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1. Ballistic long bone fracture pattern: an experimental study

Author: Schwab, Nathalie, Jordana, Xavier, Monreal, Jordi, Garrido, Xavier, Soler, Joan, Vega, Manel, Brillas, Pedro, and Galtés, Ignasi
Published: 2024
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2. The Atacama Cosmology Telescope: High-resolution component-separated maps across one-third of the sky

Author: Coulton, William R., Madhavacheril, Mathew S., Duivenvoorden, Adriaan J., Hill, J. Colin, Abril-Cabezas, Irene, Ade, Peter A. R., Aiola, Simone, Alford, Tommy, Amiri, Mandana, Amodeo, Stefania, An, Rui, Atkins, Zachary, Austermann, Jason E., Battaglia, Nicholas, Battistelli, Elia Stefano, Beall, James A., Bean, Rachel, Beringue, Benjamin, Bhandarkar, Tanay, Biermann, Emily, Bolliet, Boris, Bond, J Richard, Cai, Hongbo, Calabrese, Erminia, Calafut, Victoria, Capalbo, Valentina, Carrero, Felipe, Chesmore, Grace E., Cho, Hsiao-mei, Choi, Steve K., Clark, Susan E., Rosado, Rodrigo Córdova, Cothard, Nicholas F., Coughlin, Kevin, Crowley, Kevin T., Devlin, Mark J., Dicker, Simon, Doze, Peter, Duell, Cody J., Duff, Shannon M., Dunkley, Jo, Dünner, Rolando, Fanfani, Valentina, Fankhanel, Max, Farren, Gerrit, Ferraro, Simone, Freundt, Rodrigo, Fuzia, Brittany, Gallardo, Patricio A., Garrido, Xavier, Givans, Jahmour, Gluscevic, Vera, Golec, Joseph E., Guan, Yilun, Halpern, Mark, Han, Dongwon, Hasselfield, Matthew, Healy, Erin, Henderson, Shawn, Hensley, Brandon, Hervías-Caimapo, Carlos, Hilton, Gene C., Hilton, Matt, Hincks, Adam D., Hložek, Renée, Ho, Shuay-Pwu Patty, Huber, Zachary B., Hubmayr, Johannes, Huffenberger, Kevin M., Hughes, John P., Irwin, Kent, Isopi, Giovanni, Jense, Hidde T., Keller, Ben, Kim, Joshua, Knowles, Kenda, Koopman, Brian J., Kosowsky, Arthur, Kramer, Darby, Kusiak, Aleksandra, La Posta, Adrien, Lakey, Victoria, Lee, Eunseong, Li, Zack, Li, Yaqiong, Limon, Michele, Lokken, Martine, Louis, Thibaut, Lungu, Marius, MacCrann, Niall, MacInnis, Amanda, Maldonado, Diego, Maldonado, Felipe, Mallaby-Kay, Maya, Marques, Gabriela A., van Marrewijk, Joshiwa, McCarthy, Fiona, McMahon, Jeff, Mehta, Yogesh, Menanteau, Felipe, Moodley, Kavilan, Morris, Thomas W., Mroczkowski, Tony, Naess, Sigurd, Namikawa, Toshiya, Nati, Federico, Newburgh, Laura, Nicola, Andrina, Niemack, Michael D., Nolta, Michael R., Orlowski-Scherer, John, Page, Lyman A., Pandey, Shivam, Partridge, Bruce, Prince, Heather, Puddu, Roberto, Qu, Frank J., Radiconi, Federico, Robertson, Naomi, Rojas, Felipe, Sakuma, Tai, Salatino, Maria, Schaan, Emmanuel, Schmitt, Benjamin L., Sehgal, Neelima, Shaikh, Shabbir, Sherwin, Blake D., Sierra, Carlos, Sievers, Jon, Sifón, Cristóbal, Simon, Sara, Sonka, Rita, Spergel, David N., Staggs, Suzanne T., Storer, Emilie, Switzer, Eric R., Tampier, Niklas, Thornton, Robert, Trac, Hy, Treu, Jesse, Tucker, Carole, Ullom, Joel, Vale, Leila R., Van Engelen, Alexander, Van Lanen, Jeff, Vargas, Cristian, Vavagiakis, Eve M., Wagoner, Kasey, Wang, Yuhan, Wenzl, Lukas, Wollack, Edward J., Xu, Zhilei, Zago, Fernando, and Zheng, Kaiwen
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Observations of the millimeter sky contain valuable information on a number of signals, including the blackbody cosmic microwave background (CMB), Galactic emissions, and the Compton-$y$ distortion due to the thermal Sunyaev-Zel'dovich (tSZ) effect. Extracting new insight into cosmological and astrophysical questions often requires combining multi-wavelength observations to spectrally isolate one component. In this work, we present a new arcminute-resolution Compton-$y$ map, which traces out the line-of-sight-integrated electron pressure, as well as maps of the CMB in intensity and E-mode polarization, across a third of the sky (around 13,000 sq.~deg.). We produce these through a joint analysis of data from the Atacama Cosmology Telescope (ACT) Data Release 4 and 6 at frequencies of roughly 93, 148, and 225 GHz, together with data from the \textit{Planck} satellite at frequencies between 30 GHz and 545 GHz. We present detailed verification of an internal linear combination pipeline implemented in a needlet frame that allows us to efficiently suppress Galactic contamination and account for spatial variations in the ACT instrument noise. These maps provide a significant advance, in noise levels and resolution, over the existing \textit{Planck} component-separated maps and will enable a host of science goals including studies of cluster and galaxy astrophysics, inferences of the cosmic velocity field, primordial non-Gaussianity searches, and gravitational lensing reconstruction of the CMB., Comment: The Compton-y map and associated products will be made publicly available upon publication of the paper. The CMB T and E mode maps will be made available when the DR6 maps are made public
Published: 2023

3. The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters

Author: Madhavacheril, Mathew S., Qu, Frank J., Sherwin, Blake D., MacCrann, Niall, Li, Yaqiong, Abril-Cabezas, Irene, Ade, Peter A. R., Aiola, Simone, Alford, Tommy, Amiri, Mandana, Amodeo, Stefania, An, Rui, Atkins, Zachary, Austermann, Jason E., Battaglia, Nicholas, Battistelli, Elia Stefano, Beall, James A., Bean, Rachel, Beringue, Benjamin, Bhandarkar, Tanay, Biermann, Emily, Bolliet, Boris, Bond, J Richard, Cai, Hongbo, Calabrese, Erminia, Calafut, Victoria, Capalbo, Valentina, Carrero, Felipe, Challinor, Anthony, Chesmore, Grace E., Cho, Hsiao-mei, Choi, Steve K., Clark, Susan E., Rosado, Rodrigo Córdova, Cothard, Nicholas F., Coughlin, Kevin, Coulton, William, Crowley, Kevin T., Dalal, Roohi, Darwish, Omar, Devlin, Mark J., Dicker, Simon, Doze, Peter, Duell, Cody J., Duff, Shannon M., Duivenvoorden, Adriaan J., Dunkley, Jo, Dünner, Rolando, Fanfani, Valentina, Fankhanel, Max, Farren, Gerrit, Ferraro, Simone, Freundt, Rodrigo, Fuzia, Brittany, Gallardo, Patricio A., Garrido, Xavier, Givans, Jahmour, Gluscevic, Vera, Golec, Joseph E., Guan, Yilun, Hall, Kirsten R., Halpern, Mark, Han, Dongwon, Harrison, Ian, Hasselfield, Matthew, Healy, Erin, Henderson, Shawn, Hensley, Brandon, Hervías-Caimapo, Carlos, Hill, J. Colin, Hilton, Gene C., Hilton, Matt, Hincks, Adam D., Hložek, Renée, Ho, Shuay-Pwu Patty, Huber, Zachary B., Hubmayr, Johannes, Huffenberger, Kevin M., Hughes, John P., Irwin, Kent, Isopi, Giovanni, Jense, Hidde T., Keller, Ben, Kim, Joshua, Knowles, Kenda, Koopman, Brian J., Kosowsky, Arthur, Kramer, Darby, Kusiak, Aleksandra, La Posta, Adrien, Lague, Alex, Lakey, Victoria, Lee, Eunseong, Li, Zack, Limon, Michele, Lokken, Martine, Louis, Thibaut, Lungu, Marius, MacInnis, Amanda, Maldonado, Diego, Maldonado, Felipe, Mallaby-Kay, Maya, Marques, Gabriela A., McMahon, Jeff, Mehta, Yogesh, Menanteau, Felipe, Moodley, Kavilan, Morris, Thomas W., Mroczkowski, Tony, Naess, Sigurd, Namikawa, Toshiya, Nati, Federico, Newburgh, Laura, Nicola, Andrina, Niemack, Michael D., Nolta, Michael R., Orlowski-Scherer, John, Page, Lyman A., Pandey, Shivam, Partridge, Bruce, Prince, Heather, Puddu, Roberto, Radiconi, Federico, Robertson, Naomi, Rojas, Felipe, Sakuma, Tai, Salatino, Maria, Schaan, Emmanuel, Schmitt, Benjamin L., Sehgal, Neelima, Shaikh, Shabbir, Sierra, Carlos, Sievers, Jon, Sifón, Cristóbal, Simon, Sara, Sonka, Rita, Spergel, David N., Staggs, Suzanne T., Storer, Emilie, Switzer, Eric R., Tampier, Niklas, Thornton, Robert, Trac, Hy, Treu, Jesse, Tucker, Carole, Ullom, Joel, Vale, Leila R., Van Engelen, Alexander, Van Lanen, Jeff, van Marrewijk, Joshiwa, Vargas, Cristian, Vavagiakis, Eve M., Wagoner, Kasey, Wang, Yuhan, Wenzl, Lukas, Wollack, Edward J., Xu, Zhilei, Zago, Fernando, and Zheng, Kaiwen
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics, High Energy Physics - Phenomenology
Abstract: We present cosmological constraints from a gravitational lensing mass map covering 9400 sq. deg. reconstructed from CMB measurements made by the Atacama Cosmology Telescope (ACT) from 2017 to 2021. In combination with BAO measurements (from SDSS and 6dF), we obtain the amplitude of matter fluctuations $\sigma_8 = 0.819 \pm 0.015$ at 1.8% precision, $S_8\equiv\sigma_8({\Omega_{\rm m}}/0.3)^{0.5}=0.840\pm0.028$ and the Hubble constant $H_0= (68.3 \pm 1.1)\, \text{km}\,\text{s}^{-1}\,\text{Mpc}^{-1}$ at 1.6% precision. A joint constraint with CMB lensing measured by the Planck satellite yields even more precise values: $\sigma_8 = 0.812 \pm 0.013$, $S_8\equiv\sigma_8({\Omega_{\rm m}}/0.3)^{0.5}=0.831\pm0.023$ and $H_0= (68.1 \pm 1.0)\, \text{km}\,\text{s}^{-1}\,\text{Mpc}^{-1}$. These measurements agree well with $\Lambda$CDM-model extrapolations from the CMB anisotropies measured by Planck. To compare these constraints to those from the KiDS, DES, and HSC galaxy surveys, we revisit those data sets with a uniform set of assumptions, and find $S_8$ from all three surveys are lower than that from ACT+Planck lensing by varying levels ranging from 1.7-2.1$\sigma$. These results motivate further measurements and comparison, not just between the CMB anisotropies and galaxy lensing, but also between CMB lensing probing $z\sim 0.5-5$ on mostly-linear scales and galaxy lensing at $z\sim 0.5$ on smaller scales. We combine our CMB lensing measurements with CMB anisotropies to constrain extensions of $\Lambda$CDM, limiting the sum of the neutrino masses to $\sum m_{\nu} < 0.13$ eV (95% c.l.), for example. Our results provide independent confirmation that the universe is spatially flat, conforms with general relativity, and is described remarkably well by the $\Lambda$CDM model, while paving a promising path for neutrino physics with gravitational lensing from upcoming ground-based CMB surveys., Comment: 32 pages, 17 figures, replaced with version accepted in ApJ (Feb 2024). Cosmological likelihood data and mass maps are public here: https://lambda.gsfc.nasa.gov/product/act/actadv_prod_table.html ; likelihood software is here: https://github.com/ACTCollaboration/act_dr6_lenslike . Also see companion papers Qu et al and MacCrann et al
Published: 2023
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4. The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and its Implications for Structure Growth

