general much larger than $\Delta z$.

One Tilted Ring
---------------

The tilting of the ring is completely described by the tilt angle $\theta(t)$, which is the angle between the upward normal to the ring and the $z-$axis, and the azimuthal angle $\varphi(t)$, which is the angle between the line-of-nodes (where the ring intersects the $z=0$ plane) and the $x-$axis. The geometry is shown in Figure 3. The perturbation is assumed to be small in the respect that $\theta^2 \ll 1$. The position vector of a point on the ring is $${\bf R}=\left[~r{\rm cos}\phi,~ r{\rm sin}\phi,~h(\phi,t)~\right]~,
~~0\leq \phi \leq 2\pi~,
\eqno(7)$$ (Cartesian components), where $h(\phi,t)$ is the height of the ring above the $z=0$ plane. We have $$h(\phi,t)=r\theta(t){\rm sin}\left[\phi-\varphi(t)\right]~,$$ $$~~~~~~~~~~~~~~~~=r\theta_x(t){\rm sin}\phi-r\theta_y(t){\rm cos}\phi~,
\eqno(8a)$$ where $$\theta_x(t) \equiv \theta(t){\rm cos}\left[\varphi(t)\right]
\eqno(8b)$$ is the angle of the tilt aboutprograde but are damped by friction for all $\omega_{g12}$. As in the case of an oblate halo (Figure 8), we observe phase-locking for sufficiently large values of $\xi_{12}$.

Frictional torques between two co-rotating rings in a prolate halo also give rise to a negative energy dissipative instability. Such torques could arise from the viscous interaction between adjacent gaseous rings. These frictional torques do not change the total angular momentum of the two rings. Therefore, these frictional torques, if Newtonian (linear) in nature, are [*necessarily*]{} of the form that they contribute terms $$-\left({I_2 \over I_1}\right)^{1\over2}\beta_{12}
\left(\dot\Theta_1-\dot\Theta_2\right)~,
\eqno(51a)$$ $$-\left({I_1 \over I_2}\right)^{1\over2}\beta_{12}
\left(\dot\Theta_2-\dot\Theta_1\right)~,
\eqno(51b)$$ on the right hand sides of equations (42a) and (42b), respectively, where $\beta_{12}$ is the friction coefficient (with units of angular frequency). For a gas with kinematic shear viscosity $\nu$ (with units


adjacent rings.

Two Tilted, Counter-Rotating Rings
-----------------------------------

Here, we consider the case of two tilted rings which are rotating in opposite directions. This situation is pertinent to observed counter-rotating galaxies (see, for example, Jore, Broeils, and Haynes 1996). From equation (44), instability is possible (in the absence of dissipation) only for $\ell_{12}
<0$ in agreement with our discussion of equation (39). Thus, consider ring $2$ to be counter-rotating ($\Omega_2<0$ and $L_2<0$), while ring $1$ is co-rotating. The region of instability is bounded by the two curves $$\omega_{p2}-\omega_{p1}={\Delta_1^2\over 2|\Omega_1|}+
{\Delta_2^2 \over 2|\Omega_2|}$$ $$= \left(-1\pm 2|\ell_{12}|^{1\over2}
-|\ell_{12}|\right)\omega_{g12}~,
\eqno(52)$$ on which the square root in equation (44) is zero. The curves are shown in Figure 10. For parameters in the region between the two curves there is instability, which is seen to occur only for $\Delta_1^2$ and/orsolved to give $\varphi_j(t)$, which is the line-of-nodes angle relative to the $x-$axis.

Comparisons of the temporal responses of $25$ and $49$ ring sytems for different initial conditions show generally good agreement of the warps $\Theta_j$ for the time intervals studied. This indicates that $N=49$ rings gives a valid representation of a continuous disk. However, in contrast with a continuous disk (HT), an $N-$ring disk has $2N$ discrete modes with separate frequencies - $N$ ‘low-frequency’ modes and $N$ ‘high-frequency’ modes. Figure 15 shows the power spectrum of $\theta_{x25}(t)$ for a $49$ ring disk-halo system which is initially given a random perturbation with all radial wavelengths excited and no damping. The frequencies $\omega$ are normalized by the angular velocity of the inner ring $\Omega_1$. Note that $P_1 \equiv 2\pi/\Omega_1 \approx


integrable (HT; Sparke and Casertano 1988). Power spectra obtained for cases with $C_{jk} \rightarrow \gamma C_{jk}$ show that $\omega_1$ increases with $\gamma$ much more slowly than the higher frequency modes which is consistent with the behavior observed in Figures 6 and 12. For the conditions of Figure 15, the magnitude $\omega_1$ is considerably smaller than that predicted for the limit of strong self-gravity between the rings where $\omega_1 \rightarrow
\sum L_j\omega_{pj}/\sum L_j$ \[equation(47)\]. This limiting frequency is the same as the frequency $\omega_t$ of Sparke and Casertano (1988). In any case, the frequency $\omega_1$ is so small (the corresponding period is $>8$ Gyr) that it is irrelevant to the initial value problems considered below.

In the following four subsections we consider different possible origins of warps in an otherwise flat= 10^{10} M_\odot$ in retrograde and prograde orbits. A number of points are observed:

\(1) The warp amplitudes are larger than for the passing satellite (of mass $M_s = 2 \times 10^{10} M_\odot$) discussed in §3.1, but the amplitudes are still smaller than some observed warps (Briggs 1990).

\(2) Coiling in the $\theta(\varphi)$ curves at early times ($t\leq 2$ Gyr) tends to disappear at later times ($t \geq4$ Gyr). We believe but have not proven that this is due to the phase-mixing of the fast precession modes which propagate over the radial extent of the disk in times $< 4$ Gyr (see also §3.1).

\(3) For both the retrograde and prograde cases $\theta(\varphi)$ exhibits a leading spiral wave for $t \geq 4$ Gyr qualitatively of the form observed for M 83


t}\bigg)^2+
\Delta^2 h^2 \bigg]$$ $$+{G\over 2}\int_0^\infty dr~r^2~\Sigma
\int_0^\infty dr'~(r')^2~\Sigma'\int_0^{2\pi} d\phi~ \times$$ $$J(r,r')\left[{h(r',\phi,t)\over r'}-
{h(r,\phi,t)\over r}\right]^2~,
\eqno(70)$$ where $J(r,r')$ is given by equation (30b). Substituting $h(r,\phi,t)=r\theta(t){\rm sin}[\phi-\varphi(t)]$ from equation (8a), one readily finds that ${\cal E}_{warp}$ is identical to ${\cal E}_{rings}={\cal H}$ of equation (53b). Note that ${\cal E}_{warp}$ is non-negative and therefore the disk is stable if $\Delta^2(r) \geq 0$.

Including the dissipation terms (68) and (69) gives $${d {\cal E}_{warp} \over dt}=
-2\int d^2r~\beta~ \Sigma
\left({\partial h \over \partial t}\right)^2$$ $$-~2\int d^2r~ \nu_t~ \Sigma
\left[r{\partial \over \partial r}
\bigg({1 \over r} {\partial h \over
\partial t} \bigg) \right]^2~.
\eqno(71)$$ The relative friction is of course zero if $h/r$ is a function only of time which corresponds to a rigid tilt.

The second constant of the motion ${\cal P}_{rings}$, found in §2.1 and §3 \[equation (53c)\], caninteraction between the two rings is appropriately measured by the coupling strength $\xi_{12}$ of equation (48). As $\xi_{12}$ increases the ring motion changes from that of independent precession for $\xi_{12} < 1$ to phase-locked precession for $\xi_{12}>1$ where the lines-of-nodes coincide approximately, $\varphi_1 \approx \varphi_2$. This phase-locking persists for the case of $N>2$ rings.

We examine the influence of dissipative forces on the tilting motion of two rings. In addition to dynamical friction, which is included as linear drag torques on each ring, we include the ‘relative’ friction which can result from the differential vertical motions of two gaseous rings due to turbulent viscosity. The corresponding drag torques on each ring have a definite form owing to the requirement that the total angular momentum of the two rings be


equatins of motion for $\Theta_j=
\theta_j{\rm exp}(-i\varphi_j)$ for $j=1,..,N$. The Lagrangian has the form ${\cal L}=
{\cal L}(\theta_j, \varphi_j, \dot \theta_j,
\dot \varphi_j)$, and this gives, in the absence of dissipative torques, both an energy constant of the motion and a total canonical angular momentum constant of the motion, $P_\varphi = {\sum }_j \partial {\cal L}/\partial
\dot \varphi_j =$ Const. We comment on the numerical solutions for $\Theta_j$ for different values of $N$, and we give a sample power spectrum for $N=49$ which shows the distribution of the $2N$ mode frequencies. We argue that for treatment of intial value problems of time duration $t_{max}$, mode frequency differences $\delta \omega$ smaller than $1/t_{max}$ are irrelevant. This leads to the estimate $N = {\cal O}(10^2)$ for the number of rings needed to treat warpshave gone to the trouble of separating their waste for recycling.'

Warwick District Council yesterday apologised for the blunder.

Contract services manager Rob Hoof said: 'We are sorry Mr Harlow has experienced problems with the service.

'Contractors are expected to be practical about what they leave and what they take.

'Where they do not take a reasonable approach, that can be justified by the customer, we will always send them back to collect the items.'

A spokesman for the council added: 'The call centre officer who took Mr Harlow's call was incorrect in stating that "maggots were classed as livestock".

'We have spoken with Mr Harlow and have offered to have the contractors return to his address to make the collection for him.

'We have also reminded our Contact Centre staff and contractors of the


one of the campaign's sunny video spots, replete with leafy greens and happy children. "Join me and teachers across Oregon and say, 'Yes, keep our groceries tax free.'"

But behind those cheery ads is something deeper — a long fight between organized labor and business groups over how corporations in Oregon should be taxed. That's a fight that might take center stage in 2019, when the Oregon Legislature is expected to consider new taxes.

Shoppers stock up on supplies at New Seasons in Southeast Portland's Sellwood neighborhood, Feb. 20, 2018 as a snowstorm moves into the city. John Rosman / OPB

Now, the labor group preparing to oppose IP 37 thinks it’s got a winning message of its own: that the supposed grocery-tax ban could have far murkier implications.

"We certainly planmajority of eateries.

The AG’s office also notes the measure would wall off entities that deal in “groceries” from any increase or decrease to Oregon’s oft-criticized corporate minimum tax, one of the state’s primary means of taxing businesses.

“The state corporate minimum tax … potentially applies to all corporations that sell, distribute, purchase, or receive groceries throughout the state,” the office wrote in December. The measure would have no impact on Oregon’s business income tax, which some companies must pay in lieu of the minimum tax.

Berman’s memo to Our Oregon suggests the effects would go further.

