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19,315 results on '"Schneider, M."'

151. First HAWC Observations of the Sun Constrain Steady TeV Gamma-Ray Emission

Author

Albert, A., Alfaro, R., Alvarez, C., Arceo, R., Arteaga-Velázquez, J. C., Rojas, D. Avila, Solares, H. A. Ayala, Belmont-Moreno, E., BenZvi, S. Y., Brisbois, C., Caballero-Mora, K. S., Capistràn, T., Carramiñana, A., Casanova, S., Castillo, M., Cotzomi, J., de León, S. Coutiño, De León, C., De la Fuente, E., Dichiara, S., Dingus, B. L., DuVernois, M. A., Díaz-Vélez, J. C., Engel, K., Enríquez-Rivera, O., Espinoza, C., Fleischhack, H., Fraija, N., García-González, J. A., Garfias, F., González, M. M., Goodman, J. A., Hampel-Arias, Z., Harding, J. P., Hernandez, S., Hona, B., Hueyotl-Zahuantitla, F., Hüntemeyer, P., Iriarte, A., Jardin-Blicq, A., Joshi, V., Kaufmann, S., Vargas, H. León, Luis-Raya, G., Lundeen, J., López-Coto, R., Malone, K., Marinelli, S. S., Martinez, O., Martinez-Castellanos, I., Martínez-Castro, J., Miranda-Romagnoli, P., Moreno, E., Mostafá, M., Nayerhoda, A., Nellen, L., Newbold, M., Nisa, M. U., Noriega-Papaqui, R., Pretz, J., Pérez-Pérez, E. G., Ren, Z., Rho, C. D., Rivière, C., Rosa-González, D., Rosenberg, M., Ruiz-Velasco, E., Salazar, H., Greus, F. Salesa, Sandoval, A., Schneider, M., Schoorlemmer, H., Arroyo, M. Seglar, Sinnis, G., Smith, A. J., Surajbali, P., Taboada, I., Tibolla, O., Tollefson, K., Torres, I., Villaseñor, L., Weisgarber, T., Westerhoff, S., Wisher, I. G., Wood, J., Yapici, T., Zepeda, A., Zhou, H., Álvarez, J. D., Beacom, J. F., Leane, R. K., Linden, T., Ng, K. C. Y., Peter, A. H. G., and Zhou, B.

Subjects
Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics, High Energy Physics - Phenomenology
Abstract

Steady gamma-ray emission up to at least 200 GeV has been detected from the solar disk in the Fermi-LAT data, with the brightest, hardest emission occurring during solar minimum. The likely cause is hadronic cosmic rays undergoing collisions in the Sun's atmosphere after being redirected from ingoing to outgoing in magnetic fields, though the exact mechanism is not understood. An important new test of the gamma-ray production mechanism will follow from observations at higher energies. Only the High Altitude Water Cherenkov (HAWC) Observatory has the required sensitivity to effectively probe the Sun in the TeV range. Using three years of HAWC data from November 2014 to December 2017, just prior to the solar minimum, we search for 1--100 TeV gamma rays from the solar disk. No evidence of a signal is observed, and we set strong upper limits on the flux at a few $10^{-12}$ TeV$^{-1}$ cm$^{-2}$ s$^{-1}$ at 1 TeV. Our limit, which is the most constraining result on TeV gamma rays from the Sun, is $\sim10\%$ of the theoretical maximum flux (based on a model where all incoming cosmic rays produce outgoing photons), which in turn is comparable to the Fermi-LAT data near 100 GeV. The prospects for a first TeV detection of the Sun by HAWC are especially high during solar minimum, which began in early 2018., Comment: 14 pages, 6 figures. See also companion paper 1808.05624. Accepted for publication in Physical Review D

Published
2018
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152. Constraints on Spin-Dependent Dark Matter Scattering with Long-Lived Mediators from TeV Observations of the Sun with HAWC

Author

Albert, A., Alfaro, R., Alvarez, C., Arceo, R., Arteaga-Velázquez, J. C., Rojas, D. Avila, Solares, H. A. Ayala, Belmont-Moreno, E., BenZvi, S. Y., Brisbois, C., Caballero-Mora, K. S., Capistràn, T., Carramiñana, A., Casanova, S., Castillo, M., Cotzomi, J., de León, S. Coutiño, De León, C., De la Fuente, E., Dichiara, S., Dingus, B. L., DuVernois, M. A., Díaz-Vélez, J. C., Engel, K., Enríquez-Rivera, O., Espinoza, C., Fleischhack, H., Fraija, N., García-González, J. A., Garfias, F., González, M. M., Goodman, J. A., Hampel-Arias, Z., Harding, J. P., Hernandez, S., Hona, B., Hueyotl-Zahuantitla, F., Hüntemeyer, P., Iriarte, A., Jardin-Blicq, A., Joshi, V., Kaufmann, S., Vargas, H. León, Luis-Raya, G., Lundeen, J., López-Coto, R., Malone, K., Marinelli, S. S., Martinez, O., Martinez-Castellanos, I., Martínez-Castro, J., Miranda-Romagnoli, P., Moreno, E., Mostafá, M., Nayerhoda, A., Nellen, L., Newbold, M., Nisa, M. U., Noriega-Papaqui, R., Pretz, J., Pérez-Pérez, E. G., Ren, Z., Rho, C. D., Rivière, C., Rosa-González, D., Rosenberg, M., Ruiz-Velasco, E., Salazar, H., Greus, F. Salesa, Sandoval, A., Schneider, M., Arroyo, M. Seglar, Sinnis, G., Smith, A. J., Surajbali, P., Taboada, I., Tibolla, O., Tollefson, K., Torres, I., Villaseñor, L., Weisgarber, T., Westerhoff, S., Wisher, I. G., Wood, J., Yapici, T., Zepeda, A., Zhou, H., Álvarez, J. D., Beacom, J. F., Leane, R. K., Linden, T., Ng, K. C. Y., Peter, A. H. G., and Zhou, B.

Subjects
High Energy Physics - Phenomenology, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics
Abstract

We analyze the Sun as a source for the indirect detection of dark matter through a search for gamma rays from the solar disk. Capture of dark matter by elastic interactions with the solar nuclei followed by annihilation to long-lived mediators can produce a detectable gamma-ray flux. We search three years of data from the High Altitude Water Cherenkov Observatory and find no statistically significant detection of TeV gamma-ray emission from the Sun. Using this, we constrain the spin-dependent elastic scattering cross section of dark matter with protons for dark matter masses above 1 TeV, assuming an unstable mediator with a favorable lifetime. The results complement constraints obtained from Fermi-LAT observations of the Sun and together cover WIMP masses between 4 GeV and $10^6$ GeV. The cross section constraints for mediator decays to gamma rays can be as strong as $\sim10^{-45}$ cm$^{-2}$, which is more than four orders of magnitude stronger than current direct-detection experiments for 1 TeV dark matter mass. The cross-section constraints at higher masses are even better, nearly 7 orders of magnitude better than the current direct-detection constraints for 100 TeV dark matter mass. This demonstration of sensitivity encourages detailed development of theoretical models in light of these powerful new constraints., Comment: 11 pages, 4 figures. See also companion paper 1808.05620. Accepted for publication in Physical Review D

Published
2018
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153. Spin pinning and spin-wave dispersion in nanoscopic ferromagnetic waveguides

Author

Wang, Q., Heinz, B., Verba, R., Kewenig, M., Pirro, P., Schneider, M., Meyer, T., Lägel, B., Dubs, C., Brächer, T., and Chumak, A. V.

Subjects
Condensed Matter - Mesoscale and Nanoscale Physics, Physics - Applied Physics
Abstract

Spin waves are investigated in Yttrium Iron Garnet (YIG) waveguides with a thickness of 39 nm and widths ranging down to 50 nm, i.e., with aspect ratios thickness over width approaching unity, using Brillouin Light Scattering spectroscopy. The experimental results are verified by a semi-analytical theory and micromagnetic simulations. A critical width is found, below which the exchange interaction suppresses the dipolar pinning phenomenon. This changes the quantization criterion for the spin-wave eigenmodes and results in a pronounced modification of the spin-wave characteristics. The presented semi-analytical theory allows for the calculation of spin-wave mode profiles and dispersion relations in nano-structures.

Published
2018
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154. On the physical basis of biological signaling by interface pulses

Author

Fichtl, B., Silman, I., and Schneider, M. F.

Subjects
Physics - Biological Physics
Abstract

Currently, biological signaling is envisaged as a combination of activation and movement, triggered by local molecular interactions and molecular diffusion, respectively. However, we here suggest, that other fundamental physical mechanisms might play an at least equally important role. We have recently shown that lipid interfaces permit the excitation and propagation of sound pulses. Here we demonstrate that these reversible perturbations can control the activity of membrane-embedded enzymes without a requirement for molecular transport. They can thus facilitate rapid communication between distant biological entities at the speed of sound, which is here of the order of 1 m/s within the membrane. The mechanism described provides a new physical framework for biological signaling that is fundamentally different from the molecular approach that currently dominates the textbooks.

Published
2018

155. Observation of Anisotropy of TeV Cosmic Rays with Two Years of HAWC

Author

Abeysekara, A. U., Alfaro, R., Alvarez, C., Alvarez, J. D., Arceo, R., Arteaga-Velázquez, J. C., Rojas, D. Avila, Solares, H. A. Ayala, Becerril, A., Belmont-Moreno, E., BenZvi, S. Y., Bernal, A., Braun, J., Caballero-Mora, K. S., Capistrán, T., Carramiñana, A., Casanova, S., Castillo, M., Cotti, U., Cotzomi, J., De León, C., De la Fuente, E., Hernandez, R. Diaz, Dichiara, S., Dingus, B. L., DuVernois, M. A., Díaz-Vélez, J. C., Engel, K., Fiorino, D. W., Fraija, N., García-González, J. A., Garfias, F., Muñoz, A. González, González, M. M., Goodman, J. A., Hampel-Arias, Z., Harding, J. P., Hernandez, S., Hona, B., Hueyotl-Zahuantitla, F., Hui, C. M., Hüntemeyer, P., Iriarte, A., Jardin-Blicq, A., Joshi, V., Kaufmann, S., Lara, A., Lauer, R. J., Lee, W. H., Vargas, H. León, Longinotti, A. L., Luis-Raya, G., Luna-García, R., López-Cámara, D., López-Coto, R., Malone, K., Marinelli, S. S., Martinez, O., Martinez-Castellanos, I., Martínez-Castro, J., Martínez-Huerta, H., Matthews, J. A., Miranda-Romagnoli, P., Moreno, E., Mostafá, M., Nayerhoda, A., Nellen, L., Newbold, M., Nisa, M. U., Noriega-Papaqui, R., Pelayo, R., Pretz, J., Pérez-Pérez, E. G., Ren, Z., Rho, C. D., Rivière, C., Rosa-González, D., Rosenberg, M., Ruiz-Velasco, E., Greus, F. Salesa, Sandoval, A., Schneider, M., Schoorlemmer, H., Arroyo, M. Seglar, Sinnis, G., Smith, A. J., Springer, R. W., Surajbali, P., Taboada, I., Tibolla, O., Tollefson, K., Torres, I., Vianello, G., Villaseñor, L., Weisgarber, T., Werner, F., Westerhoff, S., Wood, J., Yapici, T., Zepeda, A., and Zhou, H.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

After two years of operation, the High-Altitude Water Cherenkov (HAWC) Observatory has analyzed the TeV cosmic-ray sky over an energy range between $2.0$ and $72.8$ TeV. The HAWC detector is a ground-based air-shower array located at high altitude in the state of Puebla, Mexico. Using 300 light-tight water tanks, it collects the Cherenkov light from the particles of extensive air showers from primary gamma rays and cosmic rays. This detection method allows for uninterrupted observation of the entire overhead sky (2~sr instantaneous, 8.5~sr integrated) in the energy range from a few TeV to hundreds of TeV. Like other detectors in the northern and southern hemisphere, HAWC observes an energy-dependent anisotropy in the arrival direction distribution of cosmic rays. The observed cosmic-ray anisotropy is dominated by a dipole moment with phase $\alpha\approx40^{\circ}$ and amplitude that slowly rises in relative intensity from $8\times10^{-4}$ at 2 TeV to $14\times10^{-4}$ around 30.3 TeV, above which the dipole decreases in strength. A significant large-scale ($>60^{\circ}$ in angular extent) signal is also observed in the quadrupole and octupole moments, and significant small-scale features are also present, with locations and shapes consistent with previous observations. Compared to previous measurements in this energy range, the HAWC cosmic-ray sky maps improve on the energy resolution and fit precision of the anisotropy. These data can be used in an effort to better constrain local cosmic-ray accelerators and the intervening magnetic fields., Comment: 22 pages, 14 figures, 2 tables, submission to ApJ

Published
2018
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156. Subsurface Cation Vacancy Stabilization of the Magnetite (001) Surface

Author

Bliem, R., McDermott, E., Ferstl, P., Setvin, M., Gamba, O., Pavelec, J., Schneider, M. A., Schmid, M., Diebold, U., Blaha, P., Hammer, L., and Parkinson, G. S.

Subjects
Condensed Matter - Materials Science
Abstract

Iron oxides play an increasingly prominent role in heterogeneous catalysis, hydrogen production, spintronics and drug delivery. The surface or material interface can be performance limiting in these applications, so it is vital to determine accurate atomic-scale structures for iron oxides and understand why they form. Using a combination of quantitative low-energy electron diffraction, scanning tunneling microscopy, and density functional theory calculations, we show that an ordered array of subsurface iron vacancies and interstitials underlies the well-known (rt2xrt2)R45{\deg} reconstruction of Fe3O4(001). This hitherto unobserved stabilization mechanism occurs because the iron oxides prefer to redistribute cations in the lattice in response to oxidizing or reducing environments. Many other metal oxides also achieve stoichiometric variation in this way, so such surface structures are likely commonplace.

Published
2018
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157. Nonperturbative and non-Markovian F\'{o}rster-interaction in waveguiding systems

Author

Sproll, T., Martens, Ch., Schneider, M. P., Intravaia, F., and Busch, K.

Subjects
Quantum Physics
Abstract

An exact solution to the interaction between two emitters mediated by F\"{o}rster resonance energy transfer is presented. The system is comprised of a one-dimensional optical waveguide with two embedded two-level systems and is analyzed using a recently developed quantum-field theoretical approach. This exactly solvable model features several competing mechanisms that lead to a rich physical behavior such as, for instance, the possibility to change from an attractive to a repulsive interaction. Our nonperturbative analysis allows on very general grounds to describe the interaction as a truly non-Markovian phenomenon mediated by the atom-photon bound states of the system. These results are of direct relevance for energy or information transfer processes as well as for atom trapping more complex systems., Comment: 5+2 pages, 4 figures

Published
2018

158. Search for Dark Matter Gamma-ray Emission from the Andromeda Galaxy with the High-Altitude Water Cherenkov Observatory

Author

Albert, A., Alfaro, R., Alvarez, C., Alvarez, J. D., Arceo, R., Arteaga-Velázquez, J. C., Rojas, D. Avila, Solares, H. A. Ayala, Becerril, A., Belmont-Moreno, E., BenZvi, S. Y., Bernal, A., Brisbois, C., Caballero-Mora, K. S., Capistrán, T., Carramiñana, A., Casanova, S., Castillo, M., Cotti, U., Cotzomi, J., de León, S. Coutiño, De León, C., Dichiara, S., Dingus, B. L., DuVernois, M. A., Díaz-Vélez, J. C., Eckner, C., Engel, K., Enríquez-Rivera, O., Espinoza, C., Fiorino, D. W., Fraija, N., Galván-Gámez, A., García-González, J. A., Garfias, F., Muñoz, A. González, González, M. M., Goodman, J. A., Hampel-Arias, Z., Harding, J. P., Hernandez, S., Hernandez-Almada, A., Hona, B., Hüntemeyer, P., Iriarte, A., Jardin-Blicq, A., Joshi, V., Kaufmann, S., Kunde, G. J., Lennarz, D., Vargas, H. León, Linnemann, J. T., Longinotti, A. L., Raya, G. Luis, Luna-García, R., Malone, K., Marinelli, S. S., Martinez, O., Martínez-Castro, J., Martínez-Huerta, H., Matthews, J. A., Miranda-Romagnoli, P., Moreno, E., Mostafá, M., Nayerhoda, A., Nellen, L., Newbold, M., Nisa, M. U., Noriega-Papaqui, R., Pelayo, R., Pretz, J., Pérez-Pérez, E. G., Ren, Z., Rho, C. D., Riviére, C., Rosa-González, D., Rosenberg, M., Ruiz-Velasco, E., Salazar, H., Greus, F. Salesa, Sandoval, A., Schneider, M., Arroyo, M. Seglar, Sinnis, G., Smith, A. J., Springer, R. W., Surajbali, P., Taboada, I., Tibolla, O., Tollefson, K., Torres, I., Ukwatta, T. N., Villaseñor, L., Weisgarber, T., Westerhoff, S., Wood, J., Yapici, T., Zaharijas, G., Zepeda, A., and Zhou, H.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

The Andromeda Galaxy (M31) is a nearby ($\sim$780 kpc) galaxy similar to our own Milky Way. Observational evidence suggests that it resides in a large halo of dark matter (DM), making it a good target for DM searches. We present a search for gamma rays from M31 using 1017 days of data from the High Altitude Water Cherenkov (HAWC) Observatory. With its wide field of view and constant monitoring, HAWC is well-suited to search for DM in extended targets like M31. No DM annihilation or decay signal was detected for DM masses from 1 to 100 TeV in the $b\bar{b}$, $t\bar{t}$, $\tau^{+}\tau^{-}$, $\mu^{+}\mu^{-}$, and $W^{+}W^{-}$ channels. Therefore we present limits on those processes. Our limits nicely complement the existing body of DM limits from other targets and instruments. Specifically the DM decay limits from our benchmark model are the most constraining for DM masses from 25 TeV to 100 TeV in the $b\bar{b}, t\bar{t}$ and $\mu^{+}\mu{-}$ channels. In addition to DM-specific limits, we also calculate general gamma-ray flux limits for M31 in 5 energy bins from 1 TeV to 100 TeV., Comment: published in JCAP. Figure 6 (bottom) has been corrected

Published
2018
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159. Constraining the $\bar{p}/p$ Ratio in TeV Cosmic Rays with Observations of the Moon Shadow by HAWC

Author

Abeysekara, A. U., Albert, A., Alfaro, R., Alvarez, C., Arceo, R., Arteaga-Velázquez, J. C., Rojas, D. Avila, Solares, H. A. Ayala, Belmont-Moreno, E., BenZvi, S. Y., Braun, J., Brisbois, C., Caballero-Mora, K. S., Capistrán, T., Carramiñana, A., Casanova, S., Castillo, M., Cotti, U., Cotzomi, J., de León, S. Coutiño, De León, C., la Fuentem, E. D, Hernandez, R. Diaz, Dichiara, S., Dingus, B. L., DuVernois, M. A., Ellsworth, R. W., Engels, K., Enríquez-Rivera, O., Fleischhack, H., Fraija, N., Galván-Gámez, A., García-González, J. A., Muñoz, A. González, González, M. M., Goodman, J. A., Hampel-Arias, Z., Harding, J. P., Hernandez, S., Hona, B., Hueyotl-Zahuantitla, F., Hui, C. M., Hüntemeyer, P., Iriarte, A., Jardin-Blicq, A., Joshi, V., Kaufmann, S., Lara, A., Lee, W. H., Vargas, H. León, Linnemann, J. T., Longinotti, A. L., Luis-Raya, G., Luna-García, R., López-Coto, R., Malone, K., Marinelli, S. S., Martinez, O., Martinez-Castellanos, I., Martínez-Castro, J., Martínez-Huerta, H., Matthews, J. A., Miranda-Romagnoli, P., Moreno, E., Mostafá, M., Nayerhoda, A., Nellena, L., Newbold, M., Nisa, M. U., Noriega-Papaqui, R., Pelayo, R., Pretz, J., Pérez-Pérez, E. G., Ren, Z., Rho, C. D., Riviére, C., Rosa-González, D., Rosenberg, M., Ruiz-Velasco, E., Greus, F. Salesa, Sandoval, A., Schneider, M., Schoorlemmer, H., Arroyo, M. Seglar, Sinnis, G., Smith, A. J., Springer, R. W., Surajbali, P., Taboada, I., Tibolla, O., Tollefson, K., Torres, I., Villaseñor, L., Weisgarber, T., Westerhoff, S., Wood, J., Yapici, T., Yodha, G. B., Zepeda, A., Zhou, H., and Alvarez, J. D.