Author: Qu, Frank J., Sherwin, Blake D., Madhavacheril, Mathew S., Han, Dongwon, Crowley, Kevin T., Abril-Cabezas, Irene, Ade, Peter A. R., Aiola, Simone, Alford, Tommy, Amiri, Mandana, Amodeo, Stefania, An, Rui, Atkins, Zachary, Austermann, Jason E., Battaglia, Nicholas, Battistelli, Elia Stefano, Beall, James A., Bean, Rachel, Beringue, Benjamin, Bhandarkar, Tanay, Biermann, Emily, Bolliet, Boris, Bond, J Richard, Cai, Hongbo, Calabrese, Erminia, Calafut, Victoria, Capalbo, Valentina, Carrero, Felipe, Carron, Julien, Challinor, Anthony, Chesmore, Grace E., Cho, Hsiao-mei, Choi, Steve K., Clark, Susan E., Rosado, Rodrigo Córdova, Cothard, Nicholas F., Coughlin, Kevin, Coulton, William, Dalal, Roohi, Darwish, Omar, Devlin, Mark J., Dicker, Simon, Doze, Peter, Duell, Cody J., Duff, Shannon M., Duivenvoorden, Adriaan J., Dunkley, Jo, Dünner, Rolando, Fanfani, Valentina, Fankhanel, Max, Farren, Gerrit, Ferraro, Simone, Freundt, Rodrigo, Fuzia, Brittany, Gallardo, Patricio A., Garrido, Xavier, Gluscevic, Vera, Golec, Joseph E., Guan, Yilun, Halpern, Mark, Harrison, Ian, Hasselfield, Matthew, Healy, Erin, Henderson, Shawn, Hensley, Brandon, Hervías-Caimapo, Carlos, Hill, J. Colin, Hilton, Gene C., Hilton, Matt, Hincks, Adam D., Hložek, Renée, Ho, Shuay-Pwu Patty, Huber, Zachary B., Hubmayr, Johannes, Huffenberger, Kevin M., Hughes, John P., Irwin, Kent, Isopi, Giovanni, Jense, Hidde T., Keller, Ben, Kim, Joshua, Knowles, Kenda, Koopman, Brian J., Kosowsky, Arthur, Kramer, Darby, Kusiak, Aleksandra, La Posta, Adrien, Lague, Alex, Lakey, Victoria, Lee, Eunseong, Li, Zack, Li, Yaqiong, Limon, Michele, Lokken, Martine, Louis, Thibaut, Lungu, Marius, MacCrann, Niall, MacInnis, Amanda, Maldonado, Diego, Maldonado, Felipe, Mallaby-Kay, Maya, Marques, Gabriela A., McMahon, Jeff, Mehta, Yogesh, Menanteau, Felipe, Moodley, Kavilan, Morris, Thomas W., Mroczkowski, Tony, Naess, Sigurd, Namikawa, Toshiya, Nati, Federico, Newburgh, Laura, Nicola, Andrina, Niemack, Michael D., Nolta, Michael R., Orlowski-Scherer, John, Page, Lyman A., Pandey, Shivam, Partridge, Bruce, Prince, Heather, Puddu, Roberto, Radiconi, Federico, Robertson, Naomi, Rojas, Felipe, Sakuma, Tai, Salatino, Maria, Schaan, Emmanuel, Schmitt, Benjamin L., Sehgal, Neelima, Shaikh, Shabbir, Sierra, Carlos, Sievers, Jon, Sifón, Cristóbal, Simon, Sara, Sonka, Rita, Spergel, David N., Staggs, Suzanne T., Storer, Emilie, Switzer, Eric R., Tampier, Niklas, Thornton, Robert, Trac, Hy, Treu, Jesse, Tucker, Carole, Ulluom, Joel, Vale, Leila R., Van Engelen, Alexander, Van Lanen, Jeff, van Marrewijk, Joshiwa, Vargas, Cristian, Vavagiakis, Eve M., Wagoner, Kasey, Wang, Yuhan, Wenzl, Lukas, Wollack, Edward J., Xu, Zhilei, Zago, Fernando, and Zhang, Kaiwen
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present new measurements of cosmic microwave background (CMB) lensing over $9400$ sq. deg. of the sky. These lensing measurements are derived from the Atacama Cosmology Telescope (ACT) Data Release 6 (DR6) CMB dataset, which consists of five seasons of ACT CMB temperature and polarization observations. We determine the amplitude of the CMB lensing power spectrum at $2.3\%$ precision ($43\sigma$ significance) using a novel pipeline that minimizes sensitivity to foregrounds and to noise properties. To ensure our results are robust, we analyze an extensive set of null tests, consistency tests, and systematic error estimates and employ a blinded analysis framework. The baseline spectrum is well fit by a lensing amplitude of $A_{\mathrm{lens}}=1.013\pm0.023$ relative to the Planck 2018 CMB power spectra best-fit $\Lambda$CDM model and $A_{\mathrm{lens}}=1.005\pm0.023$ relative to the $\text{ACT DR4} + \text{WMAP}$ best-fit model. From our lensing power spectrum measurement, we derive constraints on the parameter combination $S^{\mathrm{CMBL}}_8 \equiv \sigma_8 \left({\Omega_m}/{0.3}\right)^{0.25}$ of $S^{\mathrm{CMBL}}_8= 0.818\pm0.022$ from ACT DR6 CMB lensing alone and $S^{\mathrm{CMBL}}_8= 0.813\pm0.018$ when combining ACT DR6 and Planck NPIPE CMB lensing power spectra. These results are in excellent agreement with $\Lambda$CDM model constraints from Planck or $\text{ACT DR4} + \text{WMAP}$ CMB power spectrum measurements. Our lensing measurements from redshifts $z\sim0.5$--$5$ are thus fully consistent with $\Lambda$CDM structure growth predictions based on CMB anisotropies probing primarily $z\sim1100$. We find no evidence for a suppression of the amplitude of cosmic structure at low redshifts, Comment: 45+22 pages, 50 figures. v2 matches with published version in ApJ. Cosmological likelihood data and lensing maps are here: https://lambda.gsfc.nasa.gov/product/act/actadv_prod_table.html ; likelihood software is here: https://github.com/ACTCollaboration/act_dr6_lenslike . Also see companion papers Madhavacheril et al and MacCrann et al
Published: 2023
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5. Assessing consistency between CMB temperature and polarization measurements, with application to Planck, ACT and SPT

Author: La Posta, Adrien, Natale, Umberto, Calabrese, Erminia, Garrido, Xavier, and Louis, Thibaut
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Planck's Cosmic Microwave Background temperature and polarization observations are the premier dataset for constraining cosmological models. Cosmic variance limited temperature at large and intermediate scales today dominates the constraints; polarization provides additional constraining power and further scrutiny of the models. To complete this picture from Planck, ground-based experiments, such as the Atacama Cosmology Telescope (ACT) and the South Pole Telescope (SPT) continue to add temperature and polarization measurements at small scales, allowing for the extraction of competitive cosmological constraints from the $TE$ and $EE$ power spectra. Matching at the same time all these stringent probes is a key challenge and validation step for any cosmological model. In particular, $\Lambda$CDM requires a tight consistency between the temperature and polarization measurements. In this paper, we present a number of methods to identify and quantify possible inconsistencies between temperature and polarization, we apply them to the latest Planck, ACT and SPT data and find no evidence for a deviation from $\Lambda$CDM. Application of these methods will have increased importance for future, more constraining CMB data., Comment: 13 pages, 11 figures
Published: 2022
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6. The Simons Observatory: a new open-source power spectrum pipeline applied to the Planck legacy data

Author: Li, Zack, Louis, Thibaut, Calabrese, Erminia, Jense, Hidde, Alonso, David, Bond, J. Richard, Choi, Steve K., Dunkley, Jo, Fabbian, Giulio, Garrido, Xavier, Jaffe, Andrew H., Madhavacheril, Mathew S., Meerburg, P. Daniel, Natale, Umberto, and Qu, Frank J.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present a reproduction of the Planck 2018 angular power spectra at $\ell > 30$, and associated covariance matrices, for intensity and polarization maps at 100, 143 and 217 GHz. This uses a new, publicly available, pipeline that is part of the PSpipe package. As a test case we use the same input maps, ancillary products, and analysis choices as in the Planck 2018 analysis, and find that we can reproduce the spectra to 0.1$\sigma$ precision, and the covariance matrices to 10%. We show that cosmological parameters estimated from our re-derived products agree with the public Planck products to 0.1$\sigma$, providing an independent cross-check of the Planck team's analysis. Going forward, the publicly-available code can be easily adapted to use alternative input maps, data selections and analysis choices, for future optimal analysis of Planck data with new ground-based Cosmic Microwave Background data., Comment: 25 pages, 18 figures, code available at https://simonsobs.github.io/planck-pr3-web/
Published: 2021

7. Constraints on Pre-Recombination Early Dark Energy from SPT-3G Public Data

Author: La Posta, Adrien, Louis, Thibaut, Garrido, Xavier, and Hill, J. Colin
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Early dark energy (EDE) is a proposed solution to the Hubble tension in which a new cosmological field accelerates cosmic expansion prior to recombination and reduces the physical size of the sound horizon. In previous work, a slight preference for a non-zero EDE contribution was found in the latest Atacama Cosmology Telescope data (ACT DR4), while the Planck satellite legacy data alone do not show evidence for it. In this work, we use the most recent public data from the South Pole Telescope (SPT-3G) to constrain the parameters of the EDE scenario. We find that at the current precision level of SPT-3G, an EDE contribution to the total energy density of the universe prior to recombination of $\sim 10\%$ can not be ruled out, but that the data are also consistent with no EDE. The combination of ACT DR4 and SPT-3G with the Planck large-scale temperature anisotropy measurement shows a hint ($2.6\sigma$) for non-zero EDE; however, this preference disappears when the full Planck 2018 data set is included., Comment: 11 pages, 5 figures
Published: 2021
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8. Cosmology with Planck T-E correlation coefficient

Author: La Posta, Adrien, Louis, Thibaut, Garrido, Xavier, Tristram, Matthieu, and Henrot-Versillé, Sophie
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Tensions in cosmological parameters measurement motivate a revisit of the effects of instrumental systematics. In this article, we focus on the Pearson's correlation coefficient of the cosmic microwave background temperature and polarization E modes $\mathcal{R}_\ell^{\rm TE}$ which has the property of not being biased by multiplicative instrumental systematics. We build a $\mathcal{R}_\ell^{\rm TE}$-based likelihood for the Planck data, and present the first constraints on $\Lambda$CDM parameters from the correlation coefficient. Our results are compatible with parameters derived from a power spectra based likelihood. In particular the value of the Hubble parameter $H_0$ characterizing the expansion of the Universe today, 67.5 $\pm$ 1.3 km/s/Mpc, is consistent with the ones inferred from standard CMB analysis. We also discuss the consistency of the Planck correlation coefficient with the one computed from the most recent ACTPol power spectra., Comment: 10 pages, 5 figures
Published: 2021
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9. Can Synbone® cylinders and deer femurs reproduce ballistic fracture patterns observed in human long bones?

Author: Schwab, Nathalie, Jordana, Xavier, Soler, Joan, Garrido, Xavier, Brillas, Pedro, Savio, Andrés, Lavín, Santiago, Ortega-Sánchez, Marisa, and Galtés, Ignasi
Published: 2023
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10. Fast computation of angular power spectra and covariances of high-resolution cosmic microwave background maps using the Toeplitz approximation

Author: Louis, Thibaut, Naess, Sigurd, Garrido, Xavier, and Challinor, Anthony
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present a simple approximation that can speed up the computation of the mode-coupling matrices, which are usually the bottleneck for computing unbiased angular power spectra, as well as their associated covariance matrices, of the cosmic microwave background temperature and polarization anisotropies. The approximation results in the speed up of the MASTER algorithm by more than an order of magnitude with very little loss of precision. We demonstrate the performance on simulations of forthcoming cosmic microwave background surveys such as the Simons Observatory and CMB-S4 for a wide variety of survey window functions., Comment: 10 pages, 7 figures. The code used to produce all results of the paper is publicly available on Github
Published: 2020
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11. Consistency of CMB experiments beyond cosmic variance

Author: Louis, Thibaut, Garrido, Xavier, Soussana, Adam, Tristram, Matthieu, Henrot-Versillé, Sophie, and Vanneste, Sylvain
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: The next generation of Cosmic Microwave Background experiments will produce cosmic variance limited observations over a large fraction of sky and for a large range of multipoles. In this work we discuss different consistency tests that can be performed with the upcoming data from the Simons Observatory and the Planck data. We quantify the level of expected cosmological parameter shifts probed by these tests. We discuss the effect of difference in frequency of observation and present forecasts on a direct measurement of the Planck T-to-E leakage beam. We find that instrumental systematics in either of the experiments will be assessed with an exquisite precision, well beyond the intrinsic uncertainties due to the CMB cosmic variance., Comment: 13 pages, 9 figures (accepted for publication in PRD)
Published: 2019
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12. QUBIC: Exploring the primordial Universe with the Q\&U Bolometric Interferometer

Author: Mennella, Aniello, Ade, Peter, Amico, Giorgio, Auguste, Didier, Aumont, Jonathan, Banfi, Stefano, Barbaràn, Gustavo, Battaglia, Paola, Battistelli, Elia, Baù, Alessandro, Bélier, Benoit, Bennett, David G., Bergé, Laurent, Bernard, Jean Philippe, Bersanelli, Marco, Sazy, Marie Anne Bigot, Bleurvacq, Nathat, Bonaparte, Juan, Bonis, Julien, Bunn, Emory F., Burke, David, Buzi, Daniele, Buzzelli, Alessandro, Cavaliere, Francesco, Chanial, Pierre, Chapron, Claude, Charlassier, Romain, Columbro, Fabio, Coppi, Gabriele, Coppolecchia, Alessandro, D'Agostino, Rocco, D'Alessandro, Giuseppe, De Bernardis, Paolo, De Gasperis, Giancarlo, De Leo, Michele, De Petris, Marco, Di Donato, Andres, Dumoulin, Louis, Etchegoyen, Alberto, Fasciszewski, Adrián, Franceschet, Cristian, Lerena, Martin Miguel Gamboa, Garcia, Beatriz, Garrido, Xavier, Gaspard, Michel, Gault, Amanda, Gayer, Donnacha, Gervasi, Massimo, Giard, Martin, Héraud, Yannick Giraud, Berisso, Mariano Gómez, González, Manuel, Gradziel, Marcin, Grandsire, Laurent, Guerard, Eric, Hamilton, Jean Christophe, Harari, Diego, Haynes, Vic, Versillé, Sophie Henrot, Hoang, Duc Thuong, Holtzer, Nicolas, Incardona, Federico, Jules, Eric, Kaplan, Jean, Korotkov, Andrei, Kristukat, Christian, Lamagna, Luca, Loucatos, Soutiris, Lowitz, Amy, Lukovic, Vladimir, Thibault, Louis, Luterstein, Raùl Horacio, Maffei, Bruno, Marnieros, Stefanos, Masi, Silvia, Mattei, Angelo, May, Andrew, McCulloch, Mark, Medina, Maria C., Mele, Lorenzo, Melhuish, Simon J., Montier, Ludovic, Mousset, Louise, Mundo, Luis Mariano, Murphy, John Anthony, Murphy, James, O'Sullivan, Creidhe, Olivieri, Emiliano, Paiella, Alessandro, Pajot, Francois, Passerini, Andrea, Pastoriza, Hernan, Pelosi, Alessandro, Perbost, Camille, Perciballi, Maurizio, Pezzotta, Federico, Piacentini, Francesco, Piat, Michel, Piccirillo, Lucio, Pisano, Giampaolo, Polenta, Gianluca, Prêle, Damien, Puddu, Roberto, Rambaud, Damien, Ringegni, Pablo, Romero, Gustavo E., Salatino, Maria, Schillaci, Alessandro, Scóccola, Claudia G., Scully, Stephen P., Spinelli, Sebastiano, Stolpovskiy, Michail, Suarez, Federico, Stankowiak, Guillaume, Tartari, Andrea, Thermeau, Jean Pierre, Timbie, Peter, Tomasi, Maurizio, Torchinsky, Steve A., Tristram, Mathieu, Tucker, Gregory S., Tucker, Carole E., Vanneste, Sylvain, Viganò, Daniele, Vittorio, Nicola, Voisin, Fabrice, Watson, Robert, Wicek, Francois, Zannoni, Mario, and Zullo, Antonio
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: In this paper we describe QUBIC, an experiment that will observe the polarized microwave sky with a novel approach, which combines the sensitivity of state-of-the art bolometric detectors with the systematic effects control typical of interferometers. QUBIC unique features are the so-called "self-calibration", a technique that allows us to clean the measured data from instrumental effects, and its spectral imaging power, i.e. the ability to separate the signal in various sub-bands within each frequency band. QUBIC will observe the sky in two main frequency bands: 150 GHz and 220 GHz. A technological demonstrator is currently under testing and will be deployed in Argentina during 2019, while the final instrument is expected to be installed during 2020., Comment: Proceedings of the 2018 ICNFP conference, Crete. Published by Universe arXiv admin note: text overlap with arXiv:1801.03730
Published: 2018
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13. Comparison of results on $N_\mathrm{eff}$ from various Planck likelihoods

