2012.

Piaker, Zachary. “No ‘New World Order.’ ” 5 Nov 2014.

Lobosco, Katie. “Walmart fired 2,200 to fix the plumbing.” CNN Money. 17 Apr 2015.

Garcia, Ahiza. “Wal-Mart: ‘No Truth To The Rumors’ Of Tunnels Being Built To Take Over Texas.” TPM. 4 May 2015.primer has a copper cup and is sealed with a heavy red lacquer. The propellant charge is a ball powder with similar burning characteristics to the WC844 powder used in 5.56×45mm NATO ammunition. The 7N6 cartridge weight is .

Tests indicate the free recoil energy delivered by the 5.45×39mm AK-74 assault rifle is , compared to  delivered by the 5.56×45mm NATO in the M16 assault rifle and  delivered by the 7.62×39mm in the AKM assault rifle.

Military 5.45×39mm ammunition was produced in the former Soviet Union, GDR and Yugoslavia, and is produced in Bulgaria, Poland and Romania. In the former Soviet Union this ammunition is produced in Russia, Kyrgyzstan, Uzbekistan and Ukraine.

Cartridge dimensions
The 5.45×39mm has 1.75 ml (27 grains ) cartridge case capacity.

5.45×39mm maximum C.I.P. cartridge dimensions.

Americans would define the


United States.

The 7N10 "improved penetration" cartridge was introduced in 1992. The 7N10 boat-tail bullet weighs  and the weight of the lengthened sleeker steel (high-carbon steel U12A) penetrator made of steel 70 was increased to  and the lead plug in front of it was discarded. The hollow cavity at the front of these projectiles was reduced significantly compared to previous 7N6(M) projectiles.
In 1994 the 7N10 design was improved by filling the remaining hollow cavity in the projectiles front with lead and reducing the weight of the penetrator to  resulting in a bullet weighing . Upon impacting a hard target, soft lead is pressed sideways by the steel penetrator, tearing the jacket. It has a ballistic coefficient (G1 BC) of approximately 0.351 and (G7 BC) ofmeans).

Browse 2.Browse this gallery for inspiration.

3. Add a cutting tool to your inventory.

4. Stab the pumpkin repeatedly, until it resembles something from the world of Destiny.

5. Take a picture, and upload it somewhere.

Share your work in the comments below, or on 6.Share your work in the comments below, or on Facebook

On Sunday, October 27th, we’ll create a Facebook gallery with finalists chosen by us. On the day after Halloween, the seven sculpted creations with the most Likes will win a Beta Code.

Scare up some elbow grease and get to work.


S Washington St, Pioneer Square, 206-467-7253; www.sakenomi.us

Puerto Rican Late-Night Happy HourLA ISLA began as a Puerto Rican snack vendor at the Fremont Farmers Market, and a casual street-food vibe remains inside the restaurant’s permanent location on Market Street. At dinner you’ll eat alongside Ballard babes picking at their plátanos, but the party picks up around 10pm, when the price of mojitos drops to $3, and all appetizers are half off.La Isla, 2320 NW Market St, Ballard, 206-789-0516; www.laislaseattle.com

Irish HurlingSnicker at the fake sword–wielding wannabe knights of the Society for Creative Anachronism if you must, Seattle, but without them, you might never see a centuries-old Irish field game in Magnolia Park. Back in 2003, local SCA “knight” Rob Mullin was gettin’ medieval in the mountains of Oregon when heyear. Watch out for the guys dressed in foam beer-bottle suits—they’re nothing but trouble. Seattle International Beer Festival, www.seattlebeerfest.com

International CricketSEATTLECRICKETCLUB’s bowlers and batsmen have waged polite war in local parks since 1964, but it wasn’t until Microsoft brought waves of Indian and Pakistani programmers to the area that the SCC really found its groove. Like rec-league refugees, the club bounced from one public space to the next for decades before settling in Magnuson Park three years ago. Curious locals freaked out by cricket’s nearly indecipherable rules need not fear: Club president Bunti Sarai says players are happy to teach newbies the ways of the wicket. Seattle Cricket Club, www.seattlecricket.com

Australian-Rules FootballNine months after landing in Seattle in early 1998, Aussie Matt Muller decided the best way to cure his


- it's a principal aim of modern theoretical physics. But Perimeter has chosen an unconventional route. Much of the physics community is chasing superstring theory, the idea that the fundamental particles in the universe are actually multidimensional strings vibrating at different frequencies. But Smolin and Markopoulou Kalamara are specialists in loop quantum gravity, which holds that space-time is a foamy network of intersecting loops known as spin networks. "So what if they've placed a few bets that aren't broadly supported?" asks Sylvester J. Gates Jr., a physicist at the University of Maryland. "In physics, it doesn't matter if you're in the majority. It matters if you're right."

Perimeter has also recruited thinkers known for interdisciplinary cooperation, a rarity in a field where specialization is the rule. Smolin, for example,Christopher Phipps in Kendall, Florida a suburb of Miami in late 1986, with brother John Phipps, female vocalist BeBe Cager older sister of Elana Cager of the group L'Trimm,
Producer David Hanono of The Voice In Fashion and Engineer Douglas Edwards who Hanono had recruited from his bands' label Pantera Records.

Taking Dance/Freestyle that was the cutting edge music of the time, and wanting to combine it with Synthpop/New Wave music from the early 80's Pre-Production started with future London Exchange Producer Peter Marr at his home studio in early 1987.
The band started their first actual recording session at The University of Miami studio in February 1987.
During these recording sessions which took place at various studios around Miami over several months future London Exchange member Jose Conde was


Q:

REST Easy Webservice

Hi I have Implemented a RESTful webservice using JBOSS-Rest Easy.
Each REST service has instance variable which provides service methods.
Does having instance variables make  restful web services thread unsafe ?
Is there any thing else i need to do to make them ThreadSafe ?

A:

Does having instance variables make restful web services thread
  unsafe?

No, having instance variables does not make your Resteasy resources unsafe.  Resteasy resources are created on a per-request basis by default.

immunosuppressive medication in transplant patients \[[@pone.0184034.ref004], [@pone.0184034.ref005]\]. Squamous cell carcinoma is characterized by aneuploidy and deletions of several chromosomes (3p, 9q, 9p,13q, 17p, 17q) and P53 mutations \[[@pone.0184034.ref005]\]. Despite the generally good prognosis of cSCC, the metastatic SCC is difficult to treat and can be lethal \[[@pone.0184034.ref006]\]. Low-risk cSCCs have a high cure rate when treated with excision followed by histopathological analysis, electrodessication and curettage or cryosurgery \[[@pone.0184034.ref007]\]. For invasive cSCC surgical excision or Mohs micrographic surgery are the most appropriate and effective treatment modalities. Radiation therapy can be used as primary treatment for lesions that cannot be surgically excised \[[@pone.0184034.ref004]\]. Metastatic cSCC can be responsive to some chemotherapeutic agents e.g. cisplatin as a single agent or in combination with 5-fluorouracil (5-FU) \[[@pone.0184034.ref008]\]. EGFR inhibitors such as cetuximab


concentrations of 25 μM, 50 μM and 100 μM) were added to wells. Cells were harvested after 24 h using 0.25% trypsin with EDTA. Harvested cells were centrifuged, resuspended in fresh media, stained with trypan blue (1:1 ratio) and counted using EVE Automated Cell Counte (NANOENTEK USA INC). All experiments were performed in triplicates.

Statistical analysis {#sec012}
====================

Prior the analysis, the dataset has been checked with Dixon test to remove outliers. Breakdown and one-way ANOVA has been applied to test the hypotheses that different concentrations of selected compounds are significantly changing the cell viability. Newman-Keuls post hoc test (p = 0.05) was used to check differences in absorbance of investigated compounds at various concentrations within three cell lines.

Comparison between different cell lines at the same concentrations have been analyzed by   85±0.5
  MR5             80±0.4
  MR6             79±0.9
  MR7             77±1.5
  MR8             70±0.6

Morphology of isolated cells {#sec015}
----------------------------

Cells isolated from human skin exhibited typical epithelioid morphology ([S3a Fig](#pone.0184034.s003){ref-type="supplementary-material"}). Isolated keratinocytes did not require a fibroblast feeder layer to support their growth. Cells were not immortalized and after third passage cell populations became more heterogeneous, displaying outstretched shape and enlarged cytoplasm with ultrastructural alterations ([S3b Fig](#pone.0184034.s003){ref-type="supplementary-material"}). Although nuclei did not change in size, they presented irregular shapes. Also in


the older passages, cell division was inhibited or was very slow. Isolated skin keratinocytes (sHEK) stained positively with anti-cytokeratin 14 (CK14) antibody ([S3c Fig](#pone.0184034.s003){ref-type="supplementary-material"}).

Anti-Ki-67 antibodies staining {#sec016}
------------------------------

Untreated cells stained positively with anti-Ki-67. The average value of proliferation index Ki-67 shown as mean ± SD in SCC-25 cell line was 62.63±13,62%, in isolated sHEK cells was 35,5±9,29% and for HEKa was 53,00±16,52% ([S4 Fig](#pone.0184034.s004){ref-type="supplementary-material"}). Obtained results indicate differences in cell proliferation rate between cell lines, and isolated keratinocytes sHEK showed the lowest percentage of proliferating cells.

Cell viability {#sec017}
--------------

Cell viability, presented on graphs as an absorbance, was determined by the MTS assay and calculated by comparison to the control. We have not observed decrease in cell viability treated with 10% DMSO in water. The obtained data showed decrease in cellcolors were used. The variants differ significantly only if the asterisk color is various. Black asterisk means that selected variant differs with all the others. In contrast, the same color indicates that difference is statistically irrelevant. Moreover, number of asterisks (\*; \*\* or \*\*\*) refers to p \< 0.05; p \< 0.01 and p \< 0.005, respectively.](pone.0184034.g004){#pone.0184034.g004}

Addition of MR1 caused significant decrease of cell viability in case of SCC-25 cells for all hydrolysate concentrations used (p\<0.005). In the case of sHEK and HEKa cells, treatment with MR1 caused significant decrease of cell viability compared to control (p\<0.005 and p\<0.05, respectively). No change between variants with different concentrations was observed ([Fig 3](#pone.0184034.g003){ref-type="fig"}).

The smallest impact on cell viability was observed for MR2 ([Fig 4](#pone.0184034.g004){ref-type="fig"}). For SCC-25 cells only the highest


from this study suggest, that obtained wool hydrolysates can be used as a potential source of anticancer drugs.

Studies about isolation, characterization and cytotoxicity of biofunctional keratin particles extracted from wool were performed in the recent few years. J. Zhang et al. examined the nontoxicity and biocompatibility of wool fibers hydrolyzed in the acidic environment using hydrochloric acid \[[@pone.0184034.ref031]\]. The results showed that keratin particles KP3 and KP5 (at concentrations of 0.1 mg/ml and 1 mg/ml, respectively), possessed expedient impact on cell viability of fibroblasts cell line. These results demonstrated that both keratin particles could be tailored from wool hydrolyzed solution and had potential future application as biomaterials for wound healing and drug delivery. Another study by Li et al. revealed that 0.5 mg/ml of wool hydrolysate PP5.55 hadof hydrolysates.

(TIF)

######

Click here for additional data file.

###### Absorbance spectrum of commercial compounds (a) and two hydrolysates (b), as a control group was used dimethyl sulfoxide (DMSO) in water.

