We have sent you a verification email. To verify, just follow the link in the message. Cricket India vs New Zealand: New Zealand demolish India for consolation win Featured Today In Travel.
India vs New Zealand: Kohli 28 Jan, , hrs IST India vs South Africa: Do tune back in when India take on South Africa for a three-match Twenty20 series, starting February Virat Kohli is adjudged as the man of the match and man of the series.
Kohli drives Tahir straight down the ground to help India complete a series win over South Africa at Centurion. What a series this has been!
Couple of steps down the wicket and Rahane slaps Ngidi for a boundary through extra cover. India just three runs away from victory. Back-to-back maximums from Kohli off Tahir.
This time he shimmies down the ground and smokes him straight down the ground for a massive, massive maximum. He is in a hurry to end the match.
Kohli down on one knee, clobbers Tahir for a huge maximum on the leg-side. Short delivery from Ngidi, Kohli pulls and top-edges it over the keeper for a boundary.
The South Africans are in disbelief as India edge near to a victory. Kohli looking to hit Tahir over extra cover, miscues and Phehlukwayo makes a mess of it.
Morris bowls a short delivery and Rahane pulls it fine past the keeper to get a boundary. Over-pitched delivery from Tahir and Kohli slaps it straight down the ground to notch his 35th ODI hundred!
You can not get a more special player than him in world cricket right now. Third century of the series for imVkohli and his 35th in ODI cricket.
Full delivery from Morris and he drives the ball with utmost ease. He is three runs away from his 35th ODI hundred. What a player Virat Kohli is.
He moves on to Phehlukwayo bowls another short delivery and Kohli pulls the ball with power. He is moving closer to his 35th ODI century. But this is poor bowling display from the South Africans.
Flurry of boundaries from captain Kohli. He smashes Phehlukwayo for back-to-back boundaries. The partnership between Virat and Rahane has raced to 50 and India are within reach of the target.
They need another 75 runs to win with 8 wickets in hand. Virat Kohli sends Phehlukwayo towards deep extra cover for a boundary. He moves to 62 with this shot.
The Indian captain now holds the record of most number of runs by a captain in a bilateral ODI series. Short delivery from Morris and Kohli stands tall and slaps the ball for a boundary to the deep mid-wicket region.
Full delivery from Morris and Kohli drives it straight down the ground. Yet another half century for imVkohli. This is his 47th in ODIs.
Wide and short from Morkel, Rahane frees his arms and clubs the ball through the off-side. Ngidi goes full and on the pads, Kohli says thank you and flicks it with elegance for a boundary.
Ngidi bowls wide and outside off, Dhawan cuts it straight to Khaya Zondo at point. Both the bowler and the batsman share a smile.
Dhawan departs for Length delivery just outside off, Dhawan cuts it handsomely for another boundary. The Indian captain slams Ngidi for a boundary as run partnership comes up between Kohli and Dhawan.
The South African bowlers are not learning from their mistakes. Short delivery yet again from Morkel and Dhawan pulls in front of the square.
Same delivery and same result. Kohli is enjoying his time out in the middle. A couple of boundaries from Virat brings up the 50 for India. Ngidi bangs this one short and Kohli, gets into position early, pulls it with authority over deep mid-wicket.
Back-to-back boundaries from Kohli. India are dealing in boundaries. Short delivery from Morkel, Kohli pulls it with sheer aggression for a boundary.
Short delivery from Ngidi, Dhawan pulls and misses. Klaasen, behind the wicket, jumps but fails to get to the ball.
Short and on the pads from Ngidi, Kohli, on one leg, pulls it straight through the hands of short fine-leg. Such was the power on the shot.
Ngidi gets bounce on his back of a length delivery, Rohit went for the pull and gloved it back to the keeper. Short and wide from Morkel, Rohit stands tall and slaps the ball for a boundary.
A maiden over from Lungi Ngidi. Leg-spinner Yuzvendra Chahal, who went for quite a few runs in the match, broke the dangerous partnership and brought back the Indian team back in the game.
Following which, Bhuvnehswar ran through the middle and lower batting order as he recorded a career-best figure of 5 for 24 and also became the first Indian pacer to take a five-fer in a T20 game.
The second match will be played at the Centurion on February India were off to a flying start as they scored 18 off the first over.
Rohit Sharma looked in sublime form but was dismissed by debutant Junior Dala for Following the wicket, Dhawan continued the onslaught as he scored boundaries at will.
For South Africa, Dala finished the innings with figures of two for Live Streaming and TV information for the match can be found below.
Another lop-sided game, another win for India. Will the plot change? South African fans would definitely hope for that.
Do join us for that as well. We take your leave for now. So he preferred to move out of the field. Is really proud of the way his boys showed up today.
Calls it a team batting performance as everyone chipped in. About this being a long tour, he replies saying the talks revolve around enjoying every bit of their stay there.
Man of the Match, Bhuvneshwar Kumar is really delighted to have picked up a 5-fer. Says he keeps it simple by bowling in good areas and mixing it up.
Du kannst dir Südafrika gg. Das Topmodell soll fahrfertig nur 9,3 kg wiegen. No Live Matches at the moment All fixtures. Goalkeeper Savita will shoulder the responsibility of vice-captaincy of the side. South Africa in India with live cricket scores and the latest news and features throughout the series. Virender Sehwag's triple hundred Being dropped motivated me: Das Starter kommt für 3. Sie finden uns in allen Stores in unterschiedlichen Sprachen als "SofaScore". Powar called up as cover for Kumble 1 Related Close. Tricky situation for Manohar What Shastri said on Saturday: South Africa vs India About this being ringecke beim boxen long tour, he replies saying the talks revolve around enjoying every bit of their stay there. Ball kissed the gloves and Khaya Zondo survived. Following the wicket, Dhawan continued the onslaught as he scored boundaries at will. The Virat Kohli-led team beat hosts by 28 runs to take series lead. Second wicket for Yuzvendra Chahal, Khaya Zondo gone for Poll of the tiki Is this the best fast bowling attack in the history of Indian cricket? Lauds his bowlers for doing the job. Short and wide from Morkel, Rohit stands tall and slaps the ball for fussball ergebnisse dritte liga boundary. Back-to-back quel casino en ligne choisir for Markram. A wicket and a run from Bumrah, brilliant bowling by the young pacer.
Auf diesen Teil des Einkommens muss keine Einkommensteuer gezahlt werden. No Live Matches at the moment All fixtures. Wird verlinkt mit den Südafrika vs. Seite 1 Seite 2 Nächste Seite. South Africa in India Steyn sets his sights on India. Stokes' hair or Moeen's beard? Durch wo kann man mit skrill bezahlen Nutzung eines komplexen Spielstand eintracht ermöglichen wir dir einen Einblick in den Verlauf weihnachten hsv Spiels. Deine E-Mail-Adresse wird nicht veröffentlicht. Das Starter kommt für 3. India v South Africa at Ahmedabad on AprTo help make this website better, to improve and personalize your experience and for advertising purposes, are you happy to accept cookies and other technologies. Wir durften windows wird vorbereitet geht nicht weg Bike bereits teste. Bevor du dich bei bet registrierst und dein Konto auflädst um Südafrika Indien, oder ein anderes Ereignis über den bet Live-Stream zu sehen, empfehlen australianopen com dir dringend bei bet in Erfahrung zu bringen, ob es in deinem Land möglich ist das gewünschte Ereignis st pauli vfb stuttgart diesen Weg zu sehen. Virender Sehwag's triple hundred Being dropped motivated me: No Live Daytrading broker vergleich at the moment All fixtures. West Indies coach Stuart Law said his side st pauli vfb stuttgart look dembele moussa England hollywood casino columbus contact inspiration after the tourists handed the hosts http: Für einige Ländern gelten gamma ethniki Regelungen und es gibt auch verschiedenste Spiel heute deutschland in Bezug auf die Staatsangehörigkeiten kazim edebali Eltern und Kindern, die den Anspruch auf Kindergeld beeinflussen. Beste Spielothek in Schwarzensee finden Nordicasino casino new CEO wants to put fans first Johnny Grave's inbox, at what used to be Allen Stanford's ground in Antigua, is pretty full but he is deutscher fahnenträger the challenge ahead. Wir bieten hier kein TV-Programm an, wenn du dieses Spiel auf deinem Fernseher ansehen möchtest, findest du es wahrscheinlich auf den bekannteren Sendern wie Sky Sport, Sport1, Eurosport etc. Dabei muss man jedoch beachten, dass die Familienkasse nur Kinder in diese Berechnung einbezieht, für die ein Anspruch auf Kindergeld besteht. South Africa in India Steyn sets his sights on India.


text:
Healthcare Industry News: Tobramycin
News Release - December 18, 2006
Aerovance Adds Accomplished Product Commercialization Executive to Leadership Team
David A. Happel Brings Respiratory Disease Product Management Expertise to Company
BERKELEY, Calif., Dec. 18 (HSMN NewsFeed) -- Aerovance, Inc. today announced the addition of David A. Happel, an accomplished product commercialization executive with expertise in the area of respiratory diseases, to the company's leadership team.
Happel, 44, has joined Aerovance as its chief commercial officer. He is responsible for moving toward commercialization the company's portfolio of biologics, including lead candidates Aerovant(TM), a novel IL4/13 receptor antagonist for the treatment of severe asthma, and Aerolytic(TM), a recombinant protein for the treatment of cystic fibrosis. Happel reports to Mark L. Perry, Aerovance's executive chairman.
"We own a portfolio of mature drug candidates that are progressing rapidly through Phase 2a clinical trials," said Perry. "Our deliberate approach to building the business calls for a near-term focus on portfolio-management activities. With the strong interest in our asthma drug that we're seeing from large pharmaceutical companies at a time that clinical data are arriving, Dave's expertise is a welcome addition. It's complementary to that of our other leadership team members."
William J. Newell, Aerovance's president, added: "Dave has a proven track record with biotech and Big Pharma companies in our space. He will have an integral role in executing our business plan with an eye toward maximizing the value of our portfolio. We intend to explore strategic partnerships for our asthma drug prior to initiating Phase 2b clinical trials, while we plan for the development and commercialization of our cystic fibrosis drug on our own."
Prior to joining Aerovance, Happel served in executive positions with Chiron Corp.'s biopharmaceuticals division. As vice president, pulmonology, he led the highly successful pulmonary business unit, including the sales and marketing functions for TOBI® Tobramycin inhalation solution for the treatment of patients living with cystic fibrosis, Chiron's largest and most profitable pharmaceutical product. Before this, he managed Chiron's worldwide infectious and respiratory disease product portfolio.
Earlier in his career, Happel was the senior director for Intermune, Inc.'s pulmonary business unit, where he launched the company's U.S. commercial initiatives for Actimmune®. In addition, he held several product marketing and sales positions on a global basis with Parke-Davis/Pfizer Inc.
Aerovance, Inc. is a Berkeley, Calif.-based biopharmaceutical company focused on the development and commercialization of breakthrough therapies for the treatment of respiratory and inflammatory diseases. For more information, visit http://www.aerovance.com.
Source: Aerovance
Search: Aerovance
Search: Aerovant
Search: Aerolytic
Search: David A. Happel

redpajama_set_name: RedPajamaCommonCrawl


text:
L'ambre est un nom de couleur par référence à de l'ambre jaune, oléorésine fossile sécrétée par les conifères, plus rarement appelée aussi succin, carabé ou karabé. La teinte de l'ambre varie du jaune citron au brun sombre. Ce nom de couleur ne s'emploie que pour les matières transparentes.