Author: Henrot-Versillé, Sophie, Couchot, Francois, Garrido, Xavier, Imada, Hiroaki, Louis, Thibaut, Tristram, Matthieu, and Vanneste, Sylvain
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: In this paper, we study the estimation of the effective number of relativistic species from a combination of CMB and BAO data. We vary different ingredients of the analysis: the Planck high-$\ell$ likelihoods, the Boltzmann solvers, and the statistical approaches. The variation of the inferred values gives an indication of an additional systematic uncertainty, which is of the same order of magnitude as the error derived from each individual likelihood. We show that this systematic is essentially associated to the assumptions made in the high-$\ell$ likelihoods implementations, in particular for the foreground residuals modellings. We also compare a subset of likelihoods using only the TE power spectra, expected to be less sensitive to foreground residuals., Comment: accepted for publication in A&A
Published: 2018
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14. Atacama Cosmology Telescope: High-resolution component-separated maps across one third of the sky

Author: Coulton, William, primary, Madhavacheril, Mathew S., additional, Duivenvoorden, Adriaan J., additional, Hill, J. Colin, additional, Abril-Cabezas, Irene, additional, Ade, Peter A. R., additional, Aiola, Simone, additional, Alford, Tommy, additional, Amiri, Mandana, additional, Amodeo, Stefania, additional, An, Rui, additional, Atkins, Zachary, additional, Austermann, Jason E., additional, Battaglia, Nicholas, additional, Battistelli, Elia Stefano, additional, Beall, James A., additional, Bean, Rachel, additional, Beringue, Benjamin, additional, Bhandarkar, Tanay, additional, Biermann, Emily, additional, Bolliet, Boris, additional, Bond, J. Richard, additional, Cai, Hongbo, additional, Calabrese, Erminia, additional, Calafut, Victoria, additional, Capalbo, Valentina, additional, Carrero, Felipe, additional, Chesmore, Grace E., additional, Cho, Hsiao-mei, additional, Choi, Steve K., additional, Clark, Susan E., additional, Rosado, Rodrigo Córdova, additional, Cothard, Nicholas F., additional, Coughlin, Kevin, additional, Crowley, Kevin T., additional, Devlin, Mark J., additional, Dicker, Simon, additional, Doze, Peter, additional, Duell, Cody J., additional, Duff, Shannon M., additional, Dunkley, Jo, additional, Dünner, Rolando, additional, Fanfani, Valentina, additional, Fankhanel, Max, additional, Farren, Gerrit, additional, Ferraro, Simone, additional, Freundt, Rodrigo, additional, Fuzia, Brittany, additional, Gallardo, Patricio A., additional, Garrido, Xavier, additional, Givans, Jahmour, additional, Gluscevic, Vera, additional, Golec, Joseph E., additional, Guan, Yilun, additional, Halpern, Mark, additional, Han, Dongwon, additional, Hasselfield, Matthew, additional, Healy, Erin, additional, Henderson, Shawn, additional, Hensley, Brandon, additional, Hervías-Caimapo, Carlos, additional, Hilton, Gene C., additional, Hilton, Matt, additional, Hincks, Adam D., additional, Hložek, Renée, additional, Ho, Shuay-Pwu Patty, additional, Huber, Zachary B., additional, Hubmayr, Johannes, additional, Huffenberger, Kevin M., additional, Hughes, John P., additional, Irwin, Kent, additional, Isopi, Giovanni, additional, Jense, Hidde T., additional, Keller, Ben, additional, Kim, Joshua, additional, Knowles, Kenda, additional, Koopman, Brian J., additional, Kosowsky, Arthur, additional, Kramer, Darby, additional, Kusiak, Aleksandra, additional, La Posta, Adrien, additional, Lakey, Victoria, additional, Lee, Eunseong, additional, Li, Zack, additional, Li, Yaqiong, additional, Limon, Michele, additional, Lokken, Martine, additional, Louis, Thibaut, additional, Lungu, Marius, additional, MacCrann, Niall, additional, MacInnis, Amanda, additional, Maldonado, Diego, additional, Maldonado, Felipe, additional, Mallaby-Kay, Maya, additional, Marques, Gabriela A., additional, van Marrewijk, Joshiwa, additional, McCarthy, Fiona, additional, McMahon, Jeff, additional, Mehta, Yogesh, additional, Menanteau, Felipe, additional, Moodley, Kavilan, additional, Morris, Thomas W., additional, Mroczkowski, Tony, additional, Naess, Sigurd, additional, Namikawa, Toshiya, additional, Nati, Federico, additional, Newburgh, Laura, additional, Nicola, Andrina, additional, Niemack, Michael D., additional, Nolta, Michael R., additional, Orlowski-Scherer, John, additional, Page, Lyman A., additional, Pandey, Shivam, additional, Partridge, Bruce, additional, Prince, Heather, additional, Puddu, Roberto, additional, Qu, Frank J., additional, Radiconi, Federico, additional, Robertson, Naomi, additional, Rojas, Felipe, additional, Sakuma, Tai, additional, Salatino, Maria, additional, Schaan, Emmanuel, additional, Schmitt, Benjamin L., additional, Sehgal, Neelima, additional, Shaikh, Shabbir, additional, Sherwin, Blake D., additional, Sierra, Carlos, additional, Sievers, Jon, additional, Sifón, Cristóbal, additional, Simon, Sara, additional, Sonka, Rita, additional, Spergel, David N., additional, Staggs, Suzanne T., additional, Storer, Emilie, additional, Switzer, Eric R., additional, Tampier, Niklas, additional, Thornton, Robert, additional, Trac, Hy, additional, Treu, Jesse, additional, Tucker, Carole, additional, Ullom, Joel, additional, Vale, Leila R., additional, Van Engelen, Alexander, additional, Van Lanen, Jeff, additional, Vargas, Cristian, additional, Vavagiakis, Eve M., additional, Wagoner, Kasey, additional, Wang, Yuhan, additional, Wenzl, Lukas, additional, Wollack, Edward J., additional, Xu, Zhilei, additional, Zago, Fernando, additional, and Zheng, Kaiwen, additional
Published: 2024
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15. Osteonal Damage Patterns from Ballistic and Blunt Force Trauma in Human Long Bones

Author: Sexton, Keira, primary, Schwab, Nathalie, additional, Galtés, Ignasi, additional, Casas, Anna, additional, Armentano, Nuria, additional, Brillas, Pedro, additional, Garrido, Xavier, additional, and Jordana, Xavier, additional
Published: 2024
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16. The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters

Author: Madhavacheril, Mathew S., primary, Qu, Frank J., additional, Sherwin, Blake D., additional, MacCrann, Niall, additional, Li, Yaqiong, additional, Abril-Cabezas, Irene, additional, Ade, Peter A. R., additional, Aiola, Simone, additional, Alford, Tommy, additional, Amiri, Mandana, additional, Amodeo, Stefania, additional, An, Rui, additional, Atkins, Zachary, additional, Austermann, Jason E., additional, Battaglia, Nicholas, additional, Battistelli, Elia Stefano, additional, Beall, James A., additional, Bean, Rachel, additional, Beringue, Benjamin, additional, Bhandarkar, Tanay, additional, Biermann, Emily, additional, Bolliet, Boris, additional, Bond, J Richard, additional, Cai, Hongbo, additional, Calabrese, Erminia, additional, Calafut, Victoria, additional, Capalbo, Valentina, additional, Carrero, Felipe, additional, Challinor, Anthony, additional, Chesmore, Grace E., additional, Cho, Hsiao-mei, additional, Choi, Steve K., additional, Clark, Susan E., additional, Rosado, Rodrigo Córdova, additional, Cothard, Nicholas F., additional, Coughlin, Kevin, additional, Coulton, William, additional, Crowley, Kevin T., additional, Dalal, Roohi, additional, Darwish, Omar, additional, Devlin, Mark J., additional, Dicker, Simon, additional, Doze, Peter, additional, Duell, Cody J., additional, Duff, Shannon M., additional, Duivenvoorden, Adriaan J., additional, Dunkley, Jo, additional, Dünner, Rolando, additional, Fanfani, Valentina, additional, Fankhanel, Max, additional, Farren, Gerrit, additional, Ferraro, Simone, additional, Freundt, Rodrigo, additional, Fuzia, Brittany, additional, Gallardo, Patricio A., additional, Garrido, Xavier, additional, Givans, Jahmour, additional, Gluscevic, Vera, additional, Golec, Joseph E., additional, Guan, Yilun, additional, Hall, Kirsten R., additional, Halpern, Mark, additional, Han, Dongwon, additional, Harrison, Ian, additional, Hasselfield, Matthew, additional, Healy, Erin, additional, Henderson, Shawn, additional, Hensley, Brandon, additional, Hervías-Caimapo, Carlos, additional, Hill, J. Colin, additional, Hilton, Gene C., additional, Hilton, Matt, additional, Hincks, Adam D., additional, Hložek, Renée, additional, Ho, Shuay-Pwu Patty, additional, Huber, Zachary B., additional, Hubmayr, Johannes, additional, Huffenberger, Kevin M., additional, Hughes, John P., additional, Irwin, Kent, additional, Isopi, Giovanni, additional, Jense, Hidde T., additional, Keller, Ben, additional, Kim, Joshua, additional, Knowles, Kenda, additional, Koopman, Brian J., additional, Kosowsky, Arthur, additional, Kramer, Darby, additional, Kusiak, Aleksandra, additional, La Posta, Adrien, additional, Lague, Alex, additional, Lakey, Victoria, additional, Lee, Eunseong, additional, Li, Zack, additional, Limon, Michele, additional, Lokken, Martine, additional, Louis, Thibaut, additional, Lungu, Marius, additional, MacInnis, Amanda, additional, Maldonado, Diego, additional, Maldonado, Felipe, additional, Mallaby-Kay, Maya, additional, Marques, Gabriela A., additional, McMahon, Jeff, additional, Mehta, Yogesh, additional, Menanteau, Felipe, additional, Moodley, Kavilan, additional, Morris, Thomas W., additional, Mroczkowski, Tony, additional, Naess, Sigurd, additional, Namikawa, Toshiya, additional, Nati, Federico, additional, Newburgh, Laura, additional, Nicola, Andrina, additional, Niemack, Michael D., additional, Nolta, Michael R., additional, Orlowski-Scherer, John, additional, Page, Lyman A., additional, Pandey, Shivam, additional, Partridge, Bruce, additional, Prince, Heather, additional, Puddu, Roberto, additional, Radiconi, Federico, additional, Robertson, Naomi, additional, Rojas, Felipe, additional, Sakuma, Tai, additional, Salatino, Maria, additional, Schaan, Emmanuel, additional, Schmitt, Benjamin L., additional, Sehgal, Neelima, additional, Shaikh, Shabbir, additional, Sierra, Carlos, additional, Sievers, Jon, additional, Sifón, Cristóbal, additional, Simon, Sara, additional, Sonka, Rita, additional, Spergel, David N., additional, Staggs, Suzanne T., additional, Storer, Emilie, additional, Switzer, Eric R., additional, Tampier, Niklas, additional, Thornton, Robert, additional, Trac, Hy, additional, Treu, Jesse, additional, Tucker, Carole, additional, Ullom, Joel, additional, Vale, Leila R., additional, Van Engelen, Alexander, additional, Van Lanen, Jeff, additional, van Marrewijk, Joshiwa, additional, Vargas, Cristian, additional, Vavagiakis, Eve M., additional, Wagoner, Kasey, additional, Wang, Yuhan, additional, Wenzl, Lukas, additional, Wollack, Edward J., additional, Xu, Zhilei, additional, Zago, Fernando, additional, and Zheng, Kaiwen, additional
Published: 2024
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17. The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and Its Implications for Structure Growth

Author: Qu, Frank J., primary, Sherwin, Blake D., additional, Madhavacheril, Mathew S., additional, Han, Dongwon, additional, Crowley, Kevin T., additional, Abril-Cabezas, Irene, additional, Ade, Peter A. R., additional, Aiola, Simone, additional, Alford, Tommy, additional, Amiri, Mandana, additional, Amodeo, Stefania, additional, An, Rui, additional, Atkins, Zachary, additional, Austermann, Jason E., additional, Battaglia, Nicholas, additional, Battistelli, Elia Stefano, additional, Beall, James A., additional, Bean, Rachel, additional, Beringue, Benjamin, additional, Bhandarkar, Tanay, additional, Biermann, Emily, additional, Bolliet, Boris, additional, Bond, J Richard, additional, Cai, Hongbo, additional, Calabrese, Erminia, additional, Calafut, Victoria, additional, Capalbo, Valentina, additional, Carrero, Felipe, additional, Carron, Julien, additional, Challinor, Anthony, additional, Chesmore, Grace E., additional, Cho, Hsiao-mei, additional, Choi, Steve K., additional, Clark, Susan E., additional, Rosado, Rodrigo Córdova, additional, Cothard, Nicholas F., additional, Coughlin, Kevin, additional, Coulton, William, additional, Dalal, Roohi, additional, Darwish, Omar, additional, Devlin, Mark J., additional, Dicker, Simon, additional, Doze, Peter, additional, Duell, Cody J., additional, Duff, Shannon M., additional, Duivenvoorden, Adriaan J., additional, Dunkley, Jo, additional, Dünner, Rolando, additional, Fanfani, Valentina, additional, Fankhanel, Max, additional, Farren, Gerrit, additional, Ferraro, Simone, additional, Freundt, Rodrigo, additional, Fuzia, Brittany, additional, Gallardo, Patricio A., additional, Garrido, Xavier, additional, Gluscevic, Vera, additional, Golec, Joseph E., additional, Guan, Yilun, additional, Halpern, Mark, additional, Harrison, Ian, additional, Hasselfield, Matthew, additional, Healy, Erin, additional, Henderson, Shawn, additional, Hensley, Brandon, additional, Hervías-Caimapo, Carlos, additional, Hill, J. Colin, additional, Hilton, Gene C., additional, Hilton, Matt, additional, Hincks, Adam D., additional, Hložek, Renée, additional, Ho, Shuay-Pwu Patty, additional, Huber, Zachary B., additional, Hubmayr, Johannes, additional, Huffenberger, Kevin M., additional, Hughes, John P., additional, Irwin, Kent, additional, Isopi, Giovanni, additional, Jense, Hidde T., additional, Keller, Ben, additional, Kim, Joshua, additional, Knowles, Kenda, additional, Koopman, Brian J., additional, Kosowsky, Arthur, additional, Kramer, Darby, additional, Kusiak, Aleksandra, additional, La Posta, Adrien, additional, Lague, Alex, additional, Lakey, Victoria, additional, Lee, Eunseong, additional, Li, Zack, additional, Li, Yaqiong, additional, Limon, Michele, additional, Lokken, Martine, additional, Louis, Thibaut, additional, Lungu, Marius, additional, MacCrann, Niall, additional, MacInnis, Amanda, additional, Maldonado, Diego, additional, Maldonado, Felipe, additional, Mallaby-Kay, Maya, additional, Marques, Gabriela A., additional, McMahon, Jeff, additional, Mehta, Yogesh, additional, Menanteau, Felipe, additional, Moodley, Kavilan, additional, Morris, Thomas W., additional, Mroczkowski, Tony, additional, Naess, Sigurd, additional, Namikawa, Toshiya, additional, Nati, Federico, additional, Newburgh, Laura, additional, Nicola, Andrina, additional, Niemack, Michael D., additional, Nolta, Michael R., additional, Orlowski-Scherer, John, additional, Page, Lyman A., additional, Pandey, Shivam, additional, Partridge, Bruce, additional, Prince, Heather, additional, Puddu, Roberto, additional, Radiconi, Federico, additional, Robertson, Naomi, additional, Rojas, Felipe, additional, Sakuma, Tai, additional, Salatino, Maria, additional, Schaan, Emmanuel, additional, Schmitt, Benjamin L., additional, Sehgal, Neelima, additional, Shaikh, Shabbir, additional, Sierra, Carlos, additional, Sievers, Jon, additional, Sifón, Cristóbal, additional, Simon, Sara, additional, Sonka, Rita, additional, Spergel, David N., additional, Staggs, Suzanne T., additional, Storer, Emilie, additional, Switzer, Eric R., additional, Tampier, Niklas, additional, Thornton, Robert, additional, Trac, Hy, additional, Treu, Jesse, additional, Tucker, Carole, additional, Ullom, Joel, additional, Vale, Leila R., additional, Van Engelen, Alexander, additional, Van Lanen, Jeff, additional, van Marrewijk, Joshiwa, additional, Vargas, Cristian, additional, Vavagiakis, Eve M., additional, Wagoner, Kasey, additional, Wang, Yuhan, additional, Wenzl, Lukas, additional, Wollack, Edward J., additional, Xu, Zhilei, additional, Zago, Fernando, additional, and Zheng, Kaiwen, additional
Published: 2024
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18. The Simons Observatory: a new open-source power spectrum pipeline applied to the Planck legacy data

