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Social Media Content Of The Day Mariota Picks Excel's Zucker For Marketing NHL Announces Outdoor Games, World Cup Altered Pro Bowl Kicks Off Super Bowl Week Belichick: Patriots Not To Blame For Deflategate Selig Passes Commissioner Torch To Manfred NFL To Test New Tablet-Based Replay System Chargers Deny L.A. Stadium Report "SNL" Takes Aim At Deflategate Weekend Briefs
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SBD/Closing Bell
Sources: Univ. of Texas, ESPN To Announce Plans For Cable Net
Published January 18, 2011
The Univ. of Texas and ESPN plan to announce their venture to launch a cable channel tomorrow afternoon, according to several sources. The Longhorn Network is expected to launch in the fall. The channel will carry up to two football games, as many as 10 men's basketball games, women's basketball and Olympic sports. It also will carry non-sports programming about the university. More details will be made available tomorrow, sources say. The school worked with its multimedia rights holder, IMG College, to negotiate the deal. The channel is expected to be fully owned by ESPN.


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A Reasonable Compromise On Gun Control
Most liberals want gun control. Mostly on people other than themselves, but, I'll ignore that for the moment. So, I'll tell you what, in the spirit of compromise, here's what I'll offer:
- Reinstatement of the original 1994 Assault Weapons Ban
- Ban the manufacture, sale, and transfer of magazines higher than 1o rounds starting the date the legislation passes
- Require background checks on all weapons purchased at gun shows before the purchaser takes ownership of the weapon
- Ban private ownership of all automatic weapons
- A national 7 day waiting period for the purchase of all handguns (with a provision that in certain cases, such as someone who's life is being threatened can get an immediate check and permit from law enforcement. Provided they pass the check)
In return I want
- Ban all late term abortions (except in real cases where the mother's life is in imminent danger, and the doctor must legally sign off on a specific, and legally binding, form)
- Require parental notification for abortions for all women under 18
- Require parental consent for all under 16 (which could be over-ruled by a judge)
- Disallow all federal funding for abortion, including at Planned Parenthood. Want one? Pay for it yourself
- Require a 48 waiting period from the time a woman requests an abortion
I think that's eminently fair, a nice compromise. What do you think?
Oh, and I'll tell you what: I'll also give you
- background checks on all gun purchases, including rifles and shotguns (if someone has had a background check on a purchase within the previous 2 years, they would not need to get another permit*)
And you give me
- Corporal punishment and "hard labor" for all convicted violent felons
Do we have a deal?
*For instance, here in Wake County one must go to the Sheriff's office and pay for a background check and receive a permit for each handgun permit. I have two guns, so, two permits, two checks. I got the permit, then went to get a handgun in 2008. Then did it again early in 2012. Since I received a permit last year, if I wanted to get a Bushmaster .223 there would be no need for a check or permit.
Also see...
*GASP* Imagine that! You might have to work for something! You know, kinda like the rest of us. Thousands of childless, able-bodied adults in Maine just learned that they are...
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Politico: Women Are Better Calling 911 Than Having A Gun
The Democrat War On Women continues. Politico's Roger Simon pens an opinion piece which tells women "hey, you're safer just

subset: commoncrawl


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reviews & comments (464)
A Russian New Year with friends so we splurged on the meat and got the beef tenderloin. So good. Very tender. Expensive for sure! But so worth it. I wouldn't do that for a weeknight meal! I doubled the sauce, did not double the meat. It was so delicious. We were a little short on brandy, so augmented with dark rum, did not negatively impact flavor. Used a recommendation from an earlier review and used a can of beef consommé in addition to the broth. I made the recipe as directed, but we were not ready to eat, so I waited until we were ready to eat to put the meat back into the sauce so it wouldn't overcook. In keeping to our Russian theme, I served this over red potatoes that I had cubed and boiled then pan fried in a little olive oil to brown the edges. Holds the sauce nicely. I didn't combine them, but had the potatoes in one bowl and the Stroganoff in another. We then plated them family style at the table. Would definitely make again.
I would like to preface my review by stating that my mother made this recipe as stated from the original magazine when I was a little kid, and it was absolutely delicious as is. Now that I am a poor graduate student living away from home, I made the recipe using 1/2 pound of thinly sliced flank steak for the tenderloin, doubling the mushrooms, a splash of wine for the cognac, and sour cream for the creme fraiche. Yes, I know that is a lot of substitutions, but I can say that it is just as delicious.
*Cooked in Dutch oven. Prepped only 2 lbs. of beef (top sirloin was fine). Didn't reduce stock/broth all the way, which left more juices for sauce. Added paprika when adding crème fraîche. Added 4 Tbs. butter to sauce at the end and only 2 Tbs. butter to noodles. Doubled noodles for leftovers!!
Yeah. This recipe is fantastic. I made the recipe as written with the following modifications. * Double the sauce (This is a must.) * Added 2 T flour to the shallot & mushroom mixture then browned it for 2 minutes. * Used slightly less Cognac (about 1/3 less) * Used a Dutch oven. * Used frozen beef stock from the butcher. Next time, I'll likely reduce the beef to only 2 pounds. Indeed, Beef Tenderloin is very expensive... a real treat if you can splurge. Truly a wonderful rich flavor. Dill, Dijon, Cognac all blend together for a very wide taste.
At $23 per pound, I looked for a beef substitute. Simmered browned beef loin/boneless sirloin steak with sautéed shallots and mushrooms in unsalted beef stock for 1.5 hours. Turned out super tender, albeit not filet tender. Reduced stock and followed the recipe from there (although reduced butter amount in the egg noodles). To rave reviews.
Perfectly and exquisitely filled with the authentic stroganoff tastes, a keeper! Served over buttered spaetzle, yum!
I agree this recipe is a guide not to be used verbatim. Dill and mustard would have been overpowering if I had not reserved half. Not enough liquid to make sauce, added more sour cream and some of the cooking liquid I had reserved from the noodles. The paprika is indeed a good addition, in fact I added both when I was sauteing mushrooms (by mistake because I misread recipe when it called for pepper) and again at end. Used smoked paprika. But yes I would make it again and know it will work.
I used this recipe as a guide. I had beef tenderloin left over & morels that had been sautéed in garlic & marsala in the freezer. I did have to thicken the sauce a little bit but it turned out great. Will be making it again.
We used this recipe as a guide and found it was pretty excellent. We replaced the beef with duck, the creme fraiche with coconut creamer, the beef stock with mushroom stock, and the butter with Earth Balance, which sounds like a lot of changes, BUT the recipe put us on the path to deliciousness. The paprika is a truly inspired addition to the savory sauce.
I found this recipe absolutely wonderful! It was easy to make and a delicious variation to the Beef Stroganoff I usually make. I cut the recipe in half, except for the sauce as I was cooking for two. We still had leftovers! I didn't have the cognac in hand so substituted Grand Marnier which didn't hurt the flavor one bit. The Dijon and dill gave the sauce a wonderful flavor. I used the heavy cream and the sauce was a little thin but we spooned up every drop. Great to serve crusty bread with this recipe.


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I am forget from nova scotia canada my grand parents were forget from quebec they were french I never knew them for they died when a was a child.I am looking for any forget that might be relate to me in quebec.or any history on them they were eugene and jean forget. Notify Administrator about this message?