Subjects
Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

An indirect measurement of the antiproton flux in cosmic rays is possible as the particles undergo deflection by the geomagnetic field. This effect can be measured by studying the deficit in the flux, or shadow, created by the Moon as it absorbs cosmic rays that are headed towards the Earth. The shadow is displaced from the actual position of the Moon due to geomagnetic deflection, which is a function of the energy and charge of the cosmic rays. The displacement provides a natural tool for momentum/charge discrimination that can be used to study the composition of cosmic rays. Using 33 months of data comprising more than 80 billion cosmic rays measured by the High Altitude Water Cherenkov (HAWC) observatory, we have analyzed the Moon shadow to search for TeV antiprotons in cosmic rays. We present our first upper limits on the $\bar{p}/p$ fraction, which in the absence of any direct measurements, provide the tightest available constraints of $\sim1\%$ on the antiproton fraction for energies between 1 and 10 TeV., Comment: 10 pages, 5 figures. Accepted by Physical Review D

Published
2018
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160. Non-Maxwellian fast particle effects in gyrokinetic GENE simulations

Author

Di Siena, A., Görler, T., Doerk, H., Bilato, R., Citrin, J., Johnson, T., Schneider, M., Poli, E., and Contributors, JET

Subjects
Physics - Plasma Physics
Abstract

Fast ions have recently been found to significantly impact and partially suppress plasma turbulence both in experimental and numerical studies in a number of scenarios. Understanding the underlying physics and identifying the range of their beneficial effect is an essential task for future fusion reactors, where highly energetic ions are generated through fusion reactions and external heating schemes. However, in many of the gyrokinetic codes fast ions are, for simplicity, treated as equivalent-Maxwellian-distributed particle species, although it is well known that to rigorously model highly non-thermalised particles, a non-Maxwellian background distribution function is needed. To study the impact of this assumption, the gyrokinetic code GENE has recently been extended to support arbitrary background distribution functions which might be either analytic, e.g. slowing down and bi-Maxwellian, or obtained from numerical fast ion models. A particular JET plasma with strong fast-ion related turbulence suppression is revised with these new code capabilities both with linear and nonlinear gyrokinetic simulations. It appears that the fast ion stabilization tends to be less strong but still substantial with more realistic distributions, and this improves the quantitative power balance agreement with experiments., Comment: Submitted to Physics of Plasmas

Published
2018
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163. Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth

Author

Abeysekara, A. U., Albert, A., Alfaro, R., Alvarez, C., Álvarez, J. D., Arceo, R., Arteaga-Velázquez, J. C., Rojas, D. Avila, Solares, H. A. Ayala, Barber, A. S., Bautista-Elivar, N., Becerril, A., Belmont-Moreno, E., BenZvi, S. Y., Berley, D., Bernal, A., Braun, J., Brisbois, C., Caballero-Mora, K. S., Capistrán, T., Carramiñana, A., Casanova, S., Castillo, M., Cotti, U., Cotzomi, J., de León, S. Coutiño, De León, C., De la Fuente, E., Dingus, B. L., DuVernois, M. A., Díaz-Vélez, J. C., Ellsworth, R. W., Engel, K., Enríquez-Rivera, O., Fiorino, D. W., Fraija, N., García-González, J. A., Garfias, F., Gerhardt, M., Muñoz, A. González, González, M. M., Goodman, J. A., Hampel-Arias, Z., Harding, J. P., Hernández, S., Hernández-Almada, A., Hinton, J., Hona, B., Hui, C. M., Hüntemeyer, P., Iriarte, A., Jardin-Blicq, A., Joshi, V., Kaufmann, S., Kieda, D., Lara, A., Lauer, R. J., Lee, W. H., Lennarz, D., Vargas, H. León, Linnemann, J. T., Longinotti, A. L., Raya, G. Luis, Luna-García, R., López-Coto, R., Malone, K., Marinelli, S. S., Martinez, O., Martinez-Castellanos, I., Martínez-Castro, J., Martínez-Huerta, H., Matthews, J. A., Miranda-Romagnoli, P., Moreno, E., Mostafá, M., Nellen, L., Newbold, M., Nisa, M. U., Noriega-Papaqui, R., Pelayo, R., Pretz, J., Pérez-Pérez, E. G., Ren, Z., Rho, C. D., Rivière, C., Rosa-González, D., Rosenberg, M., Ruiz-Velasco, E., Salazar, H., Greus, F. Salesa, Sandoval, A., Schneider, M., Schoorlemmer, H., Sinnis, G., Smith, A. J., Springer, R. W., Surajbali, P., Taboada, I., Tibolla, O., Tollefson, K., Torres, I., Ukwatta, T. N., Vianello, G., Weisgarber, T., Westerhoff, S., Wisher, I. G., Wood, J., Yapici, T., Yodh, G., Younk, P. W., Zepeda, A., Zhou, H., Guo, F., Hahn, J., Li, H., and Zhang, H.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

The unexpectedly high flux of cosmic ray positrons detected at Earth may originate from nearby astrophysical sources, dark matter, or unknown processes of cosmic-ray secondary production. We report the detection, using the HighAltitude Water Cherenkov Observatory (HAWC), of extended tera-electron volt gamma-ray emission coincident with the locations of two nearby middle-aged pulsars (Geminga and PSR B0656+14). The HAWC observations demonstrate that these pulsars are indeed local sources of accelerated leptons, but the measured tera-electron volt emission profile constrains the diffusion of particles away from these sources to be much slower than previously assumed. We demonstrate that the leptons emitted by these objects are therefore unlikely to be the origin of the excess positrons, which may have a more exotic origin., Comment: 16 pages (including supplementary material), 5 figures

Published
2017
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164. All-sky Measurement of the Anisotropy of Cosmic Rays at 10 TeV and Mapping of the Local Interstellar Magnetic Field

Author

Abeysekara, AU, Alfaro, R, Alvarez, C, Arceo, R, Arteaga-Velázquez, JC, Rojas, D Avila, Belmont-Moreno, E, BenZvi, SY, Brisbois, C, Capistrán, T, Carramiana, A, Casanova, S, Cotti, U, Cotzomi, J, Díaz-Vélez, JC, De León, C, De la Fuente, E, Dichiara, S, DuVernois, MA, Espinoza, C, Fiorino, DW, Fleischhack, H, Fraija, N, Galván-Gámez, A, García-González, JA, González, MM, Goodman, JA, Hampel-Arias, Z, Harding, JP, Hernandez, S, Hona, B, Hueyotl-Zahuantitla, F, Iriarte, A, Jardin-Blicq, A, Joshi, V, Lara, A, Vargas, H León, Luis-Raya, G, Malone, K, Marinelli, SS, Martínez-Castro, J, Martinez, O, Matthews, JA, Miranda-Romagnoli, P, Moreno, E, Mostafá, M, Nellen, L, Newbold, M, Nisa, MU, Noriega-Papaqui, R, Pérez-Pérez, EG, Pretz, J, Ren, Z, Rho, CD, Rivière, C, Rosa-González, D, Rosenberg, M, Salazar, H, Greus, F Salesa, Sandoval, A, Schneider, M, Schoorlemmer, H, Sinnis, G, Smith, AJ, Surajbali, P, Taboada, I, Tollefson, K, Torres, I, Villaseor, L, Weisgarber, T, Wood, J, Zepeda, A, Zhou, H, Álvarez, JD, Aartsen, MG, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Altmann, D, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Argüelles, C, Auffenberg, J, Axani, S, Backes, P, Bagherpour, H, Bai, X, Barbano, A, Barron, JP, Barwick, SW, Baum, V, Bay, R, Beatty, JJ, Tjus, J Becker, Becker, K-H, and BenZvi, S

Subjects
Particle and High Energy Physics, Astronomical Sciences, Physical Sciences, astroparticle physics, cosmic rays, ISM: magnetic fields, astro-ph.HE, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural), Astronomy & Astrophysics, Astronomical sciences, Particle and high energy physics, Space sciences
Abstract

We present the first full-sky analysis of the cosmic ray arrival direction distribution with data collected by the High-Altitude Water Cherenkov and IceCube observatories in the northern and southern hemispheres at the same median primary particle energy of 10 TeV. The combined sky map and angular power spectrum largely eliminate biases that result from partial sky coverage and present a key to probe into the propagation properties of TeV cosmic rays through our local interstellar medium and the interaction between the interstellar and heliospheric magnetic fields. From the map, we determine the horizontal dipole components of the anisotropy δ 0h = 9.16 ×10-4 and δ 6h = 7.25 ×10-4 (±0.04 × 10-4). In addition, we infer the direction (229.°2 ± 3.°5 R.A., 11.°4 ± 3.°0 decl.) of the interstellar magnetic field from the boundary between large-scale excess and deficit regions from which we estimate the missing corresponding vertical dipole component of the large-scale anisotropy to be δN ∼ -3.97+1.0-2.0 × 10-4.

Published
2019

165. All-sky Measurement of the Anisotropy of Cosmic Rays at 10 TeV and Mapping of the Local Interstellar Magnetic Field

Author

Collaboration, H, Collaboration, I, Abeysekara, AU, Alfaro, R, Alvarez, C, Arceo, R, Arteaga-Velázquez, JC, Rojas, DA, Belmont-Moreno, E, Benzvi, SY, Brisbois, C, Capistrán, T, Carramiana, A, Casanova, S, Cotti, U, Cotzomi, J, Diaz-Vélez, JC, De León, C, Fuente, EDL, Dichiara, S, Duvernois, MA, Espinoza, C, Fiorino, DW, Fleischhack, H, Fraija, N, Galván-Gámez, A, Garcia-González, JA, González, MM, Goodman, JA, Hampel-Arias, Z, Harding, JP, Hernandez, S, Hona, B, Hueyotl-Zahuantitla, F, Iriarte, A, Jardin-Blicq, A, Joshi, V, Lara, A, Vargas, HL, Luis-Raya, G, Malone, K, Marinelli, SS, Martinez-Castro, J, Martinez, O, Matthews, JA, Miranda-Romagnoli, P, Moreno, E, Mostafá, M, Nellen, L, Newbold, M, Nisa, MU, Noriega-Papaqui, R, Pérez-Pérez, EG, Pretz, J, Ren, Z, Rho, CD, Riviere, C, Rosa-González, D, Rosenberg, M, Salazar, H, Greus, FS, Sandoval, A, Schneider, M, Schoorlemmer, H, Sinnis, G, Smith, AJ, Surajbali, P, Taboada, I, Tollefson, K, Torres, I, Villaseor, L, Weisgarber, T, Wood, J, Zepeda, A, Zhou, H, Alvarez, JD, Aartsen, MG, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Altmann, D, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Argüelles, C, Auffenberg, J, Axani, S, Backes, P, Bagherpour, H, Bai, X, Barbano, A, Barron, JP, Barwick, SW, Baum, V, Bay, R, Beatty, JJ, and Tjus, JB

Subjects
astroparticle physics, cosmic rays, ISM: magnetic fields, astro-ph.HE, Astronomy & Astrophysics, Astronomical and Space Sciences, Organic Chemistry, Physical Chemistry, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural)
Abstract

We present the first full-sky analysis of the cosmic ray arrival direction distribution with data collected by the High-Altitude Water Cherenkov and IceCube observatories in the northern and southern hemispheres at the same median primary particle energy of 10 TeV. The combined sky map and angular power spectrum largely eliminate biases that result from partial sky coverage and present a key to probe into the propagation properties of TeV cosmic rays through our local interstellar medium and the interaction between the interstellar and heliospheric magnetic fields. From the map, we determine the horizontal dipole components of the anisotropy δ 0h = 9.16 ×10 -4 and δ 6h = 7.25 ×10 -4 (±0.04 × 10 -4 ). In addition, we infer the direction (229.°2 ± 3.°5 R.A., 11.°4 ± 3.°0 decl.) of the interstellar magnetic field from the boundary between large-scale excess and deficit regions from which we estimate the missing corresponding vertical dipole component of the large-scale anisotropy to be δN ∼ -3.97 +1.0-2.0 × 10 -4 .

Published
2019

166. Transmission Electron Microscopy Studies of Transition Metal Oxides Employed as Carrier Selective Contacts in Silicon Solar Cells

Author

Ali, H, Bullock, J, Gregory, G, Yang, X, Schneider, M, Weber, K, Javey, A, and Davis, KO

Subjects
silicon, carrier selective contacts, transmission electron microscopy, transition metal oxide
Abstract

The focus of this work is on the nano-scale characterization of transition metal oxides employed as carrier selective contacts in crystalline silicon (c-Si) solar cells using crosssectional transmission electron microscopy (TEM). Both electronselective (titanium dioxide, TiO 2 ) and hole-selective (molybdenum oxide, MoO x ; tungsten oxide, WO x textbf) contacts were investigated. High-resolution TEM (HRTEM) images were obtained with a FEI Tecnai F30 TEM.

Published
2018

168. Impact of diabetes on the management and outcomes in atrial fibrillation: an analysis from the ESC-EHRA EORP-AF Long-Term General Registry