The peak of absorbance spectrum of used substances do not overlap with MTS/formazan peak absorbance between 450-500nm.

(TIFF)

######

Click here for additional data file.

###### Isolated sHEK cells under light microscope (a---second passage, b---fourth passage) and stained with CK14 (c).

Magnification 100x.

(TIF)

######

Click here for additional data file.

###### Proliferation index for cell lines SCC-25, sHEK and HEKa after 24h of incubation.

Statistical analysis used average values and comparison tests (ANOVA, Kruskal-Wallis/Dunn\'s Multiple Comparison tests) with Prism (\* p\<0,05).

(TIF)

######

Click here for additional data file.

###### Viability of cells treated with hydrolysates and stained with trypan blue after 24h of incubation.

Statistical significance: (\*) p\<0.05, (\*\*) p\<0.01,


Ontario’s medical regulator wants to force a former patient in a Toronto doctor’s ongoing sexual abuse discipline hearing to testify by having her arrested by the police.

As far as the College of Physicians and Surgeons of Ontario is aware, it is the first time it has sought what is known as a bench warrant from a judge in order to compel a reluctant witness to give evidence.

The refusal by the witness — known as Patient A due to a publication ban — to appear at the college has put the matter of Dr. Suganthan Kayilasanathan in jeopardy.

Without her, there is likely no case against the doctor, who is facing allegations of sexual abuse of a patient and unprofessional conduct, which he denies.

The case raises the obvious question ofof the Liver or Kidney, Alcoholism or Drug Addiction, or Immune Disorder?
Question "2" asks whether the applicant has been absent from work during the last year for more than five consecutive days due to a back or neck disorder. On Schlemmer's application form, the boxes labeled "No" are checked beside both questions. Farther down on the page, and immediately above Schlemmer's signature, is the printed statement, "I have read and understand this page and my answers to the health questions are true."
¶ 8 In August of 1998, Schlemmer submitted a claim to North Central for the disability benefits under the credit life and disability policy. North Central investigated the claim and learned that, at the time he applied for the disability insurance, Schlemmer had been treated within the


write these very words, dear reader, made my mind go blank. Very unusually I had no idea where to start, I had no idea what to write, I had no idea how to interest you. Now, for those readers who have not come across me in the media, in my books, on my site or through my talks or training, you need to understand that this is unusual. In fact, it's something I pride myself in, the ability to always find a way forward, but when it came to telling you about Gratitude my mind went completely blank.

So I have no idea where these blogs are going, I know the theme is Gratitude. I have several ideas, concepts I want to share, experiences that have influenced me. Weanswer to this question is, indeed, yes, and in fact (in the non-CM case) an analogue of the strong multiplicity one theorem holds: not only can we exclude finitely many primes, or a set of primes of density zero, but even a set of sufficiently small positive density. Here, the density we use is the analytic density defined as follows: a set $E$ of primes has density $\kappa>0$ if and only if $$\label{eq-density}
\sum_{p\in E}{\frac{1}{p^{\sigma}}}\sim \kappa
\sum_{p}{\frac{1}{p^{\sigma}}}\sim -\kappa\log(\sigma-1)
\qquad
(\sigma\to 1+).$$

We will prove:

\[th-1\] Let $k_1, k_2\geq 2$ be even integers, let $N_1, N_2\geq 1$ be integers and $f_1\in {\rm H}_{k_1}^*(N_1)$, $f_2\in {\rm
    H}_{k_2}^*(N_2)$.

*(1)* If the signs of $\lambda_{f_1}(p)$ and $\lambda_{f_2}(p)$ are the same for all $p$ except those in a set of analytic density $0$, then $f_1=f_2$.

*(2)* Assume that


notation as before, we have the lower bound $$\label{pointdepart}
S(f,y^u)\ge \sum_{n\le y^u} h_y(n)$$ for all $u< \kappa$, provided $y$ is large enough, e.g., $y\geq
N^{1/3}$ with $N$ large enough, which we can obviously assume in proving Theorem \[th-1\].

Indeed, let $g_y$ be the multiplicative function defined by the Dirichlet convolution identity $$\lambda_f=g_y*h_y,$$ then $g_y(n)\geq 0$ for all squarefree integers $n\geq 1$ such that $(n, N)=1$, since $$g_y(p)=\lambda_f(p)-h_y(p)\geq 0$$ for all $p\nmid N$ (the case $p\geq y$ following from Deligne’s inequality). We have trivially $$\sum_{n\leq z}{h_y(n)}\geq 0$$ if $z\leq y$ since each term is non-negative in that range, and additionally $$\sum_{n\leq y^u}{h_y(n)}\geq 0$$ for $u<\kappa$ if $y$ is large enough, by Lemma \[lm-h\].

Hence $$S(f,y^u)=\sumb_{{\substack{{{n\leq y^u}}\\{{(n,N)=1}}}}} {\lambda_f(n)}
=\sumb_{d\leq y^u}{g_y(d)\sumb_{\ell\leq y^u/d}{h_y(\ell)}} \\
\geq
\sumb_{\ell\leq y^u}{h_y(\ell)}$$ since every term in the sum over $d$ is non-negative and $g_y(1)=1$.

We now deduce$\eps_p=1$ for all $p$ (handling the other choices of signs being merely a matter of complicating the notation).

To simplify notation, we write $P=P_N(z)$ the product of primes $\leq
z$ coprime with $N$, and $\omega$ the number of such primes.

First, if we wanted only to have $\lambda_f(p)\geq 0$ for a fixed (finite) set of primes (i.e., for $z$ fixed), we would be immediately done: Proposition \[pr-equi\] shows[^6] that the $(\theta_f(p))_{p\mid P}$ become equidistributed as $kN{\rightarrow}+\infty$ with respect to the product Sato-Tate measure, if we weigh modular forms with $\omega_f$, and hence $$\sum_{{\substack{{{f\in{\mathrm{H}}_k^*(N)}}\\{{p\mid P\Rightarrow \lambda_f(p)\geq
    0}}}}}{\omega_f}{\rightarrow}\mu_{ST}([0,\pi/2])^{\omega}=\Bigl(\frac{1}{2}\Bigr)^{\omega}$$ which is of the desired type, except for the presence of the weight.[^7] However, we want to have $$\lambda_f(p)\geq 0\text{ for } p\leq z,\ (p,N)=1,$$ where $z$ grows with $kN$, and this involves


the left-hand side (which is a sum of non-negative terms) which is unbounded as $\sigma$ tends to $1+$. Since Rankin-Selberg theory also gives $$\label{eq-rs2}
\sum_{p}{\frac{\lambda_{f_1}(p)^2}{p^{\sigma}}}\sim -\log(\sigma-1)
\qquad
(\sigma\to 1+),$$ the only difficulty is that one might fear that the coefficients of $f_1$ and $f_2$ are such that whenever $\lambda_{f_1}(p)$ is not small, the value of $\lambda_{f_2}(p)$ *is* very small.[^10] In other words, we must show that the smaller order of magnitude of (\[eq-rs\]) compared with (\[eq-rs2\]) is not due to the small size of the summands, but to sign compensations. For this we use the following trick which exploits the little partial information known towards the pair Sato-Tate conjecture.

Assume first that $f_1$ and $f_2$ are non-CM cusp forms, and that neither is a quadratic twist of the other (in particular, $f_1\not=f_2$). By Ramakrishnan’sdistributed,[^11] i.e., we have $$\sum_{p} \frac{X_k(x_p)}{p^{\sigma}}
= O(1)
\qquad{\rm and}\qquad
\sum_{p} \frac{X_k(y_p)}{p^{\sigma}}
=O(1)$$ for $\sigma>1$ and $1\leq k\leq 5$, and yet $x_py_p\geq 0$ for all $p$, in fact $x_py_p=0$, so that we most certainly have $$\sum_{p} \frac{x_py_p}{p^{\sigma}}=O(1)
\qquad(\sigma>1).$$

As a final remark, one can think of other ways (than looking at signs) of reducing Fourier coefficients of modular forms to a fixed finite set: the most obvious, at least if $f$ has integral coefficients $\lambda_f(n)n^{(k-1)/2}$, is to look at the coefficients modulo some fixed prime number $\ell$. However, the situation there can be drastically different: for instance, for all (infinitely many) elliptic curves with full rational $2$-torsion, given for instance by equations $$y^2=(x-a)(x-b)(x-c)$$ with $a$, $b$, $c$ distinct integers, the reduction modulo $2$ of the odd prime coefficients of the corresponding $L$-function (or modular


the fire fighting art for mounting the thermal or infrared camera of such a thermal imaging system in a temperature protected manner so as to reduce the influence of a heated environment such as is present at a fire scene, on the camera which is thermal sensitive.
Firefighters, emergency responders and some industrial workers are exposed to extremely hazardous, toxic and hostile atmospheres in the fulfillment of their assigned duties. To accommodate the lethal atmosphere, these workers use what is called self-contained breathing apparatus. The self-contained breathing apparatus most often is an open-circuit breathing apparatus where compressed air is carried on the back in a carefully engineered, user friendly harness which spreads the load of the cylinder weight onto the user in a way that minimizes the discomfort andmounted to a pod below the rim of the helmet with a heads-up display mounted at the front of the helmet. A counterweight is mounted at the rear of the helmet, and a power and electronic processing unit is displaced from the helmet by a series of wires. This product made the helmet mounted thermal imager an actual practicality for a broad spectrum of uses, not the least of which is firefighting and emergency response.
Helmets are still very heavy. Neck fatigue remains a factor, and continuity of operations also becomes more difficult because when the need for the thermal imager and its additional weight are removed as a consequence of the atmosphere becoming clear and/or breathable, the thermal imager user typically has to remove himself from the scene,


known at high redshift. Photo-dissociation region modeling suggests physical conditions similar to nearby SFGs, showing extended [star formation]{}, which is consistent with our finding that the gas and dust emission are co-spatial. Its molecular gas excitation resembles the local major merger Arp220. The broad CO and [\[C[II]{}\]]{}lines and a pair of compact dust nuclei suggest the presence of a late-stage major merger at the center of the extended disk, again reminiscent of Arp220. The observed gas kinematics and conditions together with the presence of a companion and the pair of nuclei suggest that [HXMM05]{}is experiencing multiple mergers as a part of the evolution.'
author:
- 'T. K. Daisy Leung'
- 'Dominik A. Riechers'
- 'Andrew J. Baker'
- 'Dave L. Clements'
- Asantha Cooray
- 'Christopher C. Hayward'
- 'R. J. Ivison'
- Roberto Neri
- Alain Omont
- 'IsmaelPérez-Fournon'
- Douglas Scott
- 'Julie L. Wardlow'
bibliography:
- 'ref.bib'
title: ' The ISM Properties and Gas Kinematics of a Redshift 3 Massive Dusty Star-forming Galaxy '
---