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Publications (222)336.83 Total impact
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ABSTRACT: Using the large multiwavelength data set in the Chandra/SWIRE Survey (0.6 deg2 in the Lockman Hole), we show evidence for the existence of highly obscured (Compton-thick) AGNs, estimate a lower limit to their surface density, and characterize their multiwavelength properties. Two independent selection methods based on the X-ray and infrared spectral properties are presented. The two selected samples contain (1) five X-ray sources with hard X-ray spectra and column densities 1024 cm-2 and (2) 120 infrared sources with red and AGN-dominated infrared SEDs. We estimate a surface density of at least 25 Compton-thick AGNs deg-2 detected in the infrared in the Chandra/SWIRE field, of which ~40% show distinct AGN signatures in their optical/near-infrared SEDs, the remaining being dominated by the host galaxy emission. Only ~33% of all Compton-thick AGNs are detected in the X-rays at our depth [F(0.3-8 keV) > 10-15 ergs cm-2 s-1]. We report the discovery of two sources in our sample of Compton-thick AGNs, SWIRE J104409.95+585224.8 (z = 2.54) and SWIRE J104406.30+583954.1 (z = 2.43), which are the most luminous Compton-thick AGNs at high z currently known. The properties of these two sources are discussed in detail with an analysis of their spectra, SEDs, luminosities, and black hole masses.The Astrophysical Journal 12/2008; 642(2):673. · 6.28 Impact Factor - [Show abstract] [Hide abstract]
ABSTRACT: We report the first detection of the 205 μm 3P1 P0 [N II] line from a ground-based observatory using a direct detection spectrometer. The line was detected from the Carina star formation region using the South Pole Imaging Fabry-Perot Interferometer (SPIFI) on the Antarctic Submillimeter Telescope and Remote Observatory (AST/RO) at the South Pole. The [N II] 205 μm line strength indicates a low-density (n ~ 32 cm-3) ionized medium, similar to the low-density ionized halo previously reported in its [O III] 52 and 88 μm line emission. When compared with the Infrared Space Observatory [C II] observations of this region, we find that 27% of the [C II] line emission arises from this low-density ionized gas, but the large majority (~73%) of the observed [C II] line emission arises from the neutral interstellar medium. This result supports and underpins prior conclusions that most of the observed [C II] 158 μm line emission from Galactic and extragalactic sources arises from the warm, dense photodissociated surfaces of molecular clouds. The detection of the [N II] line demonstrates the utility of Antarctic sites for THz spectroscopy.The Astrophysical Journal 12/2008; 652(2):L125. · 6.28 Impact Factor - [Show abstract] [Hide abstract]
ABSTRACT: We present a trade study for a submillimeter direct-detection spectrometer operating at the background limit for the Cornell Caltech Atacama Telescope (CCAT). In this study we compare the classical echelle spectrometer ZEUS with the waveguide grating spectrometer Z-Spec. The science driver for this instrument is spectroscopic investigation of high redshift galaxies as their far-IR fine structure line emission is redshifted into the telluric submillimeter windows. The baseline detector consists of SQUID multiplexed TES bolometers and the ideal spectrometer to detect weak lines from distant extragalactic sources is a grating with a resolution of ~103 and a large bandwidth, covering an entire telluric submillimeter window instantaneously. Since the density of high-z sources on the sky is ~100 within a 10'×10' field of view and a redshift range of Deltaz~0.2 we also explore multi-object (~50 objects) capability, including articulated mirrors and flexible waveguide fibers.Proceedings of SPIE - The International Society for Optical Engineering 08/2008; · 0.20 Impact Factor - [Show abstract] [Hide abstract]
ABSTRACT: We propose to accurately trace molecular gas excitation and mass along the plane of the two nearby nearby edge-on spiral galaxies, NGC 4905 and 5907 through deep IRS spectroscopy of four pure rotational lines (S(3), S(2), S(1), and S(0)) of H2. Our primary goal is to investigate the physical state, mass, and heating processes in the molecular ISM in these galaxies, and compare them with our on-going study of the edge-on galaxy NGC 891. Prior modeling of the S(1) and S(0) emission from NCG 891 suggests an enormous amount of cool (T< 90K) H2 (5 to 15 times the atomic mass) for this galaxy if the ortho to para H2 ratio is 3. However, these models are hampered by the degeneracy between gas excitation and the (assumed) o/p ratio. Including the S(3) and S(2) lines in the analysis breaks the degeneracy, enabling independent determination of gas excitation for the ortho and para species, and a measure of the o/p ratio. Using three lines (S(2), S(1), and S(0)) for NGC 891, we find gas excitation near 220 K, with an o/p ratio near unity, resulting in greatly reduced molecular gas mass. We were awarded time in Cycle 4 to verify this model through deeper integrations of the S(0), S(1), and S(2) lines, and observations of the S(3) line in NGC 891. {These observations have not yet been scheduled}. Here we propose to extend our study by mapping all four lines in the disks of galaxies with different gas contents than NGC 891: the early type Sb NGC 4565 and the late type Sc NGC 5907. We are particularly intrigued with the regions outside of the CO emitting disk where the gas is likely not heated in a PDR scenario but rather by modest velocity cloud-cloud collisions in the outer galaxy. The proposed observations address the heating source as the ortho and para ratio depends on the formation temperature: a larger ratio indicates a larger formation temperature. Did H2 form in a relatively warm far-UV bathed environment near stars, or in a cold environment devoid of young stars?Spitzer Proposal. 03/2008; - [Show abstract] [Hide abstract]
ABSTRACT: We report the first detection of a mid-J isotopic CO line from an external galaxy. We detected the 13CO (6-5) line from the starburst nucleus of NGC 253. The line is suprisingly bright with an integrated intensity 7% of the 12CO (6-5) line, indicating optical depth in the 12CO line. Our LVG modeling shows that a single warm (T ~ 120 K), dense (n ~ 104 cm-3) component emits most of the 12CO and 13CO line emission from J = 2-1 through J = 7-6. The CO(1-0) line comes from an additional lower excitation envelope. About 60% of the total molecular gas mass within 70 pc of the nucleus is in the warm, dense component. We show that stellar far-UV photons or X-ray photons from a nuclear source are unlikely to be the primary sources of the gas heating. The most likely sources of heat are cosmic rays from the nuclear starburst or microturbulence within molecular clouds.EAS Publications Series 01/2008; 31:151-154. -
Article: ZEUS Detection of [CII] at z = 1.12
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ABSTRACT: We report the detection of the 158 mum [CII] line from the LIR ˜ 1014 L&sun; galaxy FSC 10026+4949 at z = 1.12. This is the first detection of [CII] from the z = 1-3 epoch of enhanced starformation. The L[CII]/LFIR ratio is 1.3 × 10-3, larger than the ratio typically seen in local ULIRGs, but similar to that measured in normal and starburst galaxies. This high ratio implies that the UV fields powering the far-infrared emission are of only modest intensity, and that FSC 10026+4949 may be undergoing a galaxy-wide starburst.EAS Publications Series 01/2008; 31:159-162. - [Show abstract] [Hide abstract]
ABSTRACT: We report the detection of 13CO J=6-->5 emission from the nucleus of the starburst galaxy NGC 253 with the redshift (z) and Early Universe Spectrometer (ZEUS), a new submillimeter grating spectrometer. This is the first extragalactic detection of the 13CO J=6-->5 transition, which traces warm, dense molecular gas. We employ a multiline LVG analysis and find ~35%-60% of the molecular interstellar medium is both warm (T~110 K) and dense (nH2~104 cm-3). We analyze the potential heat sources and conclude that ultraviolet and X-ray photons are unlikely to be energetically important. Instead, the molecular gas is most likely heated by an elevated density of cosmic rays or by the decay of supersonic turbulence through shocks. If the cosmic rays and turbulence are created by stellar feedback within the starburst, then our analysis suggests the starburst may be self-limiting.The Astrophysical Journal 01/2008; 689. · 6.28 Impact Factor - [Show abstract] [Hide abstract]