Author

Boriani, G., Lip, G.Y.H., Tavazzi, L., Maggioni, A.P., Dan, G.-A., Potpara, T., Nabauer, M., Marin, F., Kalarus, Z., Goda, A., Mairesse, G., Shalganov, T., Antoniades, L., Taborsky, M., Riahi, S., Muda, P., García Bolao, I., Piot, O., Etsadashvili, K., Simantirakis, E., Haim, M., Azhari, A., Najafian, J., Santini, M., Mirrakhimov, E., Kulzida, K.A., Erglis, A., Poposka, L., Burg, M., Crijns, H., Erküner, Ö., Atar, D., Lenarczyk, R., Martins Oliveira, M., Shah, D., Serdechnaya, E., Diker, E., Lane, D., Zëra, E., Ekmekçiu, U., Paparisto, V., Tase, M., Gjergo, H., Dragoti, J., Ciutea, M., Ahadi, N., el Husseini, Z., Raepers, M., Leroy, J., Haushan, P., Jourdan, A., Lepiece, C., Desteghe, L., Vijgen, J., Koopman, P., Van Genechten, G., Heidbuchel, H., Boussy, T., De Coninck, M., Van Eeckhoutte, H., Bouckaert, N., Friart, A., Boreux, J., Arend, C., Evrard, P., Stefan, L., Hoffer, E., Herzet, J., Massoz, M., Celentano, C., Sprynger, M., Pierard, L., Melon, P., Van Hauwaert, B., Kuppens, C., Faes, D., Van Lier, D., Van Dorpe, A., Gerardy, A., Deceuninck, O., Xhaet, O., Dormal, F., Ballant, E., Blommaert, D., Yakova, D., Hristov, M., Yncheva, T., Stancheva, N., Tisheva, S., Tokmakova, M., Nikolov, F., Gencheva, D., Kunev, B., Stoyanov, M., Marchov, D., Gelev, V., Traykov, V., Kisheva, A., Tsvyatkov, H., Shtereva, R., Bakalska-Georgieva, S., Slavcheva, S., Yotov, Y., Kubíčková, M., Marni Joensen, A., Gammelmark, A., Hvilsted Rasmussen, L., Dinesen, P., Krogh Venø, S., Sorensen, B., Korsgaard, A., Andersen, K., Fragtrup Hellum, C., Svenningsen, A., Nyvad, O., Wiggers, P., May, O., Aarup, A., Graversen, B., Jensen, L., Andersen, M., Svejgaard, M., Vester, S., Hansen, S., Lynggaard, V., Ciudad, M., Vettus, R., Maestre, A., Castaño, S., Cheggour, S., Poulard, J., Mouquet, V., Leparrée, S., Bouet, J., Taieb, J., Doucy, A., Duquenne, H., Furber, A., Dupuis, J., Rautureau, J., Font, M., Damiano, P., Lacrimini, M., Abalea, J., Boismal, S., Menez, T., Mansourati, J., Range, G., Gorka, H., Laure, C., Vassalière, C., Elbaz, N., Lellouche, N., Djouadi, K., Roubille, F., Dietz, D., Davy, J., Granier, M., Winum, P., Leperchois-Jacquey, C., Kassim, H., Marijon, E., Le Heuzey, J., Fedida, J., Maupain, C., Himbert, C., Gandjbakhch, E., Hidden-Lucet, F., Duthoit, G., Badenco, N., Chastre, T., Waintraub, X., Oudihat, M., Lacoste, J., Stephan, C., Bader, H., Delarche, N., Giry, L., Arnaud, D., Lopez, C., Boury, F., Brunello, I., Lefèvre, M., Mingam, R., Haissaguerre, M., Le Bidan, M., Pavin, D., Le Moal, V., Leclercq, C., Beitar, T., Martel, I., Schmid, A., Sadki, N., Romeyer-Bouchard, C., Da Costa, A., Arnault, I., Boyer, M., Piat, C., Lozance, N., Nastevska, S., Doneva, A., Fortomaroska Milevska, B., Sheshoski, B., Petroska, K., Taneska, N., Bakrecheski, N., Lazarovska, K., Jovevska, S., Ristovski, V., Antovski, A., Lazarova, E., Kotlar, I., Taleski, J., Kedev, S., Zlatanovik, N., Jordanova, S., Bajraktarova Proseva, T., Doncovska, S., Maisuradze, D., Esakia, A., Sagirashvili, E., Lartsuliani, K., Natelashvili, N., Gumberidze, N., Gvenetadze, R., Gotonelia, N., Kuridze, N., Papiashvili, G., Menabde, I., Glöggler, S., Napp, A., Lebherz, C., Romero, H., Schmitz, K., Berger, M., Zink, M., Köster, S., Sachse, J., Vonderhagen, E., Soiron, G., Mischke, K., Reith, R., Schneider, M., Rieker, W., Boscher, D., Taschareck, A., Beer, A., Oster, D., Ritter, O., Adamczewski, J., Walter, S., Frommhold, A., Luckner, E., Richter, J., Schellner, M., Landgraf, S., Bartholome, S., Naumann, R., Schoeler, J., Westermeier, D., William, F., Wilhelm, K., Maerkl, M., Oekinghaus, R., Denart, M., Kriete, M., Tebbe, U., Scheibner, T., Gruber, M., Gerlach, A., Beckendorf, C., Anneken, L., Arnold, M., Lengerer, S., Bal, Z., Uecker, C., Förtsch, H., Fechner, S., Mages, V., Martens, E., Methe, H., Schmidt, T., Schaeffer, B., Hoffmann, B., Moser, J., Heitmann, K., Willems, S., Klaus, C., Lange, I., Durak, M., Esen, E., Mibach, F., Mibach, H., Utech, A., Gabelmann, M., Stumm, R., Ländle, V., Gartner, C., Goerg, C., Kaul, N., Messer, S., Burkhardt, D., Sander, C., Orthen, R., Kaes, S., Baumer, A., Dodos, F., Barth, A., Schaeffer, G., Gaertner, J., Winkler, J., Fahrig, A., Aring, J., Wenzel, I., Steiner, S., Kliesch, A., Kratz, E., Winter, K., Schneider, P., Haag, A., Mutscher, I., Bosch, R., Taggeselle, J., Meixner, S., Schnabel, A., Shamalla, A., Hötz, H., Korinth, A., Rheinert, C., Mehltretter, G., Schön, B., Schön, N., Starflinger, A., Englmann, E., Baytok, G., Laschinger, T., Ritscher, G., Gerth, A., Dechering, D., Eckardt, L., Kuhlmann, M., Proskynitopoulos, N., Brunn, J., Foth, K., Axthelm, C., Hohensee, H., Eberhard, K., Turbanisch, S., Hassler, N., Koestler, A., Stenzel, G., Kschiwan, D., Schwefer, M., Neiner, S., Hettwer, S., Haeussler-Schuchardt, M., Degenhardt, R., Sennhenn, S., Brendel, M., Stoehr, A., Widjaja, W., Loehndorf, S., Logemann, A., Hoskamp, J., Grundt, J., Block, M., Ulrych, R., Reithmeier, A., Panagopoulos, V., Martignani, C., Bernucci, D., Fantecchi, E., Diemberger, I., Ziacchi, M., Biffi, M., Cimaglia, P., Frisoni, J., Giannini, I., Boni, S., Fumagalli, S., Pupo, S., Di Chiara, A., Mirone, P., Pesce, F., Zoccali, C., Malavasi, V.L., Mussagaliyeva, A., Ahyt, B., Salihova, Z., Koshum-Bayeva, K., Kerimkulova, A., Bairamukova, A., Lurina, B., Zuzans, R., Jegere, S., Mintale, I., Kupics, K., Jubele, K., Kalejs, O., Vanhear, K., Cachia, M., Abela, E., Warwicker, S., Tabone, T., Xuereb, R., Asanovic, D., Drakalovic, D., Vukmirovic, M., Pavlovic, N., Music, L., Bulatovic, N., Boskovic, A., Uiterwaal, H., Bijsterveld, N., De Groot, J., Neefs, J., van den Berg, N., Piersma, F., Wilde, A., Hagens, V., Van Es, J., Van Opstal, J., Van Rennes, B., Verheij, H., Breukers, W., Tjeerdsma, G., Nijmeijer, R., Wegink, D., Binnema, R., Said, S., Philippens, S., van Doorn, W., Szili-Torok, T., Bhagwandien, R., Janse, P., Muskens, A., van Eck, M., Gevers, R., van der Ven, N., Duygun, A., Rahel, B., Meeder, J., Vold, A., Holst Hansen, C., Engset, I., Dyduch-Fejklowicz, B., Koba, E., Cichocka, M., Sokal, A., Kubicius, A., Pruchniewicz, E., Kowalik-Sztylc, A., Czapla, W., Mróz, I., Kozlowski, M., Pawlowski, T., Tendera, M., Winiarska-Filipek, A., Fidyk, A., Slowikowski, A., Haberka, M., Lachor-Broda, M., Biedron, M., Gasior, Z., Kołodziej, M., Janion, M., Gorczyca-Michta, I., Wozakowska-Kaplon, B., Stasiak, M., Jakubowski, P., Ciurus, T., Drozdz, J., Simiera, M., Zajac, P., Wcislo, T., Zycinski, P., Kasprzak, J., Olejnik, A., Harc-Dyl, E., Miarka, J., Pasieka, M., Ziemińska-Łuć, M., Bujak, W., Śliwiński, A., Grech, A., Morka, J., Petrykowska, K., Prasał, M., Hordyński, G., Feusette, P., Lipski, P., Wester, A., Streb, W., Romanek, J., Woźniak, P., Chlebuś, M., Szafarz, P., Stanik, W., Zakrzewski, M., Kaźmierczak, J., Przybylska, A., Skorek, E., Błaszczyk, H., Stępień, M., Szabowski, S., Krysiak, W., Szymańska, M., Karasiński, J., Blicharz, J., Skura, M., Hałas, K., Michalczyk, L., Orski, Z., Krzyżanowski, K., Skrobowski, A., Zieliński, L., Tomaszewska-Kiecana, M., Dłużniewski, M., Kiliszek, M., Peller, M., Budnik, M., Balsam, P., Opolski, G., Tymińska, A., Ozierański, K., Wancerz, A., Borowiec, A., Majos, E., Dabrowski, R., Szwed, H., Musialik-Lydka, A., Leopold-Jadczyk, A., Jedrzejczyk-Patej, E., Koziel, M., Mazurek, M., Krzemien-Wolska, K., Starosta, P., Nowalany-Kozielska, E., Orzechowska, A., Szpot, M., Staszel, M., Almeida, S., Pereira, H., Brandão Alves, L., Miranda, R., Ribeiro, L., Costa, F., Morgado, F., Carmo, P., Galvao Santos, P., Bernardo, R., Adragão, P., Ferreira da Silva, G., Peres, M., Alves, M., Leal, M., Cordeiro, A., Magalhães, P., Fontes, P., Leão, S., Delgado, A., Costa, A., Marmelo, B., Rodrigues, B., Moreira, D., Santos, J., Santos, L., Terchet, A., Darabantiu, D., Mercea, S., Turcin Halka, V., Pop Moldovan, A., Gabor, A., Doka, B., Catanescu, G., Rus, H., Oboroceanu, L., Bobescu, E., Popescu, R., Dan, A., Buzea, A., Daha, I., Dan, G., Neuhoff, I., Baluta, M., Ploesteanu, R., Dumitrache, N., Vintila, M., Daraban, A., Japie, C., Badila, E., Tewelde, H., Hostiuc, M., Frunza, S., Tintea, E., Bartos, D., Ciobanu, A., Popescu, I., Toma, N., Gherghinescu, C., Cretu, D., Patrascu, N., Stoicescu, C., Udroiu, C., Bicescu, G., Vintila, V., Vinereanu, D., Cinteza, M., Rimbas, R., Grecu, M., Cozma, A., Boros, F., Ille, M., Tica, O., Tor, R., Corina, A., Jeewooth, A., Maria, B., Georgiana, C., Natalia, C., Alin, D., Dinu-Andrei, D., Livia, M., Daniela, R., Larisa, R., Umaar, S., Tamara, T., Ioachim Popescu, M., Nistor, D., Sus, I., Coborosanu, O., Alina-Ramona, N., Dan, R., Petrescu, L., Ionescu, G., Vacarescu, C., Goanta, E., Mangea, M., Ionac, A., Mornos, C., Cozma, D., Pescariu, S., Solodovnicova, E., Soldatova, I., Shutova, J., Tjuleneva, L., Zubova, T., Uskov, V., Obukhov, D., Rusanova, G., Isakova, N., Odinsova, S., Arhipova, T., Kazakevich, E., Zavyalova, O., Novikova, T., Riabaia, I., Zhigalov, S., Drozdova, E., Luchkina, I., Monogarova, Y., Hegya, D., Rodionova, L., Nevzorova, V., Lusanova, O., Arandjelovic, A., Toncev, D., Vukmirovic, L., Radisavljevic, M., Milanov, M., Sekularac, N., Zdravkovic, M., Hinic, S., Dimkovic, S., Acimovic, T., Saric, J., Radovanovic, S., Kocijancic, A., Obrenovic-Kircanski, B., Kalimanovska Ostric, D., Simic, D., Jovanovic, I., Petrovic, I., Polovina, M., Vukicevic, M., Tomasevic, M., Mujovic, N., Radivojevic, N., Petrovic, O., Aleksandric, S., Kovacevic, V., Mijatovic, Z., Ivanovic, B., Tesic, M., Ristic, A., Vujisic-Tesic, B., Nedeljkovic, M., Karadzic, A., Uscumlic, A., Prodanovic, M., Zlatar, M., Asanin, M., Bisenic, B., Vasic, V., Popovic, Z., Djikic, D., Sipic, M., Peric, V., Dejanovic, B., Milosevic, N., Backovic, S., Stevanovic, A., Andric, A., Pencic, B., Pavlovic-Kleut, M., Celic, V., Pavlovic, M., Petrovic, M., Vuleta, M., Petrovic, N., Simovic, S., Savovic, Z., Milanov, S., Davidovic, G., Iric-Cupic, V., Djordjevic, D., Damjanovic, M., Zdravkovic, S., Topic, V., Stanojevic, D., Randjelovic, M., Jankovic-Tomasevic, R., Atanaskovic, V., Antic, S., Simonovic, D., Stojanovic, M., Stojanovic, S., Mitic, V., Ilic, V., Petrovic, D., Deljanin Ilic, M., Ilic, S., Stoickov, V., Markovic, S., Mijatovic, A., Tanasic, D., Radakovic, G., Peranovic, J., Panic-Jelic, N., Vujadinovic, O., Pajic, P., Bekic, S., Kovacevic, S., García Fernandez, A., Perez Cabeza, A., Anguita, M., Tercedor Sanchez, L., Mau, E., Loayssa, J., Ayarra, M., Carpintero, M., Roldán Rabadan, I., Gil Ortega, M., Tello Montoliu, A., Orenes Piñero, E., Manzano Fernández, S., Marín, F., Romero Aniorte, A., Veliz Martínez, A., Quintana Giner, M., Ballesteros, G., Palacio, M., Alcalde, O., García-Bolao, I., Bertomeu Gonzalez, V., Otero-Raviña, F., García Seara, J., Gonzalez Juanatey, J., Dayal, N., Maziarski, P., Gentil-Baron, P., Koç, M., Onrat, E., Dural, I.E., Yilmaz, K., Özin, B., Tan Kurklu, S., Atmaca, Y., Canpolat, U., Tokgozoglu, L., Dolu, A.K., Demirtas, B., Sahin, D., Ozcan Celebi, O., Gagirci, G., Turk, U.O., Ari, H., Polat, N., Toprak, N., Sucu, M., Akin Serdar, O., Taha Alper, A., Kepez, A., Yuksel, Y., Uzunselvi, A., Yuksel, S., Sahin, M., Kayapinar, O., Ozcan, T., Kaya, H., Yilmaz, M.B., Kutlu, M., Demir, M., Gibbs, C., Kaminskiene, S., Bryce, M., Skinner, A., Belcher, G., Hunt, J., Stancombe, L., Holbrook, B., Peters, C., Tettersell, S., Shantsila, A., Senoo, K., Proietti, M., Russell, K., Domingos, P., Hussain, S., Partridge, J., Haynes, R., Bahadur, S., Brown, R., McMahon, S., McDonald, J., Balachandran, K., Singh, R., Garg, S., Desai, H., Davies, K., Goddard, W., Galasko, G., Rahman, I., Chua, Y., Payne, O., Preston, S., Brennan, O., Pedley, L., Whiteside, C., Dickinson, C., Brown, J., Jones, K., Benham, L., Brady, R., Buchanan, L., Ashton, A., Crowther, H., Fairlamb, H., Thornthwaite, S., Relph, C., McSkeane, A., Poultney, U., Kelsall, N., Rice, P., Wilson, T., Wrigley, M., Kaba, R., Patel, T., Young, E., Law, J., Runnett, C., Thomas, H., McKie, H., Fuller, J., Pick, S., Sharp, A., Hunt, A., Thorpe, K., Hardman, C., Cusack, E., Adams, L., Hough, M., Keenan, S., Bowring, A., Watts, J., Zaman, J., Goffin, K., Nutt, H., Beerachee, Y., Featherstone, J., Mills, C., Pearson, J., Stephenson, L., Grant, S., Wilson, A., Hawksworth, C., Alam, I., Robinson, M., Ryan, S., Egdell, R., Gibson, E., Holland, M., Leonard, D., Mishra, B., Ahmad, S., Randall, H., Hill, J., Reid, L., George, M., McKinley, S., Brockway, L., Milligan, W., Sobolewska, J., Muir, J., Tuckis, L., Winstanley, L., Jacob, P., Kaye, S., Morby, L., Jan, A., Sewell, T., Boos, C., Wadams, B., Cope, C., Jefferey, P., Andrews, N., Getty, A., Suttling, A., Turner, C., Hudson, K., Austin, R., Howe, S., Iqbal, R., Gandhi, N., Brophy, K., Mirza, P., Willard, E., Collins, S., Ndlovu, N., Subkovas, E., Karthikeyan, V., Waggett, L., Wood, A., Bolger, A., Stockport, J., Evans, L., Harman, E., Starling, J., Williams, L., Saul, V., Sinha, M., Bell, L., Tudgay, S., Kemp, S., Frost, L., Ingram, T., Loughlin, A., Adams, C., Adams, M., Hurford, F., Owen, C., Miller, C., Donaldson, D., Tivenan, H., Button, H., Nasser, A., Jhagra, O., Stidolph, B., Brown, C., Livingstone, C., Duffy, M., Madgwick, P., Roberts, P., Greenwood, E., Fletcher, L., Beveridge, M., Earles, S., McKenzie, D., Beacock, D., Dayer, M., Seddon, M., Greenwell, D., Luxton, F., Venn, F., Mills, H., Rewbury, J., James, K., Roberts, K., Tonks, L., Felmeden, D., Taggu, W., Summerhayes, A., Hughes, D., Sutton, J., Felmeden, L., Khan, M., Walker, E., Norris, L., O'Donohoe, L., Mozid, A., Dymond, H., Lloyd-Jones, H., Saunders, G., Simmons, D., Coles, D., Cotterill, D., Beech, S., Kidd, S., Wrigley, B., Petkar, S., Smallwood, A., Jones, R., Radford, E., Milgate, S., Metherell, S., Cottam, V., Buckley, C., Broadley, A., Wood, D., Allison, J., Rennie, K., Balian, L., Howard, L., Pippard, L., Board, S., Pitt-Kerby, T., Ding, Wern Yew, Kotalczyk, Agnieszka, Boriani, Giuseppe, Marin, Francisco, Blomström-Lundqvist, Carina, Potpara, Tatjana S., Fauchier, Laurent, and Lip, Gregory.Y.H.

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2022
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171. Cardiac troponins and adverse outcomes in European patients with atrial fibrillation: A report from the ESC-EHRA EORP atrial fibrillation general long-term registry