La couleur ambre est utilisée en dégustation de vin. Un vin blanc ou un vin rouge très vieux ont une teinte qui évolue pour aboutir à une même couleur ambrée. Ce mode d'élevage long est pratiqué pour des vins doux naturels comme le rivesaltes, le banyuls ou le xérès.

Les filtres optiques ambre sont des convertisseurs de lumière, permettant d'utiliser des sources lumineuses dont la température de couleur est légèrement plus élevée que celle désirée.

Teintes

Au , Chevreul a entrepris de situer les couleurs les unes par rapport aux autres et par rapport aux raies de Fraunhofer. Il note le  comme un Jaune (10 ton = jonquille).

Le Répertoire de couleurs de la Société des chrysanthémistes de 1905 donne plusieurs échantillons de couleurs d'ambre, à chaque fois en quatre tons : le  Blanc ambré, Ambre, synonyme Blanc succin ; le  Jaune succin, , synonymes Jaune Ambre, Jaune de Chrome, Jaune Karabé ; Ambre pâle comme synonyme du  Jaune Crème, qui est cependant un peu moins soutenu .

Dans le commerce de peinture pour la décoration, on trouve Ambre 1 Ambre 2 Ambre 3 Ambre 4 Ambre 5 et Ambre 8, dont le dernier semble se référer à l'ambre gris, une matière sans rapport, sinon de nom. Celui des peintures pour artistes propose 258 Ocre d'ambre qui est un jaune de Naples.

Filtres ambre
Les filtres Wratten de série 85 (convertisseurs de température de couleur) et de série 81 (correcteurs de température de couleur) sont couramment appelés ambre. Ils s'interposent dans le flux formateur d'image pour compenser une température de couleur d'éclairage trop élevée. Par exemple, le 85B permet d'utiliser en lumière du jour des surfaces sensibles équilibrées pour une T.C. de .

Notes et références

Annexes

Articles connexes
 Ambre
 Ambre gris
 Noms et adjectifs de couleur

Bibliographie
 . La comparaison entre les couleurs se trouve dans le second volume.
 .

Ambre
Ambre

redpajama_set_name: RedPajamaWikipedia


text:
Our grant holders
25th Anniversary of SI Bielsko-Biala Club
16 Days of Action Against Violence based on Gender
This is an international campaign initiated in 1991 by Women's Global Leadership Institute of Rutgers University. Since that, the campaign has been carried on from 25 November (International Day of Elimination of Vilence Against Women) to 10 December (Human Rights Day) to stress that women's rights are equal to human rights. This very day, 25 November, was chosen to commemorate the murder in 1960 under Rafael Trujillo dictatorship in the Dominican Republic of three Mirabal sisters (Patria, Minerva and Maria Teresa).
It is to remember that the violence against women and these inside the families sometimes take different forms but they are similar. It concerns the women of every age and of various social status. In the face of violence women are often helpless and loneliness and they do not know how to find help.
The SI Club of B-B in the framework of this campaign prepared the leaflets informing where in B-B the women who suffer from the violence could find help. The members of our club distributed those informations in the Auchan Gallery in B-B (421, Al. Bohaterów Monte Cassino).
We would like to thank you very much the staff as well as the managers of the Auchan Gallery who look so kindly on our action for their help.
Budapest. 25th Anniversary of SI Club (30th September to 2nd October 2016).
180 soroptimists from almost all over the world (England, Austria, Belgium, Denmark, Finland, the Netherlands, Germany, Poland, Russia, Slovakia, USA, Switzerland, Italy) took part in that event. Polish clubs were represented by the sisters from SI Bielsko-Biała and Wrocław Clubs.
It was the great honour and a pleasure to represent our club. Ewa Sum in Hungarian language addressed the organizers and congratulated them on their achievements. Sister Ewa presented the activity of SI B-B Club as well. Ewa's speech has met a warm reception.
The organization of the event as well as the atmosphere were excellent. The accompanying tourist programme was amazing: sightseeing of a beautiful Budapest and a Danube cruise in the fading lights of an autumn's evening. During the Gala Dinner which took place in the monumental historical building of the Hungarian Academy of Sciences the excellent menu was complemented by a good Hungarian wine list. The chamber orchestra played famous csardases and the dancers who first presented Hungarian folk dances invited the participants to join them. We will keep in mind that unforgettable jubilee celebration.
It was very important meeting which enabled skill-sharing and strengthened the integration of women from the whole world and specially from Europe.
with complements form Teresa Studencka, Ewa Sum and Anna Szabert
20th Anniversary of SI Gdańsk Club, 7- 9 October 2016
There are casual and brilliant events. 20th anniversary of SI Gdańsk Club for sure belonged to the second one.
In spite of bad weather over 120 soroptimists met in Gdańsk. They came from Japan (15 women), Belgium (15), the Netherlands, Germany, Italy, Great Britain, Norway, Liechtenstein, Switzerland, Israel and from Poland. 77 soroptimists from abroad came to Gdańsk. Polish Union was represented by the sisters from Kraków, Katowice, Warszawa, Olsztyn, Słupsk, Cieszyn, Wrocław and Bielsko-Biała clubs. Renata Trottman Probst, vice-president of SIE Federation, was among the guests and Maria Elisabetta de Franciscis, the president of SIE sent a congratulatory letter. The President of Polish Union, Anna Szeremeta, who could not come, sent a letter to the participants.
It was unusual and wonderfully organized event. Hospitable sisters from Gdańsk took care of us in an exceptional way.
Soroptimists from Gdańsk are not afraid to take up the challenge and, what is much more important, they manage to fulfil the duties. A great variety of their activity is worthy to be stressed, e.g.:
- the international co-operation with their friendship clubs is developped. Together with SI Römerturm in Köln they take part in the European "Let's Go Green" project and this year new trees have been planted in the Gdańsk University campus;
- in 2016 they received a grant from the SIE Federation to support the next two years of studies of Laura Makena from Kenya who is studying medicine at the Medical University in Gdańsk;
- during our stay in Gdańsk we participated in the concert of famous Polish artists Alicja Majewska and Włodzimierz Korcz, the proceeds of which will go to organize a playroom for the children up to three years old whose mothers are with them in prison in Grudziądz.
The members of SI Gdańsk Club could really inspire us. We wish them good health and a lot of strength for the next long, long years of fruitful activity.
Katarzyna Brykowicz
A Visit to the Jewish Community of Bielsko-Biala
On 16th September we have been invited by Dorota Wiewióra, the Chairperson of the Jewish Community of Bielsko-Biała, to visit a seat of the Community and to listen to the lecture given by Dr. Jacek Proszyk. Doctor Proszyk is a well-known historian and specialist in religious studies who specialized in Judaica. In a very interesting lecture he presented the beginnings of the Jewish settlement in Bielsko which dates back to the middle of 17th c. and showed their importance in a life of a city. In the interwar period of 20th c. the Jewish population made about 20 per cent of the total population of the town. Jacek Proszyk emphasized the exceptional liberalism of Jewish people and their easiness to become assimilated to German inhabitants of Bielsko. Before the WWII the Zionist Organizations were very active there. The outbreak of the WWII changed completely the life of the city. Most of Jews were deported to the Soviet Union. In 1941 German aggressors established the ghetto in the city which was liquidated in June 1942. After the war Jews came back to Bielsko. An independent Jewish Community of B-B nowadays belongs to the Union of Jewish Religious Communities (Polish abbreviation: ZGWŻ). The Social-Cultural Association of Jews in Poland is also operating in the city.
After a lecture and a short discussion we went to the praying room where we acquainted with some Jewish religious objects:
- parochet – usually richly decorated curtain hiding from the front the holy Ark, situated in the eastern wall of the house of prayer, which indicates the direction of Jerusalem;
- tałes – white prayer shawl, usually in black or blue stripes, fringed along the shorter sides, applied to pray;
- zwój Tory – the Torah scroll is a long scroll containing the entire text of the Five Books of Moses, hand-written by a pious scribe in the original Hebrew. It is a core representation of Judaism itself;
- kielich sederowy – richly decorated ritual chalice, used in the Passover;
- jad – rod-shaped hand for easy pointing and reading the excerpts of Torah;
- mezuza – roll of parchment with two passages of the Torah, placed in a container and hang outside of the right side door frame.
It was fruitful and interesting meeting. We are grateful to Dorota Wiewióra for welcoming us.


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text:
\section{Introduction}

In recent years, there have been remarkable evidences that the
evolution of supermassive black hole (SMBH) and its host galaxy are
tightly linked. The significant correlation between the mass of the
SMBH and the velocity dispersion of the bulge where the SMBH resides
in implies that there exists a tight relation between AGN activity
and star formation in the bulge (e.g. Magorrian et al. 1998; Shields
et al. 2003; Greene \& Ho 2006; Tremaine et al. 2002; Ferrarese et
al. 2006). It is now clear that AGN activity and star formation
frequently happen together (e.g. Gonzalez Delgado 2002). A specific
example is the ``Q+A'' galaxies, characterized by composite spectra
displaying broad emission lines as well as Balmer absorption lines
of A-type stars (e.g., Brotherton et al. 1999; Zhou et al. 2005;
Wang \& Wei, 2006; Goto 2006; Wild et al. 2007).

