text:
Public Health (JD/MPH)
JD MPH
Save time by completing both J.D. and master's degrees in our accelerated program.
Get personalized attention that's focused on you while earning your Juris Doctor and master's degree in public health. UND's specialized accelerated track allows you to earn your master's degree while getting on the law school track early.
On Campus or Online
Est. time to complete:
Why pursue JD MPH programs?
M.P.H. Application Deadlines
Fall:
J.D. Application Deadline
Our unique program allows you to specialize in a master's program while getting a jump start on law school. You complete both degrees in four years rather than five years — a savings in time and money.
The MPH portion can be done exclusively online.
The MPH program has a 100% employment rate in health careers.
In the MPH portion of the program, students will learn how to use law and policy to improve the health status of populations, how to identify the social determinants of health, and how to appreciate the diversity of structures for delivering health care delivery in various settings.
In the JD portion of the program students will learn how laws and regulations implement health policy, how to identify the legal requirements that impact public health programs and how to understand the peripheral legal ramifications health care reform
UND Law graduates consistently rank among those who graduate with the least debt.
JD MPH Specializations
Three specializations help you develop the necessary critical thinking, problem solving and communication skills to excel in this field.
The Indigenous Health specialization offered online, on-campus, and in a hybrid format provides you with a critical understanding of determinants and solutions to health disparities. UND's specialization is the only 100% online Indigenous Health program in the U.S.
Population Health Research & Analytics
The Population Health Research & Analytics specialization prepares you to produce convincing and scientifically sound information about population health, evaluate the effectiveness of interventions and provide the basis for improving health policies and programs. This specialization is offered 100% online synchronous or on-campus.
Health Management & Policy
The Health Management & Policy specialization gives you the skills needed to manage health delivery systems effectively and efficiently, analyze health policies and communicate to affect change in health policy and management. This specialization is offered 100% online, on-campus, and in a hybrid format.
Accredited JD and MPH Programs
The School of Law is accredited by the American Bar Association.
The Master of Public Health is accredited by the Council on Education for Public Health.
JD and MPH Programs
UND Law's first-time North Dakota Bar Exam pass rate is 87%
Provides the skills and expertise needed to operate in the complex and dynamic worlds of health law and public policy.
Graduates can find employment developing policy, working as lawyers specializing in health care delivery, insurance, or compliance; general counsel in a public or private hospital; or serve as experts within advocacy organizations devising legal responses to public health challenges.
Double your network when you build connections through the law school and medical school. In both the legal and medical, contacts are invaluable.
Work at an accelerated pace by dual-counting credits.
JD and MPH provides opportunities in health, medicine and law.
What can you do with a JD MPH?
Median annual salary for lawyers
Expected growth in employment of lawyers
A JD-MPH dual degree puts you in a unique group of educated individuals and opens doors to flexible career paths.
Public Health Attorney
General Counsel (Medical)
Human Rights Attorney
Pharmaceutical Counsel
Disability Rights Attorney
JD MPH Courses
Health Law & Policy Analysis
PH 555. Health Law & Policy Analysis. 3 Credits.
The U.S. health system is undergoing significant transformation, and public health has a critical role at the federal, regional, state, and local levels. Students will learn advanced skills in applied health policy including: researching health legislation (e.g., Public Health Service Act, Social Security Act, Affordable Care Act); understanding the interdependent role of laws, administrative rules, executive orders, and judicial decisions in policy making and implementation; analyzing the evidence base for public health policy interventions; writing brief summaries of proposed legislation; preparing legislative testimony to inform health policy decisions; evaluating and comparing potential health policy interventions; and identifying opponents, proponents, advocates, and other stakeholders related to specific health law policy issues and interventions. Prerequisite: POLS 552. F.
Policy in Public Health
POLS 552. Health Policy. 3 Credits.
This course examines historic and contemporary trends in health care delivery in the United States. Emphasis is placed on addressing health care cost-containment issues; access to health care and, recent efforts to invoke broadly based systemic reforms of the U.S. health care system.
Political Advocacy & Social Entrepreneurship
POLS 562. Political Advocacy and Social Entrepreneurship. 3 Credits.
This course examines the use of social enterprises, including nonprofit, to achieve political, economic, and social change. Course coverage includes the use of social enterprises as vehicles for social transformation, development and execution of advocacy campaigns for social enterprises, the role of social enterprises within democracies, and the potential for social enterprises to address and overcome problems of collective action. S, even years.
American Indian Health Policy
PH 583. American Indian Health Policy. 3 Credits.
The course will provide a detailed overview of the unique policy issues that form the legal basis for provision of public health and healthcare services to American Indians and Alaska Natives. The American Indian (AI) population is unique in the United States in that AIs are born with a legal right to health services. This is based on treaties and numerous other laws, executive orders, court decisions and other legal bases in which the tribes exchanged land and other natural resources for various social services, including housing, education, and healthcare. The Indian Health Service is the federal agency responsible for carrying out the federal government's trust responsibility to provide public health and healthcare services to AIs. Prerequisite: Enrollment in MPH degree program or certificate or consent from instructor. F.
LAW 269. Insurance Law. 2 Credits.
International Human Rights Law
LAW 234. International Human Rights Law. 3 Credits.
Best JD MPH Programs
UND is increasingly regarded as one of the top institutions in the nation for public health. Our MPH program consistently ranks among the best for educational quality, affordability and career outcomes.
Leaders in Public Health
Alison Traynor received her online master's degree in public health and is currently the North Dakota Suicide Prevention Director.
Read Alison's Story
701.777.3000 | 1.800.CALL.UND
UND.edu/programs


This funding will enable the Armidale and Region Aboriginal Cultural Centre and Keeping Place (ACCKP) to complete its gallery works, car park, footpath, landscaping and install solar panels on the building. Being the only fully operating Aboriginal cultural centre and keeping place in the New England North West region, the ACCKP has become a significant venue for the community and surrounding regions.
The Guyra Historical Museum will undergo a major refurbishment and renovation, which includes painting the whole building, electrical and plumbing repairs, replacement of doors and flooring where necessary, and the temporary removal of all museum display objects whilst these works take place. The project also includes a new research space and upgrade of data research tools.
The upgrade of the Inverell Town Hall annex will re-energise the arts landscape in Inverell by boosting the capacity of the 1905 venue to host a wider variety of events. Following the upgrade, the annex will host arts, cultural and heritage events including drama workshops, pop up theatre, short films, acoustic live music performance, contemporary dance, week-long artist-in-residence programs and visual art exhibitions.
The Moree Civic Precinct – incorporating the Memorial Hall, Banquet Hall and Moree Plains Library – is an iconic 1923 building set in the heart of Moree's main street. It has long been the home of the dramatic arts for the region, however needs redevelopment to satisfy the current and future requirements of theatrical and dance groups, visiting stage shows, schools and community groups. The redevelopment will improve heating and cooling, access, amenity, acoustics, access for people with a disability, and fire safety, and provide a safe and modern stage.
Narrabri Shire Council will purchase an outdoor cinema screen and operating accessories for use throughout the shire (and adjoining shires when requested). It will provide cinematic, cultural and artistic experiences for the broader community and be available for community fundraising activities. The equipment will be based in Narrabri and transported to various locations as needed to serve the needs of community groups, outlying towns and neighbouring shires.
The revitalisation of the Barraba Museum will provide essential upgrades to the museum buildings to better support site activation, place making and access to the museum and its collection. This volunteer run museum requires essential building maintenance to provide a safe, secure and accessible museum that adequately cares for its collection. The project is supported by a dynamic volunteer community.
TRANSMIT will provide large-scale portable and permanent digital screens to enable wide community access to events occurring in places such as state galleries and universities. It will also support education programs for all ages and abilities. The screens will be located inside the Tamworth Regional Gallery and in other locations in the region. TRANSMIT supports access to the arts in regional Australia, the principle priority of the gallery since it opened nearly 100 years ago. TRANSMIT was launched on the gallery's centenary 1 June 2019.
Uralla Shire Council has been approached by Local Aboriginal Elders wishing to loan or donate artefacts to preserve and assist the community in learning about local cultural heritage. This display will offer a diverse and distinctive cultural experience by encouraging development and growth in the regional cultural sector. The cabinets will be placed in the soon-to-be-upgraded Visitor Information Centre allowing tourists and locals to experience and learn about the local Aboriginal Culture and strengthen the relationships between the Local Elders, Uralla Shire Council, the local Community and the high tourist market.


At the Law Offices of Tedone & Morton, P.C. we have extensive experience defending cases of DUI. Not only do we understand all aspects of Illinois DUI laws, but we have also successfully challenged BAC results, field sobriety test results, violations of rights and probable cause for the arrest, as well as Breathalyzer results. We are proud of our service to clients in defending them on all types of DUI charges.
We understand that you may have questions about DUI charges and other criminal law issues. We offer a free consultation to answer your questions and address all of your concerns.
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To discuss your legal needs with an experienced Illinois criminal defense attorney serving clients in Joliet, Will County, Grundy County, Kendall County, Kankakee County and beyond, contact our offices today. Your initial consultation will be free.


