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Publications (311)1830.71 Total impact
Article: A low stellar obliquity for WASP-47, a compact multiplanet system with a hot Jupiter and an ultra-short period planet[Show abstract] [Hide abstract]
ABSTRACT: We have detected the Rossiter-Mclaughlin effect during a transit of WASP-47b, the only known hot Jupiter with close planetary companions. By combining our spectroscopic observations with Kepler photometry, we show that the projected stellar obliquity is $\lambda = 0^\circ \pm 24^\circ$. We can firmly exclude a retrograde orbit for WASP-47b, and rule out strongly misaligned prograde orbits. Low obliquities have also been found for most of the other compact multiplanet systems that have been investigated. The Kepler-56 system, with two close-in gas giants transiting their subgiant host star with an obliquity of at least 45$^\circ$, remains the only clear counterexample.
Article: Discovery and Validation of Kepler-452b: A 1.6-Re Super Earth Exoplanet in the Habitable Zone of a G2 Star[Show abstract] [Hide abstract]
ABSTRACT: We report on the discovery and validation of Kepler-452b, a transiting planet identified by a search through the 4 years of data collected by NASA's Kepler Mission. This possibly rocky 1.63$^{+0.23}_{-0.20}$ R$_\oplus$ planet orbits its G2 host star every 384.843$^{+0.007}_{0.012}$ days, the longest orbital period for a small (R$_p$ < 2 R$_\oplus$) transiting exoplanet to date. The likelihood that this planet has a rocky composition lies between 49% and 62%. The star has an effective temperature of 5757$\pm$85 K and a log g of 4.32$\pm$0.09. At a mean orbital separation of 1.046$^{+0.019}_{-0.015}$ AU, this small planet is well within the optimistic habitable zone of its star (recent Venus/early Mars), experiencing only 10% more flux than Earth receives from the Sun today, and slightly outside the conservative habitable zone (runaway greenhouse/maximum greenhouse). The star is slightly larger and older than the Sun, with a present radius of 1.11$^{+0.15}_{-0.09}$ R$_\odot$ and an estimated age of 6 Gyr. Thus, Kepler-452b has likely always been in the habitable zone and should remain there for another 3 Gyr.The Astronomical Journal 07/2015; 150(2). DOI:10.1088/0004-6256/150/2/56 · 4.02 Impact Factor
Article: Three Super-Earths Orbiting HD 7924[Show abstract] [Hide abstract]
ABSTRACT: We report the discovery of two super-Earth mass planets orbiting the nearby K0.5 dwarf HD 7924 which was previously known to host one small planet. The new companions have masses of 7.9 and 6.4 M$_\oplus$, and orbital periods of 15.3 and 24.5 days. We perform a joint analysis of high-precision radial velocity data from Keck/HIRES and the new Automated Planet Finder Telescope (APF) to robustly detect three total planets in the system. We refine the ephemeris of the previously known planet using five years of new Keck data and high-cadence observations over the last 1.3 years with the APF. With this new ephemeris, we show that a previous transit search for the inner-most planet would have covered 70% of the predicted ingress or egress times. Photometric data collected over the last eight years using the Automated Photometric Telescope shows no evidence for transits of any of the planets, which would be detectable if the planets transit and their compositions are hydrogen-dominated. We detect a long-period signal that we interpret as the stellar magnetic activity cycle since it is strongly correlated with the Ca II H and K activity index. We also detect two additional short-period signals that we attribute to rotationally-modulated starspots and a one month alias. The high-cadence APF data help to distinguish between the true orbital periods and aliases caused by the window function of the Keck data. The planets orbiting HD 7924 are a local example of the compact, multi-planet systems that the Kepler Mission found in great abundance.The Astrophysical Journal 04/2015; 805(2). DOI:10.1088/0004-637X/805/2/175 · 5.99 Impact Factor
Conference Paper: Which Planets Are Rocky?[Show abstract] [Hide abstract]
ABSTRACT: Among the hundreds of near-Earth-size planets found by the NASA Kepler mission (some in the habitable zone), which of them are rocky like the Earth, and which are mini-Neptunes with thick layers of gas and water? The Kepler Project is making Doppler and transit-timing measurements to determine the masses and densities of some of these planets, to assess their structure.American Association for the Advancement of Science 2014 Annual Meeting; 02/2015
Article: Erratum: "Detection of Stars Within ∼0.8″ of Kepler Objects of Interest" (2015, AJ, 149, 18)The Astronomical Journal 02/2015; 149(2):89. DOI:10.1088/0004-6256/149/2/89 · 4.02 Impact Factor
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ABSTRACT: We present an investigation of twelve candidate transiting planets from Kepler with orbital periods ranging from 34 to 207 days, selected from initial indications that they are small and potentially in the habitable zone (HZ) of their parent stars. Few of these objects are known. The expected Doppler signals are too small to confirm them by demonstrating that their masses are in the planetary regime. Here we verify their planetary nature by validating them statistically using the BLENDER technique, which simulates large numbers of false positives and compares the resulting light curves with the Kepler photometry. This analysis was supplemented with new follow-up observations (high-resolution optical and near-infrared spectroscopy, adaptive optics imaging, and speckle interferometry), as well as an analysis of the flux centroids. For eleven of them (KOI-0571.05, 1422.04, 1422.05, 2529.02, 3255.01, 3284.01, 4005.01, 4087.01, 4622.01, 4742.01, and 4745.01) we show that the likelihood they are true planets is far greater than that of a false positive, to a confidence level of 99.73% (3 sigma) or higher. For KOI-4427.01 the confidence level is about 99.2% (2.6 sigma). With our accurate characterization of the GKM host stars, the derived planetary radii range from 1.1 to 2.7 R_Earth. All twelve objects are confirmed to be in the HZ, and nine are small enough to be rocky. Excluding three of them that have been previously validated by others, our study doubles the number of known rocky planets in the HZ. KOI-3284.01 (Kepler-438b) and KOI-4742.01 (Kepler-442b) are the planets most similar to the Earth discovered to date when considering their size and incident flux jointly.The Astrophysical Journal 01/2015; 800(2). DOI:10.1088/0004-637X/800/2/99 · 5.99 Impact Factor
Article: The California Planet Survey IV: A Planet Orbiting the Giant Star HD 145934 and Updates to Seven Systems with Long-period Planets[Show abstract] [Hide abstract]
ABSTRACT: We present an update to seven stars with long-period planets or planetary candidates using new and archival radial velocities from Keck-HIRES and literature velocities from other telescopes. Our updated analysis better constrains orbital parameters for these planets, four of which are known multi-planet systems. HD 24040 b and HD 183263 c are super-Jupiters with circular orbits and periods longer than 8 yr. We present a previously unseen linear trend in the residuals of HD 66428 indicative on an additional planetary companion. We confirm that GJ 849 is a multi-planet system and find a good orbital solution for the c component: it is a $1 M_{\rm Jup}$ planet in a 15 yr orbit (the longest known for a planet orbiting an M dwarf). We update the HD 74156 double-planet system. We also announce the detection of HD 145934 b, a $2 M_{\rm Jup}$ planet in a 7.5 yr orbit around a giant star. Two of our stars, HD 187123 and HD 217107, at present host the only known examples of systems comprising a hot Jupiter and a planet with a well constrained period $> 5$ yr, and with no evidence of giant planets in between. Our enlargement and improvement of long-period planet parameters will aid future analysis of origins, diversity, and evolution of planetary systems.The Astrophysical Journal 01/2015; 800(1). DOI:10.1088/0004-637X/800/1/22 · 5.99 Impact Factor
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ABSTRACT: We present an algorithm to search for the faint spectrum of a second star mixed with the spectrum of a brighter star in high resolution spectra. We model optical stellar spectra as the sum of two input spectra drawn from a vast library of stars throughout the H-R diagram. From typical spectra having resolution of R=60,000, we are able to detect companions as faint as 1% relative to the primary star in approximately the V and R bandpasses of photometry. We are also able to find evidence for triple and quadruple systems, given that any additional companions are sufficiently bright. The precise threshold percentage depends on the SNR of the spectrum and the properties of the two stars. For cases of non-detection, we place a limit on the brightness of any potential companions. This algorithm is useful for detecting both faint orbiting companions and background stars that are angularly close to a foreground target star. The size of the entrance slit to the spectrometer, 0.87 x 3 arcsec (typically), sets the angular domain within which the second star can be detected. We analyzed Keck-HIRES spectra of 1160 California Kepler Survey objects of interest (KOI) searching for the secondary spectra, with the two goals of alerting the community to two possible host stars of the transiting planet and to dilution of the light curve. We report 63 California Kepler Survey objects of interest showing spectroscopic evidence of a secondary star.