Introduction {#sec:intro}
============

Most of the stellar mass in the Universe is assembled in the first few billion years of cosmic time, in the redshift range 1$\lesssim$$z$$\lesssim$3 [see e.g., review by @Madau14a]. Galaxies at this epoch typically have higher star formation rates (SFRs) compared to the present day. Among the [high-$z$]{}galaxy populations discovered, dusty star-forming galaxies (DSFGs) represent the most IR-luminous systems at this peak epoch. They are typically gas-rich, with molecular gas masses exceeding $=$10$^{10}$ and IR luminosities exceeding those of nearby (ultra-)luminous infrared galaxies (U/LIRG; $>$10$^{11-13}$; see reviews by @CW13 [@Casey14a]). Given the differences found between nearby ULIRGs and [high-$z$]{}DSFGs [e.g., @Younger10a; @Rujopakarn11a; @Rujopakarn13a], studying their


on a flux density threshold of $S_{\rm 500}\geq$80mJy at 500$\micron$. The surface density of such bright DSFGs is (0.31[$\pm$]{}0.06)deg$^{-2}$ (@Wardlow13a). Previous high-resolution imaging obtained with the [*Hubble Space Telescope (HST)*]{} and ALMA and lens modeling of $0\farcs4$ resolution dust continuum data at 870$\micron$ show that [HXMM05]{}is at most weakly lensed, with magnification factor $\mu_{870} \lesssim1.4$ [@Bussmann15a][^1]. [HXMM05]{}is therefore intrinsically extremely IR-luminous, unlike other typically strongly-lensed DFSGs in the parent sample with similar sub-millimeter flux densities. @Bussmann15a find a total of three unlensed, intrinsically-bright DSFGs out of the parent sample of 29. This yields a surface density of $\sim$0.03deg$^{-2}$ for such sources, which makes them even rarer than strongly-lensed DSFGs. [HXMM05]{}therefore belongs to a rare and understudied luminous/massive [high-$z$]{}galaxy population. Currently, the general consensus is these unlensed DSFG with& 3C147 & 3C147 & J0215$-$0222 & 121$\times$080, 36$\degr$ & DnC & Ka-band\
&& 17-Nov – 11-Dec-2014 & 8.96 & J0542$+$4951 & J0542$+$4951 & — & — & C & —\
[\[C[II]{}\]]{}& ALMA 12m& 15-Jun-2015 & 0.15 & J2232$+$1143 & Ceres & J0241$-$0815 & 018$\times$014, 61.3$\degr$ & 21$-$784 \[m\] & 472.661\
& & 27-Aug-2015 & 0.15 & J0224$+$0659 & J0224$+$0659 & J0241$-$0815 & — & 15$-$1574 \[m\] & 472.665\
& ALMA ACA& 11-Sep-2017 & 0.45 & J0006$-$0623 & Uranus & J0217$+$0144 & 535$\times$365, $-$85$\degr$ & ACA & 289.995\
& & 16-Sep-2017 & 0.45 & J0522$-$3627 & — & — & — & — & —

(CARMA)
--------

Based on the [*Herschel*]{}/SPIRE multi-band colors of $S_{\rm 500} < S_{\rm 250} < S_{\rm 350}$, we expected the redshift of [HXMM05]{}to be 2$\lesssim z \lesssim$3.5, and its line


the remaining nine sessions were carried out between 2014 November 17 and December 11 in the C array configuration, A total of 10.5hours of on-source time was obtained in the combined ten sessions. The Ka-band receivers were used to cover the redshifted line. The WIDAR correlator was used in full polarization mode, providing a total bandwidth of 2GHz covered by sixteen sub-bands, each with a bandwidth of 128MHz and a channel spacing of 2MHz (29[kms$^{-1}$]{}). Calibrators are listed in [Table \[tab:obssum\]]{}. We estimate a flux calibration accuracy of $\lesssim$15%.

Visibility data were calibrated and analyzed using version 4.7.1 of the package. We combined all calibrated data and imaged the visibilities using the CLEAN algorithm with natural weighting to maximize sensitivity, yielding a synthesized beam size of 121$\times$080 at PA[=]{}36$\degr$. Thethe line profile shape, we create two [\[C[II]{}\]]{}line cubes — with and without $uv$-tapering (see [§\[sec:obs\]]{}). The 635$\micron$ continuum emission has been subtracted from both line cubes in the $uv$-plane. We collapse them to form velocity-integrated line intensity (i.e., zeroth moment) maps as shown in [Figure \[fig:mom0\]]{}. We show the [\[C[II]{}\]]{}line spectrum of [HXMM05]{}in the last panel of [Figure \[fig:spectra\]]{} and the top right panel of [Figure \[fig:co10spec\]]{}. The best-fit parameters obtained from fitting a single-Gaussian are listed in [Table \[tab:line\]]{}, together with those derived for the CO lines.

We extract separate spectra for X-Main and X-NE from the high resolution data cube using an aperture defined by the 1[$\sigma$]{} contours of the [*tapered*]{} intensity map. The resulting spectrum of X-Main is shown in the middle right panel of [Figure \[fig:co10spec\]]{}. Fitting a single Gaussian


Blue markers show the centroid velocities of the spectra extracted at different spatial positions (see text in [§\[sec:ET\]]{}). Red dashed lines show the central position (vertical) and velocity (horizontal) determined from [[rotcur]{}]{} and from fitting a double-Gaussian to the [\[C[II]{}\]]{}spectrum. \[fig:pvfit\]](pvfit_out_envelope_vsys158_final.pdf){width="50.00000%"}

![image](co10_cii_Ka){width="100.00000%"}

H$_2$O Line Emission {#sec:h2o}
--------------------

The H$_2$O($1_{11}$[$\rightarrow$]{}$0_{00}$; 3$_{12}$[$\rightarrow$]{}$2_{21}$) lines at redshifted frequencies of 279.383 and 289.367GHz are covered by the ALMA line observations. We do not detect the ground state H$_2$O line in emission or absorption down to a 3[$\sigma$]{} limit of $<$0.80Jy[kms$^{-1}$]{}[beam$^{-1}$]{}, assuming the same linewidth as the line (760[kms$^{-1}$]{}). The H$_2$O(3$_{12}$[$\rightarrow$]{}$2_{21}$) line is next to the line and is at most weakly detected; we conservatively report a 3[$\sigma$]{} upper limit of $<$0.87Jy[kms$^{-1}$]{}[beam$^{-1}$]{}, assuming the same linewidth as for the line.

Continuum {#sec:cont}
---------

We show the [*Spitzer*]{}/IRAC images in [Figure \[fig:newcont\]]{}. Sources near [HXMM05]{}arebeam smearing means that velocity information within the inner kpc region will be largely lost in the data.

We fit an arctangent model [e.g., @Courteau97a] to the [[rotcur]{}]{} rotation curve (RC). The model is parameterized as: $$V_{\rm rot} = V_0 + \frac{2}{\pi} V_{a} \arctan\left(\frac{R}{R_{t}}\right),$$ where $V_{\rm rot}$ is the rotation velocity found with [[rotcur]{}]{}, $V_0$ is the systemic velocity, $V_{a}$ is the asymptotic velocity, and $R_{t}$ is the “turnover” radius at which the rising part of the rotation curve begins to flatten. We perform non-linear least-squares fitting using the Levenberg-Marquardt algorithm to find the best-fit parameters. We limit the turnover radius to 0$<$$R_{t}$$<$25 kpc in order to keep this parameter within a physically meaningful range. Using this model, we find $V_{a}$=503$\pm$83[kms$^{-1}$]{}, $R_{t}$=0.8$\pm$0.3kpc, and $V_0$=0$\pm$28[kms$^{-1}$]{}(relative to the systemic redshift). We thus


with the data at hand, the presence and properties of an X-ray dominated region (and/or a second PDR component, and/or shock excitation) are unconstrained and indistinguishable from a simple single PDR.

The PDR properties thus suggest that the high far-IR luminosity of [HXMM05]{}($>$10$^{13}$) may result from extended [star formation]{}, with only a modest FUV radiation field intensity. This is in stark contrast with the compact starbursts seen in the cores of many nearby ULIRGs (less than a few hundred parsecs), which are found to have stronger FUV radiation fields compared to [HXMM05]{}[e.g., @Stacey10a]. The inferred PDR conditions also suggest that [HXMM05]{}is unlikely to host an AGN or a powerful quasar, consistent with [§\[sec:agn\]]{}.

![Ratios of CO, [\[C[II]{}\]]{}, and far-IR luminosities (solid) as functions of $G_0$ and $n$. Model grids areheavily dust-obscured AGN in [HXMM05]{}or a Seyfert galaxy nucleus with modest X-ray emission. To assess the reliability of the stellar mass derived from SED fitting, we examine if the mid-IR spectral slope of [HXMM05]{}($S_\nu$$\propto \nu^{\alpha}$) may be consistent with a low X-ray luminosity AGN [see e.g., @Stern05a; @Donley07a]. We fit a power-law to the IRAC 5.8- and MIPS 24-$\micron$ photometry, which correspond to rest-frame 1.5$-$6.0$\micron$. We find a spectral index $\alpha_{\rm 1.5-6, rest}$[=]{}1.46[$\pm$]{}0.58, which is much flatter than those observed in AGN host galaxies[^10] [@Stern05a; @Donley07a; @Donley08a], suggesting that the NIR emission in [HXMM05]{}may be dominated by stellar emission. Thus, we assume in the following that all the NIR emission detected in the IRAC channels 3 and 4 bands arises solely from the starlight in [HXMM05]{}. That is,


and starburst systems.

### Gas Mass, Gas-to-Dust Ratio, and Metallicity {#sec:alpha}

Using the line intensities ([Table \[tab:line\]]{}) and assuming a CO luminosity-to-H$_2$ mass conversion factor of [$\alpha_{\rm CO}$]{}[=]{}0.8[e.g., @Downes98a], we derive molecular gas masses of $M_{\rm gas}^{\rm X-Main}$[=]{}(1.68[$\pm$]{}0.43)[$\times10^{11}$]{}for X-Main, $M_{\rm gas}^{\rm NE}$[=]{}(6.52[$\pm$]{}1.63)[$\times10^{10}$]{}for X-NE, and $M_{\rm gas}^{\rm total}$[=]{}(2.48[$\pm$]{}0.65)[$\times10^{11}$]{}for the entire system ([Figure \[fig:comom0\]]{}). Using the molecular gas mass of the system, we find a gas-to-dust mass ratio of GDR ([$\alpha_{\rm CO}$]{}$/$0.8)$^{-1}$[=]{}50$-$145, which is consistent with those measured in the Milky Way, local spiral galaxies, ULIRGs, and DSFGs [@Draine07a; @Wilson08a; @Combes13a; @Bothwell13a].

Based on the fundamental metallicity relation (FMR) determined by @Mannucci10a, we infer a gas-phase metallicity of $Z$[=]{}12$+$log(O/H)[=]{}9.07 for [HXMM05]{}[^14], which is comparable to the that of the $z$[=]{}4 SMG GN20 [@Magdis11a]. We express the metallicity on the Pettini & Pagel ([-@PP04]; PP04) scale using2.3[$^{+2.7}_{-1.8}$]{}[$\times10^{-3}$]{}, which is within the range measured in local star-forming galaxies and ULIRGs, but is among the lowest measured in intermediate-[$z$]{}ULIRGs and quasars [e.g., @Dunne11a; @Combes13a; @Leung17a]. This ratio is also lower than those measured in DSFGs at similar redshifts [e.g., @Magdis11a; @Calura17a].

The molecular gas-to-stellar mass ratio of [HXMM05]{}is $M_{\rm gas}$/[=]{}0.2[$^{+0.2}_{-0.1}$]{}, which is higher than those observed in local SFGs and early-type galaxies [e.g., @Leroy08a; @Saintonge11a; @Young14a]. Previous studies report a positive evolution in this ratio with redshift [e.g., @Tacconi10a; @Dave12a]. The $M_{\rm gas}$/ratio of [HXMM05]{}is lower than those typically measured in other [high-$z$]{}SFGs and DSFGs at [$z$]{}$>$1.2, and is the lowest[^15] found among massive galaxies at [$z$]{}$\simeq$3 to date [@Leroy08a; @Tacconi10a; @Daddi10a; @Geach11a; @Decarli16b].

