A candidate for state auditor calls for regular performance audits and better funding.
Kathy McGuiness is a Rehoboth Beach commissioner and a Democratic candidate for state auditor.
Delaware taxpayers want an independent, professional and effective auditor.
This is what I have heard from Delawareans up and down the state during the past few months.
It makes sense because our citizens pay attention to what happens in Delaware. They know that the actual job of auditor is about serving the citizens of Delaware, not about political parties or labels.
They care deeply about how their tax dollars are spent on state services and want to ensure that there is no waste, abuse or fraud taking place.
Recently, I spoke with auditing professionals, inside and outside Delaware, for suggestions, new ideas, and approaches that can be introduced here so we can be the best in the country.
The State Auditor's Office needs to be a leader in innovation. The Office must reflect a broad strategy focused on taxpayer value. This means greater use of technology and greater development of how audits help the overall wealth of the State and the individual entities in it. I want to see us undertake more performance audits.
The State Auditor's Office must be transparent. Its audits and accounting practices must be clear and understandable to those subject to state audits, and to citizens. Entities within Delaware have different levels of understanding and skill in complying with State and Federal requirements. The State Auditor must ensure that all levels of government and entities that receive government funds understand what it means to be a guardian of the funds of the citizens of Delaware.
The State Auditor must be agile in planning its review. To get the coverage we need to safeguard taxpayer resources, the State Auditor must be engaged in streamlined audit execution wherever possible.
The State Auditor's Office must recognize potential challenges. We must be aware of changes in auditing techniques and approaches. In performing our audit tasks, we must be aware of the need to protect privacy and personal data. We must determine how, why and for how long an audit needs to examine, if at all, personally identifiable information.
At the same time as we need to increase the use of technology and develop more efficient ways of doing that which the law directs us to do as auditors. We must capitalize on existing work and take advantage of existing audits projects and skills.
The Auditor's Office is more than just numbers. With the right approach, we have a tremendous opportunity to make the Auditor's Office relevant for all Delaware taxpayers.
It's my honor to be on the ballot this November. I look forward to being the next — and first female in Delaware history — State Auditor of Accounts.


, Rental On Union St Brooklyn Conception – 7 Pricey Automobile Rental Mistakes to Avoid – AS AMERICANS hit the road this summer time, many will drive rental automobiles in different components of the nation or the world. While rental vehicles can be handy, the related costs are sometimes confusing. Here's a look at automobile rental errors that could cost you money – and learn how to keep away from them.
Then again, if you do not have your individual auto policy or you're concerned about potential premium increases should you'll want to file a declare along with your auto policy, the automotive rental firm's insurance might make sense.
3. Not buying round – Automotive rental rates can range depending on the company or the amount of lead time, so it pays to buy around instead of taking a "one-and-done" strategy. Websites equivalent to CarRentalSavers.com and AutoSlash.com help you comparison store between rental corporations and look for coupons. AutoSlash will even track your rental charges and rebook for you if the speed drops.
In the event you're planning to drive long distances, test for mileage caps. "Many rental firms supply limitless miles for the car rental period, permitting you to drive the automotive as a lot as you need with out going through additional fees," says Angie Hicks, founding father of AngiesList.com. "But others might assess additional charges for surpassing a each day mileage maximum. If you hire a car, particularly for a period quite a lot of days, make sure you have unlimited miles or enough miles to cover your travels." When choosing between a rental with unlimited miles and a less expensive rental with a mileage cap, you could come out ahead with the former.
4. Prepaying for gasoline – Prepaying for fuel may seem convenient (who needs to plan additional time for a pit cease on the best way to an early morning flight?) nevertheless it means you'll pay for a full tank of gas, even in the event you return with the tank half full. "It's higher to fill up yourself since you'll be able to normally discover cheaper gas costs at a close-by station anyway," says shopper and money-saving skilled Andrea Woroch. "But don't neglect to fill it up as a result of the price to take action after drop-off is usually a total rip-off." Make sure you top off the gasoline, as a result of some firms will charge you even when the gasoline gauge is just a hair away from the place it must be.
5. Paying further for GPS or a automotive seat – Car rental companies are glad to charge you extra for equipment like a GPS or child car seat. However as Woroch points out, a GPS can cost an additional $10 per day or extra. "Use your smartphone when doable, or print instructions using your lodge's free enterprise heart," she says. You probably have a portable GPS you may pack in your suitcase and use in your trip, keep in mind to remove it from the rental automotive in your return.
In line with Sarah Schlichter, senior editor of IndependentTraveler.com, many airways will permit you to examine a automobile seat or use it on the airplane totally free, so you don't need to pay extra to make use of one from your rental automobile firm.
6. Dashing via the inspection – Totally inspect your rental automobile before you drive away. In any other case, you could be charged for harm you didn't trigger. "Most rental car fleets are maintained meticulously, however damages like scratches or dents within the body or spills, stains or tears in the interior can go unnoticed," Hicks says. "For those who see any wear, damage or defect during the inspection, be sure you instantly make the company aware – otherwise you would possibly end up paying for it." By no means assume that a ding is simply too small to warrant noting or that the car company already is aware of about damage. If it's not listed on the automotive condition type, communicate up.
7. Returning a car late. Most automotive rental corporations charge every day rates based mostly on 24-hour intervals. "While some could give a 29-minute grace interval, you could be charged late fees – or for a full further day – should you return the automotive past that time window," Schlichter says. Allow loads of time on the day you are returning your automobile to keep away from this further price.
6 automotive rental tips that may prevent money and frustration – Renting a car might be expensive, but it surely's usually a essential a part of a trip. Like airfare or hotel rates, automobile rental rates will be comparatively opaque, and it may be arduous to determine rules like timing and tricks to economize.
Whereas figuring out and predicting automobile rental charges may be troublesome, there are nonetheless a few easy ways to save money without having to make main adjustments to your journey plans.
1. Always compare rental businesses — together with some less widespread ones.
Just about everybody knows the massive brands — Hertz, Avis, Enterprise, and so on — but there are a number of much less apparent brands which will offer better rates. Budget, Sixt, Thrifty, and Fox are only a few of the out there ones. To cover all of your bases, you possibly can ebook by means of a web based travel agency website — like Hotwire or Priceline — to match a number of different leases.
Hotwire offers steep discounts through "opaque booking," a follow the place you make and prepay a reserving with out knowing exactly which agency you are booking with — it can still be a major agency, though.
Whereas it may sound risky, it's really perfectly advantageous — you will know exactly how a lot you're paying, where you'll be selecting up and dropping off, what class of car it is (and generally the particular model), and any phrases. Unless you are useless set on a sure company, it is a great solution to save a fortune.
Chances are high very good that your house auto insurance coverage coverage covers rentals that you simply drive. Whereas the rental agent may try to strain you into buying further coverage, that is typically unnecessary and redundant to your present coverage. Simply make sure that to verify your coverage earlier than assuming that you simply're coated.
If you don't own a automobile, or if your home coverage would not cover rentals, you may still have protection.
Plenty of standard credit cards, including the Chase Sapphire Preferred and the Sapphire Reserve, include free main auto rental insurance. "Main" signifies that it kicks in before another policy that you have. When you get into an accident and have main coverage separate from your private home policy, which means the accident will not need to be reported to your personal insurance coverage, so you will not see a charge spike.
In an effort to activate the insurance coverage that comes with a bank card, you may have to use that card to pay for the rental, and decline the overall rental insurance coverage, additionally known as a "collision harm waiver (CDW)" or "loss harm waiver (LDW)" provided by the rental agency. If you do not have your individual automotive insurance coverage, you may still need to contemplate including liability insurance coverage.
This is not a hard-and-fast rule, but normally, rental rates at airports are more expensive than charges a bit of bit additional away. Strive in search of rates from pick-up spots closer to your lodge, or even within the city heart.
Be sure that to at all times compare these to rates from airport agencies, though — typically, the price distinction will be negligible, or the airport may even be cheaper. Additionally keep in mind that you'll want to arrange transportation to the rental company, whether or not you'll be able to take a hotel shuttle, or it's a must to pay for mass transit or a taxi into town.
GPS navigation. Satellite radio. Speaker phone. Car rental businesses might supply these options whenever you pick up your automobile, but beware — they all come with extra charges that can add up quickly. These days, there is no must pay additional when you could have a smartphone that can do all of that and extra.
6. Verify weekly charges — even if you only want the automotive for just a few days.
It could appear paradoxical, however it may be cheaper to hire a automotive for longer.That is as a result of the majority of people that rent a automotive for just a couple of days at a time are business vacationers, who're much less cost-conscious as a result of their offices are paying or the journey is last minute and urgent. Conversely, many week-long renters try to save, since they tend to be leisure travelers. Due to that, the weekly charge is often cheaper than the rate for simply three or four days.
Related Post "12 Car Rental Rexburg , Rental On Union St Brooklyn Conception"