For instance, he writes the proposal could affect implementation of Measure 101, which Oregon voters passed in January. That measure approved a tax on hospitals that was crucial for closing a hole in the state


This project seeks to define the interactions between two major inputs to the myenteric cholinergic neurons, namely the neurokininergic (NK) and serotoninergic (5-HT) neurons of the guinea pig small intestine. Since both excitatory and inhibitory signals can be conveyed to the cholinergic neurons, we have four main objectives: (1) To examine how different agonists for NK and 5-HT receptors modulate the release of acetylcholine (ACh) from the myenteric cholinergic neurons. There is evidence to suggest a functional coupling between NK and 5-HT receptors on cholinergic neurons. We will determine if this interplay is restricted to any specific receptor subtype, or if it is mediated by a release of 5-HT evoked by NK, or if the action of NK on the cholinergic neurons is dependent on a subthreshold level  var total = 0;
    do {
      total = total + parseInt(prompt("Penilaian Responden " + i + " :"), 10);
      i++;
    }

    while (i < nt);

    var rata = parseInt(total / n);
    alert('Maka nilai MOS rata-ratanya nilai ' + rata);
</script>


/*
 * Copyright (c) 2005, 2013, Oracle and/or its affiliates. All rights reserved.
 * DO NOT ALTER OR REMOVE COPYRIGHT NOTICES OR THIS FILE HEADER.
 *
 * This code is free software; you can redistribute it and/or modify it
 * under the terms of the GNU General Public License version 2 only, as
 * published by the Free Software Foundation.  Oracle designates this
 * particular file as subject to the "Classpath" exception as provided
 * by Oracle in the LICENSE file that accompanied this code.
 *
 * This code is distributed in the hope that it will be useful, but WITHOUT
 * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or
 * FITNESS FOR A PARTICULAR PURPOSE.  See the GNU General Public License
 * versionevery 2 weeks or so in one of my 3 submarines for the last 4 years with 3 different tanks. I have used it with both 40Mhz and 433/458 Mhz r/c equipment as developed by Tim Senecal. It works with both but the lack of interference on 433/458 makes the piston tank work more smoothly.

The software is made available under an open license for people to use and modify as they wish on the basis that their software continues to be available to others. So it is not for commercial gain.

The software is written in assembler for a PIC micro.

An Arduino version written in C would be very welcome!

The mechanical construction of piston tanks is covered elsewhere in the AMS Forum but some tips include:

- threaded M5 stainless


statistically, yeah, absolutely the first and second downs lead to long third downs and long third downs," Patriots quarterback Tom Brady said Wednesday. "Nobody's good in third-and-eight-plus in the NFL. It's a passing down, the coverage is too tight, the rush is too good. If you make one or two of those per game it's usually pretty good for an offense."

Brady raises a solid point. Some of the Patriots' third-down struggles are undoubtedly tied to what has happened on early downs. The running game, in particular, has put them in long-yardage situations.

Over the past four games, all without Dion Lewis, 45.4 percent of the Patriots' rushing attempts have gone for two yards or less. See the numbers below.

Through Week 9

Dion Lewis: 14 of 49 carries (28.6 percent) wentIntroduction
============

Enzymes play a vital role in cellular activities. Apurinic/apyrimidinic endonuclease 1 (APE1) is a multifunctional enzyme involved in the base excision repair (BER) pathway, which accurately removes damaged bases and guarantees genomic integrity.[@cit1] APE1 is a prerequisite for the repair of DNA damage in both the short-patch and long-patch pathways of BER, although each pathway employs different enzymes to complete repair subsequent to APE1-mediated cleavage.[@cit2] APE1 is responsible for \>95% of apurinic/apyrimidinic (AP) site processing in mammalian cells.[@cit3] APE1 is also involved in the regulation of transcription as well as RNA transcription/modulation. Dysregulation of APE1 has been demonstrated to be associated with a couple of diseases such as cancer,[@cit4] neurodegenerative diseases[@cit5] and cardiovascular disorders.[@cit6] Abnormal expression and subcellular distribution of APE1 have been linked to tumor metastasis.[@cit7] From


an invader strand to initiate strand displacement to switch the AP site from the scaffold to the antenna. Step2: input 2 as an invader strand to neutralize input 1 to re-locate the AP site. The duplex of the two inputs is the waste. (B) Fluorescence signals of different structures reacting with APE1, the original tetrahedron (blue), the structure after the first-step strand displacement (orange), and the structure after the second-step strand displacement (green). The enzyme activity was measured in 40 min allowing the completion of strand displacement. The concentration of the inputs and tetrahedron is 100 nM, and that of APE1 is 0.16 nM.](c9sc01912j-f3){#fig3}

Highly sensitive and specific APE1 detection by the OUT-tetrahedron
-------------------------------------------------------------------

Based on the above results, the OUT-tetrahedron is a promising probe to quantify the APE1 activity. TheThere are unofficial reports of two students shot by police this afternoon at a student demonstration in the centre of Bo.

The students have been named as Mohammed Morlu and Augusta Sungai.

One of them is believed dead, and the other has been taken to hospital with serious injury.

Thirteen students are now believed to be detained at Lumley police station in the west of the capital Freetown; three detained at New England Ville Police Station; and five detained at Kenema Police station.

Some of the student leaders are reported to be meeting the president at State House for talks.

Reports from the southern district of Bo say that the town is today under siege.

Students from Njala University have taken to the streets in sympathy protest, after lecturers are denied payment of their


What happened to the money is anyone’s guess. But rumor has it that the contract was awarded to one of the relatives of the President, however, going ten years into his presidency the renovation has yet to be completed.

The students who have sacrificed so much are still looking forward to the day when they will be able to return to the Hostels. The student union which was once the voice of the student body, has been infiltrated by the APC party and politicized.

And to top this off, I have heard that part of the reason why this APC government is not too enthusiastic to complete the work on the Hostels is to keep the students from organizing and demanding better conditions.

As for Njala University, their relocation to Freetownthat he has failed and can no longer manage the country? This is pure nonsense.

The government of salone is not being truthful these days. That’s why Emerson Say’s “yesterday is better than today”. We are electing fools to rule us. But all the same, they have charmed us. Ar know say e go lef buff pan dem (in other words – it will be there loss).

WITH CORRUPTION EVERYONE PAYS

Sierra Leone Telegraph: 12 April 2018: After much anticipation from the people of Sierra Leone, and criticisms too for delaying the appointment of his cabinet ministers, president Julius Maada Bio has today announced his first [Read More]

Sierra Leone Telegraph: 18 August 2017 This article was first published by the Sierra Leone Telegraph exactly five years ago, on the 16th of


adeleshiffman

Car would not start, turned over and over and over, but never started. After 2 days in the garage the mechanic got a code for crank sensor. The car started over and over for the mechanic except around 4:00 p.m. He requested a different ignition key and it started. Does it need a crank sensor?really concerned after this game. They had zero idea of what to do on offense. When I was watching I saw nothing but bad shot after bad shot. The best Gopher I saw last night was freakin' Hoffarber. It was nice to see him come into his own a bit, with 12 points on 5-9 shooting and gain some confidence. Of course, I also saw him completely lose his man on defense, leading to a FSU layup, and be in perfect position for a rebound only to have a more athletic Seminole swoop in and grab the O-board - so there's still that to work on.

The Gophers put the ball up 71 times, compared to only 52 from FSU, but due to FSU's 27 made free throws to


to determine the exact cause of
death of one of the few Griffon vultures on the island whose carcass was found
at Zapalo beach in Episkopi, Limassol.

Conservation group BirdLife
Cyprus said an x-ray showed the presence of pellets but a necropsy was also
underway to confirm whether it was a shooting that killed the bird or if it
died of poisoning, the most frequent cause of death of vultures in Cyprus.

BirdLife said preliminary tests
showed the bird most probably died from the shooting but more tests were
underway to check for evidence of poisoning.

“This x-ray alone, however,
paints a gloomy picture for the species,” BirdLife said. “Why was it even shot
at? With only around 20 vultures left on the island, each death comes at a
great cost for the species’ survival.”

“Although it is early days for
the chickcan vote in the April referendum, which could give Mr Erdogan new powers over the budget and the appointment of ministers and judges, as well as the power to dismiss parliament.

Waning EU hopes

On Monday Mr Erdogan stepped up a week of anti-German rhetoric by accusing Chancellor Angela Merkel of "supporting terrorists".

Her spokesman described the jibe as "clearly absurd".

He also accused Germany of "Nazi practices" for blocking his ministers from speaking in Germany.

Senior German officials have cast doubt on Turkey's chances of joining the EU, as it continues to claim it is being treated unfairly by countries in western Europe.

In an interview published by Hamburg weekly Der Spiegel, Germany's foreign minister suggested that the most Turkey can hope for is to one day achieve a "privileged partnership" with the


Manchester United’s pursuit of Arturo Vidal may have hit a stumbling block after sources revealed it would take a bid of €56 million for Juventus to consider selling the midfielder.

Vidal has been on United’s radar for a long time, as they enquired about his availability last summer when David Moyes was in charge and again in January.

Vidal is thought to be open to the idea of a move, however, sources indicate that Juventus would remain extremely reluctant to sell one of their star performers even if the asking price is met, but would want a minimum of €56m, ESPN revealed.

Manchester United have spent €75m in the last week as their extensive recruitment programme gather apace and they now have their sights set on what they believe to beThe tools are designed to externally (i.e., external to a patient) couple with a magnet of the adjustable valve such that upon coupling, the setting of the valve may be determined and the valve magnet may be deliberately manipulated to thereby adjust the pressure setting of the valve without removal of the subcutaneously implanted device. Indicator and adjustment tools thus rely on magnetic coupling of the tool to the adjustable valve, where the magnetic coupling is strong enough to determine or to adjust the position of the valve magnet even through tissue (e.g., a patient's scalp). Examples of locator, indicator and adjustment tools are shown, for example, in U.S. Patent Application Publication No. 2002/0022793 (hereinafter, “the '793 application”) to Bertrand et al. entitled, “Tool for Adjusting an Implantable


implanted valve such that the valve magnet or magnets align and/or couple with the magnetized tool elements or magnets. However, the magnetized element of an indicator tool may tend toward alignment with the earth's magnetic field if the pull of the magnet in the implanted valve is not sufficiently strong (such as when the distance between the implanted valve magnet or magnets and the tool increases) and could lead to inaccurate device setting determinations or indications.
In addition, magnetic components of the adjustable valve itself may be susceptible to movement or inadvertent setting adjustment by strong nearby magnetic fields since the internal magnetic elements of a valve may tend to align with an external field. An adjustable valve might therefore be unintentionally adjusted when in the presence of astrong external magnetic field, such as encountered in a magnetic resonance imaging (MRI) procedure. Thus, some fluid flow control devices include features which provide increased resistance to inadvertent setting changes. For example, mechanical “stops” or magnet configurations designed to resist strong nearby magnetic fields may be incorporated into a device such as disclosed, for example, in U.S. patent application Ser. No. 13/804,875, referred to above. Deliberate adjustment of these types of valves, in some cases, may be more difficult to achieve without an accurate alignment of the adjustment tool to the valve magnet.
In order to accurately magnetically align or couple a tool to an implanted valve (for example, to avoid effects of the earth's magnetic field on the tool or to ensure a sufficient coupling of a tool


changelog (for developer use only, include unreleased versions)

0.5.60
****** Embed the default snippet in Fingertext

0.5.59
****** The symbol "-" is allowed in triggertext.
****** only () is used to wrap parameters