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ABSTRACT: We study the masses and radii of 65 exoplanets smaller than 4 R ⊕ with orbital periods shorter than 100 days. We calculate the weighted mean densities of planets in bins of 0.5 R ⊕ and identify a density maximum of 7.6 g cm–3 at 1.4 R ⊕. On average, planets with radii up to R P = 1.5 R ⊕ increase in density with increasing radius. Above 1.5 R ⊕, the average planet density rapidly decreases with increasing radius, indicating that these planets have a large fraction of volatiles by volume overlying a rocky core. Including the solar system terrestrial planets with the exoplanets below 1.5 R ⊕, we find ρP = 2.43 + 3.39(R P/R ⊕) g cm–3 for R P < 1.5 R ⊕, which is consistent with rocky compositions. For 1.5 ≤ R P/R ⊕ < 4, we find M P/M ⊕ = 2.69(R P/R ⊕)0.93. The rms of planet masses to the fit between 1.5 and 4 R ⊕ is 4.3 M ⊕ with reduced χ2 = 6.2. The large scatter indicates a diversity in planet composition at a given radius. The compositional diversity can be due to planets of a given volume (as determined by their large H/He envelopes) containing rocky cores of different masses or compositions.The Astrophysical Journal Letters 12/2014; 783(1):L6. DOI:10.1088/2041-8205/783/1/L6 · 5.34 Impact Factor
Article: Characterizing the cool KOIs. VII. Refined physical properties of the transiting brown dwarf LHS 6343 C[Show abstract] [Hide abstract]
ABSTRACT: We present an updated analysis of LHS 6343, a triple system in the Kepler field which consists of a brown dwarf eclipsing one member of a widely-separated M+M binary system. By analyzing the full Kepler dataset and 34 Keck/HIRES radial velocity observations, we measure both the observed eclipse depth and Doppler semiamplitude to 0.5% precision. With Robo-AO and Palomar/PHARO adaptive optics imaging as well as TripleSpec spectroscopy, we measure a model-dependent mass for LHS 6343 C of 62.1 +/- 1.2 M_Jup and a radius of 0.783 +/- 0.011 R_Jup. We detect the secondary eclipse in the Kepler data at 3.5 sigma, measuring e cos omega = 0.0228 +/- 0.0008. We also derive a method to measure the mass and radius of a star and transiting/eclipsing companion directly, without any reliance on stellar models. The mass and radius of both objects depend only on the orbital period, stellar density, reduced semimajor axis, Doppler semiamplitude, eccentricity, and inclination. With this method, we calculate a model-independent mass and radius for LHS 6343 C to a precision of 3% and 2%, respectively.The Astrophysical Journal 11/2014; 800(2). DOI:10.1088/0004-637X/800/2/134 · 5.99 Impact Factor
Article: ExoplanetsProceedings of the National Academy of Sciences 09/2014; 111(35):12599-12600. DOI:10.1073/pnas.1409934111 · 9.67 Impact Factor
Article: Exoplanets. IntroductionProceedings of the National Academy of Sciences 09/2014; 111(35):12599-600. · 9.67 Impact Factor
Article: The NASA-UC-UH eta-earth program. IV. A low-mass planet orbiting an M dwarf 3.6 PC from earth[Show abstract] [Hide abstract]
ABSTRACT: We report the discovery of a low-mass planet orbiting Gl 15 A based on radial velocities from the Eta-Earth Survey using HIRES at Keck Observatory. Gl 15 Ab is a planet with minimum mass Msini = 5.35 $\pm$ 0.75 M$_\oplus$, orbital period P = 11.4433 $\pm$ 0.0016 days, and an orbit that is consistent with circular. We characterize the host star using a variety of techniques. Photometric observations at Fairborn Observatory show no evidence for rotational modulation of spots at the orbital period to a limit of ~0.1 mmag, thus supporting the existence of the planet. We detect a second RV signal with a period of 44 days that we attribute to rotational modulation of stellar surface features, as confirmed by optical photometry and the Ca II H & K activity indicator. Using infrared spectroscopy from Palomar-TripleSpec, we measure an M2 V spectral type and a sub-solar metallicity ([M/H] = -0.22, [Fe/H] = -0.32). We measure a stellar radius of 0.3863 $\pm$ 0.0021 R$_\odot$ based on interferometry from CHARA.The Astrophysical Journal 08/2014; 794(1). DOI:10.1088/0004-637X/794/1/51 · 5.99 Impact Factor
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ABSTRACT: We report initial results from our long term search using precision radial velocities for planetary-mass companions located within a few AU of stars younger than the Sun. Based on a sample of >150 stars, we define a floor in the radial velocity scatter, sigma_RV, as a function of the chromospheric activity level R'_{HK}. This lower bound to the jitter, which increases with increasing stellar activity, sets the minimum planet mass that could be detected. Adopting a median activity-age relationship reveals the astrophysical limits to planet masses discernable via radial velocity monitoring, as a function of stellar age. Considering solar-mass primaries having the mean jitter-activity level, when they are younger than 100 / 300 / 1000 Myr, the stochastic jitter component in radial velocity measurements restricts detectable companion masses to > 0.3 / 0.2 / 0.1 M_Jupiter. These numbers require a large number -- several tens -- of radial velocity observations taken over a time frame longer than the orbital period. Lower companion mass limits can be achieved for stars with less than the mean jitter and/or with an increased number of observations.
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ABSTRACT: A Search for Extraterrestrial Life (SETI), based on the possibility of interstellar communication via laser signals, is being designed to extend the search into the near-infrared spectral region (Wright et al, this conference). The dedicated near-infrared (900 to 1700 nm) instrument takes advantage of a new generation of avalanche photodiodes (APD), based on internal discrete amplification. These discrete APD (DAPD) detectors have a high speed response (< 1 GHz) and gain comparable to photomultiplier tubes, while also achieving significantly lower noise than previous APDs. We are investigating the use of DAPD detectors in this new astronomical instrument for a SETI search and transient source observations. We investigated experimentally the advantages of using a multiple detector device operating in parallel to remove spurious signals. We present the detector characterization and performance of the instrument in terms of false positive detection rates both theoretically and empirically through lab measurements. We discuss the required criteria that will be needed for laser light pulse detection in our experiment. These criteria are defined to optimize the trade between high detection efficiency and low false positive coincident signals, which can be produced by detector dark noise, background light, cosmic rays, and astronomical sources. We investigate experimentally how false coincidence rates depend on the number of detectors in parallel, and on the signal pulse height and width. We also look into the corresponding threshold to each of the signals to optimize the sensitivity while also reducing the false coincidence rates. Lastly, we discuss the analytical solution used to predict the probability of laser pulse detection with multiple detectors.SPIE Astronomical Telescopes + Instrumentation; 07/2014
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ABSTRACT: We are designing and constructing a new SETI (Search for Extraterrestrial Intelligence) instrument to search for direct evidence of interstellar communications via pulsed laser signals at near-infrared wavelengths. The new instrument design builds upon our past optical SETI experiences, and is the first step toward a new, more versatile and sophisticated generation of very fast optical and near-infrared pulse search devices. We present our instrumental design by giving an overview of the opto-mechanical design, detector selection and characterization, signal processing, and integration procedure. This project makes use of near-infrared (950-1650 nm) discrete amplification Avalanche Photodiodes (APD) that have greater than 1 GHz bandwidths with low noise characteristics and moderate gain (~10^4). We have investigated the use of single versus multiple detectors in our instrument (see Maire et al., this conference), and have optimized the system to have both high sensitivity and low false coincidence rates. Our design is optimized for use behind a 1m telescope and includes an optical camera for acquisition and guiding. A goal is to make our instrument relatively economical and easy to duplicate. We describe our observational setup and our initial search strategies for SETI targets, and for potential interesting compact astrophysical objects.