Charles Krauthammer on Friday marvelously demonstrated just how in the pockets of Barack Obama America's news media are.
CHARLES KRAUTHAMMER: [The President] talks a good game. "Oh, I'm prepared to do entitlements, I'm ready to do entitlements." Not once has he ever enunciated in public - other than all these leaks which I don't trust for half a second – one structural change in entitlements, and without that, everybody over the age of nine knows we are not going to get a handle on the debt. So let's hear him say it in public once.
GORDON PETERSON, HOST: The grand bargain.
TOTENBERG: …the grand bargain, Republicans backed away from it?
KRAUTHAMMER: When did he offer that?
TOTENBERG: He offered that last week.
TOTENBERG: In, he did it, publicly and in negotiations.
KRAUTHAMMER: In your leaks? What's in the $4 trillion?
KRAUTHAMMER: Give me a number. Explain to me what's in it.
TOTENBERG: Why is it, in two, in matter of two days, Republicans backed away from that and said we don't want it?
KRAUTHAMMER: You accept everything he says, a $4 trillion deal, if you don't have a single item in it that you can enunciate.
TOTENBERG: Well, I'm not at the table. Perhaps you are, but I'm not.
KRAUTHAMMER: Well then how does he expect America to accept something in which he explains nothing?
TOTENBERG: He actually said I'm going to get heat from my own people.
KRAUTHAMMER: My colleagues are demonstrating a point I've been trying to make about how you have a completely compliant, pliant, supine press accepting every leak out of the White House. Tell me, we have been told, I've heard it again and again that the President's prepared to do, to make cuts in entitlements. Name me one.
PETERSON: Charles, a complete and compliant supine press. I love that.
KRAUTHAMMER: I've got, I've got other adjectives, but we're short on time.
PETERSON: Yes, and we have to keep it on the air.
Once again, Krauthammer demonstrated a fabulous point.
For weeks the media have been telling Americans the President's big budget plan offered cuts in entitlements, but none of them can actually name what those cuts are.
Seems like that would be an important part of a report on spending cuts - specifically identifying what was going to be cut and by how much.
But that hasn't been important to the Obama-loving media during this debt ceiling debate.
If the President says his plan includes cuts to entitlements, that's good enough for them.


text:
Q: jooq use custom function in order by statement I'm currently trying to introduce this function  https://stackoverflow.com/a/12257917/4375998 into my project, but struggle with the function signature generated by jooq.
The generated code has these three signatures
public static String udfNaturalsortformat(
      Configuration configuration
    , String instring
    , Integer numberlength
    , String sameorderchars
)

public static Field<String> udfNaturalsortformat(
      String instring
    , Integer numberlength
    , String sameorderchars
)

public static Field<String> udfNaturalsortformat(
      Field<String> instring
    , Field<Integer> numberlength
    , Field<String> sameorderchars
)

But none of them seem to fit my use case of ordering a table by name.
This is currently done in the following fashion: In some place a collection of search parameters is generated and this is later included in the query:
public Collection<? extends SortField<?>> getSortFields(List<Pageable.SortField> sorts) {
        if (sorts.isEmpty()) {
            return Collections.singletonList(ProjectRepositoryImpl.LAST_ACTIVITY.field("last_activity").desc());
        }
        List<SortField<?>> sortFields = new ArrayList<>();
        for (Pageable.SortField sort : sorts) {
            if (sort.getSortDirection() == Pageable.SortDirection.DESC) {
                sortFields.add(PROJECT.NAME.desc());
            } else {
                sortFields.add(PROJECT.NAME.asc());
            }
        }

        return sortFields;
}

And the final query then looks like this
        Result<Record> queryResults = jooq.select(PROJECT.fields())
                .from(PROJECT)
                .where(searchCondition)
                .orderBy(transformer.getSortFields(pageable.getSorts()))
                .limit(pageable.getPageSize())
                .offset(pageable.getOffset())
                .fetch();

So what I currently attempt to do is replace the sort field with something like this
    sortFields.add(udfNaturalsortformat(PROJECT.NAME, 10, ".").desc());

but the signature mismatches.
What is the proper way to include this method in my order by statement?

A: As you can see in signatures of generated methods:
public static Field<String> udfNaturalsortformat(
      String instring
    , Integer numberlength
    , String sameorderchars
)

public static Field<String> udfNaturalsortformat(
      Field<String> instring
    , Field<Integer> numberlength
    , Field<String> sameorderchars
)

It has only overrides for all java simple objects (first one) or Field<?> references (second one).
Since you use PROJECT.NAME as a first argument, you would probably use second generated method, but then you have to pass other arguments all of Field<?> type. So try DSL.val or DSL.inline, which is a way to pass constant value as a field:
udfNaturalsortformat(Staff.STAFF.ACQUIRED_COMPANY, DSL.val(10), DSL.val(".")).desc();

redpajama_set_name: RedPajamaStackExchange


Enjoy your outdoor area all year long thanks to our stylish fire places and fire pits. Simple, eye catching designs, made from a durable, low maintenance steel. Ideal for any patio or garden area. Available in a range of styles and finishes.


text:
RENT A BENTLEY
The wings on the Bentley emblem represent the feel the driver has when conquering the roads of the world. The stability, luxury and speed of the journey, no matter if the road is straight or winding, will be a thrilling and extremely enjoyable adventure for all that experience it.
BOOK A BENTLEY
BENTLEY RENTAL
The world renowned Bentley is a British luxury car manufacturer that was also involved in racing vehicles. They were founded in 1919 and entered their first race in 1922 which was the Indianapolis 500. They also entered the 24 hours at Le Mans in 1924 and won the race. In the years of 1927 through 1930 they also came in first at Le Mans. This would be their last race until 2003 where they won Le Mans again. Bentley was an independent luxury car company with the inspiration to build a fast car, good car and be the best in its class. By 1931 Rolls Royce took notice of them and acquired this elite British car maker. This is when the grill of the Rolls Royce was first introduced to this British line of cars, but the Rolls Royce Logo was not part of their emblem. Bentley still retained its flying wings with a B in the center. What amazed the people at Rolls Royce is that Bentley never registered their trademark emblem. This situation was immediately remedied upon their purchase. In the early years each Bentley was built as a rolling chassis and sent to a coach builder to finish the interior of the vehicle.
That is no longer the case where most of the vehicles are built in Crewe England with a few in Germany. What really distinguishes a Bentley from other car makers is they are to this day still hand built. The care and craftsmanship of each individual creating them can be seen in the way no flaws can be found on their vehicles when finished. With the creation of each Bentley by hand, the owner or driver of one sets themselves apart from all others when on the road. Under the hood in most models is the 6 ¾ liter Bentley V-8 twin Turbo that produces over 500 horse power. This can be found in the Mulsanne model along with the Grand Convertible. It can reach 60 mph in 4.2 seconds with a top speed of 190 mph. The experience of driving a Bentley is like no other. You will be surrounded with luxury of a hand crafted automobile with more speed and power most people will never need, but it is there if you so desire to let the horses run wild. All of that with a ride that is like riding on a feather.
POPULAR BENTLEY CARS
BOOK THIS CAR
THE FLYING SPUR

redpajama_set_name: RedPajamaCommonCrawl


Purpose – This chapter analyzes landowner business development and economic sustainability in the context of large-scale mining in Papua New Guinea with a focus on the Lihir gold mine.
See what employees say about what it's like to work at Lihir Gold. Salaries, reviews and more - all posted by employees working at Lihir Gold.
It is operated by Morobe Mining Joint Ventures, a 50:50 joint venture between Harmony and Newcrest Mining. Newcrest's second Papua New Guinea mine is the gold mine located on Lihir Island in the New Ireland Province of Papua New Guinea.
mining tools in 1849 - newmillenniumfoundation.org. mining tools in 1849 Equipment Used The miners of the gold rush used many different ways and equipment for mining the how many kind of stone in lihir gold mining .
NHP, Good as Lihir Gold!
In a development designed to significantly increase total annual gold production from 700,000 to 1 million ounces per annum, Lihir Gold Mine in Papua New Guinea is currently undertaking a major upgrade.
The Lihir gold mine is situated in the Kapit-Ladolam area of Aniolam Island, the largest island within the Lihir group. Unlike many other mining districts in PNG, Lihir does not have a history of alluvial gold mining.


Discussion forum for Jeremy Clement's fans (St Etienne, FFL). Please post trade rumors, injury reports and amateur scout suggestions. Please do not post inappropriate comments, this is a friendly forum for fans. If you see inappropriate comments, then please report them by clicking the report abuse link aside the comment. Comments you post may require a paid membership to delete.
You have shed a ray of susinhne into the forum. Thanks!


One of QRMC's identified formal Business Objectives is "To provide a safe and rewarding work environment for all staff". We are also committed to ensuring that we satisfy our clients' safety requirements when conducting work on-site.
As a part of meeting these objectives, we have implemented an Work Health and Safety Management System compliant with AS4801 requirements, the harmonised Work Health and Safety legislation, and industry best practice, to guide the way in which we undertake our business.
QRMC's WHS Policy can be viewed on our website.
Our Work Health and Safety Management System is regularly reviewed to achieve continuous improvement. Feedback or suggestions are welcomed via safety@qrmc.com.au or phone (07) 3229 1744.
QRMC's Work Health and Safety Policy can be viewed on our Publications page.


text:
\section{Introduction}
The launch of {\it Fermi} Gamma-ray Space Telescope in 2008 provides the opportunity to examine $\gamma$-rays emitted
from compact objects, and 117 $\gamma$-ray pulsars has been detected with the first three years archival data  \citep{Abdo2013}.
Among all the pulsars detected by {\it Fermi}, 36 were directly found by the blind search in the $\gamma$-ray band and
34 of them were identified as radio-quiet with the threshold of 30 $\mu$Jy in radio flux density at 1400 MHz.
The population of radio-quiet $\gamma$-ray pulsars is expanding due to the continuous accumulation of {\it Fermi} data
and the improvement of the searching schemes (e.g., weighting $H$ test-statistic; \citealt{Kerr2011}).
This has imposed constraints on the pulsar emission geometry which suggests the radio emission and the $\gamma$-rays are not
produced in the same region of the pulsar magnetopshere. While the radio emission is originated from the cones emerged near the stellar
surface, the pulsed $\gamma$-rays are generally accepted to arise from the outer magnetosphere (cf. Cheng \& Zhang 1998; Takata et al. 2006, 2008).
The radio-quiet pulsars can be resulted from their different orientation of their radio beam and the observer's line-of-sight.
Therefore, determining the emission
geometry (e.g. magnetic inclination, viewing angle) is important for a better understanding of their properties. However, the lack of
knowledge in the phase relationship between the $\gamma$-ray light curves and that in radio leads to an ambiguity in determining
which peak in the $\gamma$-ray light curves is leading (see Trepl et al. 2010 for a more detailed discussion). Therefore,
pulsation searches in the other wavelengths, in particular in X-ray, are needed.