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Paws to the Park – December 7th 2019
Young Achiever: Skye Art for SPCA
An artist became one of the most generous young donors to the Society for the Prevention of Cruelty to Animals after she raised more than $2,700 at her gallery. Skye Backeberg, 11, said that it felt rewarding to know how well the Paint for Paws art exhibition was received. The Somersfield Academy pupil said: "It […]
SPCA Offering Workshops With Feline Experts
The Bermuda SPCA will be welcoming feline experts Vicky Halls and Kim Horsford from International Cat Care. The organisation said, "The Bermuda SPCA and associated stakeholders are being given the unique opportunity to find out about the Cat Friendly way of working, with five days of intensive workshops and exercises to see how making some […]
Workshops to Teach 'Cat-Friendly Homing'
Workshops aimed at bettering the lot of Bermuda's feral cats will start today, courtesy of an international charity dedicated to feline care. The island's cat population outnumbers available homes, according to the Society for the Prevention of Cruelty to Animals. The five days of education sessions combine Vicky Halls, a bestselling author and expert on […]
SPCA Hits Out at Cruelty as Dogs Starved to Death
Dogs are being left to starve to death on the end of chains, the SPCA has warned. The charity told the Bermuda Sun communities are turning a blind eye to the blatant suffering of animals. The SPCA said they have witnessed a "significant rise" in the number of emaciated and malnourished dogs being taken into […]
Spicelands Horses Flown Out to Start New Lives Overseas
The last three horses left homeless by the closure of a riding school were flown last night to a new future overseas. The animals were transported free of charge by EquiJet, a specialist in horse transportation by air, who worked closely with the Bermuda Society for the Prevention of Cruelty to Animals. The SPCA took […]
Rescued Horses Euthanised
Two neglected horses seized by an animal welfare charity last year have been put down on the advice of a vet. The Society for the Prevention of Cruelty to Animals PCA said it made the "humane decision" to put down former carriage horses Charlie and Arthur last week after years of neglect left them with […]
'Humane Decision To Euthanize Charlie & Arthur'
"It is with great sadness that, under veterinarian advice, the humane decision was made to euthanize Charlie and Arthur," the SPCA said, with the organisation explaining that "years of neglect and infection had left them both with severe dental issues" and the time had come. Arthur and Charlie had previously been carriage horses and were […]
Homeless Horses Need New Owners
Horses are looking for a new home after a riding school went into liquidation. The 12 animals, from the now-closed Spicelands Riding School, were turned over to the SPCA which has launched a bid to find them new owners. A spokeswoman for the animal charity said: "The SPCA has been busy securing homes for these […]
Man Banned from Owning Animals
The owner of two neglected horses will not face criminal charges, but will never own animals again. Calix Darrell, who was banned from owning animals for five years in 2006 after admitting cruelty charges, has signed a "legally binding agreement" with animal protection agency the Society for the Prevention of Cruelty to Animals to stop […]
SPCA Rescues Malnourished Carriage Horses
Tougher ownership rules would help make sure the island's horses and ponies are properly cared for, the Bermuda Society for the Prevention of Cruelty to Animals said yesterday. Sarah Haycock, president of the SPCA, renewed the charity's call for a register that would require owners to license their horses and ponies and provide proof of […]
Two Former Carriage Horses Rescued By SPCA
The Bermuda Society for the Prevention of Cruelty to Animals [SPCA] has rescued two former carriage horses and is seeking to raise funds for their retirement. The two horses, known as Arthur and Charlie, were found in very poor condition following an anonymous tip from a member of the public. They had previously been carriage […]
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It is with profound sadness that the SPCA has rece
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text:
\section{Introduction}\label{sect:intro}
MN Hya was detected as the optical counterpart of the X-ray source RX J0929.1-2404 and identified as a polar due to the spectral characteristics \citep{Sekiguchi1994RXJ}. As one of the subtypes of cataclysmic variables (CVs), polars are interacting binaries in which mass transfers from a dwarf secondary star to the primary, a magnetic ($\sim10-200MG$) white dwarf (WD), through Roche lobe overflow. The magnetic field is sufficiently high to prevent the formation of an accretion disc and channels the accretion stream at threading point, then guides the flow plunging into the white dwarf directly around the magnetic pole \citep{Hellier2001Cataclysmic}. If only one accretion region is visible, we call the behavior as one-pole behavior. In contrast to two-pole behavior, two accretion regions appear alternatively. Because of the variation of mass transfer rate, polars switch irregularly between high state and low state. In high state, polars present fast light intensity variation which is known as flickering. Later, several observations of MN Hya, including photometry, spectrometry, X-ray, and polarimetry, let some authors classify it as a two-pole system. The primary accretion pole, below the orbital plane, appears between phase $\sim0.5-1$ and causes the intensity peak near phase 0.7 while the secondary accretion pole contributes its emission all the way \citep{Buckley1998Polarimetry}. Also in X-rays, MN Hya shows a prominent pre-eclipse dip around phase 0.9, but it is not detected in the optical passband with the same depth and phase interval \citep{Buckley1998Xray}. Moreover, MN Hya is an eclipsing system with a high orbital inclination of $\sim75^{\circ}$ \citep{Buckley1998Polarimetry}. The eclipsing nature provides a good opportunity to ascertain its geometric structure and evolutionary state, and also to search for circumbinary planets. Since 2009 our group started to detect the secular evolution of CVs and the extrasolar planets around them by the eclipse timing method (e.g. \citealt{Qian2009Orbital,Qian2010DETECTION,Qian2011Detection,Qian2015Long,Qian2016Rapid}; \citealt{Dai2009Evidence,Dai2010Orbital}; \citealt{Han2015An,Han2016Physical,Han2017Cyclic,Han2017Double,Han2017WZ}).

   In this paper we analysis the photometric observations of MN Hya. We give a revised ephemeris and find that the orbital period decreased during the state change. The light curve (LC) of low state presents one hump near phase 0.2 and those of high state show obvious flickering. The paper is organized in the following way. In Sect.~\ref{sect:observ} the observation of the datasets is described. And a detail analysis is given in Sect.~\ref{sect:analysis}. Our main results are summarized in Sect.~\ref{sect:summary}.

\section{Observations}\label{sect:observ}
MN Hya was observed since 27, November 2009 by the Roper Scientific, Versarray 1300B camera with a thinned EEV CCD36-40 de 1340 $\times$ 1300 pixel CCD chip, attached to the 2.15-m "Jorge Sahade" telescope (JST) at Complejo Astron\'omico E1 Leoncito (CASLEO), San Juan, Argentina. Later, this binary was monitored during 2012-2016 by using the Danish 1.54-m Telescope at ESO La Silla, Chile. MN Hya was detected photometrically for 12 times with no filter used mostly, apart from one observation through V filter in 17, January 2016. The CCD images were reduced with the help of the aperture photometry package of IRAF \citep{Tody1993IRAF}. Nearby non-variable stars were chosen as comparison star and check star (the stars marked C and B respectively in figure 2 of \cite{Sekiguchi1994RXJ}), so two sets of different magnitudes of each observation, i.e. the magnitudes of the object and the companion star with respect to that of companion star and check star respectively, were obtained and used for the analysis of the characteristics of the light curve of the object.
An overview of the observation of MN Hya is given in Table~\ref{tab1}. The table lists the information about an observation ID used in this paper, the data of the observation, the state of the object, the time resolution, the telescope and the filter used, and the total phase coverage.
Fig. \ref{Fig.V_K} displays all LCs obtained in 2009-2016. It is lucky of us to detect the process of the state change which gives us enough information to know the characteristics of this phase.

\begin{figure}
   \centering
   \includegraphics[width=14.0cm, angle=0]{V-K_fig1}
   \caption{All light curves detected during 2009-2016. The ordinate is the differential magnitude of the target star with respect to the comparison star. The labels indicate the observation IDs used in this paper. More information is given in Table \ref{tab1}.}
   \label{Fig.V_K}
   \end{figure}

\begin{table}[!ht]
\bc
\begin{minipage}[]{100mm}
\caption[]{Log of photometric observation of MN Hya. The meaning of the entries are given in context.\label{tab1}}\end{minipage}
\setlength{\tabcolsep}{5pt}
\small
\begin{threeparttable}
\begin{tabular}{ccccccc}
  \hline\noalign{\smallskip}
Obs-ID & Date & accretion state & resolution(s) & Telescopes & Filter & Phase Coverage\tnote{a}\\
  \hline\noalign{\smallskip}
Run0&20091127&intermediate&23&2.15m&N&0.72-1.31\\
Run1&20091128&intermediate&23&2.15m&N&0.84-1.35\\
Run2&20100115&intermediate&28&2.15m&N&0.77-1.31\\
Run3&20101227&intermediate&40&2.15m&N&0.85-1.15\\
Run4&20101230&intermediate&40&2.15m&N&0.84-1.09\\
Run5&20121225&high        &16&1.54m&N&0.82-1.82\\
Run6&20130406&high        &16&1.54m&N&0.18-1.43\\
Run7&20131223&high        &14&1.54m&N&0.89-1.08\\
Run8&20150129&high        &16&1.54m&N&0.69-1.43\\
Run9&20160101&high        &21&1.54m&N&0.03-1.08\\
Run10&20160117&high       &22&1.54m&V&0.17-1.38\\
Run11&20160310&low        &17&1.54m&N&0.89-1.95\\
  \noalign{\smallskip}\hline
\end{tabular}
      \begin{tablenotes}
        \footnotesize
        \item[a] Phase is calculated according to the ephemeris of equation (\ref{Eq.1}).
      \end{tablenotes}
\end{threeparttable}
\ec
\end{table}

\section{Analysis} \label{sect:analysis}
 \subsection{Period Change} \label{subsect:period}
    From our photometric observation, 10 mid-eclipse times, the average of eclipse ingress and egress, were obtained, and a linear least-squares fit to the timings gives the following eclipsing ephemeris:
    \begin{equation}
    \label{Eq.1}
    HJD_{min}=2457458.62831(4) + 0.1412437990(31)E
    \end{equation}
    Fig.~\ref{Fig.O-C} shows the residual (O-C, observed minus calculated) times of the linear fit. The O-C curve indicates that the orbital period decreased during the state change. Because the mid-eclipse time is that of the occultation of the primary by the secondary \citep{Schmidt2001HSTSpectroscopy} which can not be effected by the shift of the accretion spot due to the variation of accretion rate, the O-C curve of the system will give the information of orbital evolution. The new data has higher precision, it makes the possibility of analysis the orbital variation. The period decreased as $-2.4\times10^{-12}dcyc^{-1}$ with the error of $0.7\times10^{-12}dcyc^{-1}$. In the angular momentum conservation case the orbital period increases when mass transfers from the less massive secondary to the more massive primary WD star, which makes the O-C curve as a parabola with a positive quadratic term. So we infer that the mass transfers from the secondary to the primary accompanied by intense mass loss which carries angular momentum from the system and decreases the orbital period.

