text:
Gilly Back for 96 Reunion
Join us for a great night with the stars of 96
There are now just two weeks to go until the Boys of 96 are reunited.
It is 20 years since Denis Smith's side sealed promotion to the second tier of English football, embarking on a superb run in the second half of the 1995/6 season that culminated in a truly memorable win over Peterborough at the Manor on the last day of the season.
The whole squad will be back together again on Friday 9th December for a curry and a beer at a special reunion evening, with tickets still available to join them.
One of the stars of the side was centre-half Phil Gilchrist whose partnership with Matt Elliott at the back was among the greatest in the club's history.
We caught up with 'Gilly' this week and asked him whether those days at the Manor were the happiest of his career?
"They probably were, because what we achieved there and the promotion in 1996 set me up for everything else that followed in my career.
"It was a unique set up, a small ground with lots of quirky little stands but we had something very special there and the team bonded and were very close. The wives, girlfriends and kids used to get on well and everyone around the club was part of the success. It was certainly among the happiest times in my career. My two kids were born in Oxford so it is a special place for me and I am really looking forward to going back there."
It will be a chance for the defence of Phil Whitehead, Steve Wood, Les Robinson, Mike Ford, Gilly and Matty Elliott to relive old times. How easy was it to form that partnership with Matt?
"The first time we met we got on really well and we ended up living close to each other" Gilly said. "We are still friends now; I see him at Leicester games when I go there and we are good friends. You could probably see that on the pitch, but between all of us really.
"Not just the players either. Ken Ridley, who was the kitman for years, Mick Moore the Groundsman: we all socialised together back then. I'm not sure it could happen these days; there was no social media back then so if we went out for a drink nobody was tweeting pictures of it! That all helped us stick together, especially in the second half of the season when we got on a fantastic run and felt we were going to win every game we played."
Phil, who came back for a second spell later in his career, can't wait to come back and be part of what should be a very special evening.
"It culminated against Peterborough which was an unbelievable day" he told us. "I ran into Denis Smith the other day, sadly at a funeral, and was hard to imagine 20 years since that promotion. We both spoke about the reunion and I can't wait to come back, see the lads again and hopefully as many fans as possible as well."
Were you there in 96? Roll back the years and join us for a great night with the Boys of 96.
The reunion takes place at the Oxford Academy in Littlemore on Friday 9th December, starting at 7.30pm for a two course curry, with a cash bar available.
Phil Gilchrist and Denis Smith join Malcolm Crosby, Matt Elliott, Paul Moody, Matt Murphy, Joey Beauchamp, Phil Whitehead, Mike Ford, Martin Gray, Stuart Massey, Les Robinson, Chris Allen, Steve Wood, and Mark Druce, with more stars expected to confirm in the coming days.
Ticket prices are: adults £30, U18s £20 including a two-course buffet. There will be a full cash bar available on the night.
Tickets are on sale online from www.oufctickets.co.uk


Amidst the uncertainty surrounding Brexit, the UK's asset management trade body is advising its members to authorise their contingency plans for the country leaving the EU without a withdrawal agreement. According to New Financial, 43 wealth managers currently make up almost 300 companies who, regardless of Brexit negotiation outcomes, have chosen to transfer their staff to an EU base in order to ensure the undisturbed continuity of operations.
The decisions being made to move operations to Europe strengthen suspicions that the UK's position as Europe's financial centre is in jeopardy. The most effective result may be to hold fire and wait to see where banks are looking to branch their networks before making any a decision to apply for a Markets in Financial Instruments Directive (MiFID) licence and follow suit in order to have a greater presence in Europe.
Neil Woodford has been making news recently. After months of disappointing performance, it's been reported that many IFA clients are moving away from Woodford, yet director of Rowley Turton Private Wealth Management, Scott Gallacher is sticking with him. Despite Woodford's reputation as a great fund manager in the past, Gallacher believes he has the only way out of the trap he has fallen into is through a good Brexit deal. This is due to Woodford's holdings being small-cap UK domestic stocks rather than being dependent on overseas sales. A good deal, therefore would see the pound lift and affect companies with international operations.
Gallacher said his main worry, however, is that Woodford could have lost impartiality over the likelihood of a deal being struck in the Brexit negotiations. "However, as part of a larger balanced portfolio, the Woodford fund is arguably a good hedge against a good Brexit deal. A good deal is likely to see the pound recover and the value of the international holdings in a well-diversified portfolio fall," he says.
We believe the problem with this 'Brexit hedge' is that the results of the Brexit referendum, as proved, cannot be predicted. What's even more difficult, is being able to predict the market reaction that comes after the result. Woodford's previous strengths were based on investing in companies that paid dependable dividends, however, after his latest controversial swap deal, it now seems that his ventures and strategies are muddled.
Wealth managers and legal firms hold a plethora of sensitive client data, making them a prime target for cyber attackers with dire consequences. IT security must be therefore moved higher up the priory list as this threat grows. Clients are increasingly recognising the importance of cyber security and are basing their decisions to work with legal advisors on the robustness of their defence, and the way in which their data is handled and kept secure. It is imperative, therefore that legal firms are investing in, and demonstrating the processes they have in practice to guard against cybercrime in order to retain the confidence of their clients.
Discover how you can stay one step ahead in the IFA and Wealth Management industry with Ortus Group. Get in touch.


Tennis ball launcher dog toys have been around for quite some time now. I was shocked to find out how many different kinds there are. We chose the Hyper Fling, made by Hyper Pet, mainly because it has a collapsible handle. We had a hard time picturing ourselves lugging around one of those gangly neon ones. The Hyper Fling just seemed to fit our lifestyle better. It's less than 11 inches when the handle is collapsed, so it can easily fit in a small bag or backpack.
The Hyper Fling performs well, launching the ball farther than we could throw it ourselves. It is also very easy to pick up the ball. We definitely don't miss picking up the slobbery tennis ball with our bare hands. The unfortunate thing about this product is that its most desirable feature may be the reason why it won't last very long. The handle has already started to stick when we try to collapse it. I'm not sure how much longer it will work, but at least it won't be completely useless. Much like an escalator, it can't really break. It will just eventually become like the other tennis ball launchers1.


text:
#pragma once
#ifndef VOID_INT_H
#define VOID_INT_H

namespace zorba {

///////////////////////////////////////////////////////////////////////////////

/**
 * A %void_int has the same API as atomic_int except that it does no reference
 * counting.
 *
 * It can also take no space when derived from via the empty base class
 * optimization: http://www.cantrip.org/emptyopt.html
 */
class void_int {
public:
  typedef int value_type;

  explicit void_int( value_type = 0 ) {
  }

  void_int& operator=( value_type ) {
    return *this;
  }

  value_type load() const {
    return 0;
  }

  void store( value_type ) {
  }

  value_type operator++() {
    return 0;
  }

  value_type operator++(int) {
    return 0;
  }

  value_type operator--() {
    return 0;
  }

  value_type operator--(int) {
    return 0;
  }

  void_int& operator+=( value_type ) {
    return *this;
  }

  void_int& operator-=( value_type ) {
    return *this;
  }

private:
  // forbid for compatibility with atomic_int
  void_int( void_int const& );
  void_int& operator=( void_int& );
};

///////////////////////////////////////////////////////////////////////////////

} // namespace zorba

#endif /* VOID_INT_H */
/* vim:set et sw=2 ts=2: */

redpajama_set_name: RedPajamaGithub


This is a selection of our retailers and distributors. It is easy to buy our funds if you are a customer of any of these banks or trading platforms. Are you a retailer missing from the list? Please contact our sales division.
Investments in financial instruments (such as securities and mutual funds) are associated with risk. An investment can rise or fall in value and investors may fail to recover the invested capital. Past performance is no guarantee of future results. For more information, order the complete prospectus, key investor information and annual report.
Questions? Contact us and we will help.
All of our funds employ the same overall management philosophy: focused value management.
Carnegie Fonder does not invest in any company without looking into it carefully first.
Keep yourself updated on news, comments and fund performances.


This is not unique to Seattle. Shamefully, in this, the richest country in human history, fifty million of our people – one in six – live in poverty. Around the world, billions do not have access to clean water and basic sanitation and children die every day from malnutrition.
In our country, Democratic and Republican politicians alike primarily serve the interests of big business. A completely dysfunctional Congress DOES manage to agree on one thing – regular increases in their already bloated salaries – yet at the same time allows the federal minimum wage to stagnate and fall farther and farther behind inflation. We have the obscene spectacle of the average corporate CEO getting seven thousand dollars an hour, while the lowest-paid workers are called presumptuous in their demand for just fifteen.
Right here in SeaTac, we have just witnessed the tremendous and victorious campaign for fifteen dollars an hour. At the same time, in Lorain County, Ohio, twenty-four candidates ran, not as Democrats or Republicans, but as 'Independent Labor' and were elected to their City Councils.
I will do my utmost to represent the disenfranchised and the excluded, the poor and the oppressed – by fighting for a $15/hour minimum wage, affordable housing, and taxing the super-rich for a massive expansion of public transit and education. But my voice will be heard by those in power only if workers themselves shout their demands from the rooftops and organize en masse.
My colleagues and I in Socialist Alternative will stand shoulder to shoulder with all those who want to fight for a better world. But working people need a new political party, a mass organization of the working class, run by – and accountable to – themselves. A party that will struggle and campaign in their interest, and that will boldly advocate for alternatives to this crisis-ridden system.
Here in Seattle, political pundits are asking about me: will she compromise? Can she work with others? Of course, I will meet and discuss with representatives of the establishment. But when I do, I will bring the needs and aspirations of working-class people to every table I sit at, no matter who is seated across from me. And let me make one thing absolutely clear: There will be no backroom deals with corporations or their political servants. There will be no rotten sell-out of the people I represent.
I wear the badge of socialist with honor. To the nearly hundred thousand who voted for me, and to the hundreds of you who worked tirelessly on our campaign, I thank you. Let us continue.
The election of a socialist to the Council of a major city in the heartland of global capitalism has made waves around the world. We know because we have received messages of support from Europe, Latin America, Africa and from Asia. Those struggling for change have told us they have been inspired by our victory.
To all those prepared to resist the agenda of big business – in Seattle and nationwide – I appeal to you: get organized. Join with us in building a mass movement for economic and social justice, for democratic socialist change, whereby the resources of society can be harnessed, not for the greed of a small minority, but for the benefit of all people. Solidarity.
Posted: January 6th, 2014 under Councilmember Sawant, News Releases.