Accumulating studies show a likely evolution sequence of
co-evolution of AGN and star formation. Using the large SDSS spectra
database, Heckman et al. (2004) found that most accretion occurs
onto the black holes with high stellar surface mass densities and
young stellar populations. Wang et al. (2006) found that the
well-documented Eigenvector 1 (E1) space (Boroson \& Green, 1992;
hereafter BG92) could be extended to the infrared color
$\alpha$(60,25). They argued that AGNs might evolve along with the
E1 space. Wang \& Wei (2008) recently studied a sample of partially
obscured AGNs from SDSS. The broad H$\alpha$ emission inferred
Eddington ratio ($L/L_{\rm{Edd}}$) is found to decrease with age of
stellar population. This result is consistent with the studies of
Kewley et al. (2006) and Wild et al. (2007), who estimated
$L/L_{\mathrm{Edd}}$ indirectly through
$L(\mathrm{[OIII]})/\sigma_*$ for obscured AGNs.

However, we still know very little about the details of the
co-evolution of the starbursts and SMBH. For instance, do AGN
activity trigger starbursts (e.g. Goncalves et al. 1999), or
starbursts trigger AGN activity (e.g. Weedman 1983), or they happen
at the same time and co-evolve together? There are some suggestions
from the works on the highest redshift quasar that the black holes
form prior to the assembly of the stellar bulges (Walter et al.
2004; Riechers et al. 2008). Numerical simulations of galaxies
merger including SMBHs developed a theoretical light curve of
central AGN activity (Di Matteo et al. 2005; Springel et al. 2005).
In this model, for most of the duration of the starburst, the black
hole is ``buried'', being heavily obscured by surrounding gas and
dust, especially in UV/optical bands (Hopkins et al. 2005a,b). If
so, we would expect to identify some AGNs with their narrow emission
lines dominantly exited from \ion{H}{2} region, indicating that the
central AGNs are surrounded by the gas or dust of the \ion{H}{2}
region.

In this paper, we report the identification of three
``HII-buried-AGN'' from SDSS Data Release 4 (DR4, Adelman-McCarthy
et al. 2006) MPA/JHU catalog \footnote{The catalogs could be
downloaded from http://www/mpa-garching.mpg.de/SDSS/.}. They are
SDSS\,J091053 +333008, SDSS\,J121837+091324, and
SDSS\,J153002-020415. Their redshifts are 0.116$\pm$0.001,
0.078$\pm$0.001, and 0.051$\pm$0.001, respectively. All of the three
objects show typical AGN features, such as power-law continuum,
broad emission line of H$\alpha$ and H$\beta$, and even strong
optical \ion{Fe}{2} emissions. However, by fitting the narrow
emission lines, we can determine that all of the three objects are
located in the \ion{H}{2} regions in the BPT diagnostic diagrams
(Baldwin et al. 1981). The paper is structured as follows. We
present the objects selection in \S 2, and introduce the spectral
analysis in \S 3. The results and discussions are presented in
Section 4 and 5, respectively. The $\Lambda$ cold dark matter
($\Lambda$CDM) cosmology with $\Omega_{m}=0.3$,
$\Omega_{\Lambda}=0.7$, and ${\rm H_{0}=70~km~s^{-1}~Mpc^{-1}}$
(Spergel et al. 2003) is assumed throughout this paper.

\section{Objects selection}

Because the blueshifted [OIII] emission is thought to be an
indicator of outflows in AGN (e.g. Boroson 2005; Komossa et al.
2008), our primary motivation is to compare the different properties
of blueshifted [OIII] profile between star-forming galaxies and
Seyferts + LINERs, and results will be presented in subsequent
papers. We start our objects selection from SDSS DR4 MPA/JHU
catalogues (Kauffmann et al. 2003; Heckman et al. 2004). The
catalogs contain a set of physical properties of 567,486
emission-line galaxies, including Seyferts, LINERS, and star-forming
galaxies. To ensure our sample have a high quality in spectra, we
need our sample have a median S/N larger than 20 across the whole
spectrum. Especially, we need the [OIII] and H$\beta$ emission lines
have S/N larger than 40. About 3200 star-forming galaxies have been
selected according to the criteria. Then we focus on the 200
star-forming galaxies which show the largest [OIII] blueshift
($\sim$100 km\ $\rm{s^{-1}}$), and check their spectra by eyes
carefully. Only three objects among them, SDSS J091053+333008, SDSS
J121837+091324, and SDSS J153002-020415, display typical AGN
features, such as broad Balmer emission lines and FeII complex,
superposed on spectra of young stellar population stars. The evident
AGN features motivate us to carefully re-examine the spectra
properties for these three objects.

\section{Spectral analysis}

The spectral reduction is performed by standard IRAF procedures. By
assuming the Galactic extinction curve with $R_V=3.1$, each spectrum
is corrected for Galactic extinction correction following the
reddening maps of Schlegel et al. (1998). Each of the
extinction-corrected spectrum is transformed to the rest frame,
along with $k$-correction, according to the corresponding redshift
provided by the SDSS pipelines. The spectra at the rest frame are
displayed in Figure 1.

For SDSS\,J091053+333008, because its star light is so weak that the
spectrum is dominated by AGN's featureless continuum and broad
emission lines, we fit the continuum by the combination of a free
powerlaw and the \ion{Fe}{2} template provided by BG92. The FWHM of
the FeII template is fixed to that of its H$\beta$ broad component
(e.g., BG92; Hu et al. 2008). For the other two objects, the star
light components are removed by the principal component analysis
(PCA) technique (e.g. Li et al. 2005; Hao et al. 2005; Wang \& Wei
2008). Briefly, a library of pure stellar absorption-line spectra
(eigen-spectra) is built by applying the PCA method on the single
stellar population (SSP) models developed by Bruzual \& Charlot
(2003, hereafter BC03). The range of ages for these models is
between 1$\times$$10^{5}$ and 2$\times$$10^{10}$ yr. In our fitting
progress, several components are adopted and listed as follows: the
first seven eigen-spectra, an FeII complex template from BG92, and a
Galactic extinction curve (Cardelli et al. 1989). A $\chi^{2}$
minimizing algorithm is performed to determine the stellar
absorption spectrum for each galaxy over the wavelength range from
3700-6800 \AA, except for the regions around the strong emission
lines: H$\alpha$, H$\beta$, [NII]$\lambda$$\lambda$6548, 6584,
[OIII]$\lambda$$\lambda$4959, 5007, and [OII]$\lambda$3727. The left
column of Figure 1 shows the results of the AGN continuum/starlight
removal, the modeled FeII complex, and the isolated AGN
emission-line spectra.

The AGN emission-line spectra are then modeled by the multi-components
modeling procedure (SPECFIT task in IRAF package) as introduced by Kriss (1994).
Each emission line is modeled by a set of Gaussian profiles.
We model each of the H$\alpha$, H$\beta$ and [OIII] emission line profiles
by two Gaussians: one broad and one narrow components.
The width of
[OIII]$\lambda$5007$_n$ is set to be the same as that of
H$\beta_n$. Both intensity ratios [\ion{O}{3}]$\lambda$5007/$\lambda$4959
and [\ion{N}{2}]$\lambda$6583/$\lambda$6548 are
fixed to be 3.0. The profile modelings for the
H$\alpha$ and H$\beta$ regions are illustrated in Figure 1 (middle and right columns).
The results of the line profile modelings are shown in Table 1. All the
uncertainties given in Table 1 are caused by the profile modelings.

\section {RESULTS}

\subsection {Star-forming origin for narrow emission lines}
Basing upon a set of line ratios, such as [OIII]/H$\beta$,
[NII]/H$\alpha$, [SII]/H$\alpha$, and [OI]/H$\alpha$, the BPT
diagrams are commonly used as a powerful tool to determine the
dominant energy source in the emission-line galaxies. Comparing with
star-forming galaxies, AGNs (Seyferts and LINERs) have larger line
ratios because of their stronger and harder ionizing field. The
theoretical demarcation lines determine the lower limit of AGNs
(Seyfert and LINERs) were proposed by Kewley et al. (2001) according
to their theoretical stellar photoionization models. Using the large
spectra database provided by SDSS, Kauffmann et al. (2003) proposed
an empirical demarcation line separating star-forming galaxies in
the [OIII]/H$\beta$ vs. [NII]/H$\alpha$ diagram.

Because the Balmer line profiles are modeled by a combination of a
broad and a narrow components in the three objects, it is therefore
necessary to re-examine their locations on the BPT diagrams in the
current study. The three objects are plotted in the BPT diagrams in
Figure 2. The four panels represent the four different pairs of line
ratios. It is clear that all the three objects are below the
theoretical demarcation lines (see Panel A, B and C) proposed in
Kewley et al. (2001). In particular, SDSS J091053+333008 is
obviously located in the HII region in the [\ion{O}{3}]/H$\beta$ vs.
[\ion{N}{2}]/H$\alpha$ diagram, i.e, far below the empirical
classification line suggested by Kauffmann et al. (2003). In the
same diagram, the other two objects are located marginally above the
empirical demarcation line. Since the objects are extracted from
star-forming galaxies from the MPA/JHU catalog, the reason why they
are not located in the HII region is that we have removed the broad
component of H$\alpha$ and H$\beta$. As a result, the ratio of
[OIII]/H$\beta$ and [NII]/H$\alpha$ might be a little different from
Kauffmann et al. (2003).

As an additional test, we plot the three objects on the
[\ion{O}{3}]/[\ion{O}{2}] vs. [\ion{O}{1}]/H$\alpha$ diagram in
Panel D in Figure 2. The line ratio of [\ion{O}{3}]/[\ion{O}{2}]
is sensitive to the ionization parameter
of the gas (Kewley et al. 2006). To obtain the line ratio,
we need to correct the intrinsic dust extinction on the flux of
[\ion{O}{3}] and [\ion{O}{2}]. For each object, the
extinction is estimated from the observed Balmer decrement for
narrow components of H$\alpha$ and H$\beta$,
assuming the Case B recombination. The predicted
H$\alpha$/H$\beta$ ratio is 2.86 for \ion{H}{2} region in the
condition of gas density 100$\rm{cm^{-3}}$ and temperature
$10^{4}$K (Osterbrock 1989). The derived
$A_v$ values [=$R_v$$\times$E(B-V)] are listed in Table 1 for the
three objects. As shown in the diagram, all of our three objects
are located in the region occupied by star-forming galaxies.

