\tilde{\cal{P}}_{\nu}$ at fixed redshift (from left to right, $z=3,4,5$, respectively) and varying neutrino mass for two massive neutrino cosmologies, as well as for two nonstandard dark radiation models; dotted lines refer to $\sum m_{\nu}=0.1$ eV, dashed lines are for $\sum m_{\nu}=0.3$ eV – in both cases with $N_{\rm eff}=3.046$ – while long-dashed and dot-dashed line styles are used for similar models that in addition also contain a sterile neutrino, so that $N_{\rm eff} =4.046$. The bottom panels display the tomographic redshift evolution of the ‘spoon-like’ feature at fixed neutrino mass; in the left one $\sum m_{\nu} =0.1$ eV, while in the right one $\sum m_{\nu} =0.3$ eV. In both panels, the addition of a sterile neutrino on top of massive neutrinos (so that $N_{\rm eff}=4.046$) is also shown,instead a tomographic evolution of the minimum of the ‘spoon-like’ feature, also almost independent of $\sum m_{\rm \nu}$ or $N_{\rm eff}$: with increasing redshift, its position shifts to smaller scales, from $k \sim 5h{\rm Mpc^{-1}}$ $(z=3)$, to $k \sim 9h{\rm Mpc^{-1}}$ $(z=4)$, to $k \sim 14h{\rm Mpc^{-1}}$ $(z=5)$. In the next subsection we will provide some theoretical arguments on why this is finding is interesting, in the context of the halo model: essentially, it is related to the halo formation times in massive neutrino and dark radiation cosmologies. Therefore, the amplitude and position of the maximal suppression of the ‘spoon-like’ effect caused by neutrinos and dark radiation on the total matter power spectrum define a characteristic nonlinear scale (see Section \[sub\_nu\_nonlinear\_scales\]) that potentially can be useful for determining


in the language of the halo model, the $one$-halo term dominates over the $two$-halo term at scales $k>1 h {\rm Mpc^{-1}}$ of interest here; hence, one can just focus on this term to understand the physical meaning of the ‘spoon-like’ suppression of power, since from our Figures \[fig\_3dps\_spoon\_1\] and \[fig\_3dps\_spoon\_2\] it is evident that the most relevant part of the feature occurs at $k \gg1 h {\rm Mpc^{-1}}$. In principle, in a cosmology with massive neutrinos, one should characterize the contributions to the total matter power spectrum provided by all the relevant individual components (i.e., CDM, baryons, neutrinos; see for example Figures \[fig\_3dps\_components\] or \[fig\_3dps\_spoon\_2\]) as well as their cross-correlations; however, at small scales, the neutrino and cross-power spectrum contributions are subdominant, and therefore the main role isnonlinear massless neutrino cosmology – which identifies the best regime to search for small-scale neutrino or dark radiation imprints on the high-$z$ cosmic web. Bottom panels show the corresponding magnitude of the effect at the given $k_{\rm max}$, in percentage ratios, in terms of power spectrum departures from the BG nonlinear expectation.[]{data-label="fig_nu_bao_like_scale"}](3d_total_matter_ps_100_512_ratios_best_k_paper_bis.pdf "fig:"){width="21.50000%"} ![Characteristic nonlinear scales for neutrino and dark radiation models, as inferred from the ‘spoon-like effect’ on the 3D total matter power spectrum. Top panels display the wavenumber $k_{\rm max}$ that corresponds to the minimum of the spoon-like feature, namely, the maximum departure from the corresponding nonlinear massless neutrino cosmology – which identifies the best regime to search for small-scale neutrino or dark radiation imprints on the high-$z$ cosmic web. Bottom panels show the corresponding magnitude


parameter at $z$, $n_{\rm HI}(x,z)$ the neutral hydrogen density in real space, $v_{\rm p \parallel}(x,z)$ the IGM peculiar velocity along the LOS, $\Sigma(x,z)$ the IGM velocity dispersion in units of $c$, and ${{\cal{G}}}$ the Voigt profile. The neutral hydrogen density in real space $n_{HI}(x,z)$ depends on the mean IGM density and on the hydrogen photoionization rate, as well as on the IGM temperature and overdensity. The IGM velocity dispersion is defined as $$\Sigma(x,z) = \sqrt{{2 k_{\rm B} T(x,z) \over m c^2}}
\label{}$$ with $T(x,z)$ the IGM temperature and $k_{\rm B}$ the Boltzmann constant, and in general the Voigt profile is is well approximated by the Gaussian: $${{\cal{G}}} = { 1 \over \Sigma  \sqrt{\pi} }  \exp \Big \{ - \Big [ ( u-x-v_{\rm p \parallel} )  /view of upcoming high-quality data from the SDSS-IV eBOSS, and for future larger-volume surveys such as DESI. The best and most accurate way to achieve this task is via high-resolution hydrodynamical simulations, which properly account for the complicated interplay between baryonic physics, IGM thermal properties, neutrino and dark radiation effects, and nonlinearities due to small-scale clustering.

Figure \[fig\_1d\_flux\_A\] shows examples of such measurements from our high-resolution simulation suite for the BG cosmology (solid lines), for two massive neutrino models with total mass $\sum m_{\nu}=0.1$ eV (dotted) and $\sum m_{\nu}=0.3$ eV (dashed), respectively, and for two dark radiation scenarios that in addition also contain a massless sterile neutrino so that $N_{\rm eff}=4.046$ (short and long dashed?dotted lines). The various panels display the tomographic evolution in redshift intervals, ranging from $z=2.0$


(top left panel) to $z=5.0$ (bottom right panel), in intervals of $\Delta z=0.2$; note that the wavevector $k$ is now expressed in $\rm (km /s)^{-1}$. Measurements are averaged over 10,000 mock quasar absorption spectra per redshift interval, constructed from our simulation snapshots by extracting the same number of random skewers along the LOS with the methodology briefly explained before in Section \[section\_simulation\_suite\]. All the spectra here are rescaled in terms of an effective optical depth $\tau_{\rm eff}(z) = \tau_{\rm A} (1+z)^{\tau_{\rm s}}$ at any given redshift, with $\tau_{\rm A} =0.0025$ and $\tau_{\rm s} =3.7$ at $z=3$. The adjustment of the UV background allows one to reproduce an observed mean flux level compatible with the observation of the high-$z$ IGM (Becker et al. 2011) and is now standard procedure.$\sum m_{\nu}=0.4$ eV, respectively – even in the presence of a sterile neutrino. Moreover, we note that when the neutrino mass is small ($\sum m_{\nu} =0.1$ eV), an additional sterile neutrino causes a significant difference in the flux (compare, e.g., the top and bottom left panels of the figure), but when the neutrino mass increases, the effect of a sterile neutrino is somehow masked by the impact induced by the active ones on the Ly$\alpha$ flux – see, e.g., the case of $\sum m_{\nu} =0.4$ eV, top and bottom right panels.

Figure \[fig\_1d\_flux\_B\] contains similar information to Figure \[fig\_1d\_flux\_A\], but now the redshift is fixed within a given panel, while the total neutrino mass is let vary inside individual panels. Models with $N_{\rm eff}=3.046$ (i.e., massive neutrino cosmologies) are


modules; the interconnection problem for such solutions is immense.
We have solved some of the problems encountered in the prior art which we referred to above and will describe in the detailed description a way whereby multiple functions can be transmitted over the same network path.
In making our invention we recognize that others have tackled various problems in the network area. Some of this literature is discussed here.
U.S. Pat. No. 4,679,190, issued Jul. 7, 1987, to Dias et al, described a method of delivery of high priority messages in a multi-stage network using a multi-stage interconnection connector for voice and data packets. This patent relates to a different transmission scheme with synchronous, clocked, time-slotted transmission. There is no control by a Hi/Lo priority interface line, and the relatively complexwriting “community”, which compels every writer who craves self respect and success to attend community events, help to organize them, buzz over them, and—despite blitzed nerves and staggering bowels—present and perform at them. We get through it. We bully ourselves into it. We dose ourselves with beta blockers. We drink. We become our own worst enemies for a night of validation and participation.

Even when a dentist kills an adored lion, and everyone is furious, there’s loftier righteousness to be had.

Now is the point in the story of Cecil the lion—amid non-stop news coverage and passionate social-media advocacy—when people get tired of hearing about Cecil the lion. Even if they hesitate to say it.

But Cecil fatigue is only going to get worse. On Friday morning, Zimbabwe’s environment minister, Oppah


secrecy laws by handing over the names, or refuse and face criminal charges in U.S. federal court. Within months, Mrs. Clinton announced a tentative legal settlement—an unusual intervention by the top U.S. diplomat. UBS ultimately turned over information on 4,450 accounts, a fraction of the 52,000 sought by the IRS.”

During the multi-country press tour for Mission Impossible: Rogue Nation, not even Jon Stewart has dared ask Tom Cruise about Scientology.

During the media blitz for Mission Impossible: Rogue Nation over the past two weeks, Tom Cruise has seemingly been everywhere. In London, he participated in a live interview at the British Film Institute with the presenter Alex Zane, the movie’s director, Christopher McQuarrie, and a handful of his fellow cast members. In New York, he faced off with Jimmycare plans can be made and delivered for patients, there is a strong need for hospitals to adopt a more vigorous approach to identify patients who are entering the last year of their lives.

-   We contend that the culture and organisation of hospitals need to become more attuned to the high proportion of inpatients in imminent need of end-of-life care.

Introduction {#section7-0269216314526443}
============

There is growing interest in the challenge of providing appropriate end-of-life care to an ageing population, as demands on services increase and as expectations of patients and families change.^[@bibr1-0269216314526443],[@bibr2-0269216314526443]^ The role of the hospital in the delivery and planning of such care is of major significance, partly because so many patients die there, but also because hospital admission provides an opportunity to identify those who may


predictor variables and mortality at 1 year, adjusting for the possible confounding effect of age, gender, a measure of deprivation and whether admission was to a medical or surgical specialty. A univariate logistic regression analysis, also using R 3.0.1, was undertaken to examine the relationship between age and mortality. The measure of deprivation used here is the Scottish Index of Multiple Deprivation 2009 (SIMD09), an area-based deprivation score which groups the Scottish population into five equal quintiles, with quintile 1 representing the 20% most deprived areas in Scotland and quintile 5 the least deprived.^[@bibr15-0269216314526443]^ The National Records of Scotland office provided information on deaths including the date of death.^[@bibr16-0269216314526443]^

Results {#section10-0269216314526443}
=======

We identified 10,743 hospital inpatients on the census date. More were women (54.7%) than men (45.3%). Most (64.1%) were[Figure 1](#fig1-0269216314526443){ref-type="fig"}). The mortality rate rose steeply with age and was three times higher at 1 year for patients aged 85 years and over compared to those who were under 60 years of age (45.6% vs 13.1%; *p* \< 0.001) ([Table 1](#table1-0269216314526443){ref-type="table"}).