Author: Li, Zack, primary, Louis, Thibaut, additional, Calabrese, Erminia, additional, Jense, Hidde, additional, Alonso, David, additional, Atkins, Zachary, additional, Bond, J. Richard, additional, Choi, Steve K., additional, Dunkley, Jo, additional, Fabbian, Giulio, additional, Garrido, Xavier, additional, H. Jaffe, Andrew, additional, Madhavacheril, Mathew S., additional, Meerburg, P. Daniel, additional, Natale, Umberto, additional, and Qu, Frank J., additional
Published: 2023
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19. Assessing the consistency between CMB temperature and polarization measurements with application to Planck , ACT, and SPT data

Author: La Posta, Adrien, primary, Natale, Umberto, additional, Calabrese, Erminia, additional, Garrido, Xavier, additional, and Louis, Thibaut, additional
Published: 2023
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20. Can Synbone® cylinders and deer femurs reproduce ballistic fracture patterns observed in human long bones?

Author: Schwab, Nathalie, Jordana, Xavier, Soler, Joan, Garrido, Xavier, Brillas, Pedro, Savio, Andrés, Lavín, Santiago, Ortega-Sánchez, Marisa, and Galtés, Ignasi
Subjects: RED deer, DEER, FEMUR, HUMAN beings, SKULL, HUMERUS
Abstract: Whereas gunshot injuries in human craniums have been well studied, reliable data on fracture patterns in ballistic long bone trauma remains scarce. Further information useful for forensic trauma interpretation and reconstruction may be retrieved from experimentally produced gunshot fractures. In order to avoid the use of human specimens for experimental research, it is of great interest to determine whether alternative models can reproduce the ballistic fracture patterns of human long bones. To address this question, we shot seven healthy adult human femurs and humeri each, ten samples each of two different polyurethane cylinders from Synbone® and four femurs from female red deer. The specimens were embedded in ballistic gelatin and perpendicularly shot from a distance of 2 m, using a 9-mm full metal jacket projectile at an impact velocity of 360 m/s. The macroscopical appearance of the detailed fracture pattern considering entry, exit and general cortical traits as well as the bullet's energy lost upon impact were compared between the models. Despite some general similarities, neither of the two alternative models entirely reproduced the fracture patterns of human long bones. Comparing the two alternative models, the surrogate model revealed more significant differences to the human fracture than the animal model. This leads to the conclusion that the polyurethane material provides a different failure mechanism than real bone, underpinning the challenge in deploying an accurate analog. [ABSTRACT FROM AUTHOR]
Published: 2023
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21. Constraints on prerecombination early dark energy from SPT-3G public data

Author: La Posta, Adrien, primary, Louis, Thibaut, additional, Garrido, Xavier, additional, and Hill, J. Colin, additional
Published: 2022
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22. The Simons Observatory: a new open-source power spectrum pipeline applied to the Planck legacy data

Author: Li, Zack, Louis, Thibaut, Calabrese, Erminia, Jense, Hidde, Alonso, David, Bond, J. Richard, Choi, Steve K., Dunkley, Jo, Fabbian, Giulio, Garrido, Xavier, Jaffe, Andrew H., Madhavacheril, Mathew S., Meerburg, P. Daniel, Natale, Umberto, Qu, Frank J., Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), and HEP, INSPIRE
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), astro-ph.CO, FOS: Physical sciences, [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph], [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present a reproduction of the Planck 2018 angular power spectra at $\ell > 30$, and associated covariance matrices, for intensity and polarization maps at 100, 143 and 217 GHz. This uses a new, publicly available, pipeline that is part of the PSpipe package. As a test case we use the same input maps, ancillary products, and analysis choices as in the Planck 2018 analysis, and find that we can reproduce the spectra to 0.1$\sigma$ precision, and the covariance matrices to 10%. We show that cosmological parameters estimated from our re-derived products agree with the public Planck products to 0.1$\sigma$, providing an independent cross-check of the Planck team's analysis. Going forward, the publicly-available code can be easily adapted to use alternative input maps, data selections and analysis choices, for future optimal analysis of Planck data with new ground-based Cosmic Microwave Background data., Comment: 25 pages, 18 figures, code available at https://simonsobs.github.io/planck-pr3-web/
Published: 2022

23. 1st Makassar International Conference on Pharmaceutical Sciences (MICPS 2021). Faculty of Pharmacy Universitas Muslim Indonesia. Makassar, Indonesia. September 25-26, 2021

Author: Garrido, Gabino, primary, Valdés, Marisela, additional, Garrido, Xavier, additional, Fawwaz, Muammar, additional, and Ahmad, Aktsar Roskiana, additional
Published: 2021
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24. Fast computation of angular power spectra and covariances of high-resolution cosmic microwave background maps using the Toeplitz approximation

Author: Louis, Thibaut, primary, Naess, Sigurd, additional, Garrido, Xavier, additional, and Challinor, Anthony, additional
Published: 2020
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25. QUBIC: Exploring the Primordial Universe with the Q&amp

Author: Mennella, Aniello, Ade, Peter, Amico, Giorgio, Auguste, Didier, Aumont, Jonathan, Banfi, Stefano, Barbaràn, Gustavo, Battaglia, Paola, Battistelli, Elia, Baù, Alessandro, Bélier, Benoit, Bennett, David G., Bergé, Laurent, Bernard, Jean Philippe, Bersanelli, Marco, Sazy, Marie Anne Bigot, Bleurvacq, Nathan, Bonaparte, Juan, Bonis, Julien, Bunn, Emory, Burke, David, Buzi, Daniele, Buzzelli, Alessandro, Cavaliere, Francesco, Chanial, Pierre, Chapron, Claude, Charlassier, Romain, Columbro, Fabio, Coppi, Gabriele, Coppolecchia, Alessandro, D’Agostino, Rocco, D’Alessandro, Giuseppe, Bernardis, Paolo De, Gasperis, Giancarlo De, Leo, Michele De, Petris, Marco De, Donato, Andres Di, Dumoulin, Louis, Etchegoyen, Alberto, Fasciszewski, Adrián, Franceschet, Cristian, Lerena, Martin Miguel Gamboa, Garcia, Beatriz, Garrido, Xavier, Gaspard, Michel, Gault, Amanda, Gayer, Donnacha, Gervasi, Massimo, Giard, Martin, Héraud, Yannick Giraud, Berisso, Mariano Gómez, González, Manuel, Gradziel, Marcin, Grandsire, Laurent, Guerard, Eric, Hamilton, Jean Christophe, and Hara, Diego
Subjects: Cosmic Microwave Background, Astrophysics::Instrumentation and Methods for Astrophysics, B-modes, Astrophysics::Cosmology and Extragalactic Astrophysics, inflation, Astrophysics::Galaxy Astrophysics, bolometers, polarimetry
Abstract: In this paper, we describe QUBIC, an experiment that will observe the polarized microwave sky with a novel approach, which combines the sensitivity of state-of-the-art bolometric detectors with the systematic effects control typical of interferometers. QUBIC’s unique features are the so-called “self-calibration”, a technique that allows us to clean the measured data from instrumental effects, and its spectral imaging power, i.e., the ability to separate the signal into various sub-bands within each frequency band. QUBIC will observe the sky in two main frequency bands: 150 GHz and 220 GHz. A technological demonstrator is currently under testing and will be deployed in Argentina during 2019, while the final instrument is expected to be installed during 2020.
Published: 2019
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26. Comparison of results on $N_\mathrm{eff}$ from various Planck likelihoods

Author: Henrot-Versillé, Sophie, Couchot, Francois, Garrido, Xavier, Imada, Hiroaki, Louis, Thibaut, Tristram, Matthieu, Vanneste, Sylvain, Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, cosmological parameters, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: In this paper, we study the estimation of the effective number of relativistic species from a combination of CMB and BAO data. We vary different ingredients of the analysis: the Planck high-$\ell$ likelihoods, the Boltzmann solvers, and the statistical approaches. The variation of the inferred values gives an indication of an additional systematic uncertainty, which is of the same order of magnitude as the error derived from each individual likelihood. We show that this systematic is essentially associated to the assumptions made in the high-$\ell$ likelihoods implementations, in particular for the foreground residuals modellings. We also compare a subset of likelihoods using only the TE power spectra, expected to be less sensitive to foreground residuals., Comment: accepted for publication in A&A
Published: 2019