ABSTRACT: The fine structure line of [CI] at 370 μm, and the CO (7→6) rotational line at 371 μm are important coolants which can be used to probe the temperature and density of the warm gas component in regions of enhanced star formation. These lines can be used to provide key constrains on the physical properties of the warm molecular gas component and to deduce the excitation mechanism that heats the molecular gas. We have used the Cornell submillimeter spectrometer, SPIFI, on the JCMT to map the [CI] and CO (7→6) line emission from the nuclear regions of the nearby galaxies NGC 253 and M82, and from the overlap region of NGC4038/9. In both NGC 253 and NGC 4038/9 the [CI] emission appears fairly constant, while the CO (7→6) emission peaks at the nucleus and the most active star-forming region, respectively. The observations of NGC 253 suggest that the majority of the nuclear molecular gas is most likely heated by cosmic rays. The spatial distribution of the line emission in the overlap region of NGC 4038/9 is suggestive of a PDR, with a decrease in density from the most active region to the outside. In contrast, in M82 both the CO (7→6) and [CI] line intensities vary over the mapped region, with the line ratios remaining fairly constant. This suggests a change in the beam filling factor of PDRs with a higher PDR number density in the most active regions.12/2007: pages 225-230; - [Show abstract] [Hide abstract]
ABSTRACT: We discuss optical associations, spectral energy distributions (SEDs), and photometric redshifts for Spitzer Wide-Area Infrared Extragalactic (SWIRE) Survey sources in the European Large-Area ISO Survey (ELAIS) N1 area and the Lockman Validation Field (VF). The band-merged Infrared Array Camera (IRAC) (3.6, 4.5, 5.8, and 8.0 mum) and Multiband Imaging Photometer for Spitzer (24, 70, and 160 mum) data have been associated with optical UgriZ data from the Isaac Newton Telescope Wide Field Survey in ELAIS N1 and with our own optical Ugri data in Lockman-VF. Criteria for eliminating spurious infrared sources and for carrying out star-quasar-galaxy separation are discussed, and statistics of the identification rate are given. Thirty-two percent of sources in the ELAIS N1 field are found to be optically blank (to r=23.5) and 16% in Lockman-VF (to r=25). The SEDs of selected ELAIS sources in N1 detected by SWIRE, most with spectroscopic redshifts, are modeled in terms of a simple set of galaxy and quasar templates in the optical and near-infrared (NIR), and with a set of dust emission templates (cirrus, M82 starburst, Arp 220 starburst, and active galactic nucleus [AGN] dust torus) in the mid-infrared. The optical data, together with the IRAC 3.6 and 4.5 mum data, have been used to determine photometric redshifts. For galaxies with known spectroscopic redshifts, there is a notable improvement in the photometric redshift when the IRAC data are used, with a reduction in the rms scatter from 10% in (1+z) to 7%. Although further spectroscopic data are needed to confirm this result, the prospect of determining good photometric redshifts for much of the SWIRE survey, expected to yield over 2 million extragalactic objects, is excellent. Some modifications to the optical templates were required in the previously uninvestigated wavelength region 2-5 mum. The photometric redshifts are used to derive the 3.6 and 24 mum redshift distribution and to compare this with the predictions of models. For those sources with a clear mid-infrared excess, relative to the galaxy starlight model used for the optical and NIR, the mid- and far-infrared data are modeled in terms of the same dust emission templates (cirrus, M82, Arp 220, and AGN dust torus). The proportions found of each template type are cirrus, 31%; M82, 29%; Arp 220, 10%; and AGN dust tori, 29%. The distribution of the different infrared SED types in the LIR/Lopt versus LIR plane, where LIR and Lopt are the infrared and optical bolometric luminosities, respectively, is discussed. There is an interesting population of luminous cool cirrus galaxies with LIR>Lopt, implying a substantial dust optical depth. Galaxies with Arp 220-like SEDs, of which there are a surprising preponderance compared with preexisting source count models, tend to have high ratios of infrared to optical bolometric luminosity, consistent with having very high extinction. There is also a high proportion of galaxies whose mid-infrared SEDs are fitted by an AGN dust torus template (29%). Of these only 8% of these are type 1 AGNs according to the optical-NIR template fitting, whereas 25% are fitted with galaxy templates in the optical-NIR and have LIR>Lopt and so have to be type 2 AGN. The remainder have LIR<Lopt and so can be Seyfert galaxies, in which the optical AGN fails to be detected against the light of the host galaxy. The implied dust covering factor, >=75%, is much higher than that inferred for bright optically selected quasars.The Astronomical Journal 12/2007; · 4.97 Impact Factor - [Show abstract] [Hide abstract]
ABSTRACT: We present mid-infrared maps and preliminary analysis for 61 galaxies observed with the ISOCAM instrument aboard the Infrared Space Observatory. Many of the general features of galaxies observed at optical wavelengths—spiral arms, disks, rings, and bright knots of emission—are also seen in the mid-infrared, except the prominent optical bulges are absent at 6.75 and 15 μm. In addition, the maps are quite similar at 6.75 and 15 μm, except for a few cases where a central starburst leads to lower Iν(6.75 μm)/Iν(15 μm) ratios in the inner region. We also present infrared flux densities and mid-infrared sizes for these galaxies. The mid-infrared color Iν(6.75 μm)/Iν(15 μm) shows a distinct trend with the far-infrared color Iν(60 μm)/Iν(100 μm). The quiescent galaxies in our sample [Iν(60 μm)/Iν(100 μm) 0.6] show Iν(6.75 μm)/Iν(15 μm) near unity, whereas this ratio drops significantly for galaxies with higher global heating intensity levels. Azimuthally averaged surface brightness profiles indicate the extent to which the mid-infrared flux is centrally concentrated, and provide information on the radial dependence of mid-infrared colors. The galaxies are mostly well resolved in these maps: almost half of them have <10% of their flux in the central resolution element. A comparison of optical and mid-infrared isophotal profiles indicates that the flux at 4400 Å near the optical outskirts of the galaxies is approximately 8 (7) times that at 6.75 μm (15 μm), comparable to observations of the diffuse quiescent regions of the Milky Way.The Astronomical Journal 12/2007; 120(2):583. · 4.97 Impact Factor - [Show abstract] [Hide abstract]
ABSTRACT: We present the analysis of Infrared Space Observatory long-wavelength spectrometer (LWS) observations of the two nearby late-type galaxies NGC 1313 and NGC 6946. Both galaxies have been fully mapped in the [C II] far-infrared fine-structure line at 158 μm, and some regions have been observed also in the [O I] 63 μm and [N II] 122 μm lines. We use these observations to derive the physical properties of the atomic interstellar medium, to establish how they relate to other interstellar medium components (gas and dust), and to establish how they vary with different galaxy components such as nucleus, spiral arms, and disk. The [C II] line is the main cooling line of the atomic medium. In NGC 6946 and NGC 1313, its emission represents 0.8% of the infrared emission. Moreover, the [C II] emission can be spatially associated with three components: the nucleus, the star-forming regions in spiral arms, and the diffuse galaxy disk. This last component contributes 40% in NGC 6946 and ~30% in NGC 1313 to the total emission. We apply the photodissociation region (PDR) model by Kaufman et al. to derive PDR physical parameters responsible for the neutral atomic gas emission (G0, n, and Ts). The results do not significantly differ from what Malhotra et al. recently found by modeling the integrated emission of a sample of 60 normal galaxies. This suggests that the emission in each region under the LWS beam in NGC 6946 and NGC 1313 (corresponding to a linear size of ~1.5 kpc) is likely to arise from a mixture of components similar to the mixture producing the integrated emission of normal