Cluster Lensing of QSOs as a Probe of LCDM and Dark Energy Cosmologies by Lopes, A, Miller, L

“…We find that wide-separation lensed QSOs can measure sigma_8 and Omega_M in an equivalent manner to other methods such as cluster abundance studies and cosmic shear measurements. …”

Experimental and clinical study of the efficacy of medicines containing omega-3 and 6 polyunsaturated fatty acids, in the treatment of inflammatory skin diseases by Svetlana V. Grebennikova, Yuriy S. Maklyakov

“…After trying various treatment options with using Omegaven, histopathological examinations of 18 fragments of affected skin of white rats with cross sections stained with hematoxylin–eosin and pikrofuxin by Van Gieson’s method. …”
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Signalementen 2010/4 by - Redactiebureau

“…Omgaan met de gevolgen van dementie: het psychosociale perspectief …”
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The 2dF-SDSS LRG and QSO Survey: QSO clustering and the L-z degeneracy by Angela, J, Shanks, T, Croom, S, Weilbacher, P, Brunner, R, Couch, W, Miller, L, Myers, A, Nichol, R, Pimbblet, K, Propris, R, Richards, G, Ross, N, Schneider, D, Wake, D

“…By fitting the z-space correlation function and lifting the degeneracy between beta and Omega_m_0 by using linear theory predictions, we obtain beta(z=1.4) = 0.60+-0.12 and Omega_m_0=0.25+-0.08, implying a value for the QSO bias, b(z=1.4)=1.5+-0.2. …”

Cosmological weak lensing with the HST GEMS survey by Heymans, C, Brown, M, Barden, M, Caldwell, J, Jahnke, K, Peng, C, Rix, H, Taylor, A, Beckwith, S, Bell, E, Borch, A, Haeussler, B, Jogee, S, McIntosh, D, Meisenheimer, K, Sanchez, S, Somerville, R, Wisotzki, L, Wolf, C

“…We find sigma_8(Omega_m/0.3)^{0.65}=0.68 +/- 0.13 where the 1sigma error includes both our uncertainty on the median redshift of the survey and sampling variance. …”

CFHTLenS tomographic weak lensing: Quantifying accurate redshift distributions by Benjamin, J, Waerbeke, L, Heymans, C, Kilbinger, M, Erben, T, Hildebrandt, H, Hoekstra, H, Kitching, T, Mellier, Y, Miller, L, Rowe, B, Schrabback, T, Simpson, F, Coupon, J, Fu, L, Harnois-Déraps, J, Hudson, M, Kuijken, K, Semboloni, E, Vafaei, S, Velander, M

“…Combining our results with the above cosmological probes, we find Omega_m=0.2762 \pm 0.0074 and sigma_8=0.802 \pm 0.013.…”

The 2dF QSO Redshift Survey - X. Lensing of Background QSOs by Galaxy Groups by Myers, A, Outram, P, Shanks, T, Boyle, B, Croom, S, Loaring, N, Miller, L, Smith, R

“…Regardless of whether we utilise a SIS or NFW dark matter profile, our model favours more mass in groups than accounted for in a universe with density parameter Omega_m = 0.3. Detailed simulations and galaxy group redshifts will significantly reduce the current systematic uncertainties in these $\Omega_m$ estimates. …”

Through Livingstone’s eyes: Perspectives on water in nineteenth-century Southern Africa (1849-56) by J.W.N. Tempelhoff

“…Livingstone se waarnemings werp waardevolle lig oor die wyse waarop inheemse gemeenskappe met die wateromgewing omgegaan het. Ook is daar aanduidings van die wyse waarop hulle die beskikbare waterbronne bestuur het. …”
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Statistical Power Law due to Reservoir Fluctuations and the Universal Thermostat Independence Principle by Tamás Sándor Biró, Péter Ván, Gergely Gábor Barnaföldi, Károly Ürmössy

“…Certain fluctuations in particle number, \(n\), at fixed total energy, \(E\), lead exactly to a cut-power law distribution in the one-particle energy, \(\omega\), via the induced fluctuations in the phase-space volume ratio, \(\Omega_n(E-\omega)/\Omega_n(E)=(1-\omega/E)^n\). The only parameters are \(1/T=\langle \beta \rangle=\langle n \rangle/E\) and \(q=1-1/\langle n \rangle + \Delta n^2/\langle n \rangle^2\). …”
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Evidence for the accelerated expansion of the Universe from weak lensing tomography with COSMOS by Schrabback, T, Hartlap, J, Joachimi, B, Kilbinger, M, Simon, P, Benabed, K, Bradač, M, Eifler, T, Erben, T, Fassnacht, C, High, F, Hilbert, S, Hildebrandt, H, Hoekstra, H, Kuijken, K, Marshall, P, Mellier, Y, Morganson, E, Schneider, P, Semboloni, E, Waerbeke, L, Velander, M