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ABSTRACT: The Transiting Exoplanet Survey Satellite (TESS) will search for planets transiting bright and nearby stars. TESS has been selected by NASA for launch in 2017 as an Astrophysics Explorer mission. The spacecraft will be placed into a highly elliptical 13.7-day orbit around the Earth. During its two-year mission, TESS will employ four wide-field optical CCD cameras to monitor at least 200,000 main-sequence dwarf stars with I<13 for temporary drops in brightness caused by planetary transits. Each star will be observed for an interval ranging from one month to one year, depending mainly on the star's ecliptic latitude. The longest observing intervals will be for stars near the ecliptic poles, which are the optimal locations for follow-up observations with the James Webb Space Telescope. Brightness measurements of preselected target stars will be recorded every 2 min, and full frame images will be recorded every 30 min. TESS stars will be 10-100 times brighter than those surveyed by the pioneering Kepler mission. This will make TESS planets easier to characterize with follow-up observations. TESS is expected to find more than a thousand planets smaller than Neptune, including dozens that are comparable in size to the Earth. Public data releases will occur every four months, inviting immediate community-wide efforts to study the new planets. The TESS legacy will be a catalog of the nearest and brightest stars hosting transiting planets, which will endure as highly favorable targets for detailed investigations.06/2014; 1(1). DOI:10.1117/1.JATIS.1.1.014003
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ABSTRACT: Approximately half of the extrasolar planets (exoplanets) with radii less than four Earth radii are in orbits with short periods. Despite their sheer abundance, the compositions of such planets are largely unknown. The available evidence suggests that they range in composition from small, high-density rocky planets to low-density planets consisting of rocky cores surrounded by thick hydrogen and helium gas envelopes. Here we report the metallicities (that is, the abundances of elements heavier than hydrogen and helium) of more than 400 stars hosting 600 exoplanet candidates, and find that the exoplanets can be categorized into three populations defined by statistically distinct (∼4.5σ) metallicity regions. We interpret these regions as reflecting the formation regimes of terrestrial-like planets (radii less than 1.7 Earth radii), gas dwarf planets with rocky cores and hydrogen-helium envelopes (radii between 1.7 and 3.9 Earth radii) and ice or gas giant planets (radii greater than 3.9 Earth radii). These transitions correspond well with those inferred from dynamical mass estimates, implying that host star metallicity, which is a proxy for the initial solids inventory of the protoplanetary disk, is a key ingredient regulating the structure of planetary systems.Nature 05/2014; 509(7502):593-5. DOI:10.1038/nature13254 · 41.46 Impact Factor
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ABSTRACT: Small planets, 1-4x the size of Earth, are extremely common around Sun-like stars, and surprisingly so, as they are missing in our solar system. Recent detections have yielded enough information about this class of exoplanets to begin characterizing their occurrence rates, orbits, masses, densities, and internal structures. The Kepler mission finds the smallest planets to be most common, as 26% of Sun-like stars have small, 1-2 R_e planets with orbital periods under 100 days, and 11% have 1-2 R_e planets that receive 1-4x the incident stellar flux that warms our Earth. These Earth-size planets are sprinkled uniformly with orbital distance (logarithmically) out to 0.4 AU, and probably beyond. Mass measurements for 33 transiting planets of 1-4 R_e show that the smallest of them, R < 1.5 R_e, have the density expected for rocky planets. Their densities increase with increasing radius, likely caused by gravitational compression. Including solar system planets yields a relation: rho = 2.32 + 3.19 R/R_e [g/cc]. Larger planets, in the radius range 1.5-4.0 R_e, have densities that decline with increasing radius, revealing increasing amounts of low-density material in an envelope surrounding a rocky core, befitting the appellation "mini-Neptunes." Planets of ~1.5 R_e have the highest densities, averaging near 10 g/cc. The gas giant planets occur preferentially around stars that are rich in heavy elements, while rocky planets occur around stars having a range of heavy element abundances. One explanation is that the fast formation of rocky cores in protoplanetary disks enriched in heavy elements permits the gravitational accumulation of gas before it vanishes, forming giant planets. But models of the formation of 1-4 R_e planets remain uncertain. Defining habitable zones remains difficult, without benefit of either detections of life elsewhere or an understanding of life's biochemical origins.Proceedings of the National Academy of Sciences 04/2014; 111(35). DOI:10.1073/pnas.1304197111 · 9.67 Impact Factor
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ABSTRACT: The Automated Planet Finder (APF) is a facility purpose-built for the discovery and characterization of extrasolar planets through high-cadence Doppler velocimetry of the reflex barycentric accelerations of their host stars. Located atop Mt. Hamilton, the APF facility consists of a 2.4-m telescope and its Levy spectrometer, an optical echelle spectrometer optimized for precision Doppler velocimetry. APF features a fixed format spectral range from 374 nm - 970 nm, and delivers a "Throughput" (resolution * slit width product) of 114,000 arc-seconds, with spectral resolutions up to 150,000. Overall system efficiency (fraction of photons incident on the primary mirror that are detected by the science CCD) on blaze at 560 nm in planet-hunting mode is 15%. First-light tests on the RV standard stars HD 185144 and HD 9407 demonstrate sub-meter per second precision (RMS per observation) held over a 3-month period. This paper reviews the basic features of the telescope, dome, and spectrometer, and gives a brief summary of first-light performance.Publications of the Astronomical Society of the Pacific 02/2014; 126(938). DOI:10.1086/676120 · 3.50 Impact Factor
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University of California, Berkeley
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Charles is a 21-year-old college student who is working as a governess to the Powell kids (Nicole Eggert, Josie Davis, Alexander Polinsky). His friend Buddy Lembeck (Willie Aames) also returns along with his Mom (Ellen Travolta) and the rest of the Powell family (Sondra Kearns, James T. Callahan). This is a must-own collection for every Charles in Charge fan!
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I think you are crazy and stupid to think anyone would pay this much money for this season.Published 6 months ago by Wil
I enjoyed watching this season as well as all the others. I just wished that they kept going. They only have 5 seasons. All ages can watch Charles in charge and will enjoy it.Published 19 months ago by Amazon account
I love the show and I love the Powell Family.
Scott Baio is fantastic.
I would recommend this product to any Charles in Charge fan.
THE CHARLES IN CHARGE SEASON THREE IS A GREAT ADDITION TO MY COLLECTION OF CHARLES IN CHARGE. ALSO ONE OF THE BETTER MOVIES SO FAR. THANK YOU:FRANCAIS1959.Published on October 17, 2011 by FRANCAIS1959
Does the 3rd season set contains the missing episodes from the 2nd Season set or does it contain the same 3rd season episodes they showed on the 2nd Season set?Published on May 23, 2010 by Cassie
I bought this DVD the day it came out, and I loved it. I love this show!! This season is definetly my favorite season so far. I loved every episode! Read morePublished on January 15, 2009 by Television Addict
I have given this a 5 star based on the first 2 seasons. As I recall Charles in charge only lasted 2 seasons in Australia. Before being canned. Read morePublished on January 13, 2009 by Barry Osborne
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So, you want to know why the International Space Station dumped Windows in favor of Linux? Ask NASA chief technologist Mason Peck. He's doing an Ask Me Anything thread on Reddit today, and he's down to party.
Peck's been in charge of NASA's tech decisions since January 2012. He oversees the agency's tech investments and also guides how future astronauts will use new innovations in missions to come. This means he has to work not only within the confines of government space programs; he's also working with commercial space companies and academic institutions.
Before you go asking him your questions, though, check out dude's impressive background:
His research was sponsored by NASA's Institute for Advanced Concepts, and one of his experiments currently lives aboard the International Space Station. He worked at Boeing, Honeywell, Northrop Grumman, Goodrich, Lockheed Martin, and Bell Helicopter, where he worked on the V-22 Osprey and a smaller tilt-rotor aircraft that later would become the BA609. He wrote 90 academic articles and holds 17 patents about space tech. And then he was a professor at Cornell. You know, like you do. No big.
So far on the thread, he says:
"We need to create ways to help astronauts survive exposure to galactic cosmic rays and other hazards on the trip there and back. Getting there quicker would help. So that inspires the creation of advanced propulsion capabilities, but right now there's nothing on the horizon to shorten the trip time enough so that we don't have to worry about radiation."
"I'm very excited by the prospect of citizen space, that is, individuals building their own space technology and launching it. Some incredible innovations come from the do-it-yourself or maker community, and I expect the rena"
"Right now, we're working on the technologies that will get humans to an asteroid by 2025 and on to Mars in the 2030s. Some of those technologies include propulsion and navigation, but also technologies to protect astronauts from radiation on the trip there and back. Some day, the earliest explorers of the outer solar system and beyond will be robotic spacecraft, some may be as small as smart phones."
Copyright 2013, VentureBeat


text:
What FDA news did you miss for the week of September 28th to October 2nd?
The Next Generation Drug Delivery Devices
An exciting trend in drug delivery is underway: the movement toward smaller, smarter, wirelessly connected electronic devices that allow patient-administered therapy. Inspired by the technological advancements driving the consumer electronics market, new methods for drug delivery show great promise for all stakeholders.
Systems Engineering For Complex Portable Medical Device Development
As the demand for complex, portable medical devices continues to grow, reducing risk and increasing efficiency during the development of these products should be paramount.