Stylish furniture, furniture parts, frames, various objects. Particularly suitable for the application on molded parts.
Very good covering power, excellent verticality. Very good surface hardness, softness and distension.


Going beyond "Repeat after me"
Recently, I had the experience of observing several English classes at Czech elementary schools. Although I was warned in advance that in some of the classes the children hadn't been exposed to English at all before the first grade, I was surprised by how well, for example, one class of third grade children understood and responded to instructions in English when they were presented slowly and clearly. In the lesson I was observing, the third graders practiced several short plays that they were going to perform for their parents at the end of the year. They were able to recite their lines from memory and in some cases, even "ad lib" a bit, telling a few jokes in between the plays. Considering that some students had started from scratch three years ago, I was impressed both by their language abilities and by their willingness to communicate orally.
As I continued to observe classes in other elementary schools in the Prague 6 district, I noticed that when the children were taught through song and games, with multi-media such as clips from cartoons or You Tube and under a curriculum with an interactive emphasis, a majority of the children were able to actively use their new language skills. The liveliness of the lesson often correlated to the children's willingness to speak aloud. Children with English several times a week naturally made more rapid progress, particularly when they were placed in situations where they needed to speak or to respond with physical actions.
In the Czech state school system, English education is mandatory three times a week from the third grade. In the first and second grades, English education is offered by many, but not all schools. However, through grants from the city or in cooperation with private language schools, many Czech elementary schools are beginning to offer optional English education three times a week or more from the first grade. Parents are also increasingly seeing the need for their children to learn English from an early age, and private language lessons are common for children as young as preschoolers.
In Prague, there is a wellspring of private kindergartens in English, and not just those that cater to foreigners or the expat community. There are also a number of private language projects that have begun to be integrated into the Czech system in order to offer additional English lessons taught by native speakers in the Czech schools, quite often even during regular school hours.
After my daughter Anna Lee had her first few English lessons in first grade, I realized that for her the classes wouldn't be very useful unless I provided some independent work to supplement the curriculum the school used. Luckily, the teacher agreed. Now in the second grade, Anna Lee and her bilingual classmate are often used by their teacher to model the pronunciation for the lesson. They seem to like this role, and the teacher appreciates their different "native" accents, one being American and the other Australian.
Two years younger than Anna, Oliver thoroughly enjoys his preschool English classes, I expect, on one hand, it's because he's able to excel. He comes home from class singing English songs, some from the curriculum teaching basic greetings like "Hello, hello how do you do?" Other are pop songs, like the theme from the Lion King or the recent hit by Lenka, "Everything at Once," which utilizes simple metaphors such as "sly as a fox" or "strong as an ox".
When Oliver had his preschool English performance, the children performed two songs and sang their names in a call and response song with the teacher. Although Oliver's teacher gives directions and explanations in Czech, it is still clear that the children are learning how to actively use the English that they're learning. Some of the children even greet me in the locker room with "hello" or "goodbye," since they know I'm an English speaker.
As a mother I was proud of Oliver and his class, but as a TEFL teacher, I was more impressed that the children, who had only just begun to come into contact with the English language, could actively use it. During my formative years in French class, my teacher occasionally showed us a video or played a cassette tape, but we didn't have the advantage of watching French cartoons, listening to actual French children's songs or using the computer to find appropriate interactive activities for our competence level.
Times have changed and so have the type of language instruction children receive. It's encouraging to see steps being made here in the Czech Republic to bring a more active approach to English language instruction. Next year, my children's elementary school is offering a pilot "bilingual" first grade classroom through cooperation with a local language school. Within this class, the children should have about half of their daily instruction in Czech with one teacher and the other half with a native-speaking second language teacher. In order to earn a place in the 20-person class, students had to take a language competency test. Tuition is charged for the program, still there were over 60 applicants for the 20 spaces.
In the end, we didn't register Oliver for the class since we couldn't find enough information about the project on the website to convince us that it would be the right step for him next year. Still, I'm hopeful that the project will succeed, and that in the future this type of English-language instruction might be offered more frequently in state elementary schools.
Educating children in language acquisition often takes a different approach than teaching adults. From my experience TEFL teaching, children are more willing than adults to take risks, approach learning with a creative spirit and to take pride in their own linguistic advancements.
With my youngest son entering Czech preschool in the fall, I've begun my own search to find an English teaching position that will give me the opportunity to lead lively lessons with the focus on learning to speak and to respond to real-life situations. As I've been learning to speak Czech alongside my children over the last years, I know that we adults can also get just as excited about language learning when we're properly motivated.


Anonymous,. 1909. Linguistic survey of India. Volume 3: Tibeto-Burman family. Part 1: General introduction. Specimens of the Tibetan dialects, the Himalayan dialects and the North Assam group. (Linguistic Survey of India.) In Grierson, George Abraham (ed.) Calcutta: Government Printing Office.


If you want to learn to code your own WordPress plugins, you should try our new course, 3 More Practical Projects to Learn WordPress Plugin Development.
In this course with experienced WordPress developer Rachel McCollin, you'll create three practical projects to help you learn WordPress plugin development.
Create a list of pages in the current section of your site.
Customize the WordPress admin pages.
Add an attractive display of the most recent post in each category to your home page or below each post in your site.


For this exercise I will be using the VMware Linux servers: grid10g, which hosts the Grid Control management server, ha1, where the master database in a data guard couple is running, and ha2, where the standby database has benn created. Both ha1 and ha2 are configured with the grid control, both having a management agent.
We do we will be able to connect to the standby ... even if the database is only mounted and not open!
We were able to connect! The next screen is about "Add Standby Database: Configuration"
This was about configuring the dataguard broker, see the previous article of this series for the installation Enterprise Manager Repository.


One commentator has said that God's address in Israel was "one center street". What is His place in your life? Why is adherence to God's instructions regarding the design, constructions, and placement of the tabernacle not to be compromised? How does this apply to our walks with Jesus?


text:
\section{Introduction}\label{s1}

Galaxy outskirts record mass-assembly histories of merger and accretion events in a hierarchical universe \citep{Searle1978,White1978}, and also feedback processes taking place therein \citep{Dekel1986,Heckman1990}.
Past deep wide-field imaging uncovered various diffuse stellar halos of nearby galaxies and hence diverse buildup histories of outer disks \citep{Courteau2011,Deason2014,Merritt2016,Harmsen2017}, which correlate with their physical properties \citep{Elias2018}.
Combined analyses with simulations in the cosmological framework of Lambda Cold Dark Matter claim that, in general, high fractions of inner and outer stellar halos are formed by in-situ and ex-situ stellar components, respectively \citep{ZhangJ2018,Merritt2020,Font2020}.
Furthermore, the diffuse ionized gas and its physical states in the outskirt of nearby galaxies have been well investigated for understanding feedback mechanisms (e.g., \cite{Veilleux2005} and references therein).
\citet{Zhang2016,Zhang2018} successfully detected H$\alpha+$[N{\sc ii}] emission at $z=$ 0.05--0.2 out to 100 kpc by combining millions of fiber spectra from the Sloan Digital Sky Survey, providing a unique insight into cool gas from associated halos.
However, it remains significantly challenging to observe the galaxy outskirts beyond the local universe due to cosmological surface brightness dimming, which has hampered direct observations to date from the earlier phase of the mass assembling.

Nowadays, a giant wide-field imager on the Subaru Telescope with an 8.2 m primary mirror, Hyper Suprime-Cam \citep{Miyazaki2018,Furusawa2018,Kawanomoto2018,Komiyama2018} has enabled very deep wide-field observations under seeing conditions of $<1$ arcsec that provides new insights into the outskirts of nearby galaxies \citep{Fukushima2019,Okamoto2019}.
In addition, such high-quality imaging data over $>100$ deg$^2$ taken by Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP; \cite{Aihara2018}) can establish even deeper images by stacking numerous objects.
This enables us to investigate the outskirts of massive galaxies beyond the local universe \citep{Huang2018a,Wang2019}, and their environmental dependence \citep{Huang2018b}.

With such scientific backgrounds, this research aims at investigating the outskirts of H$\alpha$ line emission from star-forming galaxies at $z=0.4$.
H$\alpha$ line is used extensively as a tracer of star formation \citep{Kennicutt1998}, which helps us study galaxy outskirts from a unique standpoint.
Based on the emission-line object catalog available from the Second Public Data Release of HSC-SSP (HSC-SSP PDR2; \cite{Aihara2019,Hayashi2020}), we perform a stacking analysis of H$\alpha$ line and continuum images for 8625 H$\alpha$ emitting galaxies termed as H$\alpha$ emitters at $z=0.4$.
A wide and deep narrow-band survey by HSC-SSP successfully detects H$\alpha$ emitters at $z=$0.393--0.404 down to $\sim1\times10^{-17}$ erg~s$^{-1}$cm$^{-2}$ over 16.8 deg$^2$ (section~\ref{s2}).
We investigate radial profiles of their composite H$\alpha$ and continuum images in different stellar mass bins, and study star formation in the outskirts of H$\alpha$ emitters (section~\ref{s3}).
We also discuss other possible contributions to H$\alpha$ emission on the galaxy outskirts by shape-aligned stacked images, and lastly summarize the entire flow of this work (section~\ref{s4}).

This research adopts the AB magnitude system \citep{Oke1983} and a \citet{Chabrier2003} stellar initial mass function (IMF).
Also, we assume cosmological parameters of $\Omega_M=0.310$, $\Omega_\Lambda=0.689$, and $H_0=67.7$ km~s$^{-1}$Mpc$^{-1}$ in a flat Lambda cold dark matter model, which are consistent with those from the Planck 2018 VI results \citep{Planck2020}.

\section{Data and methodology}\label{s2}

The source catalog and data set underlying this paper are available on the HSC-SSP Public Data Release site\footnote{\url{https://hsc.mtk.nao.ac.jp/ssp/data-release/}}.
This section briefly overviews the narrow-band emitter catalog in HSC-SSP PDR2 \citep{Hayashi2020} and describes our procedure of image stacking of broad-band and narrow-band data for the targets, H$\alpha$ emitters at $z=0.4$.