The low DSR and gas-to-stellar ratio of [HXMM05]{}may indicate that it is a relatively


find that the molecular gas in X-Main (i.e., grey symbols in [Figure \[fig:sled\]]{}) is more highly excited than the system overall, which is comparable to other [high-$z$]{}DSFGs [e.g., @Riechers11e; @Sharon16a]. As noted in [§\[sec:co\]]{}, the true flux may be a factor of two higher. In this case, the excitation conditions of [HXMM05]{}and X-Main would be consistent with (and possibly more excited than) those of other DSFGs. However, higher fidelity data are needed to confirm this scenario.

![ CO SLEDs of [HXMM05]{}and other low- and [high-$z$]{}galaxies reported in the literature. Line fluxes are normalized to the line. Red stars show the SLED of [HXMM05]{}based on the total flux (i.e, X-Main and X-NE; see [Figure \[fig:comom0\]]{}). Grey markers show the SLED of X-Main only, relative to its flux. Solid black line shows theformation]{}. In other words, the stability of gas against gravitational collapse is more closely linked to [star formation]{}than the velocity structure of the existing stellar component, which may (re-)settle on a different timescale from the gas after perturbations.

Dust
----

### Morphology and Optical Depth

[HXMM05]{}remains undetected in deep UV and optical images, indicating that it is highly dust obscured, consistent with its rest-frame 158$\micron$ optical depth of $\tau_\nu\simeq$1 (determined from SED modeling; [§\[sec:sed\]]{}). This optical depth exceeds those of most “normal” star-forming galaxies and nearby disk galaxies, but is similar to that seen in Arp220 and [high-$z$]{}starburst galaxies — e.g., HFLS3, AzTEC-3, and ADFS 27 [@Riechers13a; @Riechers14a; @Riechers17a].

The dust emission morphologies at 635 and 870$\micron$ appear different ([Figure \[fig:newcont\]]{}). While two compact dust components are found to be embedded within an extended


component at 635$\micron$, only one compact component coincides with XD1 at 870$\micron$. The second 635$\micron$ dust peak, XD2, is 1.8 times fainter than XD1 at its peak flux (see [Table \[tab:cont\]]{}). If XD1 and XD2 were to have the same peak flux ratio at 635 and 870$\micron$, we would expect a peak flux density of 6.2mJy[beam$^{-1}$]{}for XD2 at 870$\micron$, which we would have detected at $>$20$\sigma$ significance. Hence, the non-detection of XD2 at 870$\micron$ may be a result of the lower dust column density at 870$\micron$, where the emission is optically thin on average based on[^19] the best-fit dust SED model ($\tau_\nu$[=]{}0.54).

### Interpretation of the compact dust components {#sec:clump}

The compact dust components, XD1 and XD2, detected at 635$\micron$ could be two regions of intense [star formation]{}, or the remnantthe Institut National des Science de l’Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. This study is also based in part on data products produced at Terapix available at the Canadian Astronomy Data Centre as part of the Canada-France-Hawaii Telescope Legacy Survey, a collaborative project of NRC and CNRS. Based on observations made with the NASA [*Galaxy Evolution Explorer*]{}. [*GALEX*]{} is operated for NASA by the California Institute of Technology under NASA contract NAS5-98034. This work uses data based on observations obtained with the [*XMM-Newton*]{}, an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA. Facilities: IRAM PdBI, CARMA, VLA, [*HST*]{}(WFC3), SMA, ALMA, [*Spitzer*]{} (IRAC, MIPS), [*WISE*]{}, [*Herschel*]{}(PACS, SPIRE), VISTA, CFHT(MegaCam), [*XMM-Newton*]{}(EPIC), [*GALEX*]{}

CO


[HXMM05]{}. We therefore model the surface brightness profiles of the sources near [HXMM05]{}based on their morphologies seen in the CFHT and VISTA images in order to de-blend the emission observed at 3.6 and 4.5$\micron$ (see Appendix [§\[sec:galfit\]]{}).

On the other hand, X-NE is detected in the UV, optical, and NIR wavebands (as shown in Figures \[fig:newcont\] and \[fig:cont\]). As discussed in [§\[sec:results\]]{}, this component is also detected in and [\[C[II]{}\]]{}line emission (see Figures \[fig:co10spec\] and \[fig:mom0\]). With the available data, we cannot discriminate and obtain reliable constraints on the stellar masses and SFRs for X-NE and X-Main separately. We thus infer the properties of the system as a whole in [§\[sec:diss\]]{} and subsequent sections. That said, optically-selected [high-$z$]{}sources (e.g, BzKs, LBGs) appear to be different populations from these highly dusty starburst galaxiesUniversity in Kingston, Canada, Paulo has encouraged the use
of Python and BioPython for daily lab and informatics work and
organizes a "Python for Bioinformatics" workshop.

Audrey M. Roy

Audrey Roy has been instrumental in the creation and initial success
of the PyLadies outreach group in Los Angeles and will be one of the
keynote speakers at PyConAU 2011. She is a core developer for
DjangoPackages and the associated Packaginator open source project.

Gavin M. Roy

Gavin Roy is the CTO of myYearbook.com, where he encourages the use of
Python and contributes internally developed code to the open source
community. He supports two local Python user groups, PhillyPUG in
Philadelphia, and PUG-IP in Princeton, NJ. He was a speaker at PyCon
2011 in Atlanta and participated in the Program Committee. Gavin is
also the primary maintainer of the pika module for interacting


is the government, a government trying to legislate benevolence, trying to correct injustices and protect its citizens. Why does that make people mad?

Why are we offended when there is no offense intended?

Racism is not an adequate explanation of what is happening; it is too simple and too exclusive. Even racism, a particular form of snobbery, is a sign of something more profound.

Rush Limbaugh and others like him know what this profound thing is; they might not understand it, but they know how to use it.

There is reasonable opposition to health care. It is good. But the animosity hinders progress, and it will interfere with all progressive motions our nation tries to make.

"We are not enemies, but friends. We must not be enemies." The words were not heeded whensmaller and much more numerous M-dwarf stars. Studies of Kepler data to date have already shown that about half of M-dwarf planetary systems are, on average, composed of about a half dozen planets in tight orbits with low mutual inclinations (see “Architecture of M-Dwarf Planetary Systems”). Planets in systems like these orbiting M-dwarf stars are easier to detect owing to their shorter orbital periods (which produces more frequent transits), their smaller orbits (which increases the probability of producing a transit) and their larger size relative to the star they orbit (which produces deeper transit events) compared to their counterparts orbiting more Sun-like stars. Some of these M-dwarf planets even orbit inside the habitable zone (HZ) of their systems (see “Habitable Planet Reality Check: 8 New Habitable Zone Planets”


required to refine them. The ongoing analysis of the data set from Kepler’s primary mission as well as the data from the extended “K2” mission should provide some new finds. NASA’s Transiting Exoplanet Survey Satellite (TESS) mission, which will observe 1,000 nearby red dwarfs among its half million relatively bright targets, should provide many finds to improve occurrence rate estimates especially in the star fields near the ecliptic poles that will be observed for longer periods of time. These planets offer the potential of detailed follow-up study that will help scientists begin to probe the potential habitability of planets orbiting M-dwarfs which are the most common star type in the galaxy.

Follow Drew Ex Machina on Facebook.

Related Reading

“Architecture of M-Dwarf Planetary Systems”, Drew Ex Machina, October 24, 2014 [Post]

“Habitableand the Google Privacy Policy and Terms of Service apply. You have successfully signed up for the TAPinto Newark Newsletter.

The vote from state lawmakers was canceled on Monday since it was unlikely to pass in the Senate.

Baraka has supported state Sens. Nicholas Scutari (D-Union) and Stephen Sweeney’s (D- Gloucester) bill to legalize marijuana for adults aged 21 or older, but only if the expungement process for past marijuana convictions becomes less tedious.

A separate expungement bill, sponsored by Jamel Holley (D-Union) in the state Assembly, was slated for a vote yesterday too, but was canceled along with the recreational bill.

The mayor has plugged for an automatic expungement process for all non-violent cannabis offenses. Under the expungement bill, a person who has a conviction that involves possessing, selling or distributing


last year. And the band decided to put together a new album to boot. Upon hearing the first new tracks – The Museum of Broken Relationships and It’s Holy – I’m eagerly anticipating its release.

Move over Victoria’s Secret. Veruca Salt will always be the world’s best VS.

I made the octopus with spaghetti and punched out a bunch of yellow stars for the starfish. Working with damp noodles was a sticky experience.

I’ve included some extra photos of the process.

Disclaimer: Every piece of music-inspired artwork on this site is an original new creation. I am not affiliated with nor do I own the rights to any of the Original music artwork that has inspired me to create the new artwork found on this site.gonna get it!" "Give it back!" "You owe me 20 bucks, you little shit!" " Don't worry about it!" " Give it, brat fucker!" " I'm gonna get it!" "I'm gonna get it!" " Brat!" "Fucker!" " What's going on?" " Nothing." " What was that?" " Nothing." "How's the Torah portion coming?" "Can you maybe use the hi-fi?" " What?" " Can I borrow this?" "I'm taking some stuff to, you know, the Jolly Roger." " Dad!" " Sure, Dad." "Dad!" "Chinese guy!" "Culture clash." "Culture clash." "With all respect, Mr. Park, I don't think it's that." " Yes." " No, it would be a culture clash if it were the custom in your land to bribe people for grades." "Yes." "So, you're saying it is the


Roger." "Excuse me?" "No, I..." "Well, yes, okay." " Yes, you are Lawrence Gopnik?" " Okay." ""Okay" means..." "Okay, yes, Lawrence Gopnik, yes." "Okay, well, you received your 12 introductory albums, and you've been receiving the monthly main selection for four months now..." "The monthly main selection?" "Is that a record?" "I didn't ask for any records." "To receive the monthly main selection, you do nothing." "You..." "That's right." "I haven't done anything." "Yes, that's why you received the monthly main selection." " But..." " The last one was Santana Abraxas." "You..." "I didn't ask for Santana Abraxas." "You request the main selection at the retail price by doing nothing." "It's automatically mailed to you, plus shipping and handling." " You're about to receive..." " I can't affordrelax." "Try to relax." "Oh, my God, Mrs. Samsky!" "So good." "Nailing it down." "So important." "Please." "I need help." "I've already talked to the other rabbis." "Please." "It's not about Danny's bar mitzvah." "My boy, Danny." "This coming Shabbas." "Very joyous event." "That's all fine." "It's more about myself." "I've had quite a bit of tsuris lately." "Marital problems, professional, you name it." "This is not a frivolous request." "This is a..." "I'm a..." "I've tried to be a serious man, you know?" "Tried to do right, be a member of the community, raise the..." "Danny, Sarah, they both go to school, Hebrew school." "A good breakfast..." "Well, Danny goes to Hebrew school, Sarah doesn't have time." "She mostly washes her hair." "Apparently there are several steps


publicity means to an author is going to vary widely depending upon the resources available. Do you have time to research conventions? Update your website? Plan a book or blog tour? Do all this and write new books, too? What is your time worth to you?