Only four of them have the X-ray pulsation detected so far (Halpern \& Holt 1992; Lin et al. 2010; Lin et al. 2013;
Marelli et al. 2014).
For those pulsars whose periodicities can only be detected in both X-ray and $\gamma$-ray bands are usually
classified as Geminga-like pulsars with Geminga (i.e. PSR B0633+17) as the prototypical example of this class \citep{HH92,Bert92}.
X-ray pulsations of three other known Geminga-like pulsars, PSR~J0007+7302 \citep{Lin2010,Car2010},
PSR J2021+4026 \citep{Lin&Hui} and PSR~J1813-1246 (Marelli et al. 2014) were subsequently discovered.
Except for PSR~J1813-1246 which has a very hard non-thermal dominant X-ray spectrum,
the phase-averaged spectrum of other three Geminga-like pulsars have multicomponent which consists of a
non-thermal contribution and at least one thermal component \citep{Car2004,Lin2010,Lin&Hui,Car2010}.
The pulse profiles in X-ray and $\gamma$-ray are dissimilar with an obvious offset \citep{Car2010,Lin2010,Lin&Hui}.
This suggests the pulsed emission in these two regimes are originated from different regions.
While the aforementioned three pulsars have similar X-ray/gamma-ray properties, we note that the derived paramaters (e.g.
characteristic age, magnetic field and spin-down power) of PSR~J0007+7302 and PSR~J2021+4026 are rather different from Geminga.

On the other hand, the X-ray counterpart of 3EG J1835+5928, RX J1836.2+5925, identified by \citet{MHEB2000} and \citet{MH2001}
has been considered as the ``next Geminga" for a long time because of the lack of radio detection
(a flux density of the radio observation at a frequency of 1.4 GHz $< 3\mu$Jy; \citealt{Abdo2010a}),
the similar spectral behavior and $\gamma$-ray luminosity to Geminga \citep{HGMC2002}.
The $\gamma$-ray pulsation of this source was finally detected by \citet{Abdo2009a}, and it was classified as a
middle-aged pulsar ($\sim 1800$~kyr) that is similar to Geminga.
The surface magnetic field ($\sim 5\times 10^{11}$~G) and the spin-down power
($\sim 1.2\times 10^{34}$~erg s$^{-1}$) of PSR~J1836+5925\ is about 1/3 to those of Geminga although its spin efficiency to
convert $\gamma$-rays is about one order of magnitude higher \citep{Abdo2010a}.
However, the lack of the pulsation detected in other wavelengths does not allow us to compare the emission properties at different energies.
Therefore, periodicity searches at other energies, particularly in X-ray band, are require to constrain its high energy emission
properties and enable us to compare its nature with other Geminga-like pulsars. The X-ray pulsation have been long sought for this
target \citep{HCG2007,Abdo2010a}. However, no positive detection has been reported yet.

Using the archival \emph{XMM-Newton} data of PSR~J1836+5925, we have performed a detailed temporal and spectral analysis observations.
In this Letter, we report the results from this investigation. In particular, we report the discovery of the X-ray pulsations
from PSR~J1836+5925\ for the first time.

\section{Observations and data analysis}

The latest {\it XMM-Newton} observations of PSR~J1836+5925\ were on 2013 February 14 and 16 (hereafter 0214 and 0216) have a total exposure
of $\sim$ 44 and 39 ks (Obs.~ID: 0693090101 and 0693090201; PI: Pavlov G.).
During these observations, the satellite was pointed to RA=$18^{\rm h}36^{\rm m}13.75^{\rm s}$ Dec=$+59^{\circ}25^{'}30.3^{''}$ (J2000), which is the timing position of the $\gamma$-ray ephemeris determined by \citet{Abdo2010a}.
In both observations,  MOS1/2 CCDs were operated in full-window mode and PN CCD was operated in small-window mode with a
temporal resolution of $\sim$5.7 ms which enables us to search for X-ray pulsations.
We reprocessed all the raw data with the tasks \emph{emchain} and \emph{epchain} in XMM-Newton {\bf S}cience {\bf A}nalysis {\bf S}oftware (XMMSAS version 13.5.0). For a rigorous analysis, we have excluded those events next to the edges of CCDs and bad pixels, which may have incorrect
energies.
The good events with ``PATTERN'' for MOS1/2 were selected in range of 0-12 to include single to quadruple pixel events, and those for the
PN in the range 0-4 to include only single and double events.
In our analysis, we only consider the events in the energy range of $0.2-12$~keV.
We also noted that all investigations have been contaminated by the X-ray background flare.
After removing all events which are potentially contaminated, the effective exposures were
found to be 41.1~ks, 41.3~ks and 41.4~ks for MOS1, MOS2, PN observed on 0214 and 32.3~ks, 32.2~ks
and 32.8~ks for MOS1, MOS2, PN observed on 0216, respectively. We determined the position of PSR~J1836+5925\ in each dataset with the
XMMSAS task {\it edetect$\_$chain}.

\subsection{Timing analysis}
For searching X-ray pulsations from PSR~J1836+5925, we utilized the PN data obtained in both observations.
Its nominal X-ray position in 0214 adn 0216 are
R.A.=$18^h36^m13^s.68$, decl.=$+59^{\circ}$ $25'30''.72$ (J2000) (with the uncertainty $\sim 0''.5$) and
R.A.=$18^h36^m13^s.92$, decl.=$+59^{\circ}25'29''.64$ (with the uncertainty $\sim 0''.7$).
Within the statisical uncertainties, they are consistent to the position determined by {\it Chandra}/ACIS (Advanced CCD Imaging Camera),
{\it Chandra}/HRC (High Resolution Camera) \citep{HGMC2002,HCG2007} and the $\gamma$-ray timing position determined in \citet{Abdo2010a}.
Since {\it Chandra}/HRC provides the most accurate positional determination, we adopted the position determined by this instrument,
R.A.=$18^h36^m13^s.674$, decl.=$+59^{\circ}25'30''.15$ (J2000) for the barycentric correction.
Events within a circular region of a 20$''$ radius centered at this position which corresponds to an encircle energy
function of $\sim76\%$ were extracted. We have 992 counts on 0214 and 806 counts on 0216 available for the timing analysis.
We then corrected the photon arrival times to Barycentric Dynamical Time (TDB) with the aforementioned X-ray position and
JPL Solar System ephemeris DE 405 using the XMMSAS task of {\it barycen}.

\begin{figure}[t]
\centering
\includegraphics[width=8cm]{BS.eps}
\caption{{\footnotesize Detection of X-ray pulsation on PSR J1836+5925.
The periodogram of Rayleigh-test in the frequency range of 5.76-5.78~Hz.
The independent trial in the search corresponds to the Fourier resolution of this observation (i.e. $\sim 4.76\times 10^{-6}$~Hz).}}
\label{PDetection}
\end{figure}

We noted that the $\gamma-$ray timing position of PSR~J1836+5925\ in the available ephemerides has a small offset from
our adopted X-ray position. For consistency, we constructed a new local ephemeris of this pulsar to cover the epoch
of these recent {\it XMM-Newton} investigations (i.e. $\sim$MJD~56338).
We used the {\it Fermi} Science Tools v9r27p1 package to perform the data reduction.
We obtained the {\it Fermi} LAT data in the energy range of 0.1-300 GeV within a circular region of interest (ROI) with a $0.8^{\circ}$ radius from the decided X-ray position of PSR~J1836+5925.
We used Pass 7 data and selected events in the ``Source" class (i.e.~event class 2).
Only a data span of $\sim1$~year, which brackets the epoch of two recent {\it XMM-Newton} observations, were
considered to avoid accumulated effects due to the timing noise propagated from a long-term data.
We also excluded the events with zenith angles larger than 100$\degr$ to reduce the contamination by the Earth albedo $\gamma$-rays.
For determining the pulse times of arrivals (TOAs), we built a template with the latest ephemeris reported by {\it Fermi} collaboration
\footnote{https://confluence.slac.stanford.edu/display/GLAMCOG/LAT+Gamma-ray+Pulsar+Timing+Models}
by means of Gaussian kernal density estimation (KDE).
We have obtained 25 TOAs by cross-correlating the template with the unbinned geocentered data. Each event was assigned to a phase
according to the KDE model.
With the position fixed at that determined by \emph{Chandra}/HRC \citep{HCG2007}, we fitted the TOAs with \textsc{TEMPO2} \citep{HEM2006,EHM2006}
to obtain a timing solution for PSR~J1836+5925\ that includes a spin frequency ($f$), a spin-down rate ($\dot{f}$) and a second derivative of frequency
($\ddot{f}$). The results are summarized in Table~\ref{ephemeris}.

\begin{table}[t]
\caption{{\footnotesize Local ephemeris of PSR~J1836+5925\ derived from LAT data which brackets the latest {\it XMM-Newton} observations on MJD~56337.45 and MJD~56339.44. The numbers in parentheses denote errors in the last digit.}}
\label{ephemeris}
\begin{tabular}{ll}
\hline\hline
{\footnotesize Pulsar name\dotfill} & {\footnotesize PSR~J1836+5925} \\
{\footnotesize Valid MJD range\dotfill} & {\footnotesize 56147.8---56522.2} \\
{\footnotesize Right ascension, $\alpha$\dotfill} & {\footnotesize 18:36:13.674} \\
{\footnotesize Declination, $\delta$\dotfill} & {\footnotesize +59:25:30.15} \\
{\footnotesize Pulse frequency, $f$ (s$^{-1}$)\dotfill} & {\footnotesize 5.7715448470(3)} \\
{\footnotesize First derivative of pulse frequency, $\dot{f}$ (s$^{-2}$)\dotfill} & {\footnotesize $-5.002(3)\times10^{-14}$} \\
{\footnotesize second derivative of pulse frequency, $\ddot{f}$ (s$^{-3}$)\dotfill} & {\footnotesize $-1(1)\times10^{-23}$} \\
{\footnotesize Epoch of frequency determination (MJD)\dotfill} & {\footnotesize 56338} \\
{\footnotesize Solar system ephemeris model\dotfill} & {\footnotesize DE405} \\
{\footnotesize Time system \dotfill} & {\footnotesize TDB} \\
\hline
\end{tabular}
\end{table}