    In oder to estimate the mass loss fraction from the system during the high state, we need to know the accretion luminosity. The period ($P\approx3.39h$) implies that the secondary has mass $M_{2}=0.22M_{\odot}$  and radius  $R_{2}=0.32R_{\odot}$ (\citealt{Knigge2010Erratum}).  Considering of the inclination of system $i=75^{\circ}$ and the phase width of eclipse about 0.036,  we deduce the mass ratio ($q=M_{2}/M_{1}$) as about 0.38 \citep{Horne1985Images} which gives the primary with mass $M_{1}=0.58M_{\odot}$ and radius $R_{1}=0.88\times10^{9}cm$ \citep{Nauenberg1972Analytic}. The $0.1-2.4$k$eV$ luminosity is about $9\times10^{32} erg s^{-1}$ \citep{Ramsay1998Spectroscopic}, with the addition of the soft X-ray excess ($\frac{L_{bb}}{L_{brems}+L_{cycs}}$) $\sim$ 10 \citep{Buckley1998Xray} and assuming $L_{brems}=L_{cycs}$, we derive that the luminosity of accretion is about $L_{acc}=2\times10^{34} erg s^{-1}$ which gives the mass accretion rate of $\dot{M_{1}}=3.6\times10^{-9}M_{\odot}yr^{-1}$.
    Combine
   \begin{equation}\label{Eq.2}
    \frac{\dot{J}}{J}=\frac{\dot{M}_{1}}{M_{1}}+\frac{\dot{M}_{2}}{M_{2}}-\frac{1}{2}\frac{\dot{M}}{M}+\frac{1}{2}\frac{\dot{a}}{a},
   \end{equation}
with Kepler's law and assuming mass loss rate $\dot{M}=\alpha\dot{M_{2}}$, we can write
   \begin{equation}\label{Eq.3}
    \frac{\dot{J}}{J}=\left(1+\frac{1}{q(\alpha-1)}-\frac{1}{3}\frac{\alpha}{(1+q)(\alpha-1)}\right)\frac{\dot{M}_{1}}{M_{1}}+\frac{1}{3}\frac{\dot{P}}{P},
   \end{equation}
    where $M=M_{1}+M_{2}$ is the mass of the system and $J=M_{1}M_{2}~\sqrt[]{Ga/M}$ is the angular momentum of system.
    $\dot{J}/J$ term consists of the angular momentum loss due to mass lost from system and redistribution of mass between two components. The first factor (denoted as loss-term) can be expressed by
  \begin{equation}\label{Eq.4}
    \left(\frac{\dot{J}}{J}\right)_{loss}=\frac{1+q}{q}\frac{\alpha}{\alpha-1}\frac{\dot{M_{1}}}{M_{1}}\left(\frac{r_{de}}{a}\right)^{2},
  \end{equation}
in terms of the effective decoupling position $r_{de}$:
   \begin{equation}\label{Eq.5}
     \left(\frac{r_{de}}{a}\right)^{2}=\left(\frac{r_{1}}{a}\right)^{2}+\left(\frac{r_{2}}{a}\right)^{2}+2\frac{r_{1}}{a}\frac{r_{2}}{a}cos\Delta\theta,
   \end{equation}
where $r_{1}$ is the line length from one of components to the mass center of system (COM), $r_{2}$ is that from the decoupling point to this component, and $\Delta\theta$ is the angel between the two lines assuming 0 degree corresponding to the decoupling point in the opposite direction to COM. And the second (denoted as syn- term) can be calculated using
  \begin{equation}\label{Eq.6}
   \left(\frac{\dot{J}}{J}\right)_{syn}=\frac{2\pi\dot{M_{1}}a^{2}}{JP}\left[\left(\frac{l_{1}}{a}\right)^{2}-\left(\frac{q}{1+q}\right)^{2}\right]=\frac{1+q}{q}\frac{\dot{M_{1}}}{M_{1}}\left[\left(\frac{l_{1}}{a}\right)^{2}-\left(\frac{q}{1+q}\right)^{2}\right],
  \end{equation}
  with
    \begin{equation}\label{Eq.7}
      l_{1}=a(0.5-0.227logq)-\frac{qa}{1+q},
    \end{equation}
giving the distance of the Lagrangian radius ($R_{L1}$, \citealt{Plavec1964Tables}) to COM.

    Substituting the parameters into the equations above deduces
    \begin{equation}\label{Eq.8}
      \left(\frac{r_{de}}{a}\right)^{2}\sim\frac{1.12}{\alpha}-0.46.
    \end{equation}
    The constraint $\alpha<1$ gives $r_{de}/a>0.81$ which implies the mass lost from the secondary. Note that the shortest length scale of the decoupling point to the COM only depends on the mass ratio, i.e., it is independent of the variation of period, mass accretion rate or other physical parameters. The maximal length scale of system about $1.2a$, corresponding to the distance of Lagrangian point L2 to COM, shows the minimal mass loss fraction $\alpha$ as about $60\%$, which reveals that the mass transfer rate from the secondary is about $6\times10^{-9}M_{\odot}yr^{-1}$ at least.
    The Alf\'ven radius, considering the equivalence of ram pressure of flow and the magnetic pressure of field, is given by \citep{Frank2002Accretion}
      \begin{equation}\label{Eq.9}
          r_{A}= 2.9 \times 10^{8} M_{1}^{-1/7} R_{6}^{10/7} L_{37}^{-2/7} B_{12}^{4/7},
       \end{equation}
from which we can estimate Alf\'ven radius $r_{A}$ is about $1.02a$. The magnetosphere centered the primary can cover about 42\% surface area of the secondary, which can cause the mass loss fraction of about $58\%$ if the secondary ejects matter symmetrically, such as the global intense wind. This kind of activity can produces mass loss fraction of about 58\% that is very close to the mass loss fraction $\alpha\sim60\%$ if mass is lost through the $L_{2}$. Whatever, we can see that the mass loss fraction is very large and any model not taking mass loss into account should be unreality.

\begin{table}[!ht]
\bc
  \begin{minipage}[]{100mm}
      \caption[]{All mid-eclipse times of MN Hya
      \label{tab2}}
  \end{minipage}
\setlength{\tabcolsep}{5pt}
\small
\begin{threeparttable}
 \begin{tabular}{cccccc}
  \hline\noalign{\smallskip}
Min.(HJD) & Cycle & Error (days) & Calculated & O-C (days) & Ref.\tnote{*}\\
  \hline\noalign{\smallskip}
2449007.58900&0    &0.001  &2449007.58808&0.00092 &(1)\\
2449009.42400&13   &0.001  &2449009.42425&-0.00025&(1)\\
2449009.56600&14   &0.001  &2449009.56549&0.00051 &(1)\\
2449010.55400&21   &0.001  &2449010.55420&-0.00020&(1)\\
2449013.52100&42   &0.001  &2449013.52032&0.00068 &(1)\\
2449397.42100&2760 &0.0005 &2449397.42097&0.00003 &(1)\\
2449397.56150&2761 &0.0002 &2449397.56221&-0.00071&(1)\\
2449398.55030&2768 &0.0002 &2449398.55092&-0.00062&(1)\\
2450045.02352&7345 &0.0010 &2450045.02378&-0.00026&(1)\\
2450109.85462&7804 &0.0002 &2450109.85469&-0.00007&(1)\\
2455163.41637&43583&0.0001 &2455163.41657&-0.00021&(2)\\
2455164.40509&43590&0.0001 &2455164.40528&-0.00019&(2)\\
2455212.28680&43929&0.0002 &2455212.28693&-0.00013&(2)\\
2455558.33420&46379&0.0002 &2455558.33424&-0.00003&(2)\\
2455561.30033&46400&0.0002 &2455561.30036&-0.00002&(2)\\
2456287.71730&51543&0.0001 &2456287.71721&0.00008 &(2)\\
2456389.69530&52265&0.0001 &2456389.69524&0.00006 &(2)\\
2456650.85510&54114&0.0001 &2456650.85502&0.00008 &(2)\\
2457052.83505&56960&0.0001 &2457052.83487&0.00017 &(2)\\
2457458.62847&59833&0.0001 &2457458.62831&0.00016 &(2)\\
  \noalign{\smallskip}\hline
\end{tabular}
      \begin{tablenotes}
        \footnotesize
        \item[*] References: (1) \cite{Sekiguchi1994RXJ}; (2) Our observations.
      \end{tablenotes}
\end{threeparttable}
\ec
\end{table}

\begin{figure}
   \centering
   \includegraphics[width=14.0cm, angle=0]{O-C_fig2}
   \caption{The residuals of the linear fit to the mid-eclipse times with the reference line for convenience. The new data overlaid by fitted parabola  shows period decrease.}
   \label{Fig.O-C}
   \end{figure}

 \subsection{The characteristic of light curve}\label{subsect:characteristic}
 Now we describe the characteristics of the LCs more carefully and analysis the reasons for corresponding variation. And the analysis of the rapid light intensity is given in Subsection~\ref{subsect:flickering}.\\

    (a) Fig.~\ref{Fig.high_state} shows the details of high-state LCs. Some LCs show the conspicuous pre-eclipse light decrease, such as near phase 0.85 in Run6 and phase 0.89 in Run9. It is reminiscence of the X-ray pre-eclipse dip but with less phase extension. Also the eclipse profile variates significantly, especially that of Run8. The intensity during the eclipse of Run8, after a possibly flat base ahead of the slow decrease, rises slowly up, which indicates that some part of the accretion flow became brighter and system had higher mass transfer rate. The smoothed increase and decrease of light during eclipse mean that the fast light intensity variation is not due to the accretion flow. All of these changes presented in LCs reflect a significant variation of the mass accretion rate during high state.\\

   \begin{figure}
   \centering
  \includegraphics[width=14.0cm, angle=0]{high_state_fig3}
   \caption{A detailed drawing of high-state LCs. The arrows point the position of per-eclipse light decrease.}
   \label{Fig.high_state}
   \end{figure}

