2,069 results on '"Hennig C."'
Search Results
2. Galaxies in X-ray Selected Clusters and Groups in Dark Energy Survey Data II: Hierarchical Bayesian Modeling of the Red-Sequence Galaxy Luminosity Function
- Author
-
Zhang, Y., Miller, C. J., Rooney, P., Bermeo, A., Romer, A. K., cervantes, C. Vergara, Rykoff, E. S., Hennig, C., Das, R., Mckay, T., Song, J., Wilcox, H., Bacon, D., Bridle, S. L., Collins, C., Conselice, C., Hilton, M., Hoyle, B., Kay, S., Liddle, A. R., Mann, R. G., Mehrtens, N., Mayers, J., Nichol, R. C., Sahlen, M., Stott, J., Viana, P. T. P., Wechsler, R. H., Abbott, T., Abdalla, F. B., Allam, S., Benoit-levy, A., Brooks, D., Buckley-geer, E., Burke, D. L., rosell, A. Carnero, kind, M. Carrasco, Carretero, J., Castander, F. J., Crocce, M., Cunha, C. E., Dandrea, C. B., Da costa, L. N., Diehl, H. T., Dietrich, J. P., Eifler, T. F., Flaugher, B., Fosalba, P., Garcia-bellido, J., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Honscheid, K., James, D. J., Jeltema, T., Kuehn, K., Kuropatkin, N., Lima, M., Lin, H., Maia, M. A. G., March, M., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Ogando, R. L. C., Plazas, A. A., Sanchez, E., Schubnell, M., Sevilla-noarbe, I., Smith, M., Soares-santos, M., Sobreira, F., Suchyta, E., Swanson, M. E. C., Tarle, G., and Walker, A. R.
- Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics ,Astrophysics - Astrophysics of Galaxies - Abstract
Using $\sim 100$ X-ray selected clusters in the Dark Energy Survey Science Verification data, we constrain the luminosity function (LF) of cluster red sequence galaxies as a function of redshift. This is the first homogeneous optical/X-ray sample large enough to constrain the evolution of the luminosity function simultaneously in redshift ($0.1
- Published
- 2017
3. Status of and expectations for flexible bioenergy to support resource efficiency and to accelerate the energy transition
- Author
-
Schipfer, F., Mäki, E., Schmieder, U., Lange, N., Schildhauer, T., Hennig, C., and Thrän, D.
- Published
- 2022
- Full Text
- View/download PDF
4. Galaxy Populations in Massive Galaxy Clusters to z=1.1: Color Distribution, Concentration, Halo Occupation Number and Red Sequence Fraction
- Author
-
Hennig, C., Mohr, J. J., Zenteno, A., Desai, S., Dietrich, J. P., Bocquet, S., Strazzullo, V., Saro, A., Abbott, T. M. C., Abdalla, F. B., Bayliss, M., Benoit-Levy, A., Bernstein, R. A., Bertin, E., Brooks, D., Capasso, R., Capozzi, D., Carnero, A., Kind, M. Carrasco, Carretero, J., Chiu, I., D'Andrea, C. B., daCosta, L. N., Diehl, H. T., Doel, P., Eifler, T. F., Evrard, A. E., Fausti-Neto, A., Fosalba, P., Frieman, J., Gangkofner, C., Gonzalez, A., Gruen, D., Gruendl, R. A., Gupta, N., Gutierrez, G., Honscheid, K., Hlavacek-Larrondo, J., James, D. J., Kuehn, K., Kuropatkin, N., Lahav, O., March, M., Marshall, J. L., Martini, P., McDonald, M., Melchior, P., Miller, C. J., Miquel, R., Neilsen, E., Nord, B., Ogando, R., Plazas, A. A., Reichardt, C., Romer, A. K., Rozo, E., Rykoff, E. S., Sanchez, E., Santiago, B., Schubnell, M., Sevilla-Noarbe, I., Smith, R. C., Soares-Santos, M., Sobreira, F., Stalder, B., Stanford, S. A., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., Vikram, V., Walker, A. R., and Zhang, Y.
- Subjects
Astrophysics - Astrophysics of Galaxies ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We study the galaxy populations in 74 Sunyaev Zeldovich Effect (SZE) selected clusters from the South Pole Telescope (SPT) survey that have been imaged in the science verification phase of the Dark Energy Survey (DES). The sample extends up to $z\sim 1.1$ with $4 \times 10^{14} M_{\odot}\le M_{200}\le 3\times 10^{15} M_{\odot}$. Using the band containing the 4000~\AA\ break and its redward neighbor, we study the color-magnitude distributions of cluster galaxies to $\sim m_*+2$, finding: (1) the intrinsic rest frame $g-r$ color width of the red sequence (RS) population is $\sim$0.03 out to $z\sim0.85$ with a preference for an increase to $\sim0.07$ at $z=1$ and (2) the prominence of the RS declines beyond $z\sim0.6$. The spatial distribution of cluster galaxies is well described by the NFW profile out to $4R_{200}$ with a concentration of $c_{\mathrm{g}} = 3.59^{+0.20}_{-0.18}$, $5.37^{+0.27}_{-0.24}$ and $1.38^{+0.21}_{-0.19}$ for the full, the RS and the blue non-RS populations, respectively, but with $\sim40$\% to 55\% cluster to cluster variation and no statistically significant redshift or mass trends. The number of galaxies within the virial region $N_{200}$ exhibits a mass trend indicating that the number of galaxies per unit total mass is lower in the most massive clusters, and shows no significant redshift trend. The red sequence (RS) fraction within $R_{200}$ is $(68\pm3)$\% at $z=0.46$, varies from $\sim$55\% at $z=1$ to $\sim$80\% at $z=0.1$, and exhibits intrinsic variation among clusters of $\sim14$\%. We discuss a model that suggests the observed redshift trend in RS fraction favors a transformation timescale for infalling field galaxies to become RS galaxies of 2 to 3~Gyr., Comment: 22 pages, 14 figures, submitted to MNRAS
- Published
- 2016
- Full Text
- View/download PDF
5. Detection of Enhancement in Number Densities of Background Galaxies due to Magnification by Massive Galaxy Clusters
- Author
-
Chiu, I., Dietrich, J. P., Mohr, J., Applegate, D. E., Benson, B. A., Bleem, L. E., Bayliss, M. B., Bocquet, S., Carlstrom, J. E., Capasso, R., Desai, S., Gangkofner, C., Gonzalez, A. H., Gupta, N., Hennig, C., Hoekstra, H., von der Linden, A., Liu, J., McDonald, M., Reichardt, C. L., Saro, A., Schrabback, T., Strazzullo, V., Stubbs, C. W., and Zenteno, A.
- Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We present a detection of the enhancement in the number densities of background galaxies induced from lensing magnification and use it to test the Sunyaev-Zel'dovich effect (SZE) inferred masses in a sample of 19 galaxy clusters with median redshift $z\simeq0.42$ selected from the South Pole Telescope SPT-SZ survey. Two background galaxy populations are selected for this study through their photometric colours; they have median redshifts ${z}_{\mathrm{median}}\simeq0.9$ (low-$z$ background) and ${z}_{\mathrm{median}}\simeq1.8$ (high-$z$ background). Stacking these populations, we detect the magnification bias effect at $3.3\sigma$ and $1.3\sigma$ for the low- and high-$z$ backgrounds, respectively. We fit NFW models simultaneously to all observed magnification bias profiles to estimate the multiplicative factor $\eta$ that describes the ratio of the weak lensing mass to the mass inferred from the SZE observable-mass relation. We further quantify systematic uncertainties in $\eta$ resulting from the photometric noise and bias, the cluster galaxy contamination and the estimations of the background properties. The resulting $\eta$ for the combined background populations with $1\sigma$ uncertainties is $0.83\pm0.24\mathrm{(stat)}\pm0.074\mathrm{(sys)}$, indicating good consistency between the lensing and the SZE-inferred masses. We use our best-fit $\eta$ to predict the weak lensing shear profiles and compare these predictions with observations, showing agreement between the magnification and shear mass constraints. This work demonstrates the promise of using the magnification as a complementary method to estimate cluster masses in large surveys., Comment: 16 pages, 10 figures, accepted for publication in MNRAS
- Published
- 2015
- Full Text
- View/download PDF
6. Constraints on the Richness-Mass Relation and the Optical-SZE Positional Offset Distribution for SZE-Selected Clusters
- Author
-
Saro, A., Bocquet, S., Rozo, E., Benson, B. A., Mohr, J., Rykoff, E. S., Soares-Santos, M., Bleem, L., Dodelson, S., Melchior, P., Sobreira, F., Upadhyay, V., Weller, J., Abbott, T., Abdalla, F. B., Allam, S., Armstrong, R., Banerji, M., Bauer, A. H., Bayliss, M., Benoit-Levy, A., Bernstein, G. M., Bertin, E., Brodwin, M., Brooks, D., Buckley-Geer, E., Burke, D. L., Carlstrom, J. E., Capasso, R., Capozzi, D., Rosell, A. Carnero, Kind, M. Carrasco, Chiu, I., Covarrubias, R., Crawford, T. M., Crocce, M., D'Andrea, C. B., da Costa, L. N., DePoy, D. L., Desai, S., de Haan, T., Diehl, H. T., Dietrich, J. P., Doel, P., Cunha, C. E, Eifler, T. F., Evrard, A. E., Neto, A. Fausti, Fernandez, E., Flaugher, B., Fosalba, P., Frieman, J., Gangkofner, C., Gaztanaga, E., Gerdes, D., Gruen, D., Gruendl, R. A., Gupta, N., Hennig, C., Holzapfel, W. L., Honscheid, K., Jain, B., James, D., Kuehn, K., Kuropatkin, N., Lahav, O., Li, T. S., Lin, H., Maia, M. A. G., March, M., Marshall, J. L., Martini, Paul, McDonald, M., Miller, C. J., Miquel, R., Nord, B., Ogando, R., Plazas, A. A., Reichardt, C. L., Romer, A. K., Roodman, A., Sako, M., Sanchez, E., Schubnell, M., Sevilla, I., Smith, R. C., Stalder, B., Stark, A. A., Strazzullo, V., Suchyta, E., Swanson, M. E. C., Tarle, G., Thaler, J., Thomas, D., Tucker, D., Vikram, V., von der Linden, A., Walker, A. R., Wechsler, R. H., Wester, W., Zenteno, A., and Ziegler, K. E.
- Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We cross-match galaxy cluster candidates selected via their Sunyaev-Zel'dovich effect (SZE) signatures in 129.1 deg$^2$ of the South Pole Telescope 2500d SPT-SZ survey with optically identified clusters selected from the Dark Energy Survey (DES) science verification data. We identify 25 clusters between $0.1\lesssim z\lesssim 0.8$ in the union of the SPT-SZ and redMaPPer (RM) samples. RM is an optical cluster finding algorithm that also returns a richness estimate for each cluster. We model the richness $\lambda$-mass relation with the following function $\langle\ln\lambda|M_{500}\rangle\propto B_\lambda\ln M_{500}+C_\lambda\ln E(z)$ and use SPT-SZ cluster masses and RM richnesses $\lambda$ to constrain the parameters. We find $B_\lambda= 1.14^{+0.21}_{-0.18}$ and $C_\lambda=0.73^{+0.77}_{-0.75}$. The associated scatter in mass at fixed richness is $\sigma_{\ln M|\lambda} = 0.18^{+0.08}_{-0.05}$ at a characteristic richness $\lambda=70$. We demonstrate that our model provides an adequate description of the matched sample, showing that the fraction of SPT-SZ selected clusters with RM counterparts is consistent with expectations and that the fraction of RM selected clusters with SPT-SZ counterparts is in mild tension with expectation. We model the optical-SZE cluster positional offset distribution with the sum of two Gaussians, showing that it is consistent with a dominant, centrally peaked population and a sub-dominant population characterized by larger offsets. We also cross-match the RM catalog with SPT-SZ candidates below the official catalog threshold significance $\xi=4.5$, using the RM catalog to provide optical confirmation and redshifts for additional low-$\xi$ SPT-SZ candidates.In this way, we identify 15 additional clusters with $\xi\in [4,4.5]$ over the redshift regime explored by RM in the overlapping region between DES science verification data and the SPT-SZ survey., Comment: 15 pages, 8 Figures, submitted to MNRAS
- Published
- 2015
- Full Text
- View/download PDF
7. Galaxies in X-ray Selected Clusters and Groups in Dark Energy Survey Data I: Stellar Mass Growth of Bright Central Galaxies Since z~1.2
- Author
-
Zhang, Y., Miller, C., Mckay, T., Rooney, P., Evrard, A. E., Romer, A. K., Perfecto, R., Song, J., Desai, S., Mohr, J., Wilcox, H., Bermeo, A., Jeltema, T., Hollowood, D., Bacon, D., Capozzi, D., Collins, C., Das, R., Gerdes, D., Hennig, C., Hilton, M., Hoyle, B., Kay, S., Liddle, A., Mann, R. G., Mehrtens, N., Nichol, R. C., Papovich, C., Sahlén, M., Soares-Santos, M., Stott, J., Viana, P. T., Abbott, T., Abdalla, F. B., Banerji, M., Bauer, A. H., Benoit-Lévy, A., Bertin, E., Brooks, D., Buckley-Geer, E., Burke, D. L., Rosell, A. Carnero, Castander, F. J., Diehl, H. T., Doel, P., Cunha, C. E, Eifler, T. F., Neto, A. Fausti, Fernandez, E., Flaugher, B., Fosalba, P., Frieman, J., Gaztanaga, E., Gruen, D., Gruendl, R. A., Honscheid, K., James, D., Kuehn, K., Kuropatkin, N., Lahav, O., Maia, M. A. G., Makler, M., Marshall, J. L., Martini, Paul, Miquel, R., Ogando, R., Plazas, A. A., Roodman, A., Rykoff, E. S., Sako, M., Sanchez, E., Scarpine, V., Schubnell, M., Sevilla, I., Smith, R. C., Sobreira, F., Suchyta, E., Swanson, M. E. C., Tarle, G., Thaler, J., Tucker, D., Vikram, V., and Da Costa, L. N.
- Subjects
Astrophysics - Astrophysics of Galaxies ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
Using the science verification data of the Dark Energy Survey (DES) for a new sample of 106 X-Ray selected clusters and groups, we study the stellar mass growth of Bright Central Galaxies (BCGs) since redshift 1.2. Compared with the expectation in a semi-analytical model applied to the Millennium Simulation, the observed BCGs become under-massive/under-luminous with decreasing redshift. We incorporate the uncertainties associated with cluster mass, redshift, and BCG stellar mass measurements into analysis of a redshift-dependent BCG-cluster mass relation, $m_{*}\propto(\frac{M_{200}}{1.5\times 10^{14}M_{\odot}})^{0.24\pm 0.08}(1+z)^{-0.19\pm0.34}$, and compare the observed relation to the model prediction. We estimate the average growth rate since $z = 1.0$ for BCGs hosted by clusters of $M_{200, z}=10^{13.8}M_{\odot}$, at $z=1.0$: $m_{*, BCG}$ appears to have grown by $0.13\pm0.11$ dex, in tension at $\sim 2.5 \sigma$ significance level with the $0.40$ dex growth rate expected from the semi-analytic model. We show that the buildup of extended intra-cluster light after $z=1.0$ may alleviate this tension in BCG growth rates., Comment: Accepted to ApJ
- Published
- 2015
- Full Text
- View/download PDF
8. Baryon Content of Massive Galaxy Clusters (0.57 < z < 1.33)
- Author
-
Chiu, I., Mohr, J., Mcdonald, M., Bocquet, S., Ashby, M. L., Bayliss, M., Benson, B. A., Bleem, L. E., Brodwin, M., Desai, S., Dietrich, J. P., Forman, W. R., Gangkofner, C., Gonzalez, A. H., Hennig, C., Liu, J., Reichardt, C. L., Saro, A., Stalder, B., Stanford, S. A., Song, J., Schrabback, T., Suhada, R., Strazzullo, V., and Zenteno, A.
- Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We study the stellar, Brightest Cluster Galaxy (BCG) and intracluster medium (ICM) masses of 14 South Pole Telescope (SPT) selected galaxy clusters with median redshift $z=0.9$ and median mass $M_{500}=6\times10^{14}M_{\odot}$. We estimate stellar masses for each cluster and BCG using six photometric bands spanning the range from the ultraviolet to the near-infrared observed with the VLT, HST and Spitzer. The ICM masses are derived from Chandra and XMM-Newton X-ray observations, and the virial masses are derived from the SPT Sunyaev-Zel'dovich Effect signature. At $z=0.9$ the BCG mass $M_{\star}^{\textrm{BCG}}$ constitutes $0.12\pm0.01$% of the halo mass for a $6\times10^{14}M_{\odot}$ cluster, and this fraction falls as $M_{500}^{-0.58\pm0.07}$. The cluster stellar mass function has a characteristic mass $M_{0}=10^{11.0\pm0.1}M_{\odot}$, and the number of galaxies per unit mass in clusters is larger than in the field by a factor $1.65\pm0.2$. Both results are consistent with measurements on group scales and at lower redshift. We combine our SPT sample with previously published samples at low redshift that we correct to a common initial mass function and for systematic differences in virial masses. We then explore mass and redshift trends in the stellar fraction (fstar), the ICM fraction (fICM), the cold baryon fraction (fc) and the baryon fraction (fb). At a pivot mass of $6\times10^{14}M_{\odot}$ and redshift $z=0.9$, the characteristic values are fstar=$1.1\pm0.1$%, fICM=$9.6\pm0.5$%, fc=$10.4\pm1.2$% and fb=$10.7\pm0.6$%. These fractions all vary with cluster mass at high significance, indicating that higher mass clusters have lower fstar and fc and higher fICM and fb. When accounting for a 15% systematic virial mass uncertainty, there is no statistically significant redshift trend at fixed mass in these baryon fractions. (abridged), Comment: Accepted for publication in MNRAS
- Published
- 2014
- Full Text
- View/download PDF
9. A Measurement of Gravitational Lensing of the Cosmic Microwave Background by Galaxy Clusters Using Data from the South Pole Telescope
- Author
-
Baxter, E. J., Keisler, R., Dodelson, S., Aird, K. A., Allen, S. W., Ashby, M. L. N., Bautz, M., Bayliss, M., Benson, B. A., Bleem, L. E., Bocquet, S., Brodwin, M., Carlstrom, J. E., Chang, C. L., Chiu, I., Cho, H-M., Clocchiatti, A., Crawford, T. M., Crites, A. T., Desai, S., Dietrich, J. P., de Haan, T., Dobbs, M. A., Foley, R. J., Forman, W. R., George, E. M., Gladders, M. D., Gonzalez, A. H., Halverson, N. W., Harrington, N. L., Hennig, C., Hoekstra, H., Holder, G. P., Holzapfel, W. L., Hou, Z., Hrubes, J. D., Jones, C., Knox, L., Lee, A. T., Leitch, E. M., Liu, J., Lueker, M., Luong-Van, D., Mantz, A., Marrone, D. P., McDonald, M., McMahon, J. J., Meyer, S. S., Millea, M., Mocanu, L. M., Murray, S. S., Padin, S., Pryke, C., Reichardt, C. L., Rest, A., Ruhl, J. E., Saliwanchik, B. R., Saro, A., Sayre, J. T., Schaffer, K. K., Shirokoff, E., Song, J., Spieler, H. G., Stalder, B., Stanford, S. A., Staniszewski, Z., Stark, A. A., Story, K. T., van Engelen, A., Vanderlinde, K., Vieira, J. D., Vikhlinin, A., Williamson, R., Zahn, O., and Zenteno, A.
- Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
Clusters of galaxies are expected to gravitationally lens the cosmic microwave background (CMB) and thereby generate a distinct signal in the CMB on arcminute scales. Measurements of this effect can be used to constrain the masses of galaxy clusters with CMB data alone. Here we present a measurement of lensing of the CMB by galaxy clusters using data from the South Pole Telescope (SPT). We develop a maximum likelihood approach to extract the CMB cluster lensing signal and validate the method on mock data. We quantify the effects on our analysis of several potential sources of systematic error and find that they generally act to reduce the best-fit cluster mass. It is estimated that this bias to lower cluster mass is roughly $0.85\sigma$ in units of the statistical error bar, although this estimate should be viewed as an upper limit. We apply our maximum likelihood technique to 513 clusters selected via their SZ signatures in SPT data, and rule out the null hypothesis of no lensing at $3.1\sigma$. The lensing-derived mass estimate for the full cluster sample is consistent with that inferred from the SZ flux: $M_{200,\mathrm{lens}} = 0.83_{-0.37}^{+0.38}\, M_{200,\mathrm{SZ}}$ (68% C.L., statistical error only)., Comment: 14 pages, 3 figures. Published in ApJ. Replaced to match published version
- Published
- 2014
- Full Text
- View/download PDF
10. Galaxy Clusters Discovered via the Sunyaev-Zel'dovich Effect in the 2500-square-degree SPT-SZ survey
- Author
-
Bleem, L. E., Stalder, B., de Haan, T., Aird, K. A., Allen, S. W., Applegate, D. E., Ashby, M. L. N., Bautz, M., Bayliss, M., Benson, B. A., Bocquet, S., Brodwin, M., Carlstrom, J. E., Chang, C. L., Chiu, I., Cho, H. M., Clocchiatti, A., Crawford, T. M., Crites, A. T., Desai, S., Dietrich, J. P., Dobbs, M. A., Foley, R. J., Forman, W. R., George, E. M., Gladders, M. D., Gonzalez, A. H., Halverson, N. W., Hennig, C., Hoekstra, H., Holder, G. P., Holzapfel, W. L., Hrubes, J. D., Jones, C., Keisler, R., Knox, L., Lee, A. T., Leitch, E. M., Liu, J., Lueker, M., Luong-Van, D., Mantz, A., Marrone, D. P., McDonald, M., McMahon, J. J., Meyer, S. S., Mocanu, L., Mohr, J. J., Murray, S. S., Padin, S., Pryke, C., Reichardt, C. L., Rest, A., Ruel, J., Ruhl, J. E., Saliwanchik, B. R., Saro, A., Sayre, J. T., Schaffer, K. K., Schrabback, T., Shirokoff, E., Song, J., Spieler, H. G., Stanford, S. A., Staniszewski, Z., Stark, A. A., Story, K. T., Stubbs, C. W., Vanderlinde, K., Vieira, J. D., Vikhlinin, A., Williamson, R., Zahn, O., and Zenteno, A.
- Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We present a catalog of galaxy clusters selected via their Sunyaev-Zel'dovich (SZ) effect signature from 2500 deg$^2$ of South Pole Telescope (SPT) data. This work represents the complete sample of clusters detected at high significance in the 2500-square-degree SPT-SZ survey, which was completed in 2011. A total of 677 (409) cluster candidates are identified above a signal-to-noise threshold of $\xi$ =4.5 (5.0). Ground- and space-based optical and near-infrared (NIR) imaging confirms overdensities of similarly colored galaxies in the direction of 516 (or 76%) of the $\xi$>4.5 candidates and 387 (or 95%) of the $\xi$>5 candidates; the measured purity is consistent with expectations from simulations. Of these confirmed clusters, 415 were first identified in SPT data, including 251 new discoveries reported in this work. We estimate photometric redshifts for all candidates with identified optical and/or NIR counterparts; we additionally report redshifts derived from spectroscopic observations for 141 of these systems. The mass threshold of the catalog is roughly independent of redshift above $z$~0.25 leading to a sample of massive clusters that extends to high redshift. The median mass of the sample is $M_{\scriptsize 500c}(\rho_\mathrm{crit})$ ~ 3.5 x 10$^{14} M_\odot h^{-1}$, the median redshift is $z_{med}$ =0.55, and the highest-redshift systems are at $z$>1.4. The combination of large redshift extent, clean selection, and high typical mass makes this cluster sample of particular interest for cosmological analyses and studies of cluster formation and evolution., Comment: Minor changes to match accepted version; Associated data products available at http://pole.uchicago.edu/public/data/sptsz-clusters/index.html
- Published
- 2014
- Full Text
- View/download PDF
11. Analysis of Sunyaev-Zel'dovich Effect Mass-Observable Relations using South Pole Telescope Observations of an X-ray Selected Sample of Low Mass Galaxy Clusters and Groups
- Author
-
Liu, J., Mohr, J., Saro, A., Aird, K. A., Ashby, M. L. N., Bautz, M., Bayliss, M., Benson, B. A., Bleem, L. E., Bocquet, S., Brodwin, M., Carlstrom, J. E., Chang, C. L., Chiu, I., Cho, H. M., Clocchiatti, A., Crawford, T. M., Crites, A. T., de Haan, T., Desai, S., Dietrich, J. P., Dobbs, M. A., Foley, R. J., Gangkofner, D., George, E. M., Gladders, M. D., Gonzalez, A. H., Halverson, N. W., Hennig, C., Hlavacek-Larrondo, J., Holder, G. P., Holzapfel, W. L., Hrubes, J. D., Jones, C., Keisler, R., Lee, A. T., Leitch, E. M., Lueker, M., Luong-Van, D., McDonald, M., McMahon, J. J., Meyer, S. S., Mocanu, L., Murray, S. S., Padin, S., Pryke, C., Reichardt, C. L., Rest, A., Ruel, J., Ruhl, J. E., Saliwanchik, B. R., Sayre, J. T., Schaffer, K. K., Shirokoff, E., Spieler, H. G., Stalder, B., Staniszewski, Z., Stark, A. A., Story, K., Suhada, R., Vanderlinde, K., Vieira, J. D., Vikhlinin, A., Williamson, R., Zahn, O., and Zenteno, A.
- Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics ,Astrophysics - Astrophysics of Galaxies - Abstract
(Abridged) We use 95, 150, and 220GHz observations from the SPT to examine the SZE signatures of a sample of 46 X-ray selected groups and clusters drawn from ~6 deg^2 of the XMM-BCS. These systems extend to redshift z=1.02, have characteristic masses ~3x lower than clusters detected directly in the SPT data and probe the SZE signal to the lowest X-ray luminosities (>10^42 erg s^-1) yet. We develop an analysis tool that combines the SZE information for the full ensemble of X-ray-selected clusters. Using X-ray luminosity as a mass proxy, we extract selection-bias corrected constraints on the SZE significance- and Y_500-mass relations. The SZE significance- mass relation is in good agreement with an extrapolation of the relation obtained from high mass clusters. However, the fit to the Y_500-mass relation at low masses, while in good agreement with the extrapolation from high mass SPT clusters, is in tension at 2.8 sigma with the constraints from the Planck sample. We examine the tension with the Planck relation, discussing sample differences and biases that could contribute. We also present an analysis of the radio galaxy point source population in this ensemble of X-ray selected systems. We find 18 of our systems have 843 MHz SUMSS sources within 2 arcmin of the X-ray centre, and three of these are also detected at significance >4 by SPT. Of these three, two are associated with the group brightest cluster galaxies, and the third is likely an unassociated quasar candidate. We examine the impact of these point sources on our SZE scaling relation analyses and find no evidence of biases. We also examine the impact of dusty galaxies using constraints from the 220 GHz data. The stacked sample provides 2.8$\sigma$ significant evidence of dusty galaxy flux, which would correspond to an average underestimate of the SPT Y_500 signal that is (17+-9) per cent in this sample of low mass systems., Comment: 15 pages, 7 figures
- Published
- 2014
- Full Text
- View/download PDF
12. Optical Confirmation and Redshift Estimation of the Planck Cluster Candidates overlapping the Pan-STARRS Survey
- Author
-
Liu, J., Hennig, C., Desai, S., Hoyle, B., Koppenhoefer, J., Mohr, J. J., Paech, K., Burgett, W. S., Chambers, K. C., Cole, S., Draper, P. W., Kaiser, N., Metcalfe, N., Morgan, J. S., Price, P. A., Stubbs, C. W., Tonry, J. L., Wainscoat, R. J., and Waters, C.
- Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We report results of a study of Planck Sunyaev-Zel'dovich effect (SZE) selected galaxy cluster candidates using the Panoramic Survey Telescope & Rapid Response System (Pan-STARRS) imaging data. We first examine 150 Planck confirmed galaxy clusters with spectroscopic redshifts to test our algorithm for identifying optical counterparts and measuring their redshifts; our redshifts have a typical accuracy of $\sigma_{z/(1+z)} \sim 0.022$ for this sample. Using 60 random sky locations, we estimate that our chance of contamination through a random superposition is ~ 3 per cent. We then examine an additional 237 Planck galaxy cluster candidates that have no redshift in the source catalogue. Of these 237 unconfirmed cluster candidates we are able to confirm 60 galaxy clusters and measure their redshifts. A further 83 candidates are so heavily contaminated by stars due to their location near the Galactic plane that we do not attempt to identify counterparts. For the remaining 94 candidates we find no optical counterpart but use the depth of the Pan-STARRS1 data to estimate a redshift lower limit $z_{\text{lim}(10^{15})}$ beyond which we would not have expected to detect enough galaxies for confirmation. Scaling from the already published Planck sample, we expect that $\sim$12 of these unconfirmed candidates may be real clusters., Comment: 11 pages, 9 figures
- Published
- 2014
- Full Text
- View/download PDF
13. Mass Calibration and Cosmological Analysis of the SPT-SZ Galaxy Cluster Sample Using Velocity Dispersion $\sigma_v$ and X-ray $Y_\textrm{X}$ Measurements
- Author
-
Bocquet, S., Saro, A., Mohr, J. J., Aird, K. A., Ashby, M. L. N., Bautz, M., Bayliss, M., Bazin, G., Benson, B. A., Bleem, L. E., Brodwin, M., Carlstrom, J. E., Chang, C. L., Chiu, I., Cho, H. M., Clocchiatti, A., Crawford, T. M., Crites, A. T., Desai, S., de Haan, T., Dietrich, J. P., Dobbs, M. A., Foley, R. J., Forman, W. R., Gangkofner, D., George, E. M., Gladders, M. D., Gonzalez, A. H., Halverson, N. W., Hennig, C., Hlavacek-Larrondo, J., Holder, G. P., Holzapfel, W. L., Hrubes, J. D., Jones, C., Keisler, R., Knox, L., Lee, A. T., Leitch, E. M., Liu, J., Lueker, M., Luong-Van, D., Marrone, D. P., McDonald, M., McMahon, J. J., Meyer, S. S., Mocanu, L., Murray, S. S., Padin, S., Pryke, C., Reichardt, C. L., Rest, A., Ruel, J., Ruhl, J. E., Saliwanchik, B. R., Sayre, J. T., Schaffer, K. K., Shirokoff, E., Spieler, H. G., Stalder, B., Stanford, S. A., Staniszewski, Z., Stark, A. A., Story, K., Stubbs, C. W., Vanderlinde, K., Vieira, J. D., Vikhlinin, A., Williamson, R., Zahn, O., and Zenteno, A.
- Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We present a velocity dispersion-based mass calibration of the South Pole Telescope Sunyaev-Zel'dovich effect survey (SPT-SZ) galaxy cluster sample. Using a homogeneously selected sample of 100 cluster candidates from 720 deg2 of the survey along with 63 velocity dispersion ($\sigma_v$) and 16 X-ray Yx measurements of sample clusters, we simultaneously calibrate the mass-observable relation and constrain cosmological parameters. The calibrations using $\sigma_v$ and Yx are consistent at the $0.6\sigma$ level, with the $\sigma_v$ calibration preferring ~16% higher masses. We use the full cluster dataset to measure $\sigma_8(\Omega_ m/0.27)^{0.3}=0.809\pm0.036$. The SPT cluster abundance is lower than preferred by either the WMAP9 or Planck+WMAP9 polarization (WP) data, but assuming the sum of the neutrino masses is $\sum m_\nu=0.06$ eV, we find the datasets to be consistent at the 1.0$\sigma$ level for WMAP9 and 1.5$\sigma$ for Planck+WP. Allowing for larger $\sum m_\nu$ further reconciles the results. When we combine the cluster and Planck+WP datasets with BAO and SNIa, the preferred cluster masses are $1.9\sigma$ higher than the Yx calibration and $0.8\sigma$ higher than the $\sigma_v$ calibration. Given the scale of these shifts (~44% and ~23% in mass, respectively), we execute a goodness of fit test; it reveals no tension, indicating that the best-fit model provides an adequate description of the data. Using the multi-probe dataset, we measure $\Omega_ m=0.299\pm0.009$ and $\sigma_8=0.829\pm0.011$. Within a $\nu$CDM model we find $\sum m_\nu = 0.148\pm0.081$ eV. We present a consistency test of the cosmic growth rate. Allowing both the growth index $\gamma$ and the dark energy equation of state parameter $w$ to vary, we find $\gamma=0.73\pm0.28$ and $w=-1.007\pm0.065$, demonstrating that the expansion and the growth histories are consistent with a LCDM model ($\gamma=0.55; \,w=-1$)., Comment: Accepted by ApJ (v2 is accepted version); 17 pages, 6 figures
- Published
- 2014
- Full Text
- View/download PDF
14. Defining bioenergy system services to accelerate the integration of bioenergy into a low-carbon economy
- Author
-
Mäki, E., Hennig, C., Thrän, Daniela, Lange, N., Schildhauer, T., Schipfer, F., Mäki, E., Hennig, C., Thrän, Daniela, Lange, N., Schildhauer, T., and Schipfer, F.
- Abstract
The global energy system is in transition. It is attempting to reach net-zero greenhouse gas emissions by 2050. The systemic changes mean that the role of bioenergy will change. The potential of bioenergy to make a flexible contribution to the energy system is key for the achievement of global emission reduction ambitions and the functioning of the low-carbon energy system and economy. As the volume of sustainably available biomass resources is limited, defining the contributions from bioenergy to a low-carbon energy system and finding balances – and ideally synergies – between the different possible energy and climate system services that biomass can provide will be very important. The recognized system services include, among others, the flexible operation of bioenergy plants to integrate variable renewable energy sources and to provide negative carbon dioxide (CO2) emissions. Interest in flexible operation of bioenergy value chains, bioenergy with carbon capture and utilization as well as synergies with renewable hydrogen-based value chains has increased recently. The objective of this paper is to present a holistic definition of flexible bioenergy as a system service based on the work conducted in International Energy Agency (IEA) Bioenergy Technology Collaboration Programme's Task 44 Flexible Bioenergy and System Integration, and to provide some practical examples. The paper also presents the different bioenergy system services and considers their definitions and interactions, as this is important in energy system design. The definition of flexible bioenergy shows that the flexibility provision from bioenergy goes far beyond the traditional definition of providing short-term flexibility in the power sector. Indicators to demonstrate the value of services as well as further quantitative assessment of synergies and trade-offs are needed to valorize the different services from bioenergy and create viable business cases.
- Published
- 2024
15. Investigation of radiation damage in the monazite-type solid solution La1-xCexPO4
- Author
-
Lender, T., Murphy, G., (0000-0002-5445-2438) Bazarkina, E., Bukaemskiy, A., Gilson, S., Henkes, M., (0000-0001-6393-2778) Hennig, C., Kaspor, A., Marquardt, J., Nießen, J., Peters, L., Poonoosamy, J., Roßberg, A., Svitlyk, V., (0000-0003-4447-4542) Kvashnina, K., (0000-0002-9930-2329) Huittinen, N. M., Lender, T., Murphy, G., (0000-0002-5445-2438) Bazarkina, E., Bukaemskiy, A., Gilson, S., Henkes, M., (0000-0001-6393-2778) Hennig, C., Kaspor, A., Marquardt, J., Nießen, J., Peters, L., Poonoosamy, J., Roßberg, A., Svitlyk, V., (0000-0003-4447-4542) Kvashnina, K., and (0000-0002-9930-2329) Huittinen, N. M.
- Abstract
Crystalline materials such as monazite have been considered for the storage of radionuclides due to their apparent radiation stability. Understanding their structural chemical response to radiation damage is a key component of determining their suitability for this application. Herein, high resolution structural studies were performed on the monazite solid solution La1-CexPO4 (x = 0.25, 0.5, 0.75, 1) in order to understand the role of structural chemistry on irradiation stability. Ceramic samples were irradiated with 14MeV Au ions with 1014 ions/cm2 and 1015 ions/cm2 to simulate the recoil of daughter nuclei from the alpha decay of actinides. The extent of radiation damage was analysed in detail using scanning electron microscopy (SEM), Raman spectroscopy, grazing incidence X-ray diffraction (GI-XRD) and high-energy-resolution fluorescence detection extended X-ray absorption fine structure (HERFD-EXAFS) spectroscopy. SEM and Raman revealed extensive structural damage as well as the importance of grain boundary regions, which appear to impede the propagation of defects. Both radiation-induced amorphisation and recrystallisation were studied by grazing incidence X-ray diffraction, highlighting the exceptional ability of monazite to remain crystalline at high fluences throughout the solid solution. Both, diffraction and HERFD-EXAFS experiments show that while atomic disorder is increased in irradiated samples compared to pristine ceramics, the short-range order was found to be largely preserved, facilitating recrystallisation. Crucially, this is consistent for all investigated samples, despite the chemical disorder introduced in the solid solution.
