0.570-0.018 is at least
two times older ($>$ 160 yr). The situation is worse in the case of sub-Chandrasekhar SNIa explosions where helium burns in a
detonation wave causing a detonation also in the interior of the white dwarf (Woosley et~al.~ 1986; Woosley \& Weaver 1994). In such
systems, substantial overproductions of \titane{Ti} from several 10$^{-4}$~$\mathrm{M}_{\odot}$ up to 4 $\times$
10$^{-3}$~$\mathrm{M}_{\odot}$ are expected and then well above our sensitivity. In summary, comparing our upper limits with various
models, we conclude that only few sub-energetic core-collapse or standard thermonuclear explosions predict \titane{Ti} yields
that explain our non-detection at the IBIS/ISGRI sensitivity.

From an observational point of view, the 1.157\un{MeV} \titane{Ti} $\gamma$-ray~ line was detected for the first time in Cas~A with
{\it GRO}/COMPTEL \citep{c:iyudin94}. Later, Vink et~al.~ (2001) reported the detection with {\it BeppoSAX}/PDS of the two low energy \titane{Ti}
lines in this SNR implying an initial \titane{Ti} mass of (0.8-2.5) $\times$ 10$^{-4}$~$\mathrm{M}_{\odot}$. Preliminary analysis
of the IBIS/ISGRI data on Cas~A yielded a detection of the 68 keV \titane{Ti} line with a flux consistent with the {\it BeppoSAX}~detections
\citep{c:vink05}. Moreover, it is suspected that the late-time light curve of SN~1987A ($\succeq$ 2000 days) is dominated by the
\titane{Ti} decay. From time-dependent models for the light curve in combination with broad band photometry, Fransson \& Kozma (2001)
estimated a \titane{Ti} mass of (0.5-2.0) $\times$ 10$^{-4}$~$\mathrm{M}_{\odot}$. On the other hand, Senda et~al.~ (2002) noticed
similarities between the X-ray~ structure of the ring of G0.570-0.018 and that of SN~1987A where strong stellar winds might produce a
gas ring being heated by SN ejecta. However, one can see from Figure \ref{f:y_age} that G0.570-0.018 should have been detected in the
\titane{Ti} $\gamma$-ray~ lines range if it had emitted yields comparable to those measured from Cas~A or those inferred from SN~1987A,
even in the worst case of considering the lower limits of \titane{Ti} yields, and the oldest age of 160 yr.

Concerning the radio observations, one can expect synchrotron emission coming from either initially accelerated or shock-accelerated
electrons and the non-observation at any radio frequency of G0.570-0.018 is then surprising. If G0.570-0.018 has an age of 80 yr, it
should be considered as an ``intermediate-age'' supernova (see Eck et~al.~ 2002 and references therein) evolving from SN to SNR.
G0.570-0.018, however, could be as old as 160 yr. With such an upper limit on the age, we cannot exclude that G0.570-0.018 is in the
SNR phase where the electrons responsible for the radio synchroton emission are accelerated at the shock front. The main difficulty
of the studies of radio emission from SNe/SNRs is that between the observed extragalactic radio SNe (hereafter, RSNe) and the youngest
known Galactic SNR (Cas~A), there is an observationnal gap of about 300 yr and then the evolution from RSN to SNR is poorly
understood. Type II SNe seem to be well described by Chevalier's models (Chevalier 1982a, 1982b, 1984) where the radio emission
is related to the circumstellar matter while that of older SNe, entering the SNR phase (predicted to take at least 100 yr), can be
related to the amount of interstellar matter (Gull 1973; Cowsik \& Sarkar 1984). Emission mechanisms in both cases are anyway
identical. Thus, we have divided our discussion in two parts, one considering that G0.570-0.018 is still a SN and an other assuming
that it could be a very young SNR.

In the first case, according to the Chevalier's model \citep{c:chevalier82b}, the flux of RSNe drastically depends on the ratio
between the mass-loss rate of the pre-SN progenitor and the wind speed. For small values, no strong radio emission is expected, thus
explaining why despite several searches ({\it e.g.~} Eck et~al.~ 1995), no Type Ia SNe have been detected in radio and why most of the
extragalactic SNe seen at radio wavelenghts (Weiler et~al.~ 2002) have progenitors with dense winds. Massive stars are thought to
experience strong mass losses during the final stages of their evolution implying that they would be bright radio sources. Our
non-detection in radio therefore points to the lower progenitor masses. Figure \ref{f:models} shows that for these lower masses, our
upper limit on the production of \titane{Ti} favours rather low energetic events. On the other hand, G0.57-0.018 could be similar to
the Type Ia SN~1885A in M31, the first extragalactic SN identified, where no radio emission has been found \citep{c:crane92}.