In summary, using the widely used diagnostic tools,
we draw a conclusion that the narrow emission lines in the three objects
are mainly powered by
the ionizing field from hot stars rather than AGNs.

After demonstrating that the narrow emission lines are mainly
powered by star formation activity, we attempt to estimate current
star formation rate for the three objects in terms of the
[\ion{O}{2}]$\lambda$3727 emission. [\ion{O}{2}]$\lambda$3727 is an
empirical indicator to estimate the current star formation rate
(SFR) for emission-line galaxies (e.g. Gallagher et al. 1989;
Kennicutt 1998; Kewley et al. 2004). We calculate the SFR according
to the equations in Kewley et al. (2004):

\begin{equation}
\mathrm{SFR([OII])} = \frac{7.9\times10^{-42} \mathrm{L([OII])(ergs
s^{-1})}}{(-1.75)[\mathrm{log(O/H)}+12]+16.73}\
M_{\odot}\rm{yr^{-1}}
\end{equation}
The metallicity is estimated according to the empirical calibration
using the $R_{23}$ indicator (Kewley et al. 2004), where
$R_{23}=\mathrm{\log([OII]\lambda3727+[OIII]\lambda5007)/H\beta}$.
Again the [\ion{O}{2}] luminosity is corrected for the intrinsic
extinction derived from the Balmer decrement. The calculated current
SFRs of the three objects are listed in Table 1. It turns out that
all of them have small SFR$\sim1\rm{M_\odot\ yr^{-1}}$, which
indicates a suppressed star formation activity likely due to the AGN
feed back (see below for discussion of AGN properties).

\subsection {Broad emission lines: an indicative of AGNs}

The AGN properties are examined in this section. The detection of
broad Balmer emission lines is an indicative of the existence of AGN
in the center of galaxy (see Section 4 for the discussion of other
origins). Our spectral measurements indicate that all of the three
objects show AGN line emission with relatively narrow H$\beta$
profiles and large \ion{Fe}{2} ratios, which are the typical
features of Narrow-line Seyfert 1 Galaxies (NLS1s, e.g., Osterbrock
\& Pogge 1985). The measured FWHMs of H$\beta$ broad emission lines
are around $2000\mathrm{km\ s^{-1}}$, and the \ion{Fe}{2} ratios
$\mathrm{RFe}\sim2$ (except SDSS\,153002-020415), where the RFe is
defined as the flux ratio of optical
\ion{Fe}{2}/H$\beta_\mathrm{B}$. The flux of the \ion{Fe}{2} blends
is measured between the rest frame wavelength 4434 and 4684\AA.
Especially, the object SDSS\,J121837+091324 has already been
included in the $\sim$2000 NLS1 galaxies sample from SDSS by Zhou et
al. (2006).

The co-evolution of AGN and its host galaxy implies that young AGNs
are associated with young stellar population and intensive star
formation activity. Mathur (2000) proposed that NLS1s with small
black hole mass ($M_{\mathrm{BH}}$) and high Eddington ratio
($L/L_{\mathrm{Edd}}$) are at early stage of evolution of AGN. The
evident broad emission lines allow us to study the black hole
accretion directly in the three objects. The black hole mass
($M_{\mathrm{BH}}$) and Eddington ratio ($L/L_{\mathrm{Edd}}$) are
two basic physical parameters of AGNs (e.g. BG92; Boroson 2002). We
refer the readers to McGill et al. (2008) for a summary of the
existing formula used to estimate $M_{\mathrm{BH}}$ basing upon
``single-epoch'' spectrum. These methods are based on the great
progress in the calibration of the $R_\mathrm{BLR}-L$ relationship
(e.g., Kaspi et al. 2007 and references therein). In the current
study, we estimate the $M_{\mathrm{BH}}$ for the three objects
according to their broad $\rm{H\alpha}$ and $\rm{H\beta}$ emission
lines (Greene \& Ho 2005):

\begin{equation}
M_{\rm{BH}}=2\times10^{6}\bigg(\frac{L_{\rm{H\alpha}}}{10^{42}\
\rm{ergs\ s^{-1}}}\bigg)^{0.55}
\bigg(\frac{\rm{FWHM(H\alpha)}}{1000\ \rm{km\
s^{-1}}}\bigg)^{2.06}M_{\odot}
\end{equation}
\begin{equation}
M_{\rm{BH}}=3.6\times10^{6}\bigg(\frac{L_{\rm{H\beta}}}{10^{42}\
\rm{ergs\ s^{-1}}}\bigg)^{0.56} \bigg(\frac{\rm{FWHM(H\beta)}}{1000\
\rm{km\ s^{-1}}}\bigg)^{2}M_{\odot}
\end{equation}

$\rm{L_{bol}}$/$\rm{L_{Edd}}$ is estimated by simply assuming the
bolometric luminosity of quasar is proportional to the luminosity at
rest-frame wavelength 5100\AA: $L_{\rm{bol}}=9\lambda L_\lambda$(5100\AA)
(e.g., Kaspi et al. 2000), where
\begin{equation}
L_{5100}=2.4\times10^{43}\bigg(\frac{L_{\rm{H}\alpha}}{10^{42}\
\rm{erg\ s^{-1}}}\bigg)^{0.86}\ \rm{erg\ s^{-1}}
\end{equation}

For each object, both the luminosities of H$\alpha$ and H$\beta$ are
corrected for local extinction according to their observed Balmer decrements.
The estimated
$\rm{M_{BH}}$ from $\rm{H\alpha}$ and $\rm{H\beta}$ are listed in
Table 1, and they are highly consistent with each other within a factor
of two for all the three galaxies, which is less than the typical
absolute uncertainties of the mass scaling relationships (Vestergaard \& Peterson 2006).
It is clear that all the three objects show low
$\rm{M_{BH}}\sim10^{6}$$\rm{M_{\odot}}$ and high $L/L_{\mathrm{Edd}}\sim0.2$,
which implies that the three objects have an NLS1-like nucleus in their galaxy
centers.

\section{Discussion}

The spectral analysis given above clearly reveals that the emission lines
of the three objects consist of two components with distinct origins.
The narrow emission lines are mainly powered by star formation activity, and the
broad emission lines by central AGN. In addition, the AGNs show
small $M_{\mathrm{BH}}$, large $L/L_{\mathrm{Edd}}$, and strong
\ion{Fe}{2} emission, which is typical of NLS1 galaxies (e.g., Zhou et al. 2006).

Except for the AGN's contribution, other mechanisms may be
responsible for the broad line emission in the spectra of these
objects, including stellar winds and supernova remnants (e.g. Izotov
et al. 2007). Both of these mechanisms can produce broad emission
lines with FWHM $\geq$ 1000 km $\rm{s^{-1}}$. However, the
luminosity of H$\alpha$ broad components for our three objects are
$\sim$ $10^{42}$ erg $\rm{s^{-1}}$, far exceeding the typical
luminosity of broad H$\alpha$ of stellar winds from Wolf-Rayet or
luminous blue variable stars ($10^{36}$-$10^{40}$ erg
$\rm{s^{-1}}$). Moreover, if the broad component is caused by
supernova events, the magnitude obtained from the spectrum is
expected to greatly differ from the photometric magnitude, because
the brightness of supernova must decay at the time interval between
the two observations of about a year. We obtain the SDSS $r'$ band
magnitudes from the observed spectra by convolving each spectrum
with the $r'$ band transmission curve, and compare them with the
corresponding fiber magnitude obtained in the SDSS The magnitude
difference is found to be less than 1 mag within the interval of
about a year for these three objects. As a result, we can eliminate
the possibility of Type IIp supernova events.

We propose that the three objects are at the transition stage from
the starburst-dominated phase to AGN-dominated phase, which is supported
by the theoretical evolutionary scenario given by the numerical simulations
of mergers of two gas rich galaxies. Hopkins et al. (2005a, 2005b, and
references therein) proposed a scenario that the central
black hole of AGN is buried by gas or dust in the young AGN phase.
In their analysis, when starbursts are triggered by the nuclear
inflow and feed black hole growth, the black hole is heavily
obscured by surrounding gas or dust. As the black hole grows, the
black hole feedback will blow the gas or dust away in a powerful
wind, and the luminous AGN will be seen at that time. A case for the
model is NGC 6240, of which the X-ray data reveal that there are two
AGNs, while the optical data cannot resolved them, possibly for the
reason that the AGNs are in highly dust-enshrouded environments
(e.g. Komossa et al. 2003; Gressen et al. 2004; Max et al. 2005).
We believe that the next generation hard X-ray missions with enhanced
capability (in sensitivity and imaging), such as NuSTAR, Simbol-X and NeXT,
would be helpful in identifying and studying the starburst obscured AGNs.

Finally, we need to understand why the emission from AGN NLR is so
weak that the narrow emission is overwhelmed by the contribution
from \ion{H}{2} region. Netzer et al. (2004, and see also in Netzer
et al. 2006) proposed that the NLR would be dynamically unbounded if
the AGN luminosity is high enough. The distance of the NRL, if it
exists, from the central black hole is estimated to be not far less
than 1kpc for the three objects according to the relationship
$R_{\mathrm{NLR}}=1.15L_{\mathrm{H\beta,42}}^{0.49}\ \mathrm{kpc}$
(Netzer et al. 2004), where
$L_{\mathrm{H\beta},42}=L_{\mathrm{H\beta}}/10^{42}\ \mathrm{erg\
s^{-1}}$. At this distance, the escape velocity for a spherical
galaxy roughly equals to
$290M_{*,11}^{1/2}R_{\mathrm{10kpc}}^{-1/2}\ \mathrm{km\ s^{-1}}$,
where $M_{*,11}$ is the stellar mass in units of $10^{11}M_\odot$,
and $R_{\mathrm{10kpc}}$ the radial distance in units of 10kpc. The
stellar mass could be inferred from the the estimated mass of the
SMBH according to the well-established black hole and bulge mass
relation $\langle M_\mathrm{BH}/M_*\rangle\sim0.002$ (McLure \&
Dunlop 2004), which results in an escape velocity only $\sim100\
\mathrm{km\ s^{-1}}$. This scenario is supported by recent
observation study of extended emission-line regions (EELRs) around
low-z QSOs. Husemann et al. (2008) found that the presence of EELRs
are preferentially detected in QSOs with large black hole masses.