- Published
- 2024
16. Microstructural Investigation of Au Ion-Irradiated Eu-Doped LaPO4 Ceramics and Single Crystals
- Author
-
Gilson, S., Svitlyk, V., Bukaemskiy, A. A., Niessen, J., Lender, T., Murphy, G. L., Henkes, M., (0000-0002-8896-7595) Lippold, H., Marquardt, J., Akhmadaliev, S., (0000-0001-6393-2778) Hennig, C., Winkler, B., Tonnesen, T., Peters, L., (0000-0003-2416-6438) Fischer, C., (0000-0002-9930-2329) Huittinen, N. M., Gilson, S., Svitlyk, V., Bukaemskiy, A. A., Niessen, J., Lender, T., Murphy, G. L., Henkes, M., (0000-0002-8896-7595) Lippold, H., Marquardt, J., Akhmadaliev, S., (0000-0001-6393-2778) Hennig, C., Winkler, B., Tonnesen, T., Peters, L., (0000-0003-2416-6438) Fischer, C., and (0000-0002-9930-2329) Huittinen, N. M.
- Abstract
To mimic radiation damage by recoiling nuclei following alpha-decay, ceramics and single crystals of LaPO4 monazite doped with Eu(III) were irradiated with 14 MeV Au5+ ions at three different fluences. The crystallinity, local coordination environments, and topography of the samples were probed using numerous methods including grazing-incidence X-ray diffraction (GIXRD), vertical scanning interferometry (VSI), scanning electron microscopy (SEM), Raman, and luminescence spectroscopy. GIXRD data collected from the irradiated regions of the ceramics revealed fluence dependent amorphization. A similar level of amorphization was detected for samples irradiated with 5×1013 ions/cm2 (fluence, F1) and 1×1014 ions/cm2 (F2), while a slightly lower contribution to the scattering signal from the amorphous part was obtained for the sample irradiated with the highest fluence of 1×1015 ions/cm2 (F3). VSI showed clear swelling of entire grains at the highest ion fluence, while more localized damage to grain boundaries was detected for ceramic samples irradiated at the lowest fluence. Single crystal specimens showed no pronounced topography changes following irradiation. SEM backscattered electron images revealed that the ceramic irradiated at the highest fluence exhibited topological features indicative of grain surface melting or softening and displacement of grains. Finally, Raman and luminescence data showed a different degree of disorder in polycrystalline vs. single crystal samples. While changes to PO4 stretching and bending vibrations could be observed in the ceramics, these changes were more subtle or not present in the single crystals. The opposite was observed when probing the local Ln-O environment using Eu(III) luminescence, where the larger changes in terms of an elongation of the Eu-O (or La-O) bond and an increasing relative disorder with increasing fluence were observed only for the single crystals. The dissimilar trends observed in irradiated single crystals and ce
- Published
- 2024
17. Probing the Long- and Short-Range Structural Chemistry in the C-Type Bixbyite Oxides Th0.40Nd0.48Ce0.12O1.76, Th0.47Nd0.43Ce0.10O1.785 and Th0.45Nd0.37Ce0.18O1.815 via Synchrotron X-ray Diffraction and Absorption Spectroscopy
- Author
-
Murphy, G. L., (0000-0002-5445-2438) Bazarkina, E., Svitlyk, V., Roßberg, A., Potts, S., (0000-0001-6393-2778) Hennig, C., Henkes, M., (0000-0003-4447-4542) Kvashnina, K., (0000-0002-9930-2329) Huittinen, N. M., Murphy, G. L., (0000-0002-5445-2438) Bazarkina, E., Svitlyk, V., Roßberg, A., Potts, S., (0000-0001-6393-2778) Hennig, C., Henkes, M., (0000-0003-4447-4542) Kvashnina, K., and (0000-0002-9930-2329) Huittinen, N. M.
- Abstract
The long- and short- range structural chemistry of the C-type bixbyite compounds Th0.40Nd0.48Ce0.12O1.76, Th0.47Nd0.43Ce0.10O1.785 and Th0.45Nd0.37Ce0.18O1.815 is systematically examined using synchrotron X-ray powder diffraction (S-PXRD), high energy resolution fluorescence detection X-ray absorption near edge (HERFD-XANES) and extended absorption fine structure spectroscopy (EXAFS) measurements supported by electronic structure calculations. S-PXRD measurements revealed the title compounds all form classical C-type bixbyite structures in space group Ia3 ̅ that have disordered cationic crystallographic sites with further observation of characteristic superlattice reflections corresponding to oxygen vacancies. Despite the occurrence of oxygen vacancies, HERFD-XANES measurements on the Ce L3-edge revealed that Ce incorporates as Ce+4 into the structures but involves significant local distortion akin to cluster behavior and loss of nearest-neighbors. In comparison, HERFD-XANES measurements on the Nd+3 L3-edge supported by electronic structure calculations reveal that Nd+3 adopts a local coordination environment similar to the long-range C-type structure whilst providing charge balancing for the formation of oxygen defects. Th L3-edge EXAFS analysis reveals shorter average Th-O distances in the title compounds in comparison to pristine ThO2 in addition to shorter Th-O and Th-Ce distances compared to Th-Th or Ce-Ce in corresponding F-type binary oxides (ThO2 and CeO2). These distances are further found to decrease with the increased Nd content of the structures despite simultaneous observation of the overall lattice structure progressively expanding. Linear combination calculations of the M-O bond lengths are used to explain these observations, where the role of oxygen defects, via Nd+3 incorporation, induces local bond contraction and enhanced Th+4 cation valence leading to the observed increased lattice expansion with progressive Nd+3 incorporation. Overall, the inves
- Published
- 2024
18. Grazing incidence synchrotron radiation diffraction studies on irradiated Ce-doped and pristine Y-stabilized ZrO2 at the Rossendorf Beamline
- Author
-
(0000-0001-5449-8009) Svitlyk, V., (0000-0001-6592-3971) Braga Ferreira Dos Santos, L., Niessen, J., Gilson, S., Marquardt, J., Findeisen, S., (0009-0008-5672-029X) Richter, S., Akhmadaliev, S., (0000-0002-9930-2329) Huittinen, N. M., (0000-0001-6393-2778) Hennig, C., (0000-0001-5449-8009) Svitlyk, V., (0000-0001-6592-3971) Braga Ferreira Dos Santos, L., Niessen, J., Gilson, S., Marquardt, J., Findeisen, S., (0009-0008-5672-029X) Richter, S., Akhmadaliev, S., (0000-0002-9930-2329) Huittinen, N. M., and (0000-0001-6393-2778) Hennig, C.
- Abstract
Ce-doped yttria-stabilized zirconia (YSZ) and pure YSZ phases were subjected to irradiation with 14 MeV Au ions. The irradiation studies were performed to simulate long-term structural and microstructural damage due to self-irradiation in YSZ phases hosting alpha-active radioactive species. It was found that both the Ce-doped YSZ and YSZ phases were rather tolerant to irradiation at high ion fluences and the bulk crystallinity was well preserved. Nevertheless, local microstrain increased in all the studied compounds after the irradiation, with the Ce-doped phases being less affected than pure YSZ. Doping with cerium ions increased the microstructural stability of YSZ phases through a possible reduction in the mobility of oxygen atoms, which limits the formation of structural defects. Doping of YSZ with tetravalent actinide elements is expected to have a similar effect. Thus, YSZ phases are promising for the safe long-term storage of radioactive elements. Using synchrotron radiation diffraction, measurements of the thin irradiated layers of the Ce-YSZ and YSZ samples were performed in grazing incidence (GI) mode. A corresponding module for measurements in GI mode was developed at ROBL and relevant technical details of sample alignment and data collection are also presented.
- Published
- 2024
19. Understanding the local structure of Eu3+- and Y3+-stabilized zirconia: insights from luminescence and X-ray absorption spectroscopic investigations
- Author
-
Eibl, M., Shaw, S., Prieur, D., Rossberg, A., Wilding, M. C., Hennig, C., Morris, K., Rothe, J., Stumpf, T., and Huittinen, N.