Wireless Dose-Compliance Monitoring In Drug-Delivery Devices
Incorporating wireless technology into medical devices is about more than just keeping up with the hottest technology trends; the benefits are real and significant, especially with regard to monitoring and encouraging dose compliance in the pharmaceutical and medical realm.
How to Maximize Efficiencies of Medical Product Development During Pilot Phases and Clinical Trials
The principal means of controlling the many variables in medical product development is to select the right supplier/partner, with the right mix of service offerings, to help guide your project.
Best Practices In Supply Chain Management: A CMO Perspective
Supply chain management has advanced rapidly over the past decade, evolving from what was once dubbed "materials management" into the essential glue that binds all aspects of a business' internal and external collaborations.
Key Considerations When Choosing A Partner For Drug Discovery
The changes in the economic landscape and pipelines over the last 10-15 years have resulted in drug developers in companies of all sizes to take a hard look at their strategy and operations.
How Califf As FDA Commissioner Could Benefit Biosimilar Market
There are still many key decisions that the FDA needs to make when it comes to biosimilars. Why should we feel optimistic that Califf is the man to make them?
Is Pharma Competitiveness Obscuring The Biosimilar Market's Potential?
There is no shortage of research reports in the pharma industry forecasting the potential success or failure of emerging therapeutic markets. However, considering the pharma industry seems to have erupted into a civil war over whether or not the market will be as successful as predicted, it is difficult to get a sense of where the market is actually headed.
Could 96 Percent FDA Drug Approval Rate Harm Biosimilar Market?
Last week, Matthew Herper of Forbes published an eye-opening article providing a closer look at FDA approvals in recent years, coming to the conclusion that the industry is facing what could be a dangerously high approval rate for new drugs. But how could high approval rates be a bad thing?
FDA Releases Long Awaited Guidance On Biosimilars Naming
After months of debate between reference product makers and generic manufacturers, the FDA released its long-awaited guidance proposing a naming strategy for biosimilars.
Could AbbVie Hurt Itself With Biosimilar Labeling Demands?
In May, the FDA changed its stance on several key points of its draft version of the "Scientific Considerations in Demonstrating Biosimilarity to a Reference Product." In accordance with these changes, any biosimilar licensed under the PHS Act § 351 (k) no longer needs to contain a statement on its label indicating that it is a biosimilar.
Single-Use Heat Transfer
The DHX from ASI is a modular heat exchanger that employs a plate and frame concept, using a single-use bag as the sterile fluid path. The bags fit tightly between five dimpled, stainless steel plates efficiently transferring heat in a counter-current flow path. The system provides efficient, sterile heat transfer that easily integrates into any new and existing process.
SPS- Insulated Pallet Shippers
SPS Pallet Shipper is designed specifically for bulk shipments of refrigerated and frozen pharmaceuticals, biological specimens and samples. Ensure the safety and quality of your most critical products with this easy-to-assemble, proven pallet shipper.
Ensuring Cold Chain Remains Cold And Control Room Temperature Remains Controlled!
Qualification testing for the newest additions to the World Courier Ground Europe suite of vehicles has just been completed at Cambridge Refrigeration Technology (CRT) and the results are looking very impressive.
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Aseptic Disconnect HFC39 Connections HFC39 aseptic disconnect couplings prevent external organisms from entering into the media flow path upon disconnection. Automatic shutoff valves close off the flow path aseptically protecting valuable sterile media while also eliminating the need for pinch clamps and tube welders. The easy-to-use thumb latch design provides a secure, leak-free connection and enables one-hand disconnects. HFC39 connections are made of polysulfone materials with silicone seals and are ADCF, meet U.S.P. Class VI requirements and can be sterilized using autoclave or gamma.
Biobanking And The Future Of Translational Medicine: Dr Gyorgy Marko-Varga Interview 2 Of 3 Dr Gyorgy Marko-Varga highlights how biobanking will be critical to realize the promise of Translational Medicine and what challenges we need to overcome quality hurdles going forward.
Advancing Translational Medicine: Dr Gyorgy Marko-Varga Interview 1 Of 3 Dr Gyorgy Marko-Varga talks about the future of Translational Medicine and the challenges in going from lab bench experiments to predicting dose in man.
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World Courier Management
World Courier is the largest, most successful specialty courier company in the world. World Courier pioneered the offering of specialty logistics services for the medical and bio-pharmaceutical communities, transporting the first human heart tissue for transplant in 1984.
Beckman Coulter Life Sciences
The integrated resources of Hach help you monitor compliance to pharmaceutical water and cleanroom facility standards. Our world-renowned instrumentation combined with our associates' expertise gives you the confidence to move towards parametric release and process peace of mind.
Bio-Rad Laboratories, Inc.
Bio-Rad Laboratories has played a leading role in the advancement of scientific discovery for over 50 years by providing a broad range of innovative products and services to the life science research and clinical diagnostic markets. Founded in 1952, Bio-Rad serves research and industry customers around the world through its global network of operations
Bioprocess Online is the leading source of technical information and thought leadership for the biotherapeutic community. If you are a bioprocess engineer, scientist, bioprocessing manager, biotechnology producer, consultant, QA/QC, project manager, director, purchaser, marketer, or if you are involved in biopharm supply chain or facilities management, you now have access to a comprehensive Web community delivering the latest updates on the business and scientific information you need to succeed in your industry. From upstream to downstream processing through bioanalysis and biomanufacturing, our goal is to provide readers with the most up-to-date information about the issues, challenges, and news they care about most.
BioProcess Online is part of the Life Science Connect media group. The vision of Life Science Leader and Life Science Connect is to help facilitate connections and foster collaborations in pharmaceutical and medical device development to find ways to get more life-saving and life-improving therapies to market. Connect, Collaborate, Contribute.
Please take a moment to join our community and discover the benefits of your free membership.
Attendees call it "an A+ show," and Pharma EXPO 2015 will deliver solutions for the entire pharma supply chain from 200 top-tier suppliers, networking opportunities with 5,000 peers and a world-class conference program from International Society for Pharmaceutical Engineering (ISPE).
1pm-2:30pm EDT, Online Training
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Vista Sol Punta Cana - All Inclusive, Punta Cana
- Free buffet breakfast and free parking
Main amenities
- 471 smoke-free guestrooms
- On a private beach
- Marina
- 4 restaurants and 3 poolside bars
- Full-service spa
- 3 outdoor pools and 2 spa tubs
- Nightclub
- Rooftop terrace
- WiFi in the lobby
- Free children's club
- Free shopping center shuttle
- 3 outdoor tennis courts
What's around
- In Bavaro Beach
- Cortecito Beach (0.4 mi / 0.7 km)
- Los Corales Beach (0.9 mi / 1.4 km)
- Palma Real Shopping Village (1.7 mi / 2.8 km)
- Cocotal Golf and Country Club (1.9 mi / 3 km)
- White Sands Golf Course (2.6 mi / 4.2 km)
The room had a horrible smell and few dead bugs that we found later in some parts of the…
Punta Cana is beautiful !!! I will NEVER stay at Vista Sol again !!! We when thru 3 rooms…
Enter dates to check prices
Hotel Info: 866-539-8117from $72
- Superior Room
- Sea View
- Comfort Room
- Double Room
- Standard Room
- Comfort Room
- Junior Suite, Ocean View- Wireless Internet Included in all areas (Golden Club)
- Pool Garden
- Family Duplex Ocean View (2 Adults & 2 Kids)
- Superior
- Sea View - Wireless Internet Included
- Standard
- Garden View
- Double Room
- Junior Suite
Also popular with travelers from the USA
At a glance
Key facts
Hotel size
- This hotel has 471 rooms
- This hotel is arranged over 4 floors
- 24-hour check-in
- Check-out time is 12:30 PM
Required at check in
- Credit card or cash deposit required
- Government-issued photo ID required
Travelling with others
- One child (12 years old and younger) stays free when occupying the parent or guardian's room, using existing bedding
- Babysitting/childcare *
- Free children's club
- No pets or service animals allowed
- WiFi and wired Internet access in public areas *
- WiFi in rooms *
- Free self parking
- Accessible parking
- Area shuttle *
- Free shopping center shuttle
Other information
- Smoke-free property
- All-inclusive (taxes included)
- Resort fee included
Nearby Four Star Punta Cana hotels
In the hotel
- Children's club (free)
- Supervised childcare/activities (free)
- Free buffet breakfast daily
- 4 restaurants
- 8 bars/lounges
- 3 poolside bars
- Coffee shop/café
- Beach bar
- Swim-up bar
- Free reception
- Coffee/tea in the lobby
- On private beach
- Beach sun loungers
- Number of outdoor pools - 3
- Children's pool
- Fitness facilities
- Outdoor tennis courts 3
- Full-service spa
- Spa treatment room(s)
- Nightclub
- Marina on site
- Beach towels
- Swim-up bar
- Number of spa tubs - 2
- Pool sun loungers
- Sauna
- Arcade/game room
- Business center
- Computer station
- 24-hour front desk
- Tours/ticket assistance
- Dry cleaning/laundry service
- Laundry facilities
- Hair salon
- Wedding services
- Number of buildings/towers - 10
- Elevator/lift
- ATM/banking
- Safe-deposit box at front desk
- Rooftop terrace
- Garden
- Terrace
- Disabled parking
- Accessible path of travel
- Braille or raised signage
- Accessible bathroom
- In-room accessibility
- Roll-in shower
In the room
- Air conditioning
- Blackout drapes/curtains
- Premium bedding
- Balcony
- Private bathroom
- Shower/tub combination
- Free toiletries
- Hair dryer
- Premium TV channels
- Phone
- Refrigerator
- Free bottled water
- Daily housekeeping
- In-room safe
Top Punta Cana hotels
Recently reviewed hotels in Punta Cana
- The MT HotelFrom
"The hotel was very nice more then had expected, but the breakfast is terrible so we went out to eat. Would go back if need be."Sep 2, 2015
- Hard Rock Hotel & Casino Punta Cana All InclusiveFrom
"The resort was beautiful. However, the resort needs to improve its entertainment and food as the food in six of the nine restaurants was inedible. Room service and food were…"Sep 2, 2015
- Riu Palace Macao – Adults Only All InclusiveFrom
"Dual Balcony with very large Jaquzzi on one balcony. All Inclusive, best service we have had in Punta Cana so far. Room service free with huge plates of bacon, amazing. Great…"Sep 1, 2015
- Grand Bahia Principe TurquesaFrom
"Hotel is personnel very serviceable; happy faces and well responding our questions and services solicitude a."Sep 1, 2015
Nearby hotels
Special features
All inclusive
This resort is all-inclusive. Onsite food and beverages are included in the room price (some restrictions may apply).