Author

Boriani, G., Lip, G.Y.H., Tavazzi, L., Maggioni, A.P., Dan, G-A., Potpara, T., Nabauer, M., Marin, F., Kalarus, Z., Fauchier, L., Goda, A., Mairesse, G., Shalganov, T., Antoniades, L., Taborsky, M., Riahi, S., Muda, P., García Bolao, I., Piot, O., Etsadashvili, K., Haim, M., Azhari, A., Najafian, J., Santini, M., Mirrakhimov, E., Kulzida, K., Erglis, A., Poposka, L., Burg, M.R., Crijns, H., Erküner, Ö., Atar, D., Lenarczyk, R., Martins Oliveira, M., Shah, D., Serdechnaya, E., Diker, E., Zëra, E., Ekmekçiu, U., Paparisto, V., Tase, M., Gjergo, H., Dragoti, J., Ciutea, M., Ahadi, N., el Husseini, Z., Raepers, M., Leroy, J., Haushan, P., Jourdan, A., Lepiece, C., Desteghe, L., Vijgen, J., Koopman, P., Van Genechten, G., Heidbuchel, H., Boussy, T., De Coninck, M., Van Eeckhoutte, H., Bouckaert, N., Friart, A., Boreux, J., Arend, C., Evrard, P., Stefan, L., Hoffer, E., Herzet, J., Massoz, M., Celentano, C., Sprynger, M., Pierard, L., Melon, P., Van Hauwaert, B., Kuppens, C., Faes, D., Van Lier, D., Van Dorpe, A., Gerardy, A., Deceuninck, O., Xhaet, O., Dormal, F., Ballant, E., Blommaert, D., Yakova, D., Hristov, M., Yncheva, T., Stancheva, N., Tisheva, S., Tokmakova, M., Nikolov, F., Gencheva, D., Kunev, B., Stoyanov, M., Marchov, D., Gelev, V., Traykov, V., Kisheva, A., Tsvyatkov, H., Shtereva, R., Bakalska-Georgieva, S., Slavcheva, S., Yotov, Y., Kubíčková, M., Marni Joensen, A., Gammelmark, A., Hvilsted Rasmussen, L., Dinesen, P., Krogh Venø, S., Sorensen, B., Korsgaard, A., Andersen, K., Fragtrup Hellum, C., Svenningsen, A., Nyvad, O., Wiggers, P., May, O., Aarup, A., Graversen, B., Jensen, L., Andersen, M., Svejgaard, M., Vester, S., Hansen, S., Lynggaard, V., Ciudad, M., Vettus, R., Maestre, A., Castaño, S., Cheggour, S., Poulard, J., Mouquet, V., Leparrée, S., Bouet, J., Taieb, J., Doucy, A., Duquenne, H., Furber, A., Dupuis, J., Rautureau, J., Font, M., Damiano, P., Lacrimini, M., Abalea, J., Boismal, S., Menez, T., Mansourati, J., Range, G., Gorka, H., Laure, C., Vassalière, C., Elbaz, N., Lellouche, N., Djouadi, K., Roubille, F., Dietz, D., Davy, J., Granier, M., Winum, P., Leperchois-Jacquey, C., Kassim, H., Marijon, E., Le Heuzey, J., Fedida, J., Maupain, C., Himbert, C., Gandjbakhch, E., Hidden-Lucet, F., Duthoit, G., Badenco, N., Chastre, T., Waintraub, X., Oudihat, M., Lacoste, J., Stephan, C., Bader, H., Delarche, N., Giry, L., Arnaud, D., Lopez, C., Boury, F., Brunello, I., Lefèvre, M., Mingam, R., Haissaguerre, M., Le Bidan, M., Pavin, D., Le Moal, V., Leclercq, C., Beitar, T., Martel, I., Schmid, A., Sadki, N., Romeyer-Bouchard, C., Da Costa, A., Arnault, I., Boyer, M., Piat, C., Lozance, N., Nastevska, S., Doneva, A., Fortomaroska Milevska, B., Sheshoski, B., Petroska, K., Taneska, N., Bakrecheski, N., Lazarovska, K., Jovevska, S., Ristovski, V., Antovski, A., Lazarova, E., Kotlar, I., Taleski, J., Kedev, S., Zlatanovik, N., Jordanova, S., Bajraktarova Proseva, T., Doncovska, S., Maisuradze, D., Esakia, A., Sagirashvili, E., Lartsuliani, K., Natelashvili, N., Gumberidze, N., Gvenetadze, R., Gotonelia, N., Kuridze, N., Papiashvili, G., Menabde, I., Glöggler, S., Napp, A., Lebherz, C., Romero, H., Schmitz, K., Berger, M., Zink, M., Köster, S., Sachse, J., Vonderhagen, E., Soiron, G., Mischke, K., Reith, R., Schneider, M., Rieker, W., Boscher, D., Taschareck, A., Beer, A., Oster, D., Ritter, O., Adamczewski, J., Walter, S., Frommhold, A., Luckner, E., Richter, J., Schellner, M., Landgraf, S., Bartholome, S., Naumann, R., Schoeler, J., Westermeier, D., William, F., Wilhelm, K., Maerkl, M., Oekinghaus, R., Denart, M., Kriete, M., Tebbe, U., Scheibner, T., Gruber, M., Gerlach, A., Beckendorf, C., Anneken, L., Arnold, M., Lengerer, S., Bal, Z., Uecker, C., Förtsch, H., Fechner, S., Mages, V., Martens, E., Methe, H., Schmidt, T., Schaeffer, B., Hoffmann, B., Moser, J., Heitmann, K., Willems, S., Klaus, C., Lange, I., Durak, M., Esen, E., Mibach, F., Mibach, H., Utech, A., Gabelmann, M., Stumm, R., Ländle, V., Gartner, C., Goerg, C., Kaul, N., Messer, S., Burkhardt, D., Sander, C., Orthen, R., Kaes, S., Baumer, A., Dodos, F., Barth, A., Schaeffer, G., Gaertner, J., Winkler, J., Fahrig, A., Aring, J., Wenzel, I., Steiner, S., Kliesch, A., Kratz, E., Winter, K., Schneider, P., Haag, A., Mutscher, I., Bosch, R., Taggeselle, J., Meixner, S., Schnabel, A., Shamalla, A., Hötz, H., Korinth, A., Rheinert, C., Mehltretter, G., Schön, B., Schön, N., Starflinger, A., Englmann, E., Baytok, G., Laschinger, T., Ritscher, G., Gerth, A., Dechering, D., Eckardt, L., Kuhlmann, M., Proskynitopoulos, N., Brunn, J., Foth, K., Axthelm, C., Hohensee, H., Eberhard, K., Turbanisch, S., Hassler, N., Koestler, A., Stenzel, G., Kschiwan, D., Schwefer, M., Neiner, S., Hettwer, S., Haeussler-Schuchardt, M., Degenhardt, R., Sennhenn, S., Brendel, M., Stoehr, A., Widjaja, W., Loehndorf, S., Logemann, A., Hoskamp, J., Grundt, J., Block, M., Ulrych, R., Reithmeier, A., Panagopoulos, V., Martignani, C., Bernucci, D., Fantecchi, E., Diemberger, I., Ziacchi, M., Biffi, M., Cimaglia, P., Frisoni, J., Giannini, I., Boni, S., Fumagalli, S., Pupo, S., Di Chiara, A., Mirone, P., Pesce, F., Zoccali, C., Malavasi, V.L., Mussagaliyeva, A., Ahyt, B., Salihova, Z., Koshum-Bayeva, K., Kerimkulova, A., Bairamukova, A., Lurina, B., Zuzans, R., Jegere, S., Mintale, I., Kupics, K., Jubele, K., Kalejs, O., Vanhear, K., Burg, M., Cachia, M., Abela, E., Warwicker, S., Tabone, T., Xuereb, R., Asanovic, D., Drakalovic, D., Vukmirovic, M., Pavlovic, N., Music, L., Bulatovic, N., Boskovic, A., Uiterwaal, H., Bijsterveld, N., De Groot, J., Neefs, J., van den Berg, N., Piersma, F., Wilde, A., Hagens, V., Van Es, J., Van Opstal, J., Van Rennes, B., Verheij, H., Breukers, W., Tjeerdsma, G., Nijmeijer, R., Wegink, D., Binnema, R., Said, S., Philippens, S., van Doorn, W., Szili-Torok, T., Bhagwandien, R., Janse, P., Muskens, A., van Eck, M., Gevers, R., van der Ven, N., Duygun, A., Rahel, B., Meeder, J., Vold, A., Holst Hansen, C., Engset, I., Dyduch-Fejklowicz, B., Koba, E., Cichocka, M., Sokal, A., Kubicius, A., Pruchniewicz, E., Kowalik-Sztylc, A., Czapla, W., Mróz, I., Kozlowski, M., Pawlowski, T., Tendera, M., Winiarska-Filipek, A., Fidyk, A., Slowikowski, A., Haberka, M., Lachor-Broda, M., Biedron, M., Gasior, Z., Kołodziej, M., Janion, M., Gorczyca-Michta, I., Wozakowska-Kaplon, B., Stasiak, M., Jakubowski, P., Ciurus, T., Drozdz, J., Simiera, M., Zajac, P., Wcislo, T., Zycinski, P., Kasprzak, J., Olejnik, A., Harc-Dyl, E., Miarka, J., Pasieka, M., Ziemińska-Łuć, M., Bujak, W., Śliwiński, A., Grech, A., Morka, J., Petrykowska, K., Prasał, M., Hordyński, G., Feusette, P., Lipski, P., Wester, A., Streb, W., Romanek, J., Woźniak, P., Chlebuś, M., Szafarz, P., Stanik, W., Zakrzewski, M., Kaźmierczak, J., Przybylska, A., Skorek, E., Błaszczyk, H., Stępień, M., Szabowski, S., Krysiak, W., Szymańska, M., Karasiński, J., Blicharz, J., Skura, M., Hałas, K., Michalczyk, L., Orski, Z., Krzyżanowski, K., Skrobowski, A., Zieliński, L., Tomaszewska-Kiecana, M., Dłużniewski, M., Kiliszek, M., Peller, M., Budnik, M., Balsam, P., Opolski, G., Tymińska, A., Ozierański, K., Wancerz, A., Borowiec, A., Majos, E., Dabrowski, R., Szwed, H., Musialik-Lydka, A., Leopold-Jadczyk, A., Jedrzejczyk-Patej, E., Koziel, M., Mazurek, M., Krzemien-Wolska, K., Starosta, P., Nowalany-Kozielska, E., Orzechowska, A., Szpot, M., Staszel, M., Almeida, S., Pereira, H., Brandão Alves, L., Miranda, R., Ribeiro, L., Costa, F., Morgado, F., Carmo, P., Galvao Santos, P., Bernardo, R., Adragão, P., Ferreira da Silva, G., Peres, M., Alves, M., Leal, M., Cordeiro, A., Magalhães, P., Fontes, P., Leão, S., Delgado, A., Costa, A., Marmelo, B., Rodrigues, B., Moreira, D., Santos, J., Santos, L., Terchet, A., Darabantiu, D., Mercea, S., Turcin Halka, V., Pop Moldovan, A., Gabor, A., Doka, B., Catanescu, G., Rus, H., Oboroceanu, L., Bobescu, E., Popescu, R., Dan, A., Buzea, A., Daha, I., Dan, G., Neuhoff, I., Baluta, M., Ploesteanu, R., Dumitrache, N., Vintila, M., Daraban, A., Japie, C., Badila, E., Tewelde, H., Hostiuc, M., Frunza, S., Tintea, E., Bartos, D., Ciobanu, A., Popescu, I., Toma, N., Gherghinescu, C., Cretu, D., Patrascu, N., Stoicescu, C., Udroiu, C., Bicescu, G., Vintila, V., Vinereanu, D., Cinteza, M., Rimbas, R., Grecu, M., Cozma, A., Boros, F., Ille, M., Tica, O., Tor, R., Corina, A., Jeewooth, A., Maria, B., Georgiana, C., Natalia, C., Alin, D., Dinu-Andrei, D., Livia, M., Daniela, R., Larisa, R., Umaar, S., Tamara, T., Ioachim Popescu, M., Nistor, D., Sus, I., Coborosanu, O., Alina-Ramona, N., Dan, R., Petrescu, L., Ionescu, G., Vacarescu, C., Goanta, E., Mangea, M., Ionac, A., Mornos, C., Cozma, D., Pescariu, S., Solodovnicova, E., Soldatova, I., Shutova, J., Tjuleneva, L., Zubova, T., Uskov, V., Obukhov, D., Rusanova, G., Isakova, N., Odinsova, S., Arhipova, T., Kazakevich, E., Zavyalova, O., Novikova, T., Riabaia, I., Zhigalov, S., Drozdova, E., Luchkina, I., Monogarova, Y., Hegya, D., Rodionova, L., Nevzorova, V., Lusanova, O., Arandjelovic, A., Toncev, D., Vukmirovic, L., Radisavljevic, M., Milanov, M., Sekularac, N., Zdravkovic, M., Hinic, S., Dimkovic, S., Acimovic, T., Saric, J., Radovanovic, S., Kocijancic, A., Obrenovic-Kircanski, B., Kalimanovska Ostric, D., Simic, D., Jovanovic, I., Petrovic, I., Polovina, M., Vukicevic, M., Tomasevic, M., Mujovic, N., Radivojevic, N., Petrovic, O., Aleksandric, S., Kovacevic, V., Mijatovic, Z., Ivanovic, B., Tesic, M., Ristic, A., Vujisic-Tesic, B., Nedeljkovic, M., Karadzic, A., Uscumlic, A., Prodanovic, M., Zlatar, M., Asanin, M., Bisenic, B., Vasic, V., Popovic, Z., Djikic, D., Sipic, M., Peric, V., Dejanovic, B., Milosevic, N., Backovic, S., Stevanovic, A., Andric, A., Pencic, B., Pavlovic-Kleut, M., Celic, V., Pavlovic, M., Petrovic, M., Vuleta, M., Petrovic, N., Simovic, S., Savovic, Z., Milanov, S., Davidovic, G., Iric-Cupic, V., Djordjevic, D., Damjanovic, M., Zdravkovic, S., Topic, V., Stanojevic, D., Randjelovic, M., Jankovic-Tomasevic, R., Atanaskovic, V., Antic, S., Simonovic, D., Stojanovic, M., Stojanovic, S., Mitic, V., Ilic, V., Petrovic, D., Deljanin Ilic, M., Ilic, S., Stoickov, V., Markovic, S., Mijatovic, A., Tanasic, D., Radakovic, G., Peranovic, J., Panic-Jelic, N., Vujadinovic, O., Pajic, P., Bekic, S., Kovacevic, S., García Fernandez, A., Perez Cabeza, A., Anguita, M., Tercedor Sanchez, L., Mau, E., Loayssa, J., Ayarra, M., Carpintero, M., Roldán Rabadan, I., Gil Ortega, M., Tello Montoliu, A., Orenes Piñero, E., Manzano Fernández, S., Marín, F., Romero Aniorte, A., Veliz Martínez, A., Quintana Giner, M., Ballesteros, G., Palacio, M., Alcalde, O., García-Bolao, I., Bertomeu Gonzalez, V., Otero-Raviña, F., García Seara, J., Gonzalez Juanatey, J., Dayal, N., Maziarski, P., Gentil-Baron, P., Koç, M., Onrat, E., Dural, I.E., Yilmaz, K., Özin, B., Tan Kurklu, S., Atmaca, Y., Canpolat, U., Tokgozoglu, L., Dolu, A.K., Demirtas, B., Sahin, D., Ozcan Celebi, O., Gagirci, G., Turk, U.O., Ari, H., Polat, N., Toprak, N., Sucu, M., Akin Serdar, O., Taha Alper, A., Kepez, A., Yuksel, Y., Uzunselvi, A., Yuksel, S., Sahin, M., Kayapinar, O., Ozcan, T., Kaya, H., Yilmaz, M.B., Kutlu, M., Demir, M., Gibbs, C., Kaminskiene, S., Bryce, M., Skinner, A., Belcher, G., Hunt, J., Stancombe, L., Holbrook, B., Peters, C., Tettersell, S., Shantsila, A., Lane, D., Senoo, K., Proietti, M., Russell, K., Domingos, P., Hussain, S., Partridge, J., Haynes, R., Bahadur, S., Brown, R., McMahon, S., McDonald, J., Balachandran, K., Singh, R., Garg, S., Desai, H., Davies, K., Goddard, W., Galasko, G., Rahman, I., Chua, Y., Payne, O., Preston, S., Brennan, O., Pedley, L., Whiteside, C., Dickinson, C., Brown, J., Jones, K., Benham, L., Brady, R., Buchanan, L., Ashton, A., Crowther, H., Fairlamb, H., Thornthwaite, S., Relph, C., McSkeane, A., Poultney, U., Kelsall, N., Rice, P., Wilson, T., Wrigley, M., Kaba, R., Patel, T., Young, E., Law, J., Runnett, C., Thomas, H., McKie, H., Fuller, J., Pick, S., Sharp, A., Hunt, A., Thorpe, K., Hardman, C., Cusack, E., Adams, L., Hough, M., Keenan, S., Bowring, A., Watts, J., Zaman, J., Goffin, K., Nutt, H., Beerachee, Y., Featherstone, J., Mills, C., Pearson, J., Stephenson, L., Grant, S., Wilson, A., Hawksworth, C., Alam, I., Robinson, M., Ryan, S., Egdell, R., Gibson, E., Holland, M., Leonard, D., Mishra, B., Ahmad, S., Randall, H., Hill, J., Reid, L., George, M., McKinley, S., Brockway, L., Milligan, W., Sobolewska, J., Muir, J., Tuckis, L., Winstanley, L., Jacob, P., Kaye, S., Morby, L., Jan, A., Sewell, T., Boos, C., Wadams, B., Cope, C., Jefferey, P., Andrews, N., Getty, A., Suttling, A., Turner, C., Hudson, K., Austin, R., Howe, S., Iqbal, R., Gandhi, N., Brophy, K., Mirza, P., Willard, E., Collins, S., Ndlovu, N., Subkovas, E., Karthikeyan, V., Waggett, L., Wood, A., Bolger, A., Stockport, J., Evans, L., Harman, E., Starling, J., Williams, L., Saul, V., Sinha, M., Bell, L., Tudgay, S., Kemp, S., Frost, L., Ingram, T., Loughlin, A., Adams, C., Adams, M., Hurford, F., Owen, C., Miller, C., Donaldson, D., Tivenan, H., Button, H., Nasser, A., Jhagra, O., Stidolph, B., Brown, C., Livingstone, C., Duffy, M., Madgwick, P., Roberts, P., Greenwood, E., Fletcher, L., Beveridge, M., Earles, S., McKenzie, D., Beacock, D., Dayer, M., Seddon, M., Greenwell, D., Luxton, F., Venn, F., Mills, H., Rewbury, J., James, K., Roberts, K., Tonks, L., Felmeden, D., Taggu, W., Summerhayes, A., Hughes, D., Sutton, J., Felmeden, L., Khan, M., Walker, E., Norris, L., O'Donohoe, L., Mozid, A., Dymond, H., Lloyd-Jones, H., Saunders, G., Simmons, D., Coles, D., Cotterill, D., Beech, S., Kidd, S., Wrigley, B., Petkar, S., Smallwood, A., Jones, R., Radford, E., Milgate, S., Metherell, S., Cottam, V., Buckley, C., Broadley, A., Wood, D., Allison, J., Rennie, K., Balian, L., Howard, L., Pippard, L., Board, S., Pitt-Kerby, T., Vitolo, Marco, Malavasi, Vincenzo L., Proietti, Marco, Diemberger, Igor, Fauchier, Laurent, Marin, Francisco, Nabauer, Michael, Potpara, Tatjana S., Dan, Gheorghe-Andrei, Kalarus, Zbigniew, Tavazzi, Luigi, Maggioni, Aldo Pietro, Lane, Deirdre A., Lip, Gregory Y.H., and Boriani, Giuseppe

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2022
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173. Design of inertial fusion implosions reaching the burning plasma regime

Author

Kritcher, A. L., Young, C. V., Robey, H. F., Weber, C. R., Zylstra, A. B., Hurricane, O. A., Callahan, D. A., Ralph, J. E., Ross, J. S., Baker, K. L., Casey, D. T., Clark, D. S., Döppner, T., Divol, L., Hohenberger, M., Hopkins, L. Berzak, Le Pape, S., Meezan, N. B., Pak, A., Patel, P. K., Tommasini, R., Ali, S. J., Amendt, P. A., Atherton, L. J., Bachmann, B., Bailey, D., Benedetti, L. R., Betti, R., Bhandarkar, S. D., Biener, J., Bionta, R. M., Birge, N. W., Bond, E. J., Bradley, D. K., Braun, T., Briggs, T. M., Bruhn, M. W., Celliers, P. M., Chang, B., Chapman, T., Chen, H., Choate, C., Christopherson, A. R., Crippen, J. W., Dewald, E. L., Dittrich, T. R., Edwards, M. J., Farmer, W. A., Field, J. E., Fittinghoff, D., Frenje, J. A., Gaffney, J. A., Johnson, M. Gatu, Glenzer, S. H., Grim, G. P., Haan, S., Hahn, K. D., Hall, G. N., Hammel, B. A., Harte, J., Hartouni, E., Heebner, J. E., Hernandez, V. J., Herrmann, H., Herrmann, M. C., Hinkel, D. E., Ho, D. D., Holder, J. P., Hsing, W. W., Huang, H., Humbird, K. D., Izumi, N., Jarrott, L. C., Jeet, J., Jones, O., Kerbel, G. D., Kerr, S. M., Khan, S. F., Kilkenny, J., Kim, Y., Geppert-Kleinrath, H., Geppert-Kleinrath, V., Kong, C., Koning, J. M., Kruse, M. K. G., Kroll, J. J., Kustowski, B., Landen, O. L., Langer, S., Larson, D., Lemos, N. C., Lindl, J. D., Ma, T., MacDonald, M. J., MacGowan, B. J., Mackinnon, A. J., MacLaren, S. A., MacPhee, A. G., Marinak, M. M., Mariscal, D. A., Marley, E. V., Masse, L., Meaney, K., Michel, P. A., Millot, M., Milovich, J. L., Moody, J. D., Moore, A. S., Morton, J. W., Murphy, T., Newman, K., Di Nicola, J.-M. G., Nikroo, A., Nora, R., Patel, M. V., Pelz, L. J., Peterson, J. L., Ping, Y., Pollock, B. B., Ratledge, M., Rice, N. G., Rinderknecht, H., Rosen, M., Rubery, M. S., Salmonson, J. D., Sater, J., Schiaffino, S., Schlossberg, D. J., Schneider, M. B., Schroeder, C. R., Scott, H. A., Sepke, S. M., Sequoia, K., Sherlock, M. W., Shin, S., Smalyuk, V. A., Spears, B. K., Springer, P. T., Stadermann, M., Stoupin, S., Strozzi, D. J., Suter, L. J., Thomas, C. A., Town, R. P. J., Trosseille, C., Tubman, E. R., Volegov, P. L., Widmann, K., Wild, C., Wilde, C. H., Van Wonterghem, B. M., Woods, D. T., Woodworth, B. N., Yamaguchi, M., Yang, S. T., and Zimmerman, G. B.

Published
2022
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180. A Search for Dark Matter in the Galactic Halo with HAWC

Author

Abeysekara, A. U., Albert, A. M., Alfaro, R., Alvarez, C., Álvarez, J. D., Arceo, R., Arteaga-Velázquez, J. C., Rojas, D. Avila, Solares, H. A. Ayala, Becerril, A., Belmont-Moreno, E., BenZvi, S. Y., Bernal, A., Brisbois, C., Caballero-Mora, K. S., Capistrán, T., Carramiñana, A., Casanova, S., Castillo, M., Cotti, U., Cotzomi, J., De León, C., De la Fuente, E., Hernandez, R. Diaz, Dingus, B. L., DuVernois, M. A., Díaz-Vélez, J. C., Engel, K., Enríquez-Rivera, O., Fiorino, D. W., Fleischhack, H., Fraija, N., García-González, J. A., Garfias, F., Muñoz, A. González, González, M. M., Goodman, J. A., Hampel-Arias, Z., Harding, J. P., Hernandez, S., Hernandez-Almada, A., Hueyotl-Zahuantitla, F., Hüntemeyer, P., Iriarte, A., Jardin-Blicq, A., Joshi, V., Kaufmann, S., Lauer, R. J., Lee, W. H., Lennarz, D., Vargas, H. León, Linnemann, J. T., Longinotti, A. L., Luis-Raya, G., Luna-García, R., López-Coto, R., Malone, K., Marinelli, S. S., Martinez, O., Martinez-Castellanos, I., Martínez-Castro, J., Matthews, J. A., Miranda-Romagnoli, P., Moreno, E., Mostafá, M., Nellen, L., Newbold, M., Nisa, M. U., Noriega-Papaqui, R., Pelayo, R., Pretz, J., Pérez-Pérez, E. G., Ren, Z., Rho, C. D., Rodd, N. L., Rosa-González, D., Rosenberg, M., Ruiz-Velasco, E., Safdi, B. R., Salazar, H., Greus, F. Salesa, Sandoval, A., Schneider, M., Sinnis, G., Smith, A. J., Springer, R. W., Surajbali, P., Taboada, I., Tibolla, O., Tollefson, K., Torres, I., Ukwatta, T. N., Vianello, G., Villaseñor, L., Weisgarber, T., Westerhoff, S., Wisher, I. G., Wood, J., Yapici, T., Yodh, G. B., Younk, P. W., Zepeda, A., and Zhou, H.

Subjects
Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Cosmology and Nongalactic Astrophysics, High Energy Physics - Phenomenology
Abstract

The High Altitude Water Cherenkov (HAWC) gamma-ray observatory is a wide field-of-view observatory sensitive to 500 GeV - 100 TeV gamma rays and cosmic rays. With its observations over 2/3 of the sky every day, the HAWC observatory is sensitive to a wide variety of astrophysical sources, including possible gamma rays from dark matter. Dark matter annihilation and decay in the Milky Way Galaxy should produce gamma-ray signals across many degrees on the sky. The HAWC instantaneous field-of-view of 2 sr enables observations of extended regions on the sky, such as those from dark matter in the Galactic halo. Here we show limits on the dark matter annihilation cross-section and decay lifetime from HAWC observations of the Galactic halo with 15 months of data. These are some of the most robust limits on TeV and PeV dark matter, largely insensitive to the dark matter morphology. These limits begin to constrain models in which PeV IceCube neutrinos are explained by dark matter which primarily decays into hadrons., Comment: 24 pages, 11 figures

Published
2017
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181. Inference of the electron temperature in ICF implosions from the hard X-ray spectral continuum

Author

Kagan, Grigory, Landen, O. L., Svyatskiy, D., Sio, H., Kabadi, N. V., Simpson, R. A., Johnson, M. Gatu, Frenje, J. A., Petrasso, R. D., Shah, R. C., Joshi, T. R., Hakel, P., Weber, T. E., Rinderknecht, H. G., Thorn, D., Schneider, M., Bradley, D., and Kilkenny, J.