galaxies. However, some regions in NGC 6946 have a G0/n ratio ~2–3 times smaller than the mean value found for the normal galaxy sample (1.3), suggesting that the beam-averaged contribution of a less active component in these regions is higher than its contribution in the integrated emission of normal galaxies or, conversely, that the bulk of the integrated emission of the normal galaxies is dominated by a few active regions probably located in their nuclei. CO(1–0) and [C II] in NGC 6946 are well correlated, and the mean [C II]/CO ratio agrees with the mean integrated ratios of the normal galaxies sample. This value (~500) is a factor of ~2 less than the mean ratio found for a sample of normal galaxies observed with the Kupier Airborne Observatory (KAO) by Stacey et al. This difference is probably due to the fact that the KAO beam (55'') is smaller than the LWS beam (75''), such that the Stacey et al. KAO observations are likely to be more biased toward the nucleus of the galaxies and therefore toward more active regions. In NGC 1313 only four LWS regions have been observed in CO(1–0), and three of them were detected. The [C II]/CO(1–0) seems to systematically increase from the northeast to the south, along the S-shaped spiral arm, indicating that the interstellar medium conditions in NGC 1313 are much more inhomogeneous than the conditions in NGC 6946. H I and [C II] in NGC 6946 are completely uncorrelated, probably because they arise from different gas components: [C II] arises principally in dense and warm PDR and H I from diffuse (n 3 × 103 cm-3) gas. On the other hand, in NGC 1313 we successfully detect two distinct gas components: a cirrus-like component, for which H I and [C II] are weakly correlated as observed in our Galaxy, and a component associated with dense PDRs completely uncorrelated from H I as observed in NGC 6946. Finally, we find that the H I residing in dense gas surrounding the star-forming regions and presumably recently photodissociated constitutes a few percent of the total H I. In turn, this dense gas component produces most of the [C II] emission emitted by the atomic neutral medium, even if its contribution is lower in NGC 1313 than in NGC 6946. On the other hand, the [C II] emission arising from ionized gas is higher in NGC 1313 than in NGC 6946.The Astronomical Journal 12/2007; 124(2):751. · 4.97 Impact Factor - [Show abstract] [Hide abstract]
ABSTRACT: The far-infrared and submillimeter regimes harbor significant numbers of strong lines useful as diagnostics of processes in the interstellar medium, regions of intense star formation, and AGN activity. Covering a decade or more in wavelength, many of them are emitted or redshifted to wavelengths where they are obscured by atmospheric absorption, and so airborne and space-based instruments must be used. Capable, sensitive detector arrays are needed for this; we have been developing such arrays based on multiplexed superconducting bolometers. At the present level of maturity, we have fielded a submillimeter spectrometer containing around ten detectors of the requisite sensitivity. In the coming months, new instruments will demonstrate up to of order 100 bolometers (e.g., 8× 16). We are working to implement over a thousand pixels in a single detector package. One application for such large arrays is the 100 μ m-655 μ m spectrometer SAFIRE on SOFIA. Future directions will be for space-based observatories such as SAFIR.09/2007; 375:217. -
Article: Warm H2 at the Edge of NGC 891: Determining the Excitation and Mass of the Most Common Molecule
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ABSTRACT: We propose to obtain deep IRS spectra of the outer disk of the nearby edge on spiral galaxy NGC 891. Our primary goal is to investigate the physical state, mass, and heating processes in the molecular ISM through investigations of four pure rotational lines of H2. Pioneering work in the S(0) and S(1) lines with ISO indicate large quantities of warm (T ~ 120 K) molecular clouds along the disk of the galaxy ? fully half of the cold H2 component traced in CO. Furthermore, the ISO results suggest vast quantities of cool (T 12 kpc) for cool molecular gas by deep integrations in the S(1) and S(0) lines. Finally, we plan a sparse map of most of the disk to detect the S(3) line using the Short-Lo spectrometer. The S(0), S(2), and S(1) and S(3) transitions constrain the excitation of para and ortho H2 respectively, and together yield the o/p ratio. The four lines will therefore solidly establish the mass of warm and cool molecular gas in NGC 891. Are there massive quantities of cool gas in the outer disks of galaxies?Spitzer Proposal. 05/2007; -
Chapter: 158 micron [CII] imaging of NGC 891
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ABSTRACT: We have obtained large scale, 1' resolution maps of the edge-on spiral galaxy NGC 891 in the 158 micron [CII] and CO(1 - 0) lines. The [CII] distribution largely follows the optical image, but is significantly asymmetric - there is a pronounced ridge of emission to the north. The CO(1 - 0) and 2.8 cm radio continuum are similarly asymmetric suggesting that the [CII] emission arises from both the UV exposed surfaces of giant molecular clouds and from the diffuse ionized medium. For low density media, we estimate 25% of the observed [CII] emission arises from ionized gas clouds. The HI 21 cm line emission bears little resemblance to the other tracers, along the major axis. Assuming "standard" atomic cloud parameters, only 15% of the observed [CII] intensity along the plane comes from the atomic medium. The remainder (60%) of the [CII] emission is associated with dense photodissociation regions (PDRs) on the surfaces of molecular clouds. The [CII]/CO(1 - 0) line intensity ratio for these regions is similar to Galactic molecular clouds, providing an important link between the molecular clouds in NGC 891 and the Milky Way. For the outer regions (r > 4 kpc) of NGC 891, most of the [CII] emission arises from atomic clouds with Galactic parameters (T 100 K, n 30 cm-3). The enhanced [CII] to FIR continuum ratio in these outer regions is a reflection of the increased efficiency for photoelectic heating in low UV field environments. Integrated over the galaxy about 25% of the observed [CII] emission arises from atomic clouds. The [CII] emission may be marginally resolved in the z direction with our 55" beam - indicating a scale height larger than that of CO. This extraplanar [CII] may be associated with the "filaments" observed in the optical recombination lines.04/2007: pages 90-91; - [Show abstract] [Hide abstract]
ABSTRACT: We present a concept for a far-IR integral field spectrograph for SOFIA, the Cornell Mapping Spectrometer (CMS). CMS takes advantage of the next generation of large bolometer arrays to deliver moderate resolution spectroscopy in the wavelength range between 40 mum and 220 mum over a large field of view. Two separate wavelength channels with each employing six SCUBA-2-like bolometer arrays will provide 64 element spectra over a 10 × 12 spatial pixel footprint. By matching the pixel size to the beam size the field of view obtained is 190" × 160" at the important [CII] line in the long-lambda channel and 77" × 64" at the [OI] line in the short-lambda channel. The sliced image is fed into an R2 echelle spectrometer of modest resolving power (R ≈ 2000). The grating will operate in 4th order at 158 mum in the long-lambda channel and 4th order at 63 mum in the short-lambda channel. This results in nearly matching orders for other important fine-structure lines of [NII] and [OIII]. Filterwheels are placed right in front of the detector arrays to separate the orders. By subdividing the detector assemblies and appropriately placing the 3 × 1 detector sub-assemblies it is possible to observe four fine-structure lines simultaneously. CMS combines the advantages of a FIFI-LS design (instantaneous spatial and spectral coverage) with the sensitivity advantage of bolometers over photo-conductors. This will make CMS the instrument of choice for deep spectroscopic integrations of extended regions in galaxies.Proceedings of SPIE - The International Society for Optical Engineering 01/2007; · 0.20 Impact Factor - [Show abstract] [Hide abstract]