Using the $\gamma-$ray ephemeris which is contemporaneous with recent X-ray observations, we can compare temporal properties in both regimes.
We directly folded up the PN data with the spin parameters in Table~\ref{ephemeris}.
For the data in 0.2-12~keV, the random probability to yield the X-ray pulsation of 5.7715448470(3) Hz at epoch of
MJD~56338 is $\sim 3.6\times 10^{-7}$ ($H$ test-statistic (TS) = 37.1) with a single harmonic (de Jager \& B\"{u}sching 2010).
We have also computed the periodogram of Rayleigh-test in the frequency range 5.76-5.78 Hz which is shown in Figure~\ref{PDetection}.
It clearly shows an X-ray periodic signal at 5.771545(5)~Hz with $Z^{2}_{1}=H~TS=39.5$. The quoted error of the frequency
corresponds to the Fourier resolution of this observation \citep{Lea87}. This is consistent with the pulse frequency in $\gamma$-ray regime.
To compare the pulse profiles between X-rays and $\gamma$-rays, we folded all the photons extracted from
{\it XMM-Newton} observations and those obtained from {\it Fermi} observations within MJD~56150--56520
in accordance with the $\gamma-$ray ephemeris Table~\ref{ephemeris}.
We also divided the obtained X-ray events into three different energy bands, which are similar to the studies
of three other Geminga-like pulsars \citep{Car2004,Car2010,Lin&Hui}.
The phase-aligned folded light curves at different energy ranges are shown in Fig.~\ref{PFXG}.
For the X-ray light curves, we have subtracted the background sampled from a nearby circular region with a radius of 20" centered
at R.A.=$18^h36^m20^s.752$, decl.=$+59^{\circ}26'07''.92$ (J2000).
The X-ray pulsation can be firmly detected in the soft X-ray band ($H$ TS=23.6 with a random probability of $\sim7.9\times10^{-5}$)
and marginally found in the medium X-ray band ($H$ TS=11.6 with a random probability of $\sim 9.7\times10^{-3}$).
Nevertheless, the significance is too low for claiming the detection in the hard band
($H$ TS=4.0 with a random probability of 0.2), which can be ascribed to the small photon statistic.

\begin{figure}[!t]
\centering
\includegraphics[width=8.5cm]{profile1.eps}
\caption{{\footnotesize Folded light curves of PSR~J1836+5925\ in different energy ranges.
Each panel shows the pulse profile of 12 bins in the energy band specified in the legend.
The epoch/phase zero of all the profiles were determined at MJD 56338 shown in Table~\ref{ephemeris}.}}
\label{PFXG}
\end{figure}

\subsection{Spectral analysis}

Because our adopted data have the total exposures of more than 80~ks, this enables us to place a tighter constraint on the
X-ray spectral properties of PSR~J1836+5925\ than the previous investigations \citep{HGMC2002,Abdo2010a}.
We extracted the spectra of PSR~J1836+5925\ from a circle with a radius of $20''$ centered at its nominal position in each EPIC data.
The background spectra were sampled from a nearby circular source-free region with a radius of $20''$ in individual dataset.
We generated the response matrices and ancillary response files with the XMMSAS task {\it rmfgen} and {\it arfgen}.
Since the X-ray emission from PSR~J1836+5925\ is relatively soft, we considered X-ray spectral fits in the energy range of 0.2--5~keV.
We grouped each spectrum so as to have a minimum of 15 counts in each bin.
We have examined each dataset individually and found that the inferred parameters are consistent within the tolerance of the uncertainties.
In order to optimize the photon statistics, we fitted all the EPIC data obtained in these two observations simultaneously.
The errors of the spectral parameters quoted in this Letter are in $1\sigma$ for 2 parameters of interest
(i.e. $\Delta\chi^{2}=2.30$ above the minimum) for single component models and in $1\sigma$ for 4 parameters of interest
(i.e. $\Delta\chi^{2}=4.72$ above the minimum) for multi-component models.

For the tested single component models (i.e. power-law and backbody), none of them can result in a statistically reasonable fit
(with reduced $\chi^2>1.5$).
It may indicate that the X-ray emission of PSR~J1836+5925\ comprises more than one spectral component.
Therefore, we proceeded to fit the data with multicomponent spectral models. We have found that the spectrum can be described by
an absorbed blackbody plus power-law model. We firstly attempted to perform the fitting with all parameters to be free, which
yields a column absorption of $n_{\rm H}<8.5\times10^{19}$~cm$^{-2}$, a photon index of $\Gamma=1.8\pm0.3$, a power-law model normalization
of $6.0^{+1.3}_{-1.2}\times10^{-6}$~photons~keV$^{-1}$~cm$^{-2}$~s$^{-1}$ at 1 keV, a blackbody temperature of $kT=62^{+11}_{-10}$~eV with
a emission radius of $R=1.32^{+2.37}_{-0.55}$~km at 800~pc. This results in a desirable goodness-of-fit ($\chi^{2}=90.46$ for 85 d.o.f.).

As the column absorption cannot be properly constrained, we also fitted the data with
$n_{\rm H}$ fixed at total Galactic HI column density of $4\times10^{20}$~cm$^{-2}$ in
the direction of PSR~J1836+5925\ \citep{Kalberla2005}. This yields the best-fit parameters of $\Gamma=2.1\pm0.3$, a power-law model normalization
of $(7.1\pm1.4)\times10^{-6}$~photons~keV$^{-1}$~cm$^{-2}$~s$^{-1}$ at 1 keV, $kT=45^{+10}_{-8}$~eV and a blackbody radius of
$R=6.3^{+7.8}_{-3.4}$~km. The corresponding goodness-of-fit is $\chi^{2}=101.8$ for 86 d.o.f. which is statistically acceptable.
The best-fit model and the observed spectra are shown in Figure~\ref{spec}.

We have also considered the spectral fit with a dual blackbody model.
However, the goodness-of-fit yielded ($\chi^{2}=109.3$ for 85 d.o.f.) by this model is worse than the power-law plus blackbody model.
Fixing the $n_{\rm H}$ at the Galactic HI value does not result in any improvement of the fitting.

\begin{figure}[t]
\centerline{\psfig{figure=ufspec.eps,width=7cm,angle=-90,clip=}}
\caption[]{The phase-averaged X-ray spectra of PSR~J1836+5925\ as observed by \emph{XMM-Newton} (MOS~1:cyan; MOS~2:yellow; PN:green) and
simultaneously fitted to an absorbed power-law plus blackbody model. The best-fit model for the thermal (red-dashed line)
and non-thermal (blue-dashed line) components are illustrated separately.}
\label{spec}
\end{figure}

\section{Discussion}

In this Letter, we report the discovery of X-ray pulsations from PSR~J1836+5925.
We found that the pulsed events both contribute in soft and medium bands (0.2--2~keV). On the other hand,
no indication of pulsation in the hard band ($>$2~keV) has been found in our investigation.
The X-ray and $\gamma$-ray pulsation from PSR~J1836+5925\ have significantly different behavior.
The pulsed $\gamma$-rays have a structure of relatively sharp double peaks which are presumably originated from
the curvature radiation emitted from the pair creation region in the magnetosphere.
The spin period of $P=173$~ms and the characteristic age of $\tau=1.8$~Myr suggest PSR~J1836+5925\ as a mature pulsar.
Assumming the emission is isotropic,
the GeV gamma-ray efficiency of PSR~J1836+5925\ is $\eta=(L_{\gamma}/\dot{E})\times 100\%=180\pm 1^{+200}_{-100}\%$
(second $Fermi$ pulsar catalog; \citealt{Abdo2013}), where $\dot{E}$ is the spin down power.
The first uncertainty of $\eta$ comes from the statistical uncertainties in the spectral fit and the second is due to
the distance uncertainty \citep{Abdo2013}.
This high efficiency of the GeV emission is similar to $\eta=97.4\pm0.3^{+300}_{-50}\%$ of typical mature pulsar --- Geminga,
if one assumes a 4$\pi$ solid angle. Considering the possible
overestimated distances and/or the beaming factor, the aforementioned conversion efficiencies can be overestimated. Taking the
more realistic parameters into account, this might result in an efficiency $\eta<100$\%.

In order to compare with Geminga, therefore, we discuss the origin of the X-ray emission of PSR~J1836+5925.
In the soft band (see Fig~\ref{PFXG}), the light curve is essentially sinusoidal which suggests the X-ray pulsation is mostly originated
from the modulation of the heated polar cap. This is consistent with the presence of a blackbody component inferred from the spectral fit.