\subsection{HSC-SSP PDR2}\label{s21}

\begin{figure}
\begin{center}
\includegraphics[width=7.5cm]{fig1.pdf}
\end{center}
\caption{
Narrow-band (H$\alpha$+[N{\sc ii}]) flux versus logarithmic stellar mass with stellar mass distributions on the top panel.
The light-gray, gray, and black symbols indicate unused emitters in this work, those for the main analysis (section~\ref{s3}), and emitters with high ellipticities ($\epsilon>0.33$) that are used in the discussion section (see section~\ref{s4}).
The horizontal line depicts the selection threshold for the narrow-band flux ($4\times10^{-17}$ erg~s$^{-1}$cm$^{-2}$).
The dotted vertical lines represent selection cuts into three stellar-mass bins.
}
\label{fig1}
\end{figure}

\begin{table}
\caption{
Summary of the sample selection from the original source catalog (\cite{Hayashi2020}; $N=8625$).
See also figure~\ref{fig1} for the selection thresholds.}
\label{tab1}
\begin{center}
	\begin{tabular}{llr}
	\hline
	Sample        & Limits  & N\\
	\hline
	All       & $f_\mathrm{NB}$$>$4$\times$10$^{-17}$, FWHM$<$0.8 & 6324\\
	\hline
	Low-mass  & M$_\star$=$10^8$-$10^9$       & 2121\\
	Mid-mass  & M$_\star$=$10^9$-$10^{10}$    & 3139\\
	High-mass & M$_\star$=$10^{10}$-$10^{11}$ &  948\\
	Shape-aligned & M$_\star$=$10^9$-$10^{11}$, $\epsilon$$>$0.33 & 1430\\
	\hline
	\end{tabular}
\end{center}
\end{table}

This work is based on the H$\alpha$ emitter sample at $z=0.4$ established by \citet{Hayashi2020}; they reported narrow-band selected emission-line objects at $z<2$ based on the Deep and Ultradeep layers in HSC-SSP PDR2 \citep{Aihara2019}.
The catalog contains 8625 H$\alpha$ emitters down to a limiting flux of $\sim1\times10^{-17}$ erg~s$^{-1}$cm$^{-2}$ (figure~\ref{fig1}) and line equivalent width (EW$_\mathrm{H\alpha+[N{\scriptscriptstyle II}]}$) of $>25$ \AA\ in the rest-frame \citep[tab.~4]{Hayashi2020}.
They show flux excesses in narrow-band, NB921 ($\lambda_\mathrm{center}=9205$ \AA), relative to $z$ and $y$-bands by capturing H$\alpha$ ([N{\sc ii}] doublet also falls into the filter, however, we omit it hereafter) emission line at $z=$0.393--0.404 \citep[tab.~3]{Hayashi2020}.
The survey area covers 22.09 deg$^2$ (16.79 deg$^2$ excluding bright star mask regions) split into 4 fields (Extended COSMOS, SXDS, ELAIS-N1, DEEP2-3; \cite[table~1]{Hayashi2020}).
Stellar masses of our sample are derived by {\tt Mizuki}, a SED-based photo-$z$ code \citep{Tanaka2015,Tanaka2018}, by fixing the source redshift of $z=0.4$ ({\tt stellar\_mass\_mizuki\_zfixed\_convflux} in the source catalog; \cite{Hayashi2020}).

To collect H$\alpha$ emitters homogeneously across the entire survey area, we set several selection criteria as follows. We adopt only H$\alpha$ emitters with narrow-band fluxes greater than $4\times10^{-17}$ erg~s$^{-1}$cm$^{-2}$ (SFR $=0.1$ M$_\odot$yr$^{-1}$ without dust correction), where the imaging depths achieve approximately 100 percent completeness over the whole survey fields \citep{Hayashi2020}.
Also, this study does not consider areas taken under relatively bad seeing conditions (FWHM $>0.8$ arcsec) in either of narrow-band (NB921) or $z$-band. We then select 6324 H$\alpha$ emitters through these thresholds.

\subsection{Stacking analysis}\label{s22}

We perform median stacking for narrow-band (NB921) and $z$-band images of the selected H$\alpha$ emitters at $z=0.4$ to derive their typical radial profiles of H$\alpha$ and stellar surface densities.
For the stacking analysis, we obtain coadd images in the NB921 and $z$-band of H$\alpha$ emitters from the Third Public Release of HSC-SSP \citep{Aihara2021}\footnote{\url{https://hsc-release.mtk.nao.ac.jp/das_cutout/pdr3/} (registration is required)}.
The data were generated by the dedicated reduction pipeline ({\tt hscPipe} version 8; \cite{Bosch2018}). Their spatial resolutions are matched to FWHM $=0.8$ arcsec by Gaussian smoothing.
We confirm that the composite PSF distributions of the NB921 and $z$-band are consistent within a margin of less than 6 percent, which is negligibly small for this study.
Consequently, we derived median pixel values of the target images in each filter.
Here, we separate the emitter sample into three stellar mass bins ($10^{8\mbox{-}9}$, $10^{9\mbox{-}10}$,$10^{10\mbox{-}11}$ M$_\odot$; see figure~\ref{fig1} and table~\ref{tab1}).
Based on the composite NB921 and $z$ images, we establish emission line and stellar continuum maps through the following calculation.
\begin{eqnarray}
F_\mathrm{H\alpha} &=& \Delta_\mathrm{NB} \frac{f_\mathrm{NB}-f_\mathrm{BB}}{1-\Delta_\mathrm{NB}/\Delta_\mathrm{BB}},\\
f_\mathrm{c} &=& \frac{f_\mathrm{BB}-f_\mathrm{NB}\cdot\Delta_{NB}/\Delta_\mathrm{BB}}{1-\Delta_\mathrm{NB}/\Delta_\mathrm{BB}},
\end{eqnarray}
where $f_\mathrm{NB}$ and $f_\mathrm{BB}$ are flux densities of the NB921 and $z$-band, and $\Delta_\mathrm{NB}$ and $\Delta_\mathrm{BB}$ indicate filter band widths of the NB921 and $z$-band, respectively \citep{Hayashi2020}.
Furthermore, we adopt a single color-term correction of $f_{BB}=1.04\times f_{z}$ to correct a difference of the central filter wavelength between the NB921 and $z$-band (296 \AA), which is consistent with a typical value of high-mass H$\alpha$ emitters.
Although the fixed color-term correction does not significantly affect our main result, this is an important issue on the discussion part regarding to the radial profile of EW$_\mathrm{H\alpha}$ (see section~\ref{s4} and Appendix~\ref{a1}).

Besides, we generate random 100 realizations of composite emission-line and stellar continuum images to measure flux uncertainties of the stacked images using a bootstrap re-sampling from the same samples but with replacement.
Based on the 100 random combined images, we calculate a standard deviation of self flux counts at a given radius.
We also derive a background deviation given a pixel area ($S$) based on randomly-positioned empty apertures.
Obtained background deviations correlate with the background areas by $\propto S^{\sim0.8}$, suggesting partial pixel-to-pixel correlations (cf. no correlation and full correlation if $\propto S^{0.5}$ and $\propto S$, respectively).
This research defines the mean square errors of deviations of the self-flux and background noises as a total uncertainty of derived flux surface density (section~\ref{s3}).
In addition, residual background counts are sampled by measuring median pixel values in the backgrounds of the randomly combined images.
Obtained residual background counts are $\sim4\times10^{-4}$ and $\sim4\times10^{-3}$ in H$\alpha$ and continuum images, respectively, in the zero point magnitude of 27 mag.
These residual backgrounds are subtracted when deriving the flux densities.

\section{Results}\label{s3}

\begin{figure*}
\begin{center}
\includegraphics[width=16cm]{fig2.pdf}
\end{center}
\caption{
Radial profiles of surface brightness of H$\alpha$ line emission (blue squares) and normalized stellar continuum (yellow circles) for H$\alpha$ emitters at $z=0.4$.
Less than $2\sigma$ detections are represented by the open symbols.
The error-bars depict $1\sigma$ errors and the light-blue regions are $1\sigma$ errors of the curve fitting (see text).
From the left to right, figures depict radial profiles for H$\alpha$ emitters with stellar masses of (a) $10^{8\mbox{-}9}$, (b) $10^{9\mbox{-}10}$, and (c) $10^{10\mbox{-}11}$ M$_\odot$, respectively.
The dotted curves indicate scaled radial profiles of the composite PSF (fitted by a Moffat distribution).
The dot-dashed curves are the best-fit Gaussian$+$exponential radial profiles, which are expected to trace bulge$+$disk components of the H$\alpha$ emitters.
}
\label{fig2}
\end{figure*}

Median radial profiles of H$\alpha$ emission ($\Sigma F_\mathrm{H\alpha}$) and stellar continuum in three different stellar masses are shown in figure~\ref{fig2}, where radial continuum distributions are normalized at the peak surface densities in H$\alpha$ line.
Examples of the composite H$\alpha$ and continuum images are represented in Appendix~\ref{a1}.
As a result, we detect both H$\alpha$ and continuum of the sample in outer regions of H$\alpha$ emitters at $z=0.4$, especially at the highest stellar mass bin ($10^{10\mbox{-}11}$ M$_\odot$).
While we observe differentials between H$\alpha$ and stellar distributions in $\sim10$ ph-kpc at the highest stellar mass as explored in more detail in section~\ref{s4}, they are generally consistent with each other.