Now if we assume that G0.57-0.018 has an age of 160 yr, it can be considered as a very young SNR \citep{c:cowsik84}.
Recently, Asvarov (2000) developed a model based on the diffusive shock acceleration mechanism to explain radio emission of adiabatic
SNRs and compared its modeled Surface Brightness - Diameter ($\Sigma$ - D) evolutionary tracks with the empirical $\Sigma$ - D diagram.
He found that adiabatic SNRs evolve at nearly constant surface brightness: $\Sigma$ $\propto$ D$^{-0.5}$. We have used this relation
and compared the surface brightness of the historical SNRs Kepler, Tycho, Cas~A and SN~1006 (we exclude the Crab nebula and 3C58
because they are continuously fed by relativistic electrons from a central neutron star) as given by Green (2005) and scaled to an age
of 160 yr, with our upper limit at 20\un{cm}, $\Sigma \sim$ 2 $\times$ 10$^{-20}$ W m$^{-2}$ Hz$^{-1}$ sr$^{-1}$. The only concordance
found is with SN1006, suggesting that G0.570-0.018 might be a Type Ia SNR evolving in a low-density medium. This is consistent with
our upper limit on the \titane{Ti} yield, since standard Type Ia SNe produce in average less \titane{Ti} than core-collapse SNe, and
with its very low radio flux density. Although SNIa can be found at any location in spiral galaxies like the Milky Way, the location of
G0.570-0.018 within the disk and close to the Galactic center, which is known to host abundant molecular material and young stars
\citep{c:figer04}, makes the scenario of a core-collapse event more likely. In any case G0.570-0.018 must be located in a region
probably depleted by a succession of strong stellar winds of massive stars and/or previous SN explosions.

In any scenario of a SN/SNR, a possible explanation for the lack of radio emission can be the fact that G0.570-0.018 appears to be
evolving in a low density hot plasma. In such medium high Mach numbers shocks may not be formed, even if velocities are high, as the
sound speed in a hot plasma is also high. Such SNR shocks will not give rise to high compression ratios, and also shock acceleration
may be less efficient. Therefore, the radio emission may not be very strong. In addition, if the SNR shock expands within a bubble
blown out by the wind of the precursor star, the possibility of creating a radio synchrotron shell is even lower.

\section{Conclusion}
\label{s:conclusion}

In conclusion, the present $\gamma$-ray~ and radio observations have not solved the basic question if G0.57-0.018 is a genuine SN/SNR. If
it is, then our upper limits on the ejected \titane{Ti} mass and radio emission from G0.57-0.018 help to constrain its
characteristics: the weak production of \titane{Ti} rules out all the sub-Chandrasekhar Type Ia SN scenarios and can be explained if
G0.57-0.018 was a sub-energetic core-collapse supernova from a moderate mass progenitor or a standard thermonuclear explosion. Since
no Type Ia SNe in radio have been detected, the second scenario looks more likely although the location of G0.57-0.018, very close to
the Galactic center, might suggest a massive star progenitor. According to Chevalier's model, the very weak radio surface
brightness is probably due to the low-density surrounding medium. If the SN/SNR nature of G0.57-0.018 is questioned, then the X-ray~
morphology, the high Fe abundance and the position and width of the Fe line observed by Senda et~al.~ (2002) remain to be explained.
In any scenario of a young SN/SNR, G0.57-0.018 seems to be unusual and only the next generation of hard X-ray~/soft $\gamma$-ray~ focusing
telescopes, such as {\it SIMBOL-X}~ \citep{c:ferrando04}, will be in position to disentangle its nature.