    (b) In Fig.~\ref{Fig.V-K_shift}, all data were shifted by the average magnitude between phase 0.07-0.09. Refer to Fig.~\ref{Fig.V_K}, we can find most high-state LCs follow the LC of Run11 very well during phase $\sim0-\sim0.4$, except those of Run5 and Run6. The reason of their deviation, we think, is due to instability of the system at the beginning of high state, such as Run2 which gives the light intensity variation of system at start of leaving low state. The large phase interval $\phi_{f}\sim0.4$ suggests that the only reasonable source giving rise to the hump near phase 0.2 is the WD itself. So from the shifting value of LCs, we can deduce the optical temperature relation of WD between low and high state. Assuming black body radiation and using the magnitude formula, we can get
         \begin{equation}\label{Eq.10}
            m_{H}-m_{L}=-2.5log\frac{f_{H}}{f_{L}}=-2.5log(\frac{S_{H}\bar{T}_{H}^{4}}{S_{L}\bar{T}_{L}^{4}}),
         \end{equation}
where $m,S,\bar{T}$ is respectively the magnitude, projected surface area and mean temperature of the system, and L, H denote low and high state respectively. Considering, during phase 0-0.4, the dominating optical radiation of the WD and the spherical symmetry of that, the projected surface area is constant at certain phase, then we find
         \begin{equation}\label{Eq.11}
            m_{H}=m_{L}-10log(\frac{\bar{T}_{H}}{\bar{T}_{L}})=m_{L}+\Delta Mag,
         \end{equation}
where $\Delta Mag$ is the amount of translation for high-state LCs to overlap that of Run11. With $\Delta Mag=-2.21$, we find $\bar{T}_{2}\approx1.66\bar{T}_{1}$. If the temperature of the WD in low state is about 9000K \citep{Ramsay2004XMM}, we deduce the optical temperature of the WD in high state as about 15000K. Also as shown in the inserted graph of Fig.~\ref{Fig.V-K_shift}, the LCs of high state wander off that of Run11 near phase 0.4 since which the cyclotron features visible \citep{Ramsay1998Spectroscopic} and the accretion region shows up. Both the large $\phi_{f}$ during phase 0-0.4 and the visible cyclotron features during phase 0.4-1 suggest that it is an one-pole system.\\

\begin{figure}
   \centering
  \includegraphics[width=14.0cm, angle=0]{V-K_shift_fig4}
   \caption{All LCs shifted by the average magnitude between 0.07-0.09. Inserted graph shows the the outline of LCs during phase 0-0.5 with the vertical line indicating the phase at which the deviation starts.}
   \label{Fig.V-K_shift}
   \end{figure}

\subsection{Flickering}\label{subsect:flickering}
  Even the LCs of intermediate state has less phase coverage than others, we can find the flickering only sticks out in high state, which indicates that the flickering accompanies high accretion rate and reminds us that transfer of material from the secondary is turbulent. In order to make clear the characteristics of the optical flickering of MN Hya, we analysis the spectrum of the LCs with enough phase coverage, the timescale of light intensity variation and the magnitude of the flickering in different parts of these LCs.

  The data of each run were subjected to period searches using a discrete Fourier transform (DFT) and the phase dispersion minimization (PDM) methods (\citealt{Stellingwerf1978Period}, or \citealt{Dai2016Cataclysmic,Dai2017Quiescent} as reference). Fig.~\ref{Fig.run6_dft} shows the spectrogram of the time series of Run6 determined by DFT. The dominate peak corresponds to the time interval of the data and others with amplitude greater than 0.05 are the harmonics of this time. PDM method provides the similar result. This result manifests the rapid time variation is random, which is same as the characteristic of X-ray \citep{Buckley1998Xray}. But the system shows obvious evidence for brightness variations on timescale of minutes, the explains maybe that there are some oscillations which last for only few phase interval and then die away to be replaced by other oscillations with a different period or at different phase.

\begin{figure}
   \centering
   \includegraphics[width=14.0cm, angle=0]{run6_dft_fig5}
   \caption{The upper panel shows the time series of Run6 and the lower panel gives its spectrogram determined by discrete Fourier transform. The dominate peak corresponds to the time interval of data.}
   \label{Fig.run6_dft}
   \end{figure}

   In order to find the characteristic timescale, we need to count up the number of different timescales. The method employed to deal with the data is described below. First,  in order to reduce the effect of variation of atmospheric seeing which can cause saw-toothed variation in adjacent sequence, we use moving average with 3 points to smooth the raw data of each run; then mark all the local extrema (maxima and minima), using which we give the histogram of the timescales between the extrema of the same type. As shown in Fig.~\ref{Fig.all_bin}, we find the dominating variation timescale as about 2 minutes, which is typical timescale in X-ray of other systems, such as EF Eri \citep{Patterson1981A} (period 6 min), VV Pup \citep{Maraschi1984Preliminary} (period 3 min), ST LMi \citep{Beuermann1985X} (period 1 min). If these variations occur at the threading point where the matter is channeled by magnetic filed, the timescale for Alfv\'en wave caused by instable accretion to cross the magnetosphere is
    \begin{equation}
    \label{Eq.12}
    P_{ins}(r) = 2 \times 10^{-3} r_{8}^{11/4} L_{34}^{1/2} f_{-2}^{-1/2} M_{1}^{-3/4} R_{8}^{-3/4} B_{7}^{-1} s,
    \end{equation}
where $r_{8}$ is the radius (in units of $10^{8} cm$, denoted as $r_{t}$ below) of the threading point, $L_{34}$ is the luminosity in units of $10^{34} erg s^{-1}$, $f$ is the fraction of the stellar surface where the accretion matter flows, $M_{1}$ is the WD mass in units of solar mass, $R_{8}$ is the radius of the WD in units of $10^{8} cm$, and $B_{7}$ is the surface magnetic field strength in units of $10^{12}G$. Adopting $f\approx 0.004$ \citep{Schmidt2001HSTSpectroscopy}, $B=40MG$ \citep{Buckley1998Polarimetry}, and other parameters mentioned earlier, we find the $r_{t}$ estimated for the timescale of 2 min as $2.8\times10^{10}cm$ or $30R_1$ ($0.62R_{L1}$). Comparing with the Alfv\'en radius, this length scale is much smaller, but is similar with that of AR UMa ($r_{t}\approx0.6-0.7R_{L1}$) shown on Doppler tomograms \citep{Hoard1999Accretion}, although the latter system has highest magnetic field. If the optical flickering is caused by the wobbling of threading point, the impact of the magnetic field strength on the position of that is very little.

    In order to quantify the flickering intensity, we remove the trend from the raw data using 30 points moving average method and calculate the standard deviation of the detrending data as the flickering intensity.
    Table~\ref{tab3} shows the flickering intensity corresponding to different phase interval, considering the two-pole model where Source1, Source2 and Total represent phase 0.03-0.4, 0.4-0.97 and all phase coverage, respectively. From this table, we can find the flickering intensity of Source1 is less than that of Source2 and that the flickering intensity reduces when the high-state system has higher accretion rate, such as Run8.

\begin{figure}
   \centering
  \includegraphics[width=14.0cm, angle=0]{all_bin_fig6}
   \caption{Histogram of the variation timescales of all data. The dominating timescale is about 2 min.}
   \label{Fig.all_bin}
\end{figure}

\begin{table}[!ht]
\bc
\begin{minipage}[]{100mm}
\caption[]{The flickering intensity of different parts given in table is the standard deviation of the detrending data of all phase, phase $\sim0.03-0.4$, and phase$\sim0.4-0.97$, those parts are denoted as Total, Source1, and Source2, respectively.\label{tab3}}\end{minipage}
\setlength{\tabcolsep}{5pt}
\small
\begin{threeparttable}
\begin{tabular}{ccccccc}
  \hline\noalign{\smallskip}
\diagbox{Source}{Intensity (Mag.)}{Data}
       &Run5 &Run6 &Run8 &Run9 &Run10&Run11\\
\hline\noalign{\smallskip}
Total  &0.117&0.104&0.065&0.085&0.142&0.033\\
Source1&0.072&0.082&0.058&0.063&0.063&0.029\\
Source2&0.137&0.121&0.072&0.100&0.181&0.035\\
  \noalign{\smallskip}\hline
\end{tabular}
\end{threeparttable}
\ec
\end{table}

\section{Discussion and Summary}\label{sect:summary}
 From the discovery mentioned above, we can describe the mass transfer process in MN Hya. The magnetosphere covers  42\% surface area of the secondary. Convection of the secondary can entangle the magnetic field which will be wound up, increasing their tension and stored energy until it reconnects to dissipate energy and cast matter globally, maybe in forms of intense stellar wind.  This kind of casted matter with high velocity will pass through the Alf\'ven radius freely. When matter flow reaches the threading point which has hight of $\sim30R_{1}$ above the surface of WD, it will be threaded by the magnetic field. As the system is in high state, the accretion rate still variates which can trigger the instability of the accretion column, and then a Alf\'ven wave will arise from the column and travel through accretion stream to the threading point. This wave causes the instability of the threading point whose wobbling could modulate the mass accretion rate then give rise to fluctuation which causes the flickering. \\

   In summary, the optical observations of the eclipsing polar MN Hya for 12 times during 2010-2016, with the addition of other observations, enable us get the following results:\\
1. A revised ephemeris is given based on 10 more mid-eclipse times, along with others obtained from literature and the quadratical fit to new data shows the period decreased during the state change as $-2.4\times10^{-12}dcyc^{-1}$, which can not be explained in the angular momentum conservation case. The X-ray observation of other authors implies the accretion rate as about $3.6\times10^{-9} M_{\odot}yr^{-1}$ during high state. Those indicate the minimal distance of the decoupling point to the COM is about $0.81a$ which implies the mass lost from the secondary. And the magnetosphere covers about 42\% surface area of the secondary, which can cause the mass loss fraction of 58\% if the secondary goes through an intense stellar wind globally. This kind of mass loss fraction is very close to that deduced from losing mass through L2. The mass loss fraction is about  60 percent at least, so any model not taking into the effect of mass lost should be unrealistic.\\
2. The primary timescale of the flickering is about 2 minutes, which implies the threading point is about $30R_1$ above the surface of the WD. Within the high state, the flickering sticks out, and springs from the modulation of the accretion rate due to the wobbling of the threading point; also the data shows the intensity of flickering reduces when the system has an increasing accretion rate.\\
3. In the frame of two-pole model, the dominate accretion region is nearly face on to us near phase 0.7. Considering the continuing mass transfer during low state, this model predicts that the low-state LC should show intensity hump near phase 0.7, which contradicts the observation. The high-state LCs follow the shifting low-state LCs from phase 0 to phase 0.4, such large fraction of phase indicates the hump near phase 0.2 is caused by the WD itself rather than a tiny accretion region, which also does not conform to two-pole model. These two facts make the two-pole model less convincing.\\