To investigate stellar halo contributions, we fit the radial profiles with a combined function of Gaussian ($G$), exponential ($E$), and power law ($P$) distributions by assuming that they respectively trace galactic bulge, disk, and stellar halo:
\begin{eqnarray}
G(r) &=& A_g \exp(-r^2 / w_g),\\
E(r) &=& A_e \exp(-r / r_s),\\
P(r) &=& A_p r^\gamma,
\end{eqnarray}
where $r$ is the physical radius (physical kpc, hereafter ph-kpc) from the center; $A_{g}$, $A_{e}$, $A_{p}$, $w_g$, $r_s$, and $\gamma$ are fitting parameters.
We do not adopt the de Vaucouleurs-law profile \citep{Vaucouleurs1948} for bulge components because our targets are barely resolved or unresolved in the seeing-limited data (FWHM $=4.4$ ph-kpc). We perform a chi-square fitting with the model function shown above using a curve fitting code, {\tt lmfit} \citep{Newville2014}.

\begin{table}
\caption{
Best-fit parameters and $1\sigma$ errors in three different stellar mass bins
(see figure~\ref{fig2}).}
\label{tab2}
\begin{center}
	\begin{tabular}{lrrr}
	\hline
	Mass range  & $10^8$--$10^9$ & $10^9$--$10^{10}$ & $10^{10}$--$10^{11}$\\
	\multicolumn{1}{c}{($N=$)} & (2121) & (3139) & (948)\\
	\hline
	$A_{g}$ ($\times10^{-17}$) & $3.0\pm0.2$  & $4.9\pm0.2$  & $14.2\pm0.6$\\
	$w_{g}$                    & $11.6\pm0.5$ & $15.9\pm0.5$ & $20.9\pm0.8$\\
	$A_{e}$ ($\times10^{-17}$) & $1.3\pm0.4$  & $1.7\pm0.4$  & $3.7\pm1.0$\\
	$r_{s}$                    & $3.1\pm0.3$  & $3.8\pm0.3$  & $4.2\pm0.4$\\
	$A_{p}$ ($\times10^{-18}$) & $0.6\pm2.1$  & $1.5\pm2.6$  & $11.8\pm9.1$\\
	$\gamma$                   & $-1.2\pm1.3$ & $-1.2\pm0.5$ & $-1.4\pm0.2$\\
	\hline
	\end{tabular}
\end{center}
\end{table}

The best-fit parameters and associated errors for the H$\alpha$ flux surface densities are summarized in table~\ref{tab2}.
Figure~\ref{fig2} shows that there are residual components beyond $\gtrsim15$ ph-kpc compared to the best-fit bulge$+$disk profiles in the intermediate and high stellar mass bins (figure~\ref{fig2}b,c).
Such residuals have been commonly observed in stellar distributions of nearby galaxies (e.g., \cite{Courteau2011,Merritt2016}), suggesting that they could originate respectively from in-situ hot young stars and old stars in outer disks and stellar halos (see section~\ref{s4} for more discussion).
The estimated power law slopes in the outskirts, $\gamma=-1.4\sim-1.2$, are flatter than those of most nearby galaxies $\gamma<-2$ \citep{Harmsen2017}.
However, given the low signal detection, it may be too early to conclude that H$\alpha$ emitters at $z=0.4$ have much shallower power-law slopes than galaxies in the local universe.
Recent studies have reported that stellar halo distributions can be fitted by broken power law; the outer slopes become significantly steeper at broken radii of a few tens of ph-kpc \citep{Deason2014}.
This may be one of the reasons of non detection in both H$\alpha$ and continuum images at $r>30$ ph-kpc.

Moreover, we convert the H$\alpha$ surface densities to SFR surface densities ($\Sigma\mathrm{SFR}$) and investigate fractions of star formation in stellar halos at $>10$ ph-kpc (figure~\ref{fig3}).
We follow the \citet{Kennicutt1998} calibration and scale by $1/1.7$ to apply the \citet{Chabrier2003} IMF.
Also, we assume 20 percent contributions of [N{\sc ii}]$\lambda\lambda6548,6583$ lines to narrow-band fluxes.
Here it should be noted that we assume no extinction and do not consider warm ionized medium \citep{Reynolds1973,Haffner2009}.
Thus, the derived $\Sigma\mathrm{SFR}$ values should have significant uncertainties beyond the measurement errors.
In particular, H$\alpha$ extinction in the central components of emitters would exceed 1 mag at the high stellar mass bin \citep{Sobral2016}.
However, central star formation is not the scope of this paper; therefore, we solely focus on the outskirts of H$\alpha$ emitters.
The stacked data have reached $\Sigma\mathrm{SFR}$ down to $\sim3\times10^{-6}$ M$_\odot$yr$^{-1}$kpc$^{-2}$, about a half of which appears to originate from stellar halos.
As inferred from the best-fit results, major fluxes beyond 30 ph-kpc are dominated by halo components; however, significant uncertainties are associated with these results.

\begin{figure}
\begin{center}
\includegraphics[width=7.5cm]{fig3.pdf}
\end{center}
\caption{
(Top panel) Radial profiles of surface SFR densities of H$\alpha$ emitters in three stellar mass bins as in figure~\ref{fig1} and table~\ref{tab1} (blue: $10^{8\mbox{-}9}$, green $10^{9\mbox{-}10}$, and red: $10^{10\mbox{-}11}$ M$_\odot$, respectively).
(Bottom panel) Fractions of power law components to the best-fitted radial profiles ($f_\mathrm{halo}$) in respective stellar mass bins at $r>10$ ph-kpc.
Non detection regions with $<2\sigma$ are extrapolated by the best-fitted curves (dashed curves).
}
\label{fig3}
\end{figure}

\section{Discussion and summary}\label{s4}

This work has identified diffuse H$\alpha$ emission and stellar continuum beyond 10 ph-kpc and up to 30 ph-kpc for the H$\alpha$ emitters at $z=0.4$ based on the deep narrow-band and broad-band stacking taken from HSC-SSP.
There are residual excesses in both H$\alpha$ line and stellar continuum compared to exponential distributions at $\gtrsim20$ ph-kpc.
While such residual emissions could originate respectively from in-situ hot young stars and old stars in outer disks and stellar halos, we cannot ignore contributions from associated halos \citep{Zhang2016,Zhang2018} and escape of ionizing radiation (e.g., \cite{Leitherer1995,Heckman2011}).
Thus physical origins of diffuse emission lines are still controversial.
In addition, we do not obtain a clear discrepancy between the radial profiles of the emission line and the continuum on the outskirts.
The observed H$\alpha$ surface densities monotonically decline in the outskirts with flatter power-law slopes of $\gamma=-1.4\sim-1.2$ than those in nearby galaxies; however, we note weak detection of some diffuse stellar halos.

Lastly, we delve into causal factors that may contribute to the observed diffuse H$\alpha$ emission on the outskirt by constructing shape-aligned composite images of H$\alpha$ emitters.
This is originally motivated to observe diffuse ionized gas arisen from biconical outflows from galaxy disks as typified by nearby starburst, M82 (e.g., \cite{Lynds1963,Visvanathan1972,Bland1988,Veilleux2003,Yoshida2019}).
Based on the second moments of the object intensity termed adaptive moments, we calculate ellipticities ($\epsilon$) and position angles of the targets \citep{Bernstein2002}.
We use the adaptive moments in the $i$-band ({\tt i\_sdssshape\_shape}) because the $i$-band data have better and more homogeneous seeing sizes ($\sim0.6$ arcsec) over the survey field.
Also, we employ only elliptic sources at M$_\star>10^{9}$ M$_\odot$ with $\epsilon>0.33$ (i.e., major-axis $>1.5\times$ minor-axis) to assure the credibility of position angle estimates.
We align objects along the major-axis; consequently, we conduct the median stacking following a similar method described in section~\ref{s22} for 1430 objects that satisfy these selection criteria (see figure~\ref{fig1} and table~\ref{tab1}).

Figure~\ref{fig4} represents radial profiles of the rest-frame EW$_\mathrm{H\alpha}$ along $\pm30$ deg of the major- and minor-axis.
For deriving radial EW$_\mathrm{H\alpha}$ profiles appropriately, the color term correction is important because the color term is significantly different between the major- and minor-axis.
We thus correct the color term effect in each radial bin on the best effort basis, by using the control sample (see Appendix~\ref{a1} for the detailed procedure).
The result shows a clear directivity of EW$_\mathrm{H\alpha}$; for instance, EW$_\mathrm{H\alpha}$ is higher on the outskirts along the minor-axis of the stellar disk (figure~\ref{fig4}).
A possible factor producing such high EW$_\mathrm{H\alpha}$ could be biconical galactic outflows.
However, as discussed above, there are various potential contributions such as star formation in outer disks and emission from associated halos; therefore, the actual cause would be more complex and complicated.
On the other hand, the moderate dip in the center can be explained by higher nebular dust extinction and/or lower specific star formation rate in the galactic bulge.

In summary, we have unveiled stellar and H$\alpha$ radial profiles on the outskirts of H$\alpha$ emitters at $z=0.4$ for the first time.
However, contributors to diffuse H$\alpha$ emission remain uncertain.
Comparing our results with hydrodynamic simulations and absorption-line observations (e.g., \cite{Werk2014,Prochaska2017}) will help us resolve its causal factors from theoretical and independent points of view, respectively.
In addition, more detailed investigations of physical properties of diffuse halos, e.g., derivation of stellar populations on the outskirts based on multi-band image stacking, will deliver further insights into mass-assembly histories surrounding galaxies beyond the local universe.

\begin{figure}
\begin{center}
\includegraphics[width=7.5cm]{fig4.pdf}
\end{center}
\caption{
Radial profiles of rest-frame EW of H$\alpha$ emission in the directions of $\pm30$ deg from major-axis (orange symbols) and minor-axis (purple symbols), respectively.
An image illustration of the areas used in the stacking analysis is denoted at the upper left corner. The error-bars and color-filled regions represent $1\sigma$ errors.
The open symbols indicate $2\sigma$ upper limits.
The dashed curves depict extrapolated lines of the best-fitted models.
The gray region indicates the standard deviations of non-aligned EW$_\mathrm{H\alpha}$ profile based on 100 composite images with random rotation.
}
\label{fig4}
\end{figure}

\begin{ack}
Based on data collected at the Subaru Telescope and retrieved from the HSC data archive system, which is operated by Subaru Telescope and Astronomy Data Center at National Astronomical Observatory of Japan. We are honored and grateful for the opportunity of observing the Universe from Maunakea, which has the cultural, historical and natural significance in Hawaii.

The Hyper Suprime-Cam (HSC) collaboration includes the astronomical communities of Japan and Taiwan, and Princeton University. The HSC instrumentation and software were developed by the National Astronomical Observatory of Japan (NAOJ), the Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU), the University of Tokyo, the High Energy Accelerator Research Organization (KEK), the Academia Sinica Institute for Astronomy and Astrophysics in Taiwan (ASIAA), and Princeton University. Funding was contributed by the FIRST program from Japanese Cabinet Office, the Ministry of Education, Culture, Sports, Science and Technology (MEXT), the Japan Society for the Promotion of Science (JSPS), Japan Science and Technology Agency (JST), the Toray Science Foundation, NAOJ, Kavli IPMU, KEK, ASIAA, and Princeton University.
This paper makes use of software developed for the Large Synoptic Survey Telescope. We thank the LSST Project for making their code available as free software at \url{http://dm.lsst.org}

The Pan-STARRS1 Surveys (PS1) have been made possible through contributions of the Institute for Astronomy, the University of Hawaii, the Pan-STARRS Project Office, the Max-Planck Society and its participating institutes, the Max Planck Institute for Astronomy, Heidelberg and the Max Planck Institute for Extraterrestrial Physics, Garching, The Johns Hopkins University, Durham University, the University of Edinburgh, Queen's University Belfast, the Harvard-Smithsonian Center for Astrophysics, the Las Cumbres Observatory Global Telescope Network Incorporated, the National Central University of Taiwan, the Space Telescope Science Institute, the National Aeronautics and Space Administration under Grant No. NNX08AR22G issued through the Planetary Science Division of the NASA Science Mission Directorate, the National Science Foundation under Grant No. AST-1238877, the University of Maryland, and Eotvos Lorand University (ELTE) and the Los Alamos National Laboratory.