ABSTRACT: We report results of a recently-completed pre-formulation phase study of SPIRIT, a candidate NASA Origins Probe mission. SPIRIT is a spatial and spectral interferometer with an operating wavelength range 25–400 μm. SPIRIT will provide sub-arcsecond resolution images and spectra with resolution R = 3000 in a 1′ field of view to accomplish three primary scientific objectives: (1) learn how planetary systems form from protostellar disks, and how they acquire their inhomogeneous composition; (2) characterize the family of extrasolar planetary systems by imaging the structure in debris disks to understand how and where planets of different types form; and (3) learn how high-redshift galaxies formed and merged to form the present-day population of galaxies. Observations with SPIRIT will be complementary to those of the James Webb Space Telescope and the ground-based Atacama Large Millimeter Array. All three observatories could be operational contemporaneously.Advances in Space Research. 01/2007; - [Show abstract] [Hide abstract]
ABSTRACT: Understanding galaxy formation is at the foundation of extragalactic astronomy. Galaxies are thought to be assembled via mergers of small dwarf-like systems at high redshift. One of the best ways of providing observational constraints to the models is through a better understanding of local examples of these "building blocks", star forming dwarf galaxies. We have exploited the SWIRE legacy database to perform an unbiased search for extreme star forming PAH-rich dwarf galaxies. We wish to observe a complete and flux-limited 8 um selected sample of 27 PAH-rich dwarf galaxies in the ELAIS N1 field with the Infrared Spectrograph. This proposal is part of a much larger study of the PAH-rich dwarf galaxy population. However, the Spitzer observations are critical for our project as this is a mid-infrared selected sample and we need to compare the mid-infrared properties with Spitzer surveys of known galaxy type. Only Spitzer enables us to measure the PAH features; directly observe the low-J rotational molecular hydrogen lines; and the fine structure lines in a practically extinction-free wavelength range. These observations will characterize the physical properties of the star-forming regions, e.g., star formation rate, excitation, electron density, warm molecular gas mass. Please note that this is a COMPLETE SURVEY OF 27 PAH-RICH DWARVES. The SPITZER TIME request is SPLIT between this GTO proposal (SJH_PDGT), which has my total GTO time allocation of 6.6 hrs for 4 sources AND a GO proposal (SJH_PDGO) to observe the remaining 23 SOURCES in 37.9 hrs.Spitzer Proposal. 05/2006; -
Article: Probing the Activity in High-Z ULIRGs: High Resolution Spectroscopy in Neon and Argon Lines
[Show abstract] [Hide abstract]
ABSTRACT: We propose to investigate the nature of a sample of high luminosity infrared bright galaxies in the redshift range of 0.6 to 3 through complete IRS high resolution spectroscopy. Our sample focuses on systems that we will observe in March 2006 in their 158 micron [CII] line emission using Cornell's submm grating spectrometer, ZEUS on the CSO. The combined [CII] and Spitzer IRS spectroscopy will comprise the thesis work of Cornell student Steven Hailey-Dunsheath. The combined data sets will (1) Determine the hardness of the ambient interstellar radiation fields thereby tracing the most massive stars on the main sequence, or revealing the presence of an AGN. (2) Determine the total ionizing flux from stars, hence the relative importance of starformation to accretion in creating the IR luminosity of these sources. (3) Determine the strength of the ambient far-UV radiation fields, hence the physical sizes of the starforming regions. The sources proposed here are among the most distant, and most luminous sources known in the Universe. As such, they are heavily studied by many research groups. We propose deep IRS high resolution spectroscopy for these sources, for which we have built a scientific case coupled to research going on in our group at Cornell. It is clear that the spectra that we obtain will be invaluable for many other science programs including future programs involving Herschel, and JWST. We therefore welcome and encourage collaborations.Spitzer Proposal. 05/2006; - [Show abstract] [Hide abstract]
ABSTRACT: We present a first cut instrument design package for the proposed 25 meter Cornell-Caltech Atacama Telescope (CCAT). The primary science for CCAT can be achieved through wide field photometric imaging in the short submillimeter through millimeter (200 mum to 2 mm) telluric windows. We present strawman designs for two cameras: a 32,000 pixel short submillimeter (200 to 650 mum) camera using transition edge sensed bare bolometer arrays that Nyquist samples (@ 350 mum) a 5'×5' field of view (FoV), and a 45,000 pixel long wavelength camera (850 mum to 2 mm) that uses slot dipole antennae coupled bolometer arrays with wavelength dependent sampling that covers up to a 20' square FoV. These are our first light instruments. We also anticipate "borrowed" instruments such as direct detection and heterodyne detection spectrometers will be available at, or nearly at first light.Proceedings of SPIE - The International Society for Optical Engineering 01/2006; 6275. · 0.20 Impact Factor - [Show abstract] [Hide abstract]
ABSTRACT: We present an 11 arcsec resolution map of the central two parsecs of the Galaxy in the CO J =7->6 rotational transition. The CO emission shows rotation about Sgr A*, but also evidence for non-circular turbulent motion and a clumpy morphology. We combine our dataset with available CO measurements to model the physical conditions in the disk. We find that the molecular gas in the region is both warm and dense, with T~200-300 K, n_H2~50,000-70,000 cm^-3. The mass of warm molecular gas we measure in the central two parsecs is at least 2000 M_solar, about 20 times the UV-excited atomic gas mass, ruling out an UV heating scenario for the molecular material. We compare the available spectral tracers with theoretical models and conclude that molecular gas is heated with magneto-hydrodynamic shocks with v~10-20 kms and B~0.3-0.5 mG. Using the conditions derived with the CO analysis, we include the other important coolants--neutral oxygen and molecular hydrogen--to estimate the total cooling budget of the molecular material. We derive a mass to luminosity ratio of 2-3 M_solar/ L_solar, which is consistent with the total power dissipated via turbulent decay in 0.1 pc cells with v_rms~15 kms. These size and velocity scales are comparable to the observed clumping scale and the velocity dispersion. At this rate, the material near Sgr A* its dissipating its orbital energy on an orbital timescale, and cannot last for more than a few orbits. Our conclusions support a scenario in which the features near Sgr A* such as the CND and northern arm are generated by infalling clouds with low specific angular momentum. Comment: 31 pages, including 5 figures, accepted for publication in ApJThe Astrophysical Journal 01/2005; · 6.28 Impact Factor
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Paradox Interact has released a new developer diary for their upcoming grand strategy title Europa Universalis IV. The dev diary is narrated by project lead Thomas Johansson, who discusses technology research in-game. In addition, the sequel pays more attention to player choice as players can amass higher levels of tech, which grants better weapons and diplomatic ideas. Check out the developer diary in the video below. |
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13 February 2013 | By JonahFalcon
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Life Extension
By: Sara |Institute of HeartMath Fresh squash or canned pumpkin makes this a flavorful thick stew, with a Mexican flavor and a bit of spice. 1 tablespoon olive oil 1 onions, chopped 2 cloves garlic, minced 1 tablespoon chili powder 1 ½ teaspoon cumin ½ 15oz. can chopped tomatoes, canned ¾ cup pumpkin, canned, or […]
You do not have to lose your mind with advancing age. Your brain has the capacity to regenerate and grow throughout the entire human lifespan – learn how to ensure your brain's continued growth and rejuvenation. Compelling evidence shows that physical exercise helps build a brain that not only resists shrinkage, but increases cognitive abilities. We now know that exercise promotes a process known as neurogenesis, i.e. your brain's ability to adapt and grow new brain cells, regardless of your age. This article highlights a number of brain-boosting benefits of exercise.