\acknowledgements{M.R. gratefully thanks J. Paul for fruitful discussions and his various suggestions. The present work was supported
		 with action ECOS A04U03 and based on observations with {\it INTEGRAL}~, an ESA project with instruments and science data
		 center (ISDC) funded by ESA members states (especially the PI countries: Denmark, France, Germany, Italy, Switzerland,
		 Spain, Czech Republic and Poland, and with the participation of Russia and the USA). ISGRI~ has been realized and
		 maintained in flight by CEA-Saclay/DAPNIA with the support of CNES. S. P. is fellow of CONICET (Argentina). G. D. and
		 E. G. are members of the {\it Carrera del Investigador Cient\'\i fico} of CONICET (Argentina). This research was
		 partially funded by the UBACYT Grant A055 and by ANPCyT-PICT04-14018 (Argentina). A.M.B. was partially supported by
		 RBRF 03-04-17433 and 04-02-16595.}

redpajama_set_name: RedPajamaArXiv


Myth: I can only go into an English-related field with my degree.
Fact: An English degree opens doors and opportunities that do not have to follow a literary path.
When students take English courses here, they're learning more than just literature: they're learning to read critically, see subtext and write effectively. A common misconception is that English classes are based on the following formula: read a book and talk about it. On the contrary, the classes you take at Bemidji State go beyond such a simple stereotype.
You will read selections of Aristotle to see the beginnings of literary criticism, selections of Cicero to understand parts of classical rhetoric, the dramas of Shakespeare, novels by British, American, German and Native American authors, epic poets such as Homer and Milton, modern poetry with the likes of Walt Whitman and John Keats and that's just a start.
One of the unique aspects of earning an English degree, as opposed to a degree in science, is that you are not pigeon-holed into one or two career paths. You do not go to school for one specific career, but go to school to discover how you can mold and build a career path, with help from the English faculty, that fits perfectly with your newly gained skills and tastes. In addition, an English degree can serve as a foil for other degrees, particularly if you choose a career path that is not English-related.
A common example is a student pursuing degrees in both Mass Communications and English literature. The primary focus of the student may be in mass marketing, advertising or journalism, but regardless of the student's path, the English degree emphasizes the student's achievements and capabilities.
When you take courses here, you build for yourself a future that amalgamates the different paths and courses into a strong foundation for you to continually build on throughout all of academia and into your career path. English courses offer the opportunity to coexist with various other degrees as long as you see them coupled together, as opposed to separate and distinct areas of study.
Seeing them together paints the brightest, most detail-oriented picture. Do you want to see the picture and get 100% out of your time spent here, or just half? The choice, as always, is yours and yours alone.
Here is a compiled list of English majors you may have heard of.


School education for a child is the first exposure to gain knowledge. It helps us understand different cultures and helps us network better. Role of a school is to develop raw child to perfect.
Education is one of the important factors which formulate the persona of a person. Education is a productive and beneficial factor in a person's life. It is everyone's right to get.
The training of a human mind is not complete without school education. Only because of education a man is able to receive information from the external humanity, to notify him with past and receive all essential information concerning the present.


My name is Sarah Hamed and I run Jellybabyz from my home in the Glebe area of Washington, Tyne and Wear. I'm a registered childminder and have been described as 'caring and responsive childminder' by... Ofsted. I offer high quality childcare in a happy, welcoming and inclusive environment. I have over 14 years experience working with young children and believe that children learn best through play.


National Volunteer Week was established in 1974 and is celebrated all over our country in many different ways. According to handsonnetwork.org "It is about inspiring, recognizing and encouraging people to seek out imaginative ways to engage in their communities." Volunteers are very important to the HHH and I would like to recognize those who have chosen to share a little of their imaginative and caring ways with us.
Over the years the HHH Board of Directors has spent countless hours planning events to benefit the Home. They offer tours to remind guests of our history, they serve treats or meals to represent the spirit of hospitality that the Hormels were known for, and they consider ways in which the Home can continue to serve our community.
In the office we have people with great organizational and people skills who help keep things running smoothly. From scheduling tour guides, to arranging historical documents, to answering phone calls and selling tickets to events, they are priceless in helping us maintain a healthy organization. We also have friends who just like being here and will often tidy up and water the plants.
Another regular group of volunteers is the Y's Women. This group has met at the Home for 20 years, and they often volunteer at events such as our Holiday Open House and German Cookie Bake, and they even set tables for our Sweetheart Dinner. You will soon see a bit of their gardening work as they fill the window boxes on the west side of the Home.
Our volunteer Board of Trustees oversees the financial position of the HHH and develops long-range goals to help us remain vital to Austin. They oversee the administrative processes and ensure that positive business decisions are being made.
So although I am late in saying it, I am extremely grateful for those who have chosen to make the HHH their outlet for volunteer work. They do it because they recognize the value of a facility such as ours and they want to see it preserved. We wouldn't be able to accomplish what we do without them.