This research was financially supported by JSPS KAKENHI Grant Number JP19K14766.
We would like to thank Editage (\url{www.editage.com}) for English language editing.
This work made extensive use of the following tools, {\tt NumPy}
\citep{Harris2020}, {\tt Matplotlib} \citep{Hunter2007}, {\tt lmfit}
\citep{Newville2014}, the Tool for OPerations on Catalogues And Tables,
{\tt TOPCAT} \citep{Taylor2005}, a community-developed core Python package for
Astronomy, {\tt Astopy} \citep{Astropy2013}, and Python Data Analysis Library
{\tt pandas} \citep{McKinney2010}.
\end{ack}

redpajama_set_name: RedPajamaArXiv


text:
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All posts by EnjoyTheTom
I once starred in a movie titled "Tomi's First Birthday" it was a straight to VHS production that received mix reviews. My parents loved it, my brother thought it was boring.
Lists, Movie Picks
Top 3 Movies on Netflix that are Based on True Events
March 28, 2018 EnjoyTheTom	Leave a comment
There's something about a movie about real events that always seems to enthrall the audience. Going back 50,60, 100 years and seeing what life was like, is inspiring and also enlightening. Without further ado a list of some of the best movies based on Real Life Events with some fun facts about each.
The Real Desmond Doss
Andrew Garfield playing Desmond Doss
Award Winning Hawksaw Ridge
The harrowing story of a Army medic in World War II who risked life and limb rescuing those who treated him poorly. Desmond Doss was a hero amongst men, his courage, and resolve serve as a benchmark as too what people should strive too. FACT: The real Desmond Doss treated and recused nearly 300 men during his 3 week deployment.
The Man who Knew Infinity (2016)
Dev Patel as Srinivasa Ramanujan
Dev Patel portrays Srinivasa Ramanujan, the brilliant mathematician from Indian who travelled from his home land to study Math at Cambridge. This movie takes place in 1913 and is set during wartime England. I enjoyed this movie from start to finish and I think it was because I had no idea Srinivasa Ramanujan existed prior to watching this. It was a inside look into the mind of genius and should be on everyone list. FACT: As his mentor Professor G. H. Hardy (Played by Jermey Irons), a celebrated mathematician himself who considered his own life's greatest contribution to mathematics as the discovery of Ramanujan, put it, numbers were "personal friends of Ramanujan."
Lee Daniel's The Butler (2013)
Allen and Whitaker
The Butler Movie Poster
Whitaker as Allen
The story of a butler who served every president from Truman to Reagan and weathered the worst of the country's brutal racial history. A great, although, sometimes difficult to watch movie, about the longest standing butler in the Whitehouse. Forest Whitaker and Oprah Winfrey lead this star studded cast and truly put further inspiring performances. FACT: When he started at the White House in 1952, he couldn't even use the public restrooms when he ventured back to his native Virginia.
ListMovies
Best Movies to Watch When you're Feeling Blue
One universal truth is that there is always a movie to watch that fits your mood. Whether you're in need of some motivation,a good scare, or (The most common) something to cheer you up.
Listed below are my picks for the best movies to watch when you're feeling a little down.
Disney movies always seem to help cheer me up, something about the bright colors, and magical story lines just work for me. Aladdin is by far my favorite Disney movie and reminds me of my childhood days, when life was simple and without care. Also Robin Williams as Genie is just incredible. (They actually animated Genie around Robin Williams improved lines)
The Princess Bride is one of those timeless classics, that touches on a bunch of different genres, it beautifully melds together action, romance, sci-fi, thriller, etc. It's no wonder this movie has stood the test of time, it's now considered a cult classic, and is regularly in the news. It's too bad the Dread Pirate Roberts (Cary Elwes) went on to play the jerk meteorologist in Twister (1996).
Raiders of the Lost Ark – Indiana Jones (1981)
A Steven Spielberg classic and one of my favorite movies of all times! Raiders of the Lost Ark is the definition of Action/Adventure movie. Booby traps and buried treasure, this movie will make you forget about everything else going on in your life and will whisk you away into a heart racing adventure where you join Indiana Jones as he scours the earth in pursuit of treasure while batting the quintessential bad guy, the Nazi's, all the while saving a damsel in distress.
Something about movies made in the 80's always cheers me up, the funny clothes, outdated views on the world, and old sayings, put a smile on my face. Back to the Future is a classic, Marty McFly and the mad scientist Dr. Emmett Brown, team up to get into trouble when the doctor creates a functioning time machine out of a DeLorean, Marty is sent back in time and the shenanigans commence.
Lists, News
Top 10 Highest Grossing Actors at the US Box Office
Total Gross: $5,149,077,633*
Average Gross: $70,535,310
Highest-Grossing Movie: The Avengers (2012), $623,357,910 (U.S.)
Average Gross: $118,185,202
Highest-Grossing Movie: Star Wars: The Force Awakens (2015), $936,662,225 (U.S.)
Lifetime Total Gross: $4,602,786,488*
Highest-Grossing Movie: Toy Story 3 (2010), $415,004,880 (U.S.)
Highest-Grossing Movie: The Dark Knight (2008), $534,858,444 (U.S.)
Highest-Grossing Movie: Shrek 2 (2004), $441,226,247 (U.S.)
Highest-Grossing Movie: War of the Worlds (2005), $234,280,354 (U.S.)
Highest-Grossing Movie: Beauty and the Beast (2017), $504,014,165 (U.S.)
The 5 Stages of Trying to Pick What Movie to Watch
March 14, 2018 EnjoyTheTom	1 Comment
You decide that tonight would be the perfect night to stay in and watch a movie (7:30PM)
We've all been there, whether it's a cold rainy night, there's nothing going on, or you just don't feel like getting off the couch. Movie's are the best way to spend a night in, you turn on the TV and decide to fire up your old friend Netflix.
The hunt for the perfect movie begins. (7:32PM)
One of the most difficult things about deciding to watch a movie is actually picking the perfect movie to watch. You flip though all the movie's on the main page, flipping through the list 2 or more times. The struggle to find the perfect movie is real.
Picking one movie is hard so you decide to try and figure out what genre movie you want to watch (8:32PM)
This in itself is an impossible task but you have far less options to choose from so you tell yourself it can be done. You flip through picking 3 different genres but you struggle committing to one of them. Finally, you decide that your in the mood for a comedy (Everyones always down to watch a comedy)
You hit a snag when, after an hour, you realize that you're not quite in the mood for a Comedy anymore. (9:32PM)
Fuck genre's, you scroll back to the main page, and go straight to the trending list on Netflix. WHAT ARE THE PEOPLE WATCHING?! Someone has to have some good idea's on movies to watch.
You've looked at every possible movie on the Main Page of Netflix and still can't decide(10:15PM)
You've actually gone over each movie twice, maybe even three times, but you can't decide. The frustration mounts as you begin to realize that you'll never find the "Perfect movie to watch.
You look at the clock and realize it's 10:35PM, you still haven't picked a movie to watch, and that your super picky nature is why you're going to grow old alone without so much as a movie to watch.
5 Movies Inspired by Stephen Hawking
Woke up to extremely sad news that Stephen Hawking passed away this morning, he will be remembered as a genuinely brilliant, and inspired physicist. I listed 5 films that were inspired by his life and the Actors who played him.
The Theory of Everything (2014) – Eddie Raymond
Hawking (2013) – Documentary/Himself
Hawking (2004) – Benedict Cumberbatch
A Brief History of Time (1991) – Documentary/Himself
Beyond the Horizon (2009) – Documentary/Himself
FANTASTIC BEASTS: THE CRIMES OF GRINDELWALD – In the New Trailer Dumbledore steals the Show
Gallery March 14, 2018 EnjoyTheTom Leave a comment
The new trailer for FANTASTIC BEASTS: THE CRIMES OF GRINDELWALD was released today, I'm sure every Harry Potter fan is excited to see this trailer, it looks like Dumbledore (Played by Jude Law) will be stealing the show, just take a look at how he carries himself in the trailer.
Johnny Depp is back and looking all sorts of weird, he grew his hair out (Thankfully) and is a much darker and twisted version of Grindelwald . Compare his look in the pictures below, this alone leads me to believe the sequel is going to be better than the original.
The movie looks amazing, but I'm bias, I loved Harry Potter and the first Fantastic Beast movie, I can admit that it wasn't nearly as good as any of the Harry Potter Movies.
I'm still super excited to see it Big fan of JK Rowling Stonessss
ActionFantasyHarry PotterJohnny DeppJude LawMoviesSci-FiThriller
Fact's About the Making of the First Jurassic Park
As we all know Jurassic Park is one of the most memorable movies for a generation of cinema fans. I remember it as being the first movie I ever saw in theaters, being absolutely terrified by the surround sound, thinking a dinosaur was waiting behind me to take a bite. It also sparked a ever-lasting love of films and filmmaking in me that I will cherish forever. In honor of the upcoming blockbuster Jurassic World: Fallen Kingdom coming to theaters on June 22, 2018, I've put together a list of some little known fact about the Marking of the first Jurassic Park. Enjoy!
1. The T-Rex would often unexpectedly turn on without warning, Terrifying the crew!
Producer Kathleen Kennedy recalled, "The T. rex went into the heebie-jeebies sometimes. Scared the crap out of us. We'd be, like, eating lunch, and all of a sudden a T. rex would come alive. At first we didn't know what was happening, and then we realized it was the rain. You'd hear people start screaming."
2. The T-Rex wasn't suppose to break through the glass roof of the Jeep while trying to eat the kids.
In the original script, the T-Rex was suppose to bump into the glass, frightening the kids, and then pull away. What actually happened was the T-Rex broke right through the glass causing to fall on the kids inside. If you watch the movie again, note how realistic the screams are!
3. Every film in the Jurassic Franchise has a reference to another Spielberg movie.
Jurassic Park: Shortly after Nedry makes his first appearance in the control room, during his argument with Hammond, one can clearly see Jaws playing in a small video window on one of Nedry's computer screens. That movie was, of course, also directed by Steven Spielberg.
The Lost World: When the bus crashes into the front of the video rental store, a poster can be seen for Hook, which Spielberg also directed.
Jurassic Park III: When the paleontologists enter the bar for dinner with the Kirbys, you can see a Jurassic Park (1993) pinball machine in the background.
Jurassic World: The great white shark being eaten in Jurassic World is a clear homage to Jaws
5. The Dinosaurs in the First Jurassic Park Were the First Fully CG Flesh and Blood Creatures Ever on Screen
For the animatronic dinosaurs, Spielberg hired Stan Winston (because of his amazing work on Aliens). Winston built the life-size lizards, including the Tyrannosaurus Rex and Triceratops. Spielberg also hired stop-motion puppeteer Phil Tippett to animate model dinosaurs that would be superimposed in post-production, and Dennis Muren (fresh from creating the molten-metal morphing effects for Terminator 2: Judgment Day) to see if dinosaurs could be created using computer-generated imagery.
The dinosaurs Muren created on the computer were the first major flesh-and-blood CGI creatures in movie history. When he screened an early test of wire-frame dinosaurs in motion for the rest of the filmmakers, Tippett realized he was out of a job. "I think I'm extinct," he told Spielberg, who liked the quip so much that he put it in the movie. In reality, Tippett stayed on as an adviser to the computer animators, using his knowledge of paleontology and pantomime to instruct the effects artists in how dinosaurs should move.
5 Thoughts when you have Social Anxiety and you're at the Movie Theater
"I have to pee, oh god, everyones going to look at me! They're going to know I have to pee, or worst they'll think it's a number 2, I'm fine, I'll wait till the movies done, its fine"
Me: Let's sit right in the middle!