- Published
- 2020
- Full Text
- View/download PDF
20. Constraints on the CMB Temperature Evolution using Multi-Band Measurements of the Sunyaev Zel'dovich Effect with the South Pole Telescope
- Author
-
Saro, A., Liu, J., Mohr, J. J., Aird, K. A., Ashby, M. L. N., Bayliss, M., Benson, B. A., Bleem, L. E., Bocquet, S., Brodwin, M., Carlstrom, J. E., Chang, C. L., Chiu, I., Cho, H. M., Clocchiatti, A., Crawford, T. M., Crites, A. T., de Haan, T., Desai, S., Dietrich, J. P., Dobbs, M. A., Dolag, K., Dudley, J. P., Foley, R. J., Gangkofner, D., George, E. M., Gladders, M. D., Gonzalez, A. H., Halverson, N. W., Hennig, C., Holzapfel, W. L., Hrubes, J. D., Jones, C., Keisler, R., Lee, A. T., Leitch, E. M., Lueker, M., Luong-Van, D., Mantz, A., Marrone, D. P., McDonald, M., McMahon, J. J., Mehl, J., Meyer, S. S., Mocanu, L., Montroy, T. E., Murray, S. S., Nurgaliev, D., Padin, S., Patej, A., Pryke, C., Reichardt, C. L., Rest, A., Ruel, J., Ruhl, J. E., Saliwanchik, B. R., Sayre, J. T., Schaffer, K. K., Shirokoff, E., Spieler, H. G., Stalder, B., Staniszewski, Z., Stark, A. A., Story, K., van Engelen, A., Vanderlinde, K., Vieira, J. D., Vikhlinin, A., Williamson, R., Zahn, O., and Zenteno, A.
- Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
The adiabatic evolution of the temperature of the cosmic microwave background (CMB) is a key prediction of standard cosmology. We study deviations from the expected adiabatic evolution of the CMB temperature of the form $T(z) =T_0(1+z)^{1-\alpha}$ using measurements of the spectrum of the Sunyaev Zel'dovich Effect with the South Pole Telescope (SPT). We present a method for using the ratio of the Sunyaev Zel'dovich signal measured at 95 and 150 GHz in the SPT data to constrain the temperature of the CMB. We demonstrate that this approach provides unbiased results using mock observations of clusters from a new set of hydrodynamical simulations. We apply this method to a sample of 158 SPT-selected clusters, spanning the redshift range $0.05 < z < 1.35$, and measure $\alpha = 0.017^{+0.030}_{-0.028}$, consistent with the standard model prediction of $\alpha=0$. In combination with other published results, we constrain $\alpha = 0.011 \pm 0.016$, an improvement of $\sim 20\%$ over published constraints. This measurement also provides a strong constraint on the effective equation of state in models of decaying dark energy $w_\mathrm{eff} = -0.987^{+0.016}_{-0.017}$., Comment: Submitted to MNRAS Letters
- Published
- 2013
- Full Text
- View/download PDF
21. Prevention of overweight and obesity in a Norwegian public health care context: a mixed-methods study
- Author
-
Westergren, T., Fegran, L., Jørstad Antonsen, A., Timenes Mikkelsen, H., Hennig, C. B., and Stamnes Köpp, U. M.
- Published
- 2021
- Full Text
- View/download PDF
22. Compression of time-vectors in W7-X archived measurements
- Author
-
Krom, J.G., Daher, R., Bluhm, T., Dumke, S., Grahl, M., Grün, M., Hennig, C., Holtz, A., Laqua, H., Lewerentz, M., Riemann, H., Spring, A., and Werner, A.
- Published
- 2018
- Full Text
- View/download PDF
23. Häufigkeit und Dosis extraoraler Röntgenaufnahmen bei Kindern und Jugendlichen
- Author
-
Scherbaum, R, additional, Hennig, C L, additional, Schüler, I M, additional, Buschek, R, additional, Scheithauer, M, additional, and Mentzel, H J, additional
- Published
- 2023
- Full Text
- View/download PDF
24. Radiation Exposure and Frequency of Dental, Bitewing and Occlusal Radiographs in Children and Adolescents
- Author
-
Schüler, I M, additional, Hennig, C L, additional, Buschek, R, additional, Scherbaum, R, additional, Jacobs, C, additional, Scheithauer, M, additional, and Mentzel, H J, additional
- Published
- 2023
- Full Text
- View/download PDF
25. Archive WEB API: A web service for the experiment data archive of Wendelstein 7-X
- Author
-
Grahl, M., Bluhm, T., Grün, M., Hennig, C., Holtz, A., Krom, J.G., Kühner, G., Laqua, H., Lewerentz, M., Riemann, H., Spring, A., and Werner, A.
- Published
- 2017
- Full Text
- View/download PDF
26. Neptunium characterization in uranium dioxide fuel: Combining a XAFS and a thermodynamic approach
- Author
-
Chollet, M., Martin, P., Degueldre, C., Poonoosamy, J., Belin, R.C., and Hennig, C.
- Published
- 2016
- Full Text
- View/download PDF
27. Quantile-based classifiers
- Author
-
HENNIG, C. and VIROLI, C.
- Published
- 2016
28. Extreme multi-valence states in mixed actinide oxides
- Author
-
Epifano, E., Naji, M., Manara, D., Scheinost, A. C., Hennig, C., Lechelle, J., Konings, R. J. M., Guéneau, C., Prieur, D., Vitova, T., Dardenne, K., Rothe, J., and Martin, P. M.
- Published
- 2019
- Full Text
- View/download PDF
29. Luminescence spectroscopy and diffraction studies of zirconia solid phases containing cerium
- Author
-
(0000-0001-6592-3971) Braga Ferreira Dos Santos, L., Svitlyk, V., (0009-0008-5672-029X) Richter, S., (0000-0001-6393-2778) Hennig, C., (0000-0002-9930-2329) Huittinen, N. M., (0000-0001-6592-3971) Braga Ferreira Dos Santos, L., Svitlyk, V., (0009-0008-5672-029X) Richter, S., (0000-0001-6393-2778) Hennig, C., and (0000-0002-9930-2329) Huittinen, N. M.
- Abstract
Zirconia is largely studied because of its ability to incorporate lanthanides and actinides; this has been one of the strategies adopted to try to immobilize ions from High-Level Radioactive Waste (HLW). Furthermore, cerium is often used as a surrogate for plutonium due to its analogous chemical properties1. In this study, zirconia samples with different Ce concentrations were syntehsized via the co-precipitation route. A small amount of Eu as co-dopants was added during synthesis to enable luminescence spectroscopic analyses of the solids phases2. Six zirconia compositions doped with 15 to 80 mol%Ce were prepared. The phase composition was evaluated by site selective luminescence spectroscopy (ss-TRLFS) and Synchrotron Powder X-Ray Diffraction. The latter method showed, that more than one phase coexists in all samples with concentrations lower than 80 mol% Ce. The tetragonal phase is predominant until 30 mol% Ce-doping, and above this concentration, a metastable phase (t’’) starts becomes dominant. The phase transformation can also be deduced from the coordination environment of europium, showing a small band at 583 nm, characteristic for the monoclinic phase, and another one at around 581.1 nm for Eu incorporated in the tetragonal phase. The systematic shift of this signal to shorter wavelengths points toward a lengthening of the Eu-O bonds with increasing Ce concentration, as the unit cell becomes systematically larger. The excitation peaks are clearly broader for the samples with predominantly t’’-ZrO2, which points toward a less ordered environement. This is in agreement with the hypothesized displacement of oxygen atoms from ideal (cubic) crystallographic positions, in this metastable (transition) phase.
- Published
- 2023
30. Fundamental investigations of actinide immobilization by incorporation into solid phases relevant for final disposal
- Author
-
(0000-0002-9930-2329) Huittinen, N. M., (0000-0001-6592-3971) Braga Ferreira Dos Santos, L., Gilson, S., (0000-0001-6393-2778) Hennig, C., Lender, T., Marquardt, J., Murphy, G. L., Nießen, J., Peters, L., Richter, S., (0000-0001-5449-8009) Svitlyk, V., Tonnesen, T., Winkler, B., (0000-0002-9930-2329) Huittinen, N. M., (0000-0001-6592-3971) Braga Ferreira Dos Santos, L., Gilson, S., (0000-0001-6393-2778) Hennig, C., Lender, T., Marquardt, J., Murphy, G. L., Nießen, J., Peters, L., Richter, S., (0000-0001-5449-8009) Svitlyk, V., Tonnesen, T., and Winkler, B.
- Abstract
This contribution provides an overview of a current research network funded by the German Federal Ministry of Education and Research (BMBF), entitled “Fundamental investigations of actinide immobilization by incorporation into solid phases relevant for final disposal” – AcE. The AcE project aims at understanding the incorporation and immobilization of actinides (An) in crystalline, repository-relevant solid phases, such as zirconia (ZrO2) and UO2, but also in zircon (ZrSiO4), pyrochlores (Ln2Zr2O7) and orthophosphates of the monazite type (LnPO4), which may find use as host matrices for the immobilization and safe disposal of high-level waste streams. Recent studies by the AcE-project consortium, addressing the structure, properties, and the radiation tolerance of monazites and Zr(IV)-based solid phases containing actinides or their surrogates from the lanthanide series will be presented. Material synthesis strategies in the AcE project have aimed at generating single-phase solid solutions in the form of polycrystalline powders, dense ceramics, and single crystals. Structural studies using powder X-ray diffraction at ambient conditions, but also at high temperatures and pressures have been complemented with a wide range of microscopic and spectroscopic techniques to address differences between the host- and dopant environments in the solid matrices at ambient and extreme conditions. The radiation tolerance of the synthetic solid phases have been investigated by combining external heavy-ion irradiation of inactive Ln-doped materials and in situ self-irradiation of 241Am-doped Zr(IV)-phases with monoclinic, cubic defect fluorite and pyrochlore structures. The latter experiments have been conducted in joint efforts with the Joint Research Center in Karlsruhe within the ActUsLab programme.