Subjects
Physics - Plasma Physics
Abstract

Using the free-free continuum self-emission spectrum at photon energies above 15 keV is one of the most promising concepts for assessing the electron temperature in ICF experiments. However, these photons are due to suprathermal electrons whose mean-free-path is much larger than thermal, making their distribution deviate from Maxwellian in a finite-size hot-spot. The first study of the free-free X-ray emission from an ICF implosion is conducted with the kinetic modifications to the electron distribution accounted for. These modifications are found to result in qualitatively new features in the hard X-ray spectral continuum. Inference of the electron temperature as if the emitting electrons are Maxwellian is shown to give a lower value than the actual one., Comment: Revised version accepted for publication

Published
2017

182. All-particle cosmic ray energy spectrum measured by the HAWC experiment from 10 to 500 TeV

Author

HAWC Collaboration, Alfaro, R., Alvarez, C., Arceo, R., Arteaga-Velázquez, J. C., Rojas, D. Avila, Solares, H. A. Ayala, Barber, A. S., Becerril, A., Belmont-Moreno, E., BenZvi, S. Y., Brisbois, C., Caballero-Mora, K. S., Capistrán, T., Carramiñana, A., Casanova, S., Castillo, M., Cotti, U., Cotzomi, J., de León, S. Coutiño, De León, C., De la Fuente, E., Hernandez, R. Diaz, Dichiara, S., Dingus, B. L., DuVernois, M. A., Díaz-Vélez, J. C., Ellsworth, R. W., Enriquez-Rivera, O., Fiorino, D. W., Fleischhack, H., Fraija, N., García-González, J. A., Muñoz, A. González, González, M. M., Goodman, J. A., Hampel-Arias, Z., Harding, J. P., Hernandez-Almada, A., Hinton, J., Hueyotl-Zahuantitla, F., Hui, C. M., Huntemeyer, P., Iriarte, A., Jardin-Blicq, A., Joshi, V., Kaufmann, S., Lara, A., Lauer, R. J., Lennarz, D., Vargas, H. León, Linnemann, J. T., Longinotti, A. L., Raya, G. Luis, Luna-García, R., López-Cámara, D., López-Coto, R., Malone, K., Marinelli, S. S., Martinez, O., Martinez-Castellanos, I., Martínez-Castro, J., Martínez-Huerta, H., Matthews, J. A., Miranda-Romagnoli, P., Moreno, E., Mostafá, M., Nellen, L., Newbold, M., Nisa, M. U., Noriega-Papaqui, R., Pelayo, R., Pretz, J., Pérez-Pérez, E. G., Ren, Z., Rho, C. D., Rivière, C., Rosa-González, D., Rosenberg, M., Ruiz-Velasco, E., Greus, F. Salesa, Sandoval, A., Schneider, M., Schoorlemmer, H., Sinnis, G., Smith, A. J., Springer, R. W., Surajbali, P., Taboada, I., Tibolla, O., Tollefson, K., Torres, I., Ukwatta, T. N., Villaseñor, L., Weisgarber, T., Westerhoff, S., Wood, J., Yapici, T., Zepeda, A., Zhou, H., and Álvarez, J. D.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

We report on the measurement of the all-particle cosmic ray energy spectrum with the High Altitude Water Cherenkov (HAWC) Observatory in the energy range 10 to 500 TeV. HAWC is a ground based air-shower array deployed on the slopes of Volcan Sierra Negra in the state of Puebla, Mexico, and is sensitive to gamma rays and cosmic rays at TeV energies. The data used in this work were taken from 234 days between June 2016 to February 2017. The primary cosmic-ray energy is determined with a maximum likelihood approach using the particle density as a function of distance to the shower core. Introducing quality cuts to isolate events with shower cores landing on the array, the reconstructed energy distribution is unfolded iteratively. The measured all-particle spectrum is consistent with a broken power law with an index of $-2.49\pm0.01$ prior to a break at $(45.7\pm0.1$) TeV, followed by an index of $-2.71\pm0.01$. The spectrum also respresents a single measurement that spans the energy range between direct detection and ground based experiments. As a verification of the detector response, the energy scale and angular resolution are validated by observation of the cosmic ray Moon shadow's dependence on energy., Comment: 16 pages, 11 figures, 4 tables, submission to Physical Review D

Published
2017
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183. Science with the Cherenkov Telescope Array

Author

Consortium, The Cherenkov Telescope Array, Acharya, B. S., Agudo, I., Samarai, I. Al, Alfaro, R., Alfaro, J., Alispach, C., Batista, R. Alves, Amans, J. -P., Amato, E., Ambrosi, G., Antolini, E., Antonelli, L. A., Aramo, C., Araya, M., Armstrong, T., Arqueros, F., Arrabito, L., Asano, K., Ashley, M., Backes, M., Balazs, C., Balbo, M., Ballester, O., Ballet, J., Bamba, A., Barkov, M., de Almeida, U. Barres, Barrio, J. A., Bastieri, D., Becherini, Y., Belfiore, A., Benbow, W., Berge, D., Bernardini, E., Bernardini, M. G., Bernardos, M., Bernlöhr, K., Bertucci, B., Biasuzzi, B., Bigongiari, C., Biland, A., Bissaldi, E., Biteau, J., Blanch, O., Blazek, J., Boisson, C., Bolmont, J., Bonanno, G., Bonardi, A., Bonavolontà, C., Bonnoli, G., Bosnjak, Z., Böttcher, M., Braiding, C., Bregeon, J., Brill, A., Brown, A. M., Brun, P., Brunetti, G., Buanes, T., Buckley, J., Bugaev, V., Bühler, R., Bulgarelli, A., Bulik, T., Burton, M., Burtovoi, A., Busetto, G., Canestrari, R., Capalbi, M., Capitanio, F., Caproni, A., Caraveo, P., Cárdenas, V., Carlile, C., Carosi, R., Carquín, E., Carr, J., Casanova, S., Cascone, E., Catalani, F., Catalano, O., Cauz, D., Cerruti, M., Chadwick, P., Chaty, S., Chaves, R. C. G., Chen, A., Chen, X., Chernyakova, M., Chikawa, M., Christov, A., Chudoba, J., Cieślar, M., Coco, V., Colafrancesco, S., Colin, P., Conforti, V., Connaughton, V., Conrad, J., Contreras, J. L., Cortina, J., Costa, A., Costantini, H., Cotter, G., Covino, S., Crocker, R., Cuadra, J., Cuevas, O., Cumani, P., D'Aì, A., D'Ammando, F., D'Avanzo, P., D'Urso, D., Daniel, M., Davids, I., Dawson, B., Dazzi, F., De Angelis, A., Anjos, R. de Cássia dos, De Cesare, G., De Franco, A., Pino, E. M. de Gouveia Dal, de la Calle, I., Lopez, R. de los Reyes, De Lotto, B., De Luca, A., De Lucia, M., de Naurois, M., Wilhelmi, E. de Oña, De Palma, F., De Persio, F., de Souza, V., Deil, C., Del Santo, M., Delgado, C., della Volpe, D., Di Girolamo, T., Di Pierro, F., Di Venere, L., Díaz, C., Dib, C., Diebold, S., Djannati-Ataï, A., Domínguez, A., Prester, D. Dominis, Dorner, D., Doro, M., Drass, H., Dravins, D., Dubus, G., Dwarkadas, V. V., Ebr, J., Eckner, C., Egberts, K., Einecke, S., Ekoume, T. R. N., Elsässer, D., Ernenwein, J. -P., Espinoza, C., Evoli, C., Fairbairn, M., Falceta-Goncalves, D., Falcone, A., Farnier, C., Fasola, G., Fedorova, E., Fegan, S., Fernandez-Alonso, M., Fernández-Barral, A., Ferrand, G., Fesquet, M., Filipovic, M., Fioretti, V., Fontaine, G., Fornasa, M., Fortson, L., Coromina, L. Freixas, Fruck, C., Fujita, Y., Fukazawa, Y., Funk, S., Füßling, M., Gabici, S., Gadola, A., Gallant, Y., Garcia, B., López, R. Garcia, Garczarczyk, M., Gaskins, J., Gasparetto, T., Gaug, M., Gerard, L., Giavitto, G., Giglietto, N., Giommi, P., Giordano, F., Giro, E., Giroletti, M., Giuliani, A., Glicenstein, J. -F., Gnatyk, R., Godinovic, N., Goldoni, P., Gómez-Vargas, G., González, M. M., González, J. M., Götz, D., Graham, J., Grandi, P., Granot, J., Green, A. J., Greenshaw, T., Griffiths, S., Gunji, S., Hadasch, D., Hara, S., Hardcastle, M. J., Hassan, T., Hayashi, K., Hayashida, M., Heller, M., Helo, J. C., Hermann, G., Hinton, J., Hnatyk, B., Hofmann, W., Holder, J., Horan, D., Hörandel, J., Horns, D., Horvath, P., Hovatta, T., Hrabovsky, M., Hrupec, D., Humensky, T. B., Hütten, M., Iarlori, M., Inada, T., Inome, Y., Inoue, S., Inoue, T., Inoue, Y., Iocco, F., Ioka, K., Iori, M., Ishio, K., Iwamura, Y., Jamrozy, M., Janecek, P., Jankowsky, D., Jean, P., Jung-Richardt, I., Jurysek, J., Kaaret, P., Karkar, S., Katagiri, H., Katz, U., Kawanaka, N., Kazanas, D., Khélifi, B., Kieda, D. B., Kimeswenger, S., Kimura, S., Kisaka, S., Knapp, J., Knödlseder, J., Koch, B., Kohri, K., Komin, N., Kosack, K., Kraus, M., Krause, M., Krauß, F., Kubo, H., Mezek, G. Kukec, Kuroda, H., Kushida, J., La Palombara, N., Lamanna, G., Lang, R. G., Lapington, J., Blanc, O. Le, Leach, S., Lees, J. -P., Lefaucheur, J., de Oliveira, M. A. Leigui, Lenain, J. -P., Lico, R., Limon, M., Lindfors, E., Lohse, T., Lombardi, S., Longo, F., López, M., López-Coto, R., Lu, C. -C., Lucarelli, F., Luque-Escamilla, P. L., Lyard, E., Maccarone, M. C., Maier, G., Majumdar, P., Malaguti, G., Mandat, D., Maneva, G., Manganaro, M., Mangano, S., Marcowith, A., Marín, J., Markoff, S., Martí, J., Martin, P., Martínez, M., Martínez, G., Masetti, N., Masuda, S., Maurin, G., Maxted, N., Mazin, D., Medina, C., Melandri, A., Mereghetti, S., Meyer, M., Minaya, I. A., Mirabal, N., Mirzoyan, R., Mitchell, A., Mizuno, T., Moderski, R., Mohammed, M., Mohrmann, L., Montaruli, T., Moralejo, A., Morcuende-Parrilla, D., Mori, K., Morlino, G., Morris, P., Morselli, A., Moulin, E., Mukherjee, R., Mundell, C., Murach, T., Muraishi, H., Murase, K., Nagai, A., Nagataki, S., Nagayoshi, T., Naito, T., Nakamori, T., Nakamura, Y., Niemiec, J., Nieto, D., Nikołajuk, M., Nishijima, K., Noda, K., Nosek, D., Novosyadlyj, B., Nozaki, S., O'Brien, P., Oakes, L., Ohira, Y., Ohishi, M., Ohm, S., Okazaki, N., Okumura, A., Ong, R. A., Orienti, M., Orito, R., Osborne, J. P., Ostrowski, M., Otte, N., Oya, I., Padovani, M., Paizis, A., Palatiello, M., Palatka, M., Paoletti, R., Paredes, J. M., Pareschi, G., Parsons, R. D., Pe'er, A., Pech, M., Pedaletti, G., Perri, M., Persic, M., Petrashyk, A., Petrucci, P., Petruk, O., Peyaud, B., Pfeifer, M., Piano, G., Pisarski, A., Pita, S., Pohl, M., Polo, M., Pozo, D., Prandini, E., Prast, J., Principe, G., Prokhorov, D., Prokoph, H., Prouza, M., Pühlhofer, G., Punch, M., Pürckhauer, S., Queiroz, F., Quirrenbach, A., Rainò, S., Razzaque, S., Reimer, O., Reimer, A., Reisenegger, A., Renaud, M., Rezaeian, A. H., Rhode, W., Ribeiro, D., Ribó, M., Richtler, T., Rico, J., Rieger, F., Riquelme, M., Rivoire, S., Rizi, V., Rodriguez, J., Fernandez, G. Rodriguez, Vázquez, J. J. Rodríguez, Rojas, G., Romano, P., Romeo, G., Rosado, J., Rovero, A. C., Rowell, G., Rudak, B., Rugliancich, A., Rulten, C., Sadeh, I., Safi-Harb, S., Saito, T., Sakaki, N., Sakurai, S., Salina, G., Sánchez-Conde, M., Sandaker, H., Sandoval, A., Sangiorgi, P., Sanguillon, M., Sano, H., Santander, M., Sarkar, S., Satalecka, K., Saturni, F. G., Schioppa, E. J., Schlenstedt, S., Schneider, M., Schoorlemmer, H., Schovanek, P., Schulz, A., Schussler, F., Schwanke, U., Sciacca, E., Scuderi, S., Seitenzahl, I., Semikoz, D., Sergijenko, O., Servillat, M., Shalchi, A., Shellard, R. C., Sidoli, L., Siejkowski, H., Sillanpää, A., Sironi, G., Sitarek, J., Sliusar, V., Slowikowska, A., Sol, H., Stamerra, A., Stanič, S., Starling, R., Stawarz, Ł., Stefanik, S., Stephan, M., Stolarczyk, T., Stratta, G., Straumann, U., Suomijarvi, T., Supanitsky, A. D., Tagliaferri, G., Tajima, H., Tavani, M., Tavecchio, F., Tavernet, J. -P., Tayabaly, K., Tejedor, L. A., Temnikov, P., Terada, Y., Terrier, R., Terzic, T., Teshima, M., Testa, V., Thoudam, S., Tian, W., Tibaldo, L., Tluczykont, M., Peixoto, C. J. Todero, Tokanai, F., Tomastik, J., Tonev, D., Tornikoski, M., Torres, D. F., Torresi, E., Tosti, G., Tothill, N., Tovmassian, G., Travnicek, P., Trichard, C., Trifoglio, M., Pujadas, I. Troyano, Tsujimoto, S., Umana, G., Vagelli, V., Vagnetti, F., Valentino, M., Vallania, P., Valore, L., van Eldik, C., Vandenbroucke, J., Varner, G. S., Vasileiadis, G., Vassiliev, V., Acosta, M. Vázquez, Vecchi, M., Vega, A., Vercellone, S., Veres, P., Vergani, S., Verzi, V., Vettolani, G. P., Viana, A., Vigorito, C., Villanueva, J., Voelk, H., Vollhardt, A., Vorobiov, S., Vrastil, M., Vuillaume, T., Wagner, S. J., Wagner, R., Walter, R., Ward, J. E., Warren, D., Watson, J. J., Werner, F., White, M., White, R., Wierzcholska, A., Wilcox, P., Will, M., Williams, D. A., Wischnewski, R., Wood, M., Yamamoto, T., Yamazaki, R., Yanagita, S., Yang, L., Yoshida, T., Yoshiike, S., Yoshikoshi, T., Zacharias, M., Zaharijas, G., Zampieri, L., Zandanel, F., Zanin, R., Zavrtanik, M., Zavrtanik, D., Zdziarski, A. A., Zech, A., Zechlin, H., Zhdanov, V. I., Ziegler, A., and Zorn, J.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Experiment
Abstract

The Cherenkov Telescope Array, CTA, will be the major global observatory for very high energy gamma-ray astronomy over the next decade and beyond. The scientific potential of CTA is extremely broad: from understanding the role of relativistic cosmic particles to the search for dark matter. CTA is an explorer of the extreme universe, probing environments from the immediate neighbourhood of black holes to cosmic voids on the largest scales. Covering a huge range in photon energy from 20 GeV to 300 TeV, CTA will improve on all aspects of performance with respect to current instruments. The observatory will operate arrays on sites in both hemispheres to provide full sky coverage and will hence maximize the potential for the rarest phenomena such as very nearby supernovae, gamma-ray bursts or gravitational wave transients. With 99 telescopes on the southern site and 19 telescopes on the northern site, flexible operation will be possible, with sub-arrays available for specific tasks. CTA will have important synergies with many of the new generation of major astronomical and astroparticle observatories. Multi-wavelength and multi-messenger approaches combining CTA data with those from other instruments will lead to a deeper understanding of the broad-band non-thermal properties of target sources. The CTA Observatory will be operated as an open, proposal-driven observatory, with all data available on a public archive after a pre-defined proprietary period. Scientists from institutions worldwide have combined together to form the CTA Consortium. This Consortium has prepared a proposal for a Core Programme of highly motivated observations. The programme, encompassing approximately 40% of the available observing time over the first ten years of CTA operation, is made up of individual Key Science Projects (KSPs), which are presented in this document., Comment: 213 pages, including references and glossary. Version 2: credits and references updated, some figures updated, and author list updated

Published
2017
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184. Data Acquisition Architecture and Online Processing System for the HAWC gamma-ray observatory

Author

HAWC collaboration, Abeysekara, A. U., Alfaro, R., Alvarez, C., Álvarez, J. D., Arceo, R., Arteaga-Velázquez, J. C., Solares, H. A. Ayala, Barber, A. S., Baughman, B. M., Bautista-Elivar, N., Gonzalez, J. Becerra, Belmont-Moreno, E., BenZvi, S. Y., Berley, D., Rosales, M. Bonilla, Braun, J., Caballero-Lopez, R. A., Caballero-Mora, K. S., Carramiñana, A., Castillo, M., Cotti, U., Cotzomi, J., de la Fuente, E., De León, C., DeYoung, T., Diaz-Cruz, J., Hernandez, R. Diaz, Díaz-Vélez, J. C., Dingus, B. L., DuVernois, M. A., Ellsworth, R. W., Fiorino, D. W., Fraija, N., Galindo, A., Garfias, F., González, M. M., Goodman, J. A., Grabski, V., Gussert, M., Hampel-Arias, Z., Harding, J. P., Hui, C. M., Hüntemeyer, P., Imran, A., Iriarte, A., Karn, P., Kieda, D., Kunde, G. J., Lara, A., Lauer, R. J., Lee, W. H., Lennarz, D., Vargas, H. León, Linares, E. C., Linnemann, J. T., Proper, M. Longo, Luna-García, R., Malone, K., Marinelli, A., Marinelli, S. S., Martinez, O., Martínez-Castro, J., Martínez-Huerta, H., Matthews, J. A. J., McEnery, J., Torres, E. Mendoza, Miranda-Romagnoli, P., Moreno, E., Mostafá, M., Nellen, L., Newbold, M., Noriega-Papaqui, R., Oceguera-Becerra, T., Patricelli, B., Pelayo, R., Pérez-Pérez, E. G., Pretz, J., Rivière, C., Rosa-González, D., Ruiz-Velasco, E., Ryan, J., Salazar, H., Greus, F. Salesa, Sanchez, F. E., Sandoval, A., Schneider, M., Silich, S., Sinni, G., Smith, A. J., Woodle, K. Sparks, Springer, R. W., Taboada, I., Toale, P. A., Tollefson, K., Torres, I., Ukwatta, T. N., Villaseñor, L., Weisgarber, T., Westerhoff, S., Wisher, I. G., Wood, J., Yapici, T., Yodh, G. B., Younk, P. W., Zaborov, D., Zepeda, A., and Zhou, H.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