Also Me: Oh, there 3 or 4 people kind of near the middle better just sit off to the side, don't want to annoy them by sitting too close.
Feeling trapped in a confined spaces with a bunch of Strangers in the dark is totally fine for anxious people.
That awkward moment when your butt fall asleep because you've been sitting for 2 hours but you don't want to get up and walk around for fear of annoying other movie goers
When someone who's 7 Feet tall is sitting behind you and accidentally keeps hitting the back of you chair but you don't want to cause a scene so you convince yourself that you enjoy it.
News, Release Dates
Ready Player One Premier's at SXSW
Steven Spielberg's newest Blockbuster Ready Player One (March 28th, 2018) premiered at SXSW to mixed reviews. Some people are hailing it as Spielberg's return to nostalgic blockbusters and others saying it offers "…nothing new or exciting.." – After going through hundred's of tweets, I would say the majority of people loved it. The common trend seems to be that normal movie goers love the movie but critics are picking it apart on technicalities on it's Story Telling.
I think critics need to understand that movies don't have to be perfect, sometimes, movies are perfectly nostalgic and are made to make evoke happiness, instead of being a commentary on social injustices. I'll update this as soon as I see the movie.
Check out the trailer and a few tweets below…
#ReadyPlayerOne is classic Spielberg fun! What a blast, can't wait to see it again. Rewards repeat viewings. Tons of great references, visuals and heart. So kick ass it blew the speakers!
— Robert Rodriguez (@Rodriguez) March 12, 2018
#ReadyPlayerOne is classic Steven Spielberg. It's got the references, the ferocious effects and the great '80s soundtrack, sure, but also the charm, the heart, the humor and a fantastic Alan Silvestri score. I loved it & so did this #SXSW crowd. Be excited for it! pic.twitter.com/xwPOGwXDxd
— Erik Davis (@ErikDavis) March 12, 2018
#ReadyPlayerOne posits a corporate big wig who exploits fan culture for profit as its villain. The irony of that is giving me a headache. This is no love letter to pop culture. It's a crass play to nostalgia; it offers nothing new or exciting.
— Kristy Puchko (@KristyPuchko) March 12, 2018
Tommy Wiseau's Auditions for the Joker (This is not a joke)
Some of you may not have heard but Tommy Wiseau (The Room) (He is also the subject of James Franco's latest film The Disaster Artist) has been saying for some time now that he'd like to star as the Joker in the any of the 3 rumored spin-off movies that are coming out. We found his audition tape and I have to say It's painfully terrifying!
Lists, Movie Picks, News, Release Dates
Top 5 Summer Blockbuster to Get Excited About
Gallery March 13, 2018 EnjoyTheTom 1 Comment
Every summer viewers are blessed with the release of the year's biggest blockbusters. I took some time to list some of the movies I'm most excited to see this summer.
Avengers: Infinity War (April 27th, 2018) – Rumor has it that the follow up Avengers movie is slated for release exactly one year after Infinity War is released.
Solo: A Star Wars Story (May 25th, 2018) – One Rumor that has been confirmed to be true, we will finally see how Han Solo acquired the Millennium Falcom from Lando!
The Incredibles 2 (June 15th, 2018) – I have been waiting for this for so long, the original was released in 2004! We've been waiting 14 years for this, let's go already!
Jurassic World: Fallen Kingdom (June 22nd, 2018) – This installment in the Jurassic franchise is being directed by J.A Bayona (The Orphanage, The Impossible, A Monster Calls), after watching the trailer I have a feeling this will be the most frightening film in the Jurassic collection.
Deadpool 2 (May 18th, 2018) – I mean it's hard not to get excited about this movie. Ryan Reynolds is back as everybody's favorite douchbag, Deadpool! Josh Brolin being added as the villain is awesome, I mean the guy is tough as nails, and is the perfect man to play Cable!
ActionComic BookHulkMarvelMoviesNew MoviePicksRelease DateThorThriller
Christopher Nolan Marathon Time
Christopher Nolan is one of my favorite film-makers, I feel in love with his movies when I watch Memento (2000) 18 years ago, and have loved every movie he's made since then. Today we list the ultimate Christopher Nolan Marathon list, Enjoy!
1. Memento (2000) – This movie only took 25 days to shoot
2. Insomnia (2002) – The only movie where Nolan is not credited for writing the movie, even though, he wrote the final draft
3. Batman Begins (2005) – Nolan was so fascinated with Cillian Murphy's bright blue eyes that he kept trying to find reasons to have Crane remove his glasses.
4. The Prestige (2006) – Nolan meticulously studied Tesla's experiments to recreate them with integrity. Especially the light globe scene.
5. The Dark Knight (2008) – Heath Ledger created the make-up for The Joker, when Nolan saw it, he immediately asked his make up team to recreate it.
6. Inception (2010) – Leonardo DiCaprio provided a lot of feedback and changes to the actual script. Nolan was quoted as saying "Once Leo came on board, I spent months and months sitting with him and discussing the script"
7. The Dark Knight Rises (2012) – This movie was the fastest to shoot out of all of Nolan's Batman movies.
8. Interstellar (2014) – The plot of this movie was so secretive, Matthew McConaughey didn't even revel the plot to his wife until the post-production was complete.
9. Dunkirk (2017) – The ticking sounds that serve as the crucial theme on the Dunkirk's score were recorded by Hans Zimmer from one of Nolan's own pocket watches.
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Movie Picks, Nerdy Trailers, News, Release Dates
Hype Movie Alert: Jurassic World 2: Fallen Kingdom
The first movie I ever saw in theaters was Jurassic Park, so it should come as no surprise that I am super excited for the release on the latest installment in the Jurassic Universe.
So far the biggest news I've seen is that Jeff Goldblum is set to return as Dr. Ian Malcolm. Ladies and Gent's Get your popcorn ready for June 22, 2018 that's when Fallen Kingdom is set to be released.
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Movie Picks, News, Release Dates
Hype Movie Alert: A Quiet Place
Ladies and Gentleman Jim from the office is all grown up and in a Horror movie now! This past weekend John was in Austin at SXSW 2018 to premier his latest film A Quiet Place, the reviews have started coming in and people are impressed/terrified! Check out some of the tweets…
#AQuietPlace is a masterclass in suspense. It weaponizes your own screams against you. The tension is so taut your stomach will turn in relentless knots. Totally deliciously terrifying. #SXSW18
#AQuietPlace: Wow. Opening night at #SXSW brought it *hard.* Thrilling, tremendous sound design and genuinely frightening. What could have been a "gimmick" flick strikes fear and tugs the heartstrings. Survival horror with the right influences.
— Matt Donato (@DoNatoBomb) March 10, 2018
#AQuietPlace was the PERFECT flick to kick off this fest: nerve-shreddingly tense, thoughtfully acted, and committed to the hopelessness of its setup. one hell of a debut for Krasinski, who's going for something part Sam Peckinpah, part Cormac McCarthy, and NAILING it #SXSW18
— Isaac Feldberg (@isaacfeldberg) March 10, 2018
Needless to say I'm looking forward to this one, the storyline seems original, and intense. Well done Jim Harper, Well done.
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Top 5 Old Movies You Need to Rewatch Now
Good Will Hunting (1997)
Something about watching snobby upper-class people fawn over a seemingly average everyday Genius is heart warming. The dialogue between Robin Williams and Matt Damon is incredible and the scene when Matt Damon has an emotional break through with Robin Williams still makes me tear up.
The Godfather Trilogy (1972, 1974, 1990)
Mario Puzo's The Godfather, one of the most iconic movie trilogy's ever created. The performances by all actor's in this movie are mesmerizing, the dedication to making this a one of a kind movie, for example, do you remember the scene with the horse's head in the movie producers bed? Guess what, they got a real horses head from a dog food company and used it without telling the actor, so when we moved the sheets and saw the head his screams are genuine as he was not expecting to see a REAL severed horse head in the scene.
E.T. The Extra-terrestrial (1982)
This movie was nominated for 9 OSCARS! A Sci-Fi movie about a weird looking alien and the group of kids who found him received more Oscar noms than some dramatic serious movies that are made with the sole intention of receiving awards. This movie was actually suppose to be very different, Spielberg originally intended this movie to be about a family that is terrorized by a group of aliens, he decided that it would be better suited as a family friendly movie and because of that we have this master piece.
Indiana Jones: Raiders of the Lost Ark (1981)
Another Speilberg movie makes the list, but are you surprised?, he is one of the most iconic storytellers. Indiana Jones is just a fun movie to watch, everything about it, you have a hero, a villain, and a whole lot of action in between. Harrison Ford cemented his place as a leading man with this movie. The iconic scene in the market when the crowd parts ways to reveal a sword swinging bad guy, the audience thinking a big over the top fight scene is about to take place, instead Indie pulls his gun out a shoots him! Guess what, that was improved by Harrison Ford and is one of my favorite parts of the movie.
Everyone should have seen this movie at least once by now, the story of a simple man, and his journey through life. Tom Hanks is one of my favorite actors, he seem like he'd be a nice guy if you ran into him on the street. Also based on everything that's going on in Hollywood it's nice to know that there are still some good guys out there. This movie garnered a total of thirteen Academy Award nominations, of which it won six, including Best Picture, Best Visual Effects, Best Director (Robert Zemeckis), and Best Actor (Tom Hanks). While you're rewatching this movie take a close look at any picture of Forrest through out the film? Notice anything? HIS EYES ARE CLOSED IN ANY PICTURE OF HIM IN THE MOVIE!
Let me know what you think of the picks for oldies to re-watch. Thanks!
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Thor: Ragnarok Out Now
March 6, 2018 EnjoyTheTom	1 Comment
Hulk Making an Appearance arance
That's not a frightening hat at all
Me jumping into my Saturday nights
The long awaited third movie in the Thor Franchise will be available online and on DVD today! – Chris Hemsworth can do no wrong, Marvel movies are always a treat! Check out Thor Ragnarok out now!
Imprisoned on the other side of the universe, the mighty Thor finds himself in a deadly gladiatorial contest that pits him against the Hulk, his former ally and fellow Avenger. Thor's quest for survival leads him in a race against time to prevent the all-powerful Hela from destroying his home world and the Asgardian civilization.
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The Definitive list of Movies About Fish Men/Sea Monsters
Gallery March 6, 2017 EnjoyTheTom Leave a comment
In light of "The Shape of Water" winning the Oscar for best picture, we thought we'd share the definitive list of movies featuring none other than Fish People/Sea Monsters. If we missed any let us know in the comments
1. The Creature from the Black Lagoon (1954)
2. Revenge of the Creature (1955)
3. The Creature Walks Among Us (1956)
4. She-Creature (1956)
5. War-Gods of the Deep (1965)
6. Humanoids from the Deep (1980)
7. Dagon
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News, Reviews
The Shape of Water wins Best Picture
March 5, 2017 EnjoyTheTom	Leave a comment
Guillermo del Toro does it again! A visually stunning movie with excellent performances from the entire cast. I can't believe a movie that would of been pitched as a thriller/musical/interspecies love story got made, let alone, won Oscar's and is being regarded as one of the best movies of the year.
Online Release Date: March 13th, 2018
It was an "uncomfortable" story line and some people might not like it but damnnnnnnn it was engaging and made me want to keep watching.
FUN FACT: Guillermo del Toro was drunk at a Golden Globes party when he pitched the idea to Hawkins
Definitely worth watching!
Acting: 5/5
Comedy: 2/5
Frightening: 2/5
Enjoyment: 3/5
Best PictureGuillermo Del ToroOscarsThe Shape of Water
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redpajama_set_name: RedPajamaCommonCrawl