\normalem
\begin{acknowledgements}
This work is supported by the Chinese Natural Science Foundation (Grant Nos. 11325315, 11611530685, 11573063, and 11133007), the Strategic Priority Research Program "The Emergence of Cosmological Structure" of the Chinese Academy of Sciences (Grant No.XDB09010202), and the Ministry of Education, Youth and Sports of the Czech Republic project LG15010. All observations in this paper were made at the 2.15-m Jorge Sahade telescope (JST) in Complejo Astron\'omico E1 Leoncito (CASLEO), San Juan, Argentina and the Danish 1.54-m Telescope at ESO La Silla, Chile. Finally, We are very grateful to the anonymous referee for an insightful report that has significantly improved the paper.
\end{acknowledgements}

\bibliographystyle{raa}

redpajama_set_name: RedPajamaArXiv


"These are good vanilla cupcakes."
Preheat oven to 350 degrees F (175 degrees C). Line 2 cups in a muffin pan with paper liners.
Whisk egg white and sugar together in a bowl; stir in melted butter and vanilla extract until smooth. Add flour, baking powder, and salt and mix well. Add milk and mix until smooth. Divide batter equally between 2 prepared cups in muffin pan.
Bake in preheated oven until cake is set, 10 to 12 minutes.
Use a heaping 1/4 teaspoon of baking powder to get the best results.
They are so smooth! Easy to make and a great result!
It was really buttery tasting, and had a odd texture.


text:
House of the Day
Broker Shows No Confidence in Blinding Hamptons Beach House
By Rob Bear Mar 18, 2011, 3:00pm EDT
Have a nomination for a jaw-dropping listing that would make a mighty fine House of the Day? Get thee to the tipline and send us your suggestions. We'd love to see what you've got.
Location: Wainscott, N.Y.
The Skinny: Cole Perkins, the young lad over at Lavish Property, featured this Wainscott, N.Y. beach house last week, and found a lot to like about the five-bedroom contemporary. Pity the broker doesn't think so. He's been marketing this $23.5M property as a teardown, and spends much of the brokerbabble describing the house one could build on the site, rather than the one that's there, which, despite it's monochromatic color scheme, seems to be a well maintained—a casual beach house without the pretense. At 3,000 square feet, it's smaller than one might expect for the money, but there's something to be said for a throwback to the Gordon Gekko corporate raider architecture of the 1980s. We're not trying to say this is some architectural masterpiece, but does the Long Island coast really need another overgrown, nouveau-Shingle Style behemoth?
· 124 Beach Lane [Corcoran]
· Estate of the Day: 124 Beach Lane [Lavish Property]
· Please Welcome the 13-Year-Old Real Estate Blogger to the Dancefloor [Curbed National]
Next Up In House of the Day
Frank Lloyd Wright Usonian (Built With Red Tidewater Cypress) Asks $425K in Wisconsin
A 'Floating' Glass House Asks $7.5M in Dallas
Carmel Oceanfront Home With Barrel-Vaulted Ceilings Asks $14.5M
Mid-Century "Cube" House Just Outside Detroit Now Wants $635K
'70s Orlando House With a River in the Backyard Asks $865K
Modern Farmhouse Asking $2M in Connecticut Has Exposed Beams in Almost Every Room


To upload your own logo, click on Settings. On the Settings page, click on Logo & Company Information. From there, click on the Choose File button and locate the logo you wish to use on your invoices. After loading the file, click on the green "Upload Logo" button. Send an invoice with your own logo makes you feel special, doesn't it?
Hi There. I am trying to update my logo however i am having a lot of trouble. First I delete my existing logo...done! Then I upload my new logo file which is 180x180 pixels and only 12kbs. I clicked the Upload Logo button but then my old logo appears again instead of the new one. It's extremely frustrating. My login is bloommarketing and my logo file is attached. Help please.
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If you still need help, feel free to email at patrick @ blinksale dot com.
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text:
Home | All news | Politics | Armenian-Turkish "row" at NATO session or why Cavusoglu decided to become a diplomat
Armenian-Turkish "row" at NATO session or why Cavusoglu decided to become a diplomat
Issues of Armenian-Turkish relations and Turkey's role in conflicts were raised at the 62nd NATO Parliamentary Assembly Session held in Istanbul November 18-25. The Q&A periods turned into heated debates at times and was described in Turkish media as "row" between Armenian and Turkish politicians.
The head of the Armenian delegation Koryun Nahapetyan asked about the closed border with Armenia and Turkey's role in the Karabakh conflict after Turkish Foreign Minister Mevlut Cavusoglu's report on the concept of "zero problems with neighbors."
"Trapped in an awkward situation, the Turkish FM tried to make some baseless accusations against Armenia and Armenians. He even referred to the issue of Genocide although we had never raised the question," Nahapetyan said.
The head of the Armenian delegation said he would not describe the debate as a "row," but added that "Cavusoglu definitely got nervous." The Turkish Foreign Minister even recalled the reasons behind his decision to become a diplomat.
"He recalled ASALA, the fact that Turkish diplomats were affected by the organization's activity. Cavusoglu said he became a diplomat ignoring his mother's objections," Koryun Nahapetyan said.
During the plenary sitting the Armenian delegates had an opportunity to address questions to NATO Secretary General. Asked about NATO's possible role in the opening of the Armenian-Turkish border, Jens Stoltenberg said "it is an issue of the two countries and NATO can play no role here."
Referring to the Karabakh conflict, the Secretary General said the organization's stance on the issue had not changed. "NATO is in no way involved in the settlement of the conflict and welcomes the negotiation process under way within the framework of the OSCE Minsk Group."


Matt Smith has revealed he is very excited about the upcoming 'Doctor Who Live' shows which will feature an array of the Time Lord's greatest enemies.
Matt Smith can't wait to see "big explosions and monsters" at the 'Doctor Who Live' shows.
And of course it will be scary it's 'Doctor Who'. I am going to the show on Friday October 8 at Wembley Arena - be there or be oblong.
The 27-year-old actor - who plays The Doctor in the BBC One sci-fi series - will be attending the opening night of the spectacular stage show next Friday (08.10.10) and admits he is very excited to see his character's greatest enemies come to life.
He said: "'Doctor Who Live' - the monsters are coming! It's going to be an extravaganza, quite simply as a 'Doctor Who' fan it's all your dreams come true at once. Every monster from the entirety of its history set to Murray Gold's brilliant and now iconic score and that's without mentioning the pyrotechnics which I always love. There's going to be explosions, big explosions with monsters.
"And of course it will be scary it's 'Doctor Who'. I am going to the show on Friday October 8 at Wembley Arena - be there or be oblong."
Matt also revealed The Doctor will be left with a crisis to solve when Vorgenson - a unique new character developed for the show and played by 'Young Ones' star Nigel Planer - summons the monsters with his invention 'The Minimiser'.
In a video interview available at www.doctorwholive.com, Matt added: "Vorgenson is an intergalactic showman who has the terrible and rather ghastly machine called 'The Minimiser'. I won't tell you what it does, but needless to say it has a lot of power and places The Doctor in a position that he needs to address."
Although Matt will not be starring in the stage show he will appear as The Doctor in several video scenes, and the show will feature a huge array of the Time Lord's enemies including the Daleks, Cybermen, Judoon and Silurians.
The upcoming 25-date stage show kicks off at London's Wembley Arena on October 8, and will visit Sheffield, Glasgow, Birmingham, Manchester, Nottingham, Cardiff and Liverpool before closing in Belfast on November 7.
Tickets are available via www.doctorwholive.com and through Ticketmaster.