Gratuities and taxes
Taxes are included.
Food and beverages
- All buffet and à la carte meals, snacks, and local beverages included
- Meals and beverages at companion properties
Activities and facilities/equipment
All non-motorized water sports are included.
Land activities
- Fitness facilities
- Miniature golf
- Soccer
- Tennis
- Tennis lessons
- Volleyball
- Aerobics
- Dancing
- Pilates
- Onsite entertainment and activities
- Access to onsite clubs
- Onsite live performances
- Theme parties
Not included
- Use of golf equipment
- Motorized water sports
- Scuba-diving excursions
- Scuba-diving lessons
- Snorkeling excursions
- Snorkeling gear
- Premium and/or non-domestic beverages
- Bottled wine
- Bottled liquor
- Room service
- Airport transfers
- Childcare
- Laundry/dry cleaning services
- Spa/beauty facilities and services
- Offsite tours
- Transportation to offsite activities
- Gratuities
Harmony and Esthetic has 4 treatment rooms including rooms for couples and outdoor treatment areas. Massages are available on the beach and in the spa; other services include deep-tissue massages, hot stone massages, and sports massages. A variety of treatment therapies are provided, including aromatherapy, hydrotherapy, and reflexology. The spa is equipped with a mud bath and a spa tub.
The spa is open daily. Children under 12 years old are not allowed in the spa without adult supervision. Guests under 6 years old are not allowed in the spa.
DiningRestaurante Buffet - Overlooking the pool and garden, this buffet restaurant specializes in international cuisine and serves breakfast, lunch, dinner, and light fare. A children's menu is available.
Restaurante Almirante - This fine-dining restaurant specializes in international cuisine and serves dinner only. Reservations are required.
Restaurante Mexicano - This beach theme restaurant specializes in Mexican cuisine and serves dinner only. Reservations are required.
Restaurante Italiano - This beachfront theme restaurant specializes in Italian cuisine and serves dinner only. Reservations are required.
Snack Bar - This beachfront buffet restaurant specializes in international cuisine and serves lunch and light fare. A children's menu is available.
Vista Sol Punta Cana - All Inclusive, Punta Cana's small print
Also known as
- All Inclusive Vista Sol Punta Cana
- Punta Cana Vista Sol
- Sol Punta Cana
- Sol Vista Punta Cana
- Vista Punta Cana
- Vista Sol
- Vista Sol All Inclusive
- Vista Sol Punta Cana
- Vista Sol Punta Cana All Inclusive
Children under 12 years old are not allowed in the spa without adult supervision.
Guests under 6 years old are not allowed in the spa.
For transfers, guests must contact the property before arrival at the number on the booking confirmation.
Reservations are required for massage services and spa treatments and can be made by contacting the property before arrival at the number on the booking confirmation.
Mandatory fees
The charges below are included in the total price displayed:
- Resort fee
Optional extras
Late check-out can be arranged for an extra charge of USD 30
Babysitting/childcare is available for an extra charge
WiFi is available in guestrooms for USD 10 per day (rates may vary)
WiFi is available in public areas for USD 5 per night (rates may vary)
High-speed Internet access (wired) is available in public areas for USD 10 per day (rates may vary)
Area shuttle service is offered for an extra charge
We have included all charges provided to us by this hotel. However, charges can vary, for example, based on length of stay or the room you book.


text:
Endorsed By
Fibromyalgia claims
Fibromyalgia is a debilitating chronic pain condition which leaves sufferers in near constant pain or discomfort. Pain can be felt all over the body, from the neck to lower back and knees. Other common complaints from fibromyalgia sufferers include chronic fatigue, mood swings, bowel and bladder issues, numbness and cognitive dysfunction.
The onset of fibromyalgia can occur as the result of a forced trauma, such as a car accident. If you believe that your situation means you could be entitled to make a claim for fibromyalgia then call our specialist team on 0800 054 6570 or fill in our online contact form to get the ball rolling.
Our team will also be able to advise you on any other costs you might be able to claim through us, ensuring you get every penny of the compensation you are entitled to.
Some of our previous cases
Fibromyalgia Arising from a Car Accident - £290,000
What could my claim cover?
Anyone who has ever suffered an injury or illness which was incapacitating will know just how much it can impact day to day life. Making a claim for your suffering from fibromyalgia as a result of an accident that wasn't your fault can include losses such as:
- Loss of earnings
- Medical costs including prescriptions
- Any lifestyle change costs which you have had to absorb, i.e. If you are taking the bus instead of walking due to constant pain
We specialise in fibromyalgia claims and all other kinds of negligence and personal injury work and will do our very best to get you the compensation you deserve. We offer clients a no win, no fee service, which also means that you are at no financial risk if you do choose to make a claim with us.
Contact our experts today
For simple jargon-free legal advice from knowledgeable and experienced fibromyalgia experts call JMW Solicitors today on free phone 0800 054 6570. Alternatively, use the contact form on this page and a specialist will get back to you as soon as possible.
6 Things Every Parent Should Know About Making a Child Brain Injury Claim
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The team are big into the bag pack! @cbituk #fundraising #asdahulme http://t.co/BRiXyJTsmr


text:
For over three decades, Data Display has been setting standards for the design and manufacture of high-quality electronic LED displays. Standard LED displays have a wide range of applications for the commercial sector including cinema, retail, schools and colleges or city applications. Our high-end electronic information display systems are supplied to many market sectors, such as Railway, Bus / Tram, Urban Signage, Roadside and Airport applications. We provide an end-to-end LED display solution, from concept through to completion, incorporating in-house design and development as well as manufacturing and system testing through to commissioning and after-sales support.
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Daktronics Partners with SBB to bring light to railway stations across Switzerland
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London Underground installs new first-class LED signs at Oxford Circus supplied by Data Display-Daktronics
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text:
Posted on 18 July 2014
- 09:00
Recognised as one of the most significant people in the Club's history, 2014 marks the 10th anniversary of Bill's passing. The kits reference one of Bill's most famous quotes - 'It is better to fail aiming high than to succeed aiming low. And we of Spurs have set our sights very high, so high in fact that even failure will have in it an echo of glory.' This 'Echo of Glory' inspiration pays tribute to Bill's achievements and significant contribution to the Club.