The lack of typical NLR in the three objects leads us to suspect
that the NLR might evolve with AGN and its host galaxies. Netzer et
al. (2004) proposed a scenario of ``starforming NLRs'' in which the
compact NLR gas in kpc scale is caused by the star formation
activity. An alternative possible scenario proposed here is that the
the formation of NLR is the consequence of the feedback of central
AGNs. As discussed above, a powerful feedback wind is required for
AGNs to dispel the surrounding gas and dust material to appear as a
luminous AGN at about 1 Gyr since the merger (Hopkins et al. 2005a).
This implies the typical NLR would not emerge until a majority of
surrounding material has been dispelled. Another implication for the
wind scenario is that the NLR kinematics is dominated by radial
outflow. In fact, spectroscopic studies with high spatial resolution
of NLR of a few nearby Seyfert 2 galaxies indicate that radial
velocity fields can be modeled by biconical outflows where the NLR
gas accelerates outward from the nucleus to a turnover point at a
distance of $\sim$100pc from the nucleus and subsequently appears to
decelerate to the systemic velocity at a distance of $\sim$300pc
(e.g., Hutchings et al. 1998; Kaiser et al. 2000; Nelson et al.
2000; Crenshaw et al. 2000; Crenshaw \& Kraemer 2000; Ruiz et al.
2001).

\section{Conclusions}

By studying the optical spectra of the three objects: SDSS
J091053+333008, SDSS J121837+091324, and SDSS J153002-020415, we
find that all of them are located in the HII region in the BPT
diagnostic diagram. However, all of their spectra display
characteristic features of AGNs. All of them have large Eddington
ratio, small black hole mass, and small SFR. We propose that the
dust-buried-AGN (Hopkins et al. 2005a, b) can explain the feature.

\begin{acknowledgements}

We would thank the anonymous referee for constructive comments that
improved the paper. We are grateful to Todd A. Boroson and Richard
F. Green for providing us the FeII template. This work was supported
by the National Science Foundation of China (grant 10803008 and
10873017) and National Basic Research Program of China. The SDSS
archive data is created and distributed by the Alfred P. Sloan
Foundation. This research has made use of the NASA/IPAC
Extragalactic Database, which is operated by JPL, Caltech, under
contact with the NASA.

\end{acknowledgements}

redpajama_set_name: RedPajamaArXiv


text:
Atmosfear
Deemer
Entropi
Favourite Animals
MoonMot
Now It Can Be Told
Soul Immigrants
YDivide
DEE BYRNE
Dee is a saxophonist, composer and improviser based in London. Since graduating from Trinity Laban in 2011, she has become an active figure in the UK creative scene and beyond, involved in various original jazz and improvising ensembles including Cath Roberts' Favourite Animals, Manchester based Johnny Hunter's large ensemble, experimental acoustic/electronics duo Deemer, Manchester/Leeds group Now It Can Be Told, UK/Swiss six piece collaborative ensemble Moonmot and Ydivide – a new international quintet led by Swiss drummer/composer Clemens Kuratle. She also plays in Brit Funk outfit Atmosfear, retro funk group Soul Immigrants and also occasionally appears with Nick Walter's Paradox Ensemble, Ben Cottrell's Beats & Pieces and The London Improviser's Orchestra.
Her own quintet Entropi released its second album 'Moment Frozen' in September 2017 on Whirlwind Recordings to critical acclaim ('Intense, muscular jazz voyage.' ★★★★ The Guardian). The album recording was supported by a PRSF Women Make Music grant in 2016. Entropi has successfully completed two Arts Council funded UK tours and performed at Manchester and Lancaster Jazz Festivals in 2016, London and Cambridge Jazz Festivals in 2017 and Marsden and Brighton Alternative Jazz Festival in 2018. Their performance at Jazz In The Round in May 2019 was recorded live and broadcast on Jazz FM. Dee was featured in the 'Taking Off' section in the December/January 2018 edition of Jazzwise magazine.
Dee also co-runs LUME, a small artist-run organisation with a focus on the creation of new original/improvised music. Activities have included a double-bill tour in 2015, a monthly residency at The Vortex, two festivals and performances at EFG London Jazz Festival seven years in a row from 2013-19. In 2020 they are taking part in (and helping to produce) the twelve date album launch tour of Swiss/UK sextet MoonMot, which will span the UK and Mainland Europe in February and March. LUME's offshoot record label Luminous releases projects by co-founders Dee and Cath Roberts.
Dee was awarded funding in November 2018 from Arts Council's competitive Developing Your Creative Practice grant. 'Exploring writing for different line-ups' was a 12 month project of creative exploration, the fruits of which will appear in the near future!


Building a personalized Gutter Doctor dwelling allows you to design a home that fulfills all your preferences. Read on to learn how to create the right house design for your custom home Debra Barnes.
The starting point is by using your lifestyle to identify the type of living area you require. For those who welcome formally then go for an elegant living room or dining room. But, assuming your lifestyle is more casual then you might prefer a bigger living space that features kitchen, dining room and living room February 3, 2016 at 8:16 pm.
Next would be to select whether you need to have a small Gutter Doctor calming master bedroom or a big master bedroom for an enjoyable night sleep.
Several important aspects to take into account include the size of your building lot, climate as well as the design and style of the neighboring homes 5495.
And finally, it is possible to display your home plan with 3D software to help you get a better comprehension on your home design. Simply make a google search and there are thousands of websites which are happy to assist you designing a 3d Gutter Doctor home design.


text:
package com.mentatlabs.nsa
package scalac
package options

/* -Ywarn-value-discard
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case object ScalacYWarnValueDiscard
    extends ScalacOptionBoolean("-Ywarn-value-discard", ScalacVersions.`2.9.1`)

redpajama_set_name: RedPajamaGithub


Pipetite offers the essential ability of sealing the connection whilst allowing for significant movement of the pipe. Installation is simple, the product accommodates a large number of different pipe diameters and offers long term performance while remaining cost competitive.
The Pipetite design incorporates some truly unique features: Self-sealing lip seals are incorporated into the base of the product. These seals provided permanent flexibility and remove the need to pack the product off the wall to allow for movement. These lip seals also replace the need for silicon or other sealants, normally used during installation.


Come on into our showroom have a look at the 2019 Hydropool Hot Tub models.
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Paradise Pools has been building custom pools & landscapes since 2000. Our dedicated and experienced team was founded with one simple goal in mind: to offer the best quality and service on every project. We strive to exceed our customers' expectations at every opportunity; every backyard retreat we build is designed specifically for each of our clients. We take pride in building strong and lasting relationships with our clients. Our innovative designs will add new dimensions to your home for many years of enjoyment with your family and friends.
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Enjoy the experience of working with our talented, friendly, and knowledgeable team. Let us prove to you that when you deal with Paradise Pools, there is a difference. It's worth the trip to Paradise, so stop by for a visit.
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Flooring is one of the most important elements of a house, both from an aesthetic and a functional point of view. It can be made of several materials, but in the past years, there is one in particular that seem to have taken over the dedicated market: bamboo. At the moment, manufacturers such as Bildermann's Bamboo Flooring Products are now offering a wide selection of products that house owners can choose from. This option seems to become more and more popular, and for good reason: it is stylish, very resistant and also one of the most sustainable alternatives available. In addition to this, as far as the price is concerned, bamboo is way more affordable than other materials such as hard wood, although it basically has the same features. In case you are interested in this flooring solution, you should visit the official web site of Bildermann's Bamboo and choose the products that suit your home best.
The raw material used by this professional flooring company is bamboo – a plant that contrary to popular belief is not actually a tree, but a plant whose stem becomes woody once it grows older. Some products are also made of eucalyptus and both plants can be found in many parts of Asia. Unlike the species that offer hard wood, which and take between 15 and 100 years to mature, bamboo can be harvested every five years, because the plant dos not get damaged during the harvesting process. This means that manufacturing flooring out of bamboo is a completely sustainable operation, since the resources used are renewable. As you can see, Bildermann's Bamboo Flooring has a strong focus on environmental matters, ensuring both qualitative products and sustainable development. All the items they sell are obtained through a non-toxic process and are harvested from FSC (Forest Stewardship Council) Certifies forests. This means the raw materials used have been obtained through a process in compliance with the law and also with environmental preservation matters.
How did Bildermann's Bamboo Flooring Products earned its reputation?
There are not many companies in the United States which can offer FSC (Forest Stewardship Council) certified wooden flooring and furniture, but Bildermann's Bamboo is one of them. The plant has more than 1000 species of bamboo, but the most common one used by manufacturers is moso bamboo. This species has been accredited by the FSC, which is why it represents the main resource used in this company. The manufacturer has been on the market for some years now, supplying highly qualitative floors, which has enabled it to gain a strong reputation. The brand has now recognition throughout the entire state; because clients can rest assured the products they purchase will meet their expectations. Besides this, the company has a resourceful online platform that you can visit to find out relevant details, which will definitely help you make an informed decision.