“…For a flat LCDM cosmology, we measure sigma_8(Omega_m/0.3)^0.51=0.75+-0.08 from lensing, in perfect agreement with WMAP-5, yielding joint constraints Omega_m=0.266+0.025-0.023, sigma_8=0.802+0.028-0.029 (all 68% conf.). …”

Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology by Spergel, D, Bean, R, Doré, O, Nolta, MR, Bennett, C, Dunkley, J, Hinshaw, G, Jarosik, N, Komatsu, E, Page, L, Peiris, H, Verde, L, Halpern, M, Hill, R, Kogut, A, Limon, M, Meyer, S, Odegard, N, Tucker, G, Weiland, J, Wollack, E, Wright, E

“…Using WMAP data only, the best fit values for cosmological parameters for the power-law flat LCDM model are (Omega_m h^2, Omega_b h^2, h, n_s, tau, sigma_8) = 0.1277+0.0080-0.0079, 0.02229+-0.00073, 0.732+0.031-0.032, 0.958+-0.016, 0.089+-0.030, 0.761+0.049-0.048). …”

Profielen van mantelzorgers van naasten met dementie by Henk Kraijo

“… Doel Onderzoeken hoe mantelzorgers hun persoonlijke mantelzorgsituatie ervaren, welke behoeften zij hebben en met welke dilemma’s zij moeten omgaan. Methode Om profielen van mantelzorgers te ontdekken gebruikten wij de Q-methodologie. …”
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Atypical presentation of pallister–Hall syndrome with central precious puberty by Hala Gasim Omer, Amal Ali Alhakami, Malak Ali Alghamdi, Reem Abdullah Al Khalifah

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(E)-3-(4-Fluorophenyl)-1-[1-(4-fluorophenyl)-5-methyl-1H-1,2,3-triazol-4-yl]prop-2-en-1-one by Gamal A. El-Hiti, Bakr F. Abdel-Wahab, Mohammad Hayal Alotaibi, Amany S. Hegazy, Benson M. Kariuki

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Adjunctive Use of Statins for COVID-19 by Mike Sathekge, Geert Byttebier, Bart De Spiegeleer, Bo Saxberg, Veronica Ueckermann, Luc Belmans, Myriam Alexander, David Fedson

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Een multidisciplinaire benadering voor een adequate aanpak van probleemgedrag bij dementie by Henriëtte Ettema

“… Probleemgedrag bij dementie komt voor bij vrijwel alle verpleeghuispatiënten in een of meerdere vormen. Het omgaan met probleemgedrag vraagt om medicamenteuze en psychosociale interventies. …”
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Slaan uit macht en onmacht. Mannen leren in groepswerk praten over het geweld en hun relaties met vrouwen en kinderen by Sietske Dijkstra

“…Meer specifiek wilden we weten hoe ze omgaan met het feit dat veel van deze mishandelende mannen vaders zijn. …”
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3D Cosmic Shear: Cosmology from CFHTLenS by Kitching, T, Heavens, A, Alsing, J, Erben, T, Heymans, C, Hildebrandt, H, Hoekstra, H, Jaffe, A, Kiessling, A, Mellier, Y, Miller, L, Waerbeke, L, Benjamin, J, Coupon, J, Fu, L, Hudson, M, Kilbinger, M, Kuijken, K, Rowe, B, Schrabback, T, Semboloni, E, Velander, M

“…We use 3D cosmic shear to constrain cosmologies with parameters OmegaM, OmegaB, sigma8, h, ns, w0, wa. For a non-evolving dark energy equation of state, and assuming a flat cosmology, lensing combined with WMAP7 results in h=0.78+/-0.12, OmegaM=0.252+/-0.079, sigma8=0.88+/-0.23 and w=-1.16+/-0.38 using only scales k<=1.5h/Mpc. …”

The mass of radio galaxies from low to high redshift by Jarvis, M, Rawlings, S, Eales, S, Blundell, K, Willott, C

“…In a spatially flat universe with a cosmological constant (Omega_M=0.3 and Omega_Lambda=0.7), the most luminous radio sources appear to be associated with galaxies with a luminosity distribution with a high mean (~5L*), and a low dispersion (~0.5 mag) which formed their stars at epochs corresponding to z >~ 2.5.…”

Weak gravitational lensing and intrinsic galaxy alignments by Heymans, C

“…When marginalising over the observationally constrained intrinsic alignment signal, the amplitude of the matter power spectrum sigma_8 is reduced by ~0.03 to sigma_8(Omega_m / 0.27)^{0.6} = 0.71 pm 0.11, where Omega_m is the matter density parameter.…”