The High Altitude Water Cherenkov observatory (HAWC) is an air shower array devised for TeV gamma-ray astronomy. HAWC is located at an altitude of 4100 m a.s.l. in Sierra Negra, Mexico. HAWC consists of 300 Water Cherenkov Detectors, each instrumented with 4 photomultiplier tubes (PMTs). HAWC re-uses the Front-End Boards from the Milagro experiment to receive the PMT signals. These boards are used in combination with Time to Digital Converters (TDCs) to record the time and the amount of light in each PMT hit (light flash). A set of VME TDC modules (128 channels each) is operated in a continuous (dead time free) mode. The TDCs are read out via the VME bus by Single-Board Computers (SBCs), which in turn are connected to a gigabit Ethernet network. The complete system produces ~ 500 MB/s of raw data. A high-throughput data processing system has been designed and built to enable real-time data analysis. The system relies on off-the-shelf hardware components, an open-source software technology for data transfers (ZeroMQ) and a custom software framework for data analysis (AERIE). Multiple trigger and reconstruction algorithms can be combined and run on blocks of data in a parallel fashion, producing a set of output data streams which can be analyzed in real time with minimal latency (< 5 s). This paper provides an overview of the hardware set-up and an in-depth description of the software design, covering both the TDC data acquisition system and the real-time data processing system. The performance of these systems is also discussed., Comment: 14 pages, 3 figures, submitted to Nucl. Instrum. Meth. A

Published
2017
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185. Cherenkov Telescope Array Contributions to the 35th International Cosmic Ray Conference (ICRC2017)

Author

Acero, F., Acharya, B. S., Portella, V. Acín, Adams, C., Agudo, I., Aharonian, F., Samarai, I. Al, Alberdi, A., Alcubierre, M., Alfaro, R., Alfaro, J., Alispach, C., Aloisio, R., Batista, R. Alves, Amans, J. -P., Amato, E., Ambrogi, L., Ambrosi, G., Ambrosio, M., Anderson, J., Anduze, M., Angüner, E. O., Antolini, E., Antonelli, L. A., Antonuccio, V., Antoranz, P., Aramo, C., Araya, M., Arcaro, C., Armstrong, T., Arqueros, F., Arrabito, L., Arrieta, M., Asano, K., Asano, A., Ashley, M., Aubert, P., Singh, C. B., Babic, A., Backes, M., Bajtlik, S., Balazs, C., Balbo, M., Ballester, O., Ballet, J., Ballo, L., Balzer, A., Bamba, A., Bandiera, R., Barai, P., Barbier, C., Barcelo, M., Barkov, M., de Almeida, U. Barres, Barrio, J. A., Bastieri, D., Bauer, C., Becciani, U., Becherini, Y., Tjus, J. Becker, Bednarek, W., Belfiore, A., Benbow, W., Benito, M., Berge, D., Bernardini, E., Bernardini, M. G., Bernardos, M., Bernhard, S., Bernlöhr, K., Salucci, C. Bertinelli, Bertucci, B., Besel, M. -A., Beshley, V., Bettane, J., Bhatt, N., Bhattacharyya, W., Bhattachryya, S., Biasuzzi, B., Bicknell, G., Bigongiari, C., Biland, A., Bilinsky, A., Bird, R., Bissaldi, E., Biteau, J., Bitossi, M., Blanch, O., Blasi, P., Blazek, J., Boccato, C., Bockermann, C., Boehm, C., Bohacova, M., Boisson, C., Bolmont, J., Bonanno, G., Bonardi, A., Bonavolontà, C., Bonnoli, G., Borkowski, J., Bose, R., Bosnjak, Z., Böttcher, M., Boutonnet, C., Bouyjou, F., Bowman, L., Bozhilov, V., Braiding, C., Brau-Nogué, S., Bregeon, J., Briggs, M., Brill, A., Brisken, W., Bristow, D., Britto, R., Brocato, E., Brown, A. M., Brown, S., Brügge, K., Brun, P., Brun, F., Brunetti, L., Brunetti, G., Bruno, P., Bryan, M., Buckley, J., Bugaev, V., Bühler, R., Bulgarelli, A., Bulik, T., Burton, M., Burtovoi, A., Busetto, G., Buson, S., Buss, J., Byrum, K., Caccianiga, A., Cameron, R., Canelli, F., Canestrari, R., Capalbi, M., Capasso, M., Capitanio, F., Caproni, A., Capuzzo-Dolcetta, R., Caraveo, P., Cárdenas, V., Cardenzana, J., Cardillo, M., Carlile, C., Caroff, S., Carosi, R., Carosi, A., Carquín, E., Carr, J., Casandjian, J. -M., Casanova, S., Cascone, E., Castro-Tirado, A. J., Mora, J. Castroviejo, Catalani, F., Catalano, O., Cauz, D., Silva, C. Celestino, Celli, S., Cerruti, M., Chabanne, E., Chadwick, P., Chakraborty, N., Champion, C., Chatterjee, A., Chaty, S., Chaves, R., Chen, A., Chen, X., Cheng, K., Chernyakova, M., Chikawa, M., Chitnis, V. R., Christov, A., Chudoba, J., Cieślar, M., Clark, P., Coco, V., Colafrancesco, S., Colin, P., Colombo, E., Colome, J., Colonges, S., Conforti, V., Connaughton, V., Conrad, J., Contreras, J. L., Cornat, R., Cortina, J., Costa, A., Costantini, H., Cotter, G., Courty, B., Covino, S., Covone, G., Cristofari, P., Criswell, S. J., Crocker, R., Croston, J., Crovari, C., Cuadra, J., Cuevas, O., Cui, X., Cumani, P., Cusumano, G., D'Aì, A., D'Ammando, F., D'Avanzo, P., D'Urso, D., Da Vela, P., Dale, Ø., Dang, V. T., Dangeon, L., Daniel, M., Davids, I., Dawson, B., Dazzi, F., De Angelis, A., De Caprio, V., Anjos, R. de Cássia dos, De Cesare, G., De Franco, A., De Frondat, F., Pino, E. M. de Gouveia Dal, de la Calle, I., De Lisio, C., Lopez, R. de los Reyes, De Lotto, B., De Luca, A., De Lucia, M., Neto, J. R. T. de Mello, de Naurois, M., Wilhelmi, E. de Oña, De Palma, F., De Persio, F., de Souza, V., Decock, J., Deil, C., Deiml, P., Del Santo, M., Delagnes, E., Deleglise, G., Reznicek, M. Delfino, Delgado, C., Mengual, J. Delgado, Della Ceca, R., della Volpe, D., Detournay, M., Devin, J., Di Girolamo, T., Di Giulio, C., Di Pierro, F., Di Venere, L., Diaz, L., Díaz, C., Dib, C., Dickinson, H., Diebold, S., Digel, S., Djannati-Ataï, A., Doert, M., Domínguez, A., Prester, D. Dominis, Donnarumma, I., Dorner, D., Doro, M., Dournaux, J. -L., Downes, T., Drake, G., Drappeau, S., Drass, H., Dravins, D., Drury, L., Dubus, G., Morå, K. Dundas, Durkalec, A., Dwarkadas, V., Ebr, J., Eckner, C., Edy, E., Egberts, K., Einecke, S., Eisch, J., Eisenkolb, F., Ekoume, T. R. N., Eleftheriadis, C., Elsässer, D., Emmanoulopoulos, D., Ernenwein, J. -P., Escarate, P., Eschbach, S., Espinoza, C., Evans, P., Evoli, C., Fairbairn, M., Falceta-Goncalves, D., Falcone, A., Ramazani, V. 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J., Hassan, T., Haubold, T., Haupt, A., Hayashi, K., Hayashida, M., He, H., Heller, M., Helo, J. C., Henault, F., Henri, G., Hermann, G., Hermel, R., Llorente, J. Herrera, Herrero, A., Hervet, O., Hidaka, N., Hinton, J., Hiroshima, N., Hirotani, K., Hnatyk, B., Hoang, J. K., Hoffmann, D., Hofmann, W., Holder, J., Horan, D., Hörandel, J., Hörbe, M., Horns, D., Horvath, P., Houles, J., Hovatta, T., Hrabovsky, M., Hrupec, D., Huet, J. -M., Hughes, G., Hui, D., Hull, G., Humensky, T. B., Hussein, M., Hütten, M., Iarlori, M., Ikeno, Y., Illa, J. M., Impiombato, D., Inada, T., Ingallinera, A., Inome, Y., Inoue, S., Inoue, T., Inoue, Y., Iocco, F., Ioka, K., Ionica, M., Iori, M., Iriarte, A., Ishio, K., Israel, G. L., Iwamura, Y., Jablonski, C., Jacholkowska, A., Jacquemier, J., Jamrozy, M., Janecek, P., Jankowsky, F., Jankowsky, D., Jansweijer, P., Jarnot, C., Jean, P., Johnson, C. A., Josselin, M., Jung-Richardt, I., Jurysek, J., Kaaret, P., Kachru, P., Kagaya, M., Kakuwa, J., Kalekin, O., Kankanyan, R., Karastergiou, A., Karczewski, M., Karkar, S., Katagiri, H., Kataoka, J., Katarzyński, K., Katz, U., Kawanaka, N., Kaye, L., Kazanas, D., Kelley-Hoskins, N., Khélifi, B., Kieda, D. B., Kihm, T., Kimeswenger, S., Kimura, S., Kisaka, S., Kishida, S., Kissmann, R., Kluźniak, W., Knapen, J., Knapp, J., Knödlseder, J., Koch, B., Kocot, J., Kohri, K., Komin, N., Kong, A., Konno, Y., Kosack, K., Kowal, G., Koyama, S., Kraus, M., Krause, M., Krauß, F., Krennrich, F., Kruger, P., Kubo, H., Kudryavtsev, V., Mezek, G. Kukec, Kumar, S., Kuroda, H., Kushida, J., Kushwaha, P., La Palombara, N., La Parola, V., La Rosa, G., Lahmann, R., Lalik, K., Lamanna, G., Landoni, M., Landriu, D., Landt, H., Lang, R. G., Lapington, J., Laporte, P., Blanc, O. Le, Flour, T. Le, Sidaner, P. Le, Leach, S., Leckngam, A., Lee, S. -H., Lee, W. H., Lees, J. -P., Lefaucheur, J., de Oliveira, M. A. 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Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

List of contributions from the Cherenkov Telescope Array Consortium presented at the 35th International Cosmic Ray Conference, July 12-20 2017, Busan, Korea., Comment: Index of Cherenkov Telescope Array conference proceedings at the ICRC2017, Busan, Korea

Published
2017

186. HAWC Contributions to the 35th International Cosmic Ray Conference (ICRC2017)

Author

Abeysekara, A. U., Albert, A., Alfaro, R., Alvarez, C., Álvarez, J. D., Arceo, R., Arteaga-Velázquez, J. C., Rojas, D. Avila, Solares, H. A. Ayala, Barber, A. S., Gonzalez, J. Becerra, Becerril, A., Belmont-Moreno, E., BenZvi, S. Y., Berley, D., Bernal, A., Brisbois, C., Caballero-Mora, K. S., Capistrán, T., Carramiñana, A., Casanova, S., Castillo, M., Cotti, U., Cotzomi, J., de León, S. Coutiño, De la Fuente, E., De León, C., DeYoung, T., Hernandez, R. Diaz, Diaz-Cruz, L., Díaz-Vélez, J. C., Dichiara, S., Dingus, B. L., DuVernois, M. A., Ellsworth, R. W., Engel, K., Enriquez-Rivera, O., Fick, B., Fiorino, D. W., Fleischhack, H., Flores, J. L., Fraija, N., García-González, J. A., Garcia-Luna, J. L., Garcia-Torales, G., Garfias, F., Gerhardt, M., González, M. M., Muñoz, A. González, Goodman, J. A., Gussert, M., Hampel-Arias, Z., Harding, J. P., Hernandez, S., Hernandez-Almada, A., Hinton, J., Hona, B., Hui, C. M., Hüntemeyer, P., Iriarte, A., Jardin-Blicq, A., Joshi, V., Kaufmann, S., Kieda, D., Kunde, G. J., Lara, A., Lauer, R. J., Lee, W. H., Lennarz, D., Vargas, H. León, Linnemann, J. T., Longinotti, A. L., Proper, M. Longo, López-Coto, R., Raya, G. Luis, Luna-García, R., Malone, K., Marandon, V., Marinelli, S. S., Martinez, O., Martinez-Castellanos, I., Martínez-Castro, J., Martínez-Huerta, H., Matthews, J. A. J., McEnery, J., Miranda-Romagnoli, P., Moreno, E., Mostafá, M., Nellen, L., Newbold, M., Nisa, M. U., Noriega-Papaqui, R., Pelayo, R., Pérez-Pérez, E. G., Pretz, J., Ren, Z., Rho, C. D., Rivière, C., Rosa-González, D., Rosenberg, M., Ruiz-Velasco, E., Ryan, J., Salazar, H., Greus, F. Salesa, Sandoval, A., Schneider, M., Schoorlemmer, H., Sinnis, G., Smith, A. J., Smith, A. W., Springer, R. W., Surajbali, P., Taboada, I., Tibolla, O., Tollefson, K., Torres, I., Ukwatta, T. N., Vianello, G., Weisgarber, T., Westerhoff, S., Wood, J., Yapici, T., Yodh, G. B., Younk, P. W., Zepeda, A., and Zhou, H.

Subjects
Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Experiment
Abstract

List of proceedings from the HAWC Collaboration presented at the 35th International Cosmic Ray Conference, 12 July - 20 July 2017, Bexco, Busan, Korea., Comment: List of proceedings from the HAWC Collaboration presented at ICRC2017. Corrected typos in the index of the previous version. Follow the "HTML" link to access the list

Published
2017

187. Collapse of superconductivity in cuprates via ultrafast quenching of phase coherence

Author

Boschini, F., Neto, E. H. da Silva, Razzoli, E., Zonno, M., Peli, S., Day, R. P., Michiardi, M., Schneider, M., Zwartsenberg, B., Nigge, P., Zhong, R. D., Schneeloch, J., Gu, G. D., Zhdanovich, S., Mills, A. K., Levy, G., Jones, D. J., Giannetti, C., and Damascelli, A.

Subjects
Condensed Matter - Superconductivity, Condensed Matter - Strongly Correlated Electrons
Abstract

The possibility of driving phase transitions in low-density condensates through the loss of phase coherence alone has far-reaching implications for the study of quantum phases of matter. This has inspired the development of tools to control and explore the collective properties of condensate phases via phase fluctuations. Electrically-gated oxide interfaces, ultracold Fermi atoms, and cuprate superconductors, which are characterized by an intrinsically small phase-stiffness, are paradigmatic examples where these tools are having a dramatic impact. Here we use light pulses shorter than the internal thermalization time to drive and probe the phase fragility of the Bi$_2$Sr$_2$CaCu$_2$O$_{8+\delta}$ cuprate superconductor, completely melting the superconducting condensate without affecting the pairing strength. The resulting ultrafast dynamics of phase fluctuations and charge excitations are captured and disentangled by time-resolved photoemission spectroscopy. This work demonstrates the dominant role of phase coherence in the superconductor-to-normal state phase transition and offers a benchmark for non-equilibrium spectroscopic investigations of the cuprate phase diagram., Comment: 24 pages, 9 figures, Main Text and Supplementary Information

Published
2017
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188. Magneto-resistance oscillations induced by high-intensity terahertz radiation

Author

Herrmann, T., Kvon, Z. D., Dmitriev, I. A., Kozlov, D. A., Jentzsch, B., Schneider, M., Schell, L., Bel'kov, V. V., Bayer, A., Schuh, D., Bougeard, D., Kuczmik, T., Oltscher, M., Weiss, D., and Ganichev, S. D.

Subjects
Condensed Matter - Mesoscale and Nanoscale Physics
Abstract

We report on observation of pronounced terahertz radiation-induced magneto-resistivity oscillations in AlGaAs/GaAs two-dimensional electron systems, the THz analog of the microwave induced resistivity oscillations (MIRO). Applying high power radiation of a pulsed molecular laser we demonstrate that MIRO, so far observed at low power only, are not destroyed even at very high intensities. Experiments with radiation intensity ranging over five orders of magnitude from $0.1$ W/cm$^2$ to $10^4$ W/cm$^2$ reveal high-power saturation of the MIRO amplitude, which is well described by an empirical fit function $I/(1 + I/I_s)^\beta$ with $\beta \sim 1$. The saturation intensity Is is of the order of tens of W/cm$^2$ and increases by six times by increasing the radiation frequency from $0.6$ to $1.1$ THz. The results are discussed in terms of microscopic mechanisms of MIRO and compared to nonlinear effects observed earlier at significantly lower excitation frequencies., Comment: 10 pages, 9 figures

Published
2017
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189. Dark Matter Limits From Dwarf Spheroidal Galaxies with The HAWC Gamma-Ray Observatory

Author

Albert, A., Alfaro, R., Alvarez, C., Álvarez, J. D., Arceo, R., Arteaga-Velázquez, J. C., Rojas, D. Avila, Solares, H. A. Ayala, Bautista-Elivar, N., Becerril, A., Belmont-Moreno, E., BenZvi, S. Y., Bernal, A., Braun, J., Caballero-Mora, K. S., Capistrán, T., Carramiñana, A., Castillo, M., Cotti, U., De León, C., De la Fuente, E., Hernandez, R. Diaz, Dingus, B. L., DuVernois, M. A., Díaz-Vélez, J. C., Ellsworth, R. W., Fiorino, D. W., Fraija, N., García-González, J. A., Garfias, F., González, M. M., Goodman, J. A., Harding, J. P., Hernandez, S., Hernandez-Almada, A., Iriarte, A., Joshi, V., Kaufmann, S., Kieda, D., Lauer, R. J., Lennarz, D., Vargas, H. León, Linnemann, J. T., Longinotti, A. L., Raya, G. Luis, López-Coto, R., Malone, K., Marinelli, S. S., Martinez-Castellanos, I., Martínez-Castro, J., Martínez-Huerta, H., Matthews, J. A., Miranda-Romagnoli, P., Moreno, E., Nellen, L., Newbold, M., Nisa, M. U., Noriega-Papaqui, R., Pelayo, R., Pretz, J., Pérez-Pérez, E. G., Ren, Z., Rho, C. D., Rivière, C., Rosa-González, D., Ruiz-Velasco, E., Greus, F. Salesa, Sandoval, A., Schneider, M., Schoorlemmer, H., Sinnis, G., Smith, A. J., Springer, R. W., Surajbali, P., Taboada, I., Tibolla, O., Tollefson, K., Torres, I., Weisgarber, T., Yapici, T., and Zhou, H.