The home kit is a traditional lilywhite shirt set off by a navy blue horizontal stripe running across the chest. A jacquard runs across the shoulders which includes the words 'Echo of Glory' taken from Bill's quote together with a pattern inspired by the famous gates which lead up to White Hart Lane on Bill Nicholson Way. Yellow taping on the sleeve cuff and collar adds an additional colour flash to set off solid navy blue shorts and white socks.
In the away kit, a yellow highlight is more visible down the front of the black shirt, with 11 stripes signifying the number of trophies won during Bill's reign. Yellow taping is also replicated along the sides of the accompanying black shorts and socks.
To explore our new home and away kits, click here...
The kits are available to purchase today at Spurs shops and online here...
17 July 2015
Following the May launch of our new Under Armour Home Kit for the 2015-16 campaign, we have today launched our new Away Kit for the upcoming season.
10 July 2015
The hard work has started as Tottenham Hotspur Ladies look to build on their best-ever season.
15 May 2015
Today marks the launch of our new Home Kit for the 2015-16 campaign.
View mobile site
© Tottenham Hotspur Ltd 2015. All rights reserved.
All photography copyright Getty Images (unless otherwise stated)


text:
Seiko Brass Floating Dial Table ClockItem # HN-SKO062
- Gold-tone solid brass case
- Dial suspended in glass
- Convenient alarm
- One "AA" battery included
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Reviewed by 3 customers
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- Attractive Design
- Clear Display
- Keeps Good Time
- Reliable
Best Uses
- Bedroom
- Desk
- Gifts
Comments about Seiko Brass Floating Dial Table Clock:
Nice change from the usual bulky clock radio. I don't need that blaring light in my face now that I am retired. It is nicely weighted so the cat doesn't knock it off the table! Beautiful piece!
- Primary use:
- Personal
Best Uses
Comments about Seiko Brass Floating Dial Table Clock:
Since this is to be a wedding gift, I did nothing more than remove it from its box to see that it hadn't been broken in transit. What a beautiful clock! I may just have to order one for myself.
I'm new to your website but will continue to review it on a regular basis. It's very easy to navigate and your offerings are first rate.
Mrs. DCSmith
- Primary use:
- Personal
- Attractive Design
- Heavy Base
- Keeps Good Time
- Reliable
- None
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- Sewing room
Comments about Seiko Brass Floating Dial Table Clock:
This is the perfect clock, a solid heavy base.
I have no wall space. And it's easy to read.
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Quality Inn Buellton
No prices found through our partners. Please contact the business directly or check some of our recommended alternatives.
How has this hotel rated in the past?
- Continental Breakfast
- Free High-Speed Internet
- Wheelchair accessibility
- Kitchenette
- Free parking
- Pets allowed
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... the dodgy navigation cord to plug in and work. What do you know...it broke again. The micro-USB plug that connects into the actual device broke off. Thankfully though, dad is very handy and between the 2 dodgy cords and use of a bobby pin and a plastic knife as a screwdriver, he was able to make 1 good cord and we were in business! 3 lessons learnt here; - always check your navigation system before leaving the rental car depot - don't hire with Avis. Not only were ...
A Day at the Reagan Presidential Library
... worth it. We then headed over to Mike's office and shop for a tour. I was quite impressed with what he has so far and all that he has built up. He has come a long way from those days some 30+ years ago when he first headed to California in a broken down old pickup. Afterwards we met up with Tom for some dinner and then back to Mike's. All in all, a good day. Tomorrow we are off to Santa ...
Bit of catching up to do...
... as the humped backs had moved south from yesterday. We headed off in search on the Condor Express. After just a few minutes, we were surrounded by hundreds of common dolphins, all eager to keep up with and to race the boat! After less than half an hour later, we were rewarded with our first humped back whales, a mother and calf. We followed them for quite some time, and then, without warning, and very close to the boat, we were ...
Santa Barbara
During our breakfast on the beach, we could see the water line from last nite's high tide and realized how close the water was to our tent (approximately 8 feet). The ocean sounds were loud but very lulling to sleep to.
We drove northwest to Santa Barbara, parked (after a quick map pick up in the tourist information center) and began to walk parts of the historic downtown. First stop the courthouse building ...
Isla Vista Santa Barbara
... Friday so we ditched all the tourist stuff to find some party's for the night. In Isla Visa the student housing and Party Island of the west coast we found a big fraternity who where playing drinking games in their Front-yard. We bought some beer and joined them. They thought us a cool drinking game called beer dice which ...


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Rockfax Description22m. A little devious but with excellent, varied and exposed climbing. Head up the awkward left-leaning groove, then move left and climb Grad's Groove until holds lead out right. Climb the crack and continuation flake to a small ledge, then move delicately right into Y Climb to finish. The Direct Version is a good HVS 5b. © ROCKFAX
UKC Logbook DescriptionThe lower crack can be climbed direct (avoiding Grad's Groove) and a delicate direct finish up the arête is recommended (avoiding Y Climb).
Ticklists: Revenge List.
08nbrierley - Lead O/S - 06/Aug/15 with jamie
Hidden - 2nd O/S - 06/Aug/15
Harder than any other HVS and most of the E1s I've led! Feet both popped off while moving through the overhang and surprisingly my hand jam stayed in leaving me hanging, got on with it after that! 3 sections of solid 5a climbing with ledges in between and reasonable gear, spent ages stood on the ledges trying to figure out how to do the next bits! Apparently I can jam when required though!spenser - Lead O/S - 22/Jul/15 with Mike NMC, Sarah Follmann
Smith42 - Lead O/S - 16/Jun/15 with kerry
Hidden - 2nd - 16/Jun/15
Adamski1986 - 2nd - 03/Jun/15 with Tim Rodgers
Tim Rodgers - Lead - 03/Jun/15 with Adam Gregg
foostu4 - Lead O/S - 26/May/15
fatbuoybazza - Lead O/S - 01/May/15 with TimG
Hidden - 2nd O/S - 01/May/15
smithjmw46 - Lead O/S - 20/Apr/15 with James Gossan
dakidunn - 2nd - 27/Aug/14 with Tris
dakidunn - 2nd - 20/Aug/14 with Tris
Direct this time. Strenuous lower crack and delicate finish. Very worthwhile.Topsy Turvy - Lead O/S - 20/Aug/14 with dakidunn
Beautiful but tough williap - Lead O/S - Aug/14
Gabe Oliver - Lead O/S - 20/Jun/14
Adamski1986 - 2nd - 19/Jun/14 with Gabe Oliver
IanHope - TR - 17/May/14 with John Haxton, matt
K Wall - Lead - 17/May/14 with Martin
Matt Poole - 2nd O/S - 17/May/14 with John84
chris smith - 2nd O/S - 06/May/14 with Malcolm watson
Adrianw - Lead O/S - 08/Sep/13 with John Wilson
Nice route, if the line was straightened out it might just make E1.Tommy Moore - 2nd O/S - 13/Jul/13 with The Mole
fun, rather greasy on a warm dayCraig Holden - Lead O/S - 09/Jul/13 with Robbie
What a Fantastic Climb, Get On It Now!!!
