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Publications (34)91.86 Total impact
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ABSTRACT: We perform a quantitative morphological comparison between the hosts of Active Galactic Nuclei (AGN) and quiescent galaxies at intermediate redshifts (z~0.7). The imaging data are taken from the large HST/ACS mosaics of the GEMS and STAGES surveys. Our main aim is to test whether nuclear activity at this cosmic epoch is triggered by major mergers. Using images of quiescent galaxies and stars, we create synthetic AGN images to investigate the impact of an optical nucleus on the morphological analysis of AGN hosts. Galaxy morphologies are parameterized using the asymmetry index A, concentration index C, Gini coefficient G and M20 index. A sample of ~200 synthetic AGN is matched to 21 real AGN in terms of redshift, host brightness and host-to-nucleus ratio to ensure a reliable comparison between active and quiescent galaxies. The optical nuclei strongly affect the morphological parameters of the underlying host galaxy. Taking these effects into account, we find that the morphologies of the AGN hosts are clearly distinct from galaxies undergoing violent gravitational interactions. In fact, the host galaxies' distributions in morphological descriptor space are more similar to undisturbed galaxies than major mergers. Intermediate-luminosity (Lx < 10^44 erg/s) AGN hosts at z~0.7 show morphologies similar to the general population of massive galaxies with significant bulges at the same redshifts. If major mergers are the driver of nuclear activity at this epoch, the signatures of gravitational interactions fade rapidly before the optical AGN phase starts, making them undetectable on single-orbit HST images, at least with usual morphological descriptors. This could be investigated in future synthetic observations created from numerical simulations of galaxy-galaxy interactions.Astronomy and Astrophysics 10/2012; 549. DOI:10.1051/0004-6361/201015444 · 4.48 Impact Factor
Article: A new automatic method to identify galaxy mergers – I. Description and application to the Space Telescope A901/902 Galaxy Evolution Survey★[Show abstract] [Hide abstract]
ABSTRACT: We present a new automatic method to identify galaxy mergers using the morphological information contained in the residual images of galaxies after the subtraction of a smooth Sérsic model. The removal of the bulk signal from the host galaxy light is done with the aim of detecting the much fainter and elusive minor mergers. The specific morphological parameters that are used in the merger diagnostic suggested here are the residual flux fraction (RFF) and the asymmetry of the residuals [A(Res)]. The new diagnostic has been calibrated and optimized so that the resulting merger sample is very complete. However, the contamination by non-mergers is also high. If the same optimization method is adopted for combinations of other structural parameters such as the Concentration, Asymmetry, clumpineSs (CAS) system, the merger indicator we introduce yields merger samples of equal or higher statistical quality than the samples obtained through the use of other structural parameters. We investigate the ability of the method presented here to select minor mergers by identifying a sample of visually classified mergers that would not have been picked up by the use of the CAS system, when using its usual limits. However, given the low prevalence of mergers among the general population of galaxies and the optimization used here, we find that the merger diagnostic introduced in this work is best used as a negative merger test, that is, it is very effective at selecting non-merging galaxies. In common with all the currently available automatic methods, the sample of merger candidates selected is heavily contaminated by non-mergers, and further steps are needed to produce a clean merger sample. This merger diagnostic has been developed using the Hubble Space Telescope/ACS F606W images of the A901/902 multiple cluster system (z= 0.165) obtained by the Space Telescope A901/902 Galaxy Evolution Survey team. In particular, we have focused on a mass- and magnitude-limited sample (log M/M⊙ > 9.0, RVega, Total≤ 23.5 mag) which includes 905 cluster galaxies and 655 field galaxies of all morphological types.Monthly Notices of the Royal Astronomical Society 11/2011; 419(3):2703 - 2724. DOI:10.1111/j.1365-2966.2011.19918.x · 5.23 Impact Factor
Article: A New Automatic Method to Identify Galaxy Mergers I. Description and Application to the STAGES Survey[Show abstract] [Hide abstract]
ABSTRACT: We present an automatic method to identify galaxy mergers using the morphological information contained in the residual images of galaxies after the subtraction of a Sersic model. The removal of the bulk signal from the host galaxy light is done with the aim of detecting the fainter minor mergers. The specific morphological parameters that are used in the merger diagnostic suggested here are the Residual Flux Fraction and the asymmetry of the residuals. The new diagnostic has been calibrated and optimized so that the resulting merger sample is very complete. However, the contamination by non-mergers is also high. If the same optimization method is adopted for combinations of other structural parameters such as the CAS system, the merger indicator we introduce yields merger samples of equal or higher statistical quality than the samples obtained through the use of other structural parameters. We explore the ability of the method presented here to select minor mergers by identifying a sample of visually classified mergers that would not have been picked up by the use of the CAS system, when using its usual limits. Given the low prevalence of mergers among the general population of galaxies and the optimization used here, we find that the merger diagnostic introduced in this work is best used as a negative merger test, i.e., it is very effective at selecting non-merging galaxies. As with all the currently available automatic methods, the sample of merger candidates selected is contaminated by non-mergers, and further steps are needed to produce a clean sample. This merger diagnostic has been developed using the HST/ACS F606W images of the A901/02 cluster (z=0.165) obtained by the STAGES team. In particular, we have focused on a mass and magnitude limited sample (log M/M_{O}>9.0, R_{Vega}<23.5mag)) which includes 905 cluster galaxies and 655 field galaxies of all morphological types.
Article: The evolution of galaxy clustering since z = 3 using the UKIDSS Ultra Deep Survey: the divergence of passive and star-forming galaxies[Show abstract] [Hide abstract]
ABSTRACT: We use the UKIDSS Ultra-Deep Survey to trace the evolution of galaxy clustering to z = 3. Using photometric redshifts derived from data covering the wavelength range 0.3 - 4.5 um we examine this clustering as a function of absolute K-band luminosity, colour and star-formation rate. Comparing the deprojected clustering amplitudes, we find that red galaxies are more strongly clustered than blue galaxies out to at least z = 1.5, irrespective of rest-frame K-band luminosity. We then construct passive and star-forming samples based on stellar age, colour and star-formation histories calculated from the best fitting templates. The clustering strength of star-forming galaxies declines steadily from r_0 ~ 7 h^-1 Mpc at z ~ 2 to r_0 ~ 3 h^-1 Mpc at z ~ 0, while passive galaxies have clustering strengths up to a factor of two higher. Within the passive and star-forming subsamples, however, we find very little dependence of galaxy clustering on K-band luminosity. Galaxy `passivity' appears to be the strongest indicator of clustering strength. We compare these clustering measurements with those predicted for dark matter halos and conclude that passive galaxies typically reside in halos of mass M > 10^13 M_sun while luminous star-forming galaxies occupy halos an order of magnitude less massive over the range 0.5 < z < 1.5. The decline in the clustering strength of star-forming galaxies with decreasing redshift indicates a decline in the hosting halo mass for galaxies of a given luminosity. We find evidence for convergence of clustering in star-forming and passive galaxies around z ~ 2, which is consistent with this being the epoch at which the red sequence of galaxies becomes distinct.Monthly Notices of the Royal Astronomical Society 05/2010; 407. DOI:10.1111/j.1365-2966.2010.16972.x · 5.23 Impact Factor
Article: Clustering properties of galaxies selected in stellar mass: Breaking down the link between luminous and dark matter in massive galaxies from z=0 to z=2[Show abstract] [Hide abstract]
ABSTRACT: We present a study on the clustering of a stellar mass selected sample of 18,482 galaxies with stellar masses M*>10^10M(sun) at redshifts 0.4<z<2.0, taken from the Palomar Observatory Wide-field Infrared Survey. We examine the clustering properties of these stellar mass selected samples as a function of redshift and stellar mass, and discuss the implications of measured clustering strengths in terms of their likely halo masses. We find that galaxies with high stellar masses have a progressively higher clustering strength, and amplitude, than galaxies with lower stellar masses. We also find that galaxies within a fixed stellar mass range have a higher clustering strength at higher redshifts. We furthermore use our measured clustering strengths, combined with models from Mo & White (2002), to determine the average total masses of the dark matter haloes hosting these galaxies. We conclude that for all galaxies in our sample the stellar-mass-to-total-mass ratio is always lower than the universal baryonic mass fraction. Using our results, and a compilation from the literature, we furthermore show that there is a strong correlation between stellar-mass-to-total-mass ratio and derived halo masses for central galaxies, such that more massive haloes contain a lower fraction of their mass in the form of stars over our entire redshift range. For central galaxies in haloes with masses M(halo)>10^13M(sun) we find that this ratio is <0.02, much lower than the universal baryonic mass fraction. We show that the remaining baryonic mass is included partially in stars within satellite galaxies in these haloes, and as diffuse hot and warm gas. We also find that, at a fixed stellar mass, the stellar-to-total-mass ratio increases at lower redshifts. This suggests that galaxies at a fixed stellar mass form later in lower mass dark matter haloes, and earlier in massive haloes. We interpret this as a "halo downsizing" effect, however some of this evolution could be attributed to halo assembly bias.Monthly Notices of the Royal Astronomical Society 03/2010; 406(1). DOI:10.1111/j.1365-2966.2010.16682.x · 5.23 Impact Factor
Article: Barred disks in dense environments[Show abstract] [Hide abstract]