![Mortality over time for all patients in teaching and general hospitals in Scotland on 31 March 2010.](10.1177_0269216314526443-fig1){#fig1-0269216314526443}

The univariate logistic regression showed that every 1 year increase in age at the census date was associated with a 1.04 fold increase in the mortality odds.

In multivariate analyses, men were more likely to die than women (odds ratio (OR): 1.18, 95% confidence interval (CI): 0.95--1.47) as were older patients (OR: 4.99, 95% CI: 3.94--6.33 for those who were 85 years and over compared to those who were under 60 years),


all teaching and general hospitals in Scotland in a method that could be (where facilities and laws allow) replicated elsewhere. We have not yet been able to establish predictors of death within 12 months that relate to clinical or health indicators, such as diagnosis, co-morbidities or previous use of services.

The study is designed as a prevalent cohort study. There are certain implications to this design. One aspect is that patients with longer hospital stays will have a larger chance of becoming part of the 'sample' (though we would regard ours more properly as a 'population'). Indeed, the probability of being sampled is proportional to length of stay (also known as length-biased sampling). This means that the results are not meaningful for individual patients, though of course that ismantleplace. You can have
sex on your mantleplace, if it's big enough, or if you are the data general.,
The word can also get you a slap in the face, or a very (ahem!) intresting
evening. According to the VanMaster sex is highly overrated. It is a very
powerful thing. Most people have it in their power. Most don't, like Matt
Ackeret, and the Champion Eternal, but I wouldn't know. (Check NewsWeek, Mar
14, '62 p.104-05 cover contains Jennifer Kirby for more information...) If you
are incapable of having sex, then life is hard, especially if you're into
masturbation and movies. Sex also brings children, which is a bad side-effect.
It is a common rumor that Sex has a direct link to reproducton, but that is not
true. (Again, check that issue of Newsweek, the one with Jennifer


Kirby on the
cover..) Sex is a new thing to most modern-day teenagers, which is why there is
no such thing as a "sweet sixteen" anymore. In fact, there dosen't seem to be
a "sweet thirteen"...(Once again check that issue of newsweek with the article
on Kirby...) Kinky sex is not advised, as it leaves scars and other noticable
marks on unique parts of the body. We won't go into such things as whips,
chains, vibrators with kickstarters, or canalope. Personally, I don't like
canalope. I like grapefruit. (Again, check that damn articial.) Telephone
sex. What a concept. I, for one, am against telephone sex, because it
destroys the mind, your fantasies, and it's tiring too! Homosexuality makes me
sick, especially in males. Females don't bother me, as I like them anyway. If
god had wanted homosexuality, there wouldRegents Policy Manual ("ABOR Manual") § 4-104 (1987) (amended 1988). In January 2003, the Board amended its policy to provide that "total mandatory undergraduate resident student tuition and fees shall not exceed the amount required to maintain a position at the top of the lower one-third of rates set by all other states for undergraduate resident tuition and mandatory fees at the senior public universities." Id. (2003) (amended 2006).
¶ 4 In March 2003, the Board considered a proposal by the presidents of the three state universities to raise tuition and fees for state residents by 39.1% for the 2003-04 academic year.[2] The presidents claimed that such an increase was necessary in part to service the debt incurred by ongoing and future capital improvements. After a public hearing, the


other revenues approved by the board and allocated to each university operating budget." A.R.S. § 15-1626(A)(13). Neither the Constitution nor our statutes offer guidance on an appropriate sum for a university operating budget, let alone as to which proportions of that budget should be satisfied through appropriated funds, tuition, registration fees, and "other revenues."
¶ 18 Instead, the ultimate size of the budget is left to the discretion of the Board. The Board sets that budget only after making a series of policy decisions about the quality of the state universities and the level of instruction to be offered. These discretionary decisions about class size, the quality of facilities and infrastructure, the pay of faculty and staff, and so ondecisions that the students do not challenge in this caseeither individually or in the aggregate. Even assuming, as the students contend, that Article XI, Section 6, requires that tuition be "reasonable" and not "excessive," there is no North Star to guide a court in making such a determination; at best, we would be substituting our subjective judgment of what is reasonable under all the circumstances for that of the Board and Legislature, the very branches of government to which our Constitution entrusts this decision. The issue of whether tuition is as nearly free as possible is thus a nonjusticiable political question. See Japan Whaling Ass'n v. Am. Cetacean Soc'y, 478 U.S. 221, 230, 106 S.Ct. 2860, 92 L.Ed.2d 166 (1986) ("The Judiciary is particularly ill suited to make such decisions, as `courts are fundamentally underequipped to formulate


tractor cabin, tablet waterproof case and a tripod for the in-field mounting of the RTK Bee Station

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This rocket has a triple solid engine first stage, a single solid engine second stage, and then a liquid fuel third stage. I flew with the SAS system on but during the initial flight you can see the fins on my rocket starting to move; it was almost too much thrust, I think. At any point you can hit the space bar to detach a stage. Solid boosters are fire and forget but the liquid fuel engine has a throttle. You can see fuel levels going down at the bottom left of the screen.

A lot of gamers will watch these videos and be bored. That’s ok, this is definitely a niche product. You can fast forward a bit through the dull parts and you’ll want to


849 F.2d 604Unpublished Disposition
NOTICE: Fourth Circuit I.O.P. 36.6 states that citation of unpublished dispositions is disfavored except for establishing res judicata, estoppel, or the law of the case and requires service of copies of cited unpublished dispositions of the Fourth Circuit.Dock H. DILLMAN, Jr., Plaintiff-Appellant,v.Edward MURRAY;  Fred E. Jordan;  Dave Williams;  I.T.Gilmore;  Keith H. Waldrop, Defendants-Appellees.
No. 87-7728.
United States Court of Appeals, Fourth Circuit.
Submitted:  Jan. 29, 1988.Decided:  June 7, 1988.

Dock H. Dillman, Jr., appellant pro se.
Alan Katz, Office of the Attorney General of Virginia, for appellees.
Before K.K. HALL, JAMES DICKSON PHILLIPS and ERVIN, Circuit Judges.
PER CURIAM:

1
In 1983, Dock H. Dillman, Jr. struck Ivan T. Gilmore, a James River Correctional Facility employee.  Dillman was subsequently convicted of knowingly and willfully inflicting bodily harmvoid testNewThread(){
        new ThreadFactory(){

            @Override
            public Thread newThread(Runnable r) {
                return new Thread();
            }
        }.newThread(new Runnable() {
            @Override
            public void run() {

            }
        });


"Yo." "Maurice!" "Jackie!" "Jack!" "Jackie!" "Jack!" "How you doing?" "And Miss lovely Amber Waves." "I'm pissed you haven't been around." "We were on vacation." "Don't you ever stay away that long from my club again." "And not for nothing, honey, but..." "You are the sexiest bitch in the entire country!" "I love you!" "You're such a charmer." "I got your booth set up." "I'll send some clams over." "Jack." "I'm ready." "I'm available." "Put me in a movie, okay?" "We're talking box office!" "Box office!" "Chi-Chi." "Jack and Amber's table, take them a order of clams." "Let's go!" "Vamos!" "How's it going here?" "Baby, me and you... we'll take a picture later on." "I love you, baby." "We were looking for you before!" "Where were you?" "I was"Class, begin." "I love to suck cock." "I love to suck cock." "Honey?" "You okay?" "Sweetheart?" "Is something wrong?" "I got to get back." "I need it again." "I have to go to work." "Come on, give it to me." "Don't make me pounce you." "I'll do it." "You promise?" "That's it." "You want it?" "How bad?" "Bad." "You sure?" "You asked for it!" "God. wait." "Stop!" "o" "What?" "Your cock is so beautiful." "Do you know how good you are doing it, Eddie?" "Having sex?" "Fucking me?" "Making love to me?" "Everyone has one thing." "Everyone's given one special thing, right?" "That's right." "Everyone's blessed with one special thing." "I want you to know I plan on being a star." "A big bring shining star." "That's what


been with."" "So, what?" "You want me to talk to Jack?" "Yeah." "I mean, what am I asking you here?" "Honey, baby, please, talk to Jack." "Tell him I can do this." "I won't be bad." "You want to be in a movie?" "Baby, please." "I'll see what I can do." "Thank you." "Thank you, mamita." "Maurice, can I talk to you?" "I need to talk you now." "Excuse me." "Can I join in?" "Certainly." "Your cowboy..." "That's not dead." "Then what the fuck is Becky talking about?" "She's got a fucking something up her ass." "Fuck that shit." "Bitch." "Do a cannonball!" "No, no." "Watch this jackknife!" "Did I look cool?" "Pretty good." "I'll show you what you did wrong.!" "Full flip." "You all right?" "m" "Youdefinitely OD'ed." "Fuck me." "I want you to handle this for me, Johnny." "You listening?" "Drive her to Saint Joe's." "Drop her off in the front." "Understand me?" "Got you." "Make sure no one sees the limo." "What is this?" "This is twice in 2 days that a chick has OD'ed on me!" "Think it means you should think about getting new shit?" "Yes sir." "Shit, she's freaking out!" "Look!" "With all this conversation!" "Come on!" "Please don't die!" "Back door, Johnny." "You got it." "Fucking shit!" "Get out of my way." "Bart is she all right?" "Shut the fuck up!" "Scotty J., how are you?" "." "You know, you know." "Who's this?" "Eddie, this is Scotty J. He works on some of the films." "Nice to meet


made it fly." "This is the film..." "I want them to remember me by." "Thank you." "As far as I'm concerned, it's all about love." "You know what I mean?" "If you love someone, how hard can the world be?" "Peole will come and they will go, and so will Problems, but ultimately... if you have got love on your side, and it is just..." "I mean, it is just deep down in your soul... what's a problem that takes your attention away from that?" "Do you understand?" "I'm Becky Barnett." "Jerome." "Nice to meet you." "Nice to meet you, too, Becky." "So, what do you do?" "I'm in the auto industry." "I'm a regional manager over at Pep Boys." "That's great, that's great." "You've got a reallythis conversation." "Hey, Scotty." "What's up?" "Fucking New Year's, right?" "1980." "Oh, man!" "Right!" "Did you see my new car?" "Got a new car?" "Want to see?" "All right." "Cool." "It's out front." "Come on." "I want you to meet my friend Todd." "Todd Parker, Dirk Diggler." "What's up, man?" "How are you?" "We finally meet." "I was telling you about him before." "You remember?" "Todd Parker?" "He works at Party Boys Strip Club?" "Cool." "You're a dancer." "Yeah, I got some moves." "You coming or you want to talk to these guys?" "I'll be around in a little bit and we can talk then, okay?" "See you later, Reed." "When you get my the lights, close your eyes." "Just follow my voice." "Here, here, here, here, here."