In the heart of happening Darlinghurst is this stylish and cozy two-bedroom terrace that screams cool. With exposed brick feature walls, polished timber floors and rustic finishes, this home echoes the style of a Brooklyn loft and makes for the perfect home base.
At first entry, guests are greeted by a warm, inviting living room, brightened with luxe interiors, plush soft furnishings and a traditional fire place in an exposed brick wall. This room is open into the dining and kitchen area, which are light, airy and spacious, and lead outside to a lush courtyard. There is also a main bathroom and internal laundry on the ground floor.
Upstairs is the master bedroom, with its own Juliet balcony looking out onto the streets of Darlinghurst, as well as a larger terrace off the hallway with views of the Sydney CBD. A loft space turned second bedroom is on the topmost floor of the property, its bay windows, white finishes and natural light creating a peaceful, bright atmosphere to retreat to in the evenings.
Darlinghurst is both close to the buzz and action of Sydney s city, and a culture hub in and of itself. It is home to an abundance of renowned cafes, restaurants and bars, where you can people watch while sipping your morning espresso, or dig into a hearty modern Australian pub meal. Oxford Street s lively nightlife scene is also just minutes away, whether you are in the mood for a quiet drink, or ready to dance until the sun rises.
Public transport is within easy reach, ready to take you further into the city or through the many more sights Sydney has to offer, including Bondi Beach, Centennial Park and the rest of our vibrant inner city hubs.


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Time24 News
Home Sports 21-year-old star dead
21-year-old star dead
The e-sports world lost one of its big stars yesterday.
Maurice "Fero" Henriquez's family even confirms the tragic death on his Twitter account, and at the same time says that he died as a result of a heart attack.
EARLY DEPARTURE: Several of e-sports' big clubs and stars have expressed their grief after Maurice Henrique's death. Photo: Florida Mutineers / Dexerto
He was one of the most prominent profiles in e-sports and was part of the club Florida Mutineers.
Internet star (25) dead
His club praises Henriquez on his official Twitter account, stating that the player died after "several heart attacks".
– The Mutineers family unfortunately confirms today the sudden death of Maurice "Fero" Henriquez after several heart attacks. This is an incredible loss for his family, friends and our Florida Mutineers team. He will be greatly missed every day, the club writes, among other things.
Incorrect messages
It was Swedish Expressen that first mentioned the news in Scandinavia.
In the midst of grief, the family has had to refute reports that Henriquez took his own life, according to the e-sports website Dexerto.
"The truth is that Maurice suffered a heart attack on Sunday night, then three heart attacks on Monday and four heart attacks today," writes mother Connie Henriquez on Twitter.
Brax (21) is dead
"Fero" has been a professional "Call of Duty" player since 2014 and won three Call of Duty Home Series tournaments with the Florida Mutineers. He is said to have been one of the team's key players since he arrived there in March this year.
PROFILE: E-sports has lost one of its big profiles. Photo: Florida Mutineers
After the death, tributes from many of e-sports' biggest profiles began to flow in on social media. Both his former clubs and countless e-sports professionals express shock and compassion.
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Call of Duty League pays tribute to him with the following words:
– His absence will be felt throughout the league and the entire "Call of Duty" e-sports community.
TV star (38) found dead
Toronto Ultra star Anthony "Methodz" Zinni is one of those who shares his grief on Twitter:
– My heart is broken. When we last spoke, it was nothing but jokes and laughter. I am grateful to have been one of his teammates and experienced such a lively, passionate person. Rest in peace, brother.
DEEP GRIEF: Chrissy Teigen and John Legend were expecting their third child together, but in one post on instagram, Teigen himself reports that they have lost the child.
Fero has previously been affiliated with major e-sports clubs such as 100 Thieves, Team Envy, Reckless and Team Kaliber.
100 Thieves describes the death as follows on Twitter:
According to Store norske leksikon, e-sports is electronic competitive gaming where athletes compete against each other in various computer games on computers or game consoles.
Support for e-sports has grown tremendously in recent years. Today, professional tournaments can be watched by millions of people around the world. In professional leagues, you can win big cash prizes.
ALSO READ: Therefore, she moves on quickly
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Shrek's Adventure! London tickets
Duration: up to 1 hour 15 minutes
Join Shrek, Donkey, and all their friends in Far Far Away
Interact with real actors in areas from the movies
Meet other famous DreamWorks characters from Madagascar, Kung Fu Panda, and How to Train Your Dragon
Join your favorite DreamWorks characters on a fascinating journey at Shrek's Adventure in London. You'll travel to the Kingdom of Far Far Away aboard a magical 4D tour bus with Donkey as your tour guide. It's sure to be a mad tour of calamity, chaos and fun! Live actors in each area will entertain you and guide you on this fantastic journey. You'll reach Shrek's Swamp where you'll have a chance to look for him with the help of Cinderella before setting off on other adventures including gazing into a crystal ball and visiting the dangerous Poison Apple Pub. Don't worry, if you get into trouble, Puss in Boots will save you! The adventure continues as you see a round of Wheel of Torture with Pinocchio and the Mirror Maze of Insanity with the Magic Mirror. You'll even visit the Muffin Man's House and cook up a spell with Gingy. At the end of the tour, you'll have the chance to relax and chill with some of your favorite DreamWorks characters from Madagascar, Kung Fu Panda, and How to Train Your Dragon. It's sure to be an unforgettable experience for the whole family!
Admission to Shrek's Adventure
Infant (0-2): Free
Children (3-15): Reduced
Riverside Building, County Hall, Westminster Bridge Road, London SE1 7PB
Please note that attractions may close areas/exhibits at their discretion on the date of your visit
No children under the age of 14 will be admitted unless supervised by an adult over 18 years old
There is no entry with luggage, however, London Waterloo Station has a left luggage facility where you can store belongings for the day for a small fee. Please enquire at the station for further information
There is a buggy park on the first floor for buggies and pushchairs as these items are not permitted on the tour
If at any time you need to leave the attraction, simply speak to the actor in the show you are in and they will arrange for someone to help you to the nearest exit as soon as possible
The Magic Bus Ride is a 4D cinema experience that includes sudden motion, water sprays, air blasts, fog and aromas. You can skip this section of the tour if you suffer from any disorder or condition that may be affected by any of the above, or if you have an overly sensitive nose and don't like the smell of swamps
The Magic Bus Ride has a minimum height restriction of 0.9 meters (3 feet). Rumpelstiltskin is too short. This ride is not suitable for guests who suffer from the following conditions: epilepsy, back or neck pain or any weakness in those areas, pregnancy, motion sickness, heart conditions or have a pacemaker, asthma or any other chronic illness
The Magic Bus Ride is accessible to wheelchair users who are able to transfer into the ride seat and have the ability to sit upright and brace themselves
Please check the calendar to verify updated availability
Tower of London tickets plus Crown Jewels and Yeoman Warder walking tour
Book your tickets to the Tower of London now to see the Crown Jewels and go on a Yeoman Warder walking tour guided by an actual Yeoman.
Windsor Castle, Oxford and Stonehenge tour
Explore Stonehenge, Oxford and Windsor Castle on a guided tour for a relaxing day trip from London to ancient sites and academic stomping grounds.
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Warner Bros. Studio Tour London - The Making of Harry Potter tickets with transport
Book the Warner Bros Studios London tour with transfer included, and enter the magical world of the Harry Potter films and sample the legendary Butterbeer!
London Eye tickets
Enjoy your London Eye and marvel at the best panoramic views of this iconic city.
Eye on the Thames river cruise
See London's best sights from the river Thames. The cruise features live commentary presented by expert guides that bring the city to life.
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London Eye fast-track tickets
Book these tickets now for fast track access to the London Eye to enjoy the best panoramic view of the city and its most loved attractions.
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Shrek's Adventure!