text:
Conquest of the Planet of the Apes (1972)
In a futuristic world that has embraced ape slavery, Caesar, the son of the late simians Cornelius and Zira, surfaces after almost twenty years of hiding out from the authorities, and prepares for a slave revolt against humanity.
—Kenneth Chisholm
Cornelius and Zira's son Caesar leads apes to revolution in this installment of the apes saga. Dogs and cats have been wiped out by a plague and now apes are household pets that are treated like slaves. Caesar has the intelligence to fight this oppression.
—Josh Pasnak <chainsaw@intouch.bc.ca>
Fourth feature in the simian series has apes domesticated and turned into work slaves in the near future. Along comes Ceasar, son of Cornelius and Zira who died in the third film, who leads his chimp brothers in rebellion against the human oppressors, thus creating the time loop that leads to the first film.
—Humberto Amador
The synopsis below may give away important plot points.
In 1983 (several years after the end of 'Escape from the Planet of the Apes'), an interstellar disease kills the world's cats and dogs, leaving humans with no pet animals. To replace them, humans began keeping monkeys and apes as household pets. In time, humans notice the apes' capacity to learn and adapt; thus they train them to perform menial household tasks. By 1991, the former United States of America and most of the North American continent has become an oppressive and fascist police superstate culture of uniformed classes and castes, based upon ape slave labor. The different apes are divided into similar caste systems; gorillas wear red jumpsuits; chimpanzees wear green jumpsuits; and orangutans wear orange jumpsuits.
In the opening scene, Armando (Ricardo Montalbán) and Caesar (Roddy McDowall), a young chimpanzee horseback rider in Armando's circus, visit a large city to distribute flyers advertising the circus' arrival to town. Armando warns the chimpanzee to be careful; should anyone learn his identity as the child of the late Cornelius and Zira, it would mean their deaths. Walking the streets, they see apes cleaning streets, delivering packages, et cetera, and are shocked by what is done to disobedient apes. Seeing an ape being beaten and drugged by black-uniformed neo-Gestapo police units, Caesar shouts: "Lousy human bastards!". Quickly, Armando takes responsibility for the exclamation, explaining to the policemen that it was he who shouted, not his chimpanzee. The surrounding crowd become agitated, and Caesar runs away.
Hiding in a stairway, Armando says he will go to the authorities and settle the matter by bluffing. Meantime, Caesar must hide among his own kind (in a cage of orangutans from Borneo), and soon finds himself being trained for slavery through violent conditioning. He then is sold at auction to the neo-Fascist Governor Breck (Don Murray). Gov. Breck allows the ape to name himself by randomly pointing to a word in a book handed to him and the chimpanzee's finger rests upon the name Caesar, as if by chance (but the audience knows that the ape can read and searched for the name). Caesar is then put to work by Gov. Breck's chief aide, the African-American MacDonald (Hari Rhodes), who sympathizes with the apes to the thinly veiled disgust of his boss, and eventually deduces Casear's true identity.
Meanwhile, Armando is being interrogated by Inspector Kolp (Severn Darden), who suspects his "circus ape" is the child of the two civilized apes from the future back in 1973. Kolp's assistant puts Armando under an authenticator machine that psychologically forces people to be truthful. Rather than confessing, Armando fights the guards and commits suicide by jumping to his death through a window. Learning of the death of the only human he loved, Caesar loses faith in human kindness and begins plotting a simian rebellion.
Secretly, Caesar teaches the combat arts to the other apes and has them gather weapons. Meanwhile, Gov. Breck learns from Inspector Kolp that the manifest of the vessel that delivered Caesar lists no chimpanzees. Suspecting Caesar is the ape the secret police are hunting, Breck's men arrest Caesar and electrically torture him until he speaks, thus betraying his identity. Hearing the confession, Breck orders Caesar's immediate death. Caesar survives his execution because MacDonald, feigning over-sensitivity to torture, reduces the electrical power of the machine. Once Gov. Breck leaves, Caesar kills the torturer and escapes.
Caesar leads an ape revolt against Ape Management and a violent and climatic 25-minute battle begins. The apes are victorious after killing most of the riot police. After bursting into Gov. Breck's command post and killing most of the personnel, Caesar has Breck marched out to be executed in the courtyard. MacDonald appeals to Caesar's humanity to show mercy to his former persecutor. Caesar ignores him, and in a rage declares:
"Where there is fire, there is smoke. And in that smoke, from this day forward, my people will crouch, and conspire, and plot, and plan for the inevitable day of Man's downfall. The day when he finally and self-destructively turns his weapons against his own kind. The day of the writing in the sky, when your cities lie buried under radioactive rubble! When the sea is a dead sea, and the land is a wasteland out of which I will lead my people from their captivity! And we will build our own cities, in which there will be no place for humans except to serve our ends! And we shall found our own armies, our own religion, our own dynasty! And that day is upon you NOW!"
However, as the apes raise their rifles to beat Breck to death, Lisa (Natalie Trundy), Caesar's beloved and later wife, voices her objection; "NO!" other than Caesar, she is the first ape to speak. Caesar reconsiders and orders the apes to lower their weapons, saying:
"But now... now we will put away our hatred. Now we will put down our weapons. We have passed through the night of the fires, and those who were our masters are now our servants. And we, who are not human, can afford to be humane. Destiny is the will of God, and if it is mans destiny to be dominated, it is Gods will that he be dominated with compassion, and understanding. So, cast out your vengeance. Tonight, we have seen the birth of the planet of the apes!"
The final shot shows Caesar standing among all his fellow gorillas, chimpanzees, and other apes among the burning buildings as the city burns to the ground.
Conquest of the Planet of the Apes
Movies I own - C
Group completion
SEVENTIES - 70'S
Our DVD - Other


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Jeremiah Green, drummer for the band Modest Mouse, has been diagnosed stage 4 cancer
According to a Facebook post by his mother, Jeremiah Green, the drummer for the band Modest Mouse, has been told he has stage 4 cancer.
Green helped start the band in 1993 alongside Isaac Brock, the lead singer, and Eric Judy, the bassist. Green is one of the band's co-founding members.
Yesterday (December 25), the drummer's mother, Carol Namatame, sent a message on Facebook pleading with followers to "please send healing energies for my son […] who is suffering stage 4 cancer." "He is hanging in there and is so strong and brave!" Added she.
Veteran Seattle, radio DJ Marco Collins also disclosed Green's condition in a Facebook post, writing: "Just learned that my friend Jeremiah Green (Modest Mouse) has canceled the band's tour since he is now having chemotherapy to fight Stage 4 Cancer.
"His outlook is favorable despite his stage 4 diagnosis! Additionally, his oncologist is a massive fan of MM (so he has that on his side!). I'm only sending him love and healing energy! Well done, friend. Everyone is rooting for you!
As Collin pointed out, the illness prevented Green from finishing the tour even though he had participated in earlier dates of Modest Mouse's recent tour honoring the 25th anniversary of their ground-breaking second album, "The Lonesome Crowded West."
Green hadn't previously been gone from the band between 2003 and 2004 and, as a result, didn't appear on the album "Good News For People Who Love Bad News" before that tour.
Modest Mouse announced in July that they had been working on fresh music and "seven new songs coming out quite soon."
Frontman Isaac Brock told NME at Spain's Mad Cool Festival: "I have seven new songs coming out soon. I was bothered by everyone asking, "Why does it take so long to put out records" as soon as we finished the last album.
I have other hobbies, therefore. They're not all great, but screw it! I have a record that I'm incredibly delighted with, so I don't want to answer that question anymore.


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Q: Multiple submit form in one html form file Id like to ask some easy and cross platform code/structure I can use for this form:
I have a form that have 3 sections
1st section : Entering course information
2nd section: Entering participants information
3rd section: entering Corporate account information
Each section has a submit button that when clicked saves the data to mysql database
User can add unlimited set of data per section (except 3rd section).
Meaning I will create an add button per section that will display one set of data in a table row. When clicked another row is added. When they are done with the desired number of set of data. They will click the submit button and these sets of data will then be saved in database.
I dont know how to approach it properly. If I use one submit button for all the section, I thought, I need to create sets of table inside mysql that corresponds to the number of fields in my html form.
The problem would be, the number of sets of data per section will be limited only to the number of tables in my sql

redpajama_set_name: RedPajamaStackExchange


http://www.top5sportsbooks.com/index.html - Top5sportsbooks.com is a leading reviewer of some of the best online sportsbooks around. Our unbiased reviews give you access to the highest rated, offshore sports betting web sites.
Top5sportsbooks.com is a leading reviewer of some of the best online sportsbooks around. Our unbiased reviews give you access to the highest rated, offshore sports betting web sites.


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Q: Can two apps have same .xap file name? I have developed a paid app for WP7. Now, I am creating free version by slightly modifying it. Can both the apps have same .xap file ? Will it not create any issue for the users who have both the versions ? How to modify the name if required ?

A: The xap name isn't important, as each app is deployed to a different folder on the phone. Just make sure that both apps have different icons and different names or they'll fail the certification.

A: They can have same XAP name or assembly name or namespace, but make sure the ProductID is different when testing and debugging. Otherwise you'll overwrite the first app when deploying but the second app.
By defining two different ProductIDs you are able to deploy them side by side and test them as two different apps.


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Request a Free Consultation.
ERISA – Bad Faith Insurance
John M. Stinar
M. James Zendejas
Ian P. Burrell
Paul G. Kloster
Christopher G. Wilhelmi
Trudy H. House
Brenten A. Ward
Evan C. Withrow
Beau Worthington
Christian D. Game
FOUNDING PARTNER & ATTORNEY
John M. Stinar was born October 6, 1956, in Los Angeles, California but grew up in Las Vegas, Nevada. He attended Bishop Gorman High School in Las Vegas and then went on to receive his undergraduate degree in accounting from the University of Santa Clara in Santa Clara, California. He attended the University on the Carroll Academic Scholarship and graduated cum laude. While attending the University, John was a member of Beta Gamma Sigma, the Business Honor Society, and the Alpha Sigma Nu National Jesuit Honor Society. After graduation, he worked in the tax department of Price Waterhouse in San Jose, California, while also attending law school at the University of Santa Clara. John was admitted to the California Bar in 1981, to practice before the United States Tax Court in 1983 and admitted to the Colorado Bar in 1985. Concurrently, in 1983, John also became licensed as a Certified Public Accountant. John went on to join the Colorado Springs law firm of Braden & Frindt as an associate in March 1986. He became a partner on January 1, 1989, and the firm name was changed to Braden, Frindt & Stinar, LLC. On January 1, 2001, John formed Stinar & Zendejas, PLLC which has become one of the prominent firms in Colorado Springs and El Paso County.
PROFESSIONAL & COMMUNITY
John is a long-standing member of the community and has served or is currently serving on several charitable boards including Colorado Springs Youth Sports Complex, Fostering Hope, Griffin Centers and St. Mary's Catholic High School. Additionally, John also serves as pro-bono legal counsel for the Colorado Springs Amateur Hockey Association.
University of Santa Clara, B.S., Accounting
University of Santa Clara Law School, J.D.
BAR ADMISSIONS & COURT ADMISSIONS
California (inactive)
Colorado Bar Association
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Housing & Building Association of Colorado Springs
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Business Planning & Acquisition
Representation before the IRS & US Tax Court
General Business Matters
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Business Planning and Acquisition
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Housing and Building Association
**Most attorneys in our firm provide a free initial consultation. Please inquire when contacting our firm for details.
info@coloradolawgroup.com
121 E Vermijo Ave #200 Colorado Springs, CO 80903
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Mobile/Cellular Service Providers Canada Post Corporation Customer Service mail not delivered to telequip systems.
Canada Post Corporation / mail not delivered to telequip systems.
We had problems with mail not showing up at our location between Nov to Dec 2018 in Barrie, Ontario at the above location, when there was a strike. Upon phoning our customers for payment of outstanding invoices, we had at least three customers said the cheque was sent in the mail. Our customers discovered the cheques had been cashed. Telequip did not cashed them. We had to claim fraud. Just thought Canada Post should know.
mail not delivered to telequip systems.