There are pros and cons to hiring a book publicist. Let’s start with the cons. Maybe they aren’t qualified. Maybe they charge too much. Maybe their communication and reporting is sub-par. Maybe they don’t have enough contacts to make it worth your while. Ending with the pros, there is one that shoots to the top of my list: publicists can save you a lot of time and headaches so you can devote your energy to writing. Maybe they managed to slot you inand client, and not just to move units. It’s less of a hard-sell, and more of a conversation. Why will the customer like this thing, and why should they like the people making it? Why should they commit their time and resources to a long-term support of my client? I also have to prepare for bad results, bad feedback, bad publicity. My job is to mitigate damage and turn it into a positive for the client.” – Jaym Gates, SFWA Publicist.

Gates’ last comment, about mitigating damage, is something I’d like to expand upon further. If you have a good relationship with your publicist, that person can act as a buffer, a sounding board for you to vent to when you’re pissed off or frustrated with a review, blogger,


But, without data to back up any publicity efforts, the emphasis often falls on saturating channels to get the word out to as many people as possible. Personally, I feel that’s a waste of resources.

Publicity “Requirements”

Circling back to the beginning, I mentioned that there are a lot of conversations happening about what authors are required to do in order to promote their books. I asked Jason Sizemore to share his publisher’s expectations:

“I expect an author to play a basic and active role in the promotion of his or her book. That means being available for a reasonable amount of online and phone interviews, taking advantage of opportunities when they arise such as Scalzi’s “Big Idea” feature, and to provide logistical support to Apex for marketing purposes (giving usjustice committee's study of the SNC-Lavalin affair instead of recalling former justice minister Jody Wilson-Raybould to testify — delayed it by dragging out a vote on a motion about MP travel.

Morneau tabled his budget and left the House without giving the speech. When he eventually returned and rose to speak, opposition members tried to drown him out by banging on their desks.

The thumping and shouts of "let her speak" and "coverup" were so loud that people gathered in the public gallery could not hear what Morneau was saying. He carried on with his speech; the Conservatives eventually staged a walkout from the chamber as he spoke.

Conservative MPs banged on desks and jeered loudly during Finance Minister Bill Morneau's budget speech making it nearly impossible to hear what Morneau


could be conveniently followed as shown in [Fig. 2](#pone-0045947-g002){ref-type="fig"}. L-aspartate shows two resonances, in a 1∶2 ratio ([Fig. 2a](#pone-0045947-g002){ref-type="fig"}). Upon addition of ADC, the signals corresponding to the product start to emerge and intensify with time while those of the substrate L-aspartate diminish and eventually completely disappear ([Fig. 2 b--e](#pone-0045947-g002){ref-type="fig"}). Note that, based on its structure, one would also expect two different ^1^H NMR peaks for β-alanine (this was confirmed by taking a spectrum for the commercial analyte). However, only the signals corresponding to the protons adjacent to the carboxylate group could be quantified in the course of the enzymatic reaction (at approximately δ = 2.44 ppm). This is a consequence of the fact that the reaction is carried out in D~2~O, and, therefore, the newly acquired β-alanine hydrogen is,predictions never materialized. Murder rates started dropping immediately after the passage of the law, prompting one of the chief opponents, Rep. Ron Silver, to admit that he had been wrong about concealed carry.

Such was the case in Texas, as well. One of the chief opponents in the Lone Star State was Senior Cpl. Glenn White, who was president of the Dallas Police Association. White lobbied against the law in 1993 and 1995 because he thought it would lead to wholesale armed conflict. Senior Cpl. White admitted to the Dallas Morning News: "All the horror stories I thought would come to pass didn't happen. No bogeyman. I think it's worked out well, and that says good things about the citizens who have permits. I'm a convert."

Another was Harris County


a weapon. We need to be armed with the facts to adequately debate the issue. Thanks for sharing this.

steelerdude99

December 14, 2013, 12:25 PM

Even if the short article referenced was somewhat unbiased, the link it referenced from "Violence Policy Center" sure was an attack on all concealed carry with an emphasis on Florida.

http://www.wctv.tv/news/headlines/70280587.html
...
chuck

Also in that Violence Policy Center (aka VPC) link is an attempt to make readers think the numbers are higher by stating that they don't actually get data from the police as to who is and is not a permit holder.

Because most state systems that allow the carrying of concealed handguns in public by private citizens release little data about crimes committed by permit holders, the VPC reviews and tallies concealed handgun permit holder killings as reportednot in the age of the internet, but I'm too lazy on a Sunday morning to look for it. Probably the VPC researchers were, too.

The anti-gun VPC is just attempting to undermine a statistic that they don't like. I don't know if my state (VA) publishes crime stats of the general vs. conceal carry populations. As the permit holders names are no longer public records in states like VA, it's harder to get an accurate count by anyone not in state government. Nonetheless, VPC spins it to say (remember, this is VPC not me): "It is likely that the actual number of fatal criminal incidents involving concealed handgun permit holders is far higher.". NOT just higher, "FAR HIGHER".

chuck

Carl N. Brown

December 22, 2013, 05:13 PM

Last time I checked Violence


all costs, I didn't lose anything there !

Vern Humphrey

January 14, 2014, 02:16 PM

It ended with the 43-year-old father shot dead amid the theater seats, and a 71-year-old retired police officer in custody.
Guy 2 was a former police officer, which makes the point of this thread. "Only police should have guns.":(

tepin

January 15, 2014, 04:45 PM

Who will murder you?
If you believe the stats, you are more likely to be murdered by someone you know than by someone you don't know. Being murdered by a LEO or CCW holder happens, but it is so uncommon it probably isn't worth discussing.

Discussing murder rate is somewhat meaningless. Folks should be focused on the aggravated assault rate - which is the rate in which people are *trying* to kill each other. Advances in medicalguns, you can't leave out the crimes/damage committed with guns, with the exception of murder. Since those numbers DO get adjudicated ( quite often) are you sure that you want to go there? :-) And it's not 3 million, its probably not more than 1 million x per year that guns stop attacks without firing a shot. It does happen, a lot, tho. I've done it myself, several times now.

Mike1234567

January 15, 2014, 07:48 PM

,,,

akodo

January 15, 2014, 10:37 PM

McDonald's is going to murder me.

Getting the numbers out there on really how many people are murdered (not suicide) or killed accidentally by guns in comparison to heart disease would help RKBA imho.

Note, however, that our right to own guns really isn't related to rates of death. If mental heath care


But the ultimate issue I (And many of my friends, if I recall) have with the player community of the LRPG forum is the lack of appreciation towards the most vital part of characters and the game: The character's personality and the development of that personality throughout the game. Personality and CD (Character Development) are really the heart and soul of the character. You shouldn't just want to make a character solely due to having an interstellar marine with a flamethrower, but due to the interesting possibilities of your character interacting with others, and possible plotlines that could be formed. It is much more enjoyable to see a driving force behind characters that isn't the hands of a puppeteer.

Don't get me wrong, I'm not trying to bash allto be more important than competition. When we tried to introduce a competitive element into the BZPRPG at the beginning of the year to spice things up, we found to our and players' dismay that it quickly fragmented the player base against itself, arousing some pretty shocking negativity from our gaming community.

Bringing the competitive aspect of the LRPGs into BRPG means that players looking for two different game experiences will be relegated to the same cramped forum. LRPG players and BRPG players, if they try to participate in one anothers' games, may be confused and frustrated by the double standards of play under one "roof."

3) The community of the BRPG forum is, for all its occasional squabbles, fairly tight-knit, and sometimes hard to breach. This is due in


like to see Outlaw Rogues or Fury Warriors excel in situations with 4 to 5 targets in close proximity to each other, while ranged casters like Frost Mages or Affliction Warlocks perform better in sustained damage against groups of 5 or more targets. To accomplish this, we need to revisit the maximum number of targets that many abilities can hit (also known as the ability’s “target cap”), and adjust them accordingly. In situations where a target cap doesn’t make sense, we’re adding a new kind of damage falloff that causes the damage done to each target to be reduced gradually as the number of targets increases.

Most players who are used to fighting 3 to 5 enemies at a time will notice very little difference with this approach. OnThe New Mighty Dead? Loss Transformed into Power

There is a new moon rising, and I feel called. I have yet to look at the chart for this moon, but here is what I’m feeling.

The Year 2016 and Death

For the past week or so, I’ve been contemplating the year 2016. On both a universal and a personal level numerologically, it is a year of endings: 2+0+1+6= 9. Nine is the end of a cycle, before we begin anew with the number one. And 2016 certainly seems like it’s had its fair share of endings, hasn’t it? Too many greats—artists, musicians, and other beloved public figures—have passed away from this side to the next in an apparent wave of mass migration. Not to mention the seeming end of civility and


similar survey, albeit with a different methodology, and vastly different results.

The ISC's Domain Name Survey has been active since August 1981 when it counted a mere 213 hosts. But the group's latest survey released in January 2004 found over 233,101,481 million hosts, over four times higher than Netcraft's numbers.

So what explains the approximately 183 million difference in the numbers? According to the ISC, the surveys are measuring different, yet similar things.

"While both numbers are important, the ISC number is probably a better indication of the size and maturity of the Internet, because it includes both producers and consumers of information. The Netcraft number counts only producers of information."

Reid speculates that Netscraft's survey is based on a spidering crawl approach (similar to the way Google indexes Web pages).

(Netcraft doesbehind the eel. It's always amazing. It's noher first crash.she's had other crashes and to her this felt like a lot of the other crhes.shno idea how bad it was till she saw the video. Wow. N me. I wouldn't dit. I'm quitter. Yeah. I'm with you. Yeah.

This transcript has been automatically generated and may not be 100% accurate.


One local shopper will win $10,000

STEPHENVILLE (October 13, 2017) — Locally-owned radio stations KSTV-AM (1510am/93.9FM) and KSTV-FM (The Mighty 93) are bringing back their Shop Local campaign.

Coming on the heels of an immensely successful inaugural event, the second annual campaign is again designed to encourage spending money locally as opposed to leaving the area and shop elsewhere, such as Weatherford, the DFW Metroplex or even online with companies that have no local ties or vested interest in the economy of Stephenville and Erath County.

It’s a simple process that has not changed since a year ago when Michael Newton purchased the winning ticket from Texas Car Detail in Dublin and was awarded $10,000.

Michael Newton won $10,000 in a shop local campaign created by KSTV-fM and KSTV-AM radio stations, whoMore on LinuxToday

Using 'ab', ApacheBench to test Web Server Performance

WEBINAR:On-demand Event

Replace Oracle with the NoSQL Engagement Database: Why and how leading companies are making the switch REGISTER >

"This tool is of course aimed at testing Apache servers, however
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"Usage
Usage is rather simple. At it’s core, the amount of requests
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can inform the application to carry out more than one request at a
time, as show in the second example.

$ ab -n 100 http://domain/
$ ab -n 100 -c 3 http://domain/

Some Results

"These are the results I gained from running this against the
server behind this, testing using 3 concurrent connections and 100
requests:"


15 So.3d 926 (2009)
Edgar Ivan GIL, Appellant,
v.
STATE of Florida, Appellee.
No. 5D08-3192.
District Court of Appeal of Florida, Fifth District.
August 7, 2009.
James S. Purdy, Public Defender, and Brynn Newton, Assistant Public Defender, Daytona Beach, for Appellant.
Bill McCollum, Attorney General, Tallahassee, and Kristen L. Davenport, Assistant Attorney General, Daytona Beach, for Appellee.
GRIFFIN, J.
Edgar Ivan Gil ["Gil"] appeals his convictions and sentences for trafficking in cocaine, conspiracy to traffic in cocaine, unlawful use of a two-way communication device, and resisting a law enforcement officer without violence. On appeal, Gil argues that the trial court erred by denying his motion to dismiss the information. He contends that law enforcement officer William Powell's ["Officer Powell"] act of notarizing two affidavits that had been signed by a confidential informant using a fictitious name, amounted tocould get a single run of 10 even light, a perfect solution for a pathway.