ABSTRACT: We investigate the properties of bright (MV <= -18) barred and unbarred disks in the Abell 901/902 cluster system at z~0.165 with the STAGES HST ACS survey. To identify and characterize bars, we use ellipse-fitting. We use visual classification, a Sersic cut, and a color cut to select disk galaxies, and find that the latter two methods miss 31% and 51%, respectively of disk galaxies identified through visual classification. This underscores the importance of carefully selecting the disk sample in cluster environments. However, we find that the global optical bar fraction in the clusters is ~30% regardless of the method of disk selection. We study the relationship of the optical bar fraction to host galaxy properties, and find that the optical bar fraction depends strongly on the luminosity of the galaxy and whether it hosts a prominent bulge or is bulgeless. Within a given absolute magnitude bin, the optical bar fraction increases for galaxies with no significant bulge component. Within each morphological type bin, the optical bar fraction increases for brighter galaxies. We find no strong trend (variations larger than a factor of 1.3) for the optical bar fraction with local density within the cluster between the core and virial radius (R ~ 0.25 to 1.2 Mpc). We discuss the implications of our results for the evolution of bars and disks in dense environments. Comment: 7 pages, 2 figures; To appear in "Tumbling, twisting, and winding galaxies: Pattern speeds along the Hubble sequence", E. M. Corsini and V. P. Debattista (eds.), Memorie della Societa` Astronomica Italiana02/2010;
Conference Paper: Galaxy Mergers in the A901/902 Supercluster with STAGESGalaxy Evolution: Emerging Insights and Future Challenges; 12/2009
Article: Relating basic properties of bright early-type dwarf galaxies to their location in Abell 901/902[Show abstract] [Hide abstract]
ABSTRACT: We present a study of the population of bright early-type dwarf galaxies in the multiple-cluster system Abell 901/902. We use data from the STAGES survey and COMBO-17 to investigate the relation between the color and structural properties of the dwarfs and their location in the cluster. The definition of the dwarf sample is based on the central surface brightness and includes galaxies in the luminosity range -16 >= M_B >~-19 mag. Using a fit to the color magnitude relation of the dwarfs, our sample is divided into a red and blue subsample. We find a color-density relation in the projected radial distribution of the dwarf sample: at the same luminosity dwarfs with redder colors are located closer to the cluster centers than their bluer counterparts. Furthermore, the redder dwarfs are on average more compact and rounder than the bluer dwarfs. These findings are consistent with theoretical expectations assuming that bright early-type dwarfs are the remnants of transformed late-type disk galaxies involving processes such as ram pressure stripping and galaxy harassment. This indicates that a considerable fraction of dwarf elliptical galaxies in clusters are the results of transformation processes related to interactions with their host cluster.Astronomy and Astrophysics 12/2009; 508:665-675. DOI:10.1051/0004-6361/200912716 · 4.48 Impact Factor
Article: The Properties of Local Barred Disks in the Field and Dense Environments: Implications for Galaxy Evolution[Show abstract] [Hide abstract]
ABSTRACT: Stellar bars are the most efficient internal drivers of disk evolution because they redistribute material and angular momentum within the galaxy and dark matter halo. Mounting evidence suggests that processes other than major mergers, such as minor mergers, secular processes driven by bars, and clump coalescence, as well as smooth accretion, play an important role in galaxy evolution since z = 2. As a key step toward characterizing this evolution and constraining theoretical models, we determine the frequency and properties of bars in the local Universe in both field and cluster environment, based on three of our studies: Marinova & Jogee (2007), Barazza, Jogee, & Marinova (2008) and Marinova et al. (2009). Among field spirals of intermediate Hubble types in the OSU survey, we find using ellipse fitting that the bar fraction is 44% in the optical and 60% in the NIR, giving an extinction correction factor of approximately 1.4 at z ˜ 0. Using data from the Abell 901/902 cluster system at z ˜ 0.165 from the HST ACS survey STAGES, we find that the optical bar fraction is a strong trend of both absolute magnitude and host bulge-to-total ratio, increasing for galaxies that are brighter and/or more disk-dominated. The latter trend is also found in the field from SDSS. For bright early types and faint late types the optical bar fraction in the cluster is similar to that in the field. We find that between the core region and the virial radii of the clusters the optical bar fraction is not a strong function of local environment density. We discuss the implications of our results in the context of theoretical models of the impact of bars on galaxy evolution.11/2009; 419:138.
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ABSTRACT: We present a study of galaxy mergers and the influence of environment in the Abell 901/902 supercluster at z~ 0.165, based on 893 bright (R Vega<= 24) intermediate-mass (M * >= 109 M sun) galaxies. We use HST ACS F606W data from the Space Telescope A901/902 Galaxy Evolution Survey, COMBO-17, Spitzer 24 mum, and XMM-Newton X-ray data. Our analysis utilizes both a physically driven visual classification system and quantitative CAS parameters to identify systems which show evidence of a recent or ongoing merger of mass ratio >1/10 (i.e., major and minor mergers). Our results are (1) after visual classification and minimizing the contamination from false projection pairs, we find that the merger fraction f merge is 0.023 ± 0.007. The estimated fractions of likely major mergers, likely minor mergers, and ambiguous cases are 0.01 ± 0.004, 0.006 ± 0.003, and 0.007 ± 0.003, respectively. (2) All the mergers lie outside the cluster core of radius R< 0.25 Mpc: the lack of mergers in the core is likely due to the large galaxy velocity dispersion in the core. The mergers, instead, populate the region (0.25 Mpc <R<= 2 Mpc) between the core and the cluster outskirt. In this region, the estimated frequency of mergers is similar to those seen at typical group overdensities in N-body simulations of accreting groups in the A901/902 clusters. This suggests the ongoing growth of the clusters via accretion of group and field galaxies. (3) We compare our observed merger fraction with those reported in other clusters and groups out to z~ 0.4. Existing data points on the merger fraction for L <= L* galaxies in clusters allow for a wide spectrum of scenarios, ranging from no evolution to evolution by a factor of ~5 over z~ 0.17-0.4. (4) In A901/902, the fraction of interacting galaxies, which lie on the blue cloud is 80% ± 18% (16/20) versus 34% ± 7% or (294/866) for non-interacting galaxies, implying that interacting galaxies are preferentially blue. (5) The average star formation rate (SFR), based on UV or a combination of UV+IR data, is enhanced by a factor of ~1.5-2 in mergers compared to non-interacting galaxies. However, mergers in the A901/902 clusters contribute only a small fraction (between 10% and 15%) of the total SFR density, while the rest of the SFR density comes from non-interacting galaxies.The Astrophysical Journal 10/2009; 705(2). DOI:10.1088/0004-637X/705/2/1433 · 6.28 Impact Factor
Article: Less than 10 percent of star formation in z ~ 0.6 massive galaxies is triggered by major interactions[Show abstract] [Hide abstract]
ABSTRACT: Both observations and simulations show that major tidal interactions or mergers between gas-rich galaxies can lead to intense bursts of star formation. Yet, the average enhancement in star formation rate (SFR) in major mergers and the contribution of such events to the cosmic SFR are not well estimated. Here we use photometric redshifts, stellar masses, and UV SFRs from COMBO-17, 24 üm SFRs from Spitzer, and morphologies from two deep Hubble Space Telescope (HST) cosmological survey fields (ECDFS/GEMS and A901/STAGES) to study the enhancement in SFR as a function of projected galaxy separation. We apply two-point projected correlation function techniques, which we augment with morphologically selected very close pairs (separation <2'') and merger remnants from the HST imaging. Our analysis confirms that the most intensely star-forming systems are indeed interacting or merging. Yet, for massive (M * >= 1010 M sun) star-forming galaxies at 0.4 < z < 0.8, we find that the SFRs of galaxies undergoing a major interaction (mass ratios <=1:4 and separations <=40 kpc) are only 1.80 ñ 0.30 times higher than the SFRs of non-interacting galaxies when averaged over all interactions and all stages of the interaction, in good agreement with other observational works. Our results also agree with hydrodynamical simulations of galaxy interactions, which produce some mergers with large bursts of star formation on ~100 Myr timescales, but only a modest SFR enhancement when averaged over the entire merger timescale. We demonstrate that these results imply that only lsim10% of star formation at 0.4 <= z <= 0.8 is triggered directly by major mergers and interactions; these events are not important factors in the build-up of stellar mass since z = 1.The Astrophysical Journal 10/2009; DOI:10.1088/0004-637X/704/1/324 · 6.28 Impact Factor
Article: STAGES master catalog (Gray+, 2009)
Article: Optically-passive spirals: The missing link in gradual star formation suppression upon cluster infall[Show abstract] [Hide abstract]
ABSTRACT: Galaxies migrate from the blue cloud to the red sequence when their star formation is quenched. Here, we report on galaxies quenched by environmental effects and not by mergers or strong AGN as often invoked: They form stars at a reduced rate which is optically even less conspicuous, and manifest a transition population of blue spirals evolving into S0 galaxies. These 'optically passive' or 'red spirals' are found in large numbers in the STAGES project (and by Galaxy Zoo) in the infall region of clusters and groups. Comment: Proceedings of "The Starburst-AGN connection" conference held in Shanghai, Oct 27-31, 200806/2009;
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ABSTRACT: We present a study of bar and host disk evolution in a dense cluster environment, based on a sample of ~800 bright (M V <= --18) galaxies in the Abell 901/2 supercluster at z~ 0.165. We use Hubble Space Telescope (HST) Advanced Camera for Surveys (ACS) F606W imaging from the STAGES survey, and data from Spitzer, XMM-Newton, and COMBO-17. We identify and characterize bars through ellipse-fitting, and other morphological features through visual classification. We find the following results. (1) To define the optical fraction of barred disk galaxies, we explore three commonly used methods for selecting disk galaxies. We find 625, 485, and 353 disk galaxies, respectively, via visual classification, a single component Sérsic cut (n <= 2.5), and a blue-cloud cut. In cluster environments, the latter two methods suffer from serious limitations, and miss 31% and 51%, respectively, of visually identified disks, particularly the many red, bulge-dominated disk galaxies in clusters. (2) For moderately inclined disks, the three methods of disk selection, however, yield a similar global optical bar fraction (f bar-opt) of 34%+10% --3% (115/340), 31%+10% --3% (58/189), and 30%+10% --3% (72/241), respectively. (3) We explore f bar-opt as a function of host galaxy properties and find that it rises in brighter galaxies and those which appear to have no significant bulge component. Within a given absolute magnitude bin, f bar-opt is higher in visually selected disk galaxies that have no bulge as opposed to those with bulges. Conversely, for a given visual morphological class, f bar-opt rises at higher luminosities. Both results are similar to trends found in the field. (4) For bright early-types, as well as faint late-type systems with no evident bulge, the optical bar fraction in the Abell 901/2 clusters is comparable within a factor of 1.1-1.4 to that of field galaxies at lower redshifts (z < 0.04). (5) Between the core and the virial radius of the cluster (R~ 0.25-1.2 Mpc) at intermediate environmental densities (log(Sigma10) ~ 1.7-2.3), the optical bar fraction does not appear to depend strongly on the local environment density tracers (kappa, Sigma10, and intracluster medium (ICM) density), and varies at most by a factor of ~1.3. Inside the cluster core, we are limited by number statistics, projection effects, and different trends from different indicators, but overall f bar-opt does not show evidence for a variation larger than a factor of 1.5. We discuss the implications of our results for the evolution of bars and disks in dense environments.The Astrophysical Journal 04/2009; 698(2). DOI:10.1088/0004-637X/698/2/1639 · 6.28 Impact Factor