in 5 minutes!" "t" "It's like a vacuum in her nose." "Just going up like crazy." "Anyway, she's got all this stuff going on." "Next thing you know, she stopped." "Something must have broken up there because blood poured everywhere." "Pouring out." "You thought she was older..." "You didn't do anything..." "She was just at the..." "She was at your place." "You didn't do anything, right?" "Right." "Nothing." "You didn't do anything?" "Not a thing." "You know me, Jack." "You didn't do anything?" "No, I didn't do anything." "But they... foud something at the house." "What?" "There's something that's..." "Jack, it's my fucking weakness." "They're so small and they're so cute, and they're so adorable." "I just can't help it when they're so cute and adorable." "Jack, listen."don't like being told what to listen to, when to listen to it or anything!" "Fuck it!" "I" "That's Cosmo." "He's Chinese." "That's why he likes lighting off firecrackers." "Ricky Springfield." "He's a buddy of mine!" "o" "Todd, we're leaving, man." "Dirk, let's go, all right?" "Sir..." "We got to split." "You just got here." "Let's hang out." "Let's party." "We got somewhere else to go." "We're not leaving yet." "We're here now, and we want something else from you." "We want something else from you." "What?" "i" "Todd, what are you doing?" "Let's just go." "In the master bedroom..." "N under the bed..., in a floor safe." "Understand?"" "What the fuck is the matter with you?" "Let's go!" "Shut up, Dirk!"" "I told you I got a


"Push, push, push!" "I see a head here." "God Almight!" "Fucking Christ!" "No, don't cuss, sweetie." "One more big push for me, all right?" "Last big push for the doctor." "This is it." "Big push!" "I got it." "I got it!" "He got it!" "r" "It's a boy!" "e" "No hurry guys." "Sometime this year." "Put it where I told you to put it." "You've got to turn the fan on." "It smells good, doesn't it?" "No, it smells like shit." "This is Puerto Rican cooking." "Everybody's complaining in the neighborhood." "They're complaining about this." "Taste this." "I can't taste it, not now." "I'll taste it later." "Rollergirl." "Honey, listen to me." "Move the dirt on one side of your to the other side." "One side of the

Firdousi, a rampart crater (center) on Mercury, illustrates electric arc erosion. Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

The Electrical Etching of Mercury

Sep 09, 2011 The MESSENGER space probe is confirming the Electric Universe theory. MESSENGER entered orbit around Mercury on March 17, 2011 after traveling nearly eight billion kilometers. Since that time, it has sent hundreds of close-up images of the surface, revealing features and topography that assure Mercury's kinship with the Solar System's other celestial bodies: its surface is pitted, gouged, punctured, and grooved in ways so like its sisters and brothers that telling it apart from some of them would be difficult. Past electrical activity on Mercury is evident in several locations around the planet. Indeed, the entire planet could be said to


powerful." "There is power in evil." ""There is power in evil," says the old, potion-brewing wise woman." "And this is a film about the power of evil, the power of evil thoughts, evil intentions, evil appearances." "But is this an evil that belongs to the 17th century or one that exists today?" "Several expert historians have written that Dreyer in his film portrays the age of the great witchcraft persecutions of early modern Europe with an insight that was decades ahead of the historical profession." "Other critics have emphasised the fact that the film was made in 1943, when Denmark was occupied by Nazi Germany, and suggested that the dark world of the film is an allegorical reflection of that grim reality." "Later in this commentary, we shall""the latent tension, the smouldering dread lying beneath the everyday life" ""of the family in the rectory."" "And that tension, that dread was something he felt was essential to bring out." "The drama, to Dreyer, is above all psychological." "In a lecture he gave a few weeks after the opening of Day of Wrath, he said:" ""In the artistic film, it is human beings that we want to see" ""and their psychological experiences we want to experience." ""We wish to get close to and inside the human beings we see on the screen." ""We wish that the film may open a door slightly for us" ""leading onto the world of the inexplicable." ""We wish to be put in a state of suspense" ""caused not so much by the


" You had to renounce God and Christ?" " Yes." "You signed an eternal contract with the devil?" "To Ginzburg, this is extremely significant." "Many historians in recent years have sought to recover the experiences of the little people, those about whom the great chronicles of wars and kings remain silent." "This scene, to Ginzburg, shows the difficulties facing such historians." "Even if the records we see being written were to survive until today, they would still be not the words of the poor woman, but the words of the priest, whose mastery of language reinforces his power over her." "Ginzburg writes that we should view the scene" ""as a confrontation between different cultures," ""and that is evident in the way the judges are dressed" ""while the poorlargely been ignored by commentators." "An important reason for this is, I think, that the clergymen are not depicted as villains." "Absalon's faith, as we can see and hear is obviously sincere." "But the character sketch of Absalon makes clear that Dreyer's sympathy for the man does not extend to his convictions." "Dreyer writes of Absalon:" ""In this man's character" ""otherwise all-of-a-piece," ""there is a single fracture," ""caused by the inner tension between his humaneness" ""and the narrow theological outlook which he preaches." ""He does not doubt that Anne's mother has practised witchcraft" ""and therefore deserves to be burnt at the stake," ""but his humaneness compelled him to spare her life." ""Out of sympathy with the person he kept silent," ""where fidelity to dogma otherwise required him to


taken to represent Nazis, and that is to my mind absurd." "The supernatural abilities which Anne comes to believe herself to possess are deeply morally ambiguous." "The power to kill at a distance, mentioned by Absalon, is one that Anne later in the story will attempt to use to murder her husband, and, at least in her own mind, she will succeed in doing just that." "The powers are also strongly eroticised." "Absalon." "Take me and make me happy." "No, no..." "We have already heard of the burning eyes, and in a moment, we will see how Absalon's inability to recognise Anne's sensual needs is linked directly with his inability to see the fire in her eyes." "Dreyer has held this shot for a very long time, slowlyus to understand why Dreyer insisted on casting the dignified, ascetic-looking Thorkil Roose in the role of Absalon, rather than the man his producers suggested - a robust, fleshy and full-blooded fellow named Eivind Johan-Svendsen." "The latter would have been much closer to the way the original play describes Absalon, but it would have been much harder for audiences to sympathise with such a figure, a dirty old man abusing his powerful position to get a beautiful young girl into his marriage bed." "The Absalon Dreyer shows us may be a fool, but he is also a kindly man, and it is therefore not easy to regard Anne's betrayal of him as an unequivocally good thing." "The contrast between indoors and outdoors is very clear in this sequence,


and it is obviously closely connected to the clash between Anne's sensual nature and the moral order of her society." "But while the film clearly does not support the oppressive and rigid religious system, it does not fully endorse Anne's actions, either." "Becoming a woman will change Anne, but not only for the better." "Hold me close." "Take me and make me happy." "This is the beginning of what I called the fourth act of the film, which corresponds to act three of the play." "In the play, six months are supposed to have passed since the end of the last act and the consummation of Anne's affair with Martin, but here we get no such indication." "We are not shown any documents, but instead we have theever baby boom during and immediately after the war, but there are probably other explanations for this." "Martin is clearly not quite comfortable with the situation." "Dreyer wrote only a brief personality sketch of Martin, which says that: "he is sincere and honest in his feelings for Anne," ""but he is inwardly disjointed, weak and vague" ""and without the courage which, when the great choice must be made," ""bears beyond life and into death."" "The great choice is, of course, the one he must make at the end of the film, where he accepts the idea that he must have been bewitched by Anne and abandons her to face the flames alone." "In the screenplay, Dreyer writes of the scene we are watching that it is intended to


entirely consistent." "One can point to several cases where Dreyer himself does things that he has cautioned against in interviews or published essays." "On the other hand, one should not, as at least one writer has done, question Dreyer's commitment to realism with the observation that he has included an evidently anachronistic object in his set, namely, the heavy sideboard in the background of this shot," "on which the date 1639 is clearly visible." "The film is set in 1623." "Rather, it is evidence of Dreyer's commitment to authenticity that he has had an actual piece of 17th-century furniture brought on to the set, very likely with the intention of helping the actors to get into the mood of the period." "A bit of dialogue that again emphasisesthe propensity of the characters to look for meaning in their surroundings was left out of the finished film at this point." "In the next shot, which for the first time shows Absalon outdoors as he struggles home through the tempestuous weather," "Absalon in the screenplay looks up at the storm-rent sky and says:" ""Look at the sky, the clouds." ""They are like strange letters." ""But where is the one who can decipher the writing?"" "Yet if we look carefully at a shot like this one, it is clear that Bordwell is on to something important." "Bordwell points out that Dreyer's lighting here and elsewhere in the film is strikingly unrealistic." "A lot of the light in these night-time interiors seems to be coming from high above the


functions. Microsoft was able to reproduce the bug and it sounds like they’ve made some progress in understanding it.

But there remained one mystery: this code was supposed to run every thirty seconds, so how come this crash wasn’t hitting every user of Chrome 54? Well, it turns out that floating-point exceptions are, by default, suppressed. When a floating-point instruction does something bad it usually just returns a best-effort result and continues running. I wrote about this a few years ago and recommended that developers try enabling some of these exceptions in order to flush out bugs that would otherwise be hidden.

So now we know why everyone isn’t crashing, but there remained one mystery: why is anyone crashing? If floating-point exceptions are suppressed then shouldn’t this bug have remained$8500mo

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CenturyLink may change, cancel, or substitute offers and services, or vary them by service area, at its sole discretion without notice. All products and services listed are governed by tariffs, terms of service, or terms and conditions posted at centurylink.com. Customers must accept HSI Subscriber Agreement prior to using service. Listed internet speeds vary due to conditions outside of network control, including customer location, equipment, and access through a wireless connection, and are not guaranteed. See centurylink.com/InternetPolicy for additional network performance information. Installation: Type of installation dependent on network technology at customer location. All installations available at no charge. Self install includes all equipment and instructionsFrench officials ban access to sacred mountain which believers claim will be refuge from 'Mayan apocalypse on December 21'

Rumours say the mountain will burst open on December 21 to reveal an alien spaceship which will save those nearby from the apocalypse

French police will control access to the mountain and village to stop expected hordes of New Age fanatics, sightseers and journalists

December 21 is the estimated end of the Mayan long calendar, which some believes marks the end of the world as we know it

Fears the end of the Mayan calendar predicts the end of the world this coming December have run rife on the internet in recent years.