0.5.58
****** Added: Download Fingertext Sample Snippets
- The last hotspot problem works for diaglog insertion too
- The "delete all snippet" command backup snippets automatically without asking
- default hotkey for insertion dialog changed to alt+/
- Ask about overwriting option only when you have snippets in your database

0.5.57.2
- restrict the addition of $[0[]0] to snippet with no hotspot and it's inserted to a document with no hotspot following the insertion

0.5.57.1
- Try to fix the final hotspot problem without an extra $[0[]0]

0.5.57
- Fixed: error in finding previous hotspot when the hotspot is located at the beginning of the document
- Fixed: error causing fingertext dothe triggertext

0.5.28
- Changed: change hotspot (cmd) to (run)
- Fixed: the problem of appending cmd /c will break some commands
- Fixed: Lang:PHP not working
- upgrade to sqlite3.7.7.1

0.5.27
- Changed: merge in jvdanilo's implementation of executecommand

0.5.26
- upgrade to sqlite3.7.6.3

0.5.25
****** Added: private snippet available, any snippet with triggertext beginning with _ cannot be triggered and will not be shown in liveupdate. But you can still see them in editMode and they can be triggered by chain snippets
- snippet triggertext completion are default to be non-inclusive
- Big performance improvement by using direct scintilla method
- Fixed: Buffer changed triggered events (like updateMode) not triggering when use attempt to close npp and cancel afterwards
- turn off live update when selection is rectangle to prevent freeze when selecting multiple line and type
- Change default snippet list


critical bug when live update is on and a long chain of chinese characters are typed

0.5.10
- Added: Language based snippets (cannot be triggered yet. basic code in the background)
- Added: Custom Scope, a user defined Global scope
- rewriting the triggerTag, snippetComplete and findTagSQLite functions
- edit mode detect full file name before changing mode
- "List of All Snippet" is now on static text

0.5.9
- Added: Option to make triggertext completion less inclusive
- Fixed: bug in importing snippets with different endline characters.
- Fixed: unknown exception and bad allocation in import snippet function
- Added: Close the temp file and Prompt to close the ftb file before import
- Fixed: A temporary fix for cmd line error

0.5.8
- Added: generation of conflict copy instead of overwrite
- Allow for underscore and period in triggertext
- fixed: creating<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.01 Transitional//EN" "http://www.w3.org/TR/html4/loose.dtd">

<title>DbKey.LinkKey</title>
<meta name="date" content="2018-10-07">
<link rel="stylesheet" type="text/css" href="../../stylesheet.css" title="Style">

JavaScript is disabled on your browser.

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said upper limit in said output current.
The seventh aspect of the invention is directed to the power supply device according to the fifth aspect, wherein
said measuring circuit prolongs the period of connecting said first and second secondary windings in parallel by controlling said phases of said first and second current supply circuits upon detecting any increase exceeding a predetermined upper limit in said output current, and shortens the period of connecting said first and second secondary windings in parallel by controlling said phases of said first and second current supply circuits upon detecting any decrease from said upper limit in said output current.
The eighth aspect of the present invention is directed to the power supply device according to the fifth aspect, wherein said first and second current supplyThen after you have your Action object returned by Action.createFromString you call its perform()
onPostExecute(String result) {
   Action a = Action.actionForResult(result);
   a.perform();
}

abstract class Action {
  abstract void perform();

  static Action actionForResult(String result) {
      if(result.equals("res1") {
          return new ActionForRes1();
      } else if(result.equals("res2") {
          return new ActionForRes2();
      } else throw new IllegalArgumentException("No action for result " + result);
   }
}

class ActionForResult1 extends Action {
  @Override
  void perform() { Log.i("ACTION", "Here's action for result 1"); }
}

class ActionForResult2 extends Action {
  @Override
  void perform() { Log.i("ACTION", "Here's action for


the biogeography of infectious diseases occurs where these fields become spatially explicit. Macroecology deals with ecological questions that demand large‐scale analysis (Brown 1995, Brown and Lomolino 1998, Cox et al. 2016). The limits between biogeography and macroecology are fuzzy. They converge when biogeography is focused on the study of how population‐ or community‐level parameters vary along geographic dimensions (Lomolino et al. 2006), or when macroecology deals with spatial patterns (e.g. the geographic distribution of a certain pathogen species or diversity patterns). The divergence occurs when spatially explicit components are not crucial to answering questions being addressed by macroecology (Blackburn and Gaston 2006), and when biogeography does not invoke structural and functional patterns of ecological systems (e.g. areography and some evolutionary biogeography approaches) (Morrone 2009). By contrast, community ecologyspatial resolution possible (i.e. GPS coordinate locations).Temporal coverage: infected hosts including humans may travel long distances during disease incubation periods, introducing uncertainty in the attribution of the geographic location of infection (Peterson 2014). Surveillance and sampling strategies should thus allow the capture of appropriate temporal scales (i.e. matching scale of disease‐relevant processes) so that data can be better aligned with covariate information such as environmental variables and human activities.Phenology: animal and plant phenology should be monitored; the behavior and biology of most species, including humans, are influenced by often relatively predictable annual changes in climate that determine when they start or finish natural events, such as flowering and fruiting, breeding and mass gatherings. Many of these activities and departures from norms due to, for example, unusual weather events


Introduction {#s1}
============

Aorto-left ventricular tunnel (ALVT) is an extremely rare defect (0.001 to 0.1% of all congenital heart defects with a male predominance) ([@B1], [@B2]). This abnormal paravalvular extracardiac communication between the ascending aorta and the left ventricle was first reported in an infant by Levy et al. ([@B3]).

Age of diagnosis and symptoms depend on the size of the ALVT, the severity of the aortic regurgitation caused by the defect, and the associated lesions. Overall, patients with ALVT are operated once the diagnosis is established given the risk of cardiac failure related with the shunt and the aortic insufficiency ([@B4]).

Fetal diagnosis of ALVT was first reported in 1995 in an autopsy study ([@B1]). Despite the recent improvement in routine ultrasound screening, prenatal diagnosis is still challenging and rare. Moreover,in the previous series, only a few newborns antenatally detected have survived whatever the performed postnatal cares ([@B5]--[@B18]).

Aortic origin of tunnel may be situated anywhere above the aortic sinus. The size and the shape of ALVT are variable (a large tubular, or saccular, protuberance on the anterior aspect of the aortic root). The tunnel ventricular orifice opens into the left ventricular cavity as in the majority of cases at the level of the fibrous triangle (90%) ([@B4]). While etiology of aorto-ventricular tunnel is unknown, the onset, severity, and progression of heart failure is, however, quite variable, and ranges from asymptomatic compensation to severe cardiac failure, sudden death, or even death in utero. This spectrum may reflect variable according to associated malformations ([@B2]).

We report the case of a fetus


3 of life. The aortic valve was found bicuspid including a postero-right leaflet, an antero-left leaflet, and a median raphe. The tunnel aortic orifice was localized above and left the right coronary ostium, close to the raphe. By median sternotomy under cardiopulmonary bypass, the ALVT was closed only on its aortic end using a heterologous pericardial patch avoiding distortion of the aortic cusps. The post-operative course was uneventful and the infant was discharged at day 8. The follow-up at 2 years demonstrated a positive outcome without any required treatment. There was no residual ALVT shunt but the aortic valve remained thick with mild regurgitation. The function of the left ventricle was completely normalized ([Figure 1F](#F1){ref-type="fig"}).

Discussion {#s3}
==========

ALVT anatomy in our case was consistent with most of those previously published.currently flowing into the Upper Midwest comes largely from Mexican cartels.

Minnesota Department of Public Safety gang and drug coordinator Brian Marquart said that around 2007, cartels figured out a way to mass produce high-quality methamphetamine.

That accounts for some of “the massive influx of methamphetamine we’re seeing across the country, including in North Dakota and Minnesota,” he said.

User-quantity level methamphetamine now ranges from 70 to 80 percent pure, Marquart said. In the early 2000s when local small-batch meth labs were more common, the quality of the product was high, but the quantity was relatively low.

“Now we are seeing very high quality, into the 80th percentile at the user level,” he said.

“A few years ago, a large seizure coming into this state would have been 3 to 5 pounds,” Marquart


said. “Now we are seeing seizures of 30, 50, 70, even 100 pounds of methamphetamine either coming into this state or bound for Minnesota and North Dakota.” Related Articles St. Paul PD highlights surveillance photos of looting suspects, seeks tips

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The user base in the region is very high now, Marquart said. Both states are seeing higher numbers of people seeking treatment.

“Methamphetamine crosses all socioeconomic boundaries,” Marquart said.

Meth at the street level is typically purchased in grams, with dosage ratesTwin Cities, the drug is distributed throughout the state and into neighboring states.

RELATED: Minnesota Patrol adds three more K-9s to sniff out drugs

Minnesota’s violent crime task forces prioritize targeting mid- to upper-level dealers operating in the state in an attempt to disrupt the flow of meth in the region.

“We continue to work with our partners for treatment and education,” Marquart said. “We can’t do this alone. We need the public’s help.”

While arrests and confiscations of methamphetamine continue to rise, so have admissions to addiction treatment centers for people battling dependency.

“What we are seeing in the data is alarming,” Minnesota Department of Human Services Commissioner Emily Piper said in a release. “Methamphetamine use is now second only to alcohol for treatment admissions in Minnesota. The good news is: Treatment


key aspects of the participants' decision-making process were controlled via instructions that guided them through the steps of deciding, thus ensuring that all participants used the same decision-making tools. Observing, once again, a strong relationship between the level of depressive symptoms and the productivity of decisions would suggest that the poorer choices of depressed persons are due to aspects of decision-making other than poor decision strategies. Alternatively, if no relationship is found between depressive symptoms and productivity of decisions, the hypothesis that the lack of sound decision-making strategies is responsible for the poor decisions of those with more depressive symptoms would receive support. As a further test of these hypotheses, we evaluated whether individual differences in decision-relevant goals could be explained by variations in depressive symptom levels.

Methods {#Sec11}
-------

###Study 1 and Study 2 were combined for a quasi-experimental joint analysis. To show the difference between the association of depression and productivity between the two studies, regression slopes of productivity as a function of BDI scores for the two studies were compared. A significant interaction of the BDI scores and Study in predicting productivity would indicate a difference between the regression slopes obtained in Study 1 and that of Study 2. The results of a regression model indeed revealed a significant interaction of BDI scores and Study in predicting productivity, *t*(230) = 3.16, *P* \< .002, *R*^2^ = .27, *F*(3, 230) = 28.19, *P* \< .0001 (Fig. [1](#Fig1){ref-type="fig"}). Simple slope analyses revealed that the slope was significant for the sample in Study 1 (*β* = −.03, *t*(230) = −7.99, *P* \< 0.001), but not significant for the sample in Study 2 (*β* = −.01, *t*(230) = −1.78, *P* \< .08).


the studies differed in the average level of depression reported by participants. Furthermore, although the analysis in which data from the two studies were combined into one dataset treated the studies as two conditions in an experiment, it was quasi-experimental. Any conclusions drawn from the comparisons between the two samples should therefore be interpreted with caution. Although the raters were blind to the participant's depression status, and every effort was made to keep the ratings unbiased, aided by the manualized rating guides, it is possible that the depression status of participants could have been revealed through either the emotional tone of the response or through participants' inadvertent comments. However, this limitation would concern only the results of Study 1, with its significant relationships between depression scores and decision-relatedmakes the same mistake that secular liberalism makes when it comes to homosexuality: They simplify and trivialize it. For “gay-affirming” secularism, homosexuality is banal, about as interesting as a preference for redheads or a love of spicy food. (This perspective requires the obviously -false corollary that men and women are not merely equal but interchangeable, thus love of a woman is exactly like love of a man in every relevant aspect.)