The applications for this type of lighting are endless, here at SDL we can advise you on which product will be most suitable for your outdoor project. We look forward to hearing from you 🙂

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$form_state parameter from hook_form_alter().
 *   - For "submit", passes in the $form_state parameter from hook_form_submit().
 * @return
 *   The index where we can find our values in Skinrs data structure.
 */
function panels_skinr_form_index_handler($op, &$form, $form_state) {
  switch ($op) {
    case 'form':
    case 'submit':
      switch ($form['#parameters'][1]['type']) {
        case 'display':
          return 'display-'. $form['#parameters'][1]['display']->did;
        case 'region':
          return 'display-'. $form['#parameters'][1]['display']->did .'-region-'. $form['#parameters'][1]['pid'];
        case 'pane':
          return 'display-'. $form['#parameters'][1]['display']->did .'-pane-'. $form['#parameters'][1]['pid'];
    }
      break;
  }

  return FALSE;
}

/**
 * Skinr data handler.
 * This is the data that populates the skinr form.
 *
 * @param &$form
 *   Passes in the $form parameter from hook_form_submit().
 * @param $form_state
 *   Passes in the $form_state parameter from hook_form_submit().
 * @param $module
 *   The module that is currently being processed.
 * @param $form_settings
 *   The settings from hook_skinr_data() for the form that's currently being
 *   processed.
 * @return
 *   TRUE if we get access, FALSE if we don't.
 */
function panels_skinr_data_handler(&$form, $form_state, $theme, $module, $form_settings) {
  // Ensure we have the required index_handler.
  if (empty($form_settings['index_handler'])) {
    trigger_error(sprintf("No index_handler


  - "access skinr classes": access to edit skinr's additional classes
 * @param &$form
 *   Passes in the $form parameter from hook_form_alter().
 * @param $form_state
 *   Passes in the $form_state parameter from hook_form_alter().
 * @return
 *   TRUE if we get access, FALSE if we don't.
 */
function panels_skinr_submit_handler_settings(&$form, $form_state, $module, $form_settings) {
  foreach ($form_state['values']['skinr_settings'][$module .'_group'] as $theme_name => $theme) {
    if ((!empty($theme['widgets']) && is_array($theme['widgets'])) || isset($theme['advanced']['_additional'])) {
      $hook  = $module;
      $key   = skinr_handler('form_index_handler', 'submit', $form_settings['index_handler'], $form, $form_state);

      // Key doesn't exist properly for new displays. Perhaps we should inject a timestamp based key into the display object
   $form_state, $module, $form_settings) {
  $form_id = $form_state['values']['form_id'];

  // Include ctools' object cache files.
  ctools_include('object-cache');

  if ($form_state['values']['op'] == t('Save') || $form_state['values']['op'] == t('Update and save')) {
    switch ($form_id) {
      case 'panels_panel_context_edit_content':
      case 'page_manager_save_page_form':
        // Panel page.
        foreach ($form_state['page']->handler_info as $id => $info) {
          if ($info['changed']) {
            _panels_skinr_save_and_clear_cache($form_state['page']->handlers[$id]->conf['did']);
          }
        }
        break;


to where Alex is headed.

Hint #3:

 @El-Guest has already translated everything. Now where is Alex?

The Question

Where is Alex P. Barker?

This puzzle took a while to create and is quite involved. I hope you all enjoy it, and I wish the best of luck to all of you!

A:

Big shoutout to my friend Google Translate for starting me off with some of these. I know the riddles aren’t perfectly translated, but here goes....
So the first clue says

 in Portuguese: “This is the man who stole the bank in town! It should not be taken lightly. He usually has a bodyguard and is heavily armed. A friend of mine claimed that he carries a rocket launcher in the back! Lastly, I heard he was heading northeast.”

Telling us he’s gone

 From PortugalQ:

Why Outlook.live.com and Outlook App show blank body, but the source is NOT empty?

It has been almost a week since this problem appeared.
Previously every thing was fine, I am using PHP mail function to send feedback from server to my E-mail; Then, out of a sudden, about 40% of the E-mails are shown to have no content, the server was not touched.. I opened outlook.live.com and I was able to see the message body from "show message source", which means my server hasn't changed any thing, it is still sending all the information I need, but Outlook would not show the content for some reason.
Does anyone have any idea about the cause and solution? Thanks!

A:

In case someone has encountered this problem, Microsoft Community has provided the valid solution


           }
          break;
          case "width":
            // field width (mapped with "width")
            __width=jacksonParser.getIntValue();
          break;
          default:
            jacksonParser.skipChildren();
          break;}
    }
    // immutable object: inizialize object
    Image instance=new Image(__url,__title,__link,__width,__height);
    return instance;
 after Test matches physically. Mentally, it's a different story but it only takes a day to recover from that. While I keep enjoying it, I'll keep doing it.

"I wouldn't say I'm overly fresh, but I'm lucky that I get to concentrate on one format of the game so that certainly helps me. We've got guys, and England have got guys that play all three formats going 12 months of the year and that's bloody difficult. For me to be able to specialise and put all my energy into that, and then be able to use my energy to keep guys like David [Warner] and Steve, and [Josh] Hazlewood and [Pat] Cummins, the guys that are playing all year round, for me to be able to energise them and


viewed a video of each student-SP encounter. The faculty's score was considered the gold standard. Correlation between scores was calculated using Spearman's rank correlation coefficient. Mean student scores were highest when rated by SPs (M = 3.8, SD = 0.9), followed by self (M = 3.0, SD = 0.9), and then faculty (M = 2.5, SD = 1.2). Spearman's rank correlation coefficient showed a strong positive correlation between students and the expert faculty rater (rs = 0.67, P < .001) and between SPs and the expert faculty rater (rs = 0.72, P < .001). The correlation was stronger for high- than for low-proficiency students. Students' self-rated scores showed significant improvement from baseline to the OSCE. PA students participating in a medical Spanish curriculum and SPs show good correlationpeople need to realize that it's just a game and don't stress over it too much. I also think the idea of they're all different legends is possible too but nonetheless they're great games and to me it really doesn't matter I just was always interested though in finding the timeline out but I learned to just forget about it and just enjoy the games for what they are. I still am interested in watching videos in what people think it is just to entertain myself. But whatever the bottom line is Zelda is a great franchise and the timeline shouldn't be too overlooked just enjoy the games for what they are.

your right there is no timeline the fact is that its just reapeating itself "find the master


as a matter of law;  in such a situation, a reversal is automatic regardless of a showing of prejudice unless the defendant has knowingly and intelligently waived his constitutional right to conflict free representation.7   Since no such waiver was present in this case, we reverse.8

B.

13
While our reversal naturally nullifies the enhanced sentence imposed on the defendant in the court below, we find it desirable to address the defendant's objections to the enhancement of his sentence in order to guide the trial court in the possible retrial of this action and to avoid a potential ground for a subsequent appeal to this Court.

14
Prior to trial, the government filed notice of its intent to seek an enhanced sentence under the "dangerous special offender" provision of 18 U.S.C.such convictions the defendant has been imprisoned prior to the commission of such felony, and less than five years have elapsed between the commission of such felony and either the defendant's release, on parole or otherwise, from imprisonment for one such conviction or his commission of the last such previous offense or another offense punishable by death or imprisonment in excess of one year under applicable laws of the United States, a State, the District of Columbia, the Commonwealth of Puerto Rico, a territory or possession of the United States, any political subdivision, or any department, agency or instrumentality thereof.

11
 18 U.S.C. Sec. 3575(f) provides:
A defendant is dangerous for purposes of this section if a period of confinement longer than that provided for such felony is required for


are likely to interact with trace metals through adsorption, coprecipitation, dissolution, or electron transfer reactions. Quantitative evaluation of mineralogy by scanning electron microscopy coupled with micro-focused X-ray diffraction, micro-X-ray fluorescence, and micro-X-ray absorption near edge structure (mXANES) spectroscopy provided detailed insights into the composition of mineral assemblages and their effect on trace metal speciation during this investigation. In the sample investigated, titanium occurs as poorly ordered ilmenite, as rutile, and is substituted in iron oxides. Manganese's spatial correlation to Ti is closely linked to ilmenite, where it appears to substitute for Fe and Ti in the ilmenite structure based on its mXANES signature. Vanadium is associated with ilmenite and goethite but always assumes the +4 oxidation state, whereas chromium is predominantly in the +3 oxidation state and solelyTOKYO — Seeking to bring its spiraling debt under control, Japan has undertaken an unlikely exercise: lawmakers are forcing bureaucrats to defend their budgets at public hearings and are slashing wanton spending.

The hearings, streamed live on the Internet, are part of an effort by the eight-month-old government of Prime Minister Yukio Hatoyama to tackle the country’s public debt, which has mushroomed to twice the size of Japan’s $5 trillion economy after years of profligate spending.

Greece’s debt crisis, which has panicked investors and forced the rest of Europe to put together a multibillion-dollar bailout, has fed fears in Tokyo that if spending is unchecked, Japan could become the center of the next global financial crisis.

Mr. Hatoyama and his ruling Democratic Party are also trying to wrest control of Japan’s


Q:

How to make FFmpeg continuously write progress on one line

When encoding FFmpeg prints a new line every second with the progress, example
frame=   31 fps=0.0 q=0.0 size=     152kB time=00:00:00.72 bitrate=1726.3kbits/s
frame=   59 fps= 57 q=0.0 size=     175kB time=00:00:01.90 bitrate= 751.1kbits/s
frame=   89 fps= 58 q=0.0 size=     204kB time=00:00:03.04 bitrate= 549.8kbits/s

With a large file these lines can quickly fill the console screen. I would like to see the progress on one line if possible, that is to say each second the same line is overwritten with the updated progress.
ffmpeg.org/trac/ffmpeg/ticket/2349

A:

At least with Windows, FFmpeg requires 85 columns to
print progress correctly. I set this using the registry
sp hkcu:console WindowSize 0x00190055 -t dword
sp hkcu:console ScreenBufferSize 0x03e80055 -tHigh West Distillery

High West Distillery is a manufacturer of distilled spirits located in Park City, Utah, United States. It is the first legally licensed distillery in Utah since the end of the American Prohibition.

Distillery, restaurant, and saloon
The distillery operates, along with a saloon and restaurant, in an old livery stable dubbed "The National Garage", and in the adjacent historic Ellsworth J Beggs house, a two-story box house that was built in 1907. The house is on the National Register of Historic Places.