Less well known is the rumour that one particular mountain in south-west France will burst open on that day revealing an


ancient Mayan calendar, and they see Bugarach as one of a few sacred mountains sheltered from the cataclysm.

Eric Freysselinard, France's top official in the area, told AFP: 'We are expecting a few visionaries, a few people who believe in this end of the world, but in extremely limited numbers.

'We are expecting greater numbers of people who are just curious, but in numbers we cannot determine. Above all, we are expecting lots of journalists.'

Expectations: With the Aztec Mayan calendar, pictured, ending on or around December 21 some fear it means the people believed it to be the end of the world

No-go zone: French officials have banned access to the Pic de Bugarach, in south-west France, to avoid a rush of New Age fanatics

Films, documentaries and websites have promoted the  Soumyabrata Dev, , Yee Hui Lee, ,\
    and Stefan Winkler,  [^1] [^2] [^3] [^4]
title: 'Color-based Segmentation of Sky/Cloud Images From Ground-based Cameras'
---

[Shell : Bare Demo of IEEEtran.cls for Journals]{}

Cloud segmentation, whole sky imager, partial least squares regression, SWIMSEG database

Introduction
============

have been extensively studied in the research community over the past few decades. The analysis of clouds and their features is important for a wide variety of applications. For example, it has been used for nowcasting to deliver accurate weather forecasts [@nowcast], rainfall and satellite precipitation estimates [@SP_estimate], in the study of contrails [@contra], and various other day-to-day meteorological applications [@met_app]. Yuan et al. have been investigating the clouds’ vertical structure [@cloud_model_compare] and cloud attenuation for optimizing satellite links [@radiosonde2014].

Sky/cloud imaging can be performed in different ways. Satellite imagery [@PALSAR; @sat_reg] and aerial photographs [@air1] are


that the sky/cloud segmentation problem is dependent on a large number of explanatory independent variables (color channels in this case). Using dimensionality reduction techniques like PCA, we observe the degree of correlation amongst the variables and the amount of variance captured. PCA provides this information based only on the independent input color channels and project the data into new sets of orthogonal axes. In PLS however, both the input color channels and the output labels (sky/cloud) are considered. Using a set of manually defined ground truth images, we model the relationship between the input features and the output label. In the testing stage, we use this estimated model to predict the output labels of the pixels of a given test image.

Suppose, for a sample $\mathbf{X}_{i} \in {\rm I\!R}^{mimperfections in modeling, the values of $\mathbf{Y}_{\mathrm{\mathrm{test}}}$ are not discrete in nature. We do not employ any thresholding at this stage, but rather normalize these values to the range $[0,1]$ ($0=\mbox{sky}, \mbox{ }1=\mbox{cloud}$). These normalized values provide a probabilistic indication of the “belongingness” of a particular pixel to a specific class (i.e. cloud or sky) instead of a binary decision.

Sky/Cloud Image Databases {#sec:database}
=========================

One of the most important pre-requisites for rigorous evaluation of any segmentation algorithm is an annotated dataset of suitable images. Most research groups working on sky/cloud segmentation use their own proprietary images that are not publicly available. In this section, we mention the currently available database containing ground truth images and describe the need for a more comprehensive and consistent database.

HYTA Database
-------------

Till date, the only publicly available


reconstruction of building roofs from airborne [LiDAR]{} data,” , vol. 7, no. 10, pp. 4081–4094, Oct. 2014.

S. Dev, F. Savoy, Y. H. Lee, and S. Winkler, “[WAHRSIS: A]{} low-cost, high-resolution whole sky imager with near-infrared capabilities,” in [*Proc. IS&T/SPIE Infrared Imaging Systems*]{}, 2014.

M. E. Farmer and A. K. Jain, “A wrapper-based approach to image segmentation and classification,” , vol. 14, no. 12, pp. 2060–2072, Dec. 2005.

C. N. Long, J. M. Sabburg, J. Calbó, and D. Pages, “Retrieving cloud characteristics from ground-based daytime color all-sky images,” , vol. 23, no. 5, pp. 633–652, May 2006.

A. Heinle, A. Macke, and A. Srivastav, “Automatic cloud classification of whole sky images,” , vol. 3, no. 3, pp. 557–567, May 2010.

S. Liu, L. Zhang, Z. Zhang, C. Wang, and B. Xiao, “Automatic cloud detection for all-sky images using superpixel segmentation,” , vol. 12, no. 2, pp. 354–358, Feb. 2015.

M. P. Souza-Echer, E. B.expense deduction. The price need not be a fixed one, but may be determinable by costs or other contingencies; but when fixed, its amount (barring use as a device to evade) is the amount of the deduction. Cost or "cost plus" is one of the Government's own methods of contracting. It is not an illicit method for a taxpayer to employ.
But it is urged that since the taxpayer could not itself pick up local business under California law, it cannot be the business of the taxpayer in a legal sense to have a subsidiary do so, and disbursements to have local business brought in are legally foreign to its business, although for its benefit. I do not suppose the taxpayer corporation can itself legally practice law or medicine,


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Gili Lakanfushi Maldives

Maldives

We have but one philosophy here. Leave your worries at home.

This is a place of positive energy, and nothing is ever going to change that. So kick back, relax, and forget about everything but the gentle, warm breeze embracing you. “Named after Robinson Crusoe’s loyal friend, Mr Friday makes your stay as pleasant as possible. Day or night,justice.

Further, they submitted that State of Gujarat has issued circular dated 06.02.2016 to all the Police Station that it is mandatory to register an FIR in cognizable offence. Hon’ble High Court in its order dated 24.09.2018 directed concerned police inspector to take into consideration the complaint filed by petitioner and follow directions issued by Hon’ble Apex Court in the case of Lalita Kumari V/s. Government of Uttar Pradesh and others reported in (2014) 2 SCC 1 as well as in the case of State of Telangana V/s. Habib Abdullah Jeelani and others reported in (2017) 2 SCC 779. Further, court directed to inform petitioner in writing in case the police inspector is of the view that no cognizable offence is made preferably in four weeks.

Hon’ble High Court also


I find that the function of the medians provides a much better estimate of the median of the function than does the estimate of the mean of the function from the function of the means. I am interested in learning the conditions for which this is true.
Question
Under what conditions will the function of a median be closer to the median of a function than the mean of a function is to a function of the mean?
Specifically for what types of $f(x)$ and $x$ is
$$|\mu (f(x)) - f(\mu (x))| > |m (f(x)) - f(m (x))|$$
I previously asked this on here on stats.stackexchange.com, but after not receiving an answer, was advised to post here on MO.
References
Merkle et al 2005 Jensen's inequality for medians. Statistics & Probability Letters, Volume- f(\mu (X)) = pf(a) + (1-p)f(b) - f(pa + (1-p)b) < 0$.
Lemma 2. If for some $a < b < c$, $f(a) = f(c) > f(b)$, then we can find a random variable $X$ such that $\mu (f(X)) - f(\mu (X)) < m(f(X)) - f(m(X))$.
Proof. Fix $\varepsilon > 0$ sufficiently small. Define random variable $X$ as follows: ${\rm P}(X=b) = 1/2 - \varepsilon$, ${\rm P}(X=a) = (1/2 + \varepsilon)(c - b)/(c - a)$, ${\rm P}(X=c) = (1/2 + \varepsilon)(b - a)/(c - a)$. Then, $\mu(X)=m(X)=b$, and ${\rm P}[f(X) = f(b)] = 1/2 - \varepsilon$,  ${\rm P}[f(X) = f(a)]= 1/2 + \varepsilon$. The lemma now follows from $\mu(f(X)) = (1/2 - \varepsilon)f(b) + (1/2 + \varepsilon)f(a) < f(a) = m(f(X))$.
From Lemmas 1 and 2, we conclude:
Corollary.


measure in the House, representing about a third of the House Republican Conference.

Even McConnell has sought to keep a degree of distance from the deal, which fiscal hawks have warned could add as much as $1.7 trillion to the deficit over a decade. In an email urging its passage, McConnell referred to the agreement as the “Administration-Pelosi Budget Deal.”

The agreement to raise spending caps, which averts deep planned spending cuts and increases 2020 spending some $50 billion over current levels, was chiefly negotiated by Speaker Nancy Pelosi Nancy PelosiPelosi slams Trump executive order on pre-existing conditions: It 'isn't worth the paper it's signed on' On The Money: Anxious Democrats push for vote on COVID-19 aid | Pelosi, Mnuchin ready to restart talks | Weekly jobless claims increase |Granulocyte lysosomal cationic protein alters fibrin assembly: a possible mechanism for granulocyte control of clot structure.
The effect of highly positively charged molecules on the assembly and structure of thrombin-induced fibrin gels was studied with turbidity techniques. Lysosomal cationic proteins (LCP) extracted from rabbit heterophils produced enhanced lateral association of fibrin fibers. A crude extract of LCP had little effect on kinetics but produced an increase in the final fiber mass/length ratios. A purified fraction, LCP-5, of the crude extract enhanced both the initial rate of increase and final turbidity of fibrin gels. Mass/length ratios obtained for fibrin fibers as a function of LCP-5 concentration varied from 4.3 X 10(12) in the absence of LCP-5 to 7.8 X 10(12) daltons/cm at 1 microgram LCP-5/ml. Similar studies were conducted with


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    opacity: 0.5;

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The css code are type correctly with # and ".", not like the way it present here. I tried but can't make it correctly

A:

Update your CDN import to
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    <script type="text/javascript" src="http://code.jquery.com/jquery-2.1.4.min.js"></script>

You can find the solution here : jQuery CDN is not loading on LocalHost


the email, and Clinton’s team declined to confirm to her whether the passages are authentic, adding that the Obama administration has “removed any reasonable doubt that the Kremlin has weaponized WikiLeaks to meddle in our election and benefit Donald Trump’s candidacy.” Assuming the excerpts are the real deal, however, it seems fairly obvious why Clinton would not want them to see the light of day in the primary—when she was trying to prove her progressive bona fides and was fighting the perception that she’d be soft on banks—or even the general election. In the excerpts, Clinton presents herself as a finance-friendly moderate who is willing to criticize the industry but who also believes it took an excessive amount of heat for the financial crisis. She also suggests politiciansand that the “conventional wisdom” that U.S. banks were to blame for the worldwide meltdown was an inaccurate “oversimplification.” On a substantive level, that should be a little worrisome for financial-regulation advocates. And politically, Sanders would have had a field day. He also likely would have hammered her for remarks Carrk labeled, “CLINTON SUGGESTS WALL STREET INSIDERS ARE WHAT IS NEEDED TO FIX WALL STREET,” which she offered at the same Goldman symposium:

There’s nothing magic about regulations, too much is bad, too little is bad. How do you get to the golden key, how do we figure out what works? And the people that know the industry better than anybody are the people who work in the industry.