text:
The Lowdown: The Smiths
Pop in the 1980s was rocked to its foundations with the arrival of The Smiths in 1983. With their blend of Morrissey's misery and Johnny Marr's melodies, they became an…
The Lowdown: Michael Jackson
When Michael Jackson joined his brothers in The Jackson 5, a star was born. As a solo artist, he went on to become one of the world's most recognisable stars…
The Lowdown: Pet Shop Boys
A former Smash Hits journalist and an architecture student who never graduated, Pet Shop Boys went on to become the most successful UK duo ever, selling more than 50 million records worldwide…
The Lowdown: ABBA
Sweden's fab four got their big break at Eurovision in 1974 and went on to dominate the global pop landscape for the following eight years, shifting hundreds of millions of…
The Lowdown – Kate Bush
Ever since her memorable Top Of The Pops debut channelling a literary heroine in 1978, Kate Bush's career has been defined by her unassailable singularity. Classic Pop lends an ear to a prodigious back…


text:
Philip Reed also Philip Reid (c. 1820 – February 6, 1892) was an African American master craftsman who worked at the foundries of self-taught sculptor Clark Mills, where historical monuments such as the 1853 equestrian statue of Andrew Jackson in Lafayette Square, near the White House in Washington, D.C., the 1860 equestrian statue of George Washington  in Washington Circle, and the 1863 Statue of Freedom  in Washington D.C., were created.  He was born in c. 1820 into slavery in South Carolina's historic city of Charleston and was emancipated on April 16, 1862, under the District of Columbia Compensated Emancipation Act After his emancipation, he assisted Mills in installing the Statue of Freedom atop the United States Capitol, which was completed on December 2, 1863. Reid began working as an enslaved apprentice to Mills in 1842, as a young man in his twenties, who was already recognized for his talents in the foundry industry. In the 1860s, after having worked at the foundry for almost two decades, Reid's skills in working with bronze casting were recognized. In 1928, Tennessee Representative, Finis J. Garrett presented a paper honoring Reid for his "faithful service and genius", and describing the key role he had played in casting the statue of Freedom, that is now part of the Congressional Record. A memorial plaque honoring Philip Reed was unveiled on April 16, 2014—the 152nd anniversary of Emancipation in Washington, D.C.—in the National Harmony Memorial Park in Hyattsville, Maryland. It reads, "Philip Reed The slave who built the Statue of Freedom atop the U.S. Capitol died a free man on February 6, 1892 and is buried here..." In 2013, he was described by the Architect of the Capitol as the "single best known enslaved person associated with the Capitol's construction history".

Background
Reid—who was an enslaved African American from South Carolina—was born in c. 1820, and became enslaved to Mills when Reid was about 22-years-old, according to the 1864 petition made by Mills for compensation, after slavery had been abolished.  Reid remained enslaved to Mills for over twenty years, and was finally emancipated in 1863.

Equestrian statue of Andrew Jackson in Washington, D.C. (1853)

In 1848, the Jackson Monument Committee commissioned Mills, a self-taught sculptor to create the equestrian statue of Andrew Jackson which is now in Lafayette Square, near the White House in Washington, D.C.

Mills moved to Washington after winning the competition and brought Reid and his other workmen with him. They erected a temporary foundry south of the White House.  According to James M. Goode, Mills with the assistance of his apprentice, Reid and laborers, produced six castings of the equestrian statue. In 1852 the casting was complete. The Architect of the Capitol  said that they had produced "first bronze statue ever cast in America" through "trial and error". This "accomplishment was extraordinary due to the absence of any formal training of any of the participants." It has been described as the first equestrian statue made in America, and possibly the first equestrian statue of a horse rearing on two legs in which no additional support was added.

Equestrian statue of George Washington in the Washington Circle (1860)

The $60, 000 equestrian statue was executed by Mills in his studio and foundry. The statue was dedicated in 1860, by then President James Buchanan.