Subjects
Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Phenomenology
Abstract

The High Altitude Water Cherenkov (HAWC) gamma-ray observatory is a wide field of view observatory sensitive to 500 GeV - 100 TeV gamma rays and cosmic rays. It can also perform diverse indirect searches for dark matter (DM) annihilation and decay. Among the most promising targets for the indirect detection of dark matter are dwarf spheroidal galaxies. These objects are expected to have few astrophysical sources of gamma rays but high dark matter content, making them ideal candidates for an indirect dark matter detection with gamma rays. Here we present individual limits on the annihilation cross section and decay lifetime for 15 dwarf spheroidal galaxies within the HAWC field-of-view, as well as their combined limit. These are the first limits on the annihilation cross section and decay lifetime using data collected with HAWC., Comment: 18 pages, 6 figures, 2 tables

Published
2017
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190. Search for very-high-energy emission from Gamma-ray Bursts using the first 18 months of data from the HAWC Gamma-ray Observatory

Author

The HAWC collaboration, Alfaro, R., Alvarez, C., Álvarez, J. D., Arceo, R., Arteaga-Velázquez, J. C., Rojas, D. Avila, Solares, H. A. Ayala, Barber, A. S., Bautista-Elivar, N., Becerril, A., Belmont-Moreno, E., BenZvi, S. Y., Bernal, A., Braun, J., Brisbois, C., Caballero-Mora, K. S., Capistrán, T., Carramiñana, A., Casanova, S., Castillo, M., Cotti, U., Cotzomi, J., de León, S. Coutiño, de la Fuente, E., De León, C., DeYoung, T., Hernandez, R. Diaz, Dingus, B. L., DuVernois, M. A., Díaz-Vélez, J. C., Ellsworth, R. W., Engel, K., Fiorino, D. W., Fraija, N., García-González, J. A., Garfias, F., Gerhardt, M., Muñoz, A. González, González, M. M., Goodman, J. A., Hampel-Arias, Z., Harding, J. P., Hernandez-Almada, A., Hernandez, S., Hona, B., Hui, C. M., Hüntemeyer, P., Iriarte, A., Jardin-Blicq, A., Joshi, V., Kaufmann, S., Kieda, D., Lauer, R. J., Lee, W. H., Lennarz, D., Vargas, H. León, Linnemann, J. T., Longinotti, A. L., Raya, G. Luis, Luna-García, R., Malone, K., Marinelli, S. S., Martinez, O., Martinez-Castellanos, I., Martínez-Castro, J., Martínez-Huerta, H., Matthews, J. A., Miranda-Romagnoli, P., Moreno, E., Mostafá, M., Nellen, L., Newbold, M., Noriega-Papaqui, R., Pelayo, R., Pérez-Pérez, E. G., Pretz, J., Ren, Z., Rho, C. D., Rivière, C., Rosa-González, D., Rosenberg, M., Ruiz-Velasco, E., Salazar, H., Greus, F. Salesa, Sandoval, A., Schneider, M., Schoorlemmer, H., Sinnis, G., Smith, A. J., Springer, R. W., Surajbali, P., Taboada, I., Tibolla, O., Tollefson, K., Torres, I., Ukwatta, T. N., Vianello, G., Weisgarber, T., Westerhoff, S., Wood, J., Yapici, T., Younk, P. W., Zepeda, A., and Zhou, H.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

The High Altitude Water Cherenkov (HAWC) Gamma-ray Observatory is an extensive air shower detector operating in central Mexico, which has recently completed its first two years of full operations. If for a burst like GRB 130427A at a redshift of 0.34 and a high-energy component following a power law with index -1.66, the high-energy component is extended to higher energies with no cut-off other than from extragalactic background light attenuation, HAWC would observe gamma rays with a peak energy of $\sim$300 GeV. This paper reports the results of HAWC observations of 64 gamma-ray bursts (GRBs) detected by $\mathit{Swift}$ and $\mathit{Fermi}$, including three GRBs that were also detected by the Large Area Telescope ($\mathit{Fermi}$-LAT). An ON/OFF analysis method is employed, searching on the time scale given by the observed light curve at keV-MeV energies and also on extended time scales. For all GRBs and time scales, no statistically significant excess of counts is found and upper limits on the number of gamma rays and the gamma-ray flux are calculated. GRB 170206A, the third brightest short GRB detected by the Gamma-ray Burst Monitor on board the $\mathit{Fermi}$ satellite ($\mathit{Fermi}$-GBM) and also detected by the LAT, occurred very close to zenith. The LAT measurements can neither exclude the presence of a synchrotron self-Compton (SSC) component nor constrain its spectrum. Instead, the HAWC upper limits constrain the expected cut-off in an additional high-energy component to be less than $100~\rm{GeV}$ for reasonable assumptions about the energetics and redshift of the burst., Comment: 19 pages, 6 figures, published in ApJ

Published
2017
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191. The HAWC real-time flare monitor for rapid detection of transient events

Author

Abeysekara, A. U., Alfaro, R., Alvarez, C., Álvarez, J. D., Arceo, R., Arteaga-Velázquez, J. C., Rojas, D. Avila, Solares, H. A. Ayala, Barber, A. S., Bautista-Elivar, N., Gonzalez, J. Becerra, Becerril, A., Belmont-Moreno, E., BenZvi, S. Y., Bernal, A., Braun, J., Brisbois, C., Caballero-Mora, K. S., Capistrán, T., Carramiñana, A., Casanova, S., Castillo, M., Cotti, U., Cotzomi, J., de León, S. Coutiño, De la Fuente, E., De León, C., Díaz-Vélez, J. C., Dingus, B. L., DuVernois, M. A., Ellsworth, R. W., Engel, K., Fiorino, D. W., Fraija, N., García-González, J. A., Garfias, F., Gerhardt, M., González, M. M., Muñoz, A. González, Goodman, J. A., Hampel-Arias, Z., Harding, J. P., Hernandez, S., Hernandez-Almada, A., Hona, B., Hui, C. M., Hüntemeyer, P., Iriarte, A., Jardin-Blicq, A., Joshi, V., Kaufmann, S., Kieda, D., Lauer, R. J., Lee, W. H., Lennarz, D., Vargas, H. León, Linnemann, J. T., Longinotti, A. L., López-Cámara, D., López-Coto, R., Raya, G. Luis, Luna-García, R., Malone, K., Marinelli, S. S., Martinez, O., Martinez-Castellanos, I., Martínez-Castro, J., Martínez-Huerta, H., Matthews, J. A., Miranda-Romagnoli, P., Moreno, E., Mostafá, M., Nellen, L., Newbold, M., Nisa, M. U., Noriega-Papaqui, R., Pelayo, R., Pérez-Pérez, E. G., Pretz, J., Ren, Z., Rho, C. D., Rivière, C., Rosa-González, D., Rosenberg, M., Ruiz-Velasco, E., Salazar, H., Greus, F. Salesa, Sandoval, A., Schneider, M., Schoorlemmer, H., Sinnis, G., Smith, A. J., Springer, R. W., Surajbali, P., Taboada, I., Tibolla, O., Tollefson, K., Torres, I., Ukwatta, T. N., Vianello, G., Weisgarber, T., Westerhoff, S., Wisher, I. G., Wood, J., Yapici, T., Younk, P. W., Zepeda, A., and Zhou, H.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

We present the development of a real-time flare monitor for the High Altitude Water Cherenkov (HAWC) observatory. The flare monitor has been fully operational since 2017 January and is designed to detect very high energy (VHE; $E\gtrsim100$ GeV) transient events from blazars on time scales lasting from 2 minutes to 10 hours in order to facilitate multiwavelength and multimessenger studies. These flares provide information for investigations into the mechanisms that power the blazars' relativistic jets and accelerate particles within them, and they may also serve as probes of the populations of particles and fields in intergalactic space. To date, the detection of blazar flares in the VHE range has relied primarily on pointed observations by imaging atmospheric Cherenkov telescopes. The recently completed HAWC observatory offers the opportunity to study VHE flares in survey mode, scanning 2/3 of the entire sky every day with a field of view of $\sim$1.8 steradians. In this work, we report on the sensitivity of the HAWC real-time flare monitor and demonstrate its capabilities via the detection of three high-confidence VHE events in the blazars Markarian 421 and Markarian 501., Comment: 19 pages, 14 figures, revised version submitted to The Astrophysical Journal on 1 June 2017

Published
2017
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192. Daily monitoring of TeV gamma-ray emission from Mrk 421, Mrk 501, and the Crab Nebula with HAWC

Author

Abeysekara, A. U., Albert, A., Alfaro, R., Alvarez, C., Álvarez, J. D., Arceo, R., Arteaga-Velázquez, J. C., Rojas, D. Avila, Solares, H. A. Ayala, Barber, A. S., Bautista-Elivar, N., Gonzalez, J. Becerra, Becerril, A., Belmont-Moreno, E., BenZvi, S. Y., Bernal, A., Braun, J., Brisbois, C., Caballero-Mora, K. S., Capistrán, T., Carramiñana, A., Casanova, S., Castillo, M., Cotti, U., Cotzomi, J., de León, S. Coutiño, De León, C., De la Fuente, E., Hernandez, R. Diaz, Dingus, B. L., DuVernois, M. A., Díaz-Vélez, J. C., Ellsworth, R. W., Engel, K., Fiorino, D. W., Fraija, N., García-González, J. A., Garfias, F., Gerhardt, M., Muñoz, A. González, González, M. M., Goodman, J. A., Hampel-Arias, Z., Harding, J. P., Hernandez, S., Hernandez-Almada, A., Hona, B., Hui, C. M., Hüntemeyer, P., Iriarte, A., Jardin-Blicq, A., Joshi, V., Kaufmann, S., Kieda, D., Lara, A., Lauer, R. J., Lee, W. H., Lennarz, D., Vargas, H. León, Linnemann, J. T., Longinotti, A. L., Raya, G. Luis, Luna-García, R., López-Coto, R., Malone, K., Marinelli, S. S., Martinez, O., Martinez-Castellanos, I., Martínez-Castro, J., Matthews, J. A., Miranda-Romagnoli, P., Moreno, E., Mostafá, M., Nellen, L., Newbold, M., Nisa, M. U., Noriega-Papaqui, R., Pretz, J., Pérez-Pérez, E. G., Ren, Z., Rho, C. D., Rivière, C., Rosa-González, D., Rosenberg, M., Ruiz-Velasco, E., Greus, F. Salesa, Sandoval, A., Schneider, M., Schoorlemmer, H., Sinnis, G., Smith, A. J., Springer, R. W., Surajbali, P., Taboada, I., Tibolla, O., Tollefson, K., Torres, I., Ukwatta, T. N., Vianello, G., Weisgarber, T., Westerhoff, S., Wisher, I. G., Wood, J., Yapici, T., Younk, P. W., Zepeda, A., and Zhou, H.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

We present results from daily monitoring of gamma rays in the energy range $\sim0.5$ to $\sim100$ TeV with the first 17 months of data from the High Altitude Water Cherenkov (HAWC) Observatory. Its wide field of view of 2 steradians and duty cycle of $>95$% are unique features compared to other TeV observatories that allow us to observe every source that transits over HAWC for up to $\sim6$ hours each sidereal day. This regular sampling yields unprecedented light curves from unbiased measurements that are independent of seasons or weather conditions. For the Crab Nebula as a reference source we find no variability in the TeV band. Our main focus is the study of the TeV blazars Markarian (Mrk) 421 and Mrk 501. A spectral fit for Mrk 421 yields a power law index $\Gamma=2.21 \pm0.14_{\mathrm{stat}}\pm0.20_{\mathrm{sys}}$ and an exponential cut-off $E_0=5.4 \pm 1.1_{\mathrm{stat}}\pm 1.0_{\mathrm{sys}}$ TeV. For Mrk 501, we find an index $\Gamma=1.60\pm 0.30_{\mathrm{stat}} \pm 0.20_{\mathrm{sys}}$ and exponential cut-off $E_0=5.7\pm 1.6_{\mathrm{stat}} \pm 1.0_{\mathrm{sys}}$ TeV. The light curves for both sources show clear variability and a Bayesian analysis is applied to identify changes between flux states. The highest per-transit fluxes observed from Mrk 421 exceed the Crab Nebula flux by a factor of approximately five. For Mrk 501, several transits show fluxes in excess of three times the Crab Nebula flux. In a comparison to lower energy gamma-ray and X-ray monitoring data with comparable sampling we cannot identify clear counterparts for the most significant flaring features observed by HAWC., Comment: 18 pages, 10 figures, accepted for publication in The Astrophysical Journal

Published
2017
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193. A foam model highlights the differences of the macro- and microrheology of respiratory horse mucus

Author

Gros, A., Torge, A., Schaefer, U. F., Schneider, M., Lehr, C. M., and Wagner, C.

Subjects
Condensed Matter - Soft Condensed Matter, Condensed Matter - Materials Science, Physics - Biological Physics, Quantitative Biology - Biomolecules
Abstract

Native horse mucus is characterized with micro- and macrorheology and compared to hydroxyethylcellulose (HEC) gel as a model. Both systems show comparable viscoelastic properties on the microscale and for the HEC the macrorheology is in good agreement with the microrheology. For the mucus, the viscoelastic moduli on the macroscale are several orders of magnitude larger than on the microscale. Large amplitude oscillatory shear experiments show that the mucus responds nonlinearly at much smaller deformations than HEC. This behavior fosters the assumption that the mucus has a foam like structure on the microscale compared to the typical mesh like structure of the HEC, a model that is supported by cryogenic-scanning-electron-microscopy (CSEM) images. These images allow also to determine the relative amount of volume that is occupied by the pores and the scaffold. Consequently, we can estimate the elastic modulus of the scaffold. We conclude that this particular foam like microstructure should be considered as a key factor for the transport of particulate matter which plays a central role in mucus function with respect to particle penetration. The mesh properties composed of very different components are responsible for macroscopic and microscopic behavior being part of particles fate after landing., Comment: Accepted for publication in the Journal of the Mechanical Behavior of Biomedical Materials

Published
2017

194. Search for Very High Energy Gamma Rays from the Northern $\textit{Fermi}$ Bubble Region with HAWC

Author

Abeysekara, A. U., Albert, A., Alfaro, R., Alvarez, C., Álvarez, J. D., Arceo, R., Arteaga-Velázquez, J. C., Solares, H. A. Ayala, Barber, A. S., Bautista-Elivar, N., Becerril, A., Belmont-Moreno, E., BenZvi, S. Y., Berley, D., Braun, J., Brisbois, C., Caballero-Mora, K. S., Capistrán, T., Carramiñana, A., Casanova, S., Castillo, M., Cotti, U., Cotzomi, J., de León, S. Coutiño, De León, C., De la Fuente, E., Hernandez, R. Diaz, Dingus, B. L., DuVernois, M. A., Díaz-Vélez, J. C., Ellsworth, R. W., Engel, K., Fick, B., Fiorino, D. W., Fleischhack, H., Fraija, N., García-González, J. A., Garfias, F., Gerhardt, M., Muñoz, A. González, González, M. M., Goodman, J. A., Hampel-Arias, Z., Harding, J. P., Hernandez, S., Hernandez-Almada, A., Hinton, J., Hona, B., Hui, C. M., Hüntemeyer, P., Iriarte, A., Jardin-Blicq, A., Joshi, V., Kaufmann, S., Kieda, D., Lara, A., Lauer, R. J., Lee, W. H., Lennarz, D., Vargas, H. León, Linnemann, J. T., Longinotti, A. L., Raya, G. Luis, Luna-García, R., López-Coto, R., Malone, K., Marinelli, S. S., Martinez, O., Martinez-Castellanos, I., Martínez-Castro, J., Martínez-Huerta, H., Matthews, J. A., Miranda-Romagnoli, P., Moreno, E., Mostafá, M., Nellen, L., Newbold, M., Nisa, M. U., Noriega-Papaqui, R., Pelayo, R., Pretz, J., Pérez-Pérez, E. G., Ren, Z., Rho, C. D., Rivière, C., Rosa-González, D., Rosenberg, M., Ruiz-Velasco, E., Salazar, H., Greus, F. Salesa, Sandoval, A., Schneider, M., Schoorlemmer, H., Sinnis, G., Smith, A. J., Springer, R. W., Surajbali, P., Taboada, I., Tibolla, O., Tollefson, K., Torres, I., Ukwatta, T. N., Vianello, G., Weisgarber, T., Westerhoff, S., Wisher, I. G., Wood, J., Yapici, T., Yodh, G. B., Zepeda, A., and Zhou, H.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

We present a search of very high energy gamma-ray emission from the Northern $\textit{Fermi}$ Bubble region using data collected with the High Altitude Water Cherenkov (HAWC) gamma-ray observatory. The size of the data set is 290 days. No significant excess is observed in the Northern $\textit{Fermi}$ Bubble region, hence upper limits above $1\,\text{TeV}$ are calculated. The upper limits are between $3\times 10^{-7}\,\text{GeV}\, \text{cm}^{-2}\, \text{s}^{-1}\,\text{sr}^{-1}$ and $4\times 10^{-8}\,\text{GeV}\,\text{cm}^{-2}\,\text{s}^{-1}\,\text{sr}^{-1}$. The upper limits disfavor a proton injection spectrum that extends beyond $100\,\text{TeV}$ without being suppressed. They also disfavor a hadronic injection spectrum derived from neutrino measurements.

Published
2017
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195. Multiwavelength follow-up of a rare IceCube neutrino multiplet