Clinton isn’t outright saying she would populate the Treasury Department with


(Reverse); *IFNA1*: 5′-GCCTCGCCCTTTGCTTTACT-3′ (Forward) and 5′-CTGTGGGTCTCAGGGAGATCA-3′ (Reverse).

3. Results {#sec3}
==========

3.1. Identification of MSC Immunophenotype {#sec3.1}
------------------------------------------

MSCs were obtained from bone marrow aspirates of both healthy volunteers and AS patients. MSCs were cultured and purified to homogeneity according to the culture method described in our previous work \[[@B9]\]. [Figure 1(a)](#fig1){ref-type="fig"} shows adherent MSCs growing like intersecting spindle bundles. In addition, immunophenotyping was performed by flow cytometry. Dot plots showing all (ungated) cells as well as gated MSCs are displayed in [Figure 1(b)](#fig1){ref-type="fig"}. MSCs constitutively expressed CD29, CD44, and CD105 but not CD34, CD45, or HLA-DR ([Figure 1(c)](#fig1){ref-type="fig"}).

3.2. Microarray Hybridization and Data Analysis {#sec3.2}
-----------------------------------------------

The experimental system was stable and fluorescent signal intensity was strong and homogenous. When cultured under inflammatory conditions, the number of differentially expressed genes in MSCs from AS patients was # Optimizer.
       optimizer = tf.train.AdamOptimizer(1e-4).minimize(loss)

       # Predictions for the training, validation, and test data.
       train_prediction = tf.nn.softmax(logits)
       valid_prediction = tf.nn.softmax(model(tf_valid_dataset, False))
       test_prediction = tf.nn.softmax(model(tf_test_dataset, False))

       # Saver
       saver = tf.train.Saver()

     num_steps = 1001
     with tf.Session(graph=graph) as session:
        if restore:
            ckpt = tf.train.get_checkpoint_state('./model/')
            saver.restore(session, ckpt.model_checkpoint_path)


make him come in.”

Neighbors who live nearby the home say the homeowner is an older man who recently started renting out rooms.

“I couldn’t see just anybody moving in because he’s very peculiar and particular about what he does and who he hangs with – he’s an older man. That’s what surprised me the most. These are not younger men, these are older men in their 50’s and 60’s,” Dunbar said.

Questions linger for LMPD as the Homicide Unit is now handling 54 cases.

For Dunbar, she calls the owner a very nice man and said he was the one who discovered the victims inside the home.

She is hopeful police will get some help solving this crime since someone knows something.

Police have not identified the victims.

If you have any information on );

/**

  Uninstall the VirtIo Device

  @param[in] Handle       Handle of the device where the VirtIo Device protocol
                          should have been installed.

  @retval EFI_SUCCESS     The device has been un-initialized successfully.

  @return                 Status code returned by UninstallProtocolInterface
                          Boot Service function.

**/
EFI_STATUS
VirtioMmioUninstallDevice (
  IN EFI_HANDLE


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As a student in our Muay Thai classes, you'll rely on repetition training, powerful striking, and high-intensity cardiovascular movements that produce results across every musclePrep-Ahead Appetizer Recipe

Hosting a party should never be stressful, and to achieve that I plan my menu with recipes where the prep or part of the cooking can be done ahead of time. This recipe fits the bill perfectly.

I assemble and wrap the brie in pastry and refrigerate for up to a day before serving.

Then, about 40 minutes before my guests are expected to arrive, I brush it with egg wash and bake it in a pre-heated oven for about 30 mins.

I take it out, and set it up on my prepared platter with crackers and fruit. That simple!

Using Cranberry Sauce to Flavor Brie

In this recipe, I make baked brie with cranberry sauce. I always make a few extra jars of my homemade cranberry sauce when they are


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» Xiaomi Redmi Note 4 will be available through offline stores in India from March 18 starting at Rs. 11499

Xiaomi Redmi Note 4 will be available through offline stores in India from March 18 starting at Rs. 11499

Xiaomi launched the Redmi Note 4 smartphone in India in January and started selling the smartphone exclusively on Mi.com and Flipkart from 23rd January. It recently said that it sold more than one million units in less than 45 days, making it the fastest selling smartphone in India till date. Today Xiaomi has announced that the smartphone … Continue reading "Xiaomi Redmi Note 4 will be available through offline stores in India from March 18 starting at Rs. 11499"
Read More at:
http://www.fonearena.com/blog/214948/xiaomi-redmi-note-4-will-be-available-through-offline-stores-in-india-from-march-18-starting-at-rs-11499.html

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and BOLD signals increase in the bilateral thalamic. Further studies demonstrated that BOLD signals in different regions were dynamic changes in the time course of GSWDs and BOLD changes in the cortical areas occurred before in the thalamus. These cortical-subcortical structures may form the neural networks associated with GSWDs generation and maintenance. More sophisticated analytic techniques will be developed to explore the BOLD time-course of GSWDs and identify the brain structures involved in seizure onset and discharges propagation respectively. The sub-network associated with different behavioral deficits between interical and ictal GSWDs, and the different subtypes of generalized seizures will be further studied. The functional connectivity of the nodes of the neural network of GSWDs can also be further investigated. A better understanding of the neural network responsible for                                      -2-
       We review a grant of summary judgment de novo. Torgerson v. City of
Rochester, 643 F.3d 1031, 1042 (8th Cir. 2011) (en banc). Summary judgment is
proper if there is no genuine issue as to any material fact and the movant is entitled
to judgment as a matter of law. Id. “[F]acts must be viewed in the light most
favorable to the nonmoving party only if there is a genuine dispute as to those facts.”
Id. (quoting Ricci v. DeStefano, 557 U.S. 557, 586 (2009)).


religion wherever he/she is," he stated

Kaigama condemned the notion that some states were "Muslim states" while some are categorised "Christian states". "This is bad and should be condemned. It does not augur well for the development of the nation. We should be able to worship anywhere and anytime without molestation. We are all the same and worship the same God and should therefore work together in fellowship," Kaigama affirmed.\begin{verbatim}
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Microbial cultures of the microkeratome blade immediately after flap construction in laser in situ keratomileusis.
To assess the incidence of positive cultures from samples of the microkeratome blade after routine laser in situ keratomileusis (LASIK) procedures as a measure of the risk for postoperative infectious keratitis. Hinsdale Surgical Center, Hinsdale, Illinois, USA. In this prospective study, 99 microkeratome blades (Hansatome) were cultured after routine LASIK procedures by multiple surgeons at an ambulatory surgery center. Cultures were sent for routine aerobic and anaerobic growth. Positive cultures were then sent for routine sensitivities. Five of 99 swabs of microkeratome blades were culture positive. Four cultures grew Staphylococcus epidermidis and 1, Staphylococcus warneri. Two of the staphylococcal cultures were resistant to ciprofloxacin and levofloxacin but sensitive to moxifloxacin and gatifloxacin. The studybatters are starting off or at different parts of their careers," said Hazlewood. "The bowling attack is steady and we’ve all pretty much cemented our spots in the team."

Langer revealed Wednesday that, prior to his appointment as the national men’s team coach in all formats earlier this month, he told Cricket Australia’s team performance chief Pat Howard that establishing a strong bond between captain and vice-captain would be a priority if he was handed the job.

And while the Test vice-captain will ultimately need to be ratified by the CA Board, Langer believes Paine’s opinion should be the most important in determining his deputy.

Pakistan survive scare to down Test debutants

"My view has always been that the captain – and this might be a little controversial – should have a


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If you have any questions or proposals please send them through our Contact us form.Group B streptococcal meningitis in adults: report of twelve cases and review.
Group B streptococcus (GBS) is the leading etiologic agent of bacterial meningitis and sepsis during the neonatal period, but it is an infrequent cause of meningitis in adults. We report 12 episodes of group B streptococcal meningitis in adults and review 52 cases reported in the literature. A total of 24 men and 40 women were included in the study; the mean age (+/- SD) was 49.2 +/- 20.5 years (range, 17-89 years). All the patients had cerebrospinal fluid cultures positive for GBS. Eighty-six percent of the patients had comorbid conditions, 50% had a distant focus of infection, and blood cultures yielded GBS for 78.7%. The overall case-fatality rate was 34.4% (22 patients). Factors associated with a


'The Field X-ray AGN Fraction to $\lowercase{z}=0.7$ from the [*Chandra*]{} Multiwavelength Project and the Sloan Digital Sky Survey'
---

Introduction {#intro}
============

A fundamental constraint on all theories modeling the interplay of supermassive black hole (SMBH) accretion and galaxy evolution should be the fraction of galaxies in the local universe that host actively accreting nuclei. Accretion onto a SMBH is the predominant source of energy produced by active galactic nuclei (AGN) and QSOs, so a measure of accretion activity (at a variety of redshifts and luminosities) provides a valuable constraint on the black hole mass function at the present day [@Soltan82; @Rees84; @Marconi04].

In both active and inactive galaxies, observations show a remarkably tight correlation between the properties of galactic spheroids and the masses of their central black holes, the $M_{BH}-\sigma$ relation [@Ferrarese00;supernova remnants, and low- and high-mass X-ray binary populations [@Fabbiano06; @Kim06]; and even in “normal” galaxies a LLAGN may persist [see @Ho08 for a review]. In this work, we consider the X-ray-active fraction of galaxies out to $z = 0.7$, in a field covering more than $20~deg^2$, at a wide range of broad-band X-ray luminosities ($10^{40}$ $L_X$\[0.5-8 keV; ergs$^{-1}$\]  $10^{46}$), including those characteristic of normal and starforming galaxies. Since the many X-ray-producing mechanisms described above can muddy the waters in lower-X-ray-luminosity systems, we focus the bulk of our analysis on sources with X-ray luminosities $L_X$(0.5-8 keV) $ \ge
10^{42}$ ergs$^{-1}$, characteristic of accreting SMBHs.