27. QUBIC: Exploring the Primordial Universe with the Q&U Bolometric Interferometer

Author: Mennella, A, Ade, P, Amico, G, Auguste, D, Aumont, J, Banfi, S, Barbaràn, G, Battaglia, P, Battistelli, E, Baù, A, Bélier, B, Bennett, D, Bergé, L, Bernard, J, Bersanelli, M, Sazy, M, Bleurvacq, N, Bonaparte, J, Bonis, J, Bunn, E, Burke, D, Buzi, D, Buzzelli, A, Cavaliere, F, Chanial, P, Chapron, C, Charlassier, R, Columbro, F, Coppi, G, Coppolecchia, A, D’Agostino, R, D’Alessandro, G, Bernardis, P, Gasperis, G, Leo, M, Petris, M, Donato, A, Dumoulin, L, Etchegoyen, A, Fasciszewski, A, Franceschet, C, Lerena, M, Garcia, B, Garrido, X, Gaspard, M, Gault, A, Gayer, D, Gervasi, M, Giard, M, Héraud, Y, Berisso, M, González, M, Gradziel, M, Grandsire, L, Guerard, E, Hamilton, J, Harari, D, Haynes, V, Versillé, S, Hoang, D, Holtzer, N, Incardona, F, Jules, E, Kaplan, J, Korotkov, A, Kristukat, C, Lamagna, L, Loucatos, S, Louis, T, Lowitz, A, Lukovic, V, Luterstein, R, Maffei, B, Marnieros, S, Masi, S, Mattei, A, May, A, Mcculloch, M, Medina, M, Mele, L, Melhuish, S, Montier, L, Mousset, L, Mundo, L, Murphy, J, O’Sullivan, C, Olivieri, E, Paiella, A, Pajot, F, Passerini, A, Pastoriza, H, Pelosi, A, Perbost, C, Perciballi, M, Pezzotta, F, Piacentini, F, Piat, M, Piccirillo, L, Pisano, G, Polenta, G, Prêle, D, Puddu, R, Rambaud, D, Ringegni, P, Romero, G, Salatino, M, Schillaci, A, Scóccola, C, Scully, S, Spinelli, S, Stankowiak, G, Stolpovskiy, M, Suarez, F, Tartari, A, Thermeau, J, Timbie, P, Tomasi, M, Torchinsky, S, Tristram, M, Tucker, C, Tucker, G, Vanneste, S, Viganò, D, Vittorio, N, Voisin, F, Watson, R, Wicek, F, Zannoni, M, Zullo, A, Mennella, Aniello, Ade, Peter, Amico, Giorgio, Auguste, Didier, Aumont, Jonathan, Banfi, Stefano, Barbaràn, Gustavo, Battaglia, Paola, Battistelli, Elia, Baù, Alessandro, Bélier, Benoit, Bennett, David, Bergé, Laurent, Bernard, Jean, Bersanelli, Marco, Sazy, Marie, Bleurvacq, Nathan, Bonaparte, Juan, Bonis, Julien, Bunn, Emory, Burke, David, Buzi, Daniele, Buzzelli, Alessandro, Cavaliere, Francesco, Chanial, Pierre, Chapron, Claude, Charlassier, Romain, Columbro, Fabio, Coppi, Gabriele, Coppolecchia, Alessandro, D’Agostino, Rocco, D’Alessandro, Giuseppe, Bernardis, Paolo, Gasperis, Giancarlo, Leo, Michele, Petris, Marco, Donato, Andres, Dumoulin, Louis, Etchegoyen, Alberto, Fasciszewski, Adrián, Franceschet, Cristian, Lerena, Martin, Garcia, Beatriz, Garrido, Xavier, Gaspard, Michel, Gault, Amanda, Gayer, Donnacha, Gervasi, Massimo, Giard, Martin, Héraud, Yannick, Berisso, Mariano, González, Manuel, Gradziel, Marcin, Grandsire, Laurent, Guerard, Eric, Hamilton, Jean, Harari, Diego, Haynes, Vic, Versillé, Sophie, Hoang, Duc, Holtzer, Nicolas, Incardona, Federico, Jules, Eric, Kaplan, Jean, Korotkov, Andrei, Kristukat, Christian, Lamagna, Luca, Loucatos, Sotiris, Louis, Thibaut, Lowitz, Amy, Lukovic, Vladimir, Luterstein, Raùl, Maffei, Bruno, Marnieros, Stefanos, Masi, Silvia, Mattei, Angelo, May, Andrew, McCulloch, Mark, Medina, Maria, Mele, Lorenzo, Melhuish, Simon, Montier, Ludovic, Mousset, Louise, Mundo, Luis, Murphy, John, Murphy, James, O’Sullivan, Creidhe, Olivieri, Emiliano, Paiella, Alessandro, Pajot, Francois, Passerini, Andrea, Pastoriza, Hernan, Pelosi, Alessandro, Perbost, Camille, Perciballi, Maurizio, Pezzotta, Federico, Piacentini, Francesco, Piat, Michel, Piccirillo, Lucio, Pisano, Giampaolo, Polenta, Gianluca, Prêle, Damien, Puddu, Roberto, Rambaud, Damien, Ringegni, Pablo, Romero, Gustavo, Salatino, Maria, Schillaci, Alessandro, Scóccola, Claudia, Scully, Stephen, Spinelli, Sebastiano, Stankowiak, Guillaume, Stolpovskiy, Michail, Suarez, Federico, Tartari, Andrea, Thermeau, Jean, Timbie, Peter, Tomasi, Maurizio, Torchinsky, Steve, Tristram, Matthieu, Tucker, Carole, Tucker, Gregory, Vanneste, Sylvain, Viganò, Daniele, Vittorio, Nicola, Voisin, Fabrice, Watson, Robert, Wicek, Francois, Zannoni, Mario, Zullo, Antonio, Mennella, A, Ade, P, Amico, G, Auguste, D, Aumont, J, Banfi, S, Barbaràn, G, Battaglia, P, Battistelli, E, Baù, A, Bélier, B, Bennett, D, Bergé, L, Bernard, J, Bersanelli, M, Sazy, M, Bleurvacq, N, Bonaparte, J, Bonis, J, Bunn, E, Burke, D, Buzi, D, Buzzelli, A, Cavaliere, F, Chanial, P, Chapron, C, Charlassier, R, Columbro, F, Coppi, G, Coppolecchia, A, D’Agostino, R, D’Alessandro, G, Bernardis, P, Gasperis, G, Leo, M, Petris, M, Donato, A, Dumoulin, L, Etchegoyen, A, Fasciszewski, A, Franceschet, C, Lerena, M, Garcia, B, Garrido, X, Gaspard, M, Gault, A, Gayer, D, Gervasi, M, Giard, M, Héraud, Y, Berisso, M, González, M, Gradziel, M, Grandsire, L, Guerard, E, Hamilton, J, Harari, D, Haynes, V, Versillé, S, Hoang, D, Holtzer, N, Incardona, F, Jules, E, Kaplan, J, Korotkov, A, Kristukat, C, Lamagna, L, Loucatos, S, Louis, T, Lowitz, A, Lukovic, V, Luterstein, R, Maffei, B, Marnieros, S, Masi, S, Mattei, A, May, A, Mcculloch, M, Medina, M, Mele, L, Melhuish, S, Montier, L, Mousset, L, Mundo, L, Murphy, J, O’Sullivan, C, Olivieri, E, Paiella, A, Pajot, F, Passerini, A, Pastoriza, H, Pelosi, A, Perbost, C, Perciballi, M, Pezzotta, F, Piacentini, F, Piat, M, Piccirillo, L, Pisano, G, Polenta, G, Prêle, D, Puddu, R, Rambaud, D, Ringegni, P, Romero, G, Salatino, M, Schillaci, A, Scóccola, C, Scully, S, Spinelli, S, Stankowiak, G, Stolpovskiy, M, Suarez, F, Tartari, A, Thermeau, J, Timbie, P, Tomasi, M, Torchinsky, S, Tristram, M, Tucker, C, Tucker, G, Vanneste, S, Viganò, D, Vittorio, N, Voisin, F, Watson, R, Wicek, F, Zannoni, M, Zullo, A, Mennella, Aniello, Ade, Peter, Amico, Giorgio, Auguste, Didier, Aumont, Jonathan, Banfi, Stefano, Barbaràn, Gustavo, Battaglia, Paola, Battistelli, Elia, Baù, Alessandro, Bélier, Benoit, Bennett, David, Bergé, Laurent, Bernard, Jean, Bersanelli, Marco, Sazy, Marie, Bleurvacq, Nathan, Bonaparte, Juan, Bonis, Julien, Bunn, Emory, Burke, David, Buzi, Daniele, Buzzelli, Alessandro, Cavaliere, Francesco, Chanial, Pierre, Chapron, Claude, Charlassier, Romain, Columbro, Fabio, Coppi, Gabriele, Coppolecchia, Alessandro, D’Agostino, Rocco, D’Alessandro, Giuseppe, Bernardis, Paolo, Gasperis, Giancarlo, Leo, Michele, Petris, Marco, Donato, Andres, Dumoulin, Louis, Etchegoyen, Alberto, Fasciszewski, Adrián, Franceschet, Cristian, Lerena, Martin, Garcia, Beatriz, Garrido, Xavier, Gaspard, Michel, Gault, Amanda, Gayer, Donnacha, Gervasi, Massimo, Giard, Martin, Héraud, Yannick, Berisso, Mariano, González, Manuel, Gradziel, Marcin, Grandsire, Laurent, Guerard, Eric, Hamilton, Jean, Harari, Diego, Haynes, Vic, Versillé, Sophie, Hoang, Duc, Holtzer, Nicolas, Incardona, Federico, Jules, Eric, Kaplan, Jean, Korotkov, Andrei, Kristukat, Christian, Lamagna, Luca, Loucatos, Sotiris, Louis, Thibaut, Lowitz, Amy, Lukovic, Vladimir, Luterstein, Raùl, Maffei, Bruno, Marnieros, Stefanos, Masi, Silvia, Mattei, Angelo, May, Andrew, McCulloch, Mark, Medina, Maria, Mele, Lorenzo, Melhuish, Simon, Montier, Ludovic, Mousset, Louise, Mundo, Luis, Murphy, John, Murphy, James, O’Sullivan, Creidhe, Olivieri, Emiliano, Paiella, Alessandro, Pajot, Francois, Passerini, Andrea, Pastoriza, Hernan, Pelosi, Alessandro, Perbost, Camille, Perciballi, Maurizio, Pezzotta, Federico, Piacentini, Francesco, Piat, Michel, Piccirillo, Lucio, Pisano, Giampaolo, Polenta, Gianluca, Prêle, Damien, Puddu, Roberto, Rambaud, Damien, Ringegni, Pablo, Romero, Gustavo, Salatino, Maria, Schillaci, Alessandro, Scóccola, Claudia, Scully, Stephen, Spinelli, Sebastiano, Stankowiak, Guillaume, Stolpovskiy, Michail, Suarez, Federico, Tartari, Andrea, Thermeau, Jean, Timbie, Peter, Tomasi, Maurizio, Torchinsky, Steve, Tristram, Matthieu, Tucker, Carole, Tucker, Gregory, Vanneste, Sylvain, Viganò, Daniele, Vittorio, Nicola, Voisin, Fabrice, Watson, Robert, Wicek, Francois, Zannoni, Mario, and Zullo, Antonio
Abstract: In this paper, we describe QUBIC, an experiment that will observe the polarized microwave sky with a novel approach, which combines the sensitivity of state-of-the-art bolometric detectors with the systematic effects control typical of interferometers. QUBIC’s unique features are the so-called “self-calibration”, a technique that allows us to clean the measured data from instrumental effects, and its spectral imaging power, i.e., the ability to separate the signal into various sub-bands within each frequency band. QUBIC will observe the sky in two main frequency bands: 150GHz and 220 GHz. A technological demonstrator is currently under testing and will be deployed in Argentina during 2019, while the final instrument is expected to be installed during 2020
Published: 2019

28. QUBIC: Exploring the Primordial Universe with the Q&U Bolometric Interferometer

Author: Mennella, A., Ade, P.A.R., Amico, G., Auguste, D., Aumont, J., Banfi, S., Barbaràn, Gustavo, Battaglia, P., Battistelli, E., Bau, A., Bélier, B., Bennett, D., Bergé, L., Bernard, J.-P., Bersanelli, M., Bigot-Sazy, M.-A., Bleurvacq, N., Bonaparte, J., Bonis, J., Bunn, E.F., Burke, D., Buzi, D., Buzzelli, A., Cavaliere, F., Chanial, P., Chapron, C., Charlassier, R., Columbro, F., Coppi, G., Coppolecchia, A., D’Agostino, Rocco, D’Alessandro, Giuseppe, De Bernardis, P., de Gasperis, G., De Leo, M., De Petris, M., Di Donato, Andres, Dumoulin, L., Etchegoyen, A., Fasciszewski, Adrián, Franceschet, C., Gamboa Lerena, M.M., Garcia, B., Garrido, Xavier, Gaspard, M., Gault, A., Gayer, D., Gervasi, M., Giard, M., Giraud Héraud, Yannick, Gómez Berisso, Mariano, González, M., Gradziel, Marcin, Grandsire, L., Guerard, Eric, Hamilton, J.-Ch., Harari, D., Haynes, V., Henrot Versillé, Sophie, Hoang, D.T., Holtzer, N., Incardona, F., Jules, E., Kaplan, J., Korotkov, A., Kristukat, C., Lamagna, L., Loucatos, S., Louis, T., Lowitz, A., Lukovic, V., Luterstein, R., Maffei, B., Marnieros, S., Masi, S., Mattei, Angelo, May, A., McCulloch, M., Medina, M.C., Mele, L., Melhuish, S.J., Montier, L., Mousset, L., Mundo, L.M., Murphy, J.Anthony, Murphy, J.D., O'Sullivan, Créidhe, Olivieri, E., Paiella, A., Pajot, F., Passerini, A., Pastoriza, Hernan, Pelosi, A., Perbost, C., Perciballi, M., Pezzotta, F., Piacentini, F., Piat, M., Piccirillo, L., Pisano, G., Plenta, Gianluca, Prêle, D., Puddu, R., Rambaud, D., Ringegni, Pablo, Romero, G.E., Salatino, M., Schillaci, A., Scóccola, Claudia G., Scully, S., Spinelli, S., Stankowiak, Guillaume, Stolpovskiy, M., Suarez, F., Tartari, A., Thermeau, Jean Pierre, Timbie, P., Tomasi, M., Torchinsky, S., Tristram, M., Tucker, C., Tucker, G., Vanneste, S., Viganò, D., Vittorio, Nicola, Voisin, F., Watson, Robert, Wicek, F., Zannoni, M., Zullo, Antonio, Mennella, A., Ade, P.A.R., Amico, G., Auguste, D., Aumont, J., Banfi, S., Barbaràn, Gustavo, Battaglia, P., Battistelli, E., Bau, A., Bélier, B., Bennett, D., Bergé, L., Bernard, J.-P., Bersanelli, M., Bigot-Sazy, M.-A., Bleurvacq, N., Bonaparte, J., Bonis, J., Bunn, E.F., Burke, D., Buzi, D., Buzzelli, A., Cavaliere, F., Chanial, P., Chapron, C., Charlassier, R., Columbro, F., Coppi, G., Coppolecchia, A., D’Agostino, Rocco, D’Alessandro, Giuseppe, De Bernardis, P., de Gasperis, G., De Leo, M., De Petris, M., Di Donato, Andres, Dumoulin, L., Etchegoyen, A., Fasciszewski, Adrián, Franceschet, C., Gamboa Lerena, M.M., Garcia, B., Garrido, Xavier, Gaspard, M., Gault, A., Gayer, D., Gervasi, M., Giard, M., Giraud Héraud, Yannick, Gómez Berisso, Mariano, González, M., Gradziel, Marcin, Grandsire, L., Guerard, Eric, Hamilton, J.-Ch., Harari, D., Haynes, V., Henrot Versillé, Sophie, Hoang, D.T., Holtzer, N., Incardona, F., Jules, E., Kaplan, J., Korotkov, A., Kristukat, C., Lamagna, L., Loucatos, S., Louis, T., Lowitz, A., Lukovic, V., Luterstein, R., Maffei, B., Marnieros, S., Masi, S., Mattei, Angelo, May, A., McCulloch, M., Medina, M.C., Mele, L., Melhuish, S.J., Montier, L., Mousset, L., Mundo, L.M., Murphy, J.Anthony, Murphy, J.D., O'Sullivan, Créidhe, Olivieri, E., Paiella, A., Pajot, F., Passerini, A., Pastoriza, Hernan, Pelosi, A., Perbost, C., Perciballi, M., Pezzotta, F., Piacentini, F., Piat, M., Piccirillo, L., Pisano, G., Plenta, Gianluca, Prêle, D., Puddu, R., Rambaud, D., Ringegni, Pablo, Romero, G.E., Salatino, M., Schillaci, A., Scóccola, Claudia G., Scully, S., Spinelli, S., Stankowiak, Guillaume, Stolpovskiy, M., Suarez, F., Tartari, A., Thermeau, Jean Pierre, Timbie, P., Tomasi, M., Torchinsky, S., Tristram, M., Tucker, C., Tucker, G., Vanneste, S., Viganò, D., Vittorio, Nicola, Voisin, F., Watson, Robert, Wicek, F., Zannoni, M., and Zullo, Antonio
Abstract: In this paper, we describe QUBIC, an experiment that will observe the polarized microwave sky with a novel approach, which combines the sensitivity of state-of-the-art bolometric detectors with the systematic effects control typical of interferometers. QUBIC’s unique features are the so-called “self-calibration”, a technique that allows us to clean the measured data from instrumental effects, and its spectral imaging power, i.e., the ability to separate the signal into various sub-bands within each frequency band. QUBIC will observe the sky in two main frequency bands: 150 GHz and 220 GHz. A technological demonstrator is currently under testing and will be deployed in Argentina during 2019, while the final instrument is expected to be installed during 2020.
Published: 2019

29. Factors objectius i de significació que influeixen en la implementació de robots socials assistencials (RSA) per a la millora de la qualitat de vida de la gent gran

Author: Corbera Garrido, Xavier and López Catalán, Óscar
Subjects: aging population, Psicologia social -- TFG, Social psychology -- TFG, cura de la gent gran, inteligencia artificial, cuidado de la gente mayor, elderly care, social construction of concepts, Psicología social -- TFG, social assistance robots, envelliment de la població, envejecimiento de la población, artificial intelligence, intel·ligència artificial, construcció social de conceptes, robots socials assistencials, construcción social de conceptos, robots sociales asistenciales
Abstract: El continu increment de la població de més edat pot posar al límit la capacitat dels sistemes de protecció social per tal de garantir la seva cura i faran falta grans recursos socials, mèdics, econòmics i per a cobrir totes les necessitats del col·lectiu. La intel·ligència artificial i els robots esdevenen uns factors a tenir en compte en un futur proper per ajudar a garantir la sostenibilitat del sistema social de benestar, però caldrà tenir en compte quins són els factors objectius i de significació que facilitaran i dificultaran aquesta implementació que es fa necessària amb les perspectives actuals. The continuous increase of the older population can put the capacity of the social protection systems to the limit to guarantee their care and will require great social, medical, economic resources and to cover all the needs of the group. Artificial intelligence and robots become factors to be taken in consideration in the near future to help ensure the sustainability of the social welfare system, but we must take into account the objective and meaningful factors that will facilitate and hinder this implementation which is necessary with the current perspectives. El continuo incremento de la población de más edad puede posar al límite la capacidad de los sistemas de protección social para garantizar su cura y harán falta grandes recursos sociales, médicos, económicos y para cubrir todas las necesidades del colectivo. La inteligencia artificial y los robots acontecen unos factores a tener en cuenta en un futuro próximo para ayudar a garantizar la sostenibilidad del sistema social de bienestar, pero habrá que tener en cuenta cuáles son los factores objetivos y de significación que facilitarán y dificultarán esta implementación que se hace necesaria con las perspectivas actuales.
Published: 2018