Author

Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Samarai, I. Al, Altmann, D., Andeen, K., Anderson, T., Ansseau, I., Anton, G., Archinger, M., Argüelles, C., Auffenberg, J., Axani, S., Bai, X., Barwick, S. W., Baum, V., Bay, R., Beatty, J. J., Tjus, J. Becker, Becker, K. -H., BenZvi, S., Berley, D., Bernardini, E., Bernhard, A., Besson, D. Z., Binder, G., Bindig, D., Blaufuss, E., Blot, S., Bohm, C., Börner, M., Bos, F., Bose, D., Böser, S., Botner, O., Braun, J., Brayeur, L., Bretz, H. -P., Bron, S., Burgman, A., Carver, T., Casier, M., Cheung, E., Chirkin, D., Christov, A., Clark, K., Classen, L., Coenders, S., Collin, G. H., Conrad, J. M., Cowen, D. F., Cross, R., Day, M., de, J. P. A. M., ré, De Clercq, C., Rosendo, E. del Pino, Dembinski, H., De Ridder, S., Desiati, P., de Vries, K. D., de Wasseige, G., de With, M., DeYoung, T., di Lorenzo, V., Dujmovic, H., Dumm, J. P., Dunkman, M., Eberhardt, B., Ehrhardt, T., Eichmann, B., Eller, P., Euler, S., Evenson, P. A., Fahey, S., Fazely, A. R., Feintzeig, J., Felde, J., Filimonov, K., Finley, C., Flis, S., Fösig, C. -C., Franckowiak, A., Friedman, E., Fuchs, T., Gaisser, T. K., Gallagher, J., Gerhardt, L., Ghorbani, K., Giang, W., Gladstone, L., Glauch, T., Glüsenkamp, T., Goldschmidt, A., Gonzalez, J. G., Grant, D., Griffith, Z., Haack, C., Hallgren, A., Halzen, F., Hansen, E., Hansmann, T., Hanson, K., Hebecker, D., Heereman, D., Helbing, K., Hellauer, R., Hickford, S., Hignight, J., Hill, G. C., Hoffman, K. D., Hoffmann, R., Hoshina, K., Huang, F., Huber, M., Hultqvist, K., In, S., Ishihara, A., Jacobi, E., Japaridze, G. S., Jeong, M., Jero, K., Jones, B. J. P., Kang, W., Kappes, A., Karg, T., Karle, A., Katz, U., Kauer, M., Keivani, A., Kelley, J. L., Kheirandish, A., Kim, J., Kim, M., Kintscher, T., Kiryluk, J., Kittler, T., Klein, S. R., Kohnen, G., Koirala, R., Kolanoski, H., Konietz, R., Köpke, L., Kopper, C., Kopper, S., Koskinen, D. J., Kowalski, M., Krings, K., Kroll, M., Krückl, G., Krüger, C., Kunnen, J., Kunwar, S., Kurahashi, N., Kuwabara, T., Kyriacou, A., Labare, M., Lanfranchi, J. L., Larson, M. J., Lauber, F., Lesiak-Bzdak, M., Leuermann, M., Lu, L., Lünemann, J., Madsen, J., Maggi, G., Mahn, K. B. M., Mancina, S., Mandelartz, M., Maruyama, R., Mase, K., Maunu, R., McNally, F., Meagher, K., Medici, M., Meier, M., Menne, T., Merino, G., Meures, T., Miarecki, S., Micallef, J., Momenté, G., Montaruli, T., Moulai, M., Nahnhauer, R., Naumann, U., Neer, G., Niederhausen, H., Nowicki, S. C., Nygren, D. R., Pollmann, A. Obertacke, Olivas, A., O'Murchadha, A., Palczewski, T., Pandya, H., Pankova, D. V., Peiffer, P., Penek, Ö., Pepper, J. A., Heros, C. Pérez de los, Pieloth, D., Pinat, E., Price, P. B., Przybylski, G. T., Quinnan, M., Raab, C., Rädel, L., Rameez, M., Rawlins, K., Reimann, R., Relethford, B., Relich, M., Resconi, E., Rhode, W., Richman, M., Riedel, B., Robertson, S., Rongen, M., Rott, C., Ruhe, T., Ryckbosch, D., Rysewyk, D., Sabbatini, L., Herrera, S. E. Sanchez, Sandrock, A., Sandroos, J., Sarkar, S., Satalecka, K., Schlunder, P., Schmidt, T., Schoenen, S., Schöneberg, S., Schumacher, L., Seckel, D., Seunarine, S., Soldin, D., Song, M., Spiczak, G. M., Spiering, C., Stachurska, J., Stanev, T., Stasik, A., Stettner, J., Steuer, A., Stezelberger, T., Stokstad, R. G., Stößl, A., Ström, R., Strotjohann, N. L., Sullivan, G. W., Sutherland, M., Taavola, H., Taboada, I., Tatar, J., Tenholt, F., Ter-Antonyan, S., Terliuk, A., Tešić, G., Tilav, S., Toale, P. A., Tobin, M. N., Toscano, S., Tosi, D., Tselengidou, M., Tung, C. F., Turcati, A., Unger, E., Usner, M., Vandenbroucke, J., van Eijndhoven, N., Vanheule, S., van Rossem, M., van Santen, J., Vehring, M., Voge, M., Vogel, E., Vraeghe, M., Walck, C., Wallace, A., Wallraff, M., Wandkowsky, N., Waza, A., Weaver, Ch., Weiss, M. J., Wendt, C., Westerhoff, S., Whelan, B. J., Wickmann, S., Wiebe, K., Wiebusch, C. H., Wille, L., Williams, D. R., Wills, L., Wolf, M., Wood, T. R., Woolsey, E., Woschnagg, K., Xu, D. L., Xu, X. W., Xu, Y., Yanez, J. P., Yodh, G., Yoshida, S., Zoll, M., Stanek, K. Z., Shappee, B. J., Kochanek, C. S., Holoien, T. W. -S., Prieto, J. L., Fox, D. B., DeLaunay, J. J., Turley, C. F., Barthelmy, S. D., Lien, A. Y., Mészáros, P., Murase, K., Kocevski, D., Buehler, R., Giomi, M., Racusin, J. L., Albert, A., Alfaro, R., Alvarez, C., Álvarez, J. D., Arceo, R., Arteaga-Velázquez, J. C., Solares, H. A. Ayala, Barber, A. S., Becerril, N. Baustista-Elivar A., Belmont-Moreno, E., Bernal, A., Brisbois, C., Caballero-Mora, K. S., Capistrán, T., Carramiñana, A., Casanova, S., Castillo, M., Cotti, U., de León, S. Coutiño, de la Fuente, E., De León, C., Hernandez, R. Diaz, Díaz-Vélez, J. C., Dingus, B. L., DuVernois, M. A., Ellsworth, R. W., Engel, K., Fiorino, D. W., Fraija, N., García-González, J. A., Gerhardt, M., Muñoz, A. González, González, M. M., Goodman, J. A., Hampel-Arias, Z., Harding, J. P., Hernandez, S., Hui, C. M., Hüntemeyer, P., Iriarte, A., Jardin-Blicq, A., Joshi, V., Kaufmann, S., Lara, A., Lauer, R. J., Lee, W. H., Lennarz, D., Vargas, H. León, Linnemann, J. T., Raya, G. Luis, Luna-García, R., López-Coto, R., Malone, K., Marinelli, S. S., Martinez, O., Martinez-Castellanos, I., Martínez-Castro, J., Martínez-Huerta, H., Matthews, J. A., Miranda-Romagnoli, P., Moreno, E., Mostafá, M., Nellen, L., Newbold, M., Nisa, M. U., Noriega-Papaqui, R., Pelayo, R., Pretz, J., Pérez-Pérez, E. G., Ren, Z., Rho, C. D., Rivière, C., Rosa-González, D., Rosenberg, M., Greus, F. Salesa, Sandoval, A., Schneider, M., Schoorlemmer, H., Sinnis, G., Smith, A. J., Springer, R. W., Surajbali, P., Tibolla, O., Tollefson, K., Torres, I., Ukwatta, T. N., Villaseñor, L., Weisgarber, T., Wisher, I. G., Wood, J., Yapici, T., Zepeda, A., Zhou, H., Arcavi, I., Hosseinzadeh, G., Howell, D. A., Valenti, S., McCully, C., Lipunov, V. M., Gorbovskoy, E. S., Tiurina, N. V., Balanutsa, P. V., Kuznetsov, A. S., Kornilov, V. G., Chazov, V., Budnev, N. M., Gress, O. A., Ivanov, K. I., Tlatov, A. G., Lopez, R. Rebolo, Serra-Ricart, M., Evans, P. A., Kennea, J. A., Gehrels, N., Osborne, J. P., Page, K. L., Abeysekara, A. U., Archer, A., Benbow, W., Bird, R., Brantseg, T., Bugaev, V., Cardenzana, J. V, Connolly, M. P., Cui, W., Falcone, A., Feng, Q., Finley, J. P., Fleischhack, H., Fortson, L., Furniss, A., Griffin, S., Grube, J., Hütten, M., Hervet, O., Holder, J., Hughes, G., Humensky, T. B., Johnson, C. A., Kaaret, P., Kar, P., Kelley-Hoskins, N., Kertzman, M., Krause, M., Kumar, S., Lang, M. J., Lin, T. T. Y., McArthur, S., Moriarty, P., Mukherjee, R., Nieto, D., Ong, R. A., Otte, A. N., Pohl, M., Popkow, A., Pueschel, E., Quinn, J., Ragan, K., Reynolds, P. T., Richards, G. T., Roache, E., Rulten, C., Sadeh, I., Santander, M., Sembroski, G. H., Staszak, D., Trépanier, S., Tyler, J., Wakely, S. P., Weinstein, A., Wilcox, P., Wilhelm, A., Williams, D. A., Zitzer, B., Bellm, E., Cano, Z., Gal-Yam, A., Kann, D. A., Ofek, E. O., Rigault, M., and Soumagnac, M.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

On February 17 2016, the IceCube real-time neutrino search identified, for the first time, three muon neutrino candidates arriving within 100 s of one another, consistent with coming from the same point in the sky. Such a triplet is expected once every 13.7 years as a random coincidence of background events. However, considering the lifetime of the follow-up program the probability of detecting at least one triplet from atmospheric background is 32%. Follow-up observatories were notified in order to search for an electromagnetic counterpart. Observations were obtained by Swift's X-ray telescope, by ASAS-SN, LCO and MASTER at optical wavelengths, and by VERITAS in the very-high-energy gamma-ray regime. Moreover, the Swift BAT serendipitously observed the location 100 s after the first neutrino was detected, and data from the Fermi LAT and HAWC observatory were analyzed. We present details of the neutrino triplet and the follow-up observations. No likely electromagnetic counterpart was detected, and we discuss the implications of these constraints on candidate neutrino sources such as gamma-ray bursts, core-collapse supernovae and active galactic nucleus flares. This study illustrates the potential of and challenges for future follow-up campaigns., Comment: 23 pages, 13 figures, accepted by A&A on July 30 2017

Published
2017
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196. The 2HWC HAWC Observatory Gamma Ray Catalog

Author

Abeysekara, A. U., Albert, A., Alfaro, R., Alvarez, C., Álvarez, J. D., Arceo, R., Arteaga-Velázquez, J. C., Solares, H. A. Ayala, Barber, A. S., Bautista-Elivar, N., Gonzalez, J. Becerra, Becerril, A., Belmont-Moreno, E., BenZvi, S. Y., Berley, D., Bernal, A., Braun, J., Brisbois, C., Caballero-Mora, K. S., Capistrán, T., Carramiñana, A., Casanova, S., Castillo, M., Cotti, U., Cotzomi, J., de León, S. Coutiño, de la Fuente, E., De León, C., Hernandez, R. Diaz, Dingus, B. L., DuVernois, M. A., Díaz-Vélez, J. C., Ellsworth, R. W., Engel, K., Fiorino, D. W., Fraija, N., García-González, J. A., Garfias, F., Gerhardt, M., Muñoz, A. González, González, M. M., Goodman, J. A., Hampel-Arias, Z., Harding, J. P., Hernandez, S., Hernandez-Almada, A., Hinton, J., Hui, C. M., Hüntemeyer, P., Iriarte, A., Jardin-Blicq, A., Joshi, V., Kaufmann, S., Kieda, D., Lara, A., Lauer, R. J., Lee, W. H., Lennarz, D., Vargas, H. León, Linnemann, J. T., Longinotti, A. L., Raya, G. Luis, Luna-García, R., López-Coto, R., Malone, K., Marinelli, S. S., Martinez, O., Martinez-Castellanos, I., Martínez-Castro, J., Martínez-Huerta, H., Matthews, J. A., Miranda-Romagnoli, P., Moreno, E., Mostafá, M., Nellen, L., Newbold, M., Nisa, M. U., Noriega-Papaqui, R., Pelayo, R., Pretz, J., Pérez-Pérez, E. G., Ren, Z., Rho, C. D., Rivière, C., Rosa-González, D., Rosenberg, M., Ruiz-Velasco, E., Salazar, H., Greus, F. Salesa, Sandoval, A., Schneider, M., Schoorlemmer, H., Sinnis, G., Smith, A. J., Springer, R. W., Surajbali, P., Taboada, I., Tibolla, O., Tollefson, K., Torres, I., Ukwatta, T. N., Vianello, G., Villaseñor, L., Weisgarber, T., Westerhoff, S., Wisher, I. G., Wood, J., Yapici, T., Younk, P. W., Zepeda, A., and Zhou, H.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

We present the first catalog of TeV gamma-ray sources realized with the recently completed High Altitude Water Cherenkov Observatory (HAWC). It is the most sensitive wide field-of-view TeV telescope currently in operation, with a 1-year survey sensitivity of ~5-10% of the flux of the Crab Nebula. With an instantaneous field of view >1.5 sr and >90% duty cycle, it continuously surveys and monitors the sky for gamma ray energies between hundreds GeV and tens of TeV. HAWC is located in Mexico at a latitude of 19 degree North and was completed in March 2015. Here, we present the 2HWC catalog, which is the result of the first source search realized with the complete HAWC detector. Realized with 507 days of data and represents the most sensitive TeV survey to date for such a large fraction of the sky. A total of 39 sources were detected, with an expected contamination of 0.5 due to background fluctuation. Out of these sources, 16 are more than one degree away from any previously reported TeV source. The source list, including the position measurement, spectrum measurement, and uncertainties, is reported. Seven of the detected sources may be associated with pulsar wind nebulae, two with supernova remnants, two with blazars, and the remaining 23 have no firm identification yet., Comment: Submitted 2017/02/09 to the Astrophysical Journal

Published
2017
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197. The first cryogenic DT layered, beryllium capsule implosion at the National Ignition Facility

Author

Wilson, D. C., Kline, J. L., Yi, S. A., Simakov, A. N., Kyrala, G. A., Olson, R. E., Perry, T. S., Merrill, F. E., Batha, S., Zylstra, A. B., Callahan, D. A., Cassata, W., Dewald, E. L., Haan, S. W., Hinkel, D. E., Hurricane, O. A., Izumi, N., Ma, T., MacPhee, A. G., Milovich, J. L., Ralph, J. E., Rygg, J. R., Schneider, M. B., Sepke, S., Strozzi, D. J., Tommasini, R., Yeamans, C., Rinderknecht, H. G., and Sio, B. H.

Subjects
Physics - Plasma Physics
Abstract

NIF experiments with Be capsules have followed a path of the highly successful "high-foot" CH capsules. Several keyhole and ConA targets preceeded a DT layered shot. In addition to backscatter subtraction, laser drive multipliers were needed to match observed X-ray drives. Those for the picket (0.95), trough (1.0) and second pulse (0.80) were determined by VISAR measurements. The time dependence of the Dante total x-ray flux and its fraction > 1.8 keV reflect the time dependence of the multipliers. A two step drive multiplier for the main pulse can match implosion times, but Dante measurements suggest the drive multiplier must increase late in time. With a single set of time dependent, multi-level multipliers the Dante data are well matched. These same third pulse drive multipliers also match the implosion times and Dante signals for two CH capsule DT. One discrepancy in the calculations is the X-ray flux in the picket. Calculations over-estimate the flux > 1.8 keV by a factor of ~100, while getting the total flux correctly. These harder X-rays cause an expansion of the Be/fuel interface of 2-3 km/s before the arrival of the first shock. VISAR measurements show only 0.2 to 0.3 km/s. The X-ray drive on the DT Be capsule was further degraded by a random decrease of 9% in the total picket flux. This small change caused the capsule fuel to change from an adiabat of 1.8 to 2.3 by mistiming of the first and second shocks. With this shock tuning and adjustments to the calculation, the first NIF Be capsule implosion achieved 29% of calculated yield, comparable to the CH DT capsules of 68% and 21%. Inclusion of a large M1 asymmetry in the DT ice layer and mixing from instability growth may help explain this final degradation. In summary when driven similarly the Be capsules performed like CH capsules. Performance degradation for both seems to be dominated by drive and capsule asymmetries.

Published
2017

198. Observation of the Crab Nebula with the HAWC Gamma-Ray Observatory

Author

Abeysekara, A. U., Albert, A., Alfaro, R., Alvarez, C., Álvarez, J. D., Arceo, R., Arteaga-Velázquez, J. C., Solares, H. A. Ayala, Barber, A. S., Bautista-Elivar, N., Becerril, A., Belmont-Moreno, E., BenZvi, S. Y., Berley, D., Braun, J., Brisbois, C., Caballero-Mora, K. S., Capistrán, T., Carramiñana, A., Casanova, S., Castillo, M., Cotti, U., Cotzomi, J., de León, S. Coutiño, de la Fuente, E., De León, C., DeYoung, T., Dingus, B. L., DuVernois, M. A., Díaz-Vélez, J. C., Ellsworth, R. W., Fiorino, D. W., Fraija, N., García-González, J. A., Gerhardt, M., Munoz, A. González, González, M. M., Goodman, J. A., Hampel-Arias, Z., Harding, J. P., Hernandez, S., Hernandez-Almada, A., Hinton, J., Hui, C. M., Hüntemeyer, P., Iriarte, A., Jardin-Blicq, A., Joshi, V., Kaufmann, S., Kieda, D., Lara, A., Lauer, R. J., Lee, W. H., Lennarz, D., Vargas, H. León, Linnemann, J. T., Longinotti, A. L., Raya, G. Luis, Luna-García, R., López-Coto, R., Malone, K., Marinelli, S. S., Martinez, O., Martinez-Castellanos, I., Martínez-Castro, J., Martínez-Huerta, H., Matthews, J. A., Miranda-Romagnoli, P., Moreno, E., Mostafá, M., Nellen, L., Newbold, M., Nisa, M. U., Noriega-Papaqui, R., Pelayo, R., Pretz, J., Pérez-Pérez, E. G., Ren, Z., Rho, C. D., Rivière, C., Rosa-González, D., Rosenberg, M., Ruiz-Velasco, E., Salazar, H., Greus, F. Salesa, Sandoval, A., Schneider, M., Schoorlemmer, H., Sinnis, G., Smith, A. J., Springer, R. W., Surajbali, P., Taboada, I., Tibolla, O., Tollefson, K., Torres, I., Ukwatta, T. N., Villaseñor, L., Weisgarber, T., Westerhoff, S., Wisher, I. G., Wood, J., Yapici, T., Yodh, G. B., Younk, P. W., Zepeda, A., and Zhou, H.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

The Crab Nebula is the brightest TeV gamma-ray source in the sky and has been used for the past 25 years as a reference source in TeV astronomy, for calibration and verification of new TeV instruments. The High Altitude Water Cherenkov Observatory (HAWC), completed in early 2015, has been used to observe the Crab Nebula at high significance across nearly the full spectrum of energies to which HAWC is sensitive. HAWC is unique for its wide field-of-view, nearly 2 sr at any instant, and its high-energy reach, up to 100 TeV. HAWC's sensitivity improves with the gamma-ray energy. Above $\sim$1 TeV the sensitivity is driven by the best background rejection and angular resolution ever achieved for a wide-field ground array. We present a time-integrated analysis of the Crab using 507 live days of HAWC data from 2014 November to 2016 June. The spectrum of the Crab is fit to a function of the form $\phi(E) = \phi_0 (E/E_{0})^{-\alpha -\beta\cdot{\rm{ln}}(E/E_{0})}$. The data is well-fit with values of $\alpha=2.63\pm0.03$, $\beta=0.15\pm0.03$, and log$_{10}(\phi_0~{\rm{cm}^2}~{\rm{s}}~{\rm{TeV}})=-12.60\pm0.02$ when $E_{0}$ is fixed at 7 TeV and the fit applies between 1 and 37 TeV. Study of the systematic errors in this HAWC measurement is discussed and estimated to be $\pm$50\% in the photon flux between 1 and 37 TeV. Confirmation of the Crab flux serves to establish the HAWC instrument's sensitivity for surveys of the sky. The HAWC survey will exceed sensitivity of current-generation observatories and open a new view of 2/3 of the sky above 10 TeV., Comment: Submitted 2017/01/06 to the Astrophysical Journal

Published
2017
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199. Statistical data analysis of x-ray spectroscopy data enabled by neural network accelerated Bayesian inference.

Author

MacDonald, M. J., Hammel, B. A., Bachmann, B., Bitter, M., Efthimion, P., Gaffney, J. A., Gao, L., Hammel, B. D., Hill, K. W., Kraus, B. F., MacPhee, A. G., Peterson, L., Schneider, M. B., Scott, H. A., Thorn, D. B., and Yeamans, C. B.

Subjects
MARKOV chain Monte Carlo, STATISTICAL sampling, ATOMIC physics, X-ray spectra, X-ray spectroscopy
Abstract

Bayesian inference applied to x-ray spectroscopy data analysis enables uncertainty quantification necessary to rigorously test theoretical models. However, when comparing to data, detailed atomic physics and radiation transfer calculations of x-ray emission from non-uniform plasma conditions are typically too slow to be performed in line with statistical sampling methods, such as Markov Chain Monte Carlo sampling. Furthermore, differences in transition energies and x-ray opacities often make direct comparisons between simulated and measured spectra unreliable. We present a spectral decomposition method that allows for corrections to line positions and bound–bound opacities to best fit experimental data, with the goal of providing quantitative feedback to improve the underlying theoretical models and guide future experiments. In this work, we use a neural network (NN) surrogate model to replace spectral calculations of isobaric hot-spots created in Kr-doped implosions at the National Ignition Facility. The NN was trained on calculations of x-ray spectra using an isobaric hot-spot model post-processed with Cretin, a multi-species atomic kinetics and radiation code. The speedup provided by the NN model to generate x-ray emission spectra enables statistical analysis of parameterized models with sufficient detail to accurately represent the physical system and extract the plasma parameters of interest. [ABSTRACT FROM AUTHOR]

Published
2024
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200. Variable-sagittal-radii elliptical x-ray crystal spectrometers for high-neutron-yield plasma diagnostics.

Author

Stoupin, S., Sagan, D., MacPhee, A. G., Kozioziemski, B., MacDonald, M. J., Schneider, M. B., Meamber, M. F., May, M. J., and Heeter, R. F.

Subjects
PLASMA diagnostics, PLASMA spectroscopy, X-ray spectrometers, TIME-resolved spectroscopy, RAY tracing
Abstract

Sagittally focusing x-ray crystal spectrometers with elliptical profiles in the meridional (x-ray dispersion) plane are proposed for plasma diagnostics in experiments accompanied by high neutron yields. The spectrometers feature a variable sagittal radius of curvature to ensure the sagittal focusing of rays for each photon energy in a chosen detection plane. The detector is placed after the ray crossing point at the second ellipse focus, and the source-to-detector distance is maximized to reduce the neutron-induced background. The elliptical shape imposes a limitation on the spectrometer geometry such that the influence of the source size on the spectral resolution can be avoided only for a demagnifying spectrometer (the source-to-crystal distance is larger than that of crystal-to-detector). Hence, two designs are proposed. The first design, featuring high magnification and limited spectral resolution can be suitable for x-ray continuum spectroscopy. The second design of high demagnification is optimized for spectral resolution, and can be used for time-resolved spectroscopy of plasma's characteristic emission lines using streak cameras. The key performance characteristics of the two designs are verified using ray tracing. [ABSTRACT FROM AUTHOR]

Published
2024
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