Measurements of the AGN fraction as a function of environment have been made using both optical spectroscopic samples and optical/radio-selected samples. [@Kauffmann04] use emission-line galaxies in the Sloan Digital Sky Survey


We employ these X-ray and optical surveys to determine the fraction of actively accreting SMBHs (or AGN) out to redshift of $\sim 0.7$. We also explore the AGN fraction as a function of galaxy luminosity, redshift, mass, and host galaxy morphology. Such measures of the AGN fraction will prove useful for constraining the fueling, lifetimes, and growth of central SMBHs.

In §\[catalogs\] we describe the Extended ChaMP ( Cycles 1–6) and SDSS surveys; in §\[sample\_select\] we detail the ChaMP/SDSS sample developed for this study, including specifics on the spectroscopic and photometric redshift catalogs we employ. Section \[properties\] outlines our methods for determining k-corrections, absolute magnitudes, masses, X-ray and optical luminosities, and our definition of five independent samples complete in redshift and $i$-band absolute magnitude. In §\[the\_frac\] we describe our determinationSpectrometer [ACIS; @Weisskopf02] on-board [^1]. The full 130-field Cycle 1–2 X-ray catalog is public [@Kim07b], and the most comprehensive X-ray number counts (log $N$-log $S$) to date have been produced thanks to 6600 sources and massive source-retrieval simulations [@Kim07a].

We have recently expanded our X-ray analysis to cover a total of 392 fields through  Cycle 6 [see detailed descriptions in @Covey08; @Green09], to improve statistics and encompass a wider range of source types — we refer to this expansion as the Extended ChaMP. The new list of  pointings avoids overlapping X-ray observations by eliminating the observation with the shorter exposure time. As described in [@Green04], we also avoid  fields with large (3 ) extended sources in either optical or X-rays (, nearby galaxies M101, NGC 4725, NGC 4457, or


pixels). The threshold maps, computed from the local background intensity, determine the magnitude of the source counts necessary for a detection at each pixel with a detection threshold of $P = 10^{-6}$ (corresponding to 1 false source per $10^6$ pixels). Thus, when an object is not detected at a given location, the threshold map value serves as an upper limit to the source counts, as normalized via the detailed simulated source retrieval results of [@Kim07b]. The [*xskycover*]{} table covers the full Extended ChaMP with sky pixels, each $10' \times 10'$, whose boundaries are chosen to match a regular commensurate grid across the sky. The final sensitivity in any given sky pixel is interpolated from the two threshold maps computed at scales that bracket the size of the pointregion contains 980,214 individual SDSS objects; we refer to this as our “Parent” sample.

To insure the deepest and most uniform X-ray coverage, we exclude area from the ACIS-S S4 chip ([CCD 8]{}) which sustained damage early in the  mission and has high background and streaking as a result. We accept only area with off-axis angles (OAA) $< 12'$ — at larger off-axis angles the PSF broadens considerably and becomes distorted [@Feigelson02; @Kim07a], which leads to large uncertainties in centroiding and source counts. We also exclude area near ACIS chip edges and in chip gaps where the exposure times are significantly shorter. To enforce this criteria, we require that the effective exposure time at each [*xskycover*]{} sky pixel be greater than 80% of the maximum exposure time for the


obsid. These X-ray quality cuts reduce our X-ray sky coverage to $26~deg^2$.

In a number of the  fields the SDSS DR5 data does not cover the full obsid. To crudely quantify the optical coverage of our X-ray fields, we perform visual inspection of the 323 ChaMP/SDSS overlap obsids and assign a coverage fraction to each. An estimate of the sky area based on these rough coverage fractions is approximately $21~deg^2$ and is a lower limit to our actual joint ChaMP-SDSS coverage. The SDSS catalog associated with this sky coverage area contains 483,940 objects (49% of the Parent sample).

For the X-ray-detected subset of the galaxy sample, we apply additional quality constraints. All X-ray-detected objects in the ChaMP survey area are visually inspected, wherein we overplot X-ray centroids and their associatedassigned point source template photo-$z$’s. We eliminate all spectroscopically-confirmed stars from our sample.

Figure \[bestz\_hist\] shows normalized histograms of the redshifts for our “Full” sample (solid black line) and for the spectroscopic sub-sample (gray dashed line). For those objects with both photometric and spectroscopic redshifts, 97% have ${\Delta~z \over (1+z)} < 0.1$ (Fig. \[photz\_specz\]). The photo-$z$ algorithms are the least reliable for quasars (Fig. \[photz\_specz\], filled circles and arrows). We discuss the impact of these potentially large photometric redshift errors on our determination of the AGN fraction in §\[mc\].

To quote a single error estimate on our  value, we utilize and/or convert the redshift errors in each catalog into a $1~\sigma$ Gaussian error. ChaMP spectroscopic redshifts and $1~\sigma$ redshift errors are estimated via radial velocities, using the cross-correlation and emission


$z$, or with both. We discuss these dependencies in §\[agn\_frac\] and §\[discussion\].

Error Estimation via the $\beta$ Distribution {#beta}
---------------------------------------------

We face small number statistics throughout this study, particularly when we bin our modest number of X-ray-detections further by mass, redshift, color,  Statistics used to estimate errors on numbers of events, , the Poisson distribution or the [@Gehrels86] statistic, are not suitable for estimating errors on *fractions*. When it comes to estimating uncertainties on a fraction, one should use the binomial distribution, or its conjugate prior, the $\beta$ distribution [@Evans00]. Given a fraction, $F$, and a number of trials, $N$, the binomial distribution describes the probability of different outcomes. Given the outcome of such a trial, the $\beta$ distribution describes the probability distribution for the fraction itself. Hence, we determine bothmean of the CDF as the best value for the X-ray-active fraction, such that $$F_{mean} = {{\alpha} \over {\alpha + \beta}} = {{N_{det} + 1} \over
  {N_{lim} + 2}}~.
\label{beta_eqn}$$

[The asymmetric $1~\sigma$ errors[^9] are calculated based on the median value of $F$ (evaluated where $P_{\beta} = 0.5$), and defined such that $F_{max}$ corresponds to $P_{\beta}(0.5) + 1~\sigma$ and $F_{min}$ corresponds to $P_{\beta}(0.5) - 1~\sigma$ (see Fig. \[beta\_fig\] for an example). Throughout the remainder of this manuscript (tables excepted), we specify the asymmetric $1~\sigma$ errors *only* in cases where the upper and lower errors differ by more than 10%; in all other cases we quote the larger of the two. (That is, if we have $F\pm^X_Y$, we will quote $F\pm max(X,Y)$, unless $X$ and $Y$ differ by more


bins, the correlation with galaxy mass is similar, but slightly stronger, $\sim$93% and 96% with and without the highest-redshift bin (Fig. \[trends\], right panel).

These trends reveal a field AGN fraction that increases toward brighter absolute magnitudes and higher masses, as might be expected from cosmological models wherein the merger of massive galaxies fuels both accretion onto a central SMBH and star formation. The weaker evolution of the AGN fraction with redshift indicates that the mechanism for black hole fueling may be changing, , shifting from high luminosity merger-driven activity to fueling via tidal interactions, bars, dynamical friction, or other lower luminosity drivers [see @Martini04 for a review]. In such a scenario, the lower AGN fraction may reflect the evolution of the AGN X-ray luminosity function, which is characterizedneighbor approach of [@Ball08], to calculate the new . We also run the MC tests using the QSO $1~\sigma$ errors described in §\[redshift\], instead of the full PDF. The results of those tests show excellent agreement with the MCs that use the QSO PDF. Thus, we do not attempt to acquire full redshift PDFs for all of the objects in our sample.

We use the new  values for non-QSO and QSO objects to determine new luminosity distances, k-corrections, and absolute magnitudes via [kcorrect]{}. We then pull five volume-limited samples analogous to those used for our primary analysis using the new  and its associated $M_i$. We adopt the same seven X-ray luminosity thresholds and calculate new X-ray-active fractions for each.

The above constitutes a single iteration of the full MC. The


AGN fraction at faint apparent magnitudes (and at high-redshift) where morphological criteria are less reliable, and to include all possible QSOs. As a result, the denominator of our fractions is likely to be contaminated by stars and the AGN fractions reported here must be taken as a lower limit to the “true” AGN fraction.

To quantify the magnitude of the stellar contamination, we return to SDSS star-galaxy separation [@Stoughton02]. We assume that all of the point sources with red colors ($u-g>0.6$) *are* actually stars and remove these 27,958 objects along with their X-ray counterparts (120 detections) from our galaxy sample. We re-run our analysis and find mean AGN fractions at $L_X^{\prime} =
10^{42}$ ergsec$^{-1}$ of: $0.16\pm{0.08}$% (sample 1), $0.61\pm{0.14}$% (sample 2), $1.53\pm{0.33}$% (sample 3), $3.45\pm{0.46}$% (sample 4), and $5.71\pm{1.37}$% (sample 5).likely AGN. However, since these objects lie preferentially outside of the limits of our five volume-limited samples — only one X-ray-detection and fewer than 300 galaxies across all five samples appear in our AGN fraction calculations — we do not recalculate $F_{AGN}$ without these objects. We do, however, caution that AGN activity may bias our derived host galaxy properties in a small number of cases and in the highest redshift, highest absolute magnitude sample, in particular.

White dwarfs are another possible contaminant in our galaxy sample. Their blue colors and X-ray brightness can cause them to masquerade as AGN, particularly if they have been incorrectly assigned a cosmological photometric redshift. However, since we removed objects with significant proper motions, we anticipate that these will not contribute more than an


enough cold gas to fuel an AGN, as is the case in the field. In another scenario, red, early-type galaxies may keep their cold gas (despite interactions with cluster potential) and thus continue to host an active SMBH. A third possibility invokes evolution of the AGN fraction in both clusters and in the field — here, AGN activity was more dependent on environment in the past, , closer to the peak in the AGN number density at $z \sim 2$, but at the present day galaxies in both environments are relatively quiescent and the differences between the field and clusters is not discernible. This last scenario can be tested by probing the AGN fraction in both clusters and the field at high redshifts (and possibly in regimes whereauthors [@Georgakakis08b; @Silverman09a] have investigated the AGN fraction in groups of galaxies (or as a function of local over-densities). Using DEEP2  observations from AEGIS for $0.7 < z < 0.9$ and $M_B < -20$, [@Georgakakis08b] find group and field fractions of $4.7\pm{1.6}$% and $4.5\pm{1.0}$%, respectively. This group fraction is about 5 times higher than that reported by [@Martini09] in clusters at similar redshifts. This discrepancy may arise from intrinsic differences in the group and cluster environments at redshifts near $z \sim 1$, but more likely it originates from differences in the X-ray and optical selection criteria of the surveys;  [@Georgakakis08b] include lower-X-ray-luminosity sources than do [@Martini09] and their host galaxy magnitude limits differ. Using only the AEGIS data, [@Georgakakis08b] report a higher AGN fraction in groups than in


the field at $z \sim 1$, but attribute this to their finding that AGN are preferentially found in red, luminous galaxies, which are themselves more likely to reside in higher density environments. They note that an exception to this trend may exist for the most X-ray-luminous AGN, which appear in higher numbers in the field.