- Published
- 2023
31. From molecular oxo-hydroxo Ce clusters to crystalline CeO2
- Author
-
Estevenon, P., Amidani, L., Bauters, S., Tamain, C., Bodensteiner, M., Meuer, F., Hennig, C., Dumas, T., Kvashnina, K., Estevenon, P., Amidani, L., Bauters, S., Tamain, C., Bodensteiner, M., Meuer, F., Hennig, C., Dumas, T., and Kvashnina, K.
- Abstract
Due to their applications in catalysis, energy storage or biomedicine, many studies report synthesis and characterizations of CeO2 NPs and intensively use X-ray sources for characterization. In this study, we report a comprehensive interpretation of X-ray measurements on CeO2 models with atomically resolved structure, namely oxo-hydroxo polynuclear Ce complexes. A set of Ce clusters with growing size (0.6 nm to 1.2 nm) and nuclearity (from 6 to 38 Ce atoms) were synthetized and characterized by single crystal XRD. The samples were then analyzed using HEXS and HERFD technics and compared to larger CeO2 NPs and bulk CeO2. Both spectroscopic methods reveal consistent trends as the particle grows or shrink from the set of molecular Ce-{n} clusters up to bulk CeO2. HEXS reveals a broadening in distribution for the short Ce-oxygen bonds for the small clusters. Concomitantly, the HERFD performed at the Ce LIII edge indicates a gradual splitting of the cerium 5d states as the particles become more CeO2 like. From the crystallographic determination of the clusters structure, atomically resolved Ce LIII edge simulation were undertaken. These simulations allow to isolate structural and electronic properties for individual Ce sites within clusters and evidence the great difference between surface and core Ce atoms. It also shows how a combination of simulations from different sites results in the accurate reproduction of the corresponding experimental data. This approach based on clusters atomic sites was then successfully extended to model larger CeO2 NPs Ce LIII edge HERFD spectra. By linking atomically resolved structures to nanoparticles and bulk material using crystallography, X-ray technics and simulation, this work extends the knowledge on cerium oxide nanomaterial and supports a better understanding and predictability of their crystalline and electronic structure
- Published
- 2023
32. Effect of Chain Length on Swelling Transitions of Brodie Graphite Oxide in Liquid 1-Alcohols
- Author
-
Iakunkov, A., Nordenström, A., Boulanger, N., Li, G., (0000-0001-6393-2778) Hennig, C., Jørgensen, M. R. V., Kantor, I., Talyzin, . A. V., Iakunkov, A., Nordenström, A., Boulanger, N., Li, G., (0000-0001-6393-2778) Hennig, C., Jørgensen, M. R. V., Kantor, I., and Talyzin, . A. V.
- Abstract
Swelling is the most fundamental property of graphite oxides (GO). Here, a structural study of Brodie graphite oxide (BGO) swelling in a set of long chain 1-alcohols (named C11 to C22 according to the number of carbons) performed using synchrotron radiation X-ray diffraction at elevated temperatures is reported. Even the longest of tested alcohols (C22) is found to intercalate BGO with enormous expansion of the interlayer distance from ≈6Å up to ≈63Å, the highest expansion of GO lattice ever reported. Swelling transitions from low temperature alpha-phase to high temperature beta-phase are found for BGO in all alcohols in the C11–C22 set. The transitions correspond to decrease of inter-layer distance correlating with the length of alcohol molecules, and change in their orientation from perpendicular to GO planes to layered parallel to GO (Type II transitions). These transitions are very different compared to BGO swelling transitions (Type I) found in smaller alcohols and related to insertion/de-insertion of additional layer of alcohol parallel to GO. Analysis of general trends in the whole set of 1-alcohols (C1 to C22) shows that the 1-alcohol chain length defines the type of swelling transition with Type I found for alcohols with C<10 and Type II for C>10.
- Published
- 2023
33. Deconvoluting Cr States in Cr-Doped UO2 Nuclear Fuels via Bulk and Single Crystal Spectroscopic Studies
- Author
-
(0000-0003-3239-9725) Murphy, G. L., (0000-0003-4669-0206) Gericke, R., Gilson, S., (0000-0002-5445-2438) Bazarkina, E., Roßberg, A., (0000-0002-9414-2936) Kaden, P., Thümmler, R., Klinkenberg, M., Henkes, M., Kegler, P., (0000-0001-5449-8009) Svitlyk, V., Marquardt, J., Lender, T., (0000-0001-6393-2778) Hennig, C., (0000-0003-4447-4542) Kvashnina, K., (0000-0002-9930-2329) Huittinen, N. M., (0000-0003-3239-9725) Murphy, G. L., (0000-0003-4669-0206) Gericke, R., Gilson, S., (0000-0002-5445-2438) Bazarkina, E., Roßberg, A., (0000-0002-9414-2936) Kaden, P., Thümmler, R., Klinkenberg, M., Henkes, M., Kegler, P., (0000-0001-5449-8009) Svitlyk, V., Marquardt, J., Lender, T., (0000-0001-6393-2778) Hennig, C., (0000-0003-4447-4542) Kvashnina, K., and (0000-0002-9930-2329) Huittinen, N. M.
- Abstract
Cr-doped UO2 is a leading accident tolerant nuclear fuel where the complexity of Cr chemical states in the bulk material has prevented acquisition of an unequivocal understanding of the redox chemistry and mechanism for incorporation of Cr in the UO2 matrix. To resolve this, we have used electron paramagnetic resonance, high energy resolution fluorescence detection X-ray absorption near energy structure and extended X-ray absorption fine structure spectroscopic measurements to examine Cr-doped UO2 single crystal grains and bulk material. Ambient condition measurements of the single crystal grains, which have been mechanically extracted from bulk material, indicated Cr is incorporated substitutionally for U+4 in the fluorite lattice as Cr+3 with formation of additional oxygen vacancies. Bulk material measurements reveal the complexity of Cr states, where metallic Cr (Cr0) and oxide related Cr+2 and Cr+32O3 were identified and attributed to grain boundary species and precipitates, with concurrent (Cr+3xU+41-x)O2-0.5x lattice matrix incorporation. The deconvolution of chemical states via crystal vs. powder measurements enables the understanding of discrepancies in literature whilst providing valuable direction for safe continued use of Cr-doped UO2 fuels for nuclear energy generation.
- Published
- 2023
34. Defining the value of bioenergy system services for accelerating the integration of bioenergy into a low-carbon economy
- Author
-
de Bari, I., Scarlat, N., Grassi, A., Mäki, E., Hennig, C., Thrän, Daniela, Lange, N., Schildhauer, T., Schipfer, F., de Bari, I., Scarlat, N., Grassi, A., Mäki, E., Hennig, C., Thrän, Daniela, Lange, N., Schildhauer, T., and Schipfer, F.
- Abstract
The strongly intended transition of global energy systems to reach net-zero GHG emissions by mid-century means that the role of bioenergy will change. The potential of bioenergy to contribute to the energy system in flexible modes is key for the fulfilment of global emission reduction ambitions and the functioning of the low-carbon energy system and economy. As sustainably available biomass resources are limited in volumes, finding balances - and ideally, synergies - between the different possible energy and climate system services will be highly important. Preliminary valorisation framework, developed by IEA Bioenergy TCP Task 44 Flexible Bioenergy and System Integration, presents considerations on system services, interactions and synergies between the services, and Key Performance Indicators (KPIs) to assess the value of system services.
- Published
- 2023
35. Data publication: Deconvoluting Cr States in Cr-Doped UO2 Nuclear Fuels via Bulk and Single Crystal Spectroscopic Studies
- Author
-
(0000-0003-3239-9725) Murphy, G. L., (0000-0003-4669-0206) Gericke, R., Gilson, S., (0000-0002-5445-2438) Bazarkina, E., Roßberg, A., (0000-0002-9414-2936) Kaden, P., Thümmler, R., Klinkenberg, M., Henkes, M., Kegler, P., (0000-0001-5449-8009) Svitlyk, V., Marquardt, J., Lender, T., (0000-0001-6393-2778) Hennig, C., (0000-0003-4447-4542) Kvashnina, K., (0000-0002-9930-2329) Huittinen, N. M., (0000-0003-3239-9725) Murphy, G. L., (0000-0003-4669-0206) Gericke, R., Gilson, S., (0000-0002-5445-2438) Bazarkina, E., Roßberg, A., (0000-0002-9414-2936) Kaden, P., Thümmler, R., Klinkenberg, M., Henkes, M., Kegler, P., (0000-0001-5449-8009) Svitlyk, V., Marquardt, J., Lender, T., (0000-0001-6393-2778) Hennig, C., (0000-0003-4447-4542) Kvashnina, K., and (0000-0002-9930-2329) Huittinen, N. M.
- Abstract
Experimental and fitted EPR data of Cr-UO2 single crystal grains, EXAFS data Cr-UO2 single crystal grain and powder with Cr redox standards, XANES data Cr-UO2 single crystal grain and powder with Cr redox standards
- Published
- 2023
36. Overview on flexible bioenergy options and implementation
- Author
-
Gabauer, C., Thrän, Daniela, Mäki, E., Lange, N., Hennig, C., Schmieder, U., Schildhauer, T., Kiel, J., Kroon, P., Schipfer, F., Philbrook, A., Andersson, K., Higa, C., Gölles, M., Gabauer, C., Thrän, Daniela, Mäki, E., Lange, N., Hennig, C., Schmieder, U., Schildhauer, T., Kiel, J., Kroon, P., Schipfer, F., Philbrook, A., Andersson, K., Higa, C., and Gölles, M.