And for most orthodox Catholic moralists, homosexuality is merely the desire for a set of prohibited sexual acts. It is “intrinsically disordered” because it is –and is defined by–the desire for forbidden actions. But the tangle of experiences we’ve decided to call “being gay” is much more complex than that, which is good news for all gay Catholics


about OpenGL options for running your game? As I often use them instead of DX when problems arise trying to run a game.

Contributing:I'd love to!, but alas I still can't run the game - so I'd only be able to help with design/concepts and content/assets like models and textures, but I wouldn't be able to play the game with what I make! :(Oh, well - you can't always have a cake AND eat it! :P

BTW: I was going to put that last paragraph in the comments on the MWFD page but it requires creating a new facebook account, and logging into my yahoo account from your site doesn't seem too kosher either - especially when I was already logged in to my yahoo email account.

Shouldn't that be; 'theNeutrophil aggregation is beta 2-integrin- and L-selectin-dependent in blood and isolated cells.
Neutrophil aggregation in response to formyl peptide was analyzed in blood and isolated cells by fluorescence flow cytometry. The isolated leukocyte aggregates and the leukocytes in blood were identified with the vital nucleic acid stain LDS-751. This method enabled us to discriminate nucleated cells from other blood cells and to detect granulocyte aggregates without isolation or E lysis. Cells isolated in the absence of endotoxin retained the characteristics of cells in blood and exhibited similar aggregation kinetics and dose-response to formyl peptide. We show that it is possible to analyze epitope expression in blood with homogeneous flow cytometric assays and that carefully isolated neutrophils retain the expression characteristics of those in blood. The expression of CD18 was


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Badminton in Central Coast NSW

Is the game still on? I'm thinking of joining.... Just moved up here and looking for new group to play with.

.

Yes, it is still on, Monday nights around 7:30 pm.
Also on Friday at about the same time.

If you don't mind traveling, Badminton can also be found at Hornsby (outer North: Sydney) and Newcastle.

I don't like Hornsby because IMO they are snooty and unfriendly. The light is not so good in their hall.

I find Newcastle is the best because theyresponses ([@r15]), and boost nationalism and patriotism ([@r28]). Linguistic studies of on-line journals after the September 11^th^ attacks point to increased social references immediately after the collective trauma occurred ([@r8]). On the other hand, it is obvious that such traumatic events often lead to deep societal divides and intragroup conflicts -- particularly when they occur in the political domain. The crash of the airplane carrying the Rwandan president Juvenal Habyarimana and the Burundian president Cyprien Ntaryamira led to the Rwandan Genocide and a violent war in the Democratic Republic Congo. The September 11^th^ attacks in the USA enhanced decades-long partisan conflict between Democrats and Republicans. The massacre in the Beslan school in 2004 escalated Ingush-Ossetian hostilities and led to human rights abuses in Russia. This societal process, known


all across the country are in great need of support from universities that may not understand what they are trying to accomplish,” said Jack Callahan, a University of Colorado Boulder student-leader, and PACG Co-Commissioner. “PACG hopes to push those organizations towards supporting their local esports clubs and maybe move towards varsity programs.”

PACG is not supposed to be a permanent solution. “It’s a political movement for students to say they are not getting what they need,” Dimick says. “We hope in five years that esports has a role in mainstream athletics and it’s one of the sports college campuses invest into and have live events for and have huge audiences for. We hope to elevate college esports to a mainstream part of college campus life.”

What remains to be seenhalf. And we are closing very fast and now that Wyoming is behind us, we are here in New York state. I have been pleased to sense a great deal of momentum... No question in my mind, we have the momentum."

Watch:

Earlier:

SCROLL TO CONTINUE WITH CONTENT Never Miss a Beat. Get our best delivered to your inbox.

A possible record turnout was expected in Wyoming on Saturday as voters caucused in the U.S. presidential election, with 14 pledged delegates and four superdelegates available for Democratic rivals Bernie Sanders and Hillary Clinton.

The numbers are not likely to determine the race one way or another, but the Sanders campaign is hoping a win in the state will keep up the momentum he built winning a handful of recent primaries—including a critical contest


in Wisconsin last Tuesday.

Winning the Cowboy State would give Sanders his eighth win in a row, just in time for the high-profile New York primary and upcoming debate with Clinton.

"If you want to talk about math, the truth is that it is very, very, very unlikely either candidate, either Secretary Clinton or Sen. Sanders, will go into the convention with a majority needed of pledged delegates in order to win," Sanders campaign manager Jeff Weaver said in a CNN interview last week.

Wyoming Democratic Party executive director Aimee Van Cleave said regardless of the outcome, the excitement of the race has re-energized Democrats in the Republican-heavy state. "The only word I can use to describe being a Democrat in Wyoming is electrifying," she said.

Politico has the live election results         5
     Except as otherwise provided in this article, every
     parent, guardian, or other person in the Commonwealth
     having control or charge of any child who will have
     reached the fifth birthday on or before September 30
     of any school year and who has not passed the
     eighteenth birthday shall, during the period of each
     year the public schools are in session and for the
     same number of days and hours per day as the public
     schools, send such child to a public school


phrase."   Commonwealth

Natural Resources, Inc. v. Commonwealth, 219 Va. 529, 536, 248

S.E.2d 791, 795 (1978).   "[S]tatutes are not to be considered

as isolated fragments of law, but as a whole, or as parts of a

great connected, homogenous system, or a single and complete

statutory arrangement."   Prillaman v. Commonwealth, 199 Va.

401, 405, 100 S.E.2d 4, 7 (1957) (quoting 50 Am. Jur.,

Statutes, § 349).   "[E]very part of a statute is presumed to

have some effect and no part will be considered meaningless

unless absolutely necessary."   Hubbard v. Henrico Ltd.

Partnership, 255 Va. 335, 340, 497 S.E.2d 335, 338 (1998).

     Where multiple sections of a statute are inconsistent or

ambiguous when read together, courts "are required to harmonize

any ambiguity or inconsistency in the statuteto give effect to

                                 8
the General Assembly's intent without usurping 'the

legislature's right to write statutes.'"   Parker v. Warren, 273

Va. 20, 24, 639 S.E.2d 179, 181 (2007) (quoting Boynton, 271

Va. at 229-30, 623 S.E.2d at 927).

     Code § 22.1-254 is the opening section of Title 22.1,

Chapter 14, Article 1.   Code § 22.1-254(A) itself has a number

of primary features that deal specifically with mandatory

enrollment:   it addresses the span of ages during which school

enrollment is required and the various permissible forms of

education (private, denominational, parochial, home

instruction, and approved alternative


absences:     because the statute refers to days and hours per

day in the same sentence, it must be read to apply to both or

neither.   Thus, in concluding that Code § 22.1-254(A) does not

apply to absences, we must likewise conclude that it does not

apply to tardiness.

     Finally, interpreting "send" to encompass tardiness would

entail construing Code § 22.1-254 as blanket authority for

prosecution of parents for even de minimis tardiness or absence

on the part of their children.     This result seems contrary to

the comprehensive and graduated approach to absences found

elsewhere in the Code.     Given the obvious attention to detail

and structured guidance that the General Assembly has provided

through other attendance- and truancy-related sections, we find

it highlyor

direct volition.”   Webster’s Third New International Dictionary

2065 (1983); see id. at 17a (stating in explanatory note 12.5

that “[t]he order of [meanings] is historical: the one known to

have been first used in English is entered first.”).    Thus,

“send” means more than “enroll.”

     Indeed, the General Assembly chose to use “enroll”

elsewhere in this article when it wanted to limit the

obligations of parents and educators to issues of mere

enrollment.   See Code § 22.1-260 (imposing a duty upon a

principal to report to the superintendent all students enrolled

and, to the extent he or she is able to, not enrolled within

ten days of the start of each school year); Code § 22.1-261

(requiring the attendance officer or division superintendent to

compose a list of all unenrolled


knowing and willful, the Commonwealth alleged that

the violation was knowing and willful, and Blake was so

arraigned.

             It is true that a variance between the
             allegations of an indictment and proof of
             the crime may be “fatal”, Etheridge v.
             Commonwealth, 210 Va. 328, 171 S.E.2d 190
             (1969), and “[t]he offense as charged must
             be proved.” Mitchell v.to “what points [appellant]’s counsel

                                27
          intends to ask a reversal of the judgment
          or decree” and prevents them from having to
          “hunt through the record for every
          conceivable error which the court below may
          have committed.”

Id. at 116, 752 S.E.2d at 871 (quoting First Nat’l Bank of

Richmond v. William R. Trigg


Co., 106 Va. 327, 341, 56 S.E.

158, 163 (1907).   Blake made a very general challenge to the

sufficiency of the evidence and never mentioned the

constitutionality of the statute in her assignments of error.

Although she filed a motion to amend her assignments of error

to insert a specific reference to the constitutionality of the

statute, the Court of Appeals denied that motion and she did

not assign error to that ruling on the present appeal.

Therefore, Blake has waived her challenges based on inadequacy

of notice and the asserted unconstitutionality of the statute

on vagueness grounds.

     Thus, for the above-stated reasons, I would affirm Blake’s

convictions.

                         tunes hanging around. Of note, friend of the blog ap0c recently took first in the YM2612 category for his track ‘Vitriol Hammer’ on their 11th Winter Chip battle. Despite what it sounds like right at the start, this isn’t an a-Ha cover – but if you’re familiar with with ap0c’s style, his love of dark sounding pieces with strong basslines and fun with pitch bends, you’ll love this track.

TELEFUTURE

I’d be willing to wager that few, if any, groups have done more to keep music on the Genesis alive than Telefuture: You may remember their commissioning of well known visualist Batsly Adams to produce a Genesis cartridge with selected tracks from Eternalist (including some secret tracks which may never be heard again, according to Mr. Adams himself), but several


Finally admitted defeat

Having successfully photographed weddings etc since 1969 both on film and digital I dont really see myself as a snapshooter with too much money.

I did not consider that possibility until your next statement, and agree it is probably out of line. However, your statements seem out of line also. Thus explaining the attitude of the response.

However I do think that a D700 should be capable of rendering a grooms suit as black rather than very dark blue straight from the box.