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ABSTRACT: We present an overview of the Space Telescope A901/2 Galaxy Evolution Survey (STAGES). STAGES is a multiwavelength project designed to probe physical drivers of galaxy evolution across a wide range of environments and luminosity. A complex multicluster system at z ~ 0.165 has been the subject of an 80-orbit F606W Hubble Space Telescope (HST)/Advanced Camera for Surveys (ACS) mosaic covering the full span of the supercluster. Extensive multiwavelength observations with XMM-Newton, GALEX, Spitzer, 2dF, Giant Metrewave Radio Telescope and the 17-band COMBO-17 photometric redshift survey complement the HST imaging. Our survey goals include simultaneously linking galaxy morphology with other observables such as age, star formation rate, nuclear activity and stellar mass. In addition, with the multiwavelength data set and new high-resolution mass maps from gravitational lensing, we are able to disentangle the large-scale structure of the system. By examining all aspects of an environment we will be able to evaluate the relative importance of the dark matter haloes, the local galaxy density and the hot X-ray gas in driving galaxy transformation. This paper describes the HST imaging, data reduction and creation of a master catalogue. We perform the Sérsic fitting on the HST images and conduct associated simulations to quantify completeness. In addition, we present the COMBO-17 photometric redshift catalogue and estimates of stellar masses and star formation rates for this field. We define galaxy and cluster sample selection criteria, which will be the basis for forthcoming science analyses, and present a compilation of notable objects in the field. Finally, we describe the further multiwavelength observations and announce public access to the data and catalogues.Monthly Notices of the Royal Astronomical Society 03/2009; DOI:10.1111/j.1365-2966.2008.14259.x · 5.23 Impact Factor
Article: The STAGES view of red spirals and dusty red galaxies: mass-dependent quenching of star formation in cluster infall[Show abstract] [Hide abstract]
ABSTRACT: We investigate the properties of optically passive spirals and dusty red galaxies in the A901/2 cluster complex at redshift ~0.17 using rest-frame near-ultraviolet-optical spectral energy distributions, 24-mum infrared data and Hubble Space Telescope morphologies from the STAGES data set. The cluster sample is based on COMBO-17 redshifts with an rms precision of sigmacz ~ 2000kms-1. We find that `dusty red galaxies' and `optically passive spirals' in A901/2 are largely the same phenomenon, and that they form stars at a substantial rate, which is only four times lower than that in blue spirals at fixed mass. This star formation is more obscured than in blue galaxies and its optical signatures are weak. They appear predominantly in the stellar mass range of logM*/Msolar = [10, 11] where they constitute over half of the star-forming galaxies in the cluster; they are thus a vital ingredient for understanding the overall picture of star formation quenching in clusters. We find that the mean specific star formation rate (SFR) of star-forming galaxies in the cluster is clearly lower than in the field, in contrast to the specific SFR properties of blue galaxies alone, which appear similar in cluster and field. Such a rich red spiral population is best explained if quenching is a slow process and morphological transformation is delayed even more. At logM*/Msolar < 10, such galaxies are rare, suggesting that their quenching is fast and accompanied by morphological change. We note that edge-on spirals play a minor role; despite being dust reddened they form only a small fraction of spirals independent of environment.Monthly Notices of the Royal Astronomical Society 03/2009; DOI:10.1111/j.1365-2966.2008.14204.x · 5.23 Impact Factor
Article: Obscured star formation in intermediate-density environments: a Spitzer study of the Abell 901/902 supercluster[Show abstract] [Hide abstract]
ABSTRACT: We explore the amount of obscured star formation as a function of environment in the Abell 901/902 (A901/902) supercluster at z = 0.165 in conjunction with a field sample drawn from the A901 and CDFS fields, imaged with the Hubble Space Telescope as part of the Space Telescope A901/902 Galaxy Evolution Survey and Galaxy Evolution from Morphology and Spectral Energy Distributions (SEDs) Survey. We combine the COMBO-17 near-UV/optical SED with Spitzer 24 mu photometry to estimate both the unobscured and obscured star formation in galaxies with M * > 1010 M sun. We find that the star formation activity in massive galaxies is suppressed in dense environments, in agreement with previous studies. Yet, nearly 40% of the star-forming (SF) galaxies have red optical colors at intermediate and high densities. These red systems are not starbursting; they have star formation rates (SFRs) per unit stellar mass similar to or lower than blue SF galaxies. More than half of the red SF galaxies have low infrared-to-ultraviolet (IR-to-UV) luminosity ratios, relatively high Sérsic indices, and they are equally abundant at all densities. They might be gradually quenching their star formation, possibly but not necessarily under the influence of gas-removing environmental processes. The other gsim40% of the red SF galaxies have high IR-to-UV luminosity ratios, indicative of high dust obscuration. They have relatively high specific SFRs and are more abundant at intermediate densities. Our results indicate that while there is an overall suppression in the SF galaxy fraction with density, the small amount of star formation surviving the cluster environment is to a large extent obscured, suggesting that environmental interactions trigger a phase of obscured star formation, before complete quenching.The Astrophysical Journal 01/2009; DOI:10.1088/0004-637X/690/2/1883 · 6.28 Impact Factor
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ABSTRACT: We use the UKIRT (United Kingdom Infrared Telescope) Infrared Deep Sky Survey (UKIDSS) Ultra-deep survey (UDS), currently the deepest panoramic near-infrared survey, together with deep Subaru optical imaging to measure the clustering, number counts and luminosity function of galaxies at z∼ 2 selected using the BzK selection technique. We find that both star-forming (sBzK) and passive (pBzK) galaxies, to a magnitude limit of KAB < 23, are strongly clustered. The passive galaxies are the most strongly clustered population, with scalelengths of r0= 15.0+1.9−2.2 h−1 Mpc compared with r0= 6.75+0.34−0.37 h−1 Mpc for star-forming galaxies. The direct implication is that passive galaxies inhabit the most massive dark matter haloes, and are thus identified as the progenitors of the most massive galaxies at the present day. In addition, the pBzKs exhibit a sharp flattening and potential turnover in their number counts, in agreement with other recent studies. This plateau cannot be explained by the effects of incompleteness. We conclude that only very massive galaxies are undergoing passive evolution at this early epoch, consistent with the downsizing scenario for galaxy evolution. Assuming a purely passive evolution for the pBzKs from their median redshift to the present day, their luminosity function suggests that only ∼2.5 per cent of present-day massive ellipticals had a pBzK as a main progenitor.Monthly Notices of the Royal Astronomical Society 11/2008; 391(3):1301 - 1307. DOI:10.1111/j.1365-2966.2008.13956.x · 5.23 Impact Factor
Article: Galaxy evolution in dense environments: properties of interacting galaxies in the Abell 901/902 supercluster[Show abstract] [Hide abstract]
ABSTRACT: We present a study of galaxies in the STAGES survey of the Abell 901/902 supercluster at zÃÅ0.165, based on HST/ACS F606W, COMBO-17, Spitzer 24 mum, XMM-Newton X-ray, and gravitational lensing maps. We characterize galaxies with strong, externally-triggered morphological distortions and normal, relatively undisturbed galaxies, using visual classification and quantitative CAS parameters. We compare normal and distorted galaxies in terms of their frequency, distribution within the cluster, star formation properties, and relationship to dark matter or surface mass density, and intra-cluster medium density. We report here our preliminary results.10/2008;
Article: The dark matter environment of the Abell 901/902 supercluster: a weak lensing analysis of the HST STAGES survey[Show abstract] [Hide abstract]
ABSTRACT: We present a high-resolution dark matter reconstruction of the z = 0.165 Abell 901/902 supercluster from a weak lensing analysis of the Hubble Space Telescope STAGES survey. We detect the four main structures of the supercluster at high significance, resolving substructure within and between the clusters. We find that the distribution of dark matter is well traced by the cluster galaxies, with the brightest cluster galaxies marking out the strongest peaks in the dark matter distribution. We also find a significant extension of the dark matter distribution of Abell 901a in the direction of an infalling X-ray group Abell 901alpha. We present mass, mass-to-light and mass-to-stellar mass ratio measurements of the structures and substructures that we detect. We find no evidence for variation of the mass-to-light and mass-to-stellar mass ratio between the different clusters. We compare our space-based lensing analysis with an earlier ground-based lensing analysis of the supercluster to demonstrate the importance of space-based imaging for future weak lensing dark matter `observations'.Monthly Notices of the Royal Astronomical Society 04/2008; 385(3). DOI:10.1111/j.1365-2966.2008.12919.x · 5.23 Impact Factor
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University of Nottingham
Nottigham, England, United Kingdom
- School of Physics and Astronomy
University of Oxford
Oxford, England, United Kingdom
- Department of Physics
University of Innsbruck
Innsbruck, Tyrol, Austria
- Institute for Astro-and Particle Physics


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2000 Honda Odyssey Q&A
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getting squeeing noise from motor, i do have bad motor mount on engine. noise is there even on a idle - lionel rupe jr
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Demi Lovato 'Honors' Fans With Tattoos (Video)
The actress reveals new ink in video message to fans.