We have a stunning Ochid and bowl available to win form Marks and Spencers, this is an easy orchid for msot people so you should have plenty of enjoyment from it.
This stylish twin stem multi-floral Phalaenopsis orchid will make a statement in any home. Allow it to cause a stir again and again by displaying by a window that doesn't get direct sun allowing it to bloom for many weeks. With care will reflower in future.
To Enter all you have to do is answer the following question.
What type of Orchid is pictured above.
Remember we will need to be able to contact you if you do win, so whilst "anonymous replies" can be made to the blog if there isn't a way to contact you then these will sadly have be discounted please leave a twitter name for us to get hold of you if you enter this way.
Extra entries can be made by sharing this competition on Twitter (include #orchidgardens so we can see your extra entry) or by liking our page and sharing the competition from Facebook.
Terms and conditions: This competition closes at 23.59 on 26 September 2013. Any entries received after this time will not be counted. Entrants must be UK residents aged 18 years or older to enter. By entering this competition you agree and consent to your name being published and by taking part in the competition, entrants are deemed to have read, understood and accepted all of the Terms and Conditions and agreed to be bound by them. The winner will be selected at random from the correct entries and will be announced here on the blog. Please make sure we are able to contact you if you do win.
The answer is a) Phalaenopsis .
I have just been to your facebook page, it is beautiful. I really enjoyed the photos.
What are the best gloves to use for gardening?


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Eclipse Resources 1Q15: Impressive Bump Up in Production & Revenue
May 7, 2015 Eclipse Resources, Energy Companies, Ohio, Statewide OH
Eclipse Resources, a relatively new driller formed by a group of former Rex Energy people, is headquartered in State College, PA but does most of its drilling in the Ohio Utica. Just a few weeks ago Eclipse announced they are cutting their 2015 drilling budget by 57% (see Eclipse Resources Nixes Joint Venture Idea, Cuts Capex 57% in 2015). Even with the cuts, Eclipse had by anyone's measure, an impressive first quarter in 2015. Yesterday Eclipse issued their 1Q15 update showing net production is up 316% from 1Q14. During the first quarter they brought 20 new wells online and began drilling 10 more. Revenue was up a huge 77% in 1Q15, but because of interest payments, taxes and other expenses, the company, overall, experienced a loss of $34.1 million during 1Q15. Here's the update…
MarkWest 1Q15: Life is Good in the Marcellus/Utica Midstream
Penn State Uses Anti-Drilling Trout Unlimited for Marcellus Monitoring


Needing some help/advice with tags - face & area.
If you add tags of either kind is there a way to remove/delete them"
What is the "link" "unlink" about? What effect does this have?
The tip says you can double-click to rename the tag so what effect does this have on the catalog label?
Is there a way to have the tag invisible and only show when the mouse pointer is over the tag?
When you link an area to a catalog label then you identified the area as being a specific catalog label representation of (typically) a person. When you delete a linked area, the catalog label wil also be unassigned of the image.
None, typically the name of the area would be the name of the person (hence the catalog label). If you decide to name the area differently then you're free to do so. Area captions are also searchable with the Search Bar, so sometime you could make use of that.
There's not. But you can enable/disable the display of areas completely. Open an image in the Viewer and there select this option.
Thanks so much. That's a big help.


Nuova gerenza, Fondue Bourguignonne eccezionale!
Hey, do you have a safe in each of your apartments?
Мини кухня есть в каждом номере?
Is Phillipe still the manager at SPB?
Hi, this is not the Swiss Palms email contact, it is Trip Advisor. You need to contact them directly info @ swisspalmbeach. com or go to the contact page on the Swiss palms webpage. Phillipe is unlikely to read the questions on TA . . .
Hi Phillipe we are booked in 23rd December till 12 Jan we have sent a couple of emails (no reply) regarding whether apt 16 is available wonder if somebody ciuld get back to us. thank you Gordon and Sheila Whyte.
Hi, this is not the Swiss Palms email contact, it is Trip Advisor. You need to contact them directly info @ swisspalmbeach. com or go to the contact page on the Swiss palms webpage. Phillipe is unlikely to read this . . .


Flying off for a beach holiday or safari is so last season. Nowadays, Casino Resorts are where "its" at. By "it", I mean the money, and all that money can buy. These opulent, beautifully designed works of art, where your every need is catered for and your dreams may just come true, are the new wonders of the world. Gambling at the casino reveals peoples true characters, and these multibillion business corporations have capitalised on years of people watching, in order to bring us what we want, what we really, really want.
Click To View The World's Top Casino Resorts Info-graphic.
At a casino resort you have a place to relax that has been designed with you in mind. With your comfort, your family and your happiness in mind, from the design to the architecture, a casino resort is a place of perfection, suitable for any type of customer that has the goal of relaxing, kicking back, unwinding and being a winner.
Fly off into the sun for clear beaches and blue skies.
Despite what you may think, a casino resort holiday is not just about gambling. There is a maze of other stuff available to you that will make sure your time off work is well spent. A casino resort combines a gambling palace, along with a luxurious hotel. They typically have spas, pools, Jacuzzis and all the other trimmings you could possible want, like massages, beauty treatments and, of course, fine dining. Casino resorts are more common than you may at first think.
Casino resorts are typically located in main cities and are near shopping centres and a whole host of other tourist attractions, that any country's big cities may have to offer. They also have cabaret shows, a nod to family entertainment from back in the day; they also feature concerts and even sporting events.
In fact, I am struggling to write this list as I keep getting distracted and checking out flights to South Africa for a couple of weeks of glitz and glamour betting all night, and safari by day.
A Casino Resort has it ALL.
The first casino was actually called a gambling house and was in Europe. Venice to be exact. It was called the Ridotto and it opened in 1638.
In America, casinos were known as saloons and grew from their early roots in New Orleans, St. Louis, Chicago and San Francisco, to today's sprawling metropolis of Nevada and the Las Vegas Strip we have all come to know and love.
Las Vegas is the second largest gambling destination in the world and has a reputation that is nearly un-rivalled when it comes to the place to gamble on a trip with friends to celebrate a special occasion. The city regularly features as the go to place in Hollywood movies, such as The Godfather Part II and The Hangover, amongst many, many other quality films.
And the greatest part is that there are so many fun things you can do in Las Vegas.
However, there is something about casino resorts that you do not know; Las Vegas isn't the only place to go if you want a top casino resort experience, complete with all the hustle and bustle of the town.
Where Are The Best Casino Resorts?
South Africa, Egypt, China, Monaco and Portugal, Argentina, Puerto Rico, Spain and the Bahamas are all home to some of the worlds best casino resorts. There are a number in Las Vegas, but other US cities also get a look in, with Connecticut and New Orleans making the top casino resorts worldwide list.
So let's get down to business and find out about the casino resorts that have won awards and are considered world leaders in resort and gambling fun.
Since 1994, the World Travel Awards have been taking notice of excellence in casino resorts and giving out awards. They concern themselves with acknowledging, rewarding and celebrating the global travel and tourism industry.
2013 has been a turnaround year for MGM Grand Hotel & Casino in Las Vegas, USA. They were awarded with the prestigious title of World's Leading Casino Resort, having last seen the award 7 years ago. They were the first casino resort to be awarded with this honour back in 1994.
The winners over the past 20 years tell us a lot about the changing tides of the casino resort. While the 90's were full of US casino resort award winners, mainly located in Las Vegas, the 00's gave rise to the Far East casino resorts. As the 10's come around, the Bahamas and other exotic destinations are starting to level up with the required standards to be eligible to make the world class casino resort list.
Caesars Palace Las Vegas made the list 7 years in a row, making it the most awarded casino resort worldwide in its time. The market is now opening up even further, with plans for a Mega Casino Resort in South Korea and Sri Lanka.
Explore Casino Resorts across Europe.
For Brits looking for a spot in the sun, at cheap, affordable European getaway prices, Spain has it all. Long a popular destination for members of the United Kingdom to get away from the dreary pitter patter of constant rain and gloomy skies, Ibiza Town also has a hidden gem in the form of The Ibiza Gran Hotel.
This luxurious casino resort nestled in the party city of Ibiza, boasts luxury, glamour and, surprisingly enough, tranquillity. Located next to the harbour, it offers everything from honeymooners to long weekenders a place to relax, enjoy and gamble. If you want a taste of Spanish nightlife and culture, check out this nearby treat.
Staying within Europe, despite a casino resort of the same name being located in China, the Casino Lisboa is in the Parque das Nações (Park of Nations). It has a major urban centre, not a tourist centre and has had its fair share of troubles due to this, but a trip to Portugal would not be the same without a visit to this architectural masterpiece.
This Argentinian delight has a 19th century Spanish colonial design, restored to its original magnificence. Consistently rated extremely highly for its succulent lodgings and updated amenities, it is a focal point for business travellers and holidaymakers alike. Be careful when you partake in the stunning wines on offer from the Mendoza region if you are going to be rolling, spinning or holding hands in the casino later that evening! Argentina is termed part of Neo-Europe, which means a place outside of Europe but with strong ties and similarities to the EU.
For some of the finer things in life, why not check out this online slot?
Why not try a Casino Safari at an African Resort?
Two of South Africa's most popular casino resorts are the Sun City Resort in Cape Town and the Tusk Rio Casino Resort in Klerksdorp, a few hours' drive from Johannesburg.
The Sun City Resort is a huge complex, containing everything you could dream of on that holiday of a lifetime. With easy access to daily safaris, you can spend your days meeting all the wildlife this beautiful country has to offer, followed by excellent service and two different casinos, The Jungle Casino and the Sun City Hotel Casino. They also run a School of Gaming for those entering the gambling world for the first time.
South Africa's second offering making this list is the widely known Rio Casino Resort. Boasting a carnival style atmosphere and a plethora of activities for daytime trips, this casino resort has a multitude to offer. There's paintballing, hiking, a zoo, horseback riding, canoeing, scuba diving and so much more. Your nights will be well spent, cosy in the Winners Circle at the 24/7 casino.
Puerto Rico is a gem in the Caribbean.
The Ritz-Carlton, San Juan is an oasis of calm. Set against the gently crashing waves of the sea, it's an exercise in complete elegance, the 24/7 casino will take you back to a forgotten era and has live music to entertain you on the weekends. Beautifully and elegantly decorated, the Ritz-Carlton surpasses itself with this diamond in the mist. A perfect place to unwind and relax by day, with spa rooms galore, and enjoy breathless nights chasing your very own Lady Luck at the tables of Puerto Rico's luxury casino resort.
Winners racing around the streets of Monaco.
The Hotel de Paris in Monte Carlo embodies a bygone era. A time when Princes wore glittering jewels and Princesses wore diamond tiaras, as they laughed, chattered and bet their way around the city. The hotel usually features on the glamorous Conde Nast Traveller Gold List and will delight your taste buds with its 3 Michelin star restaurant. Win or lose, the surroundings are exquisite and will put you in that essential winning frame of mind whilst putting you in touch with your zest for life.
The Middle East is full of amazing surprises.
Our travels bring us to a shining beacon in the desert, tucked away amongst the unrest in the Middle East. The Cairo Marriott Hotel and Omar Khayyam Casino put together are Egypt's offering to our list of the top casino resorts worldwide. The nearby sights include the Egyptian Museum and the Cairo Zoo, but it is really the casino night life that makes this a must see destination. Once a palace, the Marriott hotel facilities have a bustling casino nightlife attached, said named after the great Persian man of culture himself.
Most of the big players nominated for industry awards own a whole host of casino resorts, and just because they have not made the list above, does not mean they are not worth checking out further. A lot of already established US casino resort owners are branching out into the worldwide market and taking advantage of the growing desire for travel that includes not only a hotel, spa and swimming pool, but also a place to bet and win. They have seen great success with their Las Vegas casino resorts and are using years of expertise to improve the rest of the world.
The Far East is closer than you think!
Macau is the undisputable largest gambling city in the world, with Las Vegas long since coming in a close second behind the Chinese hub of gambling establishments full furnished with all the casino games you could dream of.
Even Versace is getting in on the Macau casino resort act. You can read more about that here.