30. Consistency of CMB experiments beyond cosmic variance

Author: Louis, Thibaut, primary, Garrido, Xavier, additional, Soussana, Adam, additional, Tristram, Matthieu, additional, Henrot-Versillé, Sophie, additional, and Vanneste, Sylvain, additional
Published: 2019
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31. Use of aspirin for primary and secondary prevention of cardiovascular disease in diabetic patients in an ambulatory care setting in Spain

Author: Fernández-de-Bobadilla Jaime, Rejas-Gutiérrez Javier, Navarro-Artieda Ruth, Sicras-Mainar Antoni, Frías-Garrido Xavier, and Ruiz-Riera Rafael
Subjects: Medicine (General), R5-920
Abstract: Abstract Background This study was conducted in order to determine the use of aspirin and to assess the achievement of therapeutic targets in diabetic patients according to primary (PP) or secondary prevention (SP). Methods This is a retrospective, observational study including patients ≥18 years with diabetes mellitus followed in four primary care centers. Measurements included demographics, use of aspirin and/or anticoagulant drugs, co-morbidities, clinical parameters and proportion of patient at therapeutic target (TT). Descriptive statistics, chi-square test and logistic regression model were used for significance. Results A total of 4,140 patients were analyzed, 79.1% (95% confidence intervals [CI]: 77.7–80.5%) in PP and 20.9% (95% CI: 18.2–23.7%) in SP. Mean age was 64.1 (13.8) years, and 49.3% of patient were men (PP: 46.3, SP: 60.7, p = 0.001). Aspirin was prescribed routinely in 20.8% (95% CI: 19.4–22.2%) in PP and 60.8% (95% CI: 57.6–64.0%) in SP. Proportion of patient at TT was 48.0% for blood pressure and 59.8% for cholesterol. Use of aspirin was associated to increased age [OR = 1.01 (95% CI: 1.00–1.02); p = 0.011], cardiovascular-risk factors [OR = 1.14 (95% CI: 1.03–1.27); p = 0.013], LDL-C [OR = 1.42 (95% CI: 1.06–1.88); p = 0.017] and higher glycated hemoglobin [OR = 1.51 (95% CI: 1.22–1.89); p = 0.000] were covariates associated to the use of aspirin in PP. Conclusion Treatment with aspirin is underused for PP in patients with diabetes mellitus in Primary Care. Achievement of TT should be improved.
Published: 2007
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32. Simulations and performance of the QUBIC optical beam combiner

Author: O'Sullivan, Créidhe, Burke, D., Gayer, D., Murphy, J.D., Scully, S., De Leo, M., De Petris, M., Mattei, Angelo, Zullo, Antonio, Mennella, A., Zannoni, M., Bleurvacq, N., Chapron, C., Hamilton, J.-Ch., Piat, M., Ade, P.A.R., Amico, G., Auguste, D., Aumont, J., Banfi, S., Barbaràn, Gustavo, Battaglia, P., Battistelli, E., Bau, A., Bélier, B., Bennett, D., Bergé, L., Bernard, J.-P., Bersanelli, M., Bigot-Sazy, M.-A., Bonaparte, J., Bonis, J., Bordier, G., Breelle, E., Bunn, E.F., Buzi, D., Buzzelli, A., Cavaliere, F., Chanial, P., Charlassier, R., Columbro, F., Coppi, G., Coppolecchia, A., Couchot, F., D'Agostino, R., D'Alessandro, G., De Bernardis, P., de Gasperis, G., Di Donato, A., Dumoulin, L., Etchegoyen, A., Fasciszewski, Adrián, Franceschet, C., Gamboa Lerena, M.M., Garcia, B., Garrido, Xavier, Gaspard, M., Gault, A., Gervasi, M., Giard, M., Giraud-Héraud, Y., Gómez Berisso, Mariano, González, M., Gradziel, Marcin, Grandsire, L., Guerrard, E., Harari, D., Haynes, V., Henrot-Versille, S., Hoang, D.T., Incardona, F., Jules, E., Kaplan, J., Korotkov, A., Kristukat, C., Lamagna, L., Loucatos, S., Louis, T., Lowitz, A., Lukovic, V., Luterstein, R., Maffei, B., Marnieros, S., Masi, S., May, A., McCulloch, M., Medina, M.C., Mele, L., Melhuish, S., Montier, L., Mundo, L.M., Murphy, J.Anthony, Olivieri, E., Paiella, A., Pajot, F., Passerini, A., Pastoriza, Hernan, Pelosi, A., Perbost, C., Perdereau, O., Pezzotta, F., Piacentini, F., Piccirillo, L., Pisano, G., Polenta, G., Prêle, D., Puddu, R., Rambaud, D., Ringegni, Pablo, Romero, G.E., Salatino, M., Schillaci, A., Scóccola, Claudia G., Spinelli, S., Stolpovskiy, M., Suarez, F., Tartari, A., Thermeau, Jean Pierre, Timbie, P., Torchinsky, S., Tristram, M., Truongcanh, V., Tucker, C., Tucker, G., Vanneste, S., Viganò, D., Vittorio, N., Voisin, F., Watson, B., Wicek, F., O'Sullivan, Créidhe, Burke, D., Gayer, D., Murphy, J.D., Scully, S., De Leo, M., De Petris, M., Mattei, Angelo, Zullo, Antonio, Mennella, A., Zannoni, M., Bleurvacq, N., Chapron, C., Hamilton, J.-Ch., Piat, M., Ade, P.A.R., Amico, G., Auguste, D., Aumont, J., Banfi, S., Barbaràn, Gustavo, Battaglia, P., Battistelli, E., Bau, A., Bélier, B., Bennett, D., Bergé, L., Bernard, J.-P., Bersanelli, M., Bigot-Sazy, M.-A., Bonaparte, J., Bonis, J., Bordier, G., Breelle, E., Bunn, E.F., Buzi, D., Buzzelli, A., Cavaliere, F., Chanial, P., Charlassier, R., Columbro, F., Coppi, G., Coppolecchia, A., Couchot, F., D'Agostino, R., D'Alessandro, G., De Bernardis, P., de Gasperis, G., Di Donato, A., Dumoulin, L., Etchegoyen, A., Fasciszewski, Adrián, Franceschet, C., Gamboa Lerena, M.M., Garcia, B., Garrido, Xavier, Gaspard, M., Gault, A., Gervasi, M., Giard, M., Giraud-Héraud, Y., Gómez Berisso, Mariano, González, M., Gradziel, Marcin, Grandsire, L., Guerrard, E., Harari, D., Haynes, V., Henrot-Versille, S., Hoang, D.T., Incardona, F., Jules, E., Kaplan, J., Korotkov, A., Kristukat, C., Lamagna, L., Loucatos, S., Louis, T., Lowitz, A., Lukovic, V., Luterstein, R., Maffei, B., Marnieros, S., Masi, S., May, A., McCulloch, M., Medina, M.C., Mele, L., Melhuish, S., Montier, L., Mundo, L.M., Murphy, J.Anthony, Olivieri, E., Paiella, A., Pajot, F., Passerini, A., Pastoriza, Hernan, Pelosi, A., Perbost, C., Perdereau, O., Pezzotta, F., Piacentini, F., Piccirillo, L., Pisano, G., Polenta, G., Prêle, D., Puddu, R., Rambaud, D., Ringegni, Pablo, Romero, G.E., Salatino, M., Schillaci, A., Scóccola, Claudia G., Spinelli, S., Stolpovskiy, M., Suarez, F., Tartari, A., Thermeau, Jean Pierre, Timbie, P., Torchinsky, S., Tristram, M., Truongcanh, V., Tucker, C., Tucker, G., Vanneste, S., Viganò, D., Vittorio, N., Voisin, F., Watson, B., and Wicek, F.
Abstract: QUBIC, the Q & U Bolometric Interferometer for Cosmology, is a novel ground-based instrument that aims to measure the extremely faint B-mode polarisation anisotropy of the cosmic microwave background at intermediate angular scales (multipoles of
Published: 2018

33. Thermal architecture for the QUBIC cryogenic receiver

Author: May, A., Chapron, C., Coppi, G., D'Alessandro, G., De Bernardis, P., Masi, S., Melhuish, S., Piat, M., Piccirillo, L., Schillaci, A., Thermeau, Jean Pierre, Ade, P.A.R., Amico, G., Auguste, D., Aumont, J., Banfi, S., Barbaràn, Gustavo, Battaglia, P., Battistelli, E., Bau, A., Bélier, B., Bennett, D., Bergé, L., Bernard, J.-P., Bersanelli, M., Bigot-Sazy, M.-A., Bleurvacq, N., Bonaparte, J., Bonis, J., Bordier, G., Breelle, E., Bunn, E.F., Burke, D., Buzi, D., Buzzelli, A., Cavaliere, F., Chanial, P., Charlassier, R., Columbro, F., Coppolecchia, A., Couchot, F., D'Agostino, R., de Gasperis, G., De Leo, M., De Petris, M., Di Donato, Andres, Dumoulin, L., Etchegoyen, A., Fasciszewski, Adrián, Franceschet, C., Gamboa Lerena, M.M., Garcia, G., Garrido, Xavier, Gaspard, M., Gault, A., Gayer, D., Gervasi, M., Giard, M., Giraud-Héraud, Y., Gómez Berisso, Mariano, González, M., Gradziel, Marcin, Grandsire, L., Guerrard, E., Hamilton, J.-Ch., Harari, D., Haynes, V., Henrot-Versille, S., Hoang, D.T., Incardona, F., Jules, E., Kaplan, J., Korotkov, A., Kirstukat, C., Lamagna, L., Loucatos, S., Louis, T., Lowitz, A., Lukovic, V., Luterstein, R., Maffei, B., Marnieros, S., Mattei, Angelo, McCulloch, M., Medina, M.C., Mele, L., Mennella, A., Montier, L., Mundo, L.M., Murphy, J.Anthony, Murphy, J.D., O'Sullivan, Créidhe, Olivieri, E., Paiella, A., Pajot, F., Passerini, A., Pastoriza, H., Pelosi, A., Perbost, C., Perdereau, O., Pezzotta, F., Piacentini, F., Pisano, G., Polenta, G., Prêle, D., Puddu, R., Rambaud, D., Ringegni, Pablo, Romero, G.E., Salatino, M., Scóccola, Claudia G., Scully, S., Spinelli, S., Stolpovskiy, M., Suarez, F., Tartari, A., Timbie, P., Torchinsky, S., Tristram, M., Truongcanh, V., Tucker, C., Tucker, G., Vanneste, S., Viganò, D., Vittorio, N., Voisin, F., Watson, B., Wicek, F., Zannoni, M., Zullo, Antonio, May, A., Chapron, C., Coppi, G., D'Alessandro, G., De Bernardis, P., Masi, S., Melhuish, S., Piat, M., Piccirillo, L., Schillaci, A., Thermeau, Jean Pierre, Ade, P.A.R., Amico, G., Auguste, D., Aumont, J., Banfi, S., Barbaràn, Gustavo, Battaglia, P., Battistelli, E., Bau, A., Bélier, B., Bennett, D., Bergé, L., Bernard, J.-P., Bersanelli, M., Bigot-Sazy, M.-A., Bleurvacq, N., Bonaparte, J., Bonis, J., Bordier, G., Breelle, E., Bunn, E.F., Burke, D., Buzi, D., Buzzelli, A., Cavaliere, F., Chanial, P., Charlassier, R., Columbro, F., Coppolecchia, A., Couchot, F., D'Agostino, R., de Gasperis, G., De Leo, M., De Petris, M., Di Donato, Andres, Dumoulin, L., Etchegoyen, A., Fasciszewski, Adrián, Franceschet, C., Gamboa Lerena, M.M., Garcia, G., Garrido, Xavier, Gaspard, M., Gault, A., Gayer, D., Gervasi, M., Giard, M., Giraud-Héraud, Y., Gómez Berisso, Mariano, González, M., Gradziel, Marcin, Grandsire, L., Guerrard, E., Hamilton, J.-Ch., Harari, D., Haynes, V., Henrot-Versille, S., Hoang, D.T., Incardona, F., Jules, E., Kaplan, J., Korotkov, A., Kirstukat, C., Lamagna, L., Loucatos, S., Louis, T., Lowitz, A., Lukovic, V., Luterstein, R., Maffei, B., Marnieros, S., Mattei, Angelo, McCulloch, M., Medina, M.C., Mele, L., Mennella, A., Montier, L., Mundo, L.M., Murphy, J.Anthony, Murphy, J.D., O'Sullivan, Créidhe, Olivieri, E., Paiella, A., Pajot, F., Passerini, A., Pastoriza, H., Pelosi, A., Perbost, C., Perdereau, O., Pezzotta, F., Piacentini, F., Pisano, G., Polenta, G., Prêle, D., Puddu, R., Rambaud, D., Ringegni, Pablo, Romero, G.E., Salatino, M., Scóccola, Claudia G., Scully, S., Spinelli, S., Stolpovskiy, M., Suarez, F., Tartari, A., Timbie, P., Torchinsky, S., Tristram, M., Truongcanh, V., Tucker, C., Tucker, G., Vanneste, S., Viganò, D., Vittorio, N., Voisin, F., Watson, B., Wicek, F., Zannoni, M., and Zullo, Antonio
Abstract: QUBIC, the QU Bolometric Interferometer for Cosmology, is a novel forthcoming instrument to measure the B-mode polarization anisotropy of the Cosmic Microwave Background. The detection of the B-mode signal will be extremely challenging; QUBIC has been designed to address this with a novel approach, namely bolometric interferometry. The receiver cryostat is exceptionally large and cools complex optical and detector stages to 40 K, 4 K, 1 K and 350 mK using two pulse tube coolers, a novel 4He sorption cooler and a double-stage 3He/4He sorption cooler. We discuss the thermal and mechanical design of the cryostat, modelling and thermal analysis, and laboratory cryogenic testing
Published: 2018