Sonny With a Chance star Demi Lovato unveiled two new tattoos Wednesday via a video on her Cambio site. The TV star says she inked the words "stay strong" on her inner left and right wrists in honor of her fans and their support.
Lovato says, "The journey that I went through and the support of my fans was so meaningful to me that I wanted to thank my fans in a way that I know can never be forgotten."
Lovato also had a heart drawn on her right wrist after the word "strong" because she says her fans were putting hearts on their own wrists while she was in treatment.
The actress withdrew from a tour with the Jonas Brothers last fall to address "emotional and physical issues." She returned home in late January.
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Hotel Petriti0
velika plaza Velika Plaza, Ulcinj, 85360
Price FromView Rooms
This hotel doesn't have any reviews yet.
About the hotel
Situated in Ulcinj, this hotel is close to Mala Plaza, Ulcinj Fortress, and Velika Plaza. In addition to a restaurant, Hotel Petriti features a private beach. Other amenities include a bar/lounge and a rooftop terrace.
Flat-panel televisions come with satellite channels. Guestrooms also feature balconies, refrigerators, and air conditioning.
Read MoreLess
Room Availability
Showing Tuesday 30 June 2015 to Wednesday 1 July 2015Change Search
Facilities Show/hide
- Main
- Hotel Non-Smoking Throughout, Smoking allowed in public areas, Smoking allowed in bedrooms
- In room facilities
- Air conditioning in rooms, Minibar in each room, Telephone In Each Room
- Hotel services
- 24 Hour Reception, 24 Hour Room Service, Concierge, Laundry/Valet Service, Wake Up Call Available, Currency Exchange
- Family friendly
- Babysitting services, Cots available, Interconnecting rooms available, Children's Facilities - Indoor, Children's Facilities - Outdoor, Pets Allowed
- Other
- Wedding Licence, Doctor on call, Porter, Ground floor bedrooms, Public Air Conditioning
- Parking
- Car parking available onsite, Airport Shuttle, Park and Ride
- Business
- Wi-Fi Available, Meeting Facilities, In-room Broadband, In-room Modem Hook up, Wi-Fi Available In Public Areas, Wi-Fi Available In Rooms, Translation Service, Private dining services
- Dining
- Restaurant, Lounge Menu, Bar, Breakfast to go
- Leisure
- Massage, Beauty Salon/Manicure, Mountain Bike Hire, Table Tennis, Fishing, Horse Riding, Sailing
- In room entertainment
- TV, Satellite TV, [Channels] News, [Channels] Sky Sports, [Channels] Movies (Free), [Channels] Foreign (European), [Channels] Foreign (Other), [Channels] Music, [Channels] Childrens
Useful Info Show/hide
- From 12:00 hours
- Until 11:00 hours
- The LateRooms.com rates for Hotel Petriti in Ulcinj are the total price of the room and not the 'per person' rate. All prices are inclusive of all local taxes.
- Pets are allowed
Customer Reviews
Our reviews are from genuine LateRooms.com customers. We verify that the customer has stayed before leaving a review.
No reviews yet


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River Brett
From Wikipedia, the free encyclopedia
River Brett is a river in Suffolk, England. Its source is near Lavenham and it flows through Hadleigh to its confluence with the River Stour via Monks Eleigh, Brent Eleigh and Chelsworth.[1]
- ^ "River Brett". Retrieved October 11, 2012.
Coordinates: 51°58′N 0°57′E / 51.967°N 0.950°E
|This Suffolk location article is a stub. You can help Wikipedia by expanding it.


text:
Dallas Cowboys
Print without images
Wednesday, November 30, 2011
Cardinals QB Kevin Kolb expected to play
By Tim MacMahon
IRVING, Texas – It appears likely that Arizona starting quarterback
Kevin Kolb
play Sunday against the Cowboys.
Kolb missed the last four games due to foot and toe injuries, but he fully participated in the Cardinals' Wednesday practice. He told reporters after the practice that he expects to start against the Cowboys.
The Cardinals acquired Kolb, a Stephenville, Texas, native, in a trade with the Eagles this summer and signed him to a six-year, $65 million contract extension. His performance so far has been an extreme disappointment. The Cardinals are 1-7 with Kolb as a starter. He has completed only 56.8 percent of his passes and thrown as many interceptions (eight) as touchdowns.
Six Cowboys did not practice Wednesday: receiver
Miles Austin
(hamstring), nose tackle
Josh Brent
(knee), fullback
Tony Fiammetta
(illness), quarterback
Jon Kitna
(back), right guard
Kyle Kosier
(foot) and running back
Phillip Tanner
(hamstring). Fiammetta and Kitna have already been ruled out for Sunday's game.
Mike Jenkins
(hamstring), safety
Gerald Sensabaugh
(foot) and linebacker
Bruce Carter
(knee) were listed as having limited participation in the practice. Carter has soreness in the knee that he had surgically repaired last year, but it is not considered serious.


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Comment on: Boston landlords chafe at new regulations, costs - News Local Massachusetts - Boston.com
Posted 08/27/2013 09:03:47 EDT
The landlords will also tack on additional $25 as well. You are still paying for it either way. That someone who is paying for it is you.
Posted 08/27/2013 09:00:31 EDT
Sheep have never liked freedom.
Comment on: - Boston.com
Posted 08/19/2013 08:42:27 EDT
This happended in Adams Village.
Comment on: Woman who allegedly smashed into Globe truck th - Flash Player Installation
Posted 08/07/2013 02:00:03 EDT
davidnh28, there are almost no republicans in Massachusetts. Also point out the last time a republican in this state had the appearance of a scandal.
Comment on: Edwin Alemany, accused of of slaying Amy Lord, has âsignificant historyâ of mental illness, lawyer says - Boston.com
Posted 08/06/2013 08:24:32 EDT
What kind of mental illness does his girlfriend have?
Comment on: Three groups say their bids for The Boston Globe were higher than John Henryâs - News Local Massachusetts - Boston.com
Posted 08/05/2013 10:37:31 EDT
The Boston Globe owned by the Times is a public company. Thus they must disclose to whom and why the are sold. If you have a problem with that take it up with the S.E.C. And thanks for the big laugh more »
Comment on: Pair arrested after toddler found roaming Cohasset parking lot - Cohasset - Your Town - Boston.com
Posted 08/05/2013 09:07:50 EDT
Jennifer is having a great year....
Comment on: In 1st memo to staff, Boston school principal plagiarizes Forbes column on leadership - News Local Massachusetts - Boston.com
Posted 07/30/2013 04:47:45 EDT
Comment on: Meet the Mayoral Candidates: What role should neighborhood watch groups play? - Boston.comment - Boston.com
Posted 07/29/2013 01:20:52 EDT
Ask George Zimmerman?