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Exclusive: Lazarus Theatre Company return
The classics rep company to perform Troilus and Cressida at the Tristan Bates Theatre.
Greg Jameson
We can exclusively announce, on William Shakespeare's (probable) birthday, that classical repertory troupe Lazarus Theatre Company are to return with a production of his play Troilus and Cressida, which will be adapted and directed by Ricky Dukes. It will be performed at the Tristan Bates Theatre as part of the Camden Fringe theatre festival this autumn.
Troilus and Cressida will play from Monday 18th through to Saturday 23rd August as part of the Camden Fringe, and extend its run from Monday 25th to Saturday 6th August, with the shows starting at 7.30pm.
Tickets will be available soon through the Tristan Bates Theatre website.
Following last year's sell out production of The Tragedy of Mariam, Lazarus are delighted to be returning to the Tristan Bates Theatre and to the Camden Fringe.
Shakespeare's Troilus and Cressida concerns two young lovers who are thrust into the tempest of war where their love is tested, punished and ultimately torn. The theme of the motives of conflict and the effect upon those in the eye of the storm is a timely one, and is set to come to the stage in a fresh and bold new adaptation.
The award-winning Lazarus Theatre Company is committed to producing the best in classical theatre for a modern audience.
Casting for Troilus and Cressida is to be announced soon.
In this article:Camden Fringe, Camden Fringe Festival, Lazarus Theatre Company, Ricky Dukes, Theatre Festival, Tristan Bates Theatre, Troilus and Cressida, William Shakespeare


Hey Uli-ers..... Not sure if thats gonna catch on. I'll make it happen. Its been a while since I posted, but I have been quite busy working on a lot of things. Some fell through, some are in progress, but all is well. The biggest thing is I might be moving sooner than planned, and if all goes well, the west coast will be my new home. More to come on all the projects Ive been working on soon. For now check out this video I appeared in, helping You-Tuber D-Cubed with a skit!


This property is located in the Westport Industrial submarket off Page and Schuetz Road, offering easy access to I-270.
This 24,500-square-foot office/warehouse building in Westport offers great visibility and accessibility to Page from Schuetz Road. The property includes 4,500 square feet of office build-out, two front loading docks, one drive in and 15-foot ceiling heights. There are also 40 parking spaces along with room for outside storage and additional income from American Family Insurance.


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Copyright Applies to
Music & Copyright
International Song and Lyrics Copyrights
While no creative work is automatically protected worldwide, there are international treaties which provide protection automatically for all creative works as soon as they are fixed in a medium. There are two primary international copyright agreements, the Buenos Aires Convention and the Berne Convention.
In most countries copyright lasts a minimum of the life of the composer / creator plus a minimum of 50 years. This is for most types of recorded, written, dramatic and artistic works,
Song and lyrics Copyright Registration - Is it Worth it?
In general, copyright registration is a simple formality intended to make a record of the basic facts of a particular copyright. However, registration is not a condition of copyright protection. Even though registration is not a requirement for protection, the copyright law provides several inducements or advantages to encourage copyright owners to make registration.
To Fully protect your rights in a court of law it is vitally important you have proof of copyright ownership. To back up any claim should a conflict of rights to a certain piece of work arise a copyright certificate would suffice.
What is Not Protected by Copyright?
Several categories of material are generally not eligible for copyright protection. These include among others:
Works that have not been fixed in a tangible form of expression (for example, choreographic works that have not been notated or recorded, or improvisational speeches or performances that have not been written or recorded.)
Titles, names, short phrases, and slogans; familiar symbols or designs; mere variations of typographic ornamentation, lettering, or colouring; mere listings of ingredients or contents.
Ideas, procedures, methods, systems, processes, concepts, principles, discoveries, or devices, as distinguished from a description, explanation, or illustration.
Works consisting entirely of information that is common property and containing no original authorship (for example: standard calendars, height and weight charts, tape measures and rulers, and lists or tables taken from public documents or other common sources.)
Copyright Infringements.
Today's technological innovations present almost limitless opportunities for the worldwide distribution of copyrighted works. But these same technologies make it possible for anyone to pirate works with a single keystroke.
Unauthorised publishing, broadcasting or copying even a small part of a song or piece of music will undoubtedly deny the original creators of all the revenue and recognition that is normally generated by a successful composition.
Click here to learn more about Copyright and Music
Copyright gives the creators of a wide range of material, such as literature, art, music, sound recordings, films and broadcasts, economic rights enabling them to control use of their material in a number of ways, such as by making copies, issuing copies to the public, performing in public, broadcasting and use on-line. It also gives moral rights to be identified as the creator of certain kinds of material, and to object to distortion or mutilation of it. (Material protected by copyright is termed a "work".)
The purpose of copyright is to allow creators to gain economic rewards for their efforts and so encourage future creativity and the development of new material which benefits us all. Copyright material is usually the result of creative skill and/or significant labour and/or investment, and without protection, it would often be very easy for others to exploit material without paying the creator.
How to Secure a Copyright.
The way in which copyright protection is secured is frequently misunderstood. No publication or registration or other action in the Copyright Office is required to secure copyright. There are, however, certain definite advantages to registration.
Copyright is secured automatically when the work is created, and a work is "created" when it is fixed in a copy or phonorecord for the first time. "Copies" are material objects from which a work can be read or visually perceived either directly or with the aid of a machine or device. Such as books, manuscripts, sheet music, film, videotape, or microfilm. "Phonorecords" are material objects embodying fixations of sounds (excluding, by statutory definition, motion picture sound tracks), such as cassette tapes, CDs, or LP's. Thus, for example, a song (the "work") can be fixed in sheet music ("copies") or in phonograph disks (" phonorecords"), or both.
If a work is prepared over a period of time, the part of the work that is fixed on a particular date constitutes the created work as of that date.
Registration may be made at any time within the life of the copyright. Unlike the law before 1978, when a work has been registered in unpublished form, it is not necessary to make another registration when the work becomes published. Although the copyright owner may register the published edition, if desired.
Poor Man's Copyright.
The practice of sending a copy of your own work to yourself in a sealed envelope or package is often referred to as a "poor man's copyright." There is no provision in the text of international copyright law that recognises this as a reliable alternative to registration. Therefore, the process of placing reliance on the "poor man's copyright" is not a viable substitute for registration.
Song and lyrics Copyrights - Online or by Regular Mail.
To register copyright ownership of all music based original works, please visit our sponsor "Songrite Copyright Office". See how easy and cost effective it is to register the copyright ownership of your songs, music, lyrics, poems etc. The Songrite Copyright office can register the copyrights of all music based intellectual property and all original written and recorded works from single compositions to complete albums.
Learn how to register the copyrights of your songs, music and lyrics
Copyright actually exists the very moment an original song, lyrical work or piece of music is created and fixed in a tangible and accessible form or media such as it being recorded or written down. However, should that work become subject to a dispute or be infringed upon, proof of copyright ownership is not only essential it is also a legal requirement in a court of law.
Proof of copyright ownership in documented form is easily obtained in one fast, efficient and economic transaction with the Songrite Copyright Office.
All composers / authors who register their songs, music and lyrics are issued with an individually numbered copyright certificate plus a song composite document both of which detail the content and the relevant composers of all the registered works including the date of registration.
Songrite Copyright Office Registration
Songrite Copyright Office International Copyright Registration of Songs - Music & Lyrics.
Learn more about Copyright and Related-Rights, Treaties and Laws Copyright Laws & Treaties
To see What Rights Copyright Provides the creator /composer Copyright Rights
How do I obtain Copyright Protection in another country than my own ? Copyrights in Other Countries
What is the term of Copyright and Intellectual Property all about? Intellectual Property
Collective Copyright comprises two main sets of rights: the economic rights and the moral rights. Collective Copyright
Downloading music or movies using peer-to-peer networks can be a temptation. It's easy, it does't cost anything, Copyright and Online Music
Copyright is the means by which a person or a business makes a living from creativity. What is Copyright?
Copyright protection is limited to an author's particular expression of an idea, process, concept, and the like. Authors Expression
Performers are entitled to various rights in their performances, whether these take place on the stage, Performers Rights
Sampling is the use of portions of prior recordings which are incorporated into a new composition Music Sampling
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