The Statue of Freedom (1863)
Commissioned in 1855, the initial full-size plaster model of Freedom was completed by American sculptor Thomas Crawford in his studio in Rome, Italy. He died suddenly in 1857. A plaster model was cast and divided into five main sections for transport in separate crates. Crawford's widow shipped the model to Washington where it was to be cast into bronze. The crates arrived in late March 1859. An Italian craftsman assembled the five sections and it was put on display in the Old Hall of the House, now National Statuary Hall.

Largely because of the impact of the equestrian statues, in May 1860, Jefferson Davis, then-Secretary of War under President Franklin Pierce—who was responsible for public works including the expansion of the U.S. Capitol—awarded the contract to cast Crawford's Freedom  statue to Mills.

The fragile full-scale plaster model, needed to be separated again into its five main sections to move it from the old House Chamber to Mills' foundry for casting. According to Mills' son Fisk, the Italian artisan refused to dismantle it until he got a major raise and a long-term contract. He had covered the seams of the sections with a layer of plaster that made them impossible to detect. He thought he was the only one capable of separating the delicate sections without harming them. Reid was able to find the seams by the ingenious use of an iron ring attached to the head of the figure and a block and tackle. He gently lifted the huge plaster model enough to crack the seals at the seams so he could reach the bolts inside. The statue was successfully separated into its five sections and carefully transported to Mills' Foundry.

Mills and his workmen began casting the statue in June 1860 at Mills Foundry—a large octagon-shaped studio and foundry on Bladensburg Road, Maryland.  The government rented the foundry for $400 a month and supplied the materials, fuel and labor to cast the statue. Because of this arrangement, the names of the craftsmen and laborers were recorded each day in Mills' monthly report. Philip Reid was listed as a "laborer". There is no evidence that any of other men listed as laborers were black or enslaved. Mills received the government payment for Reid's work, which amounted to $1.25 a day, with the exception of Sundays, when Reid was paid directly. The other workmen were paid $1 a day. Only Philip Reid was paid directly by the government for working on 33 Sundays.

The work on Freedom continued against the backdrop of the American Civil War (1861–1865). On December 2, 1863, the "final piece of the iconic Statue of Freedom" was installed "atop the new Capitol Dome" amid great celebration and a 35-gun salute.

After emancipation

On April 16, 1862, President Abraham Lincoln signed the District of Columbia Compensated Emancipation Act District slave owners, like Mills, were allowed to petition for compensation. Mills petitioned for compensation for eleven slaves, including Philip Reid. His description of Reid that he submitted with the Petition said that Reid was "aged 42 years, mullatto [sic] color, short in statue, in good health, not prepossessing in appearance but smart in mind, a good workman in a foundry…" Mills had claimed $1,500 for Reid, explaining that he had paid $1,200 for Reid in 1842 in Charleston, South Carolina. Mills said, that although Reid was a youth at that time,  he had already demonstrated "evident talent for the business in which [Mills] was engaged"—his steel foundry. Mills asked $1500 for Reid, but received only $350.40.

The 38th Congress (1863–1865) convened five days after Freedom had been installed, to "face and settle the most important questions of the century", and "passed the Thirteenth Amendment to the United States Constitution, which—when adopted by the states—abolished slavery and involuntary servitude.

Following his emancipation, he changed the spelling of his name to "Reed"—which is reflected in Census and city records—instead of "Reid", which was the spelling used by Mills since 1842.

According to Smolenyak's 2009 article in The Federal City,  by 1865, Reid had his own business and was "highly esteemed by all who [knew] him." The article also cited the 1870 Census, which said that Reid and his wife Jane—whom he had married in June 1862— had a two-year-old son. According to Smolenyak, in 1880, Reed's wife, who worked as a laundress, was listed as Mary P.

Reviews of Philip Reid's contributions

In 1863, with the Statue of Freedom newly installed on the Capital, a newspaper correspondent wrote,  "The black master-builder lifted the ponderous uncouth masses and bolted them together, joint by joint, piece by piece, till they blended into the majestic 'Freedom'.... Was there a prophecy in that moment when the slave became the artist and with rare poetic justice, reconstructed the beautiful symbol of freedom for America?" The Senate Historical Office reprinted these words in their tribute to Reid—"Philip Reid and the Statue of Freedom"—which is part of their series, The Civil War: The Senate's Story.