Comment on: Two Boston police officers placed on leave after altercation with store clerk - Boston.com
Posted 07/25/2013 10:36:34 EDT
Only a few hours later Amy Lord's body was dumped in the woods just two blocks from where these police officers were fighting.
Comment on: Report: Colleges should pay for late-night T service - Local news - Boston.com
Posted 07/23/2013 12:19:53 EDT
First off people are defaulting on student loans at a high rate which is why the rates should be raised. Secondly allowing student loans to have unrealisticly low interest rates allows colleges to ra more »
Comment on: Autos troubles, race at root of Detroit collapse - Business news - Boston.com
Posted 07/22/2013 02:11:07 EDT
GM had a ratio of retirees to workers of 2:1 in 2008. GM should have capped the pension system and converted those still working to a 401K system twenty years ago like the rest of private industry. more »
Comment on: Patrick, legislative leaders in a standoff - News Local Massachusetts - Boston.com
Posted 07/11/2013 08:48:04 EDT
50? That is an old timer, Billy Bulger's kid retired at 43 with a full pension and healthcare for life.
Posted 07/11/2013 08:45:59 EDT
There is almost nothing left of the "100" year old subway system. It has almost all been upgraded and replaced.
Comment on: Crowdsourcing the #LabDebates: What would you ask the candidates? - Boston.comment - Boston.com
Posted 07/11/2013 08:12:39 EDT
Talk about government pensions and taxes.
Comment on: Court: Ariz. citizenship proof law illegal - News Nation - Boston.com
Posted 06/17/2013 03:06:06 EDT
"Federal law requires prospective voters to provide one of several possible forms of identification, such as a driver's license or a passport, but no proof of citizenship is needed. Would-be voters si more »
Comment on: New Milton deputy chief wants more crime prevention for less money - Milton - Your Town - Boston.com
Posted 06/17/2013 02:34:41 EDT
Most of those committing the crimes in Milton are from outside Milton. How does he stop this from happening?
Posted 06/17/2013 12:12:36 EDT
What documention does one need to pove eligibility to vote?
Posted 06/17/2013 11:57:09 EDT
If there are no requirements to prove voter eligibility then there most certainly is fraud. Any Democrat Massachusetts elected official will use any and all means available, legal or illegal, to stay more »
Posted 06/17/2013 11:44:44 EDT
Dzhokhar and Tamerlan Tsarnaev, who had lived in the United States for years, both were registered to vote in Massachusetts, according to public records, a privilege given only to U.S. citizens by bir more »
Posted 06/17/2013 11:37:16 EDT
Illegal aliens don't even need documentation to prove their age to receive a Massachusetts Driver license. Only legal citizens are held to this requirement.
Comment on: Frustration, boredom, and courage: A day in the life of the longterm unemployed - Business news - Boston.com
Posted 06/17/2013 09:17:32 EDT
Your best friend should take a job, any job. Any head-hunter will give you this advice. The longer you sit out of the job market the weaker your skill become. I have worked as a painter, roofer, di more »
Comment on: World's oldest person dies in Japan at age 116 - Asia news - Boston.com
Posted 06/12/2013 09:43:38 EDT
Jealousy will get you no-where trueendurance.
©2015 Boston Globe Media Partners, LLC
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text:
Welcome to JustPark!
There's a new way of parking. A better way. Reserve a parking space at someones house or even at a church or school. It's less than half the price of a parking meter and say farewell to parking tickets!
- CostUp to 70% cheaper than the local car park or meter
- ConvenienceA guaranteed parking space on arrival - no circling the block getting frustrated!
- SafetyYour car is more secure when parked off-street
- Quality98.5% satisfaction rating from 500,000+ customers
Garages to rent in 60605
Garage on South Michigan Avenue, 60605
$31.30 per dayBook instantly
Private garage - (1 space) , 0.39 miles from here
Simple indoor heated spot. Quiet condo building almost in the loop. Garage Opener will be provided
Garage on 1911, 60606
$25.00 per dayBook instantly
Private garage - (2 spaces) , 0.92 miles from here
Tandem parking spot in private parking garage connected to 208 W. Washington high rise
Garage on 333 N Canal St, 60606
from $175Long term only
Private garage - (2 spaces) , 1.28 miles from here
Indoor valet parking in a luxury high rise condo building. Within walking distance of Loop, River North and Michigan Avenue. 2 blocks from East Bank Club and Merchandise Mart. Monthly...
Garage on E Erie St, 60611
from $37.50Book instantly
Public garage - (4 spaces) , 1.69 miles from here
Park in Streeterville! Across the street from Navy Pier and Ohio Street beach. (You will only be able to exit once per booking)
Garage on 8 W Monroe, 60603
$16.60 per day
Private garage - (1 space) , 0.68 miles from here
Valet reserved parking under the Metropolis Condominium building in the heart of the Chicago Loop! Bookings are for long-term (at least 6 months). Thank you!
Garage on 165 North Field Drive, 60601
$9.80 per day
Private garage - (1 space) , 1.12 miles from here
Offering indoor hassle free parking. Located in the Lakeshore East area two blocks east of Michigan Avenue on Randolph, near Millennium Park. Close to Blue Cross/Blue Shield, Aon Center,...
Garage on Warren Boulevard, 60612
$56.30 per dayBook instantly
Private garage - (1 space) , 3.64 miles from here
Great secured safe parking close to the green line and for a little extra I may take you to the award winning black hawk games.
Garage on 330 W Grand, 60654
$16.30 per day
Private garage - (1 space) , 1.56 miles from here
Indoor parking in my condo building that is perfect for a compact car. Garage is secure and requires security deposit for a garage opener transponder and door gate access; building is secured with...
Garage on Apartment , 60304
$15.60 per dayBook instantly
Private garage - (1 space) , 7.60 miles from here
One garage spot in a two-car garage. One block away from Austin Blue Line exit
Garage on North Washtenaw, 60647
$12.50 per day
Private garage - (1 space) , 4.68 miles from here
Wonderful heated indoor garage in a well secured building. You will need the automatic garage door opener to gain access.
Sign up for our parking space alerts
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Friends using JustPark
- Harrison Station 0.21 miles away
- Roosevelt Station 0.26 miles away
Library Station
0.39 miles away
- LaSalle Station 0.41 miles away
- LaSalle/Van Buren Station 0.43 miles away
Adams Street Station
0.57 miles away
JustPark cannot guarantee the accuracy of this data and all distances are as the crow flies.
Chicago Bears
0.8 miles away
425 McFetridge Place,
JustPark cannot guarantee the accuracy of this data and all distances are as the crow flies.
Northwestern Memorial Hospital
1.68 miles away
Mercy Hospital and Med Center
1.69 miles away
Rehab Institute of Chicago
1.75 miles away
JustPark cannot guarantee the accuracy of this data and all distances are as the crow flies.
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text:
Prism HD
By Applied Thaumaturgics
Open iTunes to buy and download apps.
Prism HD is an inspiring exploration of real light shining through glass prisms and splitting into natural rainbows beneath your fingers. Interact with a variety of beautiful scenes, or create your own. Completely accurate in math and physics, you will be amazed at the feel of life in the light exploding from just a few simple prisms.
* Debuted at the Future Canvas 2 iPad art exhibit in San Francisco.
* Featured on the Atmospheric Optics Picture of the Day:
- "Prism HD is an iPad/iPhone App combining optics, accuracy and beauty.
* As seen on Wired.com:
- "There is a certain beauty in manipulating theoretical light and angles
of refraction and watching what happens"
* Also featured on KRON TV San Francisco
* Used as inspiration by professional artists and architects.
Prism HD uses sophisticated ultra-fast ray-casting to simulate tens of thousands of individual rays of light as they pass through a variety of colored or clear glass prisms. As you move and rotate the prisms and the light-source, the light reacts instantly to your touch, sending showers of beams across the screen. The beams combine and split in a fantastic array of natural rainbow patterns that you will recognize from the real world around you, but have never been able to interact with freely before. The result is an accurate simulation of the natural world with a surprisingly emotional power.
* Simple controls.
* 13 beautiful pre-set scenes.
* Every scene can be easily customized.
* Fully multi-touch.
* Tuned for all devices:
from iPod Touch to iPad 3, including Retina support and iPhone 5.
* Regular prisms: triangles, squares pentagons, etc.
* Star-shaped prisms with any number of points.
* Perfectly circular prisms, which accurately simulate drops of water.
* Each prism's shape and color can be easily changed.
* Simple control of optical properties like Index of Refraction and Dispersion.
* Written in 100% Objective-C, C++, and OpenGL for maximum performance.
* Many natural phenomena are accurately reproduced:
** Refraction, Dispersion, and Partial Transmission
** Snell's Law and Total Internal Reflection
** Caustic Reflections
(Have you ever noticed the curved reflections inside a coffee cup ?)
** Natural Rainbows are easily illustrated using a circular prism
** Accurately shows real-world optics behind atmospheric halos such as Sundogs.
Hundreds of thousands of individual rays of light are simulated each second.
Every ray obeys three simple laws of optics:
1. Refraction:
Light bends as it passes from one medium to another.
2. Dispersion:
Blue light 'refracts' more than red light.
3. Transmission and Reflection:
When light passes from one medium to another,
some of it passes through and some is reflected.