[@Silverman09a] also study the X-ray AGN fraction for low-mass host galaxies ($10.4 < {\rm log}~M_{\star} < 11$) in the field and in groups, and find no statistical difference between the fractions in these environments. They do report a trend for log $M_{\star} > 11$, wherein high X-ray luminosity AGN are less common in more dense environs, see also [@Kauffmann04] and [@Constantin08]. For $0.58 < z < 1.05$ and log $M_{\star} > 10.4$, [@Silverman09a] find(or perhaps shifted) at higher-redshift. This may result from evolution in the galaxy population, from smearing due to photo-$z$ uncertainties, or from stellar interlopers. As an illustration of this last possibility, we note that for Sample 1 (Fig. \[greenvalley\], first panel) the peak of the red sequence in the Full galaxy sample (solid black line) is redder than the spectroscopic ALG sample (red dot-dashed line) — this offset may be due to a population of M-dwarf stellar contaminants amongst the objects with photometric redshifts. Here again, contamination of the host color by a luminous central engine may force galaxies out of the green or red portions of the diagram and onto the blue sequence (see §\[bias\]), blurring the expected bi-modality in the underlying galaxy population. However, since such


between accretion onto SMBH and star formation out to $z \sim 1$. Our findings lend additional support to this hypothesis.

It is plausible that the difference between the field AGN fractions from ChaMP/SDSS and zCOSMOS arises from evolution in the AGN fraction. If we assume a mean redshift for the zCOSMOS sample of $z
\sim 0.6$, and a mean redshift of $z \sim 0.3$ for our sample 3, we would expect PLE $(1+z)^3$ evolution in the AGN XLF to yield a zCOSMOS fraction that is a factor of $\sim 2$ higher than the ChaMP/SDSS fraction. Such a correction would bring our results closer to the zCOSMOS blue and green sequence fractions, and achieve agreement in the red sequence. Note that the fractions in the reddest bin would, however, begin toMajok Deng put in 10 points. Ongwae and sophomore Nick Coppola played 40 minutes apiece.

The Ramblers also had four double-figure scorers, led by Earl Peterson's 16 points. Christian Thomas scored 12 points, Montel James 11 and Devon Turk 10.

ULM trailed 10-5 early when it used an 8-0 run to go up 13-10, capped by a lay-in by Ongwae at the 8:14 mark. A three-pointer by Coppola gave the Warhawks a 16-12 edge with 6:58 remaining.

The Ramblers responded with a jumper and three-pointer to go back up 17-16 with 4:40 to go. Samuel hit a pair of three-pointers to put ULM back in the lead, 26-22 at the 1:58 mark. Loyola scored the last bucket of the half, but the Warhawks took a 26-24 advantage into the break.

ULM led


of the way they drove the ball and made plays at the rim. We were trying, it wasn't a lack of effort on our part. Loyola-Chicago just played with more grit and toughness on the offensive end than we did. We played more finesse, a lot of balls tipped out of our hands and missed layups. Loyola-Chicago made all those plays that we didn't and you could see why they've won all the games that they've won. They have a lack of height but it doesn't matter when they play like that offensively. We just couldn't stop them all night long and we're going to have to play at another level defensively if we want to win the next game.”

On any adjustments ULM tried to make in thethe music had been performed, however, the criticism melted away like snow in the sunshine.

A lot of folks called it the Electric Mass, but it was never Catholic, in that sense of the word. The only performances were in churches, mostly in the Midwest or along the Eastern seaboard, and the band never charged a fee for their performance. It was a major success, resulting in invitations to return for more.

After several starts and stops, and name changes, the band had ended up with five guys, all of whom liked classical music but played rock. They played hard, they wrote their own songs for the most part, toured a bit, made a record or two and then one day, for no reason, they just walked away in 1970.

In


indicated that the validated method afforded desired linearity, precision, accuracy, sensitivity and stability. At length, the newly established method was successfully applied to quantify the 10 effective ingredients in JXSZ granules from different production batches, indicating the proposed method in this paper was particularly preferable for the routine analysis of JXSZ preparation as well as the quality control, particularly in situations where high sample throughput and fast analytical speed are required.be hot soon and when i was there at the bottom all the snow was slush and brown snow. im not saying there closing in like 2 weeks. id say about 4 weeks but conditions are gonna get bad pretty fast

It was nice a few days ago. which it wouldve snowed while i was there. but with the heat coming soon go up there while they have a decent amount of snow. id guess there closing pretty soon

Snow has stopped with a nice layer of powder on top. Sun out but blowing hard. Last day today, had everything in the last two weeks. Now Vegas!

Its snowing and blowing right now!

Hot and slushy at the bottom around 11:30-12:00. Top and back country is very nice, little windy but duable.


shown in [Figure 3](#micromachines-10-00742-f003){ref-type="fig"}b. It is worth noting from TEM images that the tubes were hollow and had a uniform thickness at the center, top, and bottom parts. The detailed atomic structure of the TiO~2~ nanotubes was characterized via HRTEM. The HRTEM image in [Figure 2](#micromachines-10-00742-f002){ref-type="fig"}c shows that the ZnO nanotubes were highly crystalline and had lattice fringes corresponding to the anatase phase of TiO~2~.

For energy storage applications, TiO~2~ nanotube arrays prepared by the anodization method were used as electrode materials for supercapacitors. [Figure 4](#micromachines-10-00742-f004){ref-type="fig"} shows the CV curve of TiO~2~ nanotube arrays at different scan rates of 20, 30, 50, 100, 200, 300, 400, and 500 mV/s in the potential window of 0--2.8 V. As shown in [Figure 4](#micromachines-10-00742-f004){ref-type="fig"}, a quasi-rectangularly shaped curve can be clearly seen,electrode was found to exhibit an excellent long cycle life over all of the cycles. The specific capacitance as a function of cycle number was almost constant, even after 250 cycles, indicating the good cycling life of the electrode materials.

The EIS measurements were conducted at the open-circuit potential in the frequency range of 1--100 kHz with an AC perturbation of 100 mV. [Figure 7](#micromachines-10-00742-f007){ref-type="fig"} shows the Nyquist plot of the TiO~2~ nanotube arrays, the impedance plot shows a semicircle arc in the high-frequency, and a linear response in the low-frequency region \[[@B24-micromachines-10-00742]\]. The diameter of the semicircle corresponded to a resistance of 24 Ω, which indicates that the charge transfer resistance of the TiO~2~ nanotube arrays was low, further indicating that the charger transfer was much more conductive.


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Assessment and diagnosis of attention-deficit/hyperactivity disorder by family physicians.
In this study, our aim was to determine the extent to which family physicians in Minnesota follow the American Academy of Pediatrics (AAP) guideline in the assessment and diagnosis of attention-deficit/hyperactivity disorder (ADHD) in school-aged children and to identify barriers to using the guideline. We surveyed 1,000 randomly chosen members of the Minnesota Academy of Family Physicians. Of 303 respondents, 36% always referred children for a diagnosis and 99.7% referred children for a diagnosis of ADHD some of the time. Fifty-four percent were unaware of the AAP guideline. However, among those who said they evaluate children for ADHD, most followed the criteria in the AAP guideline. For example, most family physicians (97%) used a child's response to stimulant medication inFountain Inside Dubai Mall Picture Of Dubai Mall, Dubai

Unique Mall Fountain

On the bridge in the la isla shopping mall picture of la. Amazing water fountain in osaka station city, japan. Hotel restaurant mall unique indoor glass water wall. From singapore to dubai: future blog entry the dubai.


in a brown paper bag (I used a tupperware container).

Place butter, brown sugar, and molasses in the bowl of an electric mixer fitted with paddle attachment. Beat on medium speed until fluffy, about 3 minutes. Beat in egg and vanilla. With mixer on low speed, add flour mixture; beat until just combined. Pinch off dough in tablespoon amounts; roll into 1 1/4-inch balls. Arrange balls 1 1/2 inches apart on prepared baking sheets. (Dough can be frozen at this point, covered tightly with plastic wrap, up to 1 month.)

Bake until cookies are golden and firm to the touch with slight cracking, about 15 minutes, rotating sheets halfway through. Transfer sheets to a wire rack to cool slightly, about 10 minutes. Working in batches, place cookies in paper bag;MILWAUKEE – This is where Al Horford’s load management program starts to pay off. After missing the occasional regular season game, and having his minutes restricted to ease the tendinitis in his knees, Horford is at his most energetic of the year.

The Celtics center’s two-way play – from his 20-point, 11-rebound double-double and primary coverage on Giannis Antetokounmpo to playing 32 minutes – was pivotal in Sunday’s 112-90 Game 1 win over Milwaukee. He’s averaged 34 minutes over five playoff games, including a taxing stretch of 37 minutes in Game 2 and 36 in Game 3 of the Indiana series.

“We’ve said all year you can’t overstate Al Horford’s importance to our team,” said Brad Stevens. “The numbers back that up. It’s his ability to stretch the floor against


outdoor and greenhouse facilities on a relatively small scale.

Village Farms, on the other hand, has over 100+ acres of greenhouse facilities on the BC mainland, about an hour south of Vancouver, with decades of experience producing high-quality produce as well as managing employees and systems, but with no experience growing cannabis.the magnetic field and eventually saturates. However, in certain quantum magnets, flat regions termed as magnetization plateaus appear at fractional magnetizations before saturation. There are two types of magnetization plateaus: a classical one that is described by a collinear arrangement of classical spins and a quantum state comprising entangled spins^[@CR6]^. Classical magnetization plateaus are observed in triangular magnets, such as Cs~2~CuBr~4~^[@CR7]^ and Ba~3~CoSb~2~O~9~^[@CR8],[@CR9]^, and the quantum plateaus in dimer magnets such as NH~4~CuCl~3~^[@CR10]^ and SrCu~2~(BO~3~)~2~^[@CR11]^.