Distillation
High West makes its spirits in small batches in a 250-gallon copper pot still. High West uses a combination still, which allows for both use as either a continuous/reflux still or separately a pot still; this allows for a variety of unique distillates to be produced. In


Background {#Sec1}
==========

Creatine is widely recommended as an ergogenic aid to improve performance during short bouts of high-intensity physical activity, such as cycling sprints \[[@CR1]--[@CR5]\]. Supplementation with creatine increases an individual's total muscle creatine content (i.e. intramuscular phosphocreatine and creatine) \[[@CR6]--[@CR11]\]. Research supports that increased intramuscular phosphocreatine increases the capacity of the phosphagen system to provide rapid energy turnover during cycling sprints; thus, leading to increased power production while delaying the onset of fatigue \[[@CR1]--[@CR5]\]. Furthermore, the post-supplementation increase in intramuscular creatine availability increases the rate that phosphocreatine is resynthesized following the cessation of exercise \[[@CR7], [@CR9], [@CR10]\], potentially leading to improved performance during subsequent sprints. Consequently, previous studies have investigated the effects of creatine supplementation on peak and mean power output during individual \[[@CR12]--[@CR14]\] and repeated sprint cyclingtests \[[@CR6], [@CR10], [@CR12], [@CR15]--[@CR27]\].

The composition of the supplementation material plays a critical role in creatine uptake and the post-supplementation effect on power generating capabilities \[[@CR28]\]. The majority of previous studies examining creatine supplementation and sprint cycling performance have used creatine monohydrate \[[@CR6], [@CR12], [@CR14]--[@CR16], [@CR18]--[@CR21], [@CR23]--[@CR27], [@CR29]\]. It is important to note, however, that creatine uptake is increased in the presence of electrolytes \[[@CR30]--[@CR34]\]. Creatine transport is primarily dependent on electrogenic transporter proteins, requiring at least two sodium ions and one chloride ion to transport one creatine molecule across a cellular membrane \[[@CR30]--[@CR33]\]. Results of the studies by Dai et al. \[[@CR30]\] and Peral et al. \[[@CR32]\] demonstrate when the extracellular concentration of creatine remains constant, the rate and magnitude of creatine uptake is increased with increasing


passive recovery. We hypothesized that supplementation with the creatine-electrolyte material would lead to improved repeated sprint cycling performance, as the literature generally supports the effectiveness of creatine supplementation at improving such performance \[[@CR1]--[@CR4]\]. Supplementation with creatine increases one's intramuscular creatine and phosphocreatine contents \[[@CR6]--[@CR11]\], which has been implicated as a contributing factor for the ergogenic effect of creatine supplementation \[[@CR1]--[@CR4]\]. Increased intramuscular phosphocreatine increases the rate and duration that the phosphagen system is able to contribute rapid energy turnover; thus, increasing peak and mean power outputs during sprint cycling \[[@CR1]--[@CR4]\]. Furthermore, the increase in intramuscular creatine content increases the rate of phosphocreatine resynthesis during recovery; thus, improving subsequent sprint performances \[[@CR7], [@CR9], [@CR10]\]. Supplementation with creatine also typically increases one's body mass \[[@CR7]--[@CR10], [@CR13], [@CR18], [@CR19], [@CR21], [@CR27],[@CR28], [@CR35], [@CR36], [@CR60]--[@CR63]\], presumably due to increased intramuscular total creatine content and the associated increases in water retention and/or lean body mass \[[@CR28], [@CR36], [@CR62], [@CR63]\]. Therefore, considering the significant improvements in overall and repeated peak and mean power outputs, and significant increase in body mass, it is reasonable to expect that the creatine-electrolyte supplement increased the intramuscular creatine and phosphocreatine concentrations of the subjects following that treatment.

Improvements in sprint cycling performance observed in our study demonstrate the expected ergogenic effect of creatine-electrolyte supplementation. These outcomes were expected because creatine monohydrate supplementation improves peak and mean power output during sprint cycling \[[@CR6], [@CR10], [@CR12], [@CR16], [@CR24]--[@CR26]\]. Electrolytes further improve creatine uptake \[[@CR30]--[@CR33]\] and the ergogenic effect \[[@CR28]\]. Creatine transport into cells is mediated via transporter proteins, which


sprint during the first five of 12 sprints for their creatine-electrolyte group. However, from sprints 6--12, the differences in pre- to post-supplementation mean power output were not significantly different between the creatine-electrolyte and placebo groups. Interestingly, in the study by Kreider et al. \[[@CR36]\] the placebo group also demonstrated a 5--10% improvement in mean power output per sprint across all 12 sprints. Therefore, in the study by Kreider et al. \[[@CR36]\] the performance improvements following creatine-electrolyte supplementation were about 5--10% greater than the changes shown by the placebo group. While the post-supplementation improvements in mean power output for the creatine-electrolyte and placebo groups in the study by Kreider et al. \[[@CR36]\] appear to be large, it is important to note the study's subject demographics. The subjects in thestudy by Kreider et al. \[[@CR36]\] were NCAA division IA football players who participated in a structured exercise program consisting of 5 h per week of heavy resistance training and 3 h per week of agility and sprint training during their four-week supplementation intervention.

Results of the present study and those by Finn et al. \[[@CR35]\] and Kreider et al. \[[@CR36]\] emphasize the importance of the sprint and recovery durations when assessing the efficacy of creatine-electrolyte supplementation at improving repeated sprint cycling performance. However, since overall peak power output is typically recorded during the first sprint, it is unlikely that the either the sprint or recovery duration influenced overall peak power output in this study and those by researchers Finn et al. \[[@CR35]\] and Kreider et al. \[[@CR36]\]. Therefore,


to Henson’s group saying theirs is a family brand and would therefore no longer appear on Sex Box.

Henson told Breitbart News that PTC contacted 200 national advertising prior to the Sex Box premiere on February 27 and warned them the show would have offensive content. By the third episode, aired on March 13th, not a single national ad appeared, according to Henson. “We have monitors all over the country and we did not see a national advertiser in any market,” said Henson.

In what may be the best evidence the show is failing, tonight’s fourth episode of Sex Box has been moved from its primetime spot of 10 pm to midnight, a time when virtually all networks only ever run repeats.

A spokesman for WE tv told Breitbart News theyimportant, do not use this constant.

XmBOTTOM_TO_TOP

Specifies that the components are laid out from bottom to top.
If horizontal direction is important, do not use this constant.

XmDEFAULT_DIRECTION

Specifies that the components are laid out according to the default
direction. (This constant is primarily for widget writers.)

XmLEFT_TO_RIGHT

Specifies that the components are laid out from left to right.
If vertical direction is important, do not use this constant.

XmRIGHT_TO_LEFT

Specifies that the components are laid out from right to left.
If vertical direction is important, do not use this constant.


Your Ultimate Guide to Getting a Job While Recovering from Addiction

Addiction recovery takes a lot of hard work and dedication, and one of the hardest aspects of recovery life can be re-integrating into society. After having spent months in a rehabilitation center, it’s time to get back into the swing of things – to hold a stead position, to support a family, and to accomplish whatever goals you may have. There is a lot of hesitancy for those in recovery when it comes to finding employment, however, and it’s because of the stigma that comes with addiction recovery.

A 2017 study published in the Journal of Occupational and EnvironmentalMedicine states that national costs exceed $400 billion annually on lost productivity, absenteeism, disability and worker’s compensation related to addiction, and20 ChangeWave report from 451 said:

"Dropbox (44 per cent) remains the leading vendor for paid mobile file sharing and synchronisation services. Microsoft OneDrive (27 per cent) comes in second, closely followed by Google Drive (24 per cent)." ®


be arranged along the
positioning rail to give them some
support during the programme.
G 2XXX models:
You can set the cup rack at two
different heights.
^ Raise the rail, and lean the glasses
against it.
^ Pull the cup rack upwards and click it
back into position at the required
height.
The positioning rail can be flipped over
to the middle of the basket for easy
sorting and removing of crockery.
25
Loading the dishwasher
Support rail
This support is designed to hold tall
glasses and glasses with stems
securely.
^ Lower the support and lean tall
glasses against it.
^ You can also remove a section of the
cutlery tray to make more room for
tall glasses.
26
Loading the dishwasher
Adjusting the upper basket
In order to gain more space for taller
pieces of crockery in the bottom or
upper basket, the upper basket can be
adjusted on three levels with 2 cm
between each level.
Dependingdishwasher will continue to use
electricity until it is switched off with
the Off button o.
If the dishwasher is not going to be
used for a longer period of time, e. g.
whilst on holiday, the stopcock should
be turned off.
36
If you open the door fully after switching
off, the dishes will cool much faster.
First unload the lower basket, then the
upper basket and cutlery tray
(depending on model).
This will prevent water drops from the
upper basket and cutlery tray from
falling onto the dishes in the lower
basket.
Operation
Interrupting a programme
A programme is interrupted as soon as
the door is opened.
When the door is closed again, the
programme will continue from the point
it was at before the door was opened.
,Water in the dishwasher may be
hot. Danger of scalding.
Only open the door if absolutely
necessary and exercise extreme
caution when doing so. Before
closing the


o.
If this does not happen, start the
procedure from the beginning again.
^ Press the Turbo/Combi tabs button
five times.
The Combi tabs indicator light will flash
briefly five times at intervals.
43
Cleaning and care
Cleaning the reflector panel
Check your dishwasher regularly
(approx. every 4 - 6 months). This
way faults and problems can be
avoided.
The reflector panel for the In-operation
indicator light is situated in the
coverplate underneath the worktop.
It can be taken out of its plastic holder
to be cleaned.
*In the UK, Miele branded cleaning
and conditioning products as well as
a microfibre E-cloth which is suitable
for cleaning surfaces such as
stainless steel, glass, plastic and
chrome without the use of chemicals
are available from the Miele Spare
Parts Department or via the internet
on www.miele.co.uk.
^ Open the door and carefully remove
the reflector panel from the holder.
^ The reflector panel and its plastic
holder should only beRemove the lower basket.
Particles of food can get stuck in the
spray arm jets and bearings. The spray
arms should therefore be inspected
and cleaned regularly (approx. every
4 - 6 months).
^ Switch the dishwasher off.
Remove the spray arms as follows:
^ Take out the cutlery tray (if your
dishwasher is fitted with one).
^ Push the top spray arm upwards to
engage the inner ratchet. Then
unscrew the spray arm.
^ Push the middle spray arms upwards
a to engage the ratchet. Then
unscrew the spray arm b.
^ Pull the lower spray arm firmly
upwards to remove it.
^ Use a pointed object to push food
particles into the spray arm jets.
^ Rinse thoroughly under running
water.
^ Replace the spray arms and check
that they rotate freely.
48
Problem solving guide
With the aid of the following guide, minor problems can be easily corrected
without calling in a


rectifying the problem you
must:
– Switch the dishwasher off with
the Off button o.
– Open the stopcock fully.
– Clean the water inlet filter (see
"Maintenance").
– The water pressure at the intake
is lower than 30 kPa (0.3 bar).
Seek professional advice.
– Clean the filter combination. See
"Cleaning and care".
– Clean the drain pump. See
"Maintenance".
– Clean the non-return valve. See
"Maintenance".
– Remove any kink in the drain
hose.
51
Problem solving guide
General problems
Problem
The Salt indicator
light starts flashing.
Possible cause
The salt reservoir has
not been closed
properly.
The salt reservoir has
not been closed
properly.
The dishwasher
stops during a
programme.
The In-operation
indicator is flashing
quickly.
The buzzer sounds.
The Salt indicator
flashes when the
door is open.
Fault code F89 shows
in the display.
Items are blocking
The In-operation
indicator is flashing the path of the middle
spray arm.
quickly.
The buzzer is
sounding.
The Spray arm
indicator flashes
when the door is
open.
52
Remedy
Close the flap to the salt reservoir
properly.
– Switch the dishwasher off with
the Off buttonmay be purchased from
your local electrical supplier.
WARNING: THIS APPLIANCE
MUST BE EARTHED
Plumbing
Connection to the water supply
,Water in the dishwasher must
not be used as drinking water.
– The dishwasher may be connected
to a cold or hot water supply, max.
60 °C. We would only recommend
connection to a hot water supply if it
is economical, e.g. a solar powered
supply. When connected to a hot
water supply all programme stages
which would otherwise be carried out
with cold water will be carried out
with hot water.
– The inlet hose is approx. 1.5 m long.
A 1.5 metre long flexible metal
extension hose, pressure tested to
14,000 kPa/ 140 bar, is available as
an optional accessory if required.
! The inlet hose must not be
shortened or damaged in any way
as it contains electrical components
(see illustration).
– A stopcock with a 3/4" male thread
must be provided on