During the 70th United States Congress in 1928, Tennessee Representative, Finis J. Garrett, submitted a paper by William A. Cox, describing Reid as an "intelligent negro", a "mulatto", whose "faithful service and genius" led to the "successful taking apart and handling" of the Freedom statue.

The 1928 Congressional Record Cox's description of Reid's role in constructing Freedom.  Fox, who was a long-time admirer of the Statue of Freedom, said that it had arrived in pieces and was cast at the Clark Mill's Foundry near Bladensburg, Maryland, under the care, ironically, of a mulatto slave.

The Architect of the Capitol described Reid as the "single best known enslaved person associated with the Capitol's construction history".

National Harmony Memorial Park burial

The plaque honoring Philip Reed was unveiled the National Harmony Memorial Park in Hyattsville, Maryland, on April 16, 2014—the 152nd anniversary of Emancipation in Washington, D.C.. The plaque used the spelling "Reed", which he preferred and had chosen himself, after his emancipation in 1863, instead of "Reid" which was chosen by Mills in 1842 when he enslaved him.

Reed died on February 6, 1892, and was buried in the Graceland Cemetery in a "marked plot in clear view of the Statue of Freedom"—"his most notable achievement". His remains had been disinterred and reburied in Columbian Harmony Cemetery in 1895. According Smolenyak's documents, the D.C. government disenterred the remains of 37,000 people from the old Harmony Cemetery and transferred them to the new Harmony National Memorial Park in Maryland in 1959. The Park's offside historian could only show the general area where Reid was buried "an empty acre of grass". The Park had attempted to reach Reid's descendants about the change and when no one responded they buried the remains without a headstone.

Notes

References

Sources

 "List of Petitions." House of Representatives Executive Document No. 42. 38th Congress 1st Session,February 16, 1864.

Dr. Eugene Walton, "Philip Reid: Slave Caster of Freedom", The Examiner, Washington, March 1, 2005
Dr. Eugene Walton, "Philip Reid And The Slaves Who Built The Capitol" Video (25 min.), 2001
Dr. Eugene Walton, "Philip Reid and the Statue of Freedom", Social Education, September 1, 2005,    Published by Thomson Gale
Patrick Reynolds, "A Cartoon History of the District of Columbia", Red Rose Studio, October, 1995
National Council for the Social Studies, "Would the Statue of Freedom be Standing Without the Help of a Slave?"  - Education News, September 12, 2005

 Final chapter

Further reading

External links
Philip Reid and the Statue of Freedom
Philip Reid: Slave Caster of Freedom
http://www.randallrobinson.com/debtexc.html
 1994-2005.
The biography of Philip Reid

19th-century American slaves
Foundrymen
1820s births
1892 deaths
Burials at Columbian Harmony Cemetery
Burials at National Harmony Memorial Park


text:
Bichroma famula är en fjärilsart som beskrevs av Eugen Johann Christoph Esper 1789. Bichroma famula ingår i släktet Bichroma och familjen mätare. Inga underarter finns listade i Catalogue of Life.