It's easy to look at your T.V. as just another appliance in your home, one that entertains you on demand with a mere click of the remote. And yet it does emit energy – in the form of sound and light. BioAcoustic Biology is an integrative medicine which analyzes our body frequencies (which it calls frequency equivalents (TM)) and the frequencies of things that enter our bodies: foods, toxins, pathogens, and yes, whatever comes out of your T.V. So what is coming out of your T.V. besides your favorite television show or movie?
A groundbreaking new study published in Molecular Nutrition & Food Research titled, "Interspecies communication between plant and mouse gut host cells through edible plant derived exosome-like nanoparticles," reveals a new way that food components 'talk' to animal cells by regulating gene expression and conferring significant therapeutic effects. This is the first study of its kind to look at the role of exosomes, small vesicles secreted by plant and animal cells that participate in intercellular communication, in interspecies (plant-animal) communication. Exosomes are the missing link in how plants and animal cells communicate and collaborate.
Breathing is the first and last thing we do in life, but most of us take the breath for granted. Some veterans throughout the country are using their breath to overcome wartime trauma. For many, the breath gives back what years of medication alone have not been able to resolve. They are practicing an exercise called Sudarshan Kriya Yoga, also known as SKY, which releases trauma from the body and mind through a series of breathing exercises that also puts people into states of meditation.
Clearing the energy in your home and workspace makes it lighter and more positive, removing toxins and improving your overall health and well being. Just opening windows brings in fresh, positive energy. Other space clearing techniques include dowsing; smudging with herbs or incense; clearing with bells, cymbals and singing bowls; and clearing with chanting.
Holiday Heart Syndrome, coined in 1978, describes irregular heart rhythms that occur at holiday time, in healthy people after several days of heavy drinking. In some people, even modest amounts of alcohol (as little as one drink) can cause holiday heart syndrome. This is often compounded by psychological stress, overeating, too much sodium, dehydration, lack of sleep, and overdoing it on caffeine and/or marijuana.
We all have days, weeks, months and – for some – even years of feeling anxious and uncertain. It's a vague feeling you can't quite put your finger on. From the outside, people think you have it all together, but they can't see what's going on in your head. Emptiness fills your thoughts and emotions all too often, nagging at you throughout the day. You set goals but they never satisfy your ego. You always feel a day late and a buck short. The search can seem almost endless. And a question continues to spin in your mind: "Why can't I just be happy?" The good news is you don't have to live like this. There is a better way to view the world that will lead to what you seek. Having trouble seeing the goodness? Here's a list of things you have to smile about – some obvious signs you're doing just fine in life.
They heat a thin laser probe-up to 130 degrees-then insert it through a tiny hole and essentially burn the tumor. It works by heating the tissue around it to the point where it cooks, just like you're cooking a hard boiled egg. Traditional surgery requires a three-inch incision, two to four days in the hospital and one to two months of recovery. With the laser procedure – it's a three-quarter inch incision, one day in the hospital, and one to two week recovery.
Less than 1% of the population actually suffers from celiac disease – a serious autoimmune genetic illness characterized by gluten intolerance – , but many more have "gluten anxiety". This is when a wide range of symptoms are ascribed to gluten – wheat's main protein. There's no medical evidence that going gluten-free brings health benefits. But does it deliver environmentally?


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NC sheriff gets 40 new souped-up cruisers
The department bought 39 full-size Dodge Chargers and a Chevrolet Tahoe PPV for the K-9 unit
By Joe Killian
News & Record
GREENSBORO, NC — Guilford County Sheriff BJ Barnes couldn't be happier about getting a new fleet of patrol cars for his deputies.
"They run like scalded dogs," Barnes said of the 39 full-size Police Pursuit Dodge Chargers that the Guilford County commissioners have authorized him to buy to replace the department's aging fleet.
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He's an atheist and the bible tells me to.
I would use toasted marshmallows if I were you. ;)
Best Answer
Perhaps in time he will find his own way spiritually. Brace yourself though, in case what he ultimately chooses is not what you want, but it is his life to live. :)
Best Answer
You're kidding right?! None!
Best Answer
Just don't take him for granit.
Best Answer
Makes sense, though I thought the Jesus guy said "he without sin cast the first stone"..
Best Answer
Heavy metal music
Best Answer
pop rocks...
Best Answer
No it doesn't.
Best Answer
You don't understand the bible or what Jesus Christ accomplished. Don't throw scripture at me.
Best Answer
The ones you have in your head!
Best Answer
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SOURCE: TheLocal
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'Stunning' Stockholm shipwrecks wow experts
tags: shipwrecks, Stockholm, Stockholm harbour"I was stunned by how big it was," marine archaeologist Jim Hansson told The Local of the find.
Hansson was out for a stroll along Kastellholmen island with his girlfriend on Sunday, taking in some rare springtime sun, when he noticed a pattern of wooden stumps penetrating the surface.
"If it had only been one or two beams sticking up, I may not have noticed it," he said.
"But I saw immediately that it was a shipwreck. You could clearly see the bow and the stern."...
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What's On Weekly
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The Venue Reception & Box Office is open Monday to Friday 9am - 5pm. In the evenings times vary depending on events and activities. Please ring 0114 2838692 during Reception opening hours to check details.
The Venue Bar is open Friday's, Saturday's and Monday's from 7.00pm with fantastic cask and draught beer offers every week.
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The Venue has a wide range events taking place such as concerts, gigs, plays and other performing arts. We host Folk Nights and regularly hold Band Nights
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The Venue runs band nights open to all ages, experience and genre. If you fancy a gig either email email@example.com or private message The Venue in Facebook.
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Learn new skills such as cake decorating, scrap booking, jewellery making, crafts, digital photography and flower arranging. If you would like to learn how to use a computer or improve your computer skills, we run a number of leisure learning courses Other regular activities include Music and Song for pre-school children, Children's activities as well as Tai Chi, Slimming World, and Sequence Dancing, Zumba, Chairobics, Taekwondo and singing with the Waldershelf Choir.
There are regular car boot sales as well as craft fayres and food markets - Car boot pitches cost £10 and run from 9.30am-11.30am once a month on a Saturday (open to booters at 9.00am) These regularly sell out so please book in advance
Or why not come and join us for a tea/coffee & enjoy free Wi-Fi in V's Bar & The Atrium.
Forthcoming Events
Wed 28th January
Introduction to Reading Music
Introduction to Reading Music CourseStarting 21st January 7 Week course
9:30- 11:30am
Do you sing in a choir or play an instrument but struggle to read music? This course will teach you the theory and practice to help.
For any more information or to book a place please contact The Venue- 0114 243 8692
Wed 28th January
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Craft Club is held every Wednesday Afternoon at The Venue- 12:30pm- 2:30pm
We cover all different types of paper crafting including stamping, embossing, decoupage, die cutting and many other techniques. we also do mini projects, canvasses, altered art, mono printing using a gelli plate and so many more. Come along and join in.
Wed 28th January
Music and Song
Music and song- an hour of music, songs and interactive games for babies, toddlers and pre school children. Come alongFirst session is FREE then £3.50 per Child
Every Wednesday 9.30am
Thu 29th January
Family History For beginners
Family History course for beginnersStarting 15th January 7 Week course
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Learn how to trace your ancestors, create and design a family tree, find out about their jobs, careers and social history. Use websites and historical document to uncover your past.