- Published
- 2023
37. Fehldiagnose eines Morbus Wilson trotz positiver Genetik
- Author
-
Hermann, W., Hennig, C., and Hoffmann, J.
- Published
- 2018
- Full Text
- View/download PDF
38. Data publication: Deconvoluting Cr States in Cr-Doped UO2 Nuclear Fuels via Bulk and Single Crystal Spectroscopic Studies
- Author
-
Murphy, G. L., Gericke, R., Gilson, S., Bazarkina, E., Roßberg, A., Kaden, P., Thümmler, R., Klinkenberg, M., Henkes, M., Kegler, P., Svitlyk, V., Marquardt, J., Lender, T., Hennig, C., Kvashnina, K., and Huittinen, N. M.
- Subjects
EXAFS ,Cr-doped UO2 ,Nuclear Fuel ,Uranium ,EPR ,HERFD-XANES - Abstract
Experimental and fitted EPR data of Cr-UO2 single crystal grains, EXAFS data Cr-UO2 single crystal grain and powder with Cr redox standards, XANES data Cr-UO2 single crystal grain and powder with Cr redox standards
- Published
- 2023
- Full Text
- View/download PDF
39. Recent advances in the study of the UO2–PuO2 phase diagram at high temperatures
- Author
-
Böhler, R., Welland, M.J., Prieur, D., Cakir, P., Vitova, T., Pruessmann, T., Pidchenko, I., Hennig, C., Guéneau, C., Konings, R.J.M., and Manara, D.
- Published
- 2014
- Full Text
- View/download PDF
40. Dissolution and Isolation Robustness of Fixed Point Clusters
- Author
-
Hennig, C., Gaul, Wolfgang, editor, Bock, Hans-Hermann, editor, Imaizumi, Tadashi, editor, and Okada, Akinori, editor
- Published
- 2009
- Full Text
- View/download PDF
41. Immunization of rhesus macaques with Echinococcus multilocularis recombinant 14-3-3 antigen leads to specific antibody response
- Author
-
Lampe, Karen, Gottstein, B., Becker, T., Stahl-Hennig, C., Kaup, F.-J., and Mätz-Rensing, K.
- Published
- 2017
- Full Text
- View/download PDF
42. Characterization of uranium (VI) complexes formed by different bacteria relevant to uranium mining waste piles
- Author
-
Merroun, M., Hennig, C., Rossberg, A., Reich, T., Nicolai, R., Heise, K-H., Se-lenska-Pobell, S., Merkel, Broder J., editor, Planer-Friedrich, Britta, editor, and Wolkersdorfer, Christian, editor
- Published
- 2002
- Full Text
- View/download PDF
43. The Pathology of Experimental Poxvirus Infection in Common Marmosets (Callithrix jacchus): Further Characterization of a New Primate Model for Orthopoxvirus Infections
- Author
-
Mätz-Rensing, K., Stahl-Hennig, C., Kramski, M., Pauli, G., Ellerbrok, H., and Kaup, F.-J.
- Published
- 2012
- Full Text
- View/download PDF
44. n→π* charge transfer between an iodide anion and a quinoid ring
- Author
-
Molcanov, K., primary, Milašinović, V., additional, Vuković, V., additional, Krawczuk, A., additional, Hennig, C., additional, and Bodensteiner, M., additional
- Published
- 2022
- Full Text
- View/download PDF
45. Refinement of anomalous dispersion parameters
- Author
-
Meurer, F., primary, Dolomanov, O.V., additional, Hennig, C., additional, Peyerimhoff, N., additional, Kleemiss, F., additional, Puschmann, H., additional, and Bodensteiner, M., additional
- Published
- 2022
- Full Text
- View/download PDF
46. Models and Methods for Clusterwise Linear Regression
- Author
-
Hennig, C., Bock, H.-H., editor, Gaul, W., editor, Schader, M., editor, Gaul, Wolfgang, editor, and Locarek-Junge, Hermann, editor
- Published
- 1999
- Full Text
- View/download PDF
47. Clustering and Outlier Identification: Fixed Point Cluster Analysis
- Author
-
Hennig, C., Bock, H.-H., editor, Gaul, W., editor, Opitz, O., editor, Schader, M., editor, Rizzi, Alfredo, editor, Vichi, Maurizio, editor, and Bock, Hans-Hermann, editor
- Published
- 1998
- Full Text
- View/download PDF
48. Fixed Point Clusters and Their Relation to Stochastic Models
- Author
-
Hennig, C., Bock, H. H., editor, Opitz, O., editor, Schader, M., editor, Klar, Rüdiger, editor, and Opitz, Otto, editor
- Published
- 1997
- Full Text
- View/download PDF
49. Neutron-irradiated concrete: Structural characterisation and gamma dosimetry.
- Author
-
(0000-0002-6889-2135) Roode-Gutzmer, Q. I., (0000-0003-3241-3443) Barkleit, A., (0000-0002-9260-5052) Rachamin, R., (0000-0001-6393-2778) Hennig, C., Weiß, S., Paasch, S., Konheiser, J., Stumpf, T., (0000-0002-6889-2135) Roode-Gutzmer, Q. I., (0000-0003-3241-3443) Barkleit, A., (0000-0002-9260-5052) Rachamin, R., (0000-0001-6393-2778) Hennig, C., Weiß, S., Paasch, S., Konheiser, J., and Stumpf, T.
- Abstract
Increased reactivity of radiation-damaged quartz in the alkaline pore water of concrete and its role in radionuclide transport is a subject that is becoming increasingly important as nuclear power plants (NPPs) around the world reach end-of-life. Quartz contributes more than half the weight of most concretes and up to 40 % of the total radioactive waste volume associated with the dismantling of an NPP. The gamma-emitting radionuclides are the major contributors to the radiation dose rate in the concrete biological shield in the intermediate term after NPP shut-down. The appreciable activity and associated half-lives of these radionuclides pose a problem not only during the safe dismantling of NPPs, but also in terms of processing the concrete to reduce the active waste volume for final disposal in a repository. While thermal neutrons are captured by atomic nuclei according to their thermal neutron cross-sections, fast neutrons undergo collision cascades, which cause defects in the structure of materials. The concentration of defects accumulates as a function of neutron energy and fluence. The high covalency and the density of Si-O bonds in tectosilicates, primarily quartz, followed by feldspars, makes these minerals very susceptible to radiation damage. In this study, two inactive concrete powder samples were placed inside an instrumentation channel passing through the first biological shielding of an operating German NPP, respectively for a half- and a full fuel cycle. Using a plant-specific 3D-reactor model in conjunction with Monte Carlo neutron transport calculations, neutron fluences at the sample positions and the resulting gamma activities are calculated. We compare the measured and calculated activities of the gamma-emitting radionuclides Synchrotron X-ray powder diffractometry was used to examine structural changes on sub-nanoscale. The local structure of the silicate aggregate minerals was investigated by solid-state magic angle spinning nuclear magnetic r
- Published
- 2022
50. Experimental simulation of phase evolution in conditions of underground storage: from million years to one day
- Author
-
Svitlyk, V., Weiss, S., Hennig, C., Svitlyk, V., Weiss, S., and Hennig, C.
- Abstract
Long-living radiotoxic isotopes present in spent nuclear fuel (SNF) requires procedures of complete immobilization of these species. Incorporation of the corresponding elements on atomic level into robust host crystalline matrices is one way to secure SNF during long-term underground storage. Derivatives of zirconia, ZrO2, are promising materials for these applications since these phases are known to remain structurally stable in geological cycles of up to 109 years [1]. The candidate host matrix must provide a sufficient solubility limit for radiotoxic elements, which is studied initially. Afterwards, structural stability of these phases against irradiation and leaching are established in order to asses possible discharge of the incorporated radioactive elements over a long-time scale. In this work we studied systematically structural behaviour of ZrO2-based materials incorporated with Th4+ and Ce4+ under extreme conditions of temperature (T) and pressure (P) in order to simulate experimentally possible phase evolution in conditions of underground storage. In situ synchrotron radiation powder diffraction experiments under ambient and extreme conditions were performed at the HZDR ROBL BM20 beamline at ESRF, Grenoble, France [2]. It was found that cubic YSZ phases could dissolve 20% more of Th atoms compared to their tetragonal analogues. In situ T-dependent diffraction studies on radionuclide surrogate tetragonal and cubic Ce-YSZ series in a RT-1150 K range revealed excellent phase stabilities. No discharge of guest Ce4+ ions was observed. Nevertheless, application of external pressure on tetragonal Ce-YSZ phase induced transition towards a higher cubic symmetry around the P ~ 8.5 GPa. Remarkably, occupancy of Ce4+ remains stable throughout the transition. This together with T-dependent data indicates excellent affinity of guest Ce atoms with the YSZ structures. Thus, we suggest in situ studies under extreme conditions as a part of standard protocol to validate phas
- Published
- 2022
Catalog
Discovery Service for Jio Institute Digital Library
For full access to our library's resources, please sign in.