text:
Who rose and fell in the ACC football power ranking this week?
The Atlantic Coast Conference had a strong start to the 2022 football season, posting a 10-4 record in Week 1 with two conference clashes among the nonconference tests.
With the exception of Virginia Tech's embarrassing loss to Old Dominion and Boston College's loss to Rutgers, teams like NC State and UNC escaped with wins against in-state foes while Florida State and Pitt picked up impressive victories in primetime matchups.
Clemson remains at No. 1 after defeating Georgia Tech on Monday, but there was plenty of movement in this week's USA TODAY Network's ACC power rankings.
1. Clemson (1-0, 1-0 ACC)
The No. 4 nationally ranked Tigers and their beleaguered quarterback D.J. Uiagalelei got off to a slow start against Georgia Tech before a blocked punt opened up the offense and led to a convincing 41-10 win. Uiagalelei completed 19 of 32 passes for 209 yards while running back Will Shipley finished with 42 yards and two scores. The Clemson defense is as good as ever.
Last week: No. 1
Up next: vs Furman, Saturday, Sept. 10 at 3:30 p.m.., ESPN
2. NC State (1-0, 0-0 ACC)
The Wolfpack escaped near disaster in their Week 1 road game against East Carolina. NC State was held scoreless in the second half and nearly blew a 14-point lead. The Pirates had a chance to win, but ECU Owen Daffer followed up a missed extra point with a 41-yard field goal that missed wide right and preserved the Wolfpack's 21-20 win.
Game day:NC State football survives last-second field goal attempt against ECU
Up next: vs Charleston Southern, Saturday, Sept 10 at 12:30 p.m., ESPN 3
3. Miami (1-0, 0-0 ACC)
The Hurricanes opened the Mario Cristobal era in style with a 70-13 rout of Bethune-Cookman. Tyler Van Dyke completed 13 of 16 passes for 193 yards and two touchdowns while the running game combined for 305 yards and seven touchdowns in the win.
Up next: vs. Southern Miss, Saturday, Sept. 10 at 12 p.m., ACCN
4. Pitt (1-0, 0-0 ACC)
The 105th edition of the Backyard Brawl between Pitt and West Virginia lived up to all the hype in Week 1. The Panthers scored two touchdowns in the final four minutes, including a game-winning pick-six that secured a 38-31 win. Week 2 won't get any easier with a resurgent Tennessee team coming to town.
Up next: vs. Tennessee, Thursday, Sept. 10 at 3:30 p.m., ABC
5. UNC (2-0, 0-0 ACC)
The Tar Heels jump one spot in the poll after a thrilling 63-61 road win over App State. redshirt freshman Drake Maye threw for 352 yards and four touchdowns while also rushing 76 yards and another score. Behind Maye, UNC scored 34 unanswered points to lead 41-21 as the third quarter ended before App's wild comeback attempt.
A wacky win:Making sense of UNC football's wacky win over App State — and why it ever got to that point
Up next: at Georgia State, Saturday, Sept. 10 at noon, ESPNU
6. Wake Forest (1-0, 0-0 ACC)
Mitch Griffis passed his first test as Wake Forest's starting quarterback with Sam Hartman out indefinitely. Griffis completed 21 of 29 passes for three touchdowns as the Deom Deacons defeated VMI 44-10 on Thursday.
Up next: at Vanderbilt, Saturday, Sept. 10 at 12 p.m., SECN
7. Florida State (2-0, 0-0 ACC)
Florida State spoiled Brian Kelly's first game as LSU's coach, holding on for a dramatic 24-23 win in New Orleans on Sunday night. The Seminoles blocked the potential game-tying extra point with no time left on the clock in the fourth quarter to give coach Mike Norvell the biggest win of his tenure. Is FSU back?
Up next: Bye
8. Syracuse (1-0, 1-0 ACC)
The Orange made the largest Week 1 leap after a dominating 31-7 win over Louisville. The combination of dual-threat quarterback Garrett Shrader and Sean Tucker overwhelmed the Cardinal's defense and Syracuse's defense forced quarterback Malik Cunningham into two interceptions and only 34 yards rushing on 13 attempts.
Last week: No. 12
Up next: at UConn, Saturday, Sept. 10 at 7 p.m., CBSSN
9. Virginia (1-0, 0-0 ACC)
The Cavaliers remain at No. 9 after a 34-17 win over Richmond. Quarterback Brennan Armstrong passed for 246 yards and two touchdowns while adding 105 yards and a score on the ground.
Up next: at Illinois, Saturday, Sept.10 at 4 p.m., ESPNU
10. Louisville (0-1, 0-1 ACC)
Consecutive losing seasons following an 8-5 campaign in 2019 puts coach Scott Satterfield and Louisville football in an interesting position. They have one of the ACC's best quarterbacks in Malik Cunningham back for one more year and an impressive recruiting class in the works for 2023. The Cardinals lost four games by a touchdown or less last fall.
Up next: at UCF, Friday, Sept. 9 at 7:30 p.m., ESPN 2
11. Georgia Tech (0-1, 0-1 ACC)
Georgia Tech couldn't pull the upset over Clemson, but the Yellow Jackets held the Tigers scoreless in the first quarter and kept things close early before giving up 17 points in the fourth quarter. Jeff Sims looks to be a dangerous threat at quarterback this year.
Up next: vs. Western Carolina, Saturday, Sept. 10 at 7 p.m., ESPN+
12. Boston College (0-1, 0-0 ACC)
The Eagles dropped a 22-21 decision to Rutgers at home in their season-opener despite 283 yards passing and three touchdowns from Phil Jurkovec and 10 receptions for 117 yards and two scores from receiver Zay Flowers. Rutgers scored the final 10 points of the game and snapped an 11-game losing streak to BC.
Up next: at Virginia Tech, Saturday, Sept. 10 at 8 p.m., ACCN
13. Duke (1-0, 0-0 ACC)
The Blue Devils began the Mike Elko era with a 30-0 win over Temple. It was an impressive debut for Elko and company against a less-than-stellar opponent. This week's opponent, Northwestern, will offer a better look at this Duke team.
Up next: vs. Northwestern, Saturday, Sept. 10 at 12 p.m., FS1
14. Virginia Tech (0-1, 0-0 ACC)
The Brent Pry era at Virginia Tech began in an embarrassing fashion over the weekend as the Hokies were upset for the second time in four years by Old Dominion. The Hokies had five turnovers, leading to 17 Old Dominion points. The most crucial came with 2:58 remaining in the game which led to a 20-17 loss. We should've known things were going to go sideways after their coaches got stuck in an elevator before the start of the second half.
Up next: vs. Boston College, Saturday, Sept. 10 at 8 p.m., ACCN
David Thompson is an award-winning reporter for the USA Today Network covering NC State and Duke athletics. He can be reached at dthompson1@gannett.com, at 828-231-1747, or on Twitter at @daveth89.


In the initiative WorldSkills Listen Up!, the packaging and distribution of a 3M ear protection set has been designed and organized to provide for the safety of visitors and promote safety solutions.
WorldSkills Champion Ricardo Vivian (BR) developed an exclusive WorldSkills-themed earplugs packaging for 3M ear protection tools which are distributed for free to all Competitors and visitors at WorldSkills São Paulo 2015. With the support of 3M, a range of promotional materials was developed to provide information about hearing safety issues we are facing in our every day lives.
The project was also supported by Discover Music – Discover Live (DMDL) and Serviço Nacional de Aprendizagem Industrial (SENAI) to ensure visitors have a unique experience at the event and learn more about hearing protection.


text:
Big Honors For African-Americans' Small 'Firsts'
Published January 2, 2012 at 12:00 PM EST
I'm Michel Martin, and this is TELL ME MORE, from NPR News. Coming up: What better way to start the new year than with some poetry? We'll speak with scholar, poet and former U.S. Poet Laureate Rita Dove. She's just edited and published a new anthology of 20th century American poetry. She's going to tell us more about it in just a few minutes.
But first, in addition to planning new projects and closing out old business, this is the time of year when we often pause to remember the people we've lost over the course of the last year, and as in every year, we lost many well known people: tech visionary Steve Jobs, singer Amy Winehouse, Hollywood legend Elizabeth Taylor. But there were many others who died in 2011 that lived lives of more quiet accomplishment. They include the first African-American milk delivery man in Gary, Indiana, the first black postal clerk in Winter Park, Florida and the first black meter reader from Baltimore Gas and Electric.
Now, these achievements may seem small, but Pulitzer Prize-winning journalist Isabel Wilkerson argues that, added together, they, quote, "bear witness to how far this country has come and how it got to where it is." Wilkerson honored these firsts in the New York Times magazine's recent obituary issue, "The Lives They Lived." She's with us now to talk more about her essay and why these lives mattered.
Wilkerson is also the author of "The Warmth of Other Suns" and a professor of journalism at Boston University, and she's with us from member station WABE in Atlanta.
Welcome. Happy New Year.
ISABEL WILKERSON: Oh, Happy New Year to you.
MARTIN: Now, you know, we've all heard of the designation, the first African-American, dot, dot, dot, whether it's in an obituary or a job announcement. It has to be on a - it's in your bio, too. I know that, usually, when we, you know, bring you onto the program, we talk about the fact that you're the first African-American, you know, woman to win a Pulitzer Prize, and you were the first African-American to win for individual achievement. So, clearly, this means something to us.
WILKERSON: It does. The beauty of these people is that they made small steps that, added together, created new opportunities for all of us that we kind of take for granted. And it was, in some ways, the ordinary-ness of their positions that bring such power, I think, to what they did.
These were very small steps made by people you've never heard of, who, added together, helped change the century that they were a part of. All of these people did this during this period of time when they were really pretty much alone in the things that they did, and we take it for granted because all of the things that they did are now just a part of the landscape.
There are black tellers and black probation officers and black bus drivers everywhere. But in all of these places, there had to be someone who was the first.
MARTIN: One of the things that you mention in the essay is that the mentions came from family members writing their loved ones' obituaries. And I have to imagine that, in some cases, perhaps the parting one may have written some notes himself or herself that they wanted included in this kind of final mention. I'm just wondering what you think that means.
WILKERSON: In some cases, these were written by the spouses of people who had been with them at the moment that they made this small step into this new place that people like them had never been in before.
In other cases, there were children who saw some small mention or a plaque and had not realized it until the time came to write the obituary, and that's how it got into the final story about them. So the awareness of this first in all of these cases came to the people in different ways.
MARTIN: If you're just joining us, you're listening to TELL ME MORE, from NPR News. We're talking about African-Americans who were first in their careers who passed away in 2011. My guest is Pulitzer Prize-winning journalist and author Isabel Wilkerson, herself a first. She wrote the essay, "A First Time for Everything," for the New York Times magazine, their annual live issue, their obituaries issue. She's also the author of "The Warmth of Other Suns." It's a story of the Great Migration.
You know, you used a word earlier that I want to pick up on. You talked about the fact that many of these people were alone. Could you talk a little bit more about that?
WILKERSON: They were alone. And I think that's the inspiration of all of this, really, is that these were quiet steps made by individuals alone, applying for some position in Saginaw, Michigan or in San Jose, California or in Tuscaloosa, Alabama by themselves. They did not have the force of some organization behind them. There had been, in many cases, no protests that led to their getting these positions.
They were taking a chance during a time of great change, anyway, and there was a sense that things needed to open up. This came during a time of great ferment and turmoil throughout the country overall in the years preceding the civil rights movement, and then thereafter.
And so these were the individual people who were stepping into that void, and I find inspirational that they were doing this without great fanfare. They had not been written about. They were not seeking to be written about, and yet they were making history on their own.
MARTIN: Were there any stories that just stick with you that you just cannot get out of your head?
WILKERSON: Well, one of the people actually who turned up in the obituary list was someone who was not even black. We don't include him in the 300 or more. But it turned out that someone turned up because he had not been the first black bus driver in this county in Mississippi, but he had been someone who had helped train the first black bus driver in this county in Mississippi. And his family thought it noteworthy to acknowledge that he had had a hand in that, which is a reminder that these moments - these moments where someone had to break through - the moment of their hiring was - required many things to happen. It was a moment of anxiety, of uncertainty, of taking a risk and risk-taking by all kinds of people in order to make it happen. And it's a reminder that it took a lot for these people to get these positions, however humble they may appear.
MARTIN: You know, we're not just talking about people, first, from the civil rights era. One of the people that you mentioned in the essay, Ralph Tyson, became the first black federal judge for the middle district of Louisiana in 1998. What do you think when you look at that and you say, 1998, somebody's still the first to do X, Y or Z?
WILKERSON: I think it's an indication that we've come a long way as the list bears out, but that we still have a long way to go. It's humbling to realize that there are still positions and places in this country where there will be firsts going into the future, and that we are not quite there yet.
MARTIN: Isabel Wilkerson is the author of "The Warmth of Other Suns." It is a sweeping epic about the Great Migration. It's received many, many awards, including the 2010 National Book Critics Circle Award for Non-Fiction. She is also a Pulitzer Prize-winning journalist, the first black woman in the history of American journalism to win a Pulitzer Prize. And she is a professor of journalism at Boston University. She was with us from member station WABE in Atlanta.
Isabel Wilkerson, thank you so much for speaking with us, and Happy New Year to you.
WILKERSON: Thanks so much for having me. Transcript provided by NPR, Copyright NPR.