34. Performance of NbSi transition-edge sensors readout with a 128 MUX factor for the QUBIC experiment

Author: Salatino, M., Bélier, B., Chapron, C., Hoang, D.T., Maestre, S., Marnieros, S., Marty, W., Montier, L., Piat, M., Prêle, D., Rambaud, D., Stankowiak, Guillaume, Thermeau, Jean Pierre, Torchinsky, S., Henrot-Versille, S., Voisin, F., Ade, P.A.R., Amico, G., Auguste, D., Aumont, J., Banfi, S., Barbaràn, Gustavo, Battaglia, P., Battistelli, E., Bau, A., Bennett, D., Bergé, L., Bernard, J.-P., Bersanelli, M., Bigot-Sazy, M.-A., Bleurvacq, N., Bonaparte, J., Bonis, J., Bordier, G., Breelle, E., Bunn, E.F., Burke, D., Buzi, D., Busselli, A., Cavaliere, F., Chanial, P., Charlassier, R., Columbro, F., Coppi, G., Coppolecchia, A., Couchot, F., D'Agostino, R., D'Alessandro, G., De Bernardis, P., de Gasperis, G., De Leo, M., De Petris, M., Di Donato, Andres, Dumoulin, L., Etchegoyen, A., Fasciszewski, Adrián, Franceschet, C., Gamboa Lerena, M.M., Garcia, B., Garrido, Xavier, Gaspard, M., Gault, A., Gayer, D., Gervasi, M., Giard, M., Giraud-Héraud, Y., Gómez Berisso, Mariano, González, M., Gradziel, Marcin, Grandsire, L., Guerrard, E., Hamilton, J.-Ch., Harari, D., Haynes, V., Incardona, F., Jules, E., Kaplan, J., Korotkov, A., Kristukat, C., Lamagna, L., Loucatos, S., Louis, T., Lowitz, A., Lukovic, V., Luterstein, R., Maffei, B., Masi, S., Mattei, Angelo, May, A.J., McCulloch, M., Medina, M.C., Mele, L., Melhuish, S.J., Mennella, A., Mundo, L.M., Murphy, J.Anthony, Murphy, J.D., O'Sullivan, Créidhe, Olivieri, E., Paiella, A., Pajot, F., Passerini, A., Pastoriza, Hernan, Pelosi, A., Perbost, C., Perdereau, O., Pezzotta, F., Piacentini, F., Piccirillo, L., Pisano, G., Polenta, G., Puddu, R., Ringegni, P., Romero, G.E., Schillaci, A., Scóccola, Claudia G., Scully, S., Spinelli, S., Stolpovskiy, M., Suarez, F., Tartari, A., Timbie, P., Tristram, M., Truongcanh, V., Tucker, C., Tucker, G., Vanneste, S., Viganò, D., Vittorio, N., Watson, B., Wicek, F., Zannoni, M., Zullo, A., Salatino, M., Bélier, B., Chapron, C., Hoang, D.T., Maestre, S., Marnieros, S., Marty, W., Montier, L., Piat, M., Prêle, D., Rambaud, D., Stankowiak, Guillaume, Thermeau, Jean Pierre, Torchinsky, S., Henrot-Versille, S., Voisin, F., Ade, P.A.R., Amico, G., Auguste, D., Aumont, J., Banfi, S., Barbaràn, Gustavo, Battaglia, P., Battistelli, E., Bau, A., Bennett, D., Bergé, L., Bernard, J.-P., Bersanelli, M., Bigot-Sazy, M.-A., Bleurvacq, N., Bonaparte, J., Bonis, J., Bordier, G., Breelle, E., Bunn, E.F., Burke, D., Buzi, D., Busselli, A., Cavaliere, F., Chanial, P., Charlassier, R., Columbro, F., Coppi, G., Coppolecchia, A., Couchot, F., D'Agostino, R., D'Alessandro, G., De Bernardis, P., de Gasperis, G., De Leo, M., De Petris, M., Di Donato, Andres, Dumoulin, L., Etchegoyen, A., Fasciszewski, Adrián, Franceschet, C., Gamboa Lerena, M.M., Garcia, B., Garrido, Xavier, Gaspard, M., Gault, A., Gayer, D., Gervasi, M., Giard, M., Giraud-Héraud, Y., Gómez Berisso, Mariano, González, M., Gradziel, Marcin, Grandsire, L., Guerrard, E., Hamilton, J.-Ch., Harari, D., Haynes, V., Incardona, F., Jules, E., Kaplan, J., Korotkov, A., Kristukat, C., Lamagna, L., Loucatos, S., Louis, T., Lowitz, A., Lukovic, V., Luterstein, R., Maffei, B., Masi, S., Mattei, Angelo, May, A.J., McCulloch, M., Medina, M.C., Mele, L., Melhuish, S.J., Mennella, A., Mundo, L.M., Murphy, J.Anthony, Murphy, J.D., O'Sullivan, Créidhe, Olivieri, E., Paiella, A., Pajot, F., Passerini, A., Pastoriza, Hernan, Pelosi, A., Perbost, C., Perdereau, O., Pezzotta, F., Piacentini, F., Piccirillo, L., Pisano, G., Polenta, G., Puddu, R., Ringegni, P., Romero, G.E., Schillaci, A., Scóccola, Claudia G., Scully, S., Spinelli, S., Stolpovskiy, M., Suarez, F., Tartari, A., Timbie, P., Tristram, M., Truongcanh, V., Tucker, C., Tucker, G., Vanneste, S., Viganò, D., Vittorio, N., Watson, B., Wicek, F., Zannoni, M., and Zullo, A.
Abstract: QUBIC (the Q&U Bolometric Interferometer for Cosmology) is a ground-based experiment which seeks to improve the current constraints on the amplitude of primordial gravitational waves. It exploits the unique technique, among Cosmic Microwave Background experiments, of bolometric interferometry, combining together the sensitivity of bolometric detectors with the control of systematic effects typical of interferometers. QUBIC will perform sky observations in polarization, in two frequency bands centered at 150 and 220 GHz, with two kilopixel focal plane arrays of NbSi Transition-Edge Sensors (TES) cooled down to 350 mK. A subset of the QUBIC instrument, the so called QUBIC Technological Demonstrator (TD), with a reduced number of detectors with respect to the full instrument, will be deployed and commissioned before the end of 2018. The voltage-biased TES are read out with Time Domain Multiplexing and an unprecedented multiplexing (MUX) factor equal to 128. This MUX factor is reached with two-stage multiplexing: a traditional one exploiting Superconducting QUantum Interference Devices (SQUIDs) at 1 K and a novel SiGe Application-Specific Integrated Circuit (ASIC) at 60 K. The former provides a MUX factor of 32, while the latter provides a further 4. Each TES array is composed of 256 detectors and read out with four modules of 32 SQUIDs and two ASICs. A custom software synchronizes and manages the readout and detector operation, while the TES are sampled at 780 Hz (100kHz/128 MUX rate). In this work we present the experimental characterization of the QUBIC TES arrays and their multiplexing readout chain, including time constant, critical temperature, and noise properties.
Published: 2018

35. Dementia‐specific drug treatment in home care settings: A German multicentre study

Author: Schütz, Leonhard H., primary, Boronat‐Garrido, Xavier, additional, Moser, Fabian A., additional, Suhr, Ralf, additional, and Lahmann, Nils, additional
Published: 2018
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36. Dementia‐specific drug treatment in home care settings: A German multicentre study.

Author: Schütz, Leonhard H., Boronat‐Garrido, Xavier, Moser, Fabian A., Suhr, Ralf, and Lahmann, Nils
Subjects: *ANTICONVULSANTS, *ANTIDEPRESSANTS, *ANTIPSYCHOTIC agents, *CHI-squared test, *CONFIDENCE intervals, *DEMENTIA, *HEALTH care teams, *HOME care services, *MEDICAL quality control, *MEDICAL cooperation, *MULTIVARIATE analysis, *RESEARCH, *STATISTICS, *SURVEYS, *T-test (Statistics), *TRANQUILIZING drugs, *MULTIPLE regression analysis, *CROSS-sectional method, *DATA analysis software, *DESCRIPTIVE statistics, *MEMANTINE, *ODDS ratio
Abstract: Aims and objectives: The aim of this study was to identify and analyse factors influencing the use of drugs for dementia treatment in home care settings. Background: While the number of care‐dependent people with dementia is growing, it is not clear whether their medication follows the state of the art, especially in home care settings where over two‐thirds of them are cared for in Germany. Although dementia is not curable, it is possible to reduce cognitive, behavioural and psychological symptoms of dementia with the appropriate use of medication. However, there is a lack of information concerning the drug treatment in home care settings. Methods: The study was conducted as a multicentre cross‐sectional survey, including 923 participants from 102 home care institutions throughout Germany. Medical diagnosis, medication, consultations with a specialist within the previous 12 weeks of the initial assessment and additional general information were assessed following a standardised study protocol. Data were analysed using univariate and multivariate statistical methods. The manuscript was developed utilising the STROBE checklist for cross‐sectional studies. Results: In home care, one in seven clients (14.8%) is diagnosed with some form of dementia. 52.6% (n = 72) of them were treated with dementia medication: AchEIs 16.1% (n = 22), memantine 9.5% (n = 13), antidepressants 23.4% (n = 32), antipsychotic medication 9.5% (n = 13), tranquilisers 16.8% (n = 23) and anticonvulsant drugs 6.6% (n = 9). Drug treatment for dementia was significantly associated with the consultation of a neurologist/psychiatrist in the previous 12 weeks. Conclusions: It has been demonstrated that the use of drugs as a component of home care treatment for dementia depends on many factors and therefore varies. Relevance to clinical practice: It can be assumed that people living with dementia in home care settings are not sufficiently supplied with medication. Their medical care can be improved by establishing interdisciplinary care involving a neurologist/psychiatrist. [ABSTRACT FROM AUTHOR]
Published: 2019
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37. Incontinence-Associated Dermatitis in Nursing Homes

Author: Boronat-Garrido, Xavier, primary, Kottner, Jan, additional, Schmitz, Gabriela, additional, and Lahmann, Nils, additional
Published: 2016
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38. Study of the composition of ultra-high energy cosmic rays detected by the Pierre Auger Observatory and analysis of the associated hadronic mechanisms

Author: Garrido, Xavier, Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire SUBATECH Nantes (SUBATECH), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Université de Nantes, Alain Cordier, and Observatoire Pierre Auger
Subjects: composition analysis, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], cosmic rays, processus hadroniques, Observatoire Pierre Auger, analyse composition, section efficace cosmique air, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], muons, hadronic processes, Pierre Auger Observatory, rayons cosmiques, cosmic air cross section
Abstract: Ultra high energy cosmic rays (UHECR), i.e. E > 1 EeV, raise many questions about their origin and constitute a challenge to modern physics. These cosmic rays entering the atmosphere dissipate their huge energy by generating a shower of secondary particles whose development is significantly different depending on the nature of the primaries. The study of the composition of UHECR is therefore a major interest both in understanding the hadronic processes which govern the evolution of showers and in identifying the sources of this radiation. Given its hybrid structure and the size of its unmatched network of ground detectors, the Pierre Auger Observatory can provide clear answers to the issues raised by UHECR. In this thesis, we are particularly interested in the muon component of air showers. First, we show how the hadronic parameters define the production of muons. Then we present an original method to extract this muon component and deduce the implications on the composition of UHECR. The results of this approach suggest a transition from a heavy composition to a light one when the energy increases. Finally, we address the measurement of cosmic-air cross section and present the first results derived from the Pierre Auger Observatory data.; Les rayons cosmiques d'ultra-hautes énergies (RCUHE), i.e. E > 1 EeV, soulèvent de nombreuses interrogations quant à leur origine et constituent un défi à la physique contemporaine. Ces rayons cosmiques qui pénètrent dans l'atmosphère dissipent leur exceptionnelle énergie dans la formation de gerbes de particules secondaires dont le développement est sensiblement différent suivant la nature de la particule primaire. L'étude de la composition des RCUHEs revêt donc un intérêt majeur tant dans la compréhension des processus hadroniques qui régissent l'évolution des gerbes que dans l'identification des sources de ce rayonnement. L'Observatoire Pierre Auger peut, eu égard à sa structure hybride et à la taille inégalée de son réseau de détecteurs au sol, apporter des réponses claires aux problématiques soulevées par les RCUHEs. Au cours de cette thèse, nous nous sommes intéressés plus particulièrement à la composante muonique des gerbes atmosphériques. Dans un premier temps, nous montrons comment les paramètres hadroniques conditionnent la production de muons. Par la suite, nous présentons une méthode originale permettant d'extraire cette composante muonique et d'en déduire les implications relatives à la composition des RCUHEs. Les résultats de cette approche semblent indiquer une transition d'une composition lourde vers une composition plus légère dès lors que l'énergie augmente. Finalement nous abordons la mesure de la section efficace cosmique-air en décrivant les bases de cette étude de même que son champ d'application : les premiers résultats déduits des données de l'Observatoire Pierre Auger sont alors présentés.
Published: 2008

39. Use of aspirin for primary and secondary prevention of cardiovascular disease in diabetic patients in an ambulatory care setting in Spain

Author: Sicras-Mainar, Antoni, primary, Navarro-Artieda, Ruth, additional, Rejas-Gutiérrez, Javier, additional, Fernández-de-Bobadilla, Jaime, additional, Frías-Garrido, Xavier, additional, and Ruiz-Riera, Rafael, additional
Published: 2007
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40. Cartas al editor

Author: Sicras Mainar, Antoni, primary, Ruiz Riera, Rafael, additional, Frías Garrido, Xavier, additional, and Navarro Artieda, Ruth, additional
Published: 2004
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41. Use of aspirin for primary and secondary prevention ofcardiovascular disease in diabetic patients in an ambulatory caresetting in Spain.