To account for the power-law component, we discuss it in the context of the outergap model \citep{CZ98}.
According to this model, the non-thermal component of a canonical pulsar is synchrotron emission from the relativistic
$e^{-}/e^{+}$ in the outer magnetospheric gap \citep{TSHC2006,TCS2008} with a week absorption.
The photon index is expected to be in the range of 1.5--2.0 which is consistent with the best-fit value.
For the light curve in 0.7-2~keV, its profile is apparently different from that in 0.2-0.7~keV which might suggests a different origin.
In examining the relative
flux contributions by the thermal and non-thermal component, we found that while the non-thermal flux takes $\sim15\%$ in 0.2-0.7~keV its
contribution is $>99\%$ in 0.7-2~keV (see also Fig.~\ref{spec}).
This suggests that X-ray pulsations seen in 0.2-0.7~keV and 0.7-2~keV might have different origin.
However, the small photon statistics in the medium band precludes any firm conclusion.
To better characterize the X-rays from PSR~J1836+5925\ in different energy bands, a deeper observation is certainly required. With a larger number
of photons detected, we can also perform a phase-resolved spectroscopy to investigate how do the spectral properties vary across
the rotational phase which will provide important inputs for a physical modeling of the pulsar.

\begin{acknowledgements}
We thank Mr. Jason H. K. Wu of Max-Planck-Institut f$\ddot{u}$r Radioastronomie for providing useful comments on the temporal analysis
techniques.
This work made use of data supplied by the High Energy Astrophysics Science Archive Research Center (HEASARC).
This project is partially supported by the Ministry of Science and Technology of Taiwan through grant NSC~101-2112-M-039-001-MY3.
C.~Y~.H. is supported by the research fund of Chungnam National University in 2014.
J.~T. is supported by a GRF grant of Hong-Kong Government under HKU700911P.
C.~P.~H. and Y.~C. are supported by the Ministry of Science and Technology of Taiwan through the grant NSC 102-2112-M-008-020-MY3.
A.~K.~H.~K. is supported by the Ministry of Science and Technology of Taiwan through grants NSC~100-2628-M-007-002-MY3 and NSC~100-2923-M-007-001-MY3.
D.~C.~C.~Y. gets the financial support from the Ministry of Science and Technology of Taiwan through the grant NSC~102-2115-M-030-003 and the other FJU project of A0502004.
\end{acknowledgements}

redpajama_set_name: RedPajamaArXiv


text:
How is Illinois contributing to the Event Horizon Telescope Project?
Apr 10, 2019 8:15 am by Lois Yoksoulian | Physical Sciences Editor | 217-244-2788Expert ViewpointsPhysical Sciences
Event Horizon Telescope Project theoretical working group leader Charles Gammie, center, and graduate students Ben Prather, left, and George Wong helped interpret the massive amounts of data used to produce the first image of a black hole.
The Event Horizon Telescope Project announced that it has captured the first image of a black hole. The feature is located at the center of Messier 87 – a giant elliptical galaxy in the constellation Virgo. News Bureau physical sciences editor Lois Yoksoulian spoke with University of Illinois physics and astronomy professor Charles Gammie, who heads up the theory working group for the large, multi-institutional collaboration.
The existence of black holes has captured the attention of researchers for decades, but we have never actually seen one. How did the EHT Project achieve this task?
We could not just go to a telescope and snap a picture to capture an image like this. My collaborators gathered data from radio telescopes at six locations around the globe, from the South Pole to Hawaii to Spain. Putting that data together to make an image is one of the most complicated data analysis tasks in astronomy. It required two years of effort and vast supercomputer resources to process and interpret the petabytes of data gathered from all those telescopes.
What is Illinois' role in this project?
My research group at the U. of I. is a leader in theoretical modeling of black holes. The resources available to us at the National Center for Supercomputing Applications have allowed us to pioneer the computer simulation of matter falling into black holes. We are also one of the first groups to produce a model that consistently includes Einstein's theory of general relativity. That background played a large part in helping the project make sense of the massive amounts of data it had collected.
What are some of the discoveries made by your group, thanks to this image?
One of the things we are most excited about has to do with the luminous, fast-moving jets of gas that come from near the center of Messier 87. We were able to tie together the images and the supercomputer models to show that the jets are launched from very close to the black hole. The models say that the jets are powered by the black hole itself. Magnetic fields thread through the hole and brake its rotation, transforming the rotational energy of the hole into outgoing beams of electromagnetic energy.
Why is it important to have the ability to image a black hole?
First, we were able to check that the image is consistent with what we expect from Einstein's theory of general relativity, but in a new regime. Data from EHT allow us to probe matter in gravitational fields that are more extreme than any probed before using light. Second, the image tell us something new about how black holes work out in the wild, away from the theorist's chalkboard. Black holes famously suck in gas from their surroundings. But they can also spew out energy! Now we have a better understanding of how that works.
We are going to analyze and model the data that we have already collected on the black hole in the center of our own Milky Way galaxy. Over the next few years we are going to add radio telescopes to the Event Horizon Telescope network, improve the data collection and analysis process, and try to break and then improve our theoretical models. Even further in the future it may be possible to link Event Horizon Telescope to radio telescopes in space. That would be really exciting, because it would enable us to obtain crystal-clear images that are impossible to get from the ground.
To reach Charles Gammie, call 217-299-1527; gammie@illinois.edu.
Click here to view the U. of I. department of physics news release for the Event Horizon Telescope Project announcement.


Video presented as part of the conference Coplas Sefardies - Judeo-Spanish songs by Alberto Hemsi in Hanover on March 22nd, 2018 by Hervé Roten, director of the European Institute for Jewish Music.
Over 300 documents of the Alberto Hemsi fonds are kept on the premises of the IEMJ. It is mainly photos and scores bequeathed by Myriam Capelutto Hemsi, the widow of the composer.
In 2015 is released the CD Coplas Safardies, 5th disc in the collection « Musical Heritage of the Jews of France » published by the editions of theEIJM. A collection of Judeo-Spanish songs for piano and vocals, composed by Alberto Hemsi from 230 poems and melodies collected in the Sephardic communities of the old Ottoman empire.
10 volumes of music scores of the Coplas Sefardies will follow between1932.


text:
Q: Я не могу сделать адаптив секции на Bootstrap 5. Нужна помощь Макет сайта

Проблема в том что когда ширина становится меньше 567 px картина становится в ряд по два но безумное отступление
Проблемы с секцией Присоединяйтесь к нам в Instagram
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All Villa Estados homes currently listed for sale in Scottsdale as of 04/24/2019 are shown below. You can change the search criteria at any time by pressing the 'Change Search' button below.
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Join us for our BizTalk Speaker Series with Jerry Reynolds, from the Sacramento Kings!
Jerry Reynolds is an American former professional basketball coach and current executive in the NBA. He coached the Sacramento Kings for two different stretches; once in 1987 and from 1988 through 1989. He also served as the team's general manager. Jerry Reynolds served as general manager of the Sacramento Monarchs WNBA team, a post from which he retired in 2003. In 2005, Jerry Reynolds wrote a book about his 20 years of experiences with the Kings called Reynolds Remembers Tales from the Sacramento Kings. As of February 2006, Reynolds is a broadcaster for the NBA team alongside Grant Napear, and its director of player personnel.
The Sacramento Asian Pacific Chamber of Commerce BizTalks Speaker Series aims to inspire and educate regional businesses through powerful discussions with some of the most dynamic and influential minds in our region. Tapping into their unique experiences, BizTalks speakers enlighten attendees by sharing definitive moments in their journey that have cultivated opportunities for success.


text:
Q: How to revert a previous commit on the master branch and save the code in another branch? I just made a push on the production site and all the changes were on master. But i realized the code that i pushed needs to be altered so i need to revert the last commit but take all that code from that commit and put it in another branch so i can push it later....any way to do this

A: There are many ways to fix this.
Here's what I'd do (with a bit of extra insurance)
Assuming your HEAD is in 'the wrong place' (no pun intended), you can
 git branch rescue
 # you are still on master
 git reset HEAD^ # soft resets the last commit
 git push -f     # to undo the push - beware of other users of the push-branch

Now edit / rescue you commit in-place (because the last commit's changes are now pending again). If there is an emergency, you can always checkout the rescue branch, which is simply a copy of the HEAD when you started this post.

A: I recommend to fix already pushed commit with the correcting revert commit. You may also safely start your experiments from the reverted commit. See also Git Community Book, Undoing in Git
git revert HEAD
git push

Rewriting already published commits is considered as a bad practice (quote from the same section):

Fixing committed mistakes
If you make a commit that you later wish you hadn't, there are two
  fundamentally different ways to fix the problem:
You can create a new commit that undoes whatever was done by the old
  commit. This is the correct thing if your mistake has already been
  made public.
You can go back and modify the old commit. You should never do this if
  you have already made the history public; git does not normally expect
  the "history" of a project to change, and cannot correctly perform
  repeated merges from a branch that has had its history changed.

See also section "The Perils of Rebasing" from Pro Git, Rebasing why this is not good.

A: 2 steps:
1) do a branch off the current master.( Saving your code so you can do the fix. )
2) Roll back 1 Commit in master. git reset --hard HEAD~1


After all, he's done for you throughout your life it can be an uncomfortable feeling to have to worry about the cost when shopping for a Father's Day gift, but for those of us on a budget, it's an unfortunate reality. The good news is, there are plenty of thoughtful and affordable gift option that your father is sure to love. Have a look below for 7 of our favorite low-cost Father's Day gifts.
If you're dad commutes to work, then he's most likely familiar with the world of talk radio, NPR programming and an endless variety of podcasts. But another option for making the drive feel a little shorter is audiobooks, and Audible hands down has the best selection of titles out there. A subscription won't cost you more than a few dollars a month, and your father will think of you every time he enjoys a great new book.
It's an old joke that men don't read instructions, but the truth is sometimes a step-by-step pamphlet isn't enough to tackle every project your dad has on his "honey do" list. And while he probably won't ever buy it himself, a guidebook on any given topic is a perfect gift for a busy handyman. These days, we're used to just looking up how-to videos on YouTube, but many older dads will still prefer a book over an online tutorial.
Which dad doesn't enjoy a nice refreshing adult beverage after a long day? One way you can help him class up his cocktail game is with some artificial ice cubes. These are cubes of either stone or metal that can be frozen and then dropped into a drink in place of real cubes that will dilute his drink as they melt. They are simple, smart and on the less expensive side of the gifted scale.
Speaking of drinking, if your dad is less of a hard liquor drinker and more of a beer guy, skip the artificial ice cubes and get him coasters that double as bottle openers. Just do a quick online search for these handy beer accessories and you'll find more than a few varieties of coaster/openers. They are a fun and practical gift that any beer aficionado will appreciate.
One of the most underrated but useful inventions out there is the phone stand. Until you have one it's hard to understand the convenience of just dropping your phone into it when you get home after work and come back an hour later to find it fully charged. To find the right stand you'll need to know what model smartphone your dad owns, but after that, it won't be hard to find one at a reasonable price.
No, this isn't some kind of water or surfing related thing. A streaming stick is a device that lets you watch videos from your phone or computer on your TV, or just access video streaming services like Netflix, Hulu and Plex. There are several options to choose from, including Google's Chromecast, the Amazon Fire Stick or the Roku Streaming Stick. All of these are inexpensive options that will open the world of online media streaming to your father for around $50 or less.
This is the ultimate inexpensive gift, but it doesn't have to be a cheap one. While at first, it may seem like you're trying to squirm out of giving a real gift, the truth is that even as an adult there may be things your dad could use help with, especially when it comes to some of the more modern emergency borrowing options that are now available. You could help him answer questions like "how do I get ready for tax day?" or "Where are title loans near me?" Trust us, he'll appreciate the help navigating these money challenges.