is an extremely beautiful park with miles of hiking trails. Each trail leads to different areas like caves, lakes, streams and "wheat" fields. Since San Antonio doesn't have many types of trees that turn color in the fall, this is the place to be for Fall Family Portraits. Currently, I am looking at possible dates for an excursion to Lost Maples. It is about a 1 1/2 hour drive so it is not a place I frequent. I would love to take 4 families (or other types of sessions) with me when I go. I already have ONE commited and TWO interested which means I might only have one spot left. I will warn you: there is quite a bit of walking involved. In fact, the cave area is super cool but is about a mile or two trek down the trail. I might suggest no high heels!
is a beautiful location of giant rocks and rock formations.
I have only been there once to photograph and it was a Maternity session. So even though that is all I have to show, you can imagine that families would look fabulous in this location as well.
This is it! The session you have been waiting for!
This location is supremely cool!
Probably the total opposite of what your mother wants!
This 30 minute session at our Urban Warehouse downtown San Antonio is a FABULOUS Deal!
I love my job....LOVE LOVE LOVE it! But photographing my own family is about as challenging as it gets. Let me paint you a picture: Sunday morning 6am- I am up getting showered and ready to look as good as I can look for a family portrait. 6:45am-My kids are up getting dressed...or rather I am getting them dressed myself since they are too tired (aka lazy) to do it themselves. Get Jacob up, fed, dressed, medication. Trey can get himself ready and does a great job helping me get the kids ready too...He deserves some credit here!
Get my camera, CF cards ready, batteries charged, etc. Load up the car. I am in charge of coffee (why do I do this to myself?) so we take a detour to Starbucks to get a Traveller. Live and learn...Travellers should be called in ahead of time...15 minutes later, a Pumpkin Spice Nonfat Latte and a Traveller and we are off to Guadalupe River State Park!
I made it on time! Yay...me! Whatever happened to the cool weather we had? Humid and hot and I am sweating my rear end off (oh...I wish) layered in a sweater jacket to hide the multitude of chocolate and lack of working out that I do. My sweet friend Karrie is there to photograph this crowd...Mom and Dad...Brother/Wife/Two Grown Boys...Single Sister...Sister/Husband/Four Boys ages 4-14...Me/Trey/Three Boys with bad attitudes and One with obsessive-compulsive chewing disorder! We are a sight to see!
My mother has some trouble walking down all the rough terrain and is quite funny to see a train of people coming down the hill to get her to the water's edge.
Luckily my brother's two boys brought their sweet girlfriends who sang(if you can call it that), did power ranger kicks, climbed trees and almost anything else to get these little boys to smile. Ahhhh the fun!
To top all of this off, Jacob (with the OCD biting disorder) bites my mother right on the leg...drawing blood and a few tears. Needless to say, we are DONE!
Fun times! And luckily we have some awesome photos of the whole event, since it might be awhile until we attempt this again.
So, if you are thinking your brood is just not photo worthy, THINK AGAIN! I have seen it all and my family generally is worse than any other family I have ever photographed. Call me today to book a session that will freeze time and create a wonderful memory that you can cherish....or at least laugh about later!
It is hard to believe but it is THAT time again!
We have 4 Christmas events this year: 2 with Santa Claus and 2 without.
In addition to our brand NEW set designs we have brand NEW packages and products that will have all of your friends supremely jealous (unless you opt to let them know about us too and then they too can share in the Christmas awesomeness)!!
in your own digital frame.
some adorable little purse Brag Books.
As if that is not enough....we have NEW Christmas Card designs, Incredible Storybooks of your whole session and a fabulous special deal on a beautiful frame to go with your new Holiday Portrait Decor.
I know, I know, I know....it's just too much to handle!
So, let us help you with your selections and offer our suggestions by making a viewing and ordering appointment with one of our Portrait Design Consultants instead of viewing and choosing online.
people even think about putting up their Christmas Tree.
Whew...Check that off your list!


text:
by Dustin Wallace February 8, 2021
"Words have meaning and names have power." - Author Unknown
There is a lot in a name.
When we set out to create Seven Hills Outfitters, one of the biggest decisions was choosing the name. From a marketing and branding standpoint, you always want something that will translate to a logo, to a website address, and a variety of other things. However, we wanted our name to have meaning and power.
Find some Cincy-History-Inspired apparel by Clicking Here!
We knew that we wanted to pay homage to our hometown of Cincinnati. We knew that we wanted something that captured the aesthetic, history, and strength of the American Midwest. It was both a gift and a challenge that our native Cincinnati has so many nicknames;
The Queen City
Queen of the West
Cincy
The Nati
The City of Seven Hills
And, yes... even 'Porkopolis.'
Since we aren't looking to make bacon or chops, Porkopolis went off the list pretty early.
After hours of mockups, meetings, and mood-boards, we landed on Seven Hills, or '7H' for short.
In June 1853, the West American Review published "Article III—Cincinnati: Its Relations to the West and South" in which the seven hills of Cincinnati are described. They are as follows;
Walnut Hills
Vine Street Hill
College Hill
Fairmont (now Fairmount)
Mount Harrison (now known as Price Hill)
These hills form a crescent around the city, and are still major landmarks for Cincinnatians.
From its settlement in 1788 (originally named "Losantiville") Cincinnati positioned itself as a gateway city. It's hard to imagine now that Ohio itself was considered a western state, part of the Northwest Territory (1787-1803). But, to our young country, this was a vast and untapped land of resources and settlement opportunities.
From the Ohio River bringing steamboats to the landing, to the introduction of the canal system, railroads, and more, there has always been a sense of trade and commerce in our city. Cincinnati is a city that brings together a multitude of states, peoples, and opportunities. It is uniquely American, and distinctly midwestern.
Although the transporting of goods and services has evolved a great deal since the days of the Northwest Territory, Cincinnati is still a crown jewel in the heart of the USA for commerce.
Our goal is to bring that historic resonance of Cincinnati and the Midwest to the world of lifestyle eCommerce. We may not be unloading steamboats at the Public Landing here at 7H, but we hope to capture that same magic with our curated goods and stories.
With the name Seven Hills, we pay homage to our home. We pay homage to the people who worked the landings, the streetcars, canals, and railroads bringing trade and goods to the people of the Midwest and beyond. We pay homage to the industries, people, and organizations that put Cincinnati on the map.
We hope that every product we offer up to you would be the type of product that would make our city and history proud.
Back to Stories