Källor

Mätare
famula


text:
Bristol Estate Agents Refashioned
0117 9898 222 Login
Book Free Valuation Contact Us
AWARD WINNING ESTATE AGENT
Book Free Valuation
Estate Agency Refashioned
Why Our Customers Love Us
Save With Boardwalk
How Do We Find You A Buyer?
Online Client Interface
We Are Regulated
We're Eco-friendly
3 bed Terraced SOLD STC
Manor Road, Bishopston
20 metre west-facing garden
Close to shops and cafes
Situated in a highly desirable part of Bishopston, just minutes from the independent shops and cafes of Gloucester Road, is this three double bedroom home. The house is extended to the ground floor and into the loft, to offer an attractive and practical range of living and bedroom space. The garden is certainly a stand-out feature for this house, measuring approximately 20 metres from the rear reception room doors and benefitting from a westerly aspect. The house is well-presented throughout with stripped wooden flooring in through the interconnected living rooms, as well as many other period features giving the house a charming feel. Windows were updated throughout the house in 2012 and are still within guarantee. The position of this house on Manor Road is highly-sought after, with the well-regarded Bishop Road Primary School just a few minutes' walk. Viewing of this property is highly recommended, contact Boardwalk Property Co. for more information.
Room Measurements
Living Room - 4.6 x 4.2m (to maximum points, into bay)
Dining Room – 3.7 x 3.4m
Kitchen/Breakfast Room – 6.5 x 2.7m
Master Bedroom – 5.0 x 3.7m
Bedroom Three – 4.0 x 3.4m
Bathroom – 3.3 x 2.6m
Bedroom Two (Second Floor) – 5.3 x 5.0m (with some restricted head height, excluding eaves storage)
The rear garden measures approximately 20 metres in length and has a westerly aspect.
This house is situated on Manor Road, a quiet road which runs parallel to Gloucester Road, intersecting the lower part of Bishop Road. Residents of Manor Road can make the most of several independent shops and cafés nearby. This popular part of Bishopston is home to many families making the most of the popular local schools: Bishop Road, St Bonaventure's and Ashley Down Road. For those commuting to work, the area is well-placed for major areas of employment both in the City Centre and in North Bristol, with buses running both ways along the A38. For those looking for green spaces, this area of North Bristol is well placed for Horfield Common, The Downs and the Blaise Castle Estate, whilst sports-lovers benefit from lots of facilities and live sport in the local area including domestic and international cricket at the nearby County Ground.
Within the kitchen there is an integrated dishwasher and Bosch oven and hob, to be included within the sale. Other fixtures and fittings may be available for separate negotiation but are not automatically included.
Estimated Rental Value
£1500pcm
Our Seller Says…
'This is a comfortable, warm house with lots of sunshine throughout the day. It has the advantage of being in a quiet location, within a very lively environment. I have enjoyed living here and will miss the Gloucester Road amenities but it is time for me to downsize and move nearer to my family.'
Awaiting updated EPC. According to Bristol City Council, the property has 'Good' solar potential.
For further details on this property please call us on:
View Shortlist
Interested in Boardwalk's services or looking to buy or sell property in Bristol? Then get in touch - we'd love to hear from you.
Henleaze House
13 Harbury Road
BS9 4PN
I was impressed with how professional, courteous and helpful the team were throughout the process.
Great team and really made the stressful process of buying my first house a much easier one! Thanks guys!
Best estate agents Bristol
Cheapest estate agents Bristol
COVERING ALL OF BRISTOL
Every BS postcode
30 DAY CONTRACT
Not three months!
0.55% + VAT fee (0.66%)
Full Estate Agency Service
© 2019 Boardwalk | Blog | Terms of Use | Privacy Policy & Notice | Fair Processing Policy | Cookie Policy | Built by The Property Jungle
Minimum Price: No Minimum £50,000 £100,000 £150,000 £200,000 £250,000 £300,000 £350,000 £400,000 £450,000 £500,000 £550,000 £600,000 £650,000 £700,000 £750,000 £800,000 £850,000 £900,000 £950,000 £1,000,000 £2,000,000 £3,000,000 £4,000,000 £5,000,000 £6,000,000 £7,000,000 £8,000,000 £9,000,000 £10,000,000+
Maximum Price: No Maximum £50,000 £100,000 £150,000 £200,000 £250,000 £300,000 £350,000 £400,000 £450,000 £500,000 £550,000 £600,000 £650,000 £700,000 £750,000 £800,000 £850,000 £900,000 £950,000 £1,000,000 £2,000,000 £3,000,000 £4,000,000 £5,000,000 £6,000,000 £7,000,000 £8,000,000 £9,000,000 £10,000,000+
Minimum Bedrooms: Please Select 1 Bedroom 2 Bedrooms 3 Bedrooms 4 Bedrooms 5 Bedrooms 6 Bedrooms 7 Bedrooms 8 Bedrooms 9 Bedrooms 10 Bedrooms
Property Type: All Property Types Barn Conversion Detached Duplex End of Terrace Flat Ground Flat Semi-Detached Terraced
Show Sold STC


I admit I have a bit of an aversion to the Far West End when it comes to food. With some bright exceptions, it's bursting with chains, chains, and more chains. But Lehja is a fine-dining restaurant serving Indian food so delicious that it's worth my drive from the Northside to Short Pump. For dinner I love the Goan Lamb Vin d'alho ($17). The meat is extraordinarily tender and well-seasoned, while the chili-tomato sauce demands an order of naan to soak up what's left behind.


Please email miller.lisa.c@att.net for further information on all wholesale inquiries. We will respond as soon as we can!
Note: Your proof of non-profit status or sales tax permit number must accompany your order.