text:
Participant FAQs
Quest Spaces
We are excited to announce our keynote speaker for The Quest: Building and Growing An Ethical Organization.
Nouman Ashraf
Nouman Ashraf is an Associate Professor within the Organizational Behavior area at the Rotman School of Management.
He possesses a broad range of professional, academic and research interests, with a specialized focus on enabling inclusive and innovative practices within teams, organizations and boards. For the last decade and a half, he has held progressively senior roles at the University of Toronto, including most recently as the Director of Equity, Diversity & Inclusion the Rotman School of Management.
He is a recognized thought leader in governance and has taught thousands of directors in the national Rotman program on Not-for-Profit Governance in partnership with the Institute for Corporate Directors since its inception in 2007.
Nouman serves as Teaching Fellow at the Institute for Gender + the Economy. He is also an Associate at Trinity College within the University of Toronto and an Affiliated Faculty Member at the University of Toronto School of Cities.
At lunch time, he can be found at Massey College within the University of Toronto, where he mentors exceptional post-graduate students in his capacity as Senior Fellow Emeritus.
He has also served as a trusted advisor to executives globally across sectors.
To read more about Nouman Ashraf, please visit his biography page on the University of Toronto's website.
© 2017 York Region District School Board. All Rights Reserved.
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Quest Conference


text:
Some waste could find permanent home on-site
The Gazette staff
PIKETON – Officials overseeing the cleanup at the former Portsmouth Gaseous Diffusion Plant estimate there are 2.2 million cubic yards of waste at the site.
To put that in perspective, it's enough concrete, building materials, equipment and soil to fill Ohio University's Convocation Center 16 times.
Highly contaminated materials are shipped off-site. Clean materials, meanwhile, can be offered for recycling. As for the materials with lower levels of contamination, cleanup contractor Fluor-B&W Portsmouth has proposed a 100-acre, on-site disposal facility that would hold up to 5 million cubic yards of waste.
The facility would become the permanent home for building materials, soil from around the site and under its buildings and some of the equipment used in uranium enrichment, according to Fluor-B&W Portsmouth.
The company also is considering consolidating some of its existing landfills and excavating groundwater plumes to provide engineered fill material for the facility.
Preliminary work has begun at the proposed site of the facility — in the northeastern part of the 3,770-acre property — but it's awaiting regulatory approval from the U.S. Department of Energy and Ohio Environmental Protection Agency. A decision is expected sometime this year. The site was selected for its accessibility as well as its geology; the site sits on a deep layer of undisturbed bedrock.
Federal funding of $35 million already has been earmarked in the budget for fiscal year 2015, which begins Oct. 1, 2014.
The funding is in a capital line item that's fenced off from the rest of the site's Department of Energy budget, which is expected to decrease by $110 million. Fluor-B&W has cited the budget gap as the reason it might have to lay off 505 full-time Fluor-B&W Portsmouth employees and 170 subcontractors this fall.
Whether a reduction in the workforce will influence funding for the on-site waste facility remains to be seen. Fluor-B&W estimates the on-site disposal project alone would account for 4.3 million hours of labor.
If constructed, the facility would be built, capped and closed in about 12 years depending on funding, according to the company.


Zach will heading down to Association Forum's ENCORE event this morning at the Mid-America Club. Pretty sure they'll hand out name tags (they always do). So if you see him, say hi.
If you're here because you just heard about us today, feel free to have a look around.


text:
Picture Perfect Playgrounds, Inc.
A wealth of play and playground information at your fingertips.
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Sandbox Summit
Sandbox Summit is a series of conferences that undertake the mission to discover how technology affects the ways children play, learn, and connect with others. As technology becomes more pervasive in the lives of children, the goal of Sandbox Summit is "to ensure that the next generation of players becomes active innovators rather than passive consumers of technology."1
Sandbox Summit was co-founded by Claire Green and Wendy Smolen. As president of Parents' Choice Foundation, a nonprofit organization established in 1978 as a guide to quality children's media and toys, Claire organized the first Sandbox Summit to commemorate the foundation's 30th anniversary.2 Wendy has been involved in testing and evaluating toys for over 20 years as well as publishing her findings as editor and writer for several magazines, including Toy Wishes, Nick Jr. Family Magazine, and Parents.3
The first Sandbox Summit was held in January 2008 in conjunction with the 41st International Consumer Electronics Show held in Las Vegas, Nevada, where over 140,000 people were drawn to view the hottest, most innovative consumer electronics available.4 The four day conference brought marketers, educators, researchers, journalists, and key industry speakers together to address how "techno-toys" can be designed to engage children's minds as well as their hands. Speakers and panelists represented a variety of key players including those from Nickelodeon, Sesame Workshop, Cartoon Network, Mattel, Digital Blue, Microsoft, Disney Publishing, The New York Times, and The Princeton Review.5
Featured at the first Sandbox Summit was the release of a research study done by the Joan Ganz Cooney Center at Sesame Workshop, which is a research institute that studies the educational potential of digital media. The report entitled "D is for Digital" analyzed the current interactive media environment for children ages 3 to 11. After evaluating over 300 products, the report found that most do not take advantage of available research regarding the educational needs of children. Dr. Michael Levine, Executive Director of the Joan Ganz Cooney Center stated, "Kids today are spending almost as much time with media as attending school, so there is an opportunity to create more engaging educational products than ever before. Unfortunately, most of the new digital products we reviewed, with notable exceptions, do not yet promote the vital literacy, creativity, and problem-solving skills children need to succeed."6
Following the success of the first Sandbox Summit, the conferences continued to be held:
Sandbox Summit @ New York City – The New Playing Fields: Building a 21st Century Sandbox – September 2008 – focused on the need for toys that allowed for open-ended play, such as blocks and Play-doh7
Sandbox Summit @ The 92nd St. Y – Is Play Becoming Too Much Work? – November 2008 – addressed how and why children play and whether all toys needed a learning component8
Sandbox Summit @ ToyCon – Pay Attention/Play Attention: Making Play Your Most Valuable Asset – May 2009 – discussed ways to extend the fundamentals of play adapting existing toys to new trends and technology without destroying the essence of the play9
Child's Play Symposium @ Hofstra University – Why Pixels Need People: Technology Integration 101 – March 2010 – addressed balancing media with the classroom as a learning tool for children who are increasingly involved with technology10
Sandbox Summit @ MIT – iPlay, YouPlay, WiiPlay: How Play Is Changing Media & Media is Changing Play – May 2010 – innovators in children's media, books, toys, virtual worlds, and education discussed how traditional play has been shaped in the 21st century11
Sandbox Summit @ MIT – Game Changers: People, Products and Policies that Empower 21st Century Kids – April 2011 – presented the need to create digital media for children that engages and challenges them12
1. "About Us: The Sandbox Summit Story." Sandbox Summit. < http://www.sandboxsummit.org/aboutus.html > 19 April 2011.
2. Ibid.
3. "Bio." Wendy Smolen. < http://www.wendysmolen.com/bio.html > 21 April 2011.
4. "Sandbox Summit." Wendy Smolen. < http://www.wendysmolen.com/Sandbox%20Summit%20brochure.pdf > 21 April 2011.
5. :Sandbox Summit at CES 2008 A Playdate with Technology." Sandbox Summit. < http://www.sandboxsummit.org/summit_ces.html > 21 April 2011.
6. "Joan Ganz Cooney Center Finds Cause for Both Concern and Optimism in Billion Dollar Digital Media Industry Tarketing Kids 3-11." Joan Ganz Cooney Center. < http://www.joanganzcooneycenter.org/Press-Releases-45.html > 21 April 2011.
7. "The New Playing Fields: Building a 21st Century Sandbox." Sandbox Summit. < http://www.sandboxsummit.org/newplayingfields_summary.html > 21 April 2011.
8. "Events." Sandbox Summit. < http://www.sandboxsummit.org/events.html > 19 April 2011.
9. "Sandbox Summit @ ToyCon 2009 Pay Attention/Play Attention: Making Play Your Most Valuable Asset." Sandbox Summit. < http://www.sandboxsummit.org/speakers_toycon.html > 21 April 2011.
10. "Child Play Symposium. Why Pixels Need People: Technology Integration 101." Sandbox Summit. < http://www.sandboxsummit.org/pixelsneedpeople.html > 21 April 2011.
11. Op. cit., "Events."
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The Garmin Vivoactive is a more like a smartwatch. It includes native GPS tracking; something most devices do not have. It can display calls, texts, emails and even social media notifications. Plus, it can track a variety of activities like running, biking, swimming and golfing. A dedicated swimming app will allow you to track your swimming routine stats. It has a 5 ATM rating, which means it�s safe to go underwater up to a depth of 50 metres (164 feet). Supposedly, the battery will last for up to three weeks in watch/activity tracking mode or 10 hours with the GPS active.


Providing an evidence-based, practical guide to care in all areas of children's pain management, Managing Pain in Children offers nurses and other healthcare professionals an introduction to the skills and expertise to manage children's pain effectively.
This fully-updated second edition first explores the relevant anatomy and physiology of children, the latest policy guidelines surrounding pain management and ethical issues involved in managing children's pain. Various pain assessment tools available for children and non-drug methods of pain relief are then explored and applied to practice in relation to acute pain, chronic pain, palliative care and the management of procedural pain.
The evidence base, assessment techniques, pain-relieving interventions, and guidance for best practice in both hospital and community settings are covered throughout, making this title an ideal resource for all nurses and healthcare professionals working with children.
Alison Twycross is Head of Department of Children's Nursing and Reader in Children's Nursing, London South Bank University, London, UK.
Stephanie Dowden is Clinical Nurse Consultant (CNC) for Paediatric Palliative Care at Princess Margaret Hospital for Children in Perth, Western Australia. Prior to this she was CNC in paediatric pain management at the Royal Children's Hospital in Melbourne Australia.
Jennifer Stinson is Post-Doctorial Research Fellow and Advanced Practice Nurse for the Chronic Pain Programme at The Hospital for Sick Children in Toronto, Ontario, Canada.