For anymore information or to book on the course, please contact The Venue- 0114 243 8692


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Another nationwide food recall issued
FLUSHING, N.Y. — There is another nationwide recall of food. This is time, the focus is noodles.
Ten-ounce packages of Garvi Gujarat brand Tam Tam star noodles, distributed nationwide by House of Spices in Flushing, N.Y., because they may contain undeclared peanuts.
People who have an allergy to peanuts run the risk of serious or life-threatening allergic reaction if they consume this product.
No illnesses have been reported.
The flexible plastic bags containing the product are marked with UPC 7 23246 22347 6 on the back.
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Dear Dish-It, My Brother Keeps Beating Me Up (pg.2)
My brother is five years older than I am and he's using physical violence. I've told my mom a million times but she is always saying to keep out of his way. I've got loads of aches and pains from him. What should I do? Back to Article
stay close to your mom thats what helps me when my sister is being mean
are you tryna get her killed or are you tryna help her cuz right now you tryna hurt her
you really need to call 911 my brother or sister would never hit me that hard i think your brother need therapy
You dont know how strong he is so you dont know if she csn get use to it
thats what my mom tells my sis and brother when they be hitting me and dad
my brother does that but he dont hit me that hard and sometimes he know when to stop
my sister beats me up and i tell my mom and she always tells my sister "do not do that to your sister" in a soft way but she still does it.and today my sister chocked me. now i WANT TO RUN AWAY!


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Lemon Meringue Pie
Planning, patience essential ingredients for airy meringue pie
When making the filling of a meringue pie, bring ingredients to a boil. Stir constantly and briskly to avoid forming lumps.
Planning, patience essential ingredients for airy meringue pie
For a lofty and stable pompadour atop your pie, add a paste of cornstarch and water, cooked until thickened.
Planning, patience essential ingredients for airy meringue pie
A lemon meringue pie's sweet froth and tart citrus is a heavenly combo. The techniques aren't difficult, but they do ask for some organization and patience because a freshly whipped meringue needs to go on a still-warm filling to help "cook" the egg whites.
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Reader comments are listed below. Comments are currently closed and new comments are no longer being accepted.
I believe, this story, like many others, fails to address the core issues in Haryana; and fails to estimate the magnitude of the issue it tries to highlight. The situation is actually worse than is shown here.
The assumptions of the story have been quite wrong (the social norms are changing, etc). In a state where over 100 honor killings take place every year, it appears to be a bit superfluous to draw conclusions on any kind of social change.
The data set does not appear to be representative either; The Economist's India team always tries to portray a false picture of its knowledge, intelligence, and analysis of the heartlands by writing the story in little heard obscure villages, and in this manner usually overlooks much bigger existing trends in conurbations. Clearly, picking out a stand alone village and projecting all conclusions on the same appears to be amateur.
I grew up in Bhiwani only (to which the article refers); there have been bigger horror stories which could have been mentioned to ascertain the magnitude of the problem.
I agree with "abzs2k" for The Economist certainly seems to have missed the elephant in the room!
Before, it used to be girl harassed or even killed for dowry, now it will be reversed. The boy is rejected or cannot get married because he cannot pay the sum demanded by the girls side.
Nature has taken a curse and solved the dowry problem in India.
The article: "Mr Singh paid handsomely."
Reverse dowry?
The article: "Besides ushering in a new tolerance of outsiders, the bride shortage has changed social mores in other ways. Villagers say that no girl may marry into a neighbouring village until her in-laws promise to provide a girl in return"
Err..I think you missed the elephant in the room. Interfaith marriage in a village?! Maybe the old social stigmas are being slowly dismantled after all.
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The year is 2135, and the international program to seed the galaxy with human colonies has stalled as greedy, immoral powerbrokers park their starships in Earth's orbit and begin to convert them into space condos. Ellen Starke's head, rescued from the fiery crash that killed her mother, struggles to regrow a new body in time to restore her dead mother's financial empire. And Pre-Singularity AIs conspire to join the human race just as human clones, such as Mary Skarland and her sisters, want nothing more than to leave it.
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The Enchanted Cave 2
Delve into a strange cave with a seemingly endless supply of treasure, strategically choos
4.34 / 5.00 31,630 ViewsGhostbusters B.I.P.
COMPLETE edition of the interactive "choose next panel" comic
4.05 / 5.00 10,332 ViewsThe original game is by Zanzlanz. I do not own the original work of the game (the base) HOWEVER I do own the file and textures and whatnot. A bit buggy but soon to be fixed. Enjoy! (PS DIRT BUG FIXED)


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Corden: Streep raps like 50 Cent
Published 15/04/2014 | 12:17
Meryl Streep has been working on her rap skills, James Corden has revealed.
The three-time Oscar-winning actress has been learning to rap for a song in their new film, Into The Woods, and James - who previously collaborated with rapper Dizzee Rascal on World Cup song Shout - has been impressed with her lyrical dexterity.
"She's less an Eminem, more a 50 Cent type. Mainstream with an edge," he told The Sun.
James said her enunciation skills helped her rap and joked "a second career beckons".
The Iron Lady star plays The Witch in Into The Woods, Rob Marshall's big-screen adaptation of Stephen Sondheim's Broadway musical, while James portrays The Baker.
Johnny Depp, Emily Blunt and Anna Kendrick also star in the film, which is scheduled for release in December.
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Ginger E. Nicol, MD
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4444 Forest Park Ave., Suite 2600
St. Louis, MO 63108
(314) 286-1700
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Washington University School of Medicine
Department of Psychiatry
660 South Euclid Ave, Campus Box 8134
St. Louis, MO 63110
Areas of Clinical Interest
Childhood disruptive behavior and mood disorders, obesity and weight management in childhood depression,
Areas of Research Interest
Identification and prevention of cardiometabolic risk in mentally ill pediatric populations, psychopharmacology, child mental health care cost and utilization, collaborative care.
Board Certification
General Psychiatry -- Certified
Child & Adolescent Psychiatry -- Certified
Medical Education
B.A.: Journalism, University of Iowa, Iowa City, Iowa, 1998
Medical Degree: University of Iowa Carver College of Medicine, Iowa City, Iowa, 2002
Residency: General Psychiatry, Barnes-Jewish Hospital at Washington University School of Medicine, St. Louis, MO, 2005
Fellowship: Child and Adolescent Psychiatry, St. Louis Children's Hospital at Washington University School of Medicine, St. Louis, Missouri, 2007
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Selected or Recent Journal Articles
Nicol GE, Morrato EH, Johnson MC, Campagna E, Yingling MD, Pham V, Newcomer JW. Best practices: implementation of a glucose screening program based on diffusion of innovation theory methods. Psychiatr Serv. 2011 Jan;62(1):12-4.
Morrato EH, Nicol GE, Maahs D, Druss BG, Hartung DM, Valuck RJ, Campagna E, Newcomer JW. Metabolic screening in children receiving antipsychotic drug treatment. Arch Pediatr Adolesc Med. 2010 Apr;164(4):344-51.
Nicol G, Newcomer J. Review: children and adolescents with schizophrenia spectrum disorders respond to antipsychotics, but are susceptible to adverse events. Evid Based Ment Health. 2008 Aug;11(3):81.
Luby J, Tandon M, Nicol G. Three clinical cases of DSM-IV mania symptoms in preschoolers. J Child Adolesc Psychopharmacol. 2007 Apr;17(2):237-43.