BLACK refers to so many differing colors making the white balance critical and difficult to nail. REMEMBER The Film you just mentioned??? Every single frame needed correction [I assume you did not shoot slides for weddings]. Yet, you insist digital should get every shot correct. Totend to select as SF massive galaxies with low (but detectable) SFR will return a flatter MS compared to criteria that would not qualify as SF the same galaxies. Clearly, the use of different criteria makes less comparable to each other the corresponding results and may fuel sterile debates as to which of such criteria should be preferable.

The importance of the MS comes from the fact that most stars in the Universe have formed in galaxies lying around it within about a factor of $\sim$2 in SFR. The mere existence of the MS, and its sharpness, indicate that there is order in nature, i.e., in the growth of galaxies, as opposed to mere stochasticity. It also implies that both the mass and SFR of high redshift galaxies must


best straight-line fit to the ridge line is log(SFR) = $(0.76\pm 0.01){\rm log}(M*/\msun) - 7.64\pm 0.02$, with a slightly flatter slope than derived in P10 for $u-g$ color selected [*blue*]{} galaxies in the same catalog, which was $0.9\pm 0.01$. This difference arises from the combination of two effects: the use of SDSS DR7 instead of the DR4 release; in addition, the $u-g$ color cut included several galaxies with $M*\simeq 10^9\,\msun$ and with SFR definitely below the ridge line, that we may interpret as [*quenching*]{} galaxies.

Figure 4 shows that the ridge line is straight linear up to the highest stellar masses in the sample, without a hint of flattening with increasing mass (see also @Brinchmann04. A bending of the main sequence could be due to the growing fraction ofa factor of $\sim 2$ since $z\sim 1$ (e.g., @Bell04), which is largely due to the increase in the number of low-mass quenched galaxies, whereas the number of massive quenched galaxies is stable in this redshift range.

To illustrate our proposal, this paper is limited to use data relative to the local Universe, but it is of great interests to follow the evolution of these 3D surfaces as a function of redshift, looking at how the [*twin peaks*]{} and the galaxy population of the ([*“green”*]{}) valley between them are changing with time. Such surfaces can be used to trace the MS divide at the various redshifts, which should be feasible even if current galaxy samples at high redshifts are not as populous as those used here. This extension to


star formation, as expected in the phenomenological model of P10. At the opposite mass end, very few galaxies are now found in the course of their mass-quenching, as indeed the model predicts that most of mass-quenching should have taken place at higher redshifts.

In summary, we propose a definition for the MS which does not require a pre-selection of SF galaxies, which should facilitate the inter-comparison of results from different groups, help understanding MS galaxies as systems in a quasi-steady state equilibrium and especially provide a more objective criterion for identifying [*quenching*]{} galaxies.

- 0.9 cm

Acknowledgments {#acknowledgments .unnumbered}
===============

We are grateful to Marcella Carollo, Natascha Förster Schreiber and Simon Lilly for useful discussions on these matters. AR acknowledges support from a INAF-PRIN-2012 grant.

[2014]{} Abazajian, K.N. et al. 2007, , 182, 543the orbital phase [@sut74]. Prior to mass transfer, when the donor star is close to filling its Roche lobe, the tidal effects are particularly strong and the orbit is likely to circularise on a short timescale. For this process, angular momentum conservation yields the orbital changes for a given eccentricity, $e_0$, $$\frac{a}{a_0} = 1-e_0^2.
  \label{eq:circularise}$$ The orbit is assumed to be fully circularised at the onset of mass transfer.

### Roche-lobe overflow {#sec:roche-lobe_overflow}

The change in orbital separation upon non-conservative[^3] mass transfer depends crucially on the specific angular momentum of the matter lost (which is rather poorly known).

When the donor star expands and fills its Roche lobe [@egg83], large scale mass transfer to its companion star initiates. This transfer of matter will continue in a stable or unstable way


the fractions of mass lost from the donor in the form of a direct fast wind, the mass ejected from the vicinity of the accretor and from a circumbinary coplanar toroid (with radius, ), respectively [@vdh94a; @spv97]. The accretion efficiency of the accreting star (here index 1) is thus given by: , or equivalently $$\partial m_1 = -\epsilon{\,}\partial m_2,
  \label{eq:epsilon}$$ where $m_2$ refers to the donor star mass and is its mass loss. These factors are functions of time as the binary system evolves during the mass-transfer phase.

In [[ComBinE]{}]{}, we assume $\alpha_{\rm RLO}$, $\beta_{\rm RLO}$ and $\delta_{\rm RLO}$ to be a constant, reflecting a time average during the entire RLO. Hence, their values determine the orbital angular momentum budget. The value of is based on the possibilitycores, (hereafter, simply referred to as WDs independent of chemical composition). Our NSs result from either an electron capture SN [EC SN, @nom87] if or an iron-core collapse SN (FeCC SN) if , following binary star calculations in @tlp15. In the EC SN case, a reduction of 10 per cent in gravitational mass is assumed during formation [@hmj+10], leading to NS masses in the range $\unit{1.24\text{ to }1.29}{{{\rm M}_{\sun}}}$. For NSs produced in FeCC SNe from non-stripped and partially stripped stars, we use the relation $${m_{\rm cobj}}= 0.23{\,}m_{\rm CO-core}+\unit{0.83}{{{\rm M}_{\sun}}},
  \label{eq:NSmass}$$ while $$\frac{{m_{\rm cobj}}}{{{\rm M}_{\sun}}} = -\frac{1}{0.168}+\sqrt{\frac{1}{0.168^2}+{\,}\frac{1.06}{0.084}{\,}\left(\frac{m_{\rm CO-core}}{{{\rm M}_{\sun}}}\right)^{0.454}}
  \label{eq:ultrastrippedNSmass}$$ is used for ultra-stripped NS progenitors [by combining the results of @ly89; @tww96; @tlp15]. We note that the NSs produced with the very smallest masses (see [Fig. \[fig:ZAMS-CompactObject\_Mass\]]{}) come from FeCC SNe [@tww96]. We


the age, mass, core mass, radius, luminosity, effective temperature and the envelope structure parameter, $\lambda$, for both stars in the binary. The semi-major axis (orbital period), eccentricity, galactic position and velocity of each binary system is also tracked. Finally, after the DCO is formed, the time until the merger of the two compact objects is determined.

Stellar grids {#sec:stellar_grids}
=============

[[ComBinE]{}]{}interpolates in dense girds of detailed stellar models. The underlying stellar models are calculated with the stellar evolution code BEC [e.g. @ywl10 and references therein]. In the following, we describe how we calculate the stellar grids from hydrogen-rich stars and helium stars, and how we determine the core-envelope boundary.

Hydrogen-rich stars {#sec:hydrogen_stars}
-------------------

On the ZAMS, stars consists mainly of hydrogen. @bdc+11 calculated grids of massive stars at various metallicities. Our computed grid takesroughly 1 dex. The NS-BH systems and double BH binaries increase by roughly 2 dex. These large discrepancies demonstrate the importance of $\lambda$ and stellar tracks being calculated with the same stellar evolution code.

The mass of the stellar envelope usually decreases as nuclear burning shifts material from the inner edge of the hydrogen envelope to the helium core and, at the same time, stellar wind material is lost from the outer edge of the envelope. In the most massive stars, very strong winds strip the whole envelope. The only way to increase the mass of the envelope in single star models is to mix some core material into the envelope. The radius, on the other hand, increases during the expansion phases on the giant branch(es). Usually the binding


efficiency may depend on e.g. the stellar masses and the mass ratio, besides the composition of the stars. For further discussions and application of efficient mass transfer in [[ComBinE]{}]{}, see [Section \[sec:mass-transfer\_efficiency\]]{} and [Appendix \[app:efficient\_mass\_transfer\]]{}, respectively.

The synthesized data presented here is obtained by simulating binary systems. In general, we find that our DCO merger rates converge with – except for the double BH systems where statistical noise remains at the 2 per cent level. In a MW-like galaxy, we assume a constant star formation rate of one binary per year with a primary star mass $>\unit{0.8}{{{\rm M}_{\sun}}}$ [@htp02]. This rate is rescaled according to the adopted primary mass range and the IMF. It is also applied at other metallicities to mimic the properties of both a young MW-like galaxy and a present-dayform in our default simulations. Since mass accretion is needed for the secondary star to produce a BH in cases where the primary star produces a NS, the choice of a small accretion efficiency $\epsilon$ ([Section \[sec:results\]]{}) hinders the formation of NS-BH systems. Those few NS-BH binaries that do form have an initial mass ratio close to one. In most cases mass transfer slows down the evolution of the primary to the extent that the secondary forms the BH first before the initial primary becomes a NS. Further discussions on the formation of NS-BH binaries are given in [Section \[sec:NSBH\_rare\]]{}.

The largest region in [Fig. \[fig:initial\_masses\_beta75\]]{} is blue indicating the formation of double BH binaries. Note, double BH systems occupy the largest area in the phase space of ZAMS masses but are


rates of DCO binaries at two different metallicities of galaxies otherwise similar to the MW. [Fig. \[fig:final\_masses\_formation\_beta75\]]{} and succeeding figures differentiate formation and merger rates according to the grid cells of different mass ranges.

In the following subsections we discuss the different binary types formed at high metallicity, as shown in the upper panel of [Fig. \[fig:final\_masses\_formation\_beta75\]]{}.

### Double black hole binaries {#sec:compact_object_masses_double_black_hole_binaries}

First, we look at the remnant masses in the double BH population evolved at a MW-like metallicity as shown in the upper panel of [Fig. \[fig:final\_masses\_formation\_beta75\]]{}. The largest visible sub-population creates a triangular shape like the progenitors shown in [Fig. \[fig:initial\_masses\_beta75\]]{}. All binaries without interactions, or only minor interactions, fall into this region. The binaries where either the secondary star becomes the more massive BH or the primary BH is produced with[Fig. \[fig:final\_orbit\_formation\_MW\_beta75\_NSNS\]]{} for the mixed systems consisting of one NS and one BH. In the upper panel the NS formed first, and in the lower panel the BH formed first. The dashed lines are constant periastron separations of $\unit{5}{{{\rm R}_{\sun}}}$ and $\unit{50}{{{\rm R}_{\sun}}}$.](final_orbit_formation_MW_beta75_BHNS.pdf "fig:"){width="\columnwidth"}

The orbital parameters of the mixed binaries consisting of a BH and a NS are shown in [Fig. \[fig:final\_orbit\_formation\_MW\_beta75\_mixed\]]{}. Compared to the double NS binaries all the different sub-populations overlap into one population.

The upper panel of [Fig. \[fig:final\_orbit\_formation\_MW\_beta75\_mixed\]]{} shows the few NS-BH systems in which the NS forms first. In all cases, there is no mass transfer after the formation of the NS. Therefore, based on our default simulations, we do not produce any recycled radio pulsars orbiting a BH (however, see the discussion in [Section \[sec:NSBH\_rare\]]{} on the


R}_{\sun}}}$, respectively.](final_orbit_formation_MW_beta75_BHBH.pdf){width="\columnwidth"}

\
![image](Tmerge_LIGO_MW_beta75_s.pdf){width="\columnwidth"} ![image](Tmerge_LIGO_thubble_MW_beta75_s.pdf){width="\columnwidth"}\
\
![image](Tmerge_LIGO_IZw18_beta75_s.pdf){width="\columnwidth"} ![image](Tmerge_LIGO_thubble_IZw18_beta75_s.pdf){width="\columnwidth"}\

Our simulated double BH binaries also split into several sub-populations, as shown in [Fig. \[fig:final\_orbit\_formation\_MW\_beta75\_BHBH\]]{}. The widest systems are those without mass-transfer interactions. The systems at intermediate orbits have a stable mass transfer before the second BH forms. The tightest double BH binaries went through a CE phase.