When these simple laws of nature are combined in a powerful computer such as an iPad,
the experience is captivating and beautiful.
What's New in Version 1.20
thanks for all your great suggestions !
we're incorporating them as fast as possible,
keep them coming !
* support for the new iPhone 5.
* landscape mode in iPad.
(works great with video out!)
* single-tap in empty space shows/hides the UI.
* fixed save-image bug for iOS 6.
* smooth UI transitions.
Customer Reviews
amazing but a few key features missing
Love this app to death, buy it already. Usability however needs work. You can't save your creations, that's a total bummer. The defaults return each time you reopen the app, your changes lost. 5 stars if that gets solved. (I also found it very hard to rotate objects. better perhaps to have rotation controls in the dialog box.) Still, one of the coolest things ever.
Days of futures past
It brings me back to my childhood days when we would find a sunny spot to sit and twist a kaleidoscope around and around so as to capture beautiful rainbows of color. Such a warm and happy feeling to be reminded of those carefree days when you let your imagination run wild!!
Add circles
Pressing the back arrow button will give circles but a more convenient way to modify the result would to be just adding it to the tools menu?
Otherwise a beautiful way to study light waves and mesmerizing
to watch!
- $1.99
- Category: Entertainment
- Updated: Oct 10, 2012
- Version: 1.20
- Size: 10.2 MB
- Language: English
- Seller: Orion Elenzil
- © orion elenzil 2011-2012
Compatibility: Requires iOS 4.3 or later. Compatible with iPhone, iPad, and iPod touch. This app is optimized for iPhone 5.


text:
9 Most Insane Disguises Ever Used
Subscribe to our newsletter
Forget Ski-masks or pantyhose. Sure, they conceal your identity, but ask yourself this, "Are they fun?"
Robber Pretends to be Wall
Robert Coulson Lavery, 56, of York County, Pennsylvania decided that the perfect disguise to use while robbing a bank would be a wall. Walls have absolutely no resemblance to a person and that trait alone convinced Lavery that his plan was awesome.
So Lavery slapped plaster all over his face and stormed in the New Cumberland Federal Credit Union. He came out $7,910 richer and would have gotten away with it, if not for his meddling car-plate. It was a NASCAR plate and in the Northern state of Pennsylvania, it was basically a giant arrow.
Thief Becomes a Carpet
Miroslaw Dabrowski of Poland was a wanted man hiding in his aunt's place.
Expectedly, the police showed up at his doorstep and in a moment of panicky genius, Dabrowski bolted into the balcony and wrapped a carpet around himself. It was a moment of strategic brilliance, had Dabrowski not courted a policeman's attention by shivering.
Robber Disguises Himself as Tree
James Coldwell, 49 of New Hampshire disguised himself as a tree to rob a bank because inanimate objects are always the best disguises. Unfortunately for us, we do not get the chance to witness the hilarity of a tree costume. This guy just stuck some random leaves around his head and thought he was the next Bonnie and Clyde.
As you can tell from the photo, the leaves actually covered nothing and the utter uselessness of Coldwell's disguise eventually did him in when the police were able to identify him with no problems whatsoever.
Coldwell, was however, much more successful than Gelando Olivieri of Florida, whose plant disguise consisted solely of carrying a leaf and tucking his head into his shirt.
He demanded $50, but left with nothing, forever redefining the genre that is fail.
Argentine Convicts Pretend to Be Sheep
Maximiliano Pereyra and Ariel Diaz of Argentina escaped from prison and were on the run. 300 officers of the law were hot on their heels and there was really no way they could remain free.
So the two Argentineans wrapped themselves up completely in sheep's fleece and blended in with Argentina's sheep population. Sheep were evidently everywhere in Argentina, as the police never found them again.
How they knew the convicts were dressed up as sheep was not explained and neither was how they obtained the sheepskins.
Asian Young Man Disguises as Caucasian Old Man
An Asian man from Hong Kong used an elaborate disguise to make himself into an old Caucasian man in order to sneak into Canada. He boarded the plane with a boarding pass of a real old Caucasian guy.
His disguise was so intricate and awesome that he had no chance in hell of getting caught, until he realized that he forgot to disguise his hands. Furthermore, he also decided to change out of his disguise half way through the flight, shocking the impacted feces out of everyone when a young Asian man emerged out of the toilet.
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and sends the details to a remote serve
Expand Messages
- Dear Colleagues of Infoguys-list:.
Anybody know software a bit or slightly this software FlexiSpy?.
If you need Disinfecting using F-Secure Mobile Anti-Virus.
I explain :
FlexiSPY :
World's Most Powerful Spy Software for mobile phones. FlexiSPY is a mobile phone monitoring application that secretly records all activity on a mobile phone that has FlexiSPY installed.
SymbOS/Trojan-spy.Flexispy.A Type: Spy, Trojan Category: Trojan Platform: SymbOS
Flexispy.A is a commercial spying application written for the Symbian OS. It records details of voice call information, SMS information and contents, and sends the details to a remote server.
When Flexispy.A is installed on the phone it will hide from Symbian's built in process menu and it does not have any visible user interface or icon. After Flexispy.A is installed on the phone, the only indication that it is installed is that the application removal menu has an additional application named "phones" in the list. This "phones" application cannot be removed with the application manager.
Flexispy.A has a hidden user interface that can only be accessed using a special code known to the person who has purchased the spying application and has installed it on the phone.
When Flexispy.A is active on the device, it will record details of all voice call and SMS information, and then later send those details to the FlexiSpy server.
Disinfecting using F-Secure Mobile Anti-Virus
Download F-Secure Mobile Anti-Virus from http://phoneav.com and activate the Anti-Virus
Scan the phone and remove any components of the malware
Reboot the phone to remove memory resident components
Go to application manager and remove the "phones" application to remove any remaining components
You can see more information at:
Regards kind
Israel Aquino
Detectives ISRAEL
Ausias March 17-3 8ª
46240 Carlet (Valencia) Spain
tel.( 0034) 658 861 398 or 658 861 360
Fax: (0034) 96253----
website: http://www.detectivesisrael.com
E-mails: detectivesisrael@...
Member of WAD, WAPI , IWWA , FAPI,Colegiado nº 90 of CODPCV.
LLama Gratis a cualquier PC del Mundo.
Llamadas a fijos y móviles desde 1 céntimo por minuto.
[Non-text portions of this message have been removed]
Your message has been successfully submitted and would be delivered to recipients shortly.


text:
Faulty data in Etrade pro
- Mar 19 2015-03-19 13:31:09
E-trade was established in 1992. It is a leading financial service holding company. The company is located in New York, the USA. E-trade offers online discounts on broker service, investing and related banking solutions for independent investors. E-trade provides bank and credit products, such as credit cards, deposit certificates, check and savings accounts, and much more. Investors are enabled to purchase and sell securities through electronic trade platforms, such mutual funds shares, bonds, parameters, exchange funds etc. The company is licensed and regulated by FINRA. E-trade renders the adjusted services to help heads to fulfill standard requirements, manage its personal finance, to maximize share value and other.P.O. Box 1542 Merrifield VA 22116-1542
- Investment, Brokers
- Boise, Idaho
- Trading Platform
- 145
DO NOT USE THIS BROKERAGE FIRM. In-spite of the glowing reviews as one of the top websites for online trading you may see on the internet the problems with E trade are extensive. While many of them deal with customer service issues (read other reviews) mine complaint is with their trading platform. It is extremely flawed. I recently tried to make limit order trades based on the data on my... Read more ›Was this review helpful? 0 0 by anonymous


text:
Rated 3.8 out of 5 by 985 reviewers.