The Chinese manufacturer will premiere its new device called Vibe Z in few days at CES 2014. The smartphone is equipped with LTE, it runs on Android operating system and it has a 5.5 inch full-HD display with a resolution of 1920×1080 pixels (400 ppi) and a wide view angle. Under the case we find a quad-core processor with a Qualcomm Snapdragon 800 chip and 2 GB of RAM. The internal storage is of 16 GB.
The fans of photography will love this device because Vibe Z has a 13 MP camera with f1.8 that produces sharp images in low light and an image processing software dedicated to high resolution cameras. There is a 5 MP secondary camera equipped with a 84 ° lens for wide-angle images.
Lenovo Vibe Z is equipped with a single micro-SIM and it works on GSM / UMTS frequency band up to 2100. WiFi connectivity and Bluetooth 4.0 is present on board.


text:
Ghana Beauty Awards 2021: 30 awarded for their contribution to the beauty industry
24th Nov 2021 | Source: Citi Newsroom
Thirty (30) individuals and organizations have been recognized and awarded for their contribution to the growth of the beauty industry in Ghana at the 5th edition of the Ghana Beauty Awards (GBA) held at the Kempinski Hotel in Accra.
Formerly known as the Ghana Makeup Awards, the GBA, according to its organizers, the new name is intended to encompass all aspects of beauty.
In her address, the CEO of Makeup Ghana, Rebecca Donkor, urged beauty practitioners to uphold standard practices, which her organization has been spearheading for the past five years through the award scheme.
She said her organization is also working with the Ghana Standards Authority (GSA) to formulate an industry code of practice document, which will be used to ensure that practitioners across the country uphold agreed benchmarks to promote professionalism.
According to her, over 1 million Ghanaians are employed in the beauty industry, which indicates that it can be further harnessed to become a major avenue for job creation to help address the problem of youth unemployment.
"Makeup Ghana's research indicates that the industry is growing and shows promise as a major employer in the coming years. It is these gains that we at Makeup Ghana wish to sustain and consolidate by initiating and sponsoring worthwhile industry projects."
Member of Parliament for Manhyia South Constituency and Minister of Energy, Dr. Opoku Prempeh, lauded Make up Ghana for spearheading the launch of the first-ever National certificate 1 and 2 curriculum for Make up artistry under the national TVET qualifications framework.
Dr. Opoku Prempeh, who was Minister of Education during the period of the introduction of the curriculum in 2020, said the government will continue to partner stakeholders in technical and vocational training to build the capacity of young people to enable them to become successful entrepreneurs.
The Ghana Beauty Awards (GBA) is an annual celebration for the Beauty Industry, aimed at fostering excellence, by rewarding and celebrating pioneers, leading professionals and upcoming talent within the industry, as well as businesses and brands who are contributing to economic growth.In a bid to include other sectors in the beauty space, the following categories were included in this year's edition; Most Promising Barber, Most Promising Nail Technician, Beauty Brand Ambassador of the Year, Student/Apprentice Of The Year, Best Hair Colourist, Barber of the year, People's Choice Award, Best Hair Cutting Stylist, Best Salon/Studio, Best Spa and Wellness Centre, and Best Customer Service Experience.
Mary J Blige on getting her confidence back
Cardi B speaks out after winning lawsuit
Disney responds to 'Snow White's outrage
Kanye West calls out Kim K
Was Hefner a champion of women?
A first look at 'The Proud Family'
Dede,BBN among Ghana's most watched
Elton John reveals he has COVID
Rihanna donates to climate justice
Cardi B wins in defamation case
Showmax launches 2 for 1 Black Friday deal
The Rock' to receive People's Champion Award


Combining High Performance with versatility, the Viper 30 provides a choice of mounting location, ensuring all application requirements are satisfied.
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The map is intended to show an additional package Tricolor TV "Children"
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Today we're reading Genesis 21, Nehemiah10, Psalm 20.
This devotional is about Genesis 21.
Earlier this week I skimmed a news item about former New Jersey governor Chris Christie. Christie left the office of governor earlier this week and, it is alleged that, after he was no longer the governor, he tried to use a VIP entrance at the Newark airport to bypass a security checkpoint. Instead of allowing him through, however, the TSA escorted Christie and his security team to the back of the TSA screening line.
Whether this story is accurate or not (Christie has disputed it), there are certainly many rights, privileges, and powers that he used to have as governor which are no longer his. When a person leaves a position of power, they lose the power the position gave them. The power stays with the position not with the person.
Here in Genesis 21, Abraham's life finally achieved a measure of peace. He felt at peace with God's promises because the son God promised him was born and had begun to grow and mature (vv. 1-8). Though it was a sad occasion, his other son Ishmael was sent away in order to ensure that Abraham's estate would go to his son Isaac (vv. 9-21). That action gave him some peace with his wife (vv. 9-10). Although Abraham felt personally troubled about it (v. 11), God reassured him that Ishmael and Hagar would be cared for and become prosperous (vv. 11-21). Then Abraham made a peace treaty with others in his region with whom he'd had some difficulties (vv. 22-31). So some turbulent areas in his life were now settling down. As I was reading this passage and trying to visualize what it was like, I felt almost a sigh of relief when "Abraham planted a tamarisk tree in Beersheba" (v. 33). It's almost as if he planted that tree expecting to live there for a while (v. 34: "for a long time") to enjoy its beauty and shade. So, Abraham was feeling more settled, perhaps, than he had felt in a while.
But notice what comes next in verse 33: "there he called on the name of the Lord, the Eternal God." This takes us back to Governor Christie. I said that the power of his office stayed with the office after Mr. Christie left it. But "the Lord" is "the Eternal God" (v. 33b). He never gives up the office; he can't because only he can occupy it and only he is worthy of it. He is God for eternity. The circumstances of Abraham's life were placid now but tumultuous at other points. What carried him through the tough times in his life was the knowledge that the LORD is "the eternal God." God's promises would not fail because he eternally held the power and position needed to make his promises true in reality.
Is your life in tumult? Do you feel distressed like Abraham did in verse 11? Is there a situation in your life where you have to settle for something different than what you want? Trust the Lord. He's the Eternal God. His plans often perplex us, but they never cause him distress. Every tumultuous situation we face in life is a new lesson on trusting God and being at peace with his eternal plan.