A transition to a quantum plateau as a function of magnetic field is considered to be a superfluid-insulator transition of hard-core bosons (magnons). Interacting magnons in a BEC state tend to localize due to the suppression of kinetic energy and eventually crystallize to become "insulating" such as Mott insulators in strongly correlated electron systems^[@CR12]^.


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                \begin{document}$$\sqrt 3$$\end{document}$ unit cell with *Q*~mag~ = 9 is formed in a range of fields, thereby yielding a 7/9 magnetization plateau. A large magnon is emergently generated on a hexagon of the kagomé lattice in the KAFM, which is significantly different from dimer magnets with singlet and triplet states that naturally occur on built-in pairs of Cu ions.Fig. 1Calculated magnetization process for the spin-1/2 KAFM with the nearest-neighbor interaction(antiferromagnetic) *J*~d~. Larger unit cells, such as *Q*~mag~ = 21 and 36, can be stabilized by weak farther--neighbor interactions or the enlargement of the effective size of hexagonal magnons. Therefore, the appearance of multiple magnetization plateaus in CdK is reasonably explained by assuming a series of magnon crystals in a spin-1/2 KAFM with additional interactions.

Finally, we focus on the reason for the appearance of magnetization plateaus in CdK after the deviation from the calculation based on the *J* + DM model; the smooth rise of the calculated curve indicates that spins are gradually forced to align along the magnetic field from the coplanar **q** = 0 structure as expected for a classical spin system. One possibility is the magnetostriction that induces a lattice distortion^[@CR33]^. For example, a hexagon where a localized magnon lives can


[Mineral density of human skeletal bones in modeling of decreased gravity load].
Bone density in different skeletal compartments was measured in 9 healthy volunteers exposed for 370 days to head-down tilting (-5 degrees). Measurements were carried out using noninvasive techniques: quantitative computer tomography and dual photon absorptiometry (mono- and dichromatic). After bed rest no distinct mineral losses were seen in lumbar vertebrae, femoral diaphysis, tibial diaphysis, or forearm bones of most subjects. Mineral density of the femoral neck decreased in most subjects. The results are discussed with special emphasis on comparative values of the noninvasive methods, variations in the parameters under study during bed rest, and effectiveness of various countermeasures employed.on taxes, step back. Reorient your perspective. Fundamentally, estate planning is not about death and taxes. Instead, the most important goal of estate planning should be to provide "A Legacy for the Living."

Some of the principal elements of estate planning are to execute documents that provide for death and/or incapacity and provide information relating to your assets, liabilities and wishes.

Even after spending a lifetime of work to build an estate, many are reluctant to sit down with family and discuss the details of the estate and how it will eventually be distributed. The subject of death can be difficult to bring up, but in the end discussing your estate plan should be a priority if you want to protect your future and ensure your wishes are carried out


were recorded. Then patients' warfarin dose adjustments according to INR, was done by the clinical pharmacist for one year. Patients received continuous verbal education and written information about warfarin. Main outcome measure The primary outcome for this study was the INR control, while the secondary outcomes were the bleeding events and hospitalization due to warfarin. Results After the clinical pharmacist intervention there was significant (P < 0.01) improvement in INR control and a significant (P < 0.05) reduction in incidence of bleeding after clinical pharmacist intervention. Hospitalization due to warfarin related complications (bleeding, high INR, low INR) was also significantly (P < 0.001) reduced. Conclusion Clinical pharmacists intervention in warfarin therapy improve INR control, reduce bleeding and hospitalization due to warfarin complications.and stuff." "Mushu, if you're so worried, go stand watch." "Yeah, yeah. "Stand watch, Mushu, while I blow our secret with my stupid girlie habits. "" "Pfft!" "Hygiene!" "Me first!" "Me first!" "We're doomed!" "There are a couple of things I know they're bound to notice!" "Whooo-ooo!" "Hey, Ping!" "Oh, hi, guys." "I didn't know you were here." "I was just washing." "So now I'm clean, and I'm gonna go." "Bye-bye." "Come back here." "I know we were jerks to you before, so let's start over." "Hi." "I'm Ling." " And I'm Chien-Po." " Hello, Chien-Po." "And I am Yao!" "King of the rock!" "And there's nothin' you girls can do about it." "Oh, yeah?" "Well, I think Ping and I can take you." " I really don't


far" "You've got the guide" "To find your way" "Let your heart decide" "Be true to your heart You must be true to your heart" "." "That's when the heavens will part" "." "And show the world what you believe in" "." "Open your eyes Your heart can tell you no lies" "." "And when you're true to your heart" "." "Then you've got all you need to make it through" "." "Be true to your heart" "." "Ah, someone you know is on your side" "." "Can set you free" "." "I can do that for you if you believe in me" "." "Why second guess" "." "What feels so right" "." "Just trust your heart" "." "And you'll see the light" "." "Be true to yourdifficulty getting rid of things, I have an empathetic approach and can help them feel better about letting go of unnecessary things that take up valuable space. For the things that must be kept but aren't often used, I can find creative ways to store them out of the way.

For information on scheduling an organizational session, please see the "How it Works" page.


Republicans in Wisconsin look to repeal auto insurance law

Some members of the Wisconsin Legislature are trying to get a law repealed that makes auto insurance coverage mandatory in the state.

According to a report from the Associated Press, Republicans in the state want to get rid of a law that makes auto insurance liability coverage a requirement for drivers. Along with making the coverage mandatory, the bill raised minimums on the amount of liability coverage drivers need, along with increasing minimums for coverage against uninsured and underinsured motorists.

The AP notes that Wisconsin Republican State Senator Mike Ellis is one of the legislators who are looking to repeal the law that Governor Jim Doyle signed this year.

"[Ellis] says the new standards were a 'sloppy kiss' from Democrats to trial attorneyspackage toml

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type valueComplexity int

const (
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)

type sortNode struct {
	key        string
	complexity valueComplexity
}

// Encodes a string to a TOML-compliant multi-line string value
// This function is a clone of the existing encodeTomlString function, except that whitespace characters
// are preserved. Quotation marks and backslashes are also not escaped.
func encodeMultilineTomlString(value string, commented string) string {
	var b bytes.Buffer
	adjacentQuoteCount := 0

	b.WriteString(commented)
	for i, rr := range value {
		if rr != '"' {
			adjacentQuoteCount = 0
		} else {
			adjacentQuoteCount++
		}
		switch rr {
		case '\b':
			b.WriteString(`\b`)
		case '\t':
			b.WriteString("\t")
		case '\n':
			b.WriteString("\n" + commented)
		case '\f':
			b.WriteString(`\f`)
		case '\r':
			b.WriteString("\r")
		case '"':
			if adjacentQuoteCount >= 3 || i == len(value)-1 {
				adjacentQuoteCount = 0
				b.WriteString(`\"`)
			} else {
				b.WriteString(`"`)
			}
		case '\\':
			b.WriteString(`\`)
		default:
			intRr := uint16(rr)
			if intRr < 0x001F {
				b.WriteString(fmt.Sprintf("\\u%0.4X", intRr))
			} else {
				b.WriteRune(rr)
			}
		}
	}
	return b.String()
}

// Encodes a string to a TOML-compliant string value
func encodeTomlString(value string) string {
	var b bytes.Buffer

	for _,


situ carcinoma of the cervix, or other solid tumor treated curatively and without evidence of recurrence for ≥10 years before study entry; any significant serious illness or medical condition; concurrent or prior anticancer treatment (including radiotherapy within 4 weeks of randomization); use of prophylactic antibiotics; prior bone marrow or stem cell transplant; previous therapy with any G-CSF; or infection or positive serology for human immunodeficiency virus (HIV) or hepatitis B or C at screening.

Design {#s4}
------

After a screening period of up to 21 days, eligible patients were randomized 1:1 to 6 mg of either LA-EP2006 (Sandoz, Kundl, Austria, <http://www.sandoz.com/>) or reference pegfilgrastim (Neulasta, Amgen, Thousand Oaks, CA, <http://www.amgen.com/>).

Patients received TAC chemotherapy administered intravenously on day 1 of each cycle and every 3 weeks for up to 6 cycles. G-CSFall cycles. The secondary efficacy parameter of febrile neutropenia included the serious treatment-emergent adverse events (TEAEs) of FN (defined as oral body temperature of ≥38.3°C with ANC \<0.5 × 10^9^/L) and neutropenic sepsis (NS) (referred to as FN/NS). Further ANC was scheduled for each day a patient reported a fever episode, the next day, and every other day thereafter until the ANC reached a value \>0.5 × 10^9^/L. Neutropenic sepsis was identified by adverse event documentation page, selecting all neutropenic sepsis events as recorded by the investigator.

Safety was assessed through the incidence and occurrence of TEAEs by severity according to Common Terminology Criteria for Adverse Events, version 4.0. The safety follow-up visit was performed 4 weeks after the final administration of pegfilgrastim. Immunogenicity of pegfilgrastim, filgrastim, and polyethylene


one place.
Replacements in the source tree: You want to add code into the source tree? A variable really should be a function call? Wrap a macro around the code that 'walks' the source and changes the places where it finds the variable.
Postfix syntax: You want to write your code in postfix form? Use a macro that rewrites the code to the normal form (prefix in Lisp).
Compile-time effects: You need to run some code in the compiler environment to inform the development environment about definitions? Macros can generate code that runs at compile time.
Code simplifications/optimizations at compile-time: You want to simplify some code at compile time? Use a macro that does the simplification - that way you can shift work from runtime to compile time, based on the sourceobservational, cross-sectional, and descriptive study conducted at a hospital-based tertiary-level ophthalmology and otorhinolaryngology outpatient clinic in São Paulo, Brazil. The study protocol complied with the tenets of the Declaration of Helsinki, was approved by the Institutional Review Board of the University of São Paulo Medical School, and all participants gave their informed written consent.

Between May 2016 and August 2017, 17 patients with bilateral proptosis defined as clinical exophthalmometry readings greater than 20 mm due to orbital diseases were recruited. We also recruited 15 patients with normal orbits who had recently been submitted to CT scanning for nasal evaluation. The inclusion criteria were: (i) age above 21 years, (ii) absence of ocular abnormalities such as degenerative myopia, microphthalmos, and anophthalmic socket, (iii) absence of orbital abnormalities such as previous fractures