of water.
– The dishwasher is supplied with
approx. 1.5 m of flexible drain hose
with an internal diameter of 22 mm.
– The drain hose can be extended
using a connection piece to attach a
further length of hose.
The drainage length must not be
longer than 4 m, and the delivery
head must not exceed 1 m.
To vent it:
^ Open the dishwasher door fully.
– If the hose is to be directly fitted to
the drainage outlet on site, use the
hose clip supplied (see installation
diagram).
– The hose can be directed to the left
or the right of the appliance.
– The on-site connector for the drain
hose can be adapted to different
widths of hose. If the connector
protrudes too far into the drain hose,
it will need to be shortened.
Otherwise the drain hose may
become blocked.
– The drain hose must not be
shortened.
,Make sure        \,,\nonumber\\
  \partial_t {\mathbf B}-\nabla{\!\times\!}({\mathbf v}{\!\times\!}{\mathbf B}-\eta{\mathbf J})& = & 0    \,,\nonumber\\
  \nabla{\!\cdot\!}{\mathbf B}& = & 0\,,
\label{eq:mhd}\end{aligned}$$ with conserved variables $\rho$, $\rho{\mathbf v}$, and the *total* energy $e= \epsilon+\frac{1}{2}\rho{\mathbf v}^2 +\frac{1}{2}{\mathbf B}^2$, and where $\epsilon$ denotes the thermal energy density. We use ${\mathbf J}= {\rm
  curl}({\mathbf B})$, and introduce the total pressure $p^{\star}=
p+\frac{1}{2}{\mathbf B}^2$. The inertial acceleration due to Coriolis and centrifugal effects is $\mathbf{a}_{\rm i} = - 2{\bm{\Omega}}{\!\times\!}{\mathbf v}-
{\bm{\Omega}}{\!\times\!}({\bm{\Omega}}{\!\times\!}{\mathbf r})$, where ${\bm{\Omega}}=\Omega_0{\hat{{\mathbf z}}}$ is the axial vector representing the angular frequency at the planet radius, and ${\hat{{\mathbf z}}}$ is the unit vector pointing along the rotation axis of the protoplanetary disk. The gravitational potential is composed of the central potential of a solar-mass star


fix the free parameter $c_{\rm s0}$ according to a value of $h\equiv H/{R}=0.05$, noting that $H \equiv c_{\rm s} \Omega_{\rm K}$ where the Keplerian angular velocity $\Omega_{\rm K}({R}) = \sqrt{GM_\star}\,
{R}^{-3/2}$. Note that, via $r$, the equilibrium rotation profile has a weak vertical shear. One can also see that in the midplane (i.e. for $r={R}$), the flow is sub-Keplerian to order $(H/{R})^2$, which is a consequence of radial pressure support. We chose the normalization $\rho_0$ to yield a vertically integrated column density of $\Sigma=150{\,\rm g}{\,\rm cm}^{-2}$ at the location ${R}=5{\,\rm au}$, yielding a total disk mass of $M_{\rm disk}\simeq 3.6{M_{\rm J}}$, i.e., when accounting for the full azimuthal extent of $2\pi$. In terms of the disk temperature, we obtain $T=540{\,\rm K}$ at ${R}=1{\,\rm au}$, and $T=108{\,\rm K}$ at aplanet’s Hill radius – corresponding roughly to Callisto’s semi-major axis. This amounts to a small fraction of the mass within a sphere of $r_{\rm acc}$ being removed per time step. To avoid discontinuous behavior in the accretion flow near the planet, removal is weighted with a three-dimensional Gaussian kernel. Owing to limited computational resources, the mass augmented to the planet is artificially enhanced fourfold to facilitate a speed-up of the gap formation process. In cases where we evolve an energy equation, the modification to the gas density is accompanied by a correction in the thermal energy density as to keep the temperature constant. Within a sphere of $2r_{\rm
  acc}$, we apply additional cooling to avoid the buildup of strong pressure gradients that would otherwise modify the accretion


because each fluid element now has its own thermal history leading to moderate pressure fluctuations in the CPD. This changes in the MHD case shown in panel (a), in which the flow pattern becomes turbulent, but otherwise appears similar to the equivalent HD simulation.

In their study of giant planets embedded in fully-turbulent disks without dead-zones, @2003MNRAS.339..993N comment on the fact that the spiral wave structure in turbulent protoplanetary disks has a more washed-out and diffused appearance than observed in laminar disks. This is clearly not the case here in the midplane because the dead-zone contains only relatively low-level density perturbations due to waves propagating from the over-lying active layers. The dominant perturbations are the spiral wakes excited by the planet. At higher, more turbulent latitudes in this disk,region near the planet for the locally-isothermal run N2. Superimposed streamlines show that the flow has a high degree of symmetry. Marginally bound trajectories closely follow the Roche lobe (equipotential surfaces through L1, L2 are shown as black lines), indicating that the flow is only weakly affected by pressure forces. The flow within the CPD is nearly circular at this time, but is observed to become more distorted at late times as discussed in Sect. \[sec:details\]. In comparison, the averaged flow field appears less symmetric in the simulation with an adiabatic equation of state and thermal relaxation towards the initial temperature (upper panel of [Figure \[fig:flow\_field\_tau\]]{}). Unlike in the previous case, the circulating flow appears to extend beyond the Roche lobe, and shows some level of distortion. This is partly


due to the fact that the upper panel in [Figure \[fig:flow\_field\_tau\]]{} corresponds to a later time when gap formation is more developed; we generally find that the CPD flow becomes increasingly distorted as the simulations evolve and gap formation becomes more pronounced. The distortion is apparently also amplified by the enhanced pressure forces present in run N1, combined with the in-out asymmetry that the circumplanetary material displays because of the radial temperature profile imposed on the gas.

This trend of reduced order in the fluid trajectories is enhanced substantially when looking at the MHD case, shown in the lower panel of [Figure \[fig:flow\_field\_tau\]]{}: here the flow within the Hill sphere is significantly distorted and less symmetric, presumably due to the combined effect of pressure and magnetic forces. Notably, the flow within(i.e. $\alpha {\,\hbox{\lower0.35ex\hbox{$\sim$}\llap{\raise0.35ex\hbox{$>$}}}\,}0.1$), leading to saturation of the mass accretion rate at a higher value than obtained in a viscous model with a constant $\alpha$ value.

Implications
------------

The above results have a number of implications for planet and satellite formation. The feeding of gas into the gap region from the surface layers of the PPD may have important consequences for the chemistry and dust content of the gas that eventually accretes onto the planet, as dust settling and sequestration in the dead-zone may reduce the heavy element content of this gas as it accretes through the disk. One implication is that gas accreted through a gap in a disk with active surface layers and a midplane dead-zone will have lower opacity. Models of giant planet formation show that the upper-envelope


boundary condition that matches the envelope onto the background protoplanetary nebula model will need to be replaced with one that assumes the envelope has a quasi-free surface, perhaps surrounded by a thick circumplanetary disk. Such calculation were presented by for giant planets undergoing runaway gas accretion, but have not been performed for planets in the earlier phase of quasi-static gas settling. Alternatively this scenario could be explored using 3D radiation-hydrodynamic simulations similar to those presented by @2009MNRAS.397..657A [@2009MNRAS.393...49A].

The comments above concerning the heavy element content of accreted gas also have implications for the formation of satellite systems. @2012ApJ...747...47T have noted already that delivery of gas deep into the Hill sphere from high latitudes may lead to accretion of low-metallicity gas onto the inner CPD if grain growth andHall EMFs, both of which may significantly modify the results we have presented [@2012MNRAS.422.2737W; @2013ApJ...769...76B]. In a future paper we will be particularly interested in examining the influence of ambipolar diffusion in the gap region. The low densities there may allow this effect to quench the turbulent nature of the flow in the gap, and this will have significant consequences for the time dependence of the flow in the Hill sphere.

Related issues that need to be explored are the transport of stellar X-rays into the gap region (as this is crucial for determining the ionisation levels close to the giant planet), and the level of cosmic ray ionization experienced by the PPD. For X-ray ionization, we have taken a simple approach and adopted results from the model of


changing the numerical resolution in the simulations. These calculations did not use mesh refinement. The size of the azimuthal domain used was $\pi/4$ instead of $\pi/2$, but adopting the same grid size ratio $\Delta_r:\Delta_{\phi}$ as in the original simulation. The time evolution of the Maxwell stress evaluated between the radii $3 \le r \le
4{\,\rm au}$ for the different models is shown in the left-hand panel of [Figure \[fig:appendix\]]{}. The number shown in the inset is the number of radial grid cells, $N_r$, where $N_r=384$ in model M1. When changing the radial resolution we also changed the resolution in the other dimensions by the same factor. We see that there is little evidence of a systematic trend in the results as a function of numerical resolution. This point is furtherPhytase-Fe3O4 nanoparticles-loaded microcosms of silica for catalytic remediation of phytate-phosphorous from eutrophic water bodies.
Agriculture P management practices elevate the level of inorganic phosphates in soil that results in phosphorous (P) seepage into water-bodies. This is one of the key factors that have accelerated the menace of eutrophication. Phytic acid (phytate)-P-rich plant metabolite is infamous for its anti-nutrient activity and regularly oozing in to environment though discharge of mono-gastric animals. That has amplified the magnitudes of eutrophication. In this work, for catalysis of phytate-P, the metal-organic framework fabricated towards metal oxides (Fe3O4) and phytase in highly ordered microcosms of silica was employed. The synthesized framework was characterized through transmission electron microscopy (TEM) and nitrogen isotherm analysis. Average pore diameter of synthesized bisect oval shaped structures was measured around ≈200


nm. Herein, phytase and Fe3O4 nanoparticles were loaded to the cavities of microcosms through glutaraldehyde-mediated crosslinking. Whereas Fe3O4 nanoparticles act as nano-absorbents that adsorb P liberated from phytase-mediated catalysis of phytate. Kinetic analysis of free and loaded phytase has shown relatively small reduction in catalytic efficiency. These loaded microcosms have removed 60-80% of phytate-phosphate. The optimized process has reduced the growth of photoautotrophs by 50%. Additionally the magnet-assisted separation of loaded microcosms eased the reapplication of loaded microcosms tested for six independent instances. The primary studies conducted to evaluate the geno-toxicity of loaded microcosms have not shown any harmful effect on the process like cell division and seed germination. The efficacy of this method has evaluated towards on-field testing in Changa (Gujarat, India) lake.suffocating, oppressive, steady reminder that you were happy once, until something went wrong. You can't make it right, you can't even name it. But you have to pretend to accept it, and hope one day you fool yourself.


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