The majority (88 per cent) of the double BH binaries in our simulations are too wide to merge within a Hubble time. Only the tightest or most eccentric double BH binaries produced will merge via GW radiation. Therefore, most of the BH-BH GW detections from a high-metallicity environment are dominated by systems which evolved through a CE phase – unless they are formed by a completely different formation channel not investigated here (chemical homogeneous evolution or dynamical encounters, see [Section \[sec:alternative\_scenario\]]{}).

Gravitational wave-driven merger ratesof the exploding star. Some observed high-velocity pulsars need large kicks while some tight and nearby circular pulsar binaries must have experienced small kicks. We account for this in our new code in a systematic way by using different kick distributions depending on the evolutionary history of the exploding star, i.e. by considering how much of the envelope is stripped prior to the SN explosion ([Section \[sec:supernovae\]]{}).

Finally, we note that our implementation of the more advanced numerical Case BB RLO modelling of @tlp15 increases the double NS merger rate by an order of magnitude compared to our simulations based on the results of @dp03 which often lead to unstable RLO, causing a large fraction of close binaries to merge prior to the second SN.

### Merger-rate densities {#sec:compare_merger_rate_densities}

![\[fig:merger\_rate\_density\_beta75\] Merger-rate densities of


only under rather optimistic circumstances are we able to produce NS-NS merger-rate densities of up to in the local Universe. Although this value is within the error bar of the rate reported by @aaa+17c, we emphasize that the empirical rate of such double NS mergers is so far only based on one GW detection. From our simulations we predict that near-future GW detections, or rather non-detections, of double NS mergers from LIGO-Virgo runs O3 and O4 will decrease the empirical merger-rate density of double NSs to .

It is also evident from [Table \[tab:detection\_rates\_beta75\]]{} that assuming $\beta_{\rm min}=0.75$ we expect significantly more detections of BH-NS systems compared to double NS systems, which again illustrates GW170817 as being somewhat unexpected. The detection ratio between these two populations of DCO mergers dependswe find a spread in typical systemic velocities from a few $\kilo\meter\usk\reciprocal\second$ up to about $\unit{300}{\kilo\meter\usk\reciprocal\second}$ (with a very few systems reaching almost $\unit{500}{\kilo\meter\usk\reciprocal\second}$) with respect to the centre-of-mass reference frame of the binary system prior to the second SN ([Fig. \[fig:GW170817\_kick\_beta75\]]{}). The systemic velocities from the first SN are, in the vast majority, less than $\unit{50}{\kilo\meter\usk\reciprocal\second}$ and the final systemic velocities are therefore strongly dominated by the kinematic effect of the second SN.

### Comparison to the rates of core-collapse supernovae, short gamma–ray bursts and r-process element events {#sec:compare_SN-sGRB_rates}

In the following, we compare our simulated Galactic double NS merger rates with estimated constraints on CC SNe, sGRBs and heavy $r$-process element events.

Our default and “optimistic” estimates of a double NS merger rate of $\unit{3.0}{\mega{{\rm yr}}^{-1}}$ and $\unit{14}{\mega{{\rm yr}}^{-1}}$ for a


successfully eject the envelope of the BH progenitor, thus producing more NS-BH systems.

The number of produced NS-BH systems depends on the accretion efficiency (and thus $\beta_{\rm min}$) in a complex manner ([Fig. \[fig:formationRate\_alphaRLO\_betamin\]]{}). Applying a larger mass-transfer accretion efficiency compared to our default simulation, the number of NS-BH systems reaches a minimum before increasing again. In the most efficient case, more NS-BH systems are formed which would otherwise have become double NS systems, given the enhanced amount of material accreted by the secondary star. Reducing the mass-transfer accretion efficiency creates more NS-BH binaries as well. Because the progenitor of the BH, the initially less massive of the two ZAMS stars, accretes under such inefficient conditions, it can only be slightly less massive than the progenitor of the NS. Thereasoning is based on the hypothesis that the standard formation channel, due to mass transfer, leads to aligned spins of the BHs and the orbital angular momentum vector. However, as argued by @tkf+17, it cannot be ruled out that the spin axis of the collapsing star is tossed in a new, possibly random, direction as a result of the SN, similar to what has been suggested for NSs [@sp98; @fklk11]. If this is the case, then all past memory from mass transfer is lost. For NSs, there is evidence for such spin axis tossing in both of the two known young pulsars found in double NS systems: PSR J0737$-$3039 [@bkk+08] and J1906+0746 [@des+17 in prep.].

An alternative and novel formation channel of relative massive BH-BH binaries, which avoids the CE phase


simulated orbital parameters of systems in which both stars undergo FeCC SN. It is even clear that it is necessary to assume inefficient mass transfer to explain the observational data, cf. [Fig. \[fig:final\_orbit\_formation\_MW\_beta75\_NSNS\]]{} and the upper panel of [Fig. \[fig:final\_orbit\_MW\_NSNS\]]{}.

Mass-transfer efficiency {#app:mass-transfer_efficiency}
------------------------

![\[fig:gwMergerRate\_alphaRLO\]As [Fig. \[fig:gwMergerRate\_betamin\]]{}, but instead showing the dependence on the direct wind mass loss parameter during RLO.](gwMergerRate_alphaRLO.pdf){width="\columnwidth"}

![\[fig:formationRate\_alphaRLO\_betamin\]Formation rate of DCO binaries in a MW-like galaxy as a function of the re-emission fraction in the vicinity of the accretor, $\beta_{\rm min}$, (upper panel) and the direct wind mass loss parameter, $\alpha_{\rm RLO}$, (lower panel) during RLO. The dotted lines mark our default values of $\beta_{\rm min}$ and $\alpha _{\rm RLO}$, respectively.](formationRate_betamin.pdf "fig:"){width="\columnwidth"} ![\[fig:formationRate\_alphaRLO\_betamin\]Formation rate of DCO binaries in a MW-like galaxy as a function of the re-emission fraction in the vicinity ofheight: 100%;
   width: 30%; //can be any width
}

B takes remaining available height and width. Reduces width when A is made wider and vice versa

/*#b will automatically take the rest of main!
because it has overflow:hidden */
#b {
    overflow: hidden;
    width: auto;
    height: 100%;
}

B never flows to next line, no matter how wide the contents. (Instead a scrollbar).

Here i'm not sure what you want so the fiddle is lacking this part.
Do you want an ----> or
-|
-|
-|
-|
▼
Scrollbar? 1.
Replace overflow:hidden;
with overflow-x: scroll;
or overflow-y: scroll;
or overflow: auto for both ways
Fiddle for example :)


am unable to reproduce error from a fresh app yet

A:

Parcel by default does not transpile node modules, but they still get bundled when portions of a library is needed. By switching to webpack v4 and not excluding the node_modules directory, the bundled code, along with the library code, will get transpiled. This method does require import 'core-js' and the use of babel-loader. For a simple example:
module.exports = {
  entry: './app.js',
  modules: {
    rules: [
      {
        test: /\.m?js$/,
        use: {
          loader: 'babel-loader',
          options: {
   the full-attention printing, the processor will be spending idle time while the printer prints. The processor could be performing other tasks during this idle time.
One solution to this type of problem is the use of buffering. A simple example will illustrate.
Assume that the Sender's data bus is 32 bits wide, as shown in FIG. 2. Assume that the Receiver's data bus is smaller, at 8 bits. A very crude device adapter could operate as STEP 1 through STEP 4 indicate. The Adapter transfers data in eight-bit chunks. However, a problem with this approach is immediately apparent. While the Receiver may be receiving data as fast it can, the Sender is tied to the bus during the Receiver's activity. The Sender can do nothing else. This approach is inefficient


KSiteTV Exclusive preview clip for The 100 episode titled "Thirteen" featuring Eliza Taylor and Marie Avgeropoulos

A new episode of The 100 airs TONIGHT at 9PM (ET/PT) on The CW, and the network has provided KSiteTV with an EXCLUSIVE clip from tonight’s show!

The episode airing tonight (March 3) is called “Thirteen,” and in this clip, Clarke (Eliza Taylor) and Octavia (Marie Avgeropoulos) discuss what it is that they are going to have to do next… and Octavia doesn’t seem to agree with what Clarke has to say.

Below, find the clip and some preview images. You can find more coverage of The 100 by browsing KSiteTV!

The 100 "Thirteen" KSiteTV EXCLUSIVE Clip from KSiteTV.com on Vimeo.

The 100 ◄ Back Next ► Picture 1 of 11 The 100 -- "Thirteen" -- ImageÃÂproteins, such as MDC1 or 53BP1, that accumulate at ionising radiation induced foci (IRIF). DSBs repaired with slow kinetics predominantly localise to the periphery of genomic heterochromatin (HC). Indeed, there is mounting evidence that chromatin complexity and not damage complexity confers slow DSB repair kinetics. ATM's role in HC-DSB repair involves the direct phosphorylation of KAP-1, a key HC formation factor. KAP-1 phosphorylation (pKAP-1) arises in both a pan-nuclear and a focal manner after radiation and ATM-dependent pKAP-1 is essential for DSB repair within HC regions. Mediator proteins such as 53BP1, which are also essential for HC-DSB repair, are expendable for pan-nuclear pKAP-1 whilst being essential for pKAP-1 formation at IRIF. Data suggests that the essential function of the mediator proteins is to promote the retention of activated


at risk.” Id. But close
relationships among the parties are not fatal to the shareholder’s claim of increased
basis “if other elements are present which clearly establish the bona fides of the
transactions and their economic impact.” Id. (quoting Bhatia v. Commissioner, 72
T.C.M. (CCH) 696 (1996)). Put simply, the corporation must actually be indebted to
the shareholder for the shareholder’s own money.