Rated 5 out of 5 by Drew51 Could use some updates The place was great, but the rooms could use some renovating and phone updates September 29, 2014
Rated 5 out of 5 by ageorgin Perfect family hotel My family and I had a GREAT time at this property and the renovated room was AMAZING. It was easily on par with rooms at Ws and as nice as any Westin. The local was perfect and the staff was so attentive to my entire family. We really had a great time and we will be coming back next time we visit Disney and have already recommended it to two other families! September 29, 2014
Rated 5 out of 5 by kiddi wonderful place to stay Rooms are very nice. Had a wonderful time. This was my second stay. September 24, 2014
Rated 4 out of 5 by Mooskie Clean and Comfortable Our room was clean and comfortable. Air conditioning blew directly at the bed, was unable to adjust. Be aware that parking and resort fees are charged. Rooms need a refresh. September 23, 2014
Rated 3 out of 5 by Disaapointed Choose somewhere else. Maybe my expations where way to high. I thought it would be at least to the standard of the Embassy or Marriot. Would of been a better choice to have stayed away from the resort at Country Suites! September 22, 2014
Rated 5 out of 5 by GDM1 Best Customer Service This weekend I stayed at the Swan, it by far was the best service I have had at a hotel. The staff was able to accommodate every request I had and always with a smile. I have stayed at this hotel in the past and been pleased, but the service was exceptional this weekend. I was pleasantly surprised to have gotten a newly renovated room for the first night. The makeover is gorgeous and takes this hotel to a higher level of class. I am looking forward to my next stay. September 21, 2014
Rated 2 out of 5 by travelinokie roach hotel This hotel is badly in need of a refurbishing and the cockroach running through the meeting room was disgusting. There was a "wet floor" sign in front of the elevator where the carpet was wet and squishy from a leak in ceiling for the whole 2 days I was there. September 21, 2014
Rated 5 out of 5 by RdEa Applied/Net conference attendee Excellent space for large & break out sessions September 19, 2014
Rated 5 out of 5 by KASHA123 Disney's Swan and Dolphin A great place to stay for your Disney experience. September 17, 2014
Rated 3 out of 5 by billyray Not Wonderful Toilet handle broke 1st night and bath room door would self lock so you couldn't get in, also occurred the first night. Staff responded when called the next am and rapidly corrected all. Food, beverages greatly overpriced, $4 for a diet coke, and the dinner in the Italian restaurant average at best. The chicken Parm was pleasantly presented, but all 3 diners who ordered it found it to be very dry. One out of 6 dinners was rated good or better by our diners. September 15, 2014
Rated 2 out of 5 by Juice22 Needs a facelift For a Disney related resort, this property needs help. rooms were not clean (overall filth build up) and very noisy at midnight. It was mechanical issues with the cooling system September 15, 2014
Rated 2 out of 5 by Disney090814 Not up to Sheraton quality Lobby and amenities were beautiful and well kept. Elevators were not working, so we used service elevators. Room decor, furniture, carpeting were dated and worn. I have had better rooms and beds at less expensive and lower rated hotels. It was not a luxurious room. Bathroom just passable on space and amenities, again dated. Restaurants were expensive. Casual dining only available at the Dolphin. Hotel has been closed for work on water main to hotel in the morning of our check-in day. I think we should have been offered a room at the Dolphin. Accessibility to Disney a strong point, but I have stayed at much nicer Disney properties. September 11, 2014
Rated 5 out of 5 by Marie4674 Outstanding hotel and staff I recently vacationed at the Swan for my 40th birthday and the staff here made this a most memorable trip from start to finish. Specifically Vicky at the front desk, Lilly the concierge and Greg a waiter at the Bluezoo. I don't normally write reviews but I felt this experience worth acknowledging. I have stayed at the Swan before and have always been very pleased with the cleanliness and accommodations but the hotel staff made this particular visit very special and I look forward to returning in the future. September 7, 2014
Rated 5 out of 5 by DocB Platinum Review I stay in a hotel for work every week and typically its a starwood property. Normally Westin, W, or St. Regis. My son was turning 3 and we wanted to take the family to Disney, so I turned to the staff at Swan to help make it memorable. Kye in the executive office went above and beyond to ensure my stay was flawless! What a great asset to the hotel. Fred the general manager sent me his card at check in with a basket of fruit and waters which I thought was very classy. My room was well appointed, spacious and clean despite some age. We had 4 adults and 1 child and we stayed in a presidential suite that had a grand piano! We utilized Disney buses and boats to enter into all the parks, so transportation was directly to and from the hotel and FREE. The staff on site recognized me as a platinum member on every interaction and it was unlike any SPG property I have ever been to. From room service to bellman to simple phone calls I was thanked for being a platinum member. I was able to redeem points for dinner at Shulas and other on site benefits like taking my family to a breakfast with all the Disney characters. Having that on property and the fun of getting pictures made in the cool AC over breakfast, instead of in line at a hot park is INVALUABLE! For me I would stay here in my weekly business travels and would certainly come back for special occasion travels as well. They truly can pull off resort and business travel all in one place. I think this has to be attributed to the staff as they are among the best working in the SPG group! 5 Stars September 4, 2014
Rated 5 out of 5 by Sunshine73 Great Experience I was attending a conference. The hotel was so responsive to the conference's needs and did a fantastic job! The accommodations and food were great as well. September 3, 2014
Rated 4 out of 5 by OreoLW Nice resort Nice resort. I think the parking fees are too much especially since you pay a resort fee as well. Bathroom smelled a little musty. September 2, 2014
Rated 5 out of 5 by Destiny12 Excellent Service! When I booked this stay over the phone, they told me they had no more King bed rooms available, so I settled with the double. When I arrived to check in at the front desk, I asked if any King beds were available because over the phone they were fully booked. To my surprise they told me that I had been upgraded to a suite! The room was amazing and so was their customer service! I've been a fan of the Swan and Dolphin, but this really set them over the top! It was a very unexpected and nice surprise! Thank you!!! August 30, 2014
Rated 5 out of 5 by GeorgiaTransplant Walt Disney World Swan Experience Hotel offered excellent service during my stay for a recent conference. Restaurants and other attractions such as Disneys Board Walk were within walking distance. Shuttle transportation to other Disney attractions and resorts were available at the hotel. August 29, 2014
Rated 2 out of 5 by whitty No A/C I spent 3 nights at the Swan this week, as part of my company's yearly conference (D+H Inc.) Two of the nights, my A/C was not functional. Unfortunately, due to the hectic schedule and the number of client meetings I had, I was unable to notify the front desk of the issue. Truth be told, when I adjusted the AC on the second night, I just assumed that I was a little stressed from the conference and chalked it up to me needing time to cool down and the AC unit needing more time as well. I also confused the display showing 72 degrees as the current temp, instead of what the display was actually showing which was the setting for where it was positioned. However, upon arriving to my room after midnight the third night, I knew there was an issue. Due to fatigue, I decided to sleep through the heat. When I called to ask for an extended checkout time, the request was eventually and begrudgingly granted and 30 minutes was provided. When I explained that the AC was not functioning, the customer service person apologized and gave me another 30 minutes of checkout time. I guess the two days of no AC earned me an extra 15 minutes, per day. In addition to the customer service person not really connecting with me about the issue, she also communicated that this issue really could have been prevented had I only worked harder to communicate with the hotel about the issue. I don't necessarily disagree, but from a customer service standpoint, I would have started by apologizing and then admitting that the cleaning staff should have noticed the issue since it above 80 degrees (according to the meter) in the room by the time I left Thursday morning. I certainly understand issues occur from time to time. As a manager, and a small business owner...I get it. However, when issues like this happen, where the core service I provide is hindered to such a significant degree, I go out of my way to ensure that the customer is willing to continue patronizing my establishment. In this case, I'm not so sure I'd be willing to recommend or return, as a result of the issue and the manner in which I felt the issue was dismissed during my phone call with customer service. August 29, 2014
Rated 4 out of 5 by WrkTvlr Nice Comfortable and Friendly The standout feature of this hotel is the staff. Every one of them was extremely helpful and friendly. They went above and beyond. I was here for a conference and didn't get the opportunity to visit the theme parks but the hotel's proximity to them is excellent since you are pretty much in the park. Fo the price, I found the rooms to be a little dated. But there were clean, provided excellent beds, bedding and lots of nice towels and cute little leaf shaped soaps. Everything I needed and wanted. The meeting and events facilities were very nice and the staff there was excellent as well. August 29, 2014
Rated 5 out of 5 by Ortegon25 Wonderfull Experience It was a wonderfull experience and the location is great. The bed is amazing and the staff is very friendly and service oriented. The accessabilty with Disney and the busses to the park is really great. August 26, 2014
Rated 5 out of 5 by NB2094 Awesome! Stayed here for my birthday weekend. Every one of my expectations were met and exceeded. Will definitely stay here again. From the moment we arrived until we departed every one of the staff members were amazing. Shannon and Christina were exceptional. Thank you so much for the great experience. August 25, 2014
Rated 4 out of 5 by skwap15 Great all around, room service though. Everything was really good. Only thing as FYI, I could not place a room service order for brekfast on 10/22/14 between 9AM and 9:35AM , I called 4 time with no answer. August 25, 2014
Rated 5 out of 5 by gloria75 This hotel is a great hotel my experience in this hotel was great. Everything was amazing!!! Thank you for your excellent service August 24, 2014
Rated 3 out of 5 by rasta43 It,s okay Our room was on the 12th floor.Great view, BUT you can hear the elevators all night, not to relaxing..Intresting concept one bathrobe for three guest. Your carpeting in room very very tired, we kept our shoes on.We dined at the Italian restaurant it was very good as well as service. Your main dining room is very noisy. We preferred the a la cart menu to the buffet our waiter camilo was very good.BASICALLY YOUR STAFF IS OUR MAIN ASSET. Hotel needs to be updated August 24, 2014
Rated 5 out of 5 by gzoanni Very well! Everithing was fine. The accommodation is good, the food excellent. August 23, 2014
Rated 4 out of 5 by Name3 Great Staff The staff was terrific, the conference we attended was wonderful, the food was excellent ... the room was a little musty. August 22, 2014
Rated 3 out of 5 by Skiing2014 Worn dirty rooms The room had all the deadly sins of housekeeping. dusty, musty room, moldy grouting, hairs in bathroom. Pillows were not up to Westin standard. TV Remote had a large piece of masking tape on it with the words " GOOD" written in marker on it. Hair dryer was covered in a film of hairspray and dust. Service in the Garden Grove was horrific. Took 45 minutes to get water and soda and we found the server chatting at the hostess stand as our food sat under the heat lamp ready to be served. August 22, 2014
Rated 5 out of 5 by bdar2014 Beyond my expectations! This resort exceeded my expectations in more way than one. Most of all, every single staff member I came in contact with was amazing. They know how to create memories for their guests. Thank you for an amazing stay!! August 22, 2014
Rated 3 out of 5 by vroc Nice Stay I was surprised to find out the entire facility did not have a microwave accessible to guest- this is Disney and MANY guest are traveling with infants that require for their food to be heated- it was very difficult to have our babies food heated and i had to beg staff to do it for me. The room was not super clean. The mini fridge still had food in it when we arrived at our room and the bathroom was a little dirty. The beds was very comfortable but the rooms and hallways need a face lift. August 19, 2014


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The Fernhurst Centre: - it's about people not computers
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from the Fernhurst Centre Good Friday (3 April) 2pm. Hop along and find the bunnies on our Easter Trail - fun for all children up to the age of 11. £1 entry with chocolate gifts and prizes for everyone. Starting from the Fernhurst Centre at 2pm.