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| Mar 28, 2022
20 Years of Impact Shaping the Midwest Renewable Energy Marketplace
Kelley Welf, Communications Director
Beth Soholt has been the Executive Director of Clean Grid Alliance for 20 years
As we continue celebrating 20 years of advancing renewable energy in the Midwest, it's important to recognize that Clean Grid Alliance has been woman-led by Executive Director Beth Soholt for all of its 20 years.
During this time, and under Beth's leadership, CGA has made significant contributions to the advancement of renewable energy in the Midwest by engaging in legislative, regulatory, and MISO processes. Past CGA Board Chair Julie Voeck, Senior Director, Legislative and Regulatory Affairs, NextEra Energy Resources, stated that through Beth's leadership, she has been able to balance the interests of many organizations within the renewable industry – including owners and operators of renewables as well as non-profit organizations to advance pro-renewable energy policies. "The state and local policy work where CGA is a recognized leader has resulted in a significant addition of renewable energy being developed across the Midwest and MISO region," said Voeck. "Through its leadership, CGA has tackled many challenging issues facing the industry, including supporting the development of significant transmission to enable renewable energy to access energy markets. Transmission is a multi-faceted regional issue that requires both significant technical expertise as well as strong collaboration across a multitude of stakeholders with varying interests."
Voeck pointed to the creation of the Land & Liberty Coalition as a particularly notable development that evolved from CGA identifying a barrier to development and forming a partnership with the Conservative Energy Network. Land & Liberty Coalition is focused on local siting and permitting issues that many renewable projects have faced.
Below are a few key results and the impact of CGA's involvement:
210% growth in wind capacity in the Midwest in the last 10 years
Expanded from 700 MW of wind in 2001 to more than 28,000 megawatts of renewable energy on the MISO grid today. This represents an economic development investment of over $50 billion in the Midwest
Engaged in nearly 3,000 miles of transmission line projects, representing over $7 Billion in investment into our infrastructure and enabling over 30,000 MW of renewables to power our homes and businesses
CGA's work in state legislatures resulted in an established Renewable Portfolio Standard or goal in most every MISO state
Advocating for saving time and money, CGA's advocacy at MISO recently reduced the time needed to complete the interconnection queue process by over 25%
Streamlining regulatory processes in several states to make the siting process more efficient
Represents the Environmental Sector on MISO's Advisory Committee and Planning Advisory Committee
Leading the way to add robust amounts of new utility scale solar projects to the electric grid
In 2001, the Izaak Walton League of America (IWAL) embarked on a project to work on overcoming the two main hurdles facing utility-scale wind power development in the Midwest – bottlenecks in the power grid, and antiquated transmission rules. IWLA had been active in Minnesota Public Utilities Commission dockets regarding wind power commitments by Minnesota electric utility companies. The utilities and the regional transmission operator, Midcontinent Independent System Operator (MISO), began to raise concerns about transmission bottlenecks in getting wind power from rural southwest Minnesota to the load centers, explained Bill Grant, who was the IWLA Midwest Executive Director at the time. With that mission in mind, "Wind on the Wires" was born. The organization re-branded as "Clean Grid Alliance" in 2018 to better reflect its expanded focus on wind, solar and storage technologies. Yet, the organization's mission has remained intact for two decades, and has arguably become even more important.
Reflecting on CGA's history, current Chairman of the Board Adam Sokolski, Director, Legislative and Regulatory Affairs, EDF Renewables, recalled a trip to Southwest Minnesota's Buffalo Ridge area in the early 2000s. "The community in South Dakota really wanted wind development, but they couldn't get it and they didn't understand why. The conversation we had that day was the initial 'Wind on the Wires' discussion – some of the wind development that you want is locked in because there's no transmission to deliver it," said Sokolski.
"CGA's deep expertise on the physical energy system, broad and deep relationships, and regional presence positions it well to advance the transition we need to see to achieve the region's climate and clean energy goals," said Aimee Witteman, former Director of U.S. State Policy, Climate Imperative, and former McKnight Foundation Program Director, Midwest Climate & Energy. "CGA is an essential part of the clean energy advocacy fabric in the Midwest. Its deep knowledge, work to make clean energy a nonpartisan issue, and partnerships formed are some of the unique strengths of CGA. Its work with MISO and developers to transform the grid are essential elements of what needs to happen in the Midwest as we electrify the economy and provide clean energy for all."
CGA's leadership and engagement in the policy, regulatory, and technical processes at the state and regional level has been instrumental in driving the transition to a renewable energy economy in the Midwest. By uniting nonprofit and for-profit interests, CGA successfully crafts, then implements, clean energy policy initiatives. "The implementation piece, and our ability to build partnerships with key stakeholders and bring them to the table sets us apart from other advocacy organizations that primarily focus on setting policies," said Beth Soholt, Executive Director, Clean Grid Alliance. "We have a very knowledgeable team that works really hard to git 'er done."
"I had the pleasure of serving as Board Chair of CGA for five years and on the board for a decade," said Voeck. "During that time, CGA transitioned from a focus on wind to all forms of renewable energy, including solar and battery storage. CGA also recognized that policy decisions at the local, state, and regional level all have impacts on the ability to build renewables. They have been successful in advancing pro-renewable policy by developing coalitions and through collaboration with its diverse membership and stakeholders."
Beth Soholt – more "power behind the power"
For the past 20 years, Beth Soholt has been the most tenacious, steadfast advocate for expanding the Midwest grid to accommodate the region's renewable energy resources. Her leadership has been critical to building the political and technical support among regulatory authorities, utilities and transmission owners, and renewable energy advocates needed to get new transmission approved.
Adam Sokolski, CGA Chairman of the Board
Director, Legislative and Regulatory Affairs, EDF Renewables
"Beth's and Clean Grid Alliance's work has directly led to new transmission lines being built which have been absolutely necessary to build wind and solar in the MISO footprint," continued Sokolski. "Without Beth, the Midwest would have far fewer megawatts of renewables installed."
"Beth has been able to balance the interests of many organizations within the renewable industry – including owners and operators of renewables as well as nonprofit organizations to advance pro-renewable energy policies. The state and local policy work, where CGA is a recognized leader, has resulted in the development of thousands of megawatts of renewable energy across the Midwest and MISO region," said Voeck. "It is through Beth's leadership that CGA has become a recognized pro-renewable policy leader through vision, determination and collaboration across multiple stakeholders."
Since Beth was officially hired as Wind on the Wires Executive Director on June 3, 2002, she has been working with the electric industry in various capacities. She has received numerous awards and acknowledgments over the years.
Beth received her first Wind Energy Advocacy Award in 2006 from the American Wind Energy Association "for outstanding leadership and support of wind through effective advocacy."
In 2011, the national group Women of Wind Energy (WoWE) named her Woman of the Year.
Beth was selected by her peers as one of three NGO representatives on the Stakeholder Steering Committee of the Eastern Interconnection Planning Collaborative (EIPC).
The American Clean Power Association presented her with an "Excellence in Transmission Advocacy" award at the 2016 Windpower Conference in recognition of CGA's (WOW's) work on MISO's 17 Multi-Value Transmission Projects.
Beth received an Excellence Award in 2021 from the Energy Systems Integration Group (ESIG) for her leadership in advancing the understanding of the need for transmission for wind integration in the Upper Midwest.
Beth holds a seat on the CGA board of directors, and directs activities in the areas of technical/transmission planning, state regulatory proceedings, legislative education and outreach. She has held a seat on the Midcontinent Independent System Operator (MISO) Advisory Committee representing the Environmental Sector since 2002.
by Kelley Welf
Kelley Welf is the communications director for Clean Grid Alliance. You can reach her via email at kwelf@cleangridalliance.org. Follow CGA on Twitter @cleangridalliance.
Blog | Jun 30, 2022
Blog | Oct 13, 2021
20 Years of Big Moments: Regional Electric Transmission Planning to Support a Clean Energy Future
Blog | Aug 30, 2021
Guess Who? Profile of a CGA Employee, Member, and Board Chair


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SNMMI 2018-2020 Wagner-Torizuka Fellowship Recipients Announced
Applications available for 2019-2021 fellowships
Reston, Va. (September 20, 2018) – The Society of Nuclear Medicine and Molecular Imaging (SNMMI) is pleased to announce the recipients of the 2018-2020 SNMMI Wagner-Torizuka Fellowship. This one- or two-year fellowship, founded in 2008 by the late Henry N. Wagner, Jr., MD, and the late Kanji Torizuka, MD, PhD, is designed to provide extensive training and experience in the fields of nuclear medicine and molecular imaging for Japanese physicians in the early stages of their careers.
The program is intended to advance Fellows' research and clinical expertise, as well as facilitate professional development, and to equip them to make significant contributions to the field of nuclear medicine and molecular imaging.
The 2018-2020 fellows, each receiving an annual stipend of $24,000 (US), are:
Gensuke Akaike, MD, University of Washington Division of Nuclear Medicine, Department of Radiology, Seattle, Washington – His research focuses on SPECT/CT and PET/CT, primarily relating to oncology. Akaike is currently serving as chief resident in the nuclear medicine residency program at the University of Washington in Seattle under the supervision of Hubert Vesselle, MD, PhD.
Osamu Manabe, MD, PhD, Hokkaido University Hospital, Department of Nuclear Medicine, Sapporo, Japan – He has conducted pioneering research with several PET tracers, such as the quantification of myocardial blood flow with 15O water and 82Rb, the assessment of malignant tumors with 18F-FDG and 11C-methionine, and the evaluation of inflammatory disease with 18F-FDG. Manabe currently serves as an assistant professor at Hokkaido University Graduate School of Medicine in the Department of Nuclear Medicine under the supervision of Daniel Berman, MD.
Reiko Nakajima, MD, PhD, Memorial Sloan-Kettering Cancer Center, New York, New York – Her research interests include the association between the therapeutic efficacy of immune checkpoint inhibitors and various parameters using PET/CT, gene mutation, and patient characteristics of head and neck cancer, lung cancer, and malignant lymphoma. Nakajima is currently a visiting research fellow at Memorial Sloan-Kettering Cancer Center in the Department of Radiology and Nuclear Medicine under the supervision of Heiko Schoder, MD, MBA.
The SNMMI Wagner-Torizuka Fellowship program is sponsored by Nihon Medi-Physics Co., Ltd., in Japan.
Applications for the 2019-2021 SNMMI Wagner-Torizuka Fellowship are available online. For more information about these and other scholarships, visit www.snmmi.org/grants or contact the SNMMI Development Department at (703) 652-6780 or at developmenttemp@snmmi.org.
About the Society of Nuclear Medicine and Molecular Imaging
The Society of Nuclear Medicine and Molecular Imaging (SNMMI) is an international scientific and medical organization dedicated to advancing nuclear medicine and molecular imaging, vital elements of precision medicine that allow diagnosis and treatment to be tailored to individual patients in order to achieve the best possible outcomes.
SNMMI's more than 17,000 members set the standard for molecular imaging and nuclear medicine practice by creating guidelines, sharing information through journals and meetings and leading advocacy on key issues that affect molecular imaging and therapy research and practice. For more information, visit www.snmmi.org.
Marta Cremonesi, PhD, Selected as the 2020 Loevinger-Berman Award Recipient
New Radiotracer Offers Opportunities for Earlier Intervention after Heart Attack
Finding a Non-invasive Way to Predict Effectiveness of Cancer Therapy
Novel Theranostic Reagent Could Enhance Detection and Therapy of Prostate Cancer
New Technique Could Optimize PSMA-Targeted Prostate Cancer Therapy


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Q: Wordpress DB LOST I have a blog and currently has been lost. The company that hosts my blog had an issue with that server. And all MySQL Databases on that server has been lost (Helpfully i had a backup but it was from 2012). Never thought the server will crash and lost my data.
The good news is i've found the an archive (cached html version) of my blog on the web.archive.org
My great request is how can i get the data from there ? Does any one had that problem like me and found a solution and can share it here ?. Please it's very important to get the data back. (I know i can do a copy/paste from that site but it will take like for ever.)
Thanks for your help!