       Oren maintains that the loans were real investments and, as such, properly
increased his basis in both HS and HL. He notes that the loan agreements were
legally binding, properly memorialized, and recorded on the corporations’ books. He
also points out that because the funds were loaned to him by Dart with the approval
of First Bank, a third party was involved in the transactions. Additionally, he testified
thatfor, and the continued development of both Jayson Tatum and Jaylen Brown has also been encouraging this season for Boston. -- Michael Kaskey-Blomain

The Nets had arguably the biggest offseason in the NBA yet have little to show for it so far. Kevin Durant is sidelined for the season with an Achilles injury, while Kyrie Irving has missed over half of the team's games with a shoulder injury. Caris LeVert has also been out with a thumb injury. Though the Nets have been able to stay competitive, they're not a real threat in the East without at least one of their All-Star additions. Spencer Dinwiddie has done an excellent job of carrying the load for the team in the meantime, but ultimately the Nets will go as far as


number of smart offseason signings to supplement their young roster, it seemed like the Bulls might be on the right path; some even saw them sneaking into the playoffs at the bottom of the East. Instead, this season has been a mess. They can't score, young players such as Lauri Markkanen have disappointed and there have been further complaints about head coach Jim Boylen's tactics. Relative to expectations, it's hard to call them one of the most disappointing teams in the league, but they've certainly been disappointing. -- Jack Maloney

Cleveland Cavaliers: D

What is there to even say about this team? The Cavs are terrible, but that was always going to be the case as they continue to pay off the bill left by the second set of LeBronmaybe they should get an A? -- Colin Ward-Henninger

Houston Rockets: B

The Rockets have rebounded from a tough start, climbing to 14th on defense. Whether or not they are truly title contenders, though, depends on how much better they can get from here. While James Harden has taken his brand of one-on-one brilliance to yet another level of insanity, the Russell Westbrook experiment has had mixed results. The Rockets are different than they were with Chris Paul, but it is unclear if sacrificing point guard defense and halfcourt offense for rebounding and transition offense will raise their ceiling the way they hoped. Westbrook has shot a career-low 21.6 percent on catch-and-shoot 3s, and Houston desperately needs to improve in his minutes without Harden. -- James Herbert

With Victor Oladipo's continued


Roosevelt knew the importance of circulating wealth in order to revitalize the economy by investing in key infrastructure, including the public education system.

Today fierce battle lines are drawn over whether or not the estate tax should be repealed. On one side are Bill Gates Jr., Grover Norquist and the Wall Mart heirs and on the other side are Bill Gates Sr. and Chuck Collins. This is certainly not a case of “like father like son.”

While Bill Gates Sr. has co-penned a book with Chuck Collins calling for increased exemptions but not abolishment of the estate tax, Bill Gates Jr. has been the prime funder of Grover Norquist as Norquist tours the country relentlessly advocating a complete repeal of the tax. Like Bill Gates Sr., I believe the exemptionthe product, which coincides with its length; cooling is generally carried out on both surfaces of the product, with a constant delivery rate per area (expressed as an important volume of fluid of product per unit of area and of time), but it may also be unilateral.
This practice usually leads to serious deformation of the products and the deformation increases when the speed of cooling and/or the width of the product increase and/or if the speed at which the products advance is reduced. Particularly in the case of quenching metals and alloys, the quenching deformations appear immediately downstream of the front for the action of the fluid, within the range of the highest temperatures where the yield strength of the metal is excessively low; the amplitude of the


name. Students can easily access the 5th class annual results. The site ilmkidunya wishes best of luck to every student and pass the exams with excellent marks.

ilmkidunya publishes the result every year and the students can visit the website to view their result online through ilmkidunya. The students are required to enter their roll numbers in order to view their result.

BISE Lahore Board 5th Class Result 2020

BISE Lahore Board 5th Class Result 2020 is expected to be announced on 31, March 2020. 5th class students who are enrolled in government and public schools can check the result online. As soon as the board announces the exact date, it will be updated on our website. All the students are requested to stay in touch with our website to getto view their results. ilmkidunya will display the result and all the candidates can get their result online right from here. BISE Gujranwala Board official website sometimes gets overloaded due to heavy traffic of visitors so the candidates can view their results from our website at 10 am. The websites publish all the news updates so stay in touch to remain updated.

BISE Faisalabad Board 5th Class Result 2020

BISE Faisalabad is an autonomous body that organizes controls and regulating exams. PEC issues the date sheet and roll number slips of the students. Every year the exams of 5th class are conducted by PEC. The 5th class annual exams were held in the month of February and the BISE Faisalabad Board 5th Class Result 2020 will be announced on 31


February and the BISE Bahawalpur Board 5th Class Result 2020 is coming very soon as decided by PEC. PEC is responsible for the conduction of exams as well as the declaration of the result. The PEC staff after working hard has finalized the result. The date has been confirmed and is expected to be announced on March 31, 2020. The students will be able to check their result online on the page of ilmkidunya by providing their roll number. The result will be published on the same date it is declared. We wish good luck for all the students for their coming result of 5th class.

BISE DG Khan Board 5th Class Result 2020

PEC is dedicated in organizing middle-class exams every year in February and also declares the BISEjust start "leaning on" somebody else's pitch, or shut up altogether before anyone notices. ;-)
Virtually all the people around me sing at a higher pitch than me, and unless someone picks up a base guitar, the instruments are higher pitched as well. ;-) Singing "to pitch" / much higher than my natural singing voice strains my vocal chords, and makes my voice sound much less praiseworthy... so I would really like to practice "holding my own".
However, taking lessons would be expensive, and / or organizationally a bit hard to come by. (Music school would be quite some way off, and expensive; and none of my friends really has the time or the teaching skill to take me on as a student.)
Is there a good way I could (start


one style would leave me dropping caveats. And no one wants that.

I'm certainly a sucker for Lennon/McCartney and Strummer/Jones, but I'm also quite fond of everyone from Fela Kuti to Curtis Mayfield to Bob Dylan to Chuck D to Morrissey/Marr. I also think Alex Turner from Arctic Monkeys has a knack for storytelling.

Last edited by stuporfly; 08-06-2009 at 07:08 AM.
Reason: I can't fucking type

Re: Get to know your fellow board members....

Originally Posted by RotationSlimWang

1. If you HAD to genocide a group of people straight across the board but could use any criteria you can imagine to apply to their unquestioned painful demise throughout the world, what would it be and why?

Williamsburg hipsters - I'd take away their skinny jeans and Members Only jackets. They'd snap quickly into apoplexy1% will masturbate in the corner.

Re: Get to know your fellow board members....

Hmmm, after the post with reference to the Fan Man, perhaps you'd rather imform us of that period of your li8fe instead? LOL

Its like the Infinite Monkey Theorem, if you put X amount of monkeys in a room with a typewriter and ask them to give you Shakespeare 99% of them will fling their shit at you while the other 1% will masturbate in the corner.

Re: Get to know your fellow board members....

Going back to the day where ants in your pants was a funny thing, what other hilarious memories do you have of your childhood? (Say, between 5 and 13 years old.)

When I was 11 years old, my dumb buddies and I started a protection


Hello everyone welcome to this lecture in
the last lecture we have discussed how we
can obtain an absorption spectrum.
We had mentioned that if you plot absorbance
obtained from a spectroscopy experiment against
wavelength lambda we can obtain an absorption
spectrum. Although conventionally absorbance
is plotted against wavelength we can also
plot absorbance against frequency as these
are interchangeable. So, we can write h new
equals hc by lambda. Moreover we can also
plot absorbance against wave number.
Wave number is denoted by new bar a new bar
is related to frequency because h new equals
hc new bar or we can write new equals c new
bar. So, the next question is what is the
unit of new bar because we can write new equals
c new bar or rearranging this equation we
can write new bar equals new by c. So, we
know theLesson Plan

Info

Telling Personal Stories Through Art

In this lesson, students explore the connection between art and storytelling, focusing on how art can serve as an empowering, self-actualizing and even cathartic form of self-expression.

Lesson Summary

In this lesson, students explore the connection between art and storytelling, focusing on how art can serve as an empowering, self-actualizing and even cathartic form of self-expression. The video clips provided in this lesson are from Cutie and the Boxer, an Academy Award®-nominated film about the chaotic and unconventional 40-year love affair and creative partnership between action painter Ushio Shinohara and his wife, Noriko, also an artist. Ushio, who punches canvases with paint-laden gloves, is famous in Japan and in Manhattan's art circles, yet wider recognition has eluded him. Noriko, 21 years his junior, put her


related note they can determine what art is and who makes that call. They can produce a journal on art movements in which they submit "peer reviewed" essays on this topic; as a focus, they might discuss how art should be approached and studied in school.

Window Opacity

Feedback Form

Quick Assign

Assignment Code:

Assignment URL:

Assign directly to your students using the code or link above, without having them log in. Simply tell your students to go to
www.pbsstudents.org and enter the Assignment Code, or click on the Assignment URL to share the assignment as a link.ventures as it wants to focus on its 'core businesses' and shift from non-core businesses such as retail which have increased its debt burden.

7) EPC Industries Ltd, after Credit Renaissance Fund today offloaded its entire over 17 per cent stake in micro irrigation systems maker EPC Industries for more than Rs 61 crore in bulk deals on the exchanges.

8) Reliance Industries Ltd, after the newly formed Cabinet Committee on Investment will soon consider clearing 47 oil & gas blocks, including RIL's producing KG-D6 gas fields, where defence clearance has either been withdrawn or withheld.

9) Engineers India Ltd, after the government is expected to consider tomorrow proposals for 10% stake sale in Engineers India Ltd, which may fetch around Rs 645 crore to the exchequer, and a revival package


Q:

"PermGen space" running assets:precompile under jruby

I'm getting PermGen space errors when running rake assets:precompile under jruby 1.7.4. I've tried increasing MaxPermSize and turning on ClassUnloading, to no avail.
This is happening reliably, both on a Cloudbees m1-large instance and locally on my macbook pro.
$ MAVEN_OPTS='-XX:MaxPermSize=2048M -XX:+CMSPermGenSweepingEnabled -XX:+CMSClassUnloadingEnabled -XX:+UseConcMarkSweepGC -w' bundle exec rake dash:build RAILS_ENV=production --trace
** Invoke environment (first_time)
** Execute environment
** Invoke dash:build (first_time)
** Invoke dash:prebuild (first_time)
** Execute dash:prebuild
** Invoke assets:clean (first_time)
** Execute assets:clean
** Invoke assets:clean:all (first_time)
** Invoke assets:environment (first_time)
** Execute assets:environment
** Invoke environment
** Invoke tmp:cache:clear (first_time)
** Execute tmp:cache:clear
** Execute assets:clean:all
rm -rf /Users/andrew/code/unified_dashboard/public/assets
** Invoke assets:precompile:primary (first_time)
** Invoke assets:environment
** Invoke tmp:cache:clear
** Execute assets:precompile:primary
rake aborted!
PermGen space
org.jruby.java.proxies.JavaProxy.confirmCachedProxy(JavaProxy.java:503)
org.jruby.java.proxies.JavaProxy.getSingletonClass(JavaProxy.java:495)
org.jruby.RubyModule.extend_object(RubyModule.java:2008)
org.jruby.RubyModule$INVOKER$i$1$0$extend_object.call(RubyModule$INVOKER$i$1$0$extend_object.gen)
org.jruby.RubyClass.finvoke(RubyClass.java:741)
org.jruby.runtime.Helpers.invoke(Helpers.java:477)
org.jruby.RubyBasicObject.callMethod(RubyBasicObject.java:359)
org.jruby.RubyBasicObject.extend(RubyBasicObject.java:2756)
org.jruby.RubyKernel.extend(RubyKernel.java:2187)
org.jruby.RubyKernel$INVOKER$s$0$0$extend.call(RubyKernel$INVOKER$s$0$0$extend.gen)
org.jruby.internal.runtime.methods.JavaMethod$JavaMethodN.call(JavaMethod.java:662)
org.jruby.internal.runtime.methods.DynamicMethod.call(DynamicMethod.java:205)
org.jruby.runtime.callsite.CachingCallSite.call(CachingCallSite.java:168)
org.jruby.ast.CallOneArgNode.interpret(CallOneArgNode.java:57)
org.jruby.ast.IfNode.interpret(IfNode.java:118)
org.jruby.ast.NewlineNode.interpret(NewlineNode.java:105)
org.jruby.ast.BlockNode.interpret(BlockNode.java:71)
org.jruby.evaluator.ASTInterpreter.INTERPRET_METHOD(ASTInterpreter.java:74)
org.jruby.internal.runtime.methods.InterpretedMethod.call(InterpretedMethod.java:225)
org.jruby.internal.runtime.methods.DefaultMethod.call(DefaultMethod.java:202)
org.jruby.runtime.callsite.CachingCallSite.call(CachingCallSite.java:202)
org.jruby.ast.FCallTwoArgNode.interpret(FCallTwoArgNode.java:38)
org.jruby.ast.NewlineNode.interpret(NewlineNode.java:105)
org.jruby.ast.BlockNode.interpret(BlockNode.java:71)
org.jruby.ast.BlockNode.interpret(BlockNode.java:71)
org.jruby.ast.RescueBodyNode.interpret(RescueBodyNode.java:108)
org.jruby.ast.RescueNode.handleJavaException(RescueNode.java:205)
org.jruby.ast.RescueNode.interpret(RescueNode.java:138)
org.jruby.evaluator.ASTInterpreter.INTERPRET_METHOD(ASTInterpreter.java:74)
org.jruby.internal.runtime.methods.InterpretedMethod.call(InterpretedMethod.java:225)
org.jruby.internal.runtime.methods.DefaultMethod.call(DefaultMethod.java:202)
org.jruby.runtime.callsite.CachingCallSite.cacheAndCall(CachingCallSite.java:346)