For more articles and abstracts, take this off-site link to the National Library of Medicine
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MMG resident Stalley gets GQ over this smoothed out Ski Beatz instrumental.
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2 Responses to "Stalley – "Gentlemen's Quarterly" (prod. Ski Beatz)"
This song is so choice! Peep the video on youtube, it's really good as well… Can't believe this cat signed with Ross!?! Smh… If Ross lets him make this kind of music and doesn't force his goons to be featured on every other track then he might still make good music but I am not hopeful…
Stalley has a great ear for beats, but he's like insomnia personified. Like Currensy with even less personality.
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Getting Ready To Blog Again? - Part 1 Snakkkeeeeeeee
By gla55jAw 0 Comments
Interesting. It's been a lot longer since I attempted to keep a blog going than I thought.
Games, huh. Watching both Metal Gear Scanlon's lit a fire inside me. A few weeks ago, I seemed to be disgusted by Destiny. I put over 90 hours into that game and it feels like for nothing. My friends completed the raid without me, I wasted what seems like an entire week of my life leveling up in the Iron Banner. I'll go into more detail on Destiny later. Back to Metal Gear; So I have a stack of PS4 and a less than month old stack of Xbox One games to play, but I found myself jonesing to play Metal Gear Solid 4. Maybe 6 months ago I got most of the way through Snake Eater (I think I'll go back and finish that at some point); I believe I was up to The End's fight (which funny enough means I probably don't have to do anything now). I'm really rambling here...I'm in the middle of Act IV on MGS4, back on Shadow Moses. This game is just...great and fun! It's not quite as crazy as MGS2, but definitely more confusing.
I'll probably finish it by next week and plan to put some thoughts together on MGS and what I'm going to play next.
This is clearly a bunch of jumbled thoughts, but hopefully it turns into something more structured. Until then.


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KENTUCKY (8/24/13) – This week's photo of the week is by Sandra and Chris Graham.
As you can see, Sandra absolutely loves her puppy, and the puppy loves her just as much. Sandra and her husband Chris took this photo while at home in Logan County, Ky. It's a safe bet that this puppy will live a joyful and fulfilling life.
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Well, running club did not go as planned, because we had severe storms roll in Friday evening, along with two tornadoes just outside of town! Jeff and I were sitting at our local hamburger place, where we had just finished splitting a burger (and had plans to get some frozen yogurt next) when the tornado warning came on the television. Decided we'd better book it home (just a five minute drive), which was a good thing, as the torrential rains caused flooding all over! After a few hours of rain and some hail, it eased up a bit so we went in the front yard (along with most of our neighbors) to check out our drainage area, which is normally a nice grassy play area. It was flooded, and spilling out onto the street - I've never seen it this bad! Friday night - brave neighbor, going barefoot in the flood waters (I worry about creatures like snakes being them so I wore my rain boots)The town was flooding all over, so running club was called off - but this being Texas, our weather is so extreme that it stopped raining and most places dried out enough that Jeff and I were able to go out for a run on Saturday afternoon! We went to the scary statue park but stayed in the roadway, as the trails were covered with mud, silt and still had some pretty good puddles. On the schedule for Saturday was a 2 miler, which I did using 3 minute walk/1.5 minute run intervals. Pretty easy considering we've been walk/running around 3.5 miles, but I wanted to do what we would have done with the club. I give this run a big thumbs up! Paco, doing his whole body lean onto me, as usual... This week has been a bit off, and I've realized that I just have to work with it, because no matter what I plan, things are going weird. It started with Saturday morning's run being cancelled (so I worked with it to go in the afternoon), then on Monday, the temperature was below my 40 degree comfort cut-off for the pool - but I went anyway. Got there and noticed that the water level was way down - my pool buddy Nancy swam up to me and said "it's really cold" - oh, great. Not sure why so much water was missing, but they were adding more, with a nice cold hose...which was two lanes over from where I swam - and also? The heaters weren't on! I knew I wouldn't last too long, and I couldn't stand the thought of getting my face and head wet, so I worked with it by just doing kickboarding - 50 lengths. Better than nothing, right? On Tuesday, Jenny wasn't able to meet me for our run, and while I wasn't relishing the idea of running by myself, I planned on going out after I got my hair cut. Then I got a reminder email about the track workout that night, and while I don't plan on doing many of them (because I'm trying to limit my running to just 3 days a week), this worked out perfectly to get my run in with people...so I went. And I got another opportunity to work with it, as the track was closed (soccer game was being played), so we ended up going for a little run instead! Good thing I decided to be flexible, right? Today is another swimming workout, and I sure hope the pool is filled AND warm. But if it's not, I'll work with it, one way or another. |
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Chancellors, GU15
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2013 Turing Lecturer to reveal 'What teachers didn't teach me'
Learning curve: Blinkx founder and 2013 IET/BCS Turing Lecturer Suranga Chandratillake FREng
It's increasingly essential that technologists improve their understanding of non-technical skills to ensure that they progress their careers as far as they can, the founder and CSO of Internet search engine Blinkx, Suranga Chandratillake FREng, will argue in his 2013 IET/BCS Turing Lecture presentation on 18 February at Savoy Place, London.
Computer scientist Chandratillake will share the key insights that he has gained since deciding, 13 years ago, to turn his career direction away from academia to one fully-focused in the IT industry, and thereafter on the launch of his first successful company, the video and audio search website Blinkx, now established as a leading offering in a highly-competitive online environment.
Chandratillake's Turing Lecture will also reveal how he coped with the surprise realisation of how little his formal education prepared him for the challenges of starting an ambitious commercial venture in 21st century hi-tech: such as creating and marketing innovative product offerings, and growing his organisation during a period of unprecedented global market volatility.
"Given the economic and social impact that such an endeavour can have, what could be done to better equip those starting down this path today?" is one of the critical questions Chandratillake's Turing Lecture will address. He will also consider the trade-offs ambitious technologists face when deciding which route to steer their careers toward – as well as his approach to overcoming the dilemmas entrepreneurs from technology backgrounds encounter as they seek to balance the demands of 'pure' technology with commercial expediency.
Chandratillake's lecture will also pay tribute to 'Alan Turing's world', and reflect on "the incredible, pervasive influence of computers on our lives".
Following the 18 February inaugural event, his Turing Lecture will be repeated at three further venues – University of Manchester, 19 February; University of Glasgow, 20 February; Cardiff University, 21 February. The Turing Lecture 2013 will be streamed live as a webcast on IET.tv, and will be available to view later on the lecture webcast page. Audience members both online and at Savoy Place on 18 February will be able to participate in live interactive Q&A with Suranga Chandratillake as part of the lecture. This lecture is free to attend for members and non-members of the IET and BCS.
Further information (and online event registration details):
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Hudson River School painter Frederic Church's "Ruins at Baalbek," above, is among more than 100 artworks on display in the Fitchburg Art Museum's exhibit, "American Scenery: Different Views in Hudson River School Painting," running through Dec. 20. Museum hours are noon-4 p.m. Wednesdays-Fridays, 11 a.m.-5 p.m. Saturdays and Sundays. Admission is $9, seniors 62 and older $5, free for children 12 and younger. The museum also offers free admission 4-8 p.m. every first Thursday. 25 Merriam Parkway. To learn more, call (978) 345-4207 or visit www.fitchburgartmuseum.org.
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52 Inch Sterling Manor Select
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Q | Can this fan or any other Kichler ceiling fan be flush mounted? We have 8' ceilings, so a downrod would not work well for us. |
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