A: There is no easy answer here.
WordPress holds lots of meta data with each post, even on a default installation with no additional plugins.  All of that meta information has been lost.
You could, in theory, crawl the old web.archive.org version.  There are lots of tools to do this.  If you're using WordPress, then you're probably familiar with PHP, so something like Simple HTML DOM Parser may be useful.  You would use it like so:
// Create DOM from URL or file
$html = file_get_html('http://www.google.com/');

// Find all images
foreach($html->find('img') as $element)
       echo $element->src . '
';

// Find all links
foreach($html->find('a') as $element)
       echo $element->href . '
';

The alternative is simply to copy and paste all of the past entries manually, which is, of course, time consuming.
I would suggest that whatever method you choose you implement your own backup solution and not rely on your hosts.  There are lots of options on the WordPress plugins site or use a service such as VaultPress


The Broadcast Technology Society (BTS), the official sponsor organisation of the symposium, is one of the founding organisations of IEEE, and has a history that stretches to the formation of the Institute of Radio Engineers in 1912. The BTS mission is to serve the needs of the members of the Broadcast Technology Society to enhance their professional knowledge and vitality by keeping them informed of the latest research results and their practical applications.
Conferences are an important part of the Broadcast Technology Society, as they enable the exchange of new information and the formation of social networks. One of the major conferences is the IEEE International Symposium on Broadband Multimedia Systems and Broadcasting (BMSB) held in June of each year.
The 2018 conference will be held in Valencia, Spain from June 5th -8th.


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Sami Berdugo, an Israeli author, was born in 1970 to parents of Moroccan origin. He lost his father at the age of 13. He studied comparative literature and history at the Hebrew University of Jerusalem. At present, he teaches creative writing at Tel Aviv University and Bezalel Academy of Art and Design. He also holds writing workshops for youth. Berdugo has published novels, short stories, and novellas. His works won wide critical acclaim and are taught in schools in Israel. He was awarded numerous prizes, such as the Yaakov Shabtai Prize (2002), the Peter Schweifert Prize (2003), the Bernstein Prize (2003), the Prime Minister's Prize (2005), and the Newman Prize (2007). He lives in Tel Aviv.
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Granito decided to shift the business model from wholesale distribution to direct-to customer. Until early 2017, each 45 minutes, plating protects from corrosion. Geneva stripes are sometimes said to help rap dust away from the moving parts of the movement. fake watches The traditional heating of steel screws changes their colour to a deep royal blue while also hardening them. In any case, beveling and polishing) is of course done by hand. All wheels of the gear train are in rose gold. The single main spring provides 65 hours of autonomy.
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The hurricane is brewing. there's a religious conflict raging throughout us. As God sees the enemy lurking within the shadows, He reaches out to aid us – yet will we include Him, or will we slap His hand away?
When lightning moves your peaceable and predictable existence, how do you reply? Do you grip the hem of Jesus's garment within the face of betrayal, illness, trouble, or debt, or do you permit the enemy to rip you clear of your dating with God? The Bible is filled with tales of guys and ladies who got here lower than assault and emerged triumphant, simply because they selected God.
Your time to arrange for conflict is now. The Biblical rules in "Are You Attackable?" might help advance your dating with God, as you stand opposed to the enemy's schemes.
from God's vantage aspect. Many believers became insensitive, numb, and nearly powerless to house the occult on this planet this day. yet this isn't going to prevent demon-busting pastor Kim Daniels. In her loving but confrontational variety, she exposes the enemy's infiltration and techniques to maintain us spiritually "dumbeddown.
Within the previous testomony, King David's lifestyles was once marked through battles. David's battles have been significant—they have been fought over land and gear, and God gave him victory after victory. millions of years later, God's humans proceed to struggle battlers of a unique type. at the present time, our battles are extra major and the stakes are larger.
Worry is a debilitating strength for lots of humans. worry is available in many various varieties and will assault from many alternative angles. a few everyone is afraid to fail, afraid to be triumphant, afraid to screw up, petrified of the long run, terrified of the unknown, fearful of God, scared of a chairman or co-worker, or terrified of a mum or dad.
Search God's Grace and tool in your Marriage trip What matters do you fight with on your marriage? Do you discover it tricky to teach love in the event you suppose your wishes will not be being met? have you ever hung on to resentment for therefore lengthy that it kind of feels most unlikely to forgive? Do you want God's blessing and additional encouragement for the not easy days?


Hi-Lok is a registered trademark of the Hi-Shear Corporation. Hi-Lok pins are commonly used in applications that require high tensile strength in extreme environments. Hi-Loks pins and Hi-Lok collars offer extremely precise dimensions making Hi-Lok fasteners commonly used in space, military, and commercial aviation application. Hi-Lok pins and Hi-Lok collars are both threaded and require common installation tools making Hi-Lok Fasteners easy to install and remove.
Hi-Lok is a simple two-part fastener engineered to achieve in one all-purpose system the design features suiting many of today's aerospace assembly needs. Consistent torque on each fastener installed is achieved through the integrated functions of the system working together. A carefully regulated breakoff groove in the self-locking Hi-Lok collar provides uniform preload values by separating when the correct torque level is reached. This controlled preload of each Hi-Lok® in the structure improves the fatigue life of the airframe significantly when compared to other fastening systems, including swaged collar type. The Hi-Lok® pin is held stationary by the installation tool while the collar rotates. Progressive tightening takes place as torque is applied. At the designed torque level built into the Hi-Lok® collar, the hex portion of the collar is sheared off automatically by the driving tool.
Hi-Lok® cannot be over-torqued; the collar's automatic breakoff design assures this and eliminates the need for torque inspection. As a highly efficient and dependable system.
As a versatile fastener, Hi-Lok® matches the best qualities of a bolt/nut or pin swaged collar combination. Tooling is easily adaptable to large scale production with high speed equipment and automatic collar feed attachments that handle up to 200 collars, affording installation rates of up to 45 fasteners per minute in some cases. The compactness of the Hi-Lok® tooling is in a class by itself when installation means reaching into hidden areas and next-to-impossible places. An extensive range of installation tools satisfies standard, offset and extended offset, 200, 900 and 1800 requirements. The Hi-Lok® design does more with less, solving weighty problems and delivering high fatigue resistance without sacrificing strength. The lightweight Hi-Lok® collar further contributes to weight-saving when compared to conventional nut and bolt systems of equal strength characteristics. Manufactured in a wide range of sizes and material combinations, in terms of versatility the Hi-Lok® system offers engineering designers a ready solution to a variety of assembly problems.
Hi-Lok Pins are manufactured to the requirements of Hi-Shear Specification 342. Installation guidelines are contained in the Hi-Lok Installation Manual.
Notes: * Oversize collars may be used with lower size shank pins.
** indicates forged-type collar configuration.
Hi-Lok collars are manufactured to the requirements of Hi-Shear Specification 345.


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Sheriff's Office: Amish buggy struck by deputy met all state requirements
by: Corey Morris
Posted: Nov 1, 2022 / 10:56 AM EDT
Updated: Nov 1, 2022 / 10:56 AM EDT
(WJET/WFXP/YourErie.com) — The Chautauqua County Sheriff's Office has announced details about an recent incident when a deputy crashed a patrol car into the back of an Amish Buggy.
The accident happened at about 9 p.m. on Oct. 30 on Stockton-Hartfield Road in Chautauqua, New York. The deputy was driving when he struck the rear of the Amish buggy. The road had no lighting and he was in a 55 mph zone.
NY sheriff's deputy crashes into Amish buggy
The buggy suffered heavy damage. The horse had to be destroyed due to injuries.
Five people were riding in the buggy. They were transported to Jamestown UPMC for injuries. According to a Chautauqua County Sheriff's report, several fire departments and the county medic unit were dispatched to the scene.
The deputy was not injured.
In a follow-up report from the Chautauqua County Sheriff's Office, the five buggy passengers were identified as a 50-year-old woman, a 25-year-old man, a 25-year-old female, a 3-year-old boy, and a 1-year-old. All five had been released from the hospital and were recovering from their injuries at home, according to the report.
The deputy also was identified as Dylan Pratt.
The report noted that the buggy met all state requirements for a slow-moving vehicle drawn by an animal. It had a slow-moving vehicle emblem on the rear and two lit lanterns with red lenses near the edge of the buggy. It also had the required reflective tape.
The report noted that the investigation is ongoing and said additional information would be released.


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Home | U.S. News
NSA Withholding Intelligence From 'Untrustworthy' Trump Administration, Former Analyst Claims
John Schindler claims NSA fears Trump administration cannot be trusted with sensitive information. 'Since January 20, we've assumed that the Kremlin has ears inside the SITROOM,' he cites Pentagon official as saying.
President Donald Trump and National Security Adviser Michael Flynn at MacDill Air Force Base in Tampa, Fla., Monday, Feb. 6, 2017Credit: Susan Walsh/AP
The National Security Agency has been withholding information from the White House, fearing that President Donald Trump and his staff cannot be trusted not to leak sensitive information, a former NSA analyst claims.
'Kompromat:' The storied and sordid history of Russian blackmail
U.S. intelligence officials reportedly warn Israeli counterparts against sharing info with Trump administration
U.S. investigators reportedly corroborate part of Trump dossier
In a column written by John R. Schindler for The Observer, the security expert and former professor at the U.S. Naval War College claims that the NSA has stopped its decades-old practice of preparing special reports for U.S. presidents since Trump took office.
Schindler added that the NSA's concerns were shared across the American intelligence community, and it appears that other agencies are withholding intelligence from the White House as well.
According to Schindler, the intelligence community's fears were prompted by the ties of senior members of the Trump administration to the Kremlin, as well as "nagging questions about basic competence regarding Team Trump."
"Since January 20, we've assumed that the Kremlin has ears inside the SITROOM," Schindler cites a senior Pentagon official as saying, meaning the White House Situation Room where the president is briefed on intelligence matters.
Schindler's claims echo a January report on Yedioth Ahronoth by Israeli journalist Ronen Bergman, which said that Israeli intelligence officials are concerned that the exposure of classified information to their American counterparts under a Trump administration could lead to their being leaked to Russia and onward to Iran.
According to Bergman, the American intelligence officials implied that Israel should "be careful" when transferring intelligence information to the White House and the National Security Council (NSC) following Trump's inauguration – at least until it is clear that Trump does not have inappropriate connections with Russia.