As far as I know the project isn't doing anything unusual with its assets. I'm not very familiar with Java or Jruby (I inherited the project whenspun around, looking for Bad Luck. My middle lane became the right lane again. What was happening here? Was I hallucinating? I pawed for the turn signal but grabbed the windshield wipers. Screw it. Let them wipe. I had bigger problems. Like steering clear of Taxi -vs- Uber -vs- Lyft battles.

More left. More left. Everything is left. The Fiesta's wipers rubbed against the glasses and my left turn signal never switched off. I kept nosing the blunt little car left until nothing was aside me but the concrete divider. There! Let's see you mess with me now Bad Luck.

This content is imported from YouTube. You may be able to find the same content in another format, or you may be able to find more information, at their web


in 1922. One year earlier another tradition was begun when the Margolis Antiques Shop moved into the other half.

New-York Tribune, October 30, 1921 (copyright expired)

Ethel King sold No. 1122 Madison Avenue to the 27 East Eighty-Third Street Corp. in 1921. The firm converted the second floor to "non-housekeeping apartments." The Department of Buildings included a stark warning in its Certificate of Occupancy:

Cooking in more than Two of the apartments will render this building liable to immediate vacation by the Tenement House Department

The Margolis Shop remained here at least through 1928. The tradition was continued by Frank Lustig Antiques in the 1960s, Frank Silberman's Art & Ends antiques shop in the 1970s, and Pascoe and Solomon, Inc., dealers in art pottery beginning around 1979.

In 1937 Russo Brothers had erectedChristian college I attended, to the pastoral and theological books I read, to the seminary from which I graduated, to the thousands of sermons I …Read More

The ordinary Christian life is not the opposite of the radical Christian life. The ordinary Christian life is a radical life. The ordinary Christian life is a life of daily trusting Christ; daily repenting of our sins; daily abiding in …Read More

John Wycliffe was the morning star of the Reformation. He was a protestant and a reformer more than a century before Martin Luther ignited the Protestant Reformation in 1517. Through Wycliffe, God planted the seeds of the Reformation, He watered …Read More

I spent my ﬁrst year of college at a second-degree separatist school that was founded by the Bible Presbyterian Church.


= window_choose_get_item(wp, key, m)) == NULL)
			break;
		if (item->state & TREE_EXPANDED) {
			window_choose_collapse(wp, item->wcd->tree_session,
			    data->selected);
			window_choose_redraw_screen(wp);
		}
		break;
	case MODEKEYCHOICE_TREE_COLLAPSE_ALL:
		window_choose_collapse_all(wp);
		break;
	case MODEKEYCHOICE_TREE_EXPAND:
		if ((item = window_choose_get_item(wp, key, m)) == NULL)
			break;
		if (!(item->state & TREE_EXPANDED)) {
			window_choose_expand(wp, item->wcd->tree_session,
			    data->selected);
			window_choose_redraw_screen(wp);
		}
		break;
	case MODEKEYCHOICE_TREE_EXPAND_ALL:
		window_choose_expand_all(wp);
		break;
	case MODEKEYCHOICE_UP:
		if (items == 0)
			break;
		if (data->selected == 0) {
			data->selected = items - 1;
			if (data->selected > screen_size_y(s) - 1)
				data->top = items - screen_size_y(s);
			window_choose_redraw_screen(wp);
			break;
		}
		data->selected--;
		if (data->selected < data->top)
			window_choose_scroll_up(wp);
		else {
			screen_write_start(&ctx, wp, NULL);
			window_choose_write_line(wp, &ctx,
			    data->selected - data->top);
			window_choose_write_line(wp, &ctx,
			    data->selected + 1 - data->top);
			screen_write_stop(&ctx);
		}
		break;
	case MODEKEYCHOICE_DOWN:
		if (items == 0)
			break;
		if (data->selected == items - 1) {
			data->selected = 0;
			data->top = 0;
			window_choose_redraw_screen(wp);
			break;
		}
		data->selected++;

		if (data->selected < data->top + screen_size_y(s)) {
			screen_write_start(&ctx, wp, NULL);
			window_choose_write_line(wp, &ctx,
			    data->selected - data->top);
			window_choose_write_line(wp, &ctx,
			    data->selected - 1 - data->top);
			screen_write_stop(&ctx);
		} else
			window_choose_scroll_down(wp);
		break;
	case MODEKEYCHOICE_SCROLLUP:
		if (items == 0 || data->top == 0)
			break;
		if (data->selected == data->top +SKS Sensors is now EPIC® SENSORS

We are well known from our high-quality SKS Sensors temperature sensors. Now, as LAPP aquired Lapp Automaatio (former SKS Automaatio), we are obliged to rebrand our products.

SKS Sensors is now EPIC® SENSORS.

Lapp has many strong brands and we see this new addition of temperature sensors to our worldwide portfolio of branded products and corporate network of sales companies in more than 45 countries as a great opportunity. EPIC® is a strong LAPP brand which until now has been allocated for our strong portfolio of industrial connectors. We have a strong belief that this will strengthen our commitment to serve our customers globally, wherever they are. We would like to be where you are as a customer.

Products and high-quality production, as well as experts


I will never leave." "I will always be right here." "Do you understand that?" "They're gonna try and get rid of me again, and I need you to not let them." "Listen to me." "I will never leave you." "I will never leave you alone again." "I am Mr. Robot." "I've always told you we'd end up working together, Elliot, but still" "I have to know, why did you do it?" "I wanted to save the world." "_" "Why this mask?" "It's a bit silly, isn't it?" "Wellick." "I see." "I understand." "James, yes." "Yes, I'm aware of Mr. Goddard's request, but it needs to be removed this moment." "Can you escalate it?" "Thank you, James." "It should be ready." "What is it?" "It's happening." "It's almost asbetween them are disturbing." "Meaning the end of the world as we know it." "Tyranny in the streets." " Hello?" " Hello?" " Hello?" " Hello." "That's right." "Stop!" "Well, what am I supposed to do?" "I mean, nothing is working." "Unplug what?" "Everything is inside the walls." "That's how it was installed when I ordered the smart house package." "Now the alarm is going off, and it's freezing." "It's below 40." "I have a place in Greenwich, but you don't expect me to..." "How long is it gonna take before this all gets fixed?" "The tracking on her phone is working, and she's headed north as we speak." "How long you think she's gonna stay away for?" "Long enough." "The collective result of these attacks could be


a cyber Pearl Harbor, physical destruction and the loss of life, and create a new, profound sense of vulnerability." "As director of the CIA and Secretary of Defense," "I have understood that cyber attacks..." "I hope you don't mind I came." "Something wrong?" "It's good to see you, Gideon." "You, too." "I know we didn't leave things on the best of terms." "Is it true?" "What I heard about Allsafe?" "Oh, there is no Allsafe." "I've had to furlough everyone." "I'm hoping to get up and running again, but everyone's telling me it's over." "Gee, I wonder whose fault that is." "Was that you or me?" "Getting all mixed up, I can't recall." "Let me get to my point." "The FBI believes that I was behind the hackNSF budget is $146 million for a new
Information Technology initiative (IT2). Also included was a $50
million biocomplexity initiative and $7.5 million for a Graduate
Teaching Fellows Programs.
Also on February 1, the NSF Director held a press conference on the
NSF's budget request, and met representatives of the science and
engineering (S&E) research education communities, and with key
congressional staff members. The Director also spoke to the Association
of American Universities Council on Federal Relations, and a group of
executives from S&E societies and associations. The overall reaction to
the budget is good, and NSF continues to make the case for the national
importance of the new IT2 initiative.
b. Congressional Hearings
The Director announced that hearings on the budget proposal will begin
on March 4, with testimony before the House Appropriation Subcommittee,
on March 16, before the House Basic Research


said a senior management group at NSF has been formed to
draft the revisions, and the Board will be involved from the early
stages.
Dr. Colwell focused on the need for an expanded budget for basic
research. She noted that there would be an NSF working team with senior
management, initiated at the Director's Policy Group retreat on March
1-2, to review the GPRA strategy. An external review must also be a
part of the review in 2000. The Director reviewed the schedule and
stated that Board members would be involved in the updating process from
the beginning.
Board Discussion
Dr. Kelly noted the importance of using the revised strategic plan to
communicate to the public and to other officials in the government about
what NSF does.
Dr. Colwell said that in order to think about future NSF priorities the
Assistant Directors haveand Dr. Rita
Colwell, Director, National Science Foundation.
Dr. Jane Lubchenco, NSB member and Chair of the NSB Task Force on the
Environment, gave an overview of the symposium. Members of the Board
moderated.
The keynote address was presented by Dr. Kathryn Sullivan of the
Columbus, Ohio, Center of Science and Industry. Dr. Sullivan emphasized
that we need a common understanding of key issues and that assessments
are required to facilitate communication among scientists, decision
makers, and individuals. She exhorted NSF to look creatively at this
issue. Dr. Sullivan also suggested that NSF advance fresh approaches to
education, emphasizing lifelong learning via community education in
addition to the traditional support for schooling.
The session entitled Emerging Interdisciplinary Opportunities featured
Drs. Pamela Matson (Stanford University), David Schimel (National Center
for Atmospheric Research), Simon Levin (Princeton University), and Jerry
Melillo (The Ecosystems Center, Woods Hole, MA)