Author: Sicras-Mainar, Antoni, Navarro-Artieda, Ruth, Rejas-Gutiérrez, Javier, Fernández-de-Bobadilla, Jaime, Frías-Garrido, Xavier, and Ruiz-Riera, Rafael
Subjects: ASPIRIN, CARDIOVASCULAR diseases, PEOPLE with diabetes, OUTPATIENT medical care, PRIMARY care
Abstract: Background: This study was conducted in order to determine the use of aspirin and to assess the achievement of therapeutic targets in diabetic patients according to primary (PP) or secondary prevention (SP). Methods: This is a retrospective, observational study including patients ≥18 years with diabetes mellitus followed in four primary care centers. Measurements included demographics, use of aspirin and/or anticoagulant drugs, co-morbidities, clinical parameters and proportion of patient at therapeutic target (TT). Descriptive statistics, chi-square test and logistic regression model were used for significance. Results: A total of 4,140 patients were analyzed, 79.1% (95% confidence intervals [CI]: 77.7-80.5%) in PP and 20.9% (95% CI: 18.2-23.7%) in SP. Mean age was 64.1 (13.8) years, and 49.3% of patient were men (PP: 46.3, SP: 60.7, p = 0.001). Aspirin was prescribed routinely in 20.8% (95% CI: 19.4-22.2%) in PP and 60.8% (95% CI: 57.6-64.0%) in SP. Proportion of patient at TT was 48.0% for blood pressure and 59.8% for cholesterol. Use of aspirin was associated to increased age [OR = 1.01 (95% CI: 1.00-1.02); p = 0.011], cardiovascular-risk factors [OR = 1.14 (95% CI: 1.03-1.27); p = 0.013], LDL-C [OR = 1.42 (95% CI: 1.06-1.88); p = 0.017] and higher glycated hemoglobin [OR = 1.51 (95% CI: 1.22-1.89); p = 0.000] were covariates associated to the use of aspirin in PP. Conclusion: Treatment with aspirin is underused for PP in patients with diabetes mellitus in Primary Care. Achievement of TT should be improved. [ABSTRACT FROM AUTHOR]
Published: 2007
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42. Operations of and Future Plans for the Pierre Auger Observatory

Author: Abraham, Jorge Alberto, Abreu, Pedro, Aglietta, M., Aguirre, Carlos, Ahn, Eun-Joo, Allard, Denis, Allekotte, Ingo, Allen, Ronald J., Allison, Patrick, Alvarez-Muniz, Jaime, Ambrosio, Michelangelo, Anchordoqui, Luis Alfredo, Andringa, Sofia, Anzalone, Anna, Aramo, Carla, Arganda, E., Argiro, Stefano, Arisaka, Katsushi, Arneodo, F., Arqueros, Fernando, Asch, T., Asorey, Hernan, Assis, Pedro, Aublin, Julien, Ave, Maximo, Avila, Gualberto, Bacher, A., Backer, T., Badagnani, Daniel Omar, Barber, Kerridwen B., Barbosa, A. F., Barbosa, Henrique J. M., Barenthien, Norbert, Barroso, S. L. C., Baughman, Brian, Bauleo, Pablo Miguel, Beatty, James J., Beau, Tristan, Becker, Bernard Raymond, Becker, Karl-Heinz, Belletoile, Arnaud, Bellido, Jose Alfredo, Benzvi, Segev, Berat, Corinne, Bernardini, Paolo, Bertou, Xavier, Biermann, Peter L., Billoir, Pierre, Blanch, Oscar, Blanco, Francisco, Bleve, Carla, Blumer, Hans, Bohacova, Martina, Bollmann, E., Bolz, H., Bonifazi, Carla, Bonino, Raffaella, Borodai, N., Bracci, F., Brack, Jeffrey, Brogueira, P., Brown, William C., Bruijn, Ronald, Buchholz, Peter, Bueno, Antonio, Burton, R. E., Busca, Nicolas Guillermo, Caballero-Mora, Karen Salome, Camin, Daniel V., Caramete, L., Caruso, Rossella, Carvalho, Washington R., Castellina, Antonella, Castro-Tirado, A. J., Catalano, O., Cazon, Lorenzo, Cester, Rosanna, Chauvin, Joel, Chiavassa, A., Chinellato, Jose Augusto, Chou, Aaron S., Chudoba, Jiri, Chye, James D., Clark, Paul D. J., Clay, Roger William, Colombo, Eduardo, Conceicao, R., Connolly, Brian M., Contreras, Fernando, Coppens, Jose, Cordero-Cid, Adriana, Cordier, Alain, Cotti, Umberto, Coutu, Stephane, Covault, Corbin E., Creusot, Alexandre, Criss, Adrienne, Cronin, James Watson, Cuautle, J., Curutiu, A., Dagoret-Campagne, Sylvie, Dallier, Richard, Daudo, F., Daumiller, Kai, Dawson, Bruce R., Almeida, Rogerio Menezes, Domenico, Manlio, Donato, Cinzia, Jong, Sijbrand Jan, La Vega, G., Mello Junior, W. J. M., Mello Neto, Joao Ramos Torres, Mitri, Ivan, Souza, Vitor, Vries, K. D., Decerprit, G., Del Peral, Luis, Deligny, Olivier, Della Selva, Angelo, Delle Fratte, C., Dembinski, Hans, Di Giulio, Claudio, Diaz-Velez, J. C., Diep, P. N., Dobrigkeit, Carola, D Olivo, Juan Carlos, Dong, P. N., Dornic, Damien, Dorofeev, Alexei V., Costa Dos Anjos, Joao Carlos, Dova, Maria Teresa, D Urso, Domenico, Dutan, I., Duvernois, Michael A., Engel, Ralph, Erdmann, Martin Hans, Escobar, Carlos Ourivio, Etchegoyen, Alberto, Facal San Luis, Pedro, Falcke, Heino, Farrar, Glennys R., Fauth, Anderson C., Fazzini, N., Ferrer, Francesc, Ferrero, Armando, Fick, Brian E., Filevich, Alberto, Filipcic, Andrej, Fleck, Ivor, Fliescher, Stefan, Fonte, Roberto, Fracchiolla, Claudia E., Fraenkel, E. D., Fulgione, Walter, Gamarra, R. F., Gambetta, S., Garcia, Beatriz, Garcia-Gamez, Diego, Garcia-Pinto, D., Garrido, Xavier, Geenen, Heiko, Gelmini, Graciela B., Gemmeke, Hartmut, Ghia, Piera Luisa, Giaccari, Ugo, Gibbs, Kenneth, Giller, Maria, Gitto, J., Glass, Henry D., Goggin, Lisa M., Gold, Michael S., Golup, Geraldina T., Gomez Albarracin, F., Gomez Berisso, M., Gomez Vitale, P. F., Goncalves, Patricia, Goncalves Do Amaral, Marcia, Gonzalez, D., Gonzalez, J. G., Gora, Dariusz, Gorgi, A., Gouffon, Philippe H., Grashorn, Eric W., Grassi, V., Grebe, Stefan, Grigat, Marius, Grillo, Aurelio F., Grygar, Jiri, Guardincerri, Y., Guardone, Nunzio, Guerard, Carlos, Guarino, Francesco, Gumbsheimer, Rainer, Guedes, G. P., Gutierrez, J., Hague, J. D., Halenka, V., Hansen, P., Harari, Diego, Harmsma, Sybren, Hartmann, Steffen, Harton, John L., Haungs, Andreas, Healy, Matthew D., Hebbeker, Thomas, Hebrero, G., Heck, Dieter, Hojvat, Carlos F., Holmes, Vanessa Catherine, Homola, Piotr, Hofman, G., Hoerandel, Joerg R., Horneffer, A., Horvat, Matje, Hrabovsky, Miroslav, Hucker, H., Huege, Tim, Hussain, M., Iarlori, Marco, Insolia, Antonio, Ionita, F., Italiano, A., Jiraskova, S., Kaducak, Marc L., Kampert, Karl-Heinz, Karova, Tatiana, Kasper, Peter H., Kegl, B., Keilhauer, Bianca G., Kemp, Ernesto, Kern, H., Kieckhafer, Roger M., Klages, Hans O., Kleifges, Matthias, Kleinfeller, Jonny, Knapik, Robert, Knapp, Johannes, Koang, Dy-Holm, Kopmann, Andreas, Krieger, A., Kromer, O., Kruppke-Hansen, Daniel, Kuempel, Daniel, Kunka, Norbert, Kusenko, Alexander, La Rosa, Giovanni, Lachaud, C., Lago, B. L., Lautridou, Pascal, Leao, M. S. A. B., Lebrun, D., Lebrun, Paul L. G., Lee, Joong, Leigui Oliveira, Marcelo A., Lemiere, Anne, Letessier-Selvon, Antoine, Leuthold, Matthias J., Lhenry-Yvon, Isabelle, Lopez, Rebeca, Lopez Aguera, Angeles, Louedec, Karim, Lozano Bahilo, Julio, Lucero, A., Lyberis, H., Maccarone, Marie Concetta, Macolino, Carla, Maldera, Simone, Malek, Matthew Samir, Mandat, Dusan, Mantsch, Paul M., Marchetto, Flavio Pietro, Mariazzi, Analisa G., Maris, Ioana C., Marquez-Falcon, Hugo Raymundo, Martello, Daniele, Martineau-Huynh, O., Martinez Bravo, Oscar Mario, Mathes, Hermann-Josef, Matthews, J., Matthews, John A. J., Matthiae, Giorgio, Maurizio, Daniela, Mazur, Peter O., Mcewen, Megan, Mcneil, Roger Richard, Medina-Tanco, Gustavo A., Melissas, Maximilien, Melo, Diego G., Menichetti, Ezio A., Menshikov, Alexander, Meyhandan, Rishi, Micheletti, Maria Isabel, Miele, Gennaro, Miller, William, Miramonti, Lino, Mollerach, Silvia, Monasor, Maria, Monnier-Ragaigne, Delphine, Montanet, Francois, Morales, Benjamin Alejandro, Morello, C., Moreno, Juan Cruz, Morris, D. C., Mostafa, Miguel Alejandro, Moura, C. A., Mucchi, M., Mueller, S., Muller, M. A., Mussa, Roberto, Navarra, Gianni, Navarro, Jose Luis, Navas, Sergio, Necesal, P., Nellen, Lukas, Nerling, F., Newman-Holmes, Catherine, Newton, D., Nhung, P. T., Nicotra, Domenico, Nierstenhoefer, Nils, Nitz, David F., Nosek, Dalibor, Nozka, Libor, Nyklicek, M., Oehlschlager, J., Olinto, Angela V., Oliva, Pietro, Olmos-Gilbaja, Victor Manuel, Ortiz, Montserrat, Ortolani, Fabrizio, Osswald, B., Pacheco, N., Pakk Selmi-Dei, D., Palatka, Miroslav, Pallotta, J., Parente, Gonzalo, Parizot, Etienne, Parlati, S., Pastor, Sergio, Patel, M., Paul, Thomas Cantzon, Payet, Kevin, Pech, Miroslav, Pekala, J., Pepe, Iuri M., Perrone, Lorenzo, Pesce, R., Petermann, E., Petrera, Sergio, Petrinca, P., Petrolini, Alessandro, Petrov, Yuri V., Petrovic, J., Pfendner, C., Pichel, A., Piegaia, Ricardo, Pierog, Tanguy, Pimenta, Mario, Pinto, Teguayco, Pirronello, Valerio, Pisanti, Ofelia, Platino, M., Pochon, Jonathan, Ponce, Victor Hugo, Pontz, Michael, Pouryamout, J., Prado, Luis, Privitera, Paolo, Prouza, Michael, Quel, E. J., Raia, G., Rautenberg, Julian, Ravel, Olivier, Ravignani, Diego, Redondo, A., Reis, H. C., Reucroft, Stephen, Revenu, Benoit, Seixas Rezende, Fabio Antonio, Ridky, Jan, Riggi, Simone, Risse, Markus, Riviere, Christophe, Rizi, Vincenzo, Robledo, C., Roberts, M. D., Rodriguez-Fernandez, Gonzalo, Rodriguez Martino, Julio Cesar, Rodriguez Rojo, J., Rodriguez-Cabo, I., Rodriguez-Frias, M. Dolores, Ros, German, Rosado, Jaime, Rossler, T., Roth, Markus, Rouille-D Orfeuil, Benjamin, Roulet, Esteban, Rovero, Adrian C., Salamida, Francesco, Salina, Gaetano, Sanchez, Federico, Santander, Juan Marcos, Santo, C. E., Moura Santos, Edivaldo, Sarazin, Fred, Subir Sarkar, Sato, Ricardo, Scharf, Nils, Scherini, Viviana, Schieler, Harald, Schiffer, Peter, Schleif, G., Schmidt, A. A., Schmidt, Fabian, Schmidt, Talianna, Scholten, Olaf, Schoorlemmer, Harm, Schovancova, J., Schovanek, Petr, Schroeder, F., Schulte, Stephan, Schussler, Fabian, Schuster, David, Sciutto, Sergio J., Scuderi, Mario, Segreto, A., Semikoz, Dmitri V., Sequieros, G., Settimo, Mariangela, Shellard, Ronald Cintra, Sidelnik, Ivan, Siffert, Beatriz B., Smialkowski, Andrzej, Smida, Radomir, Smith, Andrew G. K., Smith, Ben E., Snow, Gregory R., Sommers, Paul D., Sorokin, J., Spinka, Harold M., Squartini, Ruben, Strazzeri, Elisabetta, Stutz, Anne, Suarez, F., Suomijarvi, Tiina, Supanitsky, A. D., Sutherland, Michael S., Swain, John D., Szadkowski, Zbigniew, Tamashiro, Alejandro Andres, Tamburro, Alessio, Tarutina, T., Tascau, Oana, Tcaciuc, Rodica, Tcherniakhovski, Denis, Thao, Nguyen Thi, Thomas, David, Ticona, R., Tiffenberg, Javier, Timmermans, Charles, Tkaczyk, Wieslaw, Todero Peixoto, C. J., Tome, Brigitte, Tonachini, Aurelio, Torres, I., Trapani, P., Travnicek, Petr, Tridapalli, Diogo B., Tristram, Gerard, Trovato, E., Tuci, V., Tueros, Matias, Tusi, E., Ulrich, Ralf, Unger, Michael, Urban, Marcel, Valdes Galicia, J. F., Valino, Ines, Valore, Laura, Den Berg, Ad M., Vazquez, J. R., Vazquez, Ricardo A., Veberic, Darko, Velarde, Alfonso, Venters, Tonia M., Verzi, Valerio, Videla, M., Villasenor Cendejas, Luis Manuel, Vitali, G., Vorobiov, Serguei, Wahlberg, Hernan Pablo, Wahrlich, Philip, Wainberg, O., Warner, Brian D., Westerhoff, Stefan, Whelan, B. J., Wild, N., Wiebusch, Christopher H., Wieczorek, G., Wiencke, Lawrence R., Wilczynska, Barbara, Wilczynski, Henryk, Wileman, Christopher, Winnick, M. G., Worner, G., Wu, H., Wundheiler, B., Younk, Patrick, Yuan, Guofeng, Yushkov, Alexey V., Zas, Enrique, Zavrtanik, Danilo, Zavrtanik, Marko, Zaw, Ingyin, Ziolkowski, M., APC - Astrophysique des Hautes Energies (APC - AHE), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire SUBATECH Nantes (SUBATECH), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire d'Orsay (IPNO), APC - THEORIE, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut für theoretische Physik, Universität Hamburg (UHH)-Universität Hamburg (UHH), PIERRE AUGER, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - 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Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut für theoretische Physik, and Research unit Astroparticle Physics
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], FOS: Physical sciences, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Instrumentation and Methods for Astrophysics (astro-ph.IM), [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
Abstract: Technical reports on operations and features of the Pierre Auger Observatory, including ongoing and planned enhancements and the status of the future northern hemisphere portion of the Observatory. Contributions to the 31st International Cosmic Ray Conference, Lodz, Poland, July 2009., Comment: Contributions to the 31st ICRC, Lodz, Poland, July 2009

43. [Aspirin use in patients with diabetes mellitus].

Author: Sicras Mainar A, Ruiz Riera R, Frías Garrido X, and Navarro Artieda R
Subjects: Cardiovascular Diseases complications, Cardiovascular Diseases epidemiology, Diabetes Complications, Diabetes Mellitus drug therapy, Diabetes Mellitus epidemiology, Female, Humans, Male, Prevalence, Primary Prevention, Risk Factors, Aspirin therapeutic use, Cardiovascular Diseases prevention & control, Platelet Aggregation Inhibitors therapeutic use
Published: 2004

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