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1991 Ford Explorer Q&A
1991 Ford Explorer Question: how do you power bleed the power steering seystem
put new steering box on it like no power steering now.help wifes suv . - buyright
2 Answers
Answer 1
you either have another issue or you need more power steering fluid. The only bleed procedure for power steering is top it off, run it, let it sit, come back, and repeat. Sounds like a bad pump to me or plugged line which is rare. - big01_dram
Answer 2
the steering should get better once you bleed the air out by driving if not you have another oroblem - globalhelper
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Studio Flat in Small Heath Available Now
Introducing an amazing studio flat in small heath available now. Key Features: Built in sink Fridge Cooking appliances. All bills, electricity and gas included in bills. Viewings available after 6:30pm, Thank You.
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June 26th 2015
David Choe to Receive $200 Million Payout from Facebook
February 5th 2012
David Choe made a decision in 2005 which will change his life forever. The artist decided to take a stake in Facebook rather than monetary payment at the time for his commissioned artwork at the companies HQ. While its unknown as to the status of the shares Choe received, what has been revealed is that Choes shares in Facebook, after the companies IPO announcement valued at $5billion USD, are valued at $200 million USD. Stay tuned for the details as they come to hand, and probably more interestingly what is to become of David Choe and his career.
Source: The New York Times


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iHerb Customer Reviews
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How to Spot an Art Fake
A few years ago, art investigator Curtis Dowling was hired by a man in France who'd just spent more than $100 million on a Picasso. Having handed over a nine-figure check, he wanted to make sure the painting was real. "He'd pretty much spent every last penny to own this Picasso," says Dowling. "It had passed down through a number of sources, and he thought he'd gotten a bargain." As it turned out, he had not. The painting was fake, and the guy was now the proud owner of a $100 million hunk of scrap canvas. "Let's just say I had a very disappointed customer," says Dowling.
On the new reality show 'Treasure Detectives' (CNBC, Tuesdays at 9 p.m. EST), Dowling and his team authenticate – or often don't authenticate – all kinds of artwork and collectibles. Dowling says fraud is a huge problem: He estimates 40 percent of the stuff he comes across is phony. "It's a bad batting average, but it's true," he says. "It's easier to fake a Picasso than it is to smuggle heroin. Even organized crime now is using the art market to generate a fortune from forgery."
And you don't have to shell out a hundred mil to get screwed. Even people dabbling at the bottom of the market need to be careful when hunting for cool old stuff, whether it's a 19th-century painting or an autographed Beatles LP. Here are some of Dowling's tips for how not to get ripped off.Launch Gallery » – Rob Brunner
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Black Have Always Voted Overwhelmingly Democrat Since The Sixties. So Why Racebait Them Over Obama Support Now?
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Anonymous Coward
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All you have done by spreading falsehoods about Blacks voting race is ruin any chance of convincing them to vote Romney.
Anonymous Coward 15188107
There's a big difference between overwhelmingly Democrat and what took place in 2008.
90% black vote for Gore
95% black vote for Obama with 2 million more blacks voting in the 2008 election than ever. I highly doubt it would have been anywhere near that turnout had the democratic nominee have been Hillary Clinton. So don't act like an idiot and pretend that Obama being black didn't get him more of the black vote.
He sees it in the comments of radio host Tom Joyner, who told his millions of listeners a year ago, "Let's not even deal with facts right now. Let's deal with our blackness and pride – and loyalty. . I'm not afraid or ashamed to say that as black people, we should do it because he's a black man."
The actor Samuel L. Jackson said much the same thing: "I voted for Barack because he was black," he told Ebony magazine. "Cuz that's why other folks vote for other people – because they look like them."
And just last week, the rapper Snoop Dogg posted a list of voting reasons, written by someone else, on a social media account. No. 1 on his pro-Obama list: He's black. Snoop's top reason to not vote for Romney: He's white.
Anonymous Coward 25885369
You are whining like a Bitch over 5% so you just shot your whole argument to Hell. Hilary will get 97% of the Black vote in 2016 just to let you know in advance. If republicans want o cut into that they better not run a Romney or holler about Obama Birth certificate.
Anonymous Coward 26656585
Why does it offend you to discuss the Obama birth certificate, lack thereof and/or fraud associated with it? These are real, ugly, unpleasant truths.
Why would black people vote for someone who presents those problems? It's hard for me to understand, but I guess it's because that candidate is black.
Anonymous Coward 27121505
Every presidential and vice presidential candidate is thoroughly vetted before they even run. To create and support a meme to delegitimize Obama's citizenship strikes at the heat of what is wrong with America. RACISM.
It not only insults President Obama and his family but it insults the citizenship of every African American. Its not all bad though because the backlash has motivated even more Blacks to come out in support of Obama who might have supported him but would have stayed home, now they will vote.
A diseased, entitled mind would not even consider how insulting it is to treat Americas FIRST Black President in such a disrespectful manner considering that he went through the same vetting process as every candidate before him.
Its been a running joke for five years and a knife in th thigh of ever African American for five years.
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Remember when the schools started having students rat their parents out? Video Reveals Jade Helm Plans For Children
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RT @Uniquecorn91: Watching @liannelahavas again at #bbcglasto I just think she's so slept on man. I can't wait to see her live!
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The In Loving Memory Funeral Program Template 005 is great for any memorial or funeral event. In this package you'll find 2 Photoshop files. All text and graphics in the files are editable, color coded and simple to edit. The files also contain 5 one-click color options, but endless colors are possible. http://goo.gl/eP4HT
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Adrenal Fatigue Center
Empowering Sufferers Since 2001
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For fast reading, scan through the topic headings in BOLD BLACK, important conclusions in BOLD BLUE, and "Must Know" in BOLD RED. To jump to specific sections in this article, click on the respective LINKS in the Table of Contents.
Information presented here is for general educational purposes only. Each one of us is biochemically and metabolically different. If you have a specific health concern and wish my personalized nutritional recommendation, write to me by clicking here.
Acrylamide, used to produce plastics and dyes and to purify drinking water, has been shown to be carcinogenic in animal experiments and is suspected of causing cancer among people exposed to high levels for long periods. Although traces of it have been found in water, its possible presence at high levels in basic foods came as a shock. A Swedish study, published in April 2002, sounded the first alarm that some starch-based foods cooked at high temperatures contained acrylamide. Subsequent studies in Norway, Britain, Switzerland and the United States basically backed up the findings of Sweden's National Food Administration. The U.S. findings agreed with European findings that French fries had the highest levels of acrylamide. Potato and corn chips also had high levels.
In addition to the toxin, French fries and processed food, especially those that are deep fried, contain large quantity of hydrogenated oil (also called trans-fat) that has been shown to be carcinogenic.
For a detail report prepared
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About The Author
Michael Lam, M.D., M.P.H., A.B.A.A.M., is a western trained physician specializing in nutritional and anti-aging medicine. Dr. Lam received his Bachelor of Science degree from Oregon State University, and his Doctor of Medicine degree from the Loma Linda University School of Medicine in California. He also holds a Master's degree in Public Health. He is board certified by the American Board of Anti-Aging Medicine where he has also served as a board examiner. Dr. Lam is a pioneer in using nontoxic, natural compounds to promote the healing of many age-related degenerative conditions. He utilizes optimum blends of nutritional supplementation that manipulate food, vitamins, natural hormones, herbs, enzymes, and minerals into specific protocols to rejuvenate cellular function.
Dr. Lam was first to coin the term, ovarian-adrenal-thyroid (OAT) hormone axis, and to describe its imbalances. He was first to scientifically tie in Adrenal Fatigue Syndrome (AFS) as part of the overall neuroendocrine stress response continuum of the body. He systematized the clinical significance and coined the various phases of Adrenal Exhaustion. He has written five books: Adrenal Fatigue Syndrome - Reclaim Your Energy and Vitality with Clinically Proven Natural Programs, The Five Proven Secrets to Longevity, Beating Cancer with Natural Medicine (Free PDF version), How to Stay Young and Live Longer, and Estrogen Dominance. In 2001, Dr. Lam established www.DrLam.com as a free, educational website on evidence-based alternative medicine for the public and for health professionals. It featured the world's most comprehensive library on AFS. Provided free as a public service, he has answered countless questions through the website on alternative health and AFS. His personal, telephone-based nutritional coaching services have enabled many around the world to regain control of their health using natural therapies.
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