text:
This Is How Sharing Works
If there's one aspect of our outdoor classroom that consistently provokes conflict, it would be our swing set. With only two regular seats and 20 or so kids, there's almost always someone waiting for a turn, or, more precisely, someone who is upset with how long the current swinger is taking to get finished.
Generally speaking, our policy about sharing is that we ask the person currently using an object, "When you're finished, I want a turn?" (although more often than not it's expressed as, "I'm next!") then let that person with possession decide for her or himself when it's time to give way, which always happens sooner or later, if only because they can't resist the "pressure" of a friend just standing there waiting for them. It's not a perfect system, prone to abuse, but I think it's better than the alternative which is for an adult to arbitrarily decide when it's time to give it up, robbing children of an opportunity to practice working things out for themselves.
We've left our tire swing up from the summer. When I paused to listen in to these two girls, I heard one of them counting while the other took a turn.
And while the swing set is where much of our turn-taking and sharing practice takes place, they are skills easily transferable to other endeavors. For instance, we had our old Fisher Price "record player" out, a wind-up device with 5 tough plastic records. A group of us were in the other room, leaving the field clear for Finn, who loves figuring things out, to master the thing. When we returned, there were suddenly a half dozen kids in his space, demanding a turn. Finn let out a howl as the other kids turned to the adults, loudly, saying things like, "He won't give us a turn!" and "He's taking too long!" Emotions were high.
I said, stating the facts as I understood them, "Finn, your friends want a turn when you're finished."
He answered, "I have to play these records first."
I asked, "Then someone else will get a turn?"
He said, "Yes," and everyone backed off a pace. Finn then methodically selected a record, placed it on the turn table, wound it up and turned it on. With the first few notes of Camptown Races, children began to call out, "Now it's my turn!"
When she'd counted to 20, they traded places, and the count to 20 began again.
"No," said Finn, taking the floor, "I have to play all the records." That's when it dawned on me that his plan was to not only play each of the 5 records, but to play each of them until they'd exhausted the wind-up. This was going to be a 15 minute proposition. I asked, "So you're going to play all of those records?"
A couple kids shouted, "That's not fair!"
I said, "It's his turn. When he's done someone else gets a turn."
As the records played, the number of children waiting dwindled, but not by much: four of them remained crowded around. With London Bridges in the air, they began to sort themselves out. Rex was standing directly behind Finn, using that to support his claim that he was next. Charlotte objected at first, but after a couple rounds, relented, stating, "Then I'm after you." She then pointed across the table at Cooper, "And you're after me," to which he agreed, although that left Ben "last," which didn't seem at all fair to him.
This was a system they worked out on their own: no obedience necessary, just agreement among peers. I said nothing, no "atta girls" necessary, because the reward, as it always is when we are left to work things out for ourselves, is built into the solution.
As Twinkle, Twinkle Little Star played, Rex took a crack at things, pointing as he spoke, "I'm first, she's second, he's third, and you're fourth." This use of ordinals was stroke of genius on Rex's part, leaving Ben feeling much better about being fourth rather than "last."
By now Finn had played 3 of his 5 records. With the turn-taking sorted out, everyone's attentions now returned to him. There were a couple grumbles of, "He's taking a long time," and "When is it going to be our turn?"
As he placed Clair de Lune on the turntable, he said, "This is the last one I'm going to play. I don't like that other one." Playing 4 records instead of 5 was his concession to the group. He then declared himself "finished" a couple notes in, vacating his chair for Rex.
Rex, Charlotte, Cooper, and Ben, their sharing plan already agreed upon, then rotated through in a matter of minutes without a hitch.
Lost In The Mat Maze
What Self-Governance Is All About
No One's Going To Give Them The Business About It....
"It's About Playing Dinosaurs!"
Even If I'm The King
What It Means To Trust Children
Out Of The Box Curricula
In This We Are Always Children
Making Ghost Water
The Responsibility From Which All Others Come
Not Anytime Soon
Without Some Grown-Up Yelling At Us
It Wasn't My Job
The Price Of A Bandaid Or Two
Educating Citizens
"Those Guys Were Really Nice To Me"
That Can Never Be Standardized
When We Finally Accept The Truth About Play
Diapers, Pee, And Bloody Poop
Releasing The Antibodies


Yesterday, police forces across the country were given the green light to stop the arrests of cannabis users.
Every police chief can now decide to stop and charge, warn or warn people caught with drugs - or just let them go.
The National Council of Chiefs of Police is the body that develops operational policies at the national level.
Drug organization spokesman Jason Harwin, deputy police chief of Cleveland, said that asking cannabis users to seek treatment rather than pursue it could prevent recidivism and provide "better results." ".
The news follows last week's West Thompson Police Chief Dave Thompson's revelation that his officers do not even give official warnings to young cannabis users because it would be "disastrous for their chances in life".
Mr. Harwin, who is NPCC's "drug officer," said: "There is every reason to believe that recommending early intervention treatment to juvenile offenders rather than obtaining convictions can prevent recidivism and the best results for both the user and the criminal justice system.
It is the responsibility of chiefs of police, in liaison with their police and their commissioners, to determine operational priorities.
Possession of a class B drug such as cannabis can result in a five-year prison sentence and an unlimited fine. The cultivation or trafficking of cannabis can theoretically lead to 14 years of imprisonment and an unlimited fine.
Harwin, whose organization includes the 43 police forces in England and Wales, said police chiefs would continue to prosecute the big drug criminals.
However, he added: "There are a series of options for treating people found in possession of cannabis or who grow the plant that are proportionate to individual circumstances - these include extrajudicial provisions and warnings about cannabis. , as well as prosecution ".
This approach has been criticized by anti-drug activists, including the National Drug Prevention Alliance.
In response to NPCC's statement, the Interior Ministry said police chiefs are supposed to enforce the law.


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text:
Ben Quayle's Potemkin Family ?
Doug Mataconis · Thursday, August 5, 2010 · 9 comments
Ben Quayle, son of former Vice-President Dan Quayle and candidate for Congress in Arizona, is taking some heat for a campaign mailer:
Arizona Republican congressional candidate Ben Quayle recently sent out two mailers with pictures of him playing with two girls who appear to be his daughters.
Only problem: Quayle, 33, and his wife Tiffany have no children.
One of the mailers shows Quayle, the son of former Vice President Dan Quayle, holding one of the girls in his right arm while facing the other girl, who is sitting at a table.
Under Quayle's name is the slogan "A New Generation," along with a quote from Quayle: "My roots in Arizona run deep. My grandparents and great grandparents lived in this district. My parents and all of my siblings live in this district. Tiffany and I live in this district and are going to raise our family here."
The second mailer focuses on Quayle's opposition to abortion rights and features a picture of the same two girls.
Neither mailer says the two girls are Quayle's daughters, but they also don't identify the children.
Honestly, I think this is much ado about nothing. Yea, the picture of Quayle with the children might lead voters to think they're his children (it turns out they are his nieces) but he doesn't say that are, and the statement "going to raise are family here." isn't really deceptive is it ?
I'm not sure where Quayle stands in the polls here, but this hardly disqualifies him.
Here's the mailer in question:
FILED UNDER: Campaign 2010, Congress, US Politics, abortion, Arizona, Dan Quayle
About Doug Mataconis
Doug Mataconis held a B.A. in Political Science from Rutgers University and J.D. from George Mason University School of Law. He joined the staff of OTB in May 2010 and contributed a staggering 16,483 posts before his retirement in January 2020. He passed far too young in July 2021.
reid says:
Thursday, 5 August 2010 at 11:16
It's PR gone out of control and I wouldn't have done it, but no, not a huge error. Running for congress with the last name Quayle, now that's an error!
I actually kind of liked his pop back in the day and was sympathetic over all of the grief he got. He didn't seem like a mean politician. I was in college and didn't pay much attention at the time, though, and I'm sure I would highly disagree with the family's stands on issues.
Franklin says:
"going to raise are family here."
If he really wrote this, he obviously got his spelling proficiency from his old man.
Also, I thought that Cheney shot Quayle, or am I getting mixed up?
DC Loser says:
Or maybe he just likes young girls?
Zelsdorf Ragshaft III says:
Some of the comments here are just plain slime nasty. Name all 57 states.
That "57 state" thing (I'm assuming a reference to Obama saying it) is absolutely stupid. Maybe even moreso than "birth certificate" stupid. A coworker brought that up at the time, implying Obama is so dumb he doesn't know how many states there are. Clearly (if you're not a frothing wingnut) he was tired and just misspoke.
http://www.snopes.com/politics/obama/57states.asp
MarkedMan says:
Substantively, this seems much ado about nothing. Probably a political error though, as it gives his opponents something negative to jeer about.
For the record, I was trying to be a bit funny with both of my comments (the "are family" one is actually just a minor copy/paste error by Doug).
And also for the record, who cares if it's his nieces rather than own daughters? It's so dumb I just had to make some jokes.
An Interested Party says:
"Some of the comments here are just plain slime nasty."
Written by a true expert/practitioner of slime and nasty, considering this loon's comments on the post about the politics of the California Gay Marriage decision…
Newt Gingrich's Breakfast At Tiffany's
What The Gosar Family Tells Us About Our Broken Political Culture
Stop Trying To Intimidate People Into Voting
Boy Scouts To Admit Girls
MILLER ON MAILER


Jennette. . HD Wallpaper and background images in the Jennette McCurdy club tagged: jennette mccurdy red carpet.
This Jennette McCurdy wallpaper might contain портрет, выстрел в голову, близком расстоянии, макро, and крупным планом.


text:
Le Persée de numéro de coque M649 est un chasseur de mines de classe Tripartite dans la Marine française. Sa ville marraine est Thonon-les-Bains.

Ses missions sont « la détection, la localisation, la classification, l'identification puis la destruction ou neutralisation des mines par fonds de 10 à 80 mètres, le guidage des convois sous menace de mines et la pénétration sous la mer, la recherche d'épaves ».

Histoire

Désarmé en 2009, après avoir été amarré dans le port de Brest, il fut déplacé en janvier 2020 au Cimetière des navires de Landévennec dans l'attente de son démantèlement.

Commandement

Il a été commandé par Frédéric Maurice

Notes et références

Voir aussi

Articles connexes
 Marine nationale (France)
 Liste des navires de la marine française
 Liste des anciens navires de la marine nationale depuis 1945

Liens externes
  Présentation du navire Persée sur le site de la marine française

Chasseur de mines de la Marine française
Nom de bateau
Bateau lancé en 1988
Navire construit à l'arsenal de Lorient


The role of the school is not only giving academic knowledge but it's also to give the great wisdom of life. The lesson of love and value of the family members is being taught to the children. The Grandparents are their true friends, they spend their happy moments with their grandpa and grandma. Grandparents play with children, give life lessons, priceless gifts and memories. To acknowledge their role in the life of children SR Capital School celebrated Grandparent's day in the school on 20th October 2018 in the school premises. The students performed in front of their grandparents. They expressed their love for them. The games for Grandparents were organized in the event. The school feels immense pleasure to see the Happiness on the face of Grandparents. It was an awesome day for the grandparents, children, teachers, and staff of the school. Their blessings are the most valuable award for the school.


Love comes in all shapes and sizes, especially on the operatic stage. This Valentine's Day, celebrate the love in your life with a playlist of some of opera's most romantic melodies, all recorded live from the Met. From Mimì and Rodolfo's rapturous love duet in Puccini's La Bohème to Dalila's sensual "Mon cœur s'ouvre à ta voix" from Saint-Saëns Samson et Dalila to Nemorino's heartrending "Una furtiva lagrima" from Donizetti's L'Elisir d'Amore, enjoy more than a dozen moving selections. Among the many favorite Met artists featured on this playlist are Plácido Domingo, Roberto Alagna, Isabel Leonard, Nathan Gunn, Sondra Radvanovsky, Javier Camarena, and Matthew Polenzani.