Did take a fall, because super greasy after some drizzle and got hands mixed up making holds slightly negative. lots of gear tho!peter.ravenscroft27 - Lead dog - 30/Jun/13 with Matt Gatley
Gatley - 2nd - 30/Jun/13
elyben - 2nd - 29/Jun/13
slippery when wetcolin milton - 2nd dog - 27/Jun/13 with shaun l
Richard Alderton - 2nd - 10/Aug/12 with Liam
Dervey - Lead - 10/Aug/12 with Rich
Went direct (twice) at 5b. Excellent.Richard Alderton - 2nd - 18/Jun/12 with Al
David Cowley - 2nd O/S - 12/Jun/12 with Chris Smith
chris smith - Lead O/S - 12/Jun/12 with david cowley
ushi - Lead O/S - 05/Jun/12 with Andy Marshall
smollett - Lead - 25/May/12 with paul
ed.burton - 2nd dog - 12/May/12 with Henry H�kkinen
Hidden - Lead O/S - 12/May/12
Dervey - 2012
y2keable - 2nd O/S - 23/Aug/11 with John
KevB - 2nd - 03/Aug/11 with Tony P
Hidden - Lead O/S - 30/Jul/11
Direct route, tricky for HVSmarkfairbank - Lead O/S - 30/Jul/11 with Sandra Lee, Ray Sharples
Pohil - Lead - 04/Jun/11
davewsargent - 2nd - 21/May/11
jshields - Lead - 21/May/11 with Dave Sargent, Ed James
Hidden - Lead - 21/May/11
Brilliant, sustained and varied. Should have hand-traversed right instead of trying to mantle onto the ledge near the top. Got stuck with my leg thrown over the left-hand bit of the ledge and had to weight the rope to :o(graphiclunarkid - 2nd dog - 30/Apr/11 with Huw
mikecollins - Lead O/S - 21/Aug/10 with stg
Hidden - Lead O/S - 30/Jul/10
Em66 - 2nd - 30/Jul/10 with Jack uni
Hidden - 2nd - 07/Jul/10
Some nice moves on this route. Took a big fall after some poor decision making. I've left a nut stuck at the start of the traverse round the arete I'm afraid.jonny taylor - Lead dog - 29/Jun/10 with Andy B
ablackett - 2nd dog - 29/Jun/10 with Jonny
Quite hard traversing after the crack near the top, maybe I did it wrong.David Bulley - Lead O/S - 26/Jun/10 with Andy Chisholm
Hidden - Lead O/S - 24/Apr/10
Hidden - Lead dog - 01/Oct/09
Have to say I wasn't that impressed by this climb. It had some nice moves on it, but the wandering line means it doesn't deserve more than one star, in my view.PeteH - Lead O/S - 22/Aug/09 with Naomi Hart
NaomiHart - 2nd O/S - 22/Aug/09 with Peter Hart
andyhutch77 - Lead - 04/Jul/09 with Marc Tomlinson
Fantastic varied climbing on a long pitch with 3 star moves up every section. Brilliant.odox - 2nd O/S - 24/Jun/09 with Tom Pitchforth
petegunn - 2nd - 21/Jun/09 with Davina & Steve
stimpey - Lead O/S - 21/Jun/09 with Pete, Davina
Sylvi - 2nd - 21/Jun/09 with Rog
Hidden - 2nd O/S - 21/Jun/09
robinsi197 - Lead O/S - 03/Jun/09 with Nick
oliwarlow - 2nd - 31/May/09 with Polly
7om - Lead O/S - Sep/08 with Chris Morish
Fell on the steep hand jamming crack, powered through the crack. Got established on the flake then fell again. Finally finished, Awesome route. Can't wait to go back and lead it clean.Daniel Sutherland - Lead dog - 23/Aug/08 with Chris
JonathanJones - 2nd O/S - 15/Jul/08 with Curly Chris
Chriswallis2 - Lead O/S - 15/Jul/08 with Anna
thomaspassmore - Lead O/S - 03/Nov/07 with Dave Jones
Claire S-J - 2nd - Nov/07
Hidden - 2nd - 20/Oct/07
Hidden - Lead O/S - 22/Sep/07
Matt crawford - 2nd - 22/Sep/07 with Taba
Hidden - Lead O/S - 2007
nic42 - 2nd - 17/Aug/06 with dru
dj_brigham05 - Lead dog - 25/Jul/06 with Chris Thain
Hidden - 2nd - 24/Jul/06
chris2451 - 2nd O/S - Jul/06 with David Brigham
Superb. Disappointed to make the moves into and up the crack then blow (repeatedly) the mantel at the top.Sankey - 2nd dog - Sep/05 with Luke
Andy Graham - Lead O/S - 2005 with Steve Anderson
GPN - 2nd - Jun/04 with Jamie Moss
gripped01 - 2nd O/S - Jul/02 with Martin Bohl
Steve Crowe - Lead O/S - 28/Jun/86
Gary Coggon - 2nd - 26/May/85 with Mike Block
Hidden - 1980
MikeDowsett - Lead - 1979 with Andy Lynch
Paula Hamilton-Gibson - 1973
granitbahn - AltLd - 1970
RichardMc - 2nd - 22/Oct/67 with Ian Stromberg
Users with this climb on their wishlist are:
blue_sundown, sarah hawker, Matt_Hardy, Matt Poole, Ian Jones


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How Much Money Would You Make If You Bought Apple Stock Rather Than Their Products?
Kyle Conroy is going to have a lot of Apple customers experiencing buyer's remorse, because he's done some homework and figured out how much money one could make if they had invested in Apple stock instead of their fancy products. »


text:
Capital Markets
Company Overview of X-Clearing Corporation
Company Overview
X-Clearing Corporation, a transfer agent, provides issuer solutions to public companies. It offers various issuer solutions, including online access, dividend processing and handling, DRP/plan administration, trustee services, and transfer and record keeping, as well as bond, dividend, and ESPP / DRPP facilities. The company's online issuer access allows public companies to tally proxy votes, view transfer activity, and export shareholder data for their own use. X-Clearing is based in Denver, Colorado.
535 Sixteenth Street Mall
Suite 810
Denver, CO 80202
United States
Key Executives for X-Clearing Corporation
X-Clearing Corporation does not have any Key Executives recorded.
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PortAventura Hotel Gold River, Vila-seca de Solcina
- Free WiFi and free parking
Direct theme park access
Located on Spain's Costa Daurada, PortAventura Gold River has direct access to the Wild West-themed area of PortAventura, one of Europe's largest theme parks. The hotel is just 10 minutes drive from the nearby Reus airport, and only an hour from Barcelona by direct train.
Unlimited theme park fun
Unlimited access to the PortAventura theme park is included for all registered guests, as well as a complimentary theme park shuttle. The 3 outdoor pools and discounted entry to the Costa Caribe Aquatic Park will keep the kids cool in summer. Guests have access to the spa area (spa tub, indoor heated pool in Hotel Caribe, sauna, steam bath) and fitness center at PortAventura Hotel Caribe and Hotel PortAventura; surcharge applies. Golfers also enjoy reduced green fees at a nearby resort's 3 greens.
Relive the Wild West
Recreating the spirit of the 19th century town of Sullivan, the resort invites you to lose yourself in the golden age of the Wild West! When it's time to recharge, the Victorian-style Grand Opera restaurant offers à la carte dining, and the Gold River Saloon is the perfect place to soak up the frontier vibe.
Breakfast included
Standard rooms are located in the majestic City Hall building. For a real adventure, line up a Wild West-era wooden log cabin, or book a deluxe room in the exclusive Victorian Lucy's Mansion, with its own private pool and restaurant. All rooms have free WiFi, and guests love the generous buffet breakfasts.
Main amenities
- 502 guestrooms
- Near the beach
- 2 restaurants
- 4 outdoor pools
- Water park
- Rooftop terrace
- Internet in the lobby
- Free theme park shuttle
- 4 meeting rooms
- 24-hour front desk
- Air conditioning
- Garden
What's around
- Port Aventura Theme Park (1.1 mi / 1.7 km)
- Levante Beach (1.9 mi / 3 km)
- Capellans Beach (2.1 mi / 3.4 km)
- Ponent Beach (2.5 mi / 4.1 km)
- Port Aventura Golf Course (2.7 mi / 4.4 km)
The hotel room is good and comfortable but the cleaning is not so good The staff is ok…
Great room, clean and comfortable. Staff was helpful. Our room had 2 double beds big…
Enter dates to check prices
Hotel Info: 866-539-8117from $143
- Suite Save 50%
- Deluxe Superior Room Lucy (Theme Park access included)
- Standard Room (Theme Park access included)
- Standard Double Room (Theme Park access included)
- Standard double max. 4 people Save 50%
- Standard double max. 4 people, Special Offer
- Superior Room (Theme Park access included)
- Deluxe Callaghan Room (Theme Park access included)
- Deluxe Room (Callaghan, Theme Park access included)
- Standard Double Room (Theme Park access included)
- Standard double max. 2 people Save 50%
- Standard Room (Gran Hotel,Theme Park access included)
- Standard double max. 2 people, Special Offer
- Superior Room (Theme Park access included)
- Cabin (4 people, Theme Park access included)
- Suite Special Offer
- Standard Room (Theme Park access included)
- Cabin (2 people, Theme Park access included)
- Standard Room ( Theme Park access included)
Also popular with travelers from the USA
At a glance
Key facts
Hotel size
- This hotel has 502 rooms
- Check-in time 3 PM-midnight
- Check-out time is 11 AM
Required at check in
- Credit card or cash deposit required
- Government-issued photo ID required
Travelling with others
- Children (2 years old and younger) stay free when occupying the parent or guardian's room, using existing bedding
- No pets or service animals allowed
- Free WiFi in public areas
- Free WiFi and wired Internet access in rooms
- Free self parking (limited)
- Accessible parking
- Free theme park shuttle
Nearby Four Star Vila-seca de Solcina hotels
In the hotel
- 2 restaurants
- Bar/lounge
- Poolside bar
- Number of outdoor pools - 4
- Children's pool
- Water park access (surcharge)
- Pool umbrellas
- Arcade/game room
- Number of meeting rooms - 4
- 24-hour front desk
- Concierge services
- Tours/ticket assistance
- Year Built 2009
- Elevator/lift
- ATM/banking
- Safe-deposit box at front desk
- Rooftop terrace
- Garden
- Disabled parking
- Accessible bathroom
- In-room accessibility
In the room
- Air conditioning
- Minibar
- Private bathroom
- Bathtub or shower
- Free toiletries
- Hair dryer
- Flat-screen TV
- Satellite TV channels
- Free WiFi
- Phone
- In-room safe
Top Vila-seca de Solcina hotels
Recently reviewed hotels in Vila-seca de Solcina
- Hotel Sant JordiFrom
- Hotel Termes MontbrioFrom
"Our stay was much too short... less than a day. Unfortunately, we couldn't find the place because google maps directed us to a back entrance from within the small town of Montbrio…"Jul 29, 2015
- Hotel 4R Salou Park
- Gran Palas HotelFrom
"great hotel I'll go back to the same hotel close to the beach and 100 places where to eat..."Jul 12, 2015
Nearby hotels
Special features
DiningBuffet Grand Hall - Onsite buffet restaurant.
PortAventura Hotel Gold River, Vila-seca de Solcina's small print
Also known as
- PortAventura Gold River
- PortAventura Gold River Vila-Seca
- PortAventura Hotel Gold River
- PortAventura Hotel Gold River Vila-Seca
Cash transactions at this property cannot exceed EUR 2500, due to national regulations. For further details, please contact the property using information in the booking confirmation.
Only registered guests are allowed in the guestrooms.
Mandatory fees
You'll be asked to pay the following charges at check in or check out:
A tourist tax will be collected at the property upon arrival. The tax applies up to a maximum of 7 nights per person per stay. Children under 17 years of age are exempt from this tax.
- A tax is imposed by the city: EUR 0.99 per person, per night, up to 7 nights. This tax does not apply to children under 17 years of age.
The charges below are included in the total price displayed:
- Christmas Eve gala dinner fee for stays on 24 December
- New Year's Eve gala dinner fee for stays on 31 December
Optional extras
Facility access costs EUR 10 per person, per day. Facilities include fitness facilities, a sauna, a spa, a spa tub, and a swimming pool.
High-speed Internet access (wired) is available in public areas for an extra charge
We have included all charges provided to us by this hotel. However, charges can vary, for example, based on length of stay or the room you book.
Hotel registry number: HT-85504


text:
Serse Cosmi: "Roma deserved the victory, even if we could have and should've done more after taking the lead. We have it all to gamble every single Sunday."
Zdenek Zeman: "I am happy with the team's response after going a goal down. It was much better compared to the performance in Pescara, but we still need to find concentration and consistency."
Check out OLBG.com's list of ££ Free Bets from UK bookmakers before placing your bets!


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Extended Stay America - Washington, D.C. - Herndon - Dulles
No prices found through our partners. Please contact the business directly or check some of our recommended alternatives.
How has this hotel rated in the past?
- Continental Breakfast
- Free High-Speed Internet
- Wheelchair accessibility
- Kitchenette
- Free parking
- Pets allowed
Travelers also recommend:
- More recommendations
TripAdvisor Reviews Extended Stay America - Washington, D.C. - Herndon - Dulles
Travel Blogs from Herndon
A Rainy Day at the Smithsonian Museums
... convert part of the Customs House in New York to a satellite museum. The new museum is an impressive building, but I have mixed feelings about the displays. The trend in museums is more toward frequently changing exhibits of parts of the collection on specific themes rather than showcasing massive numbers of artifacts as in older museums like the American Museum of Natural History in New York. Some of the current exhibits at the museum are interesting, ...
A Big Day in the Washington DC
... have mainly Burgers or Pizza that looks nothing like the Pizza
that we are used to at home. No, we are not complaining, just making an observation.
We both slept for a short time on
the train, the train departed Washington DC at 7:20pm and arrived back at the
Penn Street Station at 11:00pm, fortunately its less than a 5 minute walk to
the Hotel from here, we were both tired, but it was another fantastic ...
Day 173: Reunion Time in Washington DC
... with Nick and Maura. They live in a really nice neighbourhood and we were immediately taken up onto the roof of the apartment block for some impressive sunset views across DC. Maura then cooked a tasty chicken dinner for us and we shared a fair amount of wine while the stories both old and new were in full flow. I'm really happy to finally be here, it's just a shame we haven't seen each other for so long but I'm sure we can make up for it. ...
The kids are safely taped in their rooms.....
... could have drawn blood from Mrs. Ham's arm if it hadn't calmed down when it did. The gentleman to my left was also relieved I released his shoulder... I don't think our new travelers were as traumatized as I was worried they might be! PHEW!!!
Bathroom breaks take forever with a group our size... Emma had time to buy 12 doughnuts and consume them all, while Fergus and Mason drove the toy train. Our tour guide and bus driver were very easy to find ...
... quite special to be standing outside the White House. DC is a nice place to visit, but also nice to get out of there. Way too busy.
On our way again. Were in 6 states today. Maryland, Delaware, New Jersey, NY State, Pennsylvania and Connecticut. Drove through Annapolis, the capital of Maryland. Drove on the I95 highway through Queens and The Bronx, avoiding the drive through New York city. Paid lots of tolls along our way, think a total ...


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What in the world is the vehicle you see above? Well, um... yeah. We have no idea. According to the video description from YouTube, however, it's a modified Jeep Wrangler, and it comes from the same person who created the equally insane side-by-side merged Wrangler you saw here.
1 / 1
74Another crazy custom Jeep Wrangler spotted in Morocco
23VIDEO: C/D channels inner redneck with International LoneStar Harley-Davidson
- Chris Shunk
- Aug 5, 2009
- 23
5Chicago 2008: LoneStar semi might just create green envy in trucking industry
- Sebastian Blanco
- Feb 7, 2008
- 5
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Question asked by Joseph Cannon 438 days ago
Looking for an AFAA certified personal trainer to interview
I want to interview an AFAA personal trainer, preferably someone who has been recently certified. I'll send you the questions and you just have to answer 0them. The interview will appear on my website with a link back to your website, FB page etc.


text: It is in our opinion the best in Memphis. We found this place because our favorite place was too crowded. The service is simple, go to the counter and order your pizza and beer and sit down. In short order they will call you and after your first bite, you'll know why we love this place.


text:
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Trupanion's Top 5 Instagram Pics of January 2013
Did you know that we're on Instagram? We love all things pets, so of course we're posting photos! Follow @trupanion on Instagram to keep up with our office dog and cat shenanigans, and we may even share a photo of
January 31, 2013
25 Cats to Follow on Twitter
If you're a pet lover and you frequent Twitter, then we have a few must-follow accounts for you! Of course, be sure to follow us too @Trupanion! Send us a tweet and we'll follow back! Top 5 Internet Famous Cats @IAMLILBUB Lil
January 24, 2013
This Week in Testimonials – 1/18
Funny story – I was arguing with a woman I work with about who has the best insurance – we finally duked it out and realized we both were under Trupanion -Sara B. I have a very sick dog insured
January 18, 2013
Tagged with: cat, dog, Pet Insurance
Warm and Fuzzy Pets
The weather outside is chilly (for most of us) and it's important that we keep our pets warm, safe, and healthy during these cold winter months. We've provided some cold weather pet tips and asked for you to share a
January 18, 2013
This Week in Testimonials – 1/4
Dinglehopper's 2012 vet costs totalled $6,949.04. Thank-you Trupanion for covering $4,288.60 of that! -Michelle D. GLAD TO BE A PART OF THIS FAMILY! MY DOG DOLLAR IS HAPPY TOO…. -Craig T. Just received a call from Mel at Trupanion.. Making
January 4, 2013
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Welcome to The Fooks Team!
Here you will find a wide variety of useful information and resources designed to help you buy or sell a home more effectively in the Warwick areas. From information on the local community, to advice about finding a mortgage or preparing your home to sell, it's all available here on my web site.
You can also search for your ideal home by viewing current listings with detailed descriptions and photos. Or you can get help determining the value of your home by requesting a report that includes the prices of similar homes that recently sold or are currently for sale in the Warwick areas.
So, whether you're buying or selling, feel free to contact me and I will be happy to help you with all of your real estate needs.
The following websites are great tools for searching beautiful homes in your area! See something you like? Give us a call and we will gladly get you in to view the property.
Also, visit our Facebook page for some of our newest listings, fun DIY ideas and recipes! https://www.